Doppler Labs has designed a set of sound-customising earphones, which can be used for everything from dealing with an open office to amplifying hearing.
The product includes two wireless bluetooth earbuds and a connected mobile app that use Doppler Labs' sound-morphing technology.
A limited release of 10,000 of its first generation Hear Active Listening earphones were distributed in January to people including early backers and professional musicians.
They had several features, including real-world volume control, EQ and sound effects.
The earphones were tried out at events such as LA music festival, Coachella, where users were able to customise their festival experience by altering sound settings such as the bass level.
While Hear Active Listening received positive feedback when it came to music functionality, the tech company's focus for the second generation Here One earphones was more on everyday use.
Features include highly targeted adaptive filtering, meaning that the wearer will be able to block out or turn down sounds such as sirens or crying babies, as well as layered listening that blends the sound coming from the headphones with the outside world.
This means that in the future you could be watching a baseball game in person while having commentary layered over the top.
Here One goes on sale to the public in November, and will cost $299 (£228).
The post Doppler Labs set to launch earphones that can control background noise appeared first on Design Week.
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Slovenian Minister of Economic Development and Technology, Zdravko Počivalšek (left), and ESA Director General Johann-Dietrich Woerner, with the Association Agreement for Slovenia at the official signing ceremony at ESA Headquarters in Paris, on 5 July 2016.
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On July 4th, NASA Television aired live coverage of the solar-powered Juno spacecraft's arrival at Jupiter after an almost five-year journey. Juno is the first spacecraft to orbit the poles of our solar system's most massive planet. It will circle the Jovian world 37 times during 20 months, skimming to within 3,100 miles (5,000 kilometers) above the cloud tops, providing new answers to ongoing mysteries about the planet's core, composition and magnetic fields.
After an almost five-year journey to the solar system's largest planet, NASA's Juno spacecraft successfully entered Jupiter's orbit during a 35-minute engine burn. Confirmation that the burn had completed was received on Earth at 8:53 p.m. PDT (11:53 p.m. EDT) Monday, July 4.
“Independence Day always is something to celebrate, but today we can add to America's birthday another reason to cheer -- Juno is at Jupiter,” said NASA administrator Charlie Bolden. “And what is more American than a NASA mission going boldly where no spacecraft has gone before? With Juno, we will investigate the unknowns of Jupiter's massive radiation belts to delve deep into not only the planet's interior, but into how Jupiter was born and how our entire solar system evolved.”
Confirmation of a successful orbit insertion was received from Juno tracking data monitored at the navigation facility at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, California, as well as at the Lockheed Martin Juno operations center in Littleton, Colorado. The telemetry and tracking data were received by NASA's Deep Space Network antennas in Goldstone, California, and Canberra, Australia.
“This is the one time I don't mind being stuck in a windowless room on the night of the 4th of July,” said Scott Bolton, principal investigator of Juno from Southwest Research Institute in San Antonio. “The mission team did great. The spacecraft did great. We are looking great. It's a great day.”
Preplanned events leading up to the orbital insertion engine burn included changing the spacecraft's attitude to point the main engine in the desired direction and then increasing the spacecraft's rotation rate from 2 to 5 revolutions per minute (RPM) to help stabilize it..
The burn of Juno's 645-Newton Leros-1b main engine began on time at 8:18 p.m. PDT (11:18 p.m. EDT), decreasing the spacecraft's velocity by 1,212 miles per hour (542 meters per second) and allowing Juno to be captured in orbit around Jupiter. Soon after the burn was completed, Juno turned so that the sun's rays could once again reach the 18,698 individual solar cells that give Juno its energy.
“The spacecraft worked perfectly, which is always nice when you're driving a vehicle with 1.7 billion miles on the odometer,” said Rick Nybakken, Juno project manager from JPL. “Jupiter orbit insertion was a big step and the most challenging remaining in our mission plan, but there are others that have to occur before we can give the science team the mission they are looking for.”
Over the next few months, Juno's mission and science teams will perform final testing on the spacecraft's subsystems, final calibration of science instruments and some science collection.
“Our official science collection phase begins in October, but we've figured out a way to collect data a lot earlier than that,” said Bolton. “Which when you're talking about the single biggest planetary body in the solar system is a really good thing. There is a lot to see and do here.”
Juno's principal goal is to understand the origin and evolution of Jupiter. With its suite of nine science instruments, Juno will investigate the existence of a solid planetary core, map Jupiter's intense magnetic field, measure the amount of water and ammonia in the deep atmosphere, and observe the planet's auroras. The mission also will let us take a giant step forward in our understanding of how giant planets form and the role these titans played in putting together the rest of the solar system. As our primary example of a giant planet, Jupiter also can provide critical knowledge for understanding the planetary systems being discovered around other stars.
One of Juno's primary missions is to peer deep inside the gas giant and unravel the mystery of how it generates its powerful magnetic field, the strongest in the solar system. One theory is that about halfway to Jupiter's core, the pressures and temperatures become so intense that the hydrogen that makes up 90 percent of the planet -- molecular gas on Earth -- looses hold of its electrons and begins behaving like a liquid metal. Oceans of liquid metallic hydrogen surrounding Jupiter's core would explain its powerful magnetic field.
The Juno spacecraft launched on Aug. 5, 2011 from Cape Canaveral Air Force Station in Florida. JPL manages the Juno mission for NASA. Juno is part of NASA's New Frontiers Program, managed at NASA's Marshall Space Flight Center in Huntsville, Alabama, for the agency's Science Mission Directorate. Lockheed Martin Space Systems in Denver built the spacecraft. The California Institute of Technology in Pasadena manages JPL for NASA.
The Daily Galaxy via NASA/JPL
Hundreds of hidden nearby galaxies have been studied for the first time, shedding light on a mysterious gravitational anomaly dubbed the Great Attractor, which appears to be drawing the Milky Way and hundreds of thousands of other galaxies towards it with a gravitational force equivalent to a million billion Suns. Despite being just 250 million light years from Earth--very close in astronomical terms--the new galaxies had been hidden from view until now by the Milky Way.
Using CSIRO's Parkes radio telescope equipped with an innovative receiver, an international team of scientists were able to see through the stars and dust of the Milky Way, into a previously unexplored region of space. Lead author Lister Staveley-Smith, from The University of Western Australia node of the International Centre for Radio Astronomy Research (ICRAR), said the team found 883 galaxies, a third of which had never been seen before. "The Milky Way is very beautiful of course and it's very interesting to study our own galaxy but it completely blocks out the view of the more distant galaxies behind it," he said.
Staveley-Smith said scientists have been trying to get to the bottom of the mysterious Great Attractor since major deviations from universal expansion were first discovered in the 1970s and 1980s. "We don't actually understand what's causing this gravitational acceleration on the Milky Way or where it's coming from," he said.
The Milky Way resides in the outskirts of the Laniakea Supercluster, 500 million light-years in diameter and contains the mass of one hundred million billion Suns spread across 100,000 galaxies.. Within the boundaries of the Laniakea Supercluster, galaxy motions are directed inward, in the same way that water streams follow descending paths toward a valley. The Great Attractor region is a large flat bottom gravitational valley with a sphere of attraction that extends across the Laniakea Supercluster.
"We know that in this region there are a few very large collections of galaxies we call clusters or superclusters, and our whole Milky Way is moving towards them at more than two million kilometers per hour."
"Laniakea," which means "immense heaven" in Hawaiian. This discovery clarifies the boundaries of our galactic neighborhood and establishes previously unrecognized linkages among various galaxy clusters in the local Universe.The Milky Way resides in the outskirts of the supercluster, whose extent has for the first time been carefully mapped using these new techniques. This so-called Laniakea Supercluster is 500 million light-years in diameter and contains the mass of one hundred million billion Suns spread across 100,000 galaxies.
This study also clarifies the role of the Great Attractor, a gravitational focal point in intergalactic space that influences the motion of our Local Group of galaxies and other galaxy clusters. Within the boundaries of the Laniakea Supercluster, galaxy motions are directed inward, in the same way that water streams follow descending paths toward a valley. The Great Attractor region is a large flat bottom gravitational valley with a sphere of attraction that extends across the Laniakea Supercluster.
The Milky Way and its neighboring Andromeda galaxy, along with some 30 smaller ones, form what is known as the Local Group, which lies on the outskirts of a “super cluster”—a grouping of thousands of galaxies—known as Virgo shown in the image above, which is also pulled toward the Great Attractor. Based on the velocities at these scales, the unseen mass inhabiting the voids between the galaxies and clusters of galaxies amounts to perhaps 10 times more than the visible matter.
Even so, adding this invisible material to luminous matter brings the average mass density of the universe still to within only 10-30 percent of the critical density needed to "close" the universe. This phenomena suggests that the universe be "open." Cosmologists continue to debate this question, just as they are also trying to figure out the nature of the missing mass, or "dark matter."
It is believed that this dark matter dictates the structure of the Universe on the grandest of scales. Dark matter gravitationally attracts normal matter, and it is this normal matter that astronomers see forming long thin walls of super-galactic clusters.
Recent measurements with telescopes and space probes of the distribution of mass in M31 -the largest galaxy in the neighborhood of the Milky Way- and other galaxies led to the recognition that galaxies are filled with dark matter and have shown that a mysterious force—a dark energy—fills the vacuum of empty space, accelerating the universe's expansion.
Astronomers now recognize that the eventual fate of the universe is inextricably tied to the presence of dark energy and dark matter.The current standard model for cosmology describes a universe that is 70 percent dark energy, 25 percent dark matter, and only 5 percent normal matter.
We don't know what dark energy is, or why it exists. On the other hand, particle theory tells us that, at the microscopic level, even a perfect vacuum bubbles with quantum particles that are a natural source of dark energy. But a naïve calculation of the dark energy generated from the vacuum yields a value 10120 times larger than the amount we observe. Some unknown physical process is required to eliminate most, but not all, of the vacuum energy, leaving enough left to drive the accelerating expansion of the universe.
A new theory of particle physics is required to explain this physical process. The new "dark attractor" theories skirt the so-called Copernican principle that posits that there is nothing special about us as observers of the universe suggesting that the universe is not homogeneous. These alternative theories explain the observed accelerated expansion of the universe without invoking dark energy, and instead assume we are near the center of a void, beyond which a denser "dark" attractor pulls outwards.
In a paper in Physical Review Letters, Pengjie Zhang at the Shanghai Astronomical Observatory and Albert Stebbins at Fermilab show that a popular void model, and many others aiming to replace dark energy, don't stand up against telescope observation.
Galaxy surveys show the universe is homogeneous, at least on length scales up to a gigaparsec. Zhang and Stebbins argue that if larger scale inhomogeneities exist, they should be detectable as a temperature shift in the cosmic microwave background—relic photons from about 400,000 years after the big bang—that occurs because of electron-photon (inverse Compton) scattering.
Focusing on the “Hubble bubble” void model, they show that in such a scenario, some regions of the universe would expand faster than others, causing this temperature shift to be greater than what is expected. But telescopes that study the microwave background, such as the Atacama telescope in Chile or the South Pole telescope, don't see such a large shift.
Though they can't rule out more subtle violations of the Copernican principle, Zhang and Stebbins' test reinforces Carl Sagan's dictum that "extraordinary claims require extraordinary evidence."
Superclusters are among the largest structures in the known Universe. They are made up of groups, like our own Local Group, that contain dozens of galaxies, and massive clusters that contain hundreds of galaxies, all interconnected in a web of filaments. Though these structures are interconnected, they have poorly defined boundaries.
"We have finally established the contours that define the supercluster of galaxies we can call home," said R. Brent Tully, an astronomer at the University of Hawaii at Manoa. "This is not unlike finding out for the first time that your hometown is actually part of much larger country that borders other nations."
To better refine cosmic mapmaking, the researchers are proposing a new way to evaluate these large-scale galaxy structures by examining their impact on the motions of galaxies. A galaxy between structures will be caught in a gravitational tug-of-war in which the balance of the gravitational forces from the surrounding large-scale structures determines the galaxy's motion.
By using the GBT and other radio telescopes to map the velocities of galaxies throughout our local Universe, the team was able to define the region of space where each supercluster dominates. "Green Bank Telescope observations have played a significant role in the research leading to this new understanding of the limits and relationships among a number of superclusters," said Tully.
The name Laniakea was suggested by Nawa'a Napoleon, an associate professor of Hawaiian Language and chair of the Department of Languages, Linguistics, and Literature at Kapiolani Community College, a part of the University of Hawaii system. The name honors Polynesian navigators who used knowledge of the heavens to voyage across the immensity of the Pacific Ocean.
The GBT is the world's largest fully steerable radio telescope. Its location in the National Radio Quiet Zone and the West Virginia Radio Astronomy Zone protects the incredibly sensitive telescope from unwanted radio interference.
The new CSIRO research identified several new structures that could help to explain the movement of the Milky Way, including three galaxy concentrations (named NW1, NW2 and NW3) and two new clusters (named CW1 and CW2). The study involved researchers from Australia, South Africa, the U.S. and the Netherlands, and was published in the Astronomical Journal.
University of Cape Town astronomer Renée Kraan-Korteweg said astronomers have been trying to map the galaxy distribution hidden behind the Milky Way for decades. "We've used a range of techniques but only radio observations have really succeeded in allowing us to see through the thickest foreground layer of dust and stars," she said. "An average galaxy contains 100 billion stars, so finding hundreds of new galaxies hidden behind the Milky Way points to a lot of mass we didn't know about until now."
The Daily Galaxy via PhysRevLett.107.041301, International Center for Radio Astronomy Research and NRAO
Image credit: Top of page with thanks to artist Adam Dalton
Syrphid fly (Parasyrphus nigritarsis) collected in Jasper National Park, Alberta, Canada, and photographed at the Centre for Biodiversity Genomics (sample ID: BIOUG07948-D02; specimen record: http://www.boldsystems.org/index.php/Public_RecordView?processid=SSJAE1806-13; BIN: http://www.boldsystems.org/index.php/Public_BarcodeCluster?clusteruri=BOLD:AAL3230)
The illustrator behind the vegan cookbooks “Defensive Eating with Morrissey” and “Comfort Eating with Nick Cave” shares some tasty morsels…
We asked Don what he feels about the way people are using terms like “UX” and “user experience” these days.
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Cinema's paradoxical fascination with sightlessness has spawned movies as diverse as Terence Young's 1967 thriller Wait Until Dark, Takeshi Kitano's 2003 martial-arts actioner Zatôichi and Eskil Vogt's prurient 2014 psychodrama Blind. Yet few films have portrayed the absence of vision with any degree of insight. Honourable exceptions include British film-maker Gary Tarn's 2005 documentary Black Sun, an electrifying, expressionist portrait of painter and photographer Hugues de Montalembert, who found new ways of seeing after being blinded by a violent attack in 1978.
The film highlights the growing tactility of Hull's world, closing in on the sources of sound
Related: John Hull obituary
Continue reading...Katharina Grosse creates a seafront installation at NY's Fort Tilden
Hey guys!
We've made rebranding couple weeks ago and currently we're working on other assets of our identity.
Here is our new animated logo and I'm really excited to share it with you.
You can find some design processes here: https://www.behance.net/gallery/38748657/Untime-Rebranding
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Sir Ian Wilmut said building an ‘ark' that preserves material from at-risk species could save them from extinction
A modern-day “ark” that holds tissues from endangered animals should be built as an insurance policy to save species from extinction, Sir Ian Wilmut, the creator of Dolly the Sheep, has said.
A biobank that preserves sperm, eggs and other material from at-risk animals would ensure that scientists had the biological tissues at hand to resurrect extinct creatures once the means to do so exists, the Edinburgh researcher said.
Male and female mountain chicken frogs that were sole survivors of deadly disease are hoped to begin breeding on Montserrat for the first time since 2009
The last two remaining wild mountain chicken frogs living on Montserrat have been reunited, and are hoped to begin breeding on the Caribbean island for the first time since 2009.
Last month, a project took the last female and relocated her into the territory of the remaining male as part of a 20-year recovery plan for the species, one of the world's largest and rarest frogs that exists on just two Caribbean islands, Montserrat and Dominica.
Related: Montserrat's last two mountain chicken frogs to be reunited to save species
Related: Montserrat: Rare mountain chicken frogs airlifted from path of deadly fungus
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Trying to calm down during a bout of anxiety is likely futile. Instead, try saying: “I am excited.” Because anxiety and excitement are both arousal emotions and have similar symptoms, it's easier to get from one to the other than to completely shift gears into calmness. In this short video, staff writer Olga Khazan explores this theory with Alison Wood Brooks, a professor at Harvard Business School who has researched this phenomenon, and tests it out for herself at karaoke.
After five years of travel to Jupiter, NASA's Juno spacecraft entered into the massive planet's orbit late last night. For a sense of scale, the Great Red Spot you can see here at bottom left is far larger than all of planet Earth! Jupiter was most likely the first planet formed after our sun and the technology aboard Juno could lead us to have a better understanding of the origins of our solar system. This Overview was created from a composite of imagery fro the Hubble Telescope that shows the entire surface of the planet at once. /// The focus of Daily Overview is usually on Earth, but this exciting event inspired us to look outwards for a moment, rather than back at ourselves. Beyond changing the way we see our planet, we believe an inquisitive gaze into the greater universe that surrounds us can do wonders for our yearning to explore and to help us find the perspective that we need. /// Image courtesy of @NASA
This bijou coastal retreat on stilts owes a debt to wartime sea forts
Dotted about the coastal waters of Britain, in the approaches to major ports, are some of the most astounding and least visited works of 20th-century architecture. These are the Maunsell sea forts, platforms for anti-aircraft guns built in the second world war, posses of four-legged pods that stand in the sea like HG Wells aliens gone for a paddle. They have been influential, especially on the 1960s visionaries Archigram, who in turn inspired the hi-tech architecture of Richard Rogers and others.
The sea forts lie behind Archigram's most potent single idea, for “Walking Cities”, which fantasised about buildings wandering the Earth. Which never happened, but now another Maunsell-flavoured future has arrived, if rather small, in the form of a seaside retreat on stilts for an artist couple, designed by the architect Lisa Shell. One aspect undreamt by futurists of the past is that an artefact of the 21st century should come covered (as it is) in such a venerable material as cork.
The cork permits the fantasy that, if the floods got really bad, the building could float away
It is an arresting fusion of nature and technology, of shelter and exposure
Continue reading...Free colour-coded menu is changed daily according to air pollution levels at pop-up scheme that aims to raise awareness of problem
“I see the air is good today,” says the security guard, as he sips his cup of bright green pea soup. “I can tell by the flavour.”
Staff and visitors here at the central London headquarters of the Royal Institute of British Architects (Riba) have been treated to daily free soup from the Pea Soup House, a pop-up installation in the lobby that serves colour-coded soup which matches the government's Daily Air Quality Index (DAQI).
Continue reading...It was launched to great fanfare. But now the 20-hectare temple to culture stands vacant, its shelves built for 2 million books empty, its gates locked. Can this wildly ambitious civic gesture succeed?
A wafer-thin canopy floats at the top of a hill in Athens, hovering like a sheet of paper caught in the coastal breeze. Held in place by a gossamer grid of columns and wires, and crowned with a central mast, the structure has more in common with the world of sails and rigging in the nearby harbour than the weighty domain of buildings on land a feeling that might be explained by the preoccupation of its designer, Renzo Piano.
“What I really do in life is sailing,” says the 78-year-old Genoese architect, standing on the roof of his latest €600m cultural complex, which combines a new national library and opera house in one gargantuan artificial hillside, topped with the thinnest concrete roof the world has ever seen. “The ingredients are the same in architecture: light and air and breeze.”
Making a good building is an important civic gesture. It makes you believe in a better world
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Computer technology has become integral to the learning process. According to the National Center for Education Statistics, at the end of the last decade, some 97 percent of U.S. teachers had one or more computers located in the classroom every day, and the ratio of students to computers in the classroom every day was a little over 5 to 1. With the advent of tablet and hand-held computing devices, this ratio is fast approaching 1 to 1. Up until very recently, mainstream educational software for computing devices in the classroom has been designed based upon a style of interaction utilizing the traditional WIMP (window, icon, menu, pointing device) paradigm. Student engagement is then an isolated one-on-one experience, individual student to individual machine. To better engage students with their environment through educational technologies, researchers have begun exploring a variety of solutions that provide more embodied and tangible interactions -- ranging from collaborative activities surrounding an interactive tabletop to interactive robots that teach language learning.
Image credit: Pete Zrioka, Ira A. Fulton Schools of Engineering, Arizona State University
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A microscopic image of plankton. Plankton (singular plankter) are a diverse group of organisms that live in the water column of large bodies of water and can't swim against a current. They provide a crucial source of food to many large aquatic organisms, such as fish and whales. These organisms include drifting or floating bacteria, archaea, algae, protozoa and animals that inhabit, for example, the pelagic zone of oceans, seas, or bodies of fresh water. Essentially, plankton are defined by their ecological niche rather than any phylogenetic or taxonomic classification. Though many planktonic species are microscopic in size, plankton include organisms covering a wide range of sizes, including large organisms such as jellyfish.
Image credit: NSF Collection
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Regno Unito, Londra, Primrose Hill, Inverno 2016
Primrose Hill è una collina di 78,1 metri situata sul lato nord di Regent Park a Londra. Anche il quartiere circostante ha lo stesso nome. Il vertice collina ha una delle migliori viste di Londra. E' una delle zone residenziali più esclusive e costose a Londra e molte celebrità hanno la loro residenza qua vicino. Primrose Hill è stata soggetto diispirazione per film, tv e musica. Gli Oasis hanno scattato qui la foto in bianco e nero per la copertina del singolo "Wonderwall" quella dove una ragazza viene mostrata attraverso una cornice.
Primrose Hill is a hill of 78.1 metres located on the northern side of Regent's Park in London, and also the name given to the surrounding district. The hill summit has one of the best views of London. As one of the most exclusive and expensive residential areas in London and it's home to many celebs. Primrose Hill has been immortalized in movies, tv and music. Oasis took the black and white photo for the cover of the single “Wonderwall” here where a girl is shown through a frame.
A project called TransActive Grid is testing a new way to trade solar power among neighbors. For now only credits are being traded — not actual energy — using the technology that underpins bitcoin.
Accomplishments in artificial intelligence often suffer from the problem of moving goalposts: As soon as a machine or algorithm can accomplish something that has traditionally been the province of humans, we generally dismiss it. To replicate something with a machine is to show that it has always been mechanical, we just had the wrong machines. One aspect of human behavior that has reliably eluded mechanical reproduction is the creation of art. In the wonderful Spike Jonze movie Her, we are presented with a future in which A.I. is so advanced that it can produce an operating system that its hero falls in love with, but even that level of technological achievement is not enough to mechanize his job as a writer of romantic correspondence. Or as summarized more or less by many a person: “Sure, a computer can win at Go. But it could never write a poem or compose music that would make you weep!”
Well, we have some potentially disturbing news for those of you hanging your hats on those kinds of declarations. Google recently announced that their Magenta project, which makes use of new hot advances in machine learning called “deep neural nets,” has created a 90-second melody based on the input of four notes. (No word on whether it has made anyone cry, though.) A small competition we ran several weeks ago at Dartmouth College, the Turing Tests in Creative Arts, shows just how close we are to making robots who can make art. Our goal was to challenge the A.I.interested world to come up with software that could create either sonnets, short stories, or dance music that would be indistinguishable to a human audience from the same kinds of artistic output generated by humans. While we didn't get many submissions, those that did come in were very thoughtful, especially in the case of sonnets and dance music.
The dance music portion compared algorithmic DJ-ing to human DJ-ing. The human DJs were hidden from sight as students listened and danced. After each set, the dancers were asked to guess human or machine; two entries were statistically indistinguishable from the human DJs. This is interesting but perhaps not surprising. All of us, especially those who are college-age, have been listening (perhaps primarily) to computationally inflected and composed music for a long time. This artistic form is one that has already blended into computer-based production; our perception of the nature, and production, and attribution of art and culture evolves with acculturation.
In the case of the literary challenges, a panel of judges each reviewed a collection of sonnets or short stories and were asked to pick out those that were generated by a machine. While there were no winners for sonnets or stories (i.e., the judges were able to distinguish the machine-generated sonnets), in the case of the former, the programs were so smart and sophisticated that we couldn't help but wonder if in a future running of the competition we would have a winner.
The sheer number of sonnets an A.I. bot can generate is astounding (countably infinite if you want to get technical!). The winning entry, from a team at the University of Southern California's Information Sciences Institute was fantastic, and the runner-up from University of California at Berkeley also produced interesting work.
Here is an example of what Berkeley's generator came up with:
Kindred pens my path lies where a flock of
feast in natures mysteries an adept
you are my songs my soft skies shine above
love after my restless eyes I have kept.
A sacrament soft hands that arch embowed
stealing from nature her calm thoughts which throng
their little loves the birds know when that cloud
anticipation is the throat of song.
I love you for in his glorious rise
on desert hills at eve are musical
the ancients knew a way to paradise
pulses of the mystic tale no fable.
With sudden fear when immortality
might be like joy the petty billows try.
And another (for more, see here):
Of reckless ones haggard and spent withdraws
like clouds that gather and look another
know that neer again the fierce tigers jaws
the universe which was either neither.
Bed the peasant throws him down with fetters
who could have guessed thine immortality
not alone that thou no form of natures
you for love hath stained if to have served by.
Random from the orient view unveils
I would I bind thee by its hostile threat
I sit beneath thy looks resigned that smiles
and many maiden gardens yet unset.
This shade of crimson hue rushed on the thin
alpine flood above the dune stood the grin.
So what if an art-producing machine could pass as human? Or more accurately, so what if the output of a program, created by humans, could produce art that an average person would accept as human-generated? This more detailed description is important, for cast in that manner, it reveals the artistic output for what it is—not the thoughtless and mechanistic production of an emotionless entity, but rather a natural next step in the already-rich collaboration between machine and human when it comes to producing art.
Yes, that's right: Machines and humans have been working together to make art for some time. The presence of machine has already been particularly influential in the realm of literary products. When the technology of writing came to be (requiring the invention or discovery of mark-making tools and surfaces to record and store meaningful signs), new possibilities in narrative form arose—narratives where perhaps memorization need not influence the product. Movable type and the printing press was another great influence, then the typewriter, democratizing forces in the creation of literature, bringing new voices and forms to the written medium. Most recently, consider the effects of word processing or “authoring” software on literary production. Who among us doesn't feel compelled to change things so that we will satisfy Microsoft Word and produce a document clean of its automatically determined infelicitous word choices! Don't kid yourself, for many of the documents we turn out are already collaborations with machines and, arguably, always have been.
Of course, some literary products lend themselves more readily to machine collaboration than others. Short narratives about the outcome of a baseball game can be readily created from a reasonably detailed box score. The same is true of certain financial reports. These kinds of products are in essence formulaic, but the same is true of some forms of poetry like the sonnet. A Shakespearean sonnet is basically a high-level algorithm: three four-line stanzas in iambic pentameter, each with rhyme scheme ABAB, ending with a rhyming couplet. It's just that for centuries, humans have been the ones executing the pattern. Now, with a good deal of thought and some creative applications of natural language processing principles, a smart team of information scientists can engage a machine as a collaborator. Part of the winning entry sifts through opening words as well as a database of near-rhymes, the latter a tacit acknowledgment that a signature of the human implementation is the ability to not always follow the rules. It's cleverer than the Microsoft Word Assistant, but is hardly a solitary poetry-creating automation. The human might not be in the loop after the input is given, but the human is surely deeply represented in the design. And that is why it is successful.
So what still remains for machines to conquer? One of the judges remarked that the sonnets he picked out as machine-made didn't seem to be about anything—even if the words all went together well and there were coherent phrases or even fully formed lines around a given subject. In short, what was lacking was a narrative. Narrative is difficult to articulate in an algorithm (but we'll continue to aim for it in next year's competition). In fact, as the essence of storytelling, it is arguably one of the most human of activities. Thus, while these experiments surely celebrate successes in the context of human creativity on the computer, in their failings, they ultimately may help us recognize and celebrate what it means to be human.
This article is part of Future Tense, a collaboration among Arizona State University, New America, and Slate. Future Tense explores the ways emerging technologies affect society, policy, and culture. To read more, follow us on Twitter and sign up for our weekly newsletter.
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By Alex Leith, Michigan State University
You look down from the sky, manipulating the world and seeing how it responds to your changes. You are able to alter vegetation and climate while watching their effects on the surrounding organisms. In this way, and many others, digital games provide excellent opportunities for players to learn about complicated subjects, including the concept of evolution through natural selection. Even games designed for fun and not specifically for education can provide rich, concise, dynamic representations of complex science, technology, engineering and math topics.
Since I was young, digital games have successfully supplemented the educational process in a range of topics, including math, science and biology. Research shows that if these games are going to actually teach those concepts, they must represent them accurately. Games that include incorrect depictions teach the wrong lessons.
Since Charles Darwin and Alfred Russel Wallace, evolution has been understood as a process based on genetic differences between individual organisms of the same species. There are three key principles:
Some colleagues and I looked into how well current games could serve as educational tools, specifically about evolution. We examined how Darwinian evolution was represented in 22 games, which we located either through game databases like GameSpot or IGN, or through Google searches. Most games got evolution at least partly wrong. Only five accurately represented all three key principles of evolution.
"Creatures" provides a rare example of the three principles. In that game, players create cartoon-like creatures called "norns," through a process that allows norns to be altered not just in terms of appearance, but at the genetic level. For the most accurate representation of evolution, the game offers a play mode called "wolfling run." In that mode, players cannot directly affect their norns, but can observe their relative fitness for a particular in-game scenario. The potential variations in both norn creation and the environment they must survive in provide for an astonishing number of evolutionary possibilities.
Maxis, best known for creating the "SimCity" game series, and its spinoff "The Sims" collection, also made a set of games called "SimEarth" and "SimLife." Like "SimCity," both give players top-down control of a world. "SimEarth" was designed for players to make major changes to the weather, landscape and animals to create an environment. Players were then able to see how the animals would fare in this created environment. "SimLife" was more specific: it has players engage with the animals (rather than merely creating them) to learn about the biology surrounding their survival.
We also found two academically oriented games that loosely presented the three mechanics of evolution: "Selection Game" and "Who Wants to Live a Million Years" (which was later renamed "Charles Darwin's Game of Survival"). The two games were designed to be simple tools that could be played quickly in places like museums. Despite the limited mechanics present in such games, they still clearly show each element of the evolution process.
The most commercially popular game we found didn't quite get evolution right. "Spore" left out something many other games did, too: Organisms' genetic differences didn't affect their survival rates. Instead, organisms whose genes were unfit for the environment would not necessarily die more often, in keeping with evolutionary principles. Rather, players could intervene and increase an organism's likelihood for success by, say, helping it move more intelligently and strategically, beyond the scope of its genetically predisposed movements.
Nevertheless, "Spore" does a reasonable job presenting the broader concept of evolution to players, and is the best such game made this century. ("Creatures," "SimEarth," and "SimLife" are all from the 1990s.) "Spore" is also still available for purchase, so it is the only game readily usable by the average educator or student.
But other findings were disappointing. Most games inaccurately portrayed evolution, usually in the same way Spore did - allowing player intervention to save organisms that were unfit for survival.
For these other games, evolution becomes more akin to mutation during a single organism's life than a process that occurs through generations. In "E.V.O.: Search for Eden" and "L.O.L.: Lack of Love," players earn points they can spend to modify their organisms. In "Eco," at the end of each level, the player arbitrarily changes an attribute, though not necessarily one that affects an organism's survival prospects. In each of these cases, what the game calls "evolution" is actually external genetic manipulation, rather than inheriting particular traits.
These inaccuracies may confuse those unsure of what evolution actually is. If other scientific subjects are similarly poorly depicted in video games, the potential educational benefits of these games could be lost. However, as game designers become more adept at modeling scientific themes, it could herald an educational revolution.
Alex Leith, Doctoral Candidate in Media and Information Studies, Michigan State University
This article was originally published on The Conversation. Read the original article.
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NASA's super-pressure balloon project has once again fallen short of its 100-day target, but still managed to set some records on the way.…
TechRepublic | Amazon's robot worker challenge won by AI-powered suction arm TechRepublic ... packing goods. Without automation, Amazon would be unable to ship items to millions of people each day and as the retail giant moves towards its goal of using drones to deliver packages within 30 minutes, it needs to continue to streamline delivery ... New warehouse robots roll out after Amazon corners marketArkansas Online Robotic arms race for online retailersFort Wayne Journal Gazette Adrian Weckler: Robots helped to cause Brexit - and they're not done yetIrish Independent all 9 news articles » |
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The Globe and Mail | Beauty and the bot: Artificial intelligence is the key to personalizing aesthetic products The Globe and Mail Physical beauty is subjective and often difficult to define. But for the robot jury of Beauty.AI, an online competition billed as “the first international beauty contest judged by artificial intelligence,” beauty is calculated by a set of complex ... |
Daily Mail | Robots could replace low-skilled migrant workers Daily Mail Summarising the findings, author Adam Corlett explained: 'Looking at those sectors with the highest proportion of EU migrants, we find that some such as cleaning and domestic staffing face relatively low prospects for automation, while others ... and more » |
The countdown is on for the Juno spacecraft to reach its destination at Jupiter in a matter of hours after a five-year journey, the first solar-powered spacecraft to travel this far from the sun. This evening, July 4, Juno will fire its main engine for 35 minutes, placing it into an eccentric polar orbit around the gas giant. At its closest approach, Juno's orbit will pass a mere 2,900 miles (4,667 kilometers) from Jupiter's cloud tops, closer than any previous spacecraft, and it will be moving at roughly 129,000 mph (65 kps), faster than any previous man-made object.
At that altitude, the probe will be subjected to the harshest radiation environment in the solar system. Jupiter's powerful magnetic field surrounds the planet with a doughnut-shaped field of high-energy electrons, protons, and ions traveling at nearly the speed of light.
Juno will orbit the gas giant 37 times over the next 20 months, with the goal that it will collect data and images that offer clues to the origins of our solar system and the formation of the planets and moons. It will be only the second time that a probe has gone into orbit around the giant planet.
The critical moment will be the end of the engine burn, at 11:53 p.m. Eastern time. NASA Television will begin coverage at 10:30 p.m.
The Daily Galaxy via NASA
China will launch a mission to land on the dark side of the moon in two years' time, state media reported, in what will be a first for humanity. The moon's far hemisphere is never directly visible from Earth and while it has been photographed, with the first images appearing in 1959, it has never been explored. Earlier reports from the Xinhua news agency hinted that China may be considering the construction of a pioneering radio telescope on the moons virgin far side, which will give it an unobstructed window on the Cosmos that was confirmed this June, 2016 when an agreement was announced between the Netherlands and China, that a Dutch-built radio antenna will travel to the Moon aboard the Chinese Chang'e 4 satellite and usher in a new era of radio astronomy allowing for the study of objects that might otherwise be invisible or hidden in other parts of the electromagnetic spectrum.
“Radio astronomers study the universe using radio waves, light coming from stars and planets, for example, which is not visible with the naked eye," commented Heino Falke a professor of Astroparticle Physics and Radio Astronomy at Radboud University. "We can receive almost all celestial radio wave frequencies here on Earth. We cannot detect radio waves below 30 MHz, however, as these are blocked by our atmosphere. It is these frequencies in particular that contain information about the early universe, which is why we want to measure them.”
The Chang'e-4 probe -- named for the goddess of the moon in Chinese mythology -- will be launched to it in 2018, the official Xinhua news agency reported. "The Chang'e-4's lander and rover will make a soft landing on the back side of the moon, and will carry out in-place and patrolling surveys," according to the country's lunar exploration chief Liu Jizhong.
Beijing sees its military-run, multi-billion-dollar space program as a marker of its rising global stature and mounting technical expertise, as well as evidence of the ruling Communist Party's success in transforming the once poverty-stricken nation.
But for the most part it has so far replicated activities that the US and Soviet Union pioneered decades ago. "The implementation of the Chang'e-4 mission has helped our country make the leap from following to leading in the field of lunar exploration," Liu added.
In 2013, China landed a rover dubbed Yutu on the moon and the following year an unmanned probe completed its first return mission to the earth's only natural satellite. Beijing has plans for a permanent orbiting station by 2020 and eventually to send a human to the moon.
Space flight is "an important manifestation of overall national strength", Xinhua cited science official Qian Yan as saying, adding that every success had "greatly stimulated the public's... pride in the achievements of the motherland's development."
Clive Neal, chair of the Lunar Exploration Analysis Group affiliated with NASA, confirmed that the Chang'e-4 mission was unprecedented. "There has been no surface exploration of the far side," he told AFP Friday. It is "very different to the near side because of the biggest hole in the solar system -- the South Pole-Aitken basin, shown above, which may have exposed mantle materials -- and the thicker lunar crust". The basin is the largest known impact crater in the solar system, nearly 2,500 kilometers wide and 13 kilometers deep.
The Daily Galaxy via NASA and Beijing (AFP) and Xinhua News Agency
Furnishing industry charity, The Furniture Makers' Company has revealed a new award that aims to increase exports of UK furnishing manufacturers.
The Export Award, which is open to any furnishings company that manufactures in Britain, has been introduced to help combat the current trade deficit of £3.3bn, according to figures from The Office for National Statistics.
Through the award, The Furniture Makers Company will acknowledge companies that already excel in export, and promote them as an example to other manufacturers.
Paul von der Heyde, chairman of the Manufacturing Guild Mark Committee, says: “The goal of the Export Award is to recognise and champion companies that are flying the flag for British manufacture in export markets.
“The UK has a great tradition of fine furniture, bedding and furnishing design and manufacturing and, while imitations are often manufactured overseas, there is an increasing demand for ‘the real thing'.”
Heyde is included among the panel of judges, alongside Ben Burbidge, master of the Worshipful Company of Furniture Makers; chief executive of the British Contracts Furniture Association, Jeremy Stein; chairman of the British Furniture Association, Jeremy Stein and Stephen McPartland MP, who is the chair of the All Party Parliamentary Furniture Industry Group.
When assessing applicants, judges will consider factors such as any development initiatives; growth; techniques; long term commitment and relevant accreditations.
To apply, applicants should fill out an entry form on The Furniture Makers' Company website before 31 August. More information is available here.
The post The Furniture Makers' Company looks to boost UK furniture exports with new award scheme appeared first on Design Week.
Jewellery designer Tatty Devine has designed a series of site specific installations at The Royal London Hospital's new building.
Vital Arts, the arts organisation for Barts Health NHS Trust has commissioned the works, which are entitled All That Glitters May Be Bones and now cover the children's imaging department.
Tatty Devine, which is known for its laser cut acrylic jewellery, has created thousands of bright acrylic pieces along the theme of x-rays and bones.
Waiting areas, corridors and treatment rooms have all been redesigned so that they're less frightening and more engaging for children according to Vital Arts.
Tatty Devine partner Rosie Wolfenden says the installations: “Will help make hospital visits a better experience for children, especially those within our local community.
“It was fantastic to realise our ideas in such a different environment and we hope it makes people smile for years to come.”
Barts Health lead paediatric radiographer at NHS Trust Martin Shute says: “Working closely with Vital Arts and Tatty Devine at the beginning of the project meant that the artists understood exactly how all the spaces within the imaging department are used, and the specificity of our patient demographics.
“The variety of colour serves to distinguish separate areas, including a soothing pink area for breastfeeding mothers, and an Autumnal palette for the adolescent waiting room, which, again, is different from the softer hues in the waiting area for our youngest patients”.
Royal London has worked with many artists and designers in recent years including Morag Myerscough, Tord Boontje and Chris Haughton.
The post Tatty Devine designs for Royal London Hospital appeared first on Design Week.
Small UK businesses could lose financial opportunities and support as a result of the EU referendum result, according to business lender Funding Circle.
On 20 June, prior to the EU referendum, it was announced that the European Investment Bank (EIB) would provide £100 million to support small British businesses, working with UK-based lender Funding Circle. Funding Circle provides loans of roughly £50,000 to businesses sized on average 30 people or less.
But following the majority Leave result on 24 June, co-founder at Funding Circle James Meekings told the Business, Innovation and Skills (BIS) Committee which assesses spending by governmental department BIS that the £100m funding project is now “at risk”.
“The deal with the EIB was a start to create a multi-billion pound programme for getting more funds into UK business,” Meekings says. “The programme is at risk. If I'm honest, it's very unlikely to happen now.”
According to Meekings, loans to Small and Medium-Sized Enterprises (SMEs) employ roughly 60% of people across the country.
In a statement, the EIB says it is yet to come to any decisions about its ties with the UK.
It says: “At present, the EIB's shareholders have not requested the Bank to change its approach to operations in the UK.
“It is premature to speculate on the impact of the referendum result on the EIB, including the Bank's future relationship with the UK Government and its future engagement to support long-term investment in the UK without clarity on the timing, circumstances and conditions of a withdrawal settlement.”
The majority of design consultancy businesses fall under the SME category small businesses are defined by Europa as those with a staff count of maximum 50, and a turnover of maximum €10 million (£8.4 million), while a medium-sized business is one with maximum 250 staff, and a turnover of maximum €50 million (£42 million).
Meekings adds that with doubts around funding from Europe, UK-based banks like the British Business Bank will need to be utilised, and the UK Government should be “putting more money in” to help SMEs.
“To date, we have had £60 million from the British Business Bank,” he says. “During this time of uncertainty, the British government should be backing small businesses.”
“Our question is what are the programmes that the Government could put in place given this new world of uncertainty to help get public funds and encourage growth and money directly into small businesses?” he says.
Marcus Stuttard, head of AIM, the London Stock Exchange's international market in place to help small companies grow, told the Business, Innovation and Skills Committee that the business community is looking for “certainty” so that they can “plan”.
“We would expect that companies will delay making investment decisions and therefore requesting finance as well,” he says. “The greatest thing we can all do is remain collaborative and provide as much certainty as quickly as possible.”
Samir Desai, chief executive officer at Funding Circle, says in a statement that investors are unlikely to be affected in the “short term”.
“Many of our UK small businesses do not trade with the European Union and are unlikely to be immediately affected,” says Desai. “Our small business customers have been trading for ten years on average, and have experienced economic volatility before. We have conducted rigorous stress tests on our loanbook which show that even in the most stressed conditions, investors will continue to earn positive returns.”
Deborah Dawton, chief executive officer at the Design Business Association, says of the design industry following the referendum vote: “UK design is world leading UK design is still a potent business asset and a sound commercial investment.”
According to the UK Government, between 2013 and 2014 the creative industries' value to the economy grew at almost double the rate of other UK industries, with design including product, graphic and fashion increasing the most at 16.6%. It also states the value of the creative industries was £84 billion in 2014 and accounted for 5% of the UK economy.
“The value design brings to the economy is undeniable,” says Dawton. “It is fundamentally important that this continues to be recognised.”
Creative Industries Federation (CIF) adds that while access to regional and sector-specific funding is a key concern for those working in the industry following Brexit, as is access to markets, IP protection and freedom of movement of talent.
In reaction to the vote, the organisation has announced it will be holding a series of “practical” events around the UK which will aim to “bring the sector together”, “marshal opinions” and “come to decisions” about the future.
The first meeting takes place in London on 7 July. A venue is yet to be announced.
The post Small businesses could lose financial support following EU referendum appeared first on Design Week.
Northern blue butterfly (Plebejus idas) collected in Churchill, Manitoba, Canada, and photographed at the Centre for Biodiversity Genomics (sample ID: 04HBL003084; specimen record: http://www.boldsystems.org/index.php/Public_RecordView?processid=LCH084-04)
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A very young baby cotton-top tamarin. Isn't it cute? You can see it near the entrance of the Singapore Zoo.
Taken at the Singapore Zoo.
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NASA's Juno spacecraft is set to enter its most critical stage as it attempts to fly into Jupiter's orbit.…
Irish Independent | New warehouse robots roll out after Amazon corners market Arkansas Online "Warehouses are very high-tech places," said Bruce Welty, co-founder and chairman of Locus Robotics, a firm that's developed robots to work alongside, rather than replace, human workers. "Because the only way you can take costs out is automation.". Robotic arms race for online retailersFort Wayne Journal Gazette Adrian Weckler: Robots helped to cause Brexit - and they're not done yetIrish Independent all 4 news articles » |
CNN | Giant spacecraft nears Jupiter CNN (CNN) It's been speeding toward Jupiter for nearly five years. Now -- can it slow down? On Monday, NASA's Juno spacecraft -- a spinning, robotic probe as wide as a basketball court -- will perform what the space agency calls a 35-minute long ... NASA Probe Ready for Fourth of July Rendezvous With JupiterNBCNews.com NASA Swears It Didn't Mean to Interrupt Your July 4 CookoutWIRED NASA's dangerous Juno mission: Unravel Jupiter's secrets and solve the mysteries of lifePhys.Org Scientific American -Wall Street Journal -International Business Times -Ars Technica all 308 news articles » |
Happy Fourth of July! The incredible shot shows the Statue of Liberty in New York City. The colossal copper structure depicts a robed female figure — Libertas, the Roman goddess of liberty — who bears a torch and a tablet upon which is inscribed the date of the American Declaration of Independence — July 4, 1776. The statue is an American icon of freedom and a welcoming sight to immigrants arriving from abroad. We hope everyone in the US has had a fantastic holiday weekend! ? by @jeffreymilstein (at Statue Of Liberty)
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Weathered chain on the beach by Chiswick Bridge at low tide.
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Fireworks Black Bean and Mango Salad
This salad is so quick and easy, it barely qualifies as a recipe. But it explodes with pizzazz, pairing the sweet summer burst mango (let's hear it for fresh, seasonal and local -- summer means mango season in South Florida) with a zing of chili. Black beans add fiber for fullness and protein because that's what your body wants. Besides, everything works with basic black. All this and it's fat-free, too.
Serve atop the fresh local farmers market greens of your choice.
1 jalapeno, minced (wear gloves when handling chilies -- really. Yes, even you.)
1 red pepper, diced
2 ribs celery, chopped fine
2 15-ounce cans black beans, rinsed and drained (or 4 cups cooked black beans)
1 teaspoon cumin
juice of 1/2 lime
2 mangos, peeled and diced
1 bunch cilantro, chopped
sea salt and fresh ground pepper to taste
1/4 cup toasted pepitas (pumpkin seeds) for garnish, optional but adding fabulous crunch, not to mention goodly amounts of manganese and magnesium
3-4 cups fresh greens like spinach, arugula or frisbee
In a large bowl, gently mix together jalapeno, diced red pepper and celery. Add the black beans and combine well.
Add the cumin and the lime and toss to coat.
Just before serving, add the mangos and chopped cilantro. Season to taste. Place atop greens and serve at once, garnishing with toasted pepitas, if you like (and you will).
Serves 4 to 6.
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Overall rates of the surgical snip have declined nationally in the past decade. But, despite advice, some hospitals and certain doctors still routinely cut the vagina to ease a baby's birth.
The genetic pathway toward social behavior for honey bees and mammals is more similar than previously thought, according to a new study published in PLOS Computational Biology titled "Conservation in Mammals of Genes Associated with Aggression-Related Behavioral Phenotypes in Honey Bees."…
We talk to Respawn Entertainment about its forthcoming sci-fi sequel, which adds a campaign mode, new weapons and fresh ideas, to the acclaimed original
When Jason West and Vince Zampella set up Respawn Entertainment in 2010, they had one ambition: to produce a new first-person shooter that would have as massive an impact on the genre as their previous creation: the Call of Duty series. It was a big ask, but when Titanfall arrived three years later, the game was certainly a brilliant attempt. The sci-fi shooter boasted an innovative mechanic allowing players to summon a giant robot into the arena, and an incredibly fluid, free-running movement style all combined into a set of blisteringly loud and detailed map designs.
But one thing many players said about Titanfall was that, beyond the raw speed and inarguable thrill of the highly vertical, highly acrobatic gameplay, there was little in the way of tactical depth. It's something the team says it wants to address.
Continue reading...Space navigation is tricky. There's no up or down, no left or right, and no road signs. This device uses stars to help determine if a spacecraft is off course. It takes nifty pictures, too.
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A whole pile of “this is how your brain looks like” MRI-based science has been invalidated because someone finally got around to checking the data.…
[Following is the censorship email Kull refers to above -- it was not written by Denis Noble:
"Could I request that you stop referring to the forthcoming RS-BA meeting ("New Trends in Evolutionary Biology: Biological, Philosophical and Social Science Perspectives"), and to the extended evolutionary synthesis, more generally, as in some way advocating a "paradigm shift". Such language is both misleading (the vast majority of scientists working towards an extended synthesis do not seek revolutionary change in neo-Darwinism) and counterproductive (such talk undermines calm scientific discussion by creating an unnecessarily emotive and antagonistic atmosphere). I view the Kuhnian model as superseded long ago: the data suggests that sciences rarely if ever change through "revolutions". Lakatos' framework of "research programmes" offers a more up-to-date, accurate and useful conceptualization of (gradual and progressive) scientific change. The extended evolutionary synthesis is best regarded as an alternative research programme, entirely complementary to orthodox evolutionary biology. Talk of "paradigm shift" gives the false impression that the differences amongst evolutionary biologists are far more extreme than they actually are. . . ."]
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Gameplanet | Black Ops III: Descent DLC brings dragons to CoD Gameplanet Descent features four new multiplayer maps, including a cryogenic prison, a Viking village, a giant robot combat arena, and a modern day reconstruction of an ancient Roman villa. The new DLC will also thrusts players to an alternate universe of Nikolai ... Call of Duty: Black Ops III Descent DLC Empire map previewed in new trailerFlickering Myth (blog) This Call of Duty: Black Ops II map could return in Black Ops IIIGamespresso The problem with Black Ops III multiplayer - Reader's FeatureMetro Express.co.uk -Gotta Be Mobile -Gamenguide -Parent Herald all 26 news articles » |
IGN India | A super-heavy soldier class expands our options. IGN India What I look for in expansions to a dynamic game like XCOM 2 are a means of increasing diversity and opportunities to change up not just my next campaign, but every game thereafter in interesting ways. Shen's Last Gift provides that, substantially ... 'XCOM 2' DLC, 'Shen's Last Gift' Promises Robot AlliesMovie News Guide XCOM 2 Short Circuits With Final Shen's Last Gift DLCGame Debate XCOM 2: Shen's Last Gift DLC Released, Video AvailableGamers Hell all 5 news articles » |
Satya Nadella sets rules for Artificial Intelligence Economic Times In a 1942 short story called Runaround, science fiction author Isaac Asimove formulated his famous 'Three Laws of Robotics'. As per the Handbook of Robotics, 56th Edition, 2058 AD, the three laws are: A robot may not injure a human being or, through ... |
Robotic arms race for online retailers Fort Wayne Journal Gazette After all, Kiva bots proved that this kind of automation is more efficient than an all-human workforce. The only problem was that there were no other options. Kiva was pretty much it. It's taken four years, but a handful of startups are finally ready ... |
The Vitra Design Museum in Germany has opened a new archive and exhibition space, called Schaudepot, which houses a collection of approximately 7,000 designs including prototypes of 20th century classics by Charles and Ray Eames.
The Swiss furniture manufacturer's collections were previously stowed underground and out of public view, but the Schaudepot, directly translating to “show depot”, brings the collections out of hiding and into the open.
The 1,000m2 addition was designed by Basel-based architecture firm Herzog & de Meuron, who designed the recent addition to the Tate Modern. Basel-based studio Dieter Thiel designed the interior and exhibition spaces. Thiel previously worked with Vitra on exhibition design and has done projects for Adidas, pen manufacturer Lamy and lighting company Ansorg, among others.
The centrepiece of the Schaudepot is a permanent exhibition with more than 400 pieces of modern industrial design from 1800 to the present, including early Bentwood design, Classical Modernist icons by Le Corbusier, Alvar Aalto and Gerrit Rietveld, colourful Pop-era plastics and more recent 3D printed designs.
The permanent exhibition, which features the chronological “canon of Vitra” along with some lesser-known pieces, is accompanied by smaller temporary exhibitions relating to the main collection, beginning with a 430-piece display that follows the history of furniture design from the late 18th century to present.
The modern interior design makes use of large steel and glass shelving and fluorescent lighting to eschew showiness and emphasise the furniture designs as the focal point in a cathedral-like space, says the Vitra Design Museum's chief curator Jochen Eisenbrand. Each design is assigned a number, which patrons can enter into a tablet to learn more information about the piece's designer, manufacturer and date of creation. As its name suggests, the building's curatorial design aestheticises its function as an open-viewing storehouse.
“Dieter Thiel decided to move away from the too-busy shelving system that we had used on other projects for a more minimal and flexible design that can be moved up or down depending on what pieces go in it,” says Eisenbrand. “We wanted the pieces to be the main source of visual interest in the space.”
The building's basement, which formerly housed the collection out of public view, can now be accessed via a staircase. Four large windows invite visitors to peer in at the Scandinavian, Italian, lighting and Eames collections.
“We're just relieved and excited to finally have the space to bring the pieces out of storage and into the public museum. Many of them have been in storage since 1989 when the main museum opened,” says Eisenbrand.
The building sits on the Vitra campus, which acts as a hub for the Swiss furniture manufacturer and was visited by 350,000 people last year. The site features buildings by contemporary architects including Frank Gehry, Tadao Ando and the late Zaha Hadid.
All images courtesy of the Vitra Design Museum.
The post Vitra Design Museum opens new exhibition space showcasing design classics appeared first on Design Week.
Exactly what powered the dynamo remains a mystery. One possibility is that the lunar dynamo was self-sustaining, like Earth's: As the planet has cooled, its liquid core has moved in response, sustaining the dynamo and the magnetic field it produces. In the absence of a long-lived heat supply, most planetary bodies will cool within hundreds of millions of years of formation.
MIT's research on an ancient lunar rock in 2011 suggested that the moon harbored the long-lived dynamo — a molten, convecting core of liquid metal that generated a strong magnetic field 3.56 billion years ago. The findings point to a dynamo that lasted much longer than scientists previously thought, and suggest that an alternative energy source may have powered the dynamo.
The magnetic field existed until at least 3.56 billion years ago, an MIT study suggests — about 160 million years longer than scientists had thought. “It seems like the lunar dynamo lasted very late in the Moon's history,” says Benjamin Weiss, a palaeomagnetics expert at the Massachusetts Institute of Technology (MIT) in Cambridge. “That's a very surprising result.” Weiss and his colleagues, led by MIT planetary scientist Clément Suavet, report the findings today in the Proceedings of the National Academy of Sciences1.
“The moon has this protracted history that's surprising,” says Weiss, an associate professor of planetary science at MIT. “This provides evidence of a fundamentally new way of making a magnetic field in a planet a new power source.”
The MIT paper is the latest piece in a puzzle that planetary scientists have been working out for decades. In 1969, the Apollo 11 mission brought the first lunar rocks back to Earth — souvenirs from Neil Armstrong and Buzz Aldrin's historic moonwalk. Since then, scientists have probed the rocky remnants for clues to the moon's history. They soon discovered that many rocks were magnetized, which suggested that the moon was more than a cold, undifferentiated pile of space rubble. Instead, it may have harbored a convecting metallic core that produced a large magnetic field, recorded in the moon's rocks.
A dynamo still exists within Earth because heat, produced by the radioactive decay of elements within the planet, maintains the core's convection. Models have shown that if a lunar dynamo were powered solely by cooling of the moon's interior, it would have been able to sustain itself only for a few hundred million years after the moon formed — dissipating by 4.2 billion years ago, at the very latest.
However, Weiss and his colleagues found some surprising evidence in a bit of lunar basalt dubbed 10020. The Apollo 11 astronauts collected the rock at the southwestern edge of the Sea of Tranquility; scientists believe it was likely ejected from deep within the moon 100 million years ago, after a meteor impact. The group confirmed previous work dating the rock at 3.7 billion years old, and found that it was magnetized — a finding that clashes with current dynamo models.
Weiss collaborated with researchers at the University of California at Berkeley and the Berkeley Geochronology Center, who determined the rock's age using radiometric dating. After a rock forms, a radioactive potassium isotope decays to a stable argon isotope at a known rate. The group measured the ratio of potassium to argon in a small piece of the rock, using this information to ascertain that the rock cooled from magma 3.7 billion years ago.
Weiss and graduate student Erin Shea then measured the rock's magnetization, and found that the rock was magnetized. However, this didn't necessarily mean that the rock, and the moon, had a dynamo-generated magnetic field 3.7 billion years ago: Subsequent impacts may have heated the rock and reset its magnetization.
To discard this possibility, the team examined whether the rock experienced any significant heating since its ejection onto the moon's surface. Again, they looked to isotopes of potassium and argon, finding that the only heating the rock had experienced since it was ejected onto the lunar surface came from simple exposure to the sun's rays.
“It's basically been in cold storage for 3.7 billion years, essentially undisturbed,” Weiss says. “It retains a beautiful magnetization record.”
Weiss says the rock's evidence supports a new mechanism of dynamo generation that was proposed by scientists at University of California at Santa Cruz (UCSC). This hypothesis posits that the moon's dynamo may have been powered by Earth's gravitational pull. Billions of years ago, the moon was much closer to Earth than it is today; terrestrial gravity may have had a stirring effect within the moon's core, keeping the liquid metal moving even after the lunar body had cooled.
Francis Nimmo, a professor of earth and planetary sciences at UCSC and one of the researchers who originally put forth the new dynamo theory, says Weiss' evidence provides scientists with a new picture of the moon's evolution.
“We generally assume that cooling is the main mechanism for driving a dynamo anywhere,” says Nimmo, who was not involved in the study. “This lunar data is telling us that other mechanisms may also play a role, not just at the moon, but elsewhere, too.”
The Daily Galaxy via Massachusetts Institute of Technology and nature.com
China's bolted down the last mirror of its Five-hundred-metre Aperture Spherical Telescope (FAST), put away the hex key, and is about to start trial observations with the instrument.…
using ordinary objects from rubber bands and rope, to shoelaces and sponges, the graphic designer has created the ongoing series 'food not food'.
The post kristina lechner cooks up domestic-object dishes from household products appeared first on designboom | architecture & design magazine.
by choosing to edit recognizable photographs, the artist intends to maintain the original aspects of the celebrity beneath layers of skin and wrinkles.
The post sara zaher imagines how late famous figures might look today appeared first on designboom | architecture & design magazine.
309
Argentinean poster for THE DEER HUNTER (Michael Cimino, USA, 1978)
Artist: uncredited
Poster source: Heritage Auctions
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Sometimes the very best can be found very close to home...
Bloomberg:
Four years after Amazon acquired Kiva, a handful of startups look to fill the void by equipping warehouses with robots — In 2012 Jeff Bezos scooped up warehouse automation firm Kiva. Everyone else is still trying to catch up. — An Amazon warehouse is a flurry of activity.
Alex Stoen posted a photo:
During a recent workshop with Alex and Rebecca Webb, I had to submit one photo inspired on the light in London. I made it my daily quest to get out on the streets every day just before sunset in search of a special moment. This is one of them, taken from the Southbank, facing the Palace of Westminster, with its iconic Big Ben.
© 2016 Alex Stoen, All rights reserved.
No Group Invites/Graphics Please.
www.alexstoen.com
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1st July 2016
Setting sun over the city of London seen from Greenwich Park
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London, England.
Olympus OM-D E-M10.
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Space navigation is tricky. There's no up or down, no left or right, and no road signs. This device uses stars to help determine if a spacecraft is off course. It takes nifty pictures, too.
Read more: Viral Video, Gif, Bon Jovi, Postmodern Jukebox, You Give Love a Bad Name, Entertainment News
The craft is designed to glean data from Jupiter that could also help us learn how Earth formed. But first, Juno has to get into orbit — determined by a crucial half-hour of firing by its main engine.
strupert posted a photo:
One more from the Thames barrier
Officers can instantly freeze or seize the funds loaded on prepaid cards using the handheld device, and some civil liberties advocates say the machines may be abused.
From a profile of Samantha Bee to the views of Chelsea Manning on the military's new transgender rules, these stories are about how we see the world.
Former counterterrorism coordinator for Homeland Security John Cohen tells NPR's Scott Simon why the federal government may ask Visa Waiver Program applicants to hand over social media account info.
The first reported death involving a driverless car raises questions about their future. Not just over safety concerns, but our own attitudes to relinquishing control.
Star Swain did a spontaneous rendition of the national anthem at the Lincoln Memorial and a friend caught it on video. The clip has since gone viral, and changed the way Swain thinks about her future.
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Happy Independence weekend to my American Flickr friends! Have an enjoyable 4th of July weekend
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Listen to Jupiter's strange voice as the robotic explorer moves into the magnetic field and enters into a polar orbit around the gas giant. "We have over five years of spaceflight experience and only 10 days to Jupiter orbit insertion," said Rick Nybakken, Juno project manager from NASA's Jet Propulsion Laboratory in Pasadena, California. "It is a great feeling to put all the interplanetary space in the rearview mirror and have the biggest planet in the solar system in our windshield."
In three days, July 4th, the spacecraft Juno will arrive at Jupiter, the culmination of a five-year, billion-dollar journey. It's mission: to peer deep inside the gas giant and unravel its origin and evolution. One of the biggest mysteries surrounding Jupiter is how it generates its powerful magnetic field, the strongest in the solar system.
One theory is that about halfway to Jupiter's core, the pressures and temperatures become so intense that the hydrogen that makes up 90 percent of the planet -- molecular gas on Earth -- looses hold of its electrons and begins behaving like a liquid metal. Oceans of liquid metallic hydrogen surrounding Jupiter's core would explain its powerful magnetic field.
But how and when does this transition from gas to liquid metal occur? How does it behave? Researchers hope that Juno will shed some light on this exotic state of hydrogen -- but one doesn't need to travel all the way to Jupiter to study it.
Four hundred million miles away, in a small, windowless room in the basement of Lyman Laboratory on Oxford Street in Cambridge, Massachusetts, there was, for a fraction of a fraction of a second, a small piece of Jupiter.
Earlier this year, in an experiment about five-feet long, Harvard University researchers say they observed evidence of the abrupt transition of hydrogen from liquid insulator to liquid metal. It is one of the first times such a transition has ever been observed in any experiment.
"This is planetary science on the bench," said Mohamed Zaghoo, the NASA Earth & Space Science Fellow at the Harvard John A. Paulson School of Engineering and Applied Sciences (SEAS). "The question of how hydrogen transitions into a metallic state -- whether that is an abrupt transition or not -- has huge implications for planetary science. How hydrogen transitions inside Jupiter, for example, says a lot about the evolution, the temperature and the structure of these gas giants interiors."
In the experiment, Zaghoo, Ashkan Salamat, and senior author Isaac Silvera, the Thomas D. Cabot Professor of the Natural Sciences, recreated the extreme pressures and temperatures of Jupiter by squeezing a sample of hydrogen between two diamond tips, about 100 microns wide, and firing short bursts of lasers of increasing intensity to raise the temperature.
This experimental setup is significantly smaller and cheaper than other current techniques to generate metallic hydrogen, most of which rely on huge guns or lasers that generate shock waves to heat and pressurize hydrogen.
The transition of the liquid to metallic hydrogen happens too quickly for human eyes to observe and the sample lasts only a fraction of a second before it deteriorates. So, instead of watching the sample itself for evidence of the transition, the team watched lasers pointed at the sample. When the phase transition occurred, the lasers abruptly reflected.
"At some point, the hydrogen abruptly transitioned from an insulating, transparent state, like glass, to a shiny metallic state that reflected light, like copper, gold or any other metal," Zaghoo said. "Because this experiment, unlike shock wave experiments, isn't destructive, we could run the experiment continuously, doing measurements and monitoring for weeks and months to learn about the transition."
"This is the simplest and most fundamental atomic system, yet modern theory has large variances in predictions for the transition pressure," Silvera said. "Our observation serves as a crucial guide to modern theory."
The results represent a culmination of decades of research by the Silvera group. The data collected could begin to answer some of the fundamental questions about the origins of solar systems.
Metallic hydrogen also has important ramifications here on Earth, especially in energy and materials science. "A lot of people are talking about the hydrogen economy because hydrogen is combustibly clean and it's very abundant," said Zaghoo. "If you can compress hydrogen into high density, it has a lot of energy compacted into it."
"As a rocket fuel, metallic hydrogen would revolutionize rocketry as propellant an order of magnitude more powerful than any known chemical," said Silvera. "This could cut down the time it takes to get to Mars from nine months to about two months, transforming prospects of human space endeavors."
Metallic hydrogen could be used to make room temperature or even higher than room temperature super-conductors. The Juno mission goes hand-in-hand with laboratory experiments into metallic hydrogen, Zaghoo said."The measurements of Jupiter's magnetic field that Juno will be collecting is directly related to our data," he said. "We're not in competition with NASA but, in some ways, we got to Jupiter first."
In the Gemini Observatory image at the top of the page, white indicates cloud features at relatively high altitudes; blue indicates lower cloud structures; and red represents still deeper cloud features. The two red spots appear more white than red, because their tops hover high above the surrounding clouds. Also prominent is the polar stratospheric haze, which makes Jupiter bright near the pole. Other tiny white spots are regions of high clouds, like towering thunderheads. In visible light Jupiter looks orangish, but in the near-infrared the blue color is due to strong absorption features. The blue mid-level clouds are also closest to what one would see in a visual light image.
The Daily Galaxy via NASA and Harvard University
"The most exciting possibility is that the missing photons are coming from some exotic new source, not galaxies or quasars at all," said Neal Katz of the University of Massachusetts at Amherst. "For example, the mysterious dark matter, which holds galaxies together but has never been seen directly, could itself decay and ultimately be responsible for this extra light. You know it's a crisis when you start seriously talking about decaying dark matter!"
"It's as if you're in a big, brightly-lit room, but you look around and see only a few 40-watt light bulbs," says Carnegie Institute's Juna Kollmeier. "Where is all that light coming from? It's missing from our census."
The vast reaches of empty space between galaxies are bridged by tendrils of hydrogen and helium, which can be used as a precise "light meter." In a recent study published in The Astrophysical Journal Letters, a team of scientists finds that the light from known populations of galaxies and quasars is not nearly enough to explain observations of intergalactic hydrogen. The difference is a stunning 400 percent.
"The great thing about a 400% discrepancy is that you know something is really wrong," commented co-author David Weinberg of The Ohio State University. "We still don't know for sure what it is, but at least one thing we thought we knew about the present day universe isn't true."
Strangely, this mismatch only appears in the nearby, relatively well-studied cosmos. When telescopes focus on galaxies billions of light years away (and therefore are viewing the universe billions of years in its past), everything seems to add up. The fact that this accounting works in the early universe but falls apart locally has scientists puzzled.
The light in question consists of highly energetic ultraviolet photons that are able to convert electrically neutral hydrogen atoms into electrically charged ions. The two known sources for such ionizing photons are quasars—powered by hot gas falling onto supermassive black holes over a million times the mass of the sun—and the hottest young stars.
Observations indicate that the ionizing photons from young stars are almost always absorbed by gas in their host galaxy, so they never escape to affect intergalactic hydrogen. But the number of known quasars is far lower than needed to produce the required light.
"Either our accounting of the light from galaxies and quasars is very far off, or there's some other major source of ionizing photons that we've never recognized," Kollmeier said. "We are calling this missing light the photon underproduction crisis. But it's the astronomers who are in crisis—somehow or other, the universe is getting along just fine."
The mismatch emerged from comparing supercomputer simulations of intergalactic gas to the most recent analysis of observations from Hubble Space Telescope's Cosmic Origins Spectrograph. "The simulations fit the data beautifully in the early universe, and they fit the local data beautifully if we're allowed to assume that this extra light is really there," explained Ben Oppenheimer a co-author from the University of Colorado. "It's possible the simulations do not reflect reality, which by itself would be a surprise, because intergalactic hydrogen is the component of the Universe that we think we understand the best."
The Daily Galaxy via the Carnegie Institution.
308
Danish poster for THE HEIRESS (William Wyler, USA, 1949)
Artist: BS
Poster source: MTime
Happy 100th Birthday (and a day) Olivia de Havilland
the exhibition brings together literature, architecture, philosophy and sound.
The post pedro reyes presents ‘savage sunday' at la tallera gallery in cuernavaca appeared first on designboom | architecture & design magazine.
PatrickJamesB posted a photo:
On June 2, the government held a press meeting to announce that the cause behind the deaths had been identified, but it was being challenged by experts in order to ensure it was based on scientific, legal, and objective grounds before a final conclusion was confirmed.
What, for journalists, was largely apolitical investigative work now has a stronger political background thanks to a growing number of young activists and a more general unease over both pollution and food security in the population.
This social media aspect of journalism can have the effect of distortion: untruths can be propagated in a blogosphere unrestricted by editorial standards. Even so, the reporting feels more honest than the official line printed in the papers.
As food safety becomes a strong preoccupation, the environmental movement is going to pick up steam. And the freedom to report on it might be waning -- for now at least.
-- This feed and its contents are the property of The Huffington Post, and use is subject to our terms. It may be used for personal consumption, but may not be distributed on a website.
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London timelapse sunrise
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Canary Wharf & O2 from Pontoon Dock DLR
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Jeongwang-dong is an industrial sector in the city of Ansan, South Korea. The Korean government intensively drove a plan to develop the modern city, particularly in this area, with an emphasis on manufacturing. The striking blue color that you see here results from the use of aluminum roofing, which is used for its low cost and longevity. /// Source imagery: @digitalglobe (at Ansan South Korea)
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Beautiful rainbow last night out our back window.
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Emirates Cable Car
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Westminster
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Sky Garden
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Greenwich Pier
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Heron Quays
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Hay's Galleria, late evening, from the warf walk.
OMD EM5Mll; Oly 12-40 f2.8 Pro; 1/8 @ f8; 16mm; ISO 800
Like many artists, Lily Nishita has been drawing for as long as she can remember. “The story my family told me is that I could hold a pencil before I could really talk,” she says. A steady diet of cartoons and animated movies led her to think about working in animation, but eventually she shifted gears and went on to study graphic design at school. “In retrospect I'd probably be really terrible doing anything else,” she says.
Nishita went on to freelance for several years, and more recently she's been working at Naughty Dog — the studio behind games like The Last of Us and Uncharted — helping steer the company's visual design. That includes everything from slight tweaks to the studio's logo to creating adorable digital stickers for...
Entomologist Sara Lewis talks about Photuris, a species of firefly that lures males of other species in and eats them.
The National Highway Traffic Safety Administration is investigating a fatal crash involving a Tesla car using the "autopilot" feature. NPR's Robert Siegel talks to Alex Davies of Wired about the crash and what it means for self-driving car technology.
Virtually all major car and tech companies are pursuing self-driving technology as the future of transportation. But Tesla and Google are the earliest innovators, taking very different approaches.
The fatal crash of a Model S that was in autopilot when it collided with a truck in Florida is prompting a preliminary evaluation of the feature by the National Highway Transportation Safety Board.
ShutterJack posted a photo:
Took this with my iPhone as I couldn't get a low enough angle with my D800. Just love the beauty of mushrooms!
WHO WE ARE
EDITORS: Nathan Gardels, Co-Founder and Executive Advisor to the Berggruen Institute, is the Editor-in-Chief of The WorldPost. Kathleen Miles is the Executive Editor of The WorldPost. Farah Mohamed is the Managing Editor of The WorldPost. Alex Gardels and Peter Mellgard are the Associate Editors of The WorldPost. Suzanne Gaber is the Editorial Assistant of The WorldPost. Katie Nelson is the National Editor at the Huffington Post, overseeing The WorldPost and HuffPost's editorial coverage. Charlotte Alfred and Nick Robins-Early are World Reporters. Rowaida Abdelaziz is Social Media Editor.
CORRESPONDENTS: Sophia Jones in Istanbul
EDITORIAL BOARD: Nicolas Berggruen, Nathan Gardels, Arianna Huffington, Eric Schmidt (Google Inc.), Pierre Omidyar (First Look Media) Juan Luis Cebrian (El Pais/PRISA), Walter Isaacson (Aspen Institute/TIME-CNN), John Elkann (Corriere della Sera, La Stampa), Wadah Khanfar (Al Jazeera), Dileep Padgaonkar (Times of India) and Yoichi Funabashi (Asahi Shimbun).
VICE PRESIDENT OF OPERATIONS: Dawn Nakagawa.
CONTRIBUTING EDITORS: Moises Naim (former editor of Foreign Policy), Nayan Chanda (Yale/Global; Far Eastern Economic Review) and Katherine Keating (One-On-One). Sergio Munoz Bata and Parag Khanna are Contributing Editors-At-Large.
The Asia Society and its ChinaFile, edited by Orville Schell, is our primary partner on Asia coverage. Eric X. Li and the Chunqiu Institute/Fudan University in Shanghai and Guancha.cn also provide first person voices from China. We also draw on the content of China Digital Times. Seung-yoon Lee is The WorldPost link in South Korea.
Jared Cohen of Google Ideas provides regular commentary from young thinkers, leaders and activists around the globe. Bruce Mau provides regular columns from MassiveChangeNetwork.com on the "whole mind" way of thinking. Patrick Soon-Shiong is Contributing Editor for Health and Medicine.
ADVISORY COUNCIL: Members of the Berggruen Institute's 21st Century Council and Council for the Future of Europe serve as the Advisory Council -- as well as regular contributors -- to the site. These include, Jacques Attali, Shaukat Aziz, Gordon Brown, Fernando Henrique Cardoso, Juan Luis Cebrian, Jack Dorsey, Mohamed El-Erian, Francis Fukuyama, Felipe Gonzalez, John Gray, Reid Hoffman, Fred Hu, Mo Ibrahim, Alexei Kudrin, Pascal Lamy, Kishore Mahbubani, Alain Minc, Dambisa Moyo, Laura Tyson, Elon Musk, Pierre Omidyar, Raghuram Rajan, Nouriel Roubini, Nicolas Sarkozy, Eric Schmidt, Gerhard Schroeder, Peter Schwartz, Amartya Sen, Jeff Skoll, Michael Spence, Joe Stiglitz, Larry Summers, Wu Jianmin, George Yeo, Fareed Zakaria, Ernesto Zedillo, Ahmed Zewail, and Zheng Bijian.
From the Europe group, these include: Marek Belka, Tony Blair, Jacques Delors, Niall Ferguson, Anthony Giddens, Otmar Issing, Mario Monti, Robert Mundell, Peter Sutherland and Guy Verhofstadt.
-- This feed and its contents are the property of The Huffington Post, and use is subject to our terms. It may be used for personal consumption, but may not be distributed on a website.
-- This feed and its contents are the property of The Huffington Post, and use is subject to our terms. It may be used for personal consumption, but may not be distributed on a website.
- Because of exponential growth since World War II, we now live in a full world, but we still behave as if it were empty.
- That richer (more net wealth) is better than poorer is a truism. The relevant question, though, is, does growth still make us richer, or has it begun to make us poorer by increasing "illth" faster than wealth?
- Examples of "illth" are everywhere, even if they are still unmeasured in national accounts. They include things like nuclear wastes, climate change from excess carbon in the atmosphere, biodiversity loss, depleted mines, deforestation, eroded topsoil, dry wells and rivers, sea level rise, the dead zone in the Gulf of Mexico, gyres of plastic trash in the oceans, and the ozone hole.
- Their refusal to acknowledge [ecological limits] is why many economists cannot conceive of the possibility that growth in GDP could ever be uneconomic.
- The economy should not be used as an idiot machine dedicated to maximizing waste.
- Our vision and policies should be based on the integrated view of the economy as a subsystem of the finite and non-growing ecosphere.
- And, quoting John Ruskin, "There is no wealth but life."
-- This feed and its contents are the property of The Huffington Post, and use is subject to our terms. It may be used for personal consumption, but may not be distributed on a website.
-- This feed and its contents are the property of The Huffington Post, and use is subject to our terms. It may be used for personal consumption, but may not be distributed on a website.
NASA's Science Program Support Office posted a photo:
NASA Goddard Photo and Video posted a photo:
From June 28 through 30, 2016, the OPTIMUS PRIME Spinoff Promotion and Research Challenge (OPSPARC) gave the contest's winning students the opportunity to explore NASA's Goddard Space Flight Center in Greenbelt, Maryland.
Three teams of students from elementary, middle and high school won the contest by creating the most popular ideas to use NASA technology in new and innovative ways. The students used an online platform called Glogster to make posters about their ideas, and the general public voted for their favorites.
Sophia Sheehan won the elementary school prize for her invention of the “blow coat,” which would be powered by solar panels and blow warm air into winter coats, helping people in her hometown of Chicago stay warm in the winter. Heidi Long, Aubrey Nesti, Katherine Valbuena and Jasmine Wu won in the middle school category for their idea called Tent-cordion, which would use spacesuit and satellite insulation materials in a foldable tent to house refugees and the homeless. Finally, Jake Laddis, Alex Li, Isaac Wecht and Isabel Wecht won in the high school category for their idea to use James Webb Space Telescope sunshield technology to shield houses from summer heat and reduce the need for air conditioning around the world. The high school winners also had the opportunity to compete in the NASA InWorld challenge, sponsored by the James Webb Space Telescope project, and continued developing their idea in a virtual world and gaming environment.
During their three-day workshop at Goddard, the students toured the center, met with scientists and engineers, took a look at the James Webb Space Telescope in Goddard's clean room, and even made their own videos in Goddard's TV studio. One of the students talked about how the experience inspired her. Read more: go.nasa.gov/298fGdQ
Alternative one sheet design for BOY AND THE WORLD (Alê Abreu, Brazil, 2013)
Design: Paul Jeffrey/Passage
Poster source: Paul Jeffrey
US one sheet for THE CHILDHOOD OF A LEADER (Brady Corbet, UK/France, 2015)
Designer: Brandon Schaefer
Poster source: SeekandSpeak
307
^^this person :)
the unique motives generated are constantly repeated in an addictive, disturbing and poetic way at the same time.
The post david moreno's sculptures create with steel rods drawings in space appeared first on designboom | architecture & design magazine.
Astronomers have spotted glowing droplets of condensed water in the distant Spiderweb Galaxy but not where they expected to find them. Detections with the Atacama Large Millimeter/submillimeter Array (ALMA) show that the water is located far out in the galaxy and therefore cannot be associated with central, dusty, star-forming regions, as previously thought.
“Observations of light emitted by water and by dust often go hand-in-hand. We usually interpret them as an insight into star-forming regions, with the illumination from young stars warming dust particles and water molecules until they start to glow. Now, thanks to the power of ALMA, we can -- for the first time -- separate out the emissions from the dust and water populations, and pinpoint their exact origins in the galaxy. The results are quite unexpected in that we've found that the water is located nowhere near the dusty stellar nurseries,” explained Bitten Gullberg, of the Centre for Extragalactic Astronomy, Durham University, UK.
The Spiderweb Galaxy above as seen by the Hubble Space Telescope (optical) in red, the Very Large Array (radio) in green and the Atacama Large Millimeter/submillimeter Array (sub-millimetre) in blue. The red colour shows where the stars are located within this system of galaxies. The radio jet is shown in green, and the position of the dust and water are seen in blue. The water is located to the left and right of the central galaxy. The water to the right is at the position where the radio jet bends down wards. The dust is also seen in blue. The dust is located at the central galaxy and in smaller companion galaxies in its surroundings. Credit: NASA/ESA/HST/STScI/NRAO/ESO
The Spiderweb Galaxy is one of the most massive galaxies known. It lies 10 billion light-years away and is made up of dozens of star-forming galaxies in the process of merging together. The ALMA observations show that the light from the dust originates in the Spiderweb Galaxy itself. However, the light from the water is concentrated in two regions far to the east and west of the galaxy core.
Gullberg and her colleagues believe that the explanation lies with powerful jets of radio waves that are ejected from a supermassive black hole at the centre of the Spiderweb Galaxy. The radio jets compress clouds of gas along their path and heat up water molecules contained within the clouds until they emit radiation.
“Our results show how important it is to pinpoint the exact locations and origins for light in galaxies. We may also have new clues to the processes that trigger star formation in interstellar clouds,” said Gullberg. “Stars are born out of cold, dense molecular gas. The regions in the Spiderweb where we've detected water are currently too hot for stars to form. But the interaction with the radio jets changes the composition of the gas clouds. When the molecules have cooled down again, it will be possible for the seeds of new stars to form. These “dew drop” regions could become the next stellar nurseries in this massive, complex galaxy.”
The Daily Galaxy via RAS
In three days, July 4th, the spacecraft Juno will arrive at Jupiter, the culmination of a five-year, billion-dollar journey. It's mission: to peer deep inside the gas giant and unravel its origin and evolution. One of the biggest mysteries surrounding Jupiter is how it generates its powerful magnetic field, the strongest in the solar system.
One theory is that about halfway to Jupiter's core, the pressures and temperatures become so intense that the hydrogen that makes up 90 percent of the planet -- molecular gas on Earth -- looses hold of its electrons and begins behaving like a liquid metal. Oceans of liquid metallic hydrogen surrounding Jupiter's core would explain its powerful magnetic field.
But how and when does this transition from gas to liquid metal occur? How does it behave? Researchers hope that Juno will shed some light on this exotic state of hydrogen -- but one doesn't need to travel all the way to Jupiter to study it.
Four hundred million miles away, in a small, windowless room in the basement of Lyman Laboratory on Oxford Street in Cambridge, Massachusetts, there was, for a fraction of a fraction of a second, a small piece of Jupiter.
Earlier this year, in an experiment about five-feet long, Harvard University researchers say they observed evidence of the abrupt transition of hydrogen from liquid insulator to liquid metal. It is one of the first times such a transition has ever been observed in any experiment.
"This is planetary science on the bench," said Mohamed Zaghoo, the NASA Earth & Space Science Fellow at the Harvard John A. Paulson School of Engineering and Applied Sciences (SEAS). "The question of how hydrogen transitions into a metallic state -- whether that is an abrupt transition or not -- has huge implications for planetary science. How hydrogen transitions inside Jupiter, for example, says a lot about the evolution, the temperature and the structure of these gas giants interiors."
In the experiment, Zaghoo, Ashkan Salamat, and senior author Isaac Silvera, the Thomas D. Cabot Professor of the Natural Sciences, recreated the extreme pressures and temperatures of Jupiter by squeezing a sample of hydrogen between two diamond tips, about 100 microns wide, and firing short bursts of lasers of increasing intensity to raise the temperature.
This experimental setup is significantly smaller and cheaper than other current techniques to generate metallic hydrogen, most of which rely on huge guns or lasers that generate shock waves to heat and pressurize hydrogen.
The transition of the liquid to metallic hydrogen happens too quickly for human eyes to observe and the sample lasts only a fraction of a second before it deteriorates. So, instead of watching the sample itself for evidence of the transition, the team watched lasers pointed at the sample. When the phase transition occurred, the lasers abruptly reflected.
"At some point, the hydrogen abruptly transitioned from an insulating, transparent state, like glass, to a shiny metallic state that reflected light, like copper, gold or any other metal," Zaghoo said. "Because this experiment, unlike shock wave experiments, isn't destructive, we could run the experiment continuously, doing measurements and monitoring for weeks and months to learn about the transition."
"This is the simplest and most fundamental atomic system, yet modern theory has large variances in predictions for the transition pressure," Silvera said. "Our observation serves as a crucial guide to modern theory."
The results represent a culmination of decades of research by the Silvera group. The data collected could begin to answer some of the fundamental questions about the origins of solar systems.
Metallic hydrogen also has important ramifications here on Earth, especially in energy and materials science. "A lot of people are talking about the hydrogen economy because hydrogen is combustibly clean and it's very abundant," said Zaghoo. "If you can compress hydrogen into high density, it has a lot of energy compacted into it."
"As a rocket fuel, metallic hydrogen would revolutionize rocketry as propellant an order of magnitude more powerful than any known chemical," said Silvera. "This could cut down the time it takes to get to Mars from nine months to about two months, transforming prospects of human space endeavors."
Metallic hydrogen could be used to make room temperature or even higher than room temperature super-conductors. The Juno mission goes hand-in-hand with laboratory experiments into metallic hydrogen, Zaghoo said."The measurements of Jupiter's magnetic field that Juno will be collecting is directly related to our data," he said. "We're not in competition with NASA but, in some ways, we got to Jupiter first."
In the Gemini Observatory image at the top of the page, white indicates cloud features at relatively high altitudes; blue indicates lower cloud structures; and red represents still deeper cloud features. The two red spots appear more white than red, because their tops hover high above the surrounding clouds. Also prominent is the polar stratospheric haze, which makes Jupiter bright near the pole. Other tiny white spots are regions of high clouds, like towering thunderheads. In visible light Jupiter looks orangish, but in the near-infrared the blue color is due to strong absorption features. The blue mid-level clouds are also closest to what one would see in a visual light image.
The Daily Galaxy via Harvard University
"Both the planet we live on and the star we orbit are made up of 'normal' matter," said Tanmay Vachaspati a theoretical physicist at Arizona State University working at the intersections of particle physics, astrophysics, general relativity, and cosmology. "Although it features in many science fiction stories, antimatter seems to be incredibly rare in nature. With this new result, we have one of the first hints that we might be able to solve this mystery."
In 2001 Vachaspati published theoretical models to try to solve this puzzle, which predict that the entire universe is filled with helical (screw-like) magnetic fields. He and his team were inspired to search for evidence of these fields in data from the NASA Fermi Gamma ray Space Telescope (FGST). Vachaspati has written extensively on cosmic strings, magnetic monopoles, black holes, and cosmological magnetic fields, and has authored the monograph "Kinks and Domain Walls: an introduction to classical and quantum solitons". He was a Rosenbaum Fellow at the Isaac Newton Institute in Cambridge, a Member of the Institute for Advanced Study, Princeton, and is a Fellow of the American Physical Society.
In 2015, a group of scientists, led by Vachaspati, with collaborators at the University of Washington and Nagoya University, announce their result in Monthly Notices of the Royal Astronomical Society.
FGST, launched in 2008, observes gamma rays (electromagnetic radiation with a shorter wavelength than X-rays) from very distant sources, such as the supermassive black holes found in many large galaxies. The gamma rays are sensitive to effect of the magnetic field they travel through on their long journey to the Earth. If the field is helical, it will imprint a spiral pattern on the distribution of gamma rays.
Vachaspati and his team see exactly this effect in the FGST data, allowing them to not only detect the magnetic field but also to measure its properties. The data shows not only a helical field, but also that there is an excess of left-handedness - a fundamental discovery that for the first time suggests the precise mechanism that led to the absence of antimatter.
For example, mechanisms that occur nanoseconds after the Big Bang, when the Higgs field gave masses to all known particles, predict left-handed fields, while mechanisms based on interactions that occur even earlier predict right-handed fields.
This discovery has wide ramifications, as a cosmological magnetic field could play an important role in the formation of the first stars and could seed the stronger field seen in galaxies and clusters of galaxies in the present day.
The image at the top of the page shows colliding matter and antimatter. Credit: NASA/CXC/M. Weiss
The Daily Galaxy via RAS
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Sentinel-2A captured this image of Mount St Helens in the US state of Washington on 8 February.
The active volcano is known for its 18 May 1980 eruption. The event claimed some 57 lives and damaged homes and infrastructure. The eruption was caused by an earthquake that lead to a massive landslide of the volcano's north face, exposing it to lower pressures. The volcano then exploded, depositing widespread ash and melting the mountain's snow, ice and glaciers that formed a number of volcanic mudslides or lahars.
Some of these lahars are still visible, particularly in the upper left in pink.
In this false-colour image, snow cover appears light blue while pink represents areas with little to no vegetation. In the lower-central part of the image, we can see how snow cover ends in the rectangular areas as the elevation drops closer to the river.
The rectangular areas show land division, possibly for timber extraction, with the blue and red areas revealing where the trees have been cleared.
Sentinel-2 can be used to manage natural resources, to check rates of deforestation, reforestation and areas affected by wildfire. Information from Sentinel-2 can help governing bodies and commercial enterprises make informed decisions about how best to manage, protect and sustain our important forest resources.
This image is also featured on the Earth from Space video programme .
Credit: Contains modified Copernicus Sentinel data (2016), processed by ESA
Pic Gameplay streaming site Twitch.tv says it will be launching a dedicated channel for live videos of people eating.…
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Read more: Brazil, Endangered Species, Wildlife Conservation, Birds, Parrot, Critically Endangered Species, Spix's Macaw, Good News News
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The July 4 weekend marks our nation's birthday and the time when Americans celebrate -- not only with fireworks, but with picnics, backyard BBQs, pool parties. Sadly, one byproduct of these celebrations are the many tons of food that we will inevitably waste after these family gatherings. Today, 40 percent of food produced in the United States is thrown away each year (over two-thirds of that by consumers).
Ketchup with a date label that says it has expired." Salad dressings that are past their "use by" dates, chips and cheese with passed expiration dates. As a result of confusing date labeling policies, consumers regularly toss out foods that are perfectly safe, wholesome, and still taste good.
Our three organizations are actively involved in the national campaign to reduce food waste in America. High on our list of priorities is standardizing date labels on food; indeed it might be the most cost effective intervention to achieving the U.S. government's stated goal of reducing food waste by 50 percent by 2030. Solutions are on the horizon.
Rep. Chellie Pingree (D-ME) and Senator Richard Blumenthal (D-CT) have introduced the Food Date Labeling Act, (HR 5298) to address the confusion surrounding date labeling and tackle our nation's mounting food waste problem.
Our three organizations -- the Harvard Food Law and Policy Clinic, the National Consumers League, and the Johns Hopkins Center for a Livable Future -- performed a survey in April 2016 to learn more about what American consumers actually know about date labels. The findings? Consumers are confused and misled. Thirty-seven percent said they always throw away food close to or past the date on the package, and 84 percent reported at least occasionally doing so.
What many consumers don't know is that most food is still safe to eat after its expiration date. Date labels are placed on foods by manufacturers and retailers. Wording like "best by" or "freshest by," are simply estimates of when a food item will be at its peak quality, and not an indicator of how safe the food is. Consumers, however, fear that eating food past the date on the label puts them at risk of foodborne illness. In fact, only a few foods -- deli meat and unpasteurized cheeses, for example -- actually pose an increased safety risk if eaten after the expiration date. No one wants to throw out good food or waste the money spent on it. But, relying on today's date labels leads consumers to do just that.
A misunderstanding of who regulates date labels is contributing to the problem. One third of respondents in our survey thought that date labels are federally regulated, and 26 percent said they were unsure who put those labels on. In actuality, except for infant formula, there are no federally mandated date labeling rules. Each state has its own regulations for what the labels mean and what stores can do with food after the date passes. Research from the Harvard Food Law and Policy Clinic and Natural Resources Defense Council (NRDC) shows that 20 states currently restrict sales, and in certain cases, even donations of past-date foods, even if the label is an arbitrary quality estimate.
The Food Date Labeling Act aims to clear up this confusion by requiring manufacturers and retailers to stick with just two date labels: an optional "best if used by" to indicate the estimated date a product will no longer be at its peak quality (such as top flavor or texture); and a required "expires on" label for the few high-risk foods that the Food and Drug Administration (FDA) and U.S. Department of Agriculture (USDA) find are actually less safe to eat after a certain date. Retailers would also be able to donate or sell foods after the "best if used by" date passes, which would encourage the distribution of otherwise discarded, but perfectly safe and still tasty food. The bill would have an educational mandate for the FDA and USDA aimed at raising awareness among consumers about what the new labels mean.
Research from the Center for a Livable Future suggests that many consumers are aware of the problem of wasted food and want to be part of the solution -- unfortunately, our nation's current date labeling system is getting in their way. Clearer date labels and more education about what they mean will inevitably help Americans save money, eat safely, and conserve natural resources. That's something worth celebrating.
Emily Broad Leib is the Director of the Harvard Food Law and Policy Clinic, the nation's first food law school clinic, and is an Assistant Clinical Professor of Law at Harvard Law School.
Sally Greenberg is Executive Director of the National Consumers League, the nation's pioneering consumer and worker advocacy organization, founded in 1899.
Roni Neff, PhD, directs the Food System Sustainability and Public Health Program at the Johns Hopkins Center for a Livable Future and is an Assistant Professor of Environmental Health Sciences at the Johns Hopkins Bloomberg School of Public Health.
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Check out this incredible overview from the top of the Eiffel Tower in Paris, France. This shot captures the Euro 2016 Fan Zone at Champ de Mars and was taken by our friend @kaylabernardino. The quarterfinals of the tournament are currently underway with a match today between Wales and Belgium. If you are ever in Paris, the Eiffel Tower offers the highest vantage point in the city, rising 1,063 feet (324 meters). (at Eiffel Tower)
Read more: Critical Thinking, Education, Learning, Teaching, Teachers, Environment, Environmental Education, Climate Change, Land, Natural Resources, Education News
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Gravitational waves released from black hole “super kicks” may soon be detectable, according to new research published in Physical Review Letters.…
Robert Stawell Ball Scientist of the Day
Robert Stawell Ball, an Irish astronomer and popular writer, was born July 1, 1840.
Inspired by the presidential campaign, the stock-footage company Dissolve created a satirical version of the traditionally cheesy campaign advertisement. It's predictable, and also hilarious. If you'd like to watch more videos by Dissolve, you may enjoy this satire of generic branding and this whimsical mockumentary about emoji.
Troubled wildchild turned Brexit commenter Lindsay Lohan has accepted the challenge of turning on Kettering for Christmas, in order to “redeem her political reputation”.…
Not so long ago you could barely move on Facebook for all the exquisitely crafted beheading videos. Now you can't even watch a cute cat video if your first name is Isis, anyway.…
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The debate over the merits of renewable energy is over. For the overwhelming majority of Americans, the advantages of replacing coal, oil, and gas with clean, renewable energy sources come under the heading of glaringly obvious.
Our challenge then, is not to convince people that renewable energy makes sense, but to help them see for themselves that the wave of the future is already breaking all around them. And although that seems like it should be easy, people have spent their entire lives in a fossil-fuel economy that has an illusion of permanence that can be hard to shake off. But The Grid is not The Matrix. People don't need a mysterious red pill to have their eyes opened to a world that's powered by renewable energy. It can be as simple as looking out the window.
Fact: Once someone sees solar panels appear on their neighbor's roof, they are far more likely to go solar themselves. This viral solar effect has been documented by researchers. One house gets solar and then it spreads outward from there. Despite the fact that most people agree that renewable energy is a good idea, seeing it happen in their own neighborhood somehow makes it more real.
This viral effect is helping to drive dramatic double-digit growth for rooftop solar installations year after year after year. Last year the U.S. set a record for rooftop solar installations, and this year is expected to have about twice as many. It took 40 years for solar to be installed on 1 million rooftops in the United States. We should hit the next million within two years.
And there are ways to make this growth happen even faster. One is through public awareness campaigns like the Sierra Club's Ready for 100, which just launched a national tour of nine cities across the U.S. to showcase the demand for clean, renewable energy. Last week, I attended the first one, in Aspen, Colorado (a town that has already achieved 100 percent renewable electricity), and it was fantastic.
But here's an idea: What if we could supercharge that rooftop solar viral effect by making it easy to see the solar potential of every home? To that end, the Sierra Club is collaborating with Google to help map the solar possibilities of residential rooftops across the U.S. Google's solar mapping tool is called Project Sunroof, and it's both powerful and incredibly easy to use. Enter your address into the mapping tool and -- bam! -- you'll see your home's solar potential based on your roof's position, shading, and usable hours of sunlight each year. At the same time, you'll get an estimate of your potential energy bill savings, details about different financing options, and next steps to explore making solar work for you.
Project Sunroof is currently available in 43 states (not yet included are Texas, Hawaii, Rhode Island, Idaho, South Dakota, Mississippi, Tennessee, Alaska, and the District of Columbia). If you haven't already gone solar and are curious about how much you could save, you should check it out. Fighting climate change isn't just an obligation; it's an opportunity to create the future we want.
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Last week, Pacific Gas and Electric Co. announced that it wants to retire California's Diablo Canyon nuclear power plant by 2025. If the California Public Utilities Commission accepts the utility's proposal, it will mean the end of the nuclear era in California. Beyond that milestone, though, it marks what is now an undeniable trend. Clean, renewable energy like wind and solar -- combined with energy efficiency and storage -- can compete with any dirty fuel, be it coal, gas, or nuclear power.
The Sierra Club has unequivocally opposed nuclear energy for more than three decades, and Diablo Canyon is a good illustration of why we do. From the beginning it was a reckless enterprise. Nuclear power plants are not just accidents waiting to happen -- they are mega-disasters waiting to happen. Diablo Canyon was especially risky owing to the discovery of nearby earthquake faults, but no nuclear plant can be guaranteed to be safe. The potential consequences of a nuclear disaster are so horrific by themselves that they overwhelm any risk analysis.
In spite of all that, PG&E would likely have attempted to keep Diablo Canyon open if it could have done so profitably. What's driving the closure of this and other nuclear plants is not the obvious risks they pose, but their inability to compete economically. In Nebraska, the Omaha Public Power District decided to decommission its Fort Calhoun nuclear plant this year not because it had to be shut down owing to flooding of the Missouri River in 2011 but because clean, renewable energy and energy efficiency have helped drive the cost of electricity to levels that the plant couldn't match.
In fact, renewable energy has gotten so cheap so quickly that PG&E says it intends to replace all of the power from Diablo Canyon with carbon-free clean energy. That's a big deal, because Diablo currently generates around 18,000 gigawatt hours per year or 8.5 percent of the state's power mix. It's important to hold PG&E to that commitment. Diablo needs to be replaced with additional clean energy -- above and beyond what it would otherwise have developed -- by the time the plant shuts down less than 10 years from now. How PG&E actually does that (solar, wind, energy efficiency, and storage could all play a role) is less important -- as long as greenhouse gas emissions do not increase as a result of Diablo Canyon's retirement.
The good news is that last year, clean and renewable sources accounted for almost two-thirds of new electrical generation in the U.S. Even so, replacing Diablo Canyon with 100 percent clean, renewable energy is an ambitious goal for both PG&E and the state of California. But the fact that PG&E believes it's possible to do that in less than a decade speaks volumes about how far renewables have come and how quickly it is expected to dominate the energy industry.
It also sets a new, higher bar nationally. If indeed it is possible to do this for the largest power plant in California, then there's no excuse not to attempt to do the same thing on a rapid and responsible timeline for every polluting plant in the United States. From now on, the burden of proof is on polluters to show that clean, renewable energy can't do the job. In our work on retiring coal plants, we've seen utilities repeatedly fail at making that case, and it's only going to get harder to do so going forward.
The Diablo Canyon announcement is more than just another setback for polluting power plants. It reaffirms in a big way that renewable energy will be first and foremost in our future.
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Inside of The Lab at Panorama, the music festival and accompanying art show debuting in New York City next month, there'll be light projections, a trippy tunnel of mirrors, and other interactive artworks. There will also be people playing pinball.
That'll be the doing of Red Paper Heart, a small studio in Brooklyn that's transforming a 1970s pinball machine into a tool for creating digital art. "Things like pinball get people over the seriousness of artwork," says Zander Brimijoin, the company's creative director. "People love pinball, so they instantly have an emotional attachment to it, and we can use that to create this amazing experience."
"They're gonna be sort of like a concert...
Science research funding from the European Union to the UK is set to continue until Britain officially terminates its membership of the bloc by triggering Article 50 of the Lisbon Treaty.…
A West Point cadet's freshly shaved head, Ramadan prayers, Chinese children floating home from school, a Mongolian voter's stare, Olympic trials across the world, a fire ravaged home in California, an especially awkward political handshake, and much more.
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Mathematician Benoit Mandelbrot introduced a set of equations in 1975 that impressed artists more than scientists. That's because his equations -- called fractals -- become amazing geometrical pictures. The Mandelbrot set is a fractal. Pictured here is the "Blue Swirl" fractal, part of the Mandelbrot set. As the image is enlarged -- the picture going deeper and deeper into the region near the boundary of the Mandelbrot set itself (black bits) -- we see infinitely many fabulous patterns including miniature copies of the whole set, spidery filaments, pools and lagoons of color, devilish pitchforks and complicated spirals.
Image credit: Courtesy Frances Griffin
The European Space Agency (ESA) has set the date for the Rosetta probe's deathday and says that on September 30 the spacecraft will crash into the comet it has been orbiting for nearly two years.…
Scientists have revealed new data about two giant blobs at the edge of the Earth's core, larger than continents and possibly older than any rock on the planet.…
Toffler's warnings about 'information overload' and the accelerating pace of change in modern society made his seminal 1970 book a best-seller in the U.S. and around the world.
The technology giant now has a patent for a system that could prevent you from taking photos or recording videos in specific places, like concert venues or movie theaters.
A new Pokémon mobile app will bring the virtual monsters into the real world. But the challenge for developers is to see if people are ready for AR in their daily lives.
They have provided physical evidence to a famous story of heroism during the Holocaust — known before only through the testimony of the 11 Jews who escaped a Lithuanian massacre site.
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MIT researchers have developed low-cost chemical sensors, made from chemically altered carbon nanotubes, that enable smartphones or other wireless devices to detect trace amounts of toxic gases. Using the sensors, the researchers hope to design lightweight, inexpensive radio-frequency identification badges to be used for personal safety and security. Such badges could be worn by soldiers on the battlefield to rapidly detect the presence of chemical weapons -- such as nerve gas or choking agents -- and by people who work around hazardous chemicals prone to leakage.
Image credit: Christine Daniloff/MIT
A Tennessee man is suing Utah because, like the rest of America, it won't let him marry his computer.…
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"Well, I suggest we work on the money (for all of us) first and quickly! I've proposed to Val [Giddings, former vice president of BIO, the biotech industry trade association] that he and I meet while I'm in DC next week so we can (not via e-mail) get a clear picture of options for taking the Academic Review project and other opportunities forward. The "Center for Consumer Freedom" (ActivistCash.com) has cashed in on this to the extreme."
"I believe Val and I can identify and serve as the appropriate (non-academic) commercial vehicles by which we can connect these entities with the project in a manner which helps to ensure the credibility and independence (and thus value) of the primary contributors/owners... I believe our kitchen cabinet here can serve as gatekeepers (in some cases toll takers) for effective, credible responses, inoculation and proactive activities using this project platform..."
"You and I need to talk more about the "academics review" site and concept. I believe that there is a path to a process that would better respond to scientific concerns and allegations. I shared with Val yesterday. From my perspective the problem is one of expert engagement and that could be solved by paying experts to provide responses. You and I have discussed this in the past. Val explained that step one is establishing 501(c)3 not-for-profit status to facilitate fund raising. That makes sense but there is more. I discussed with Jerry Steiner today (Monsanto Executive Team) and can help motivate CLI/BIO/CBI and other organizations to support. The key will be keeping Monsanto in the background so as not to harm the credibility of the information."
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Derbid planthopper (Anotia uhleri) collected in Puslinch, Ontario, Canada, and photographed at the Centre for Biodiversity Genomics (sample ID: BIOUG00856-B08; specimen record: http://www.boldsystems.org/index.php/Public_RecordView?processid=TTHFW359-11; BIN: http://www.boldsystems.org/index.php/Public_BarcodeCluster?clusteruri=BOLD:ACB2705)
Astronomers are using the NASA/ESA Hubble Space Telescope to study auroras -- stunning light shows in a planet's atmosphere -- on the poles of the largest planet in the Solar System, Jupiter. This observation program is supported by measurements made by NASA's Juno spacecraft, currently on its way to Jupiter. Jupiter's auroras were first discovered by the Voyager 1 spacecraft in 1979. A thin ring of light on Jupiter's nightside looked like a stretched-out version of our own auroras on Earth. Only later on was it discovered that the auroras were best visible using the ultraviolet capabilities of the NASA/ESA Hubble Space Telescope.
This observation program is perfectly timed as NASA's Juno spacecraft is currently in the solar wind near Jupiter and will enter the orbit of the planet in early July 2016. While Hubble is observing and measuring the auroras on Jupiter, Juno is measuring the properties of the solar wind itself; a perfect collaboration between a telescope and a space probe.
"These auroras are very dramatic and among the most active I have ever seen", says Jonathan Nichols from the University of Leicester, UK, and principal investigator of the study. "It almost seems as if Jupiter is throwing a firework party for the imminent arrival of Juno."
To highlight changes in the auroras Hubble is observing Jupiter daily for around one month. Using this series of images it is possible for scientists to create videos that demonstrate the movement of the vivid auroras, which cover areas bigger than the Earth.
Not only are the auroras huge, they are also hundreds of times more energetic than auroras on Earth. And, unlike those on Earth, they never cease. Whilst on Earth the most intense auroras are caused by solar storms -- when charged particles rain down on the upper atmosphere, excite gases, and cause them to glow red, green and purple -- Jupiter has an additional source for its auroras.
The strong magnetic field of the gas giant grabs charged particles from its surroundings. This includes not only the charged particles within the solar wind but also the particles thrown into space by its orbiting moon Io, known for its numerous and large volcanos.
The new observations and measurements made with Hubble and Juno will help to better understand how the Sun and other sources influence auroras. While the observations with Hubble are still ongoing and the analysis of the data will take several more months, the first images and videos are already available and show the auroras on Jupiter's north pole in their full beauty.
The Daily Galaxy via ESA/Hubble
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Astronomers are using the NASA/ESA Hubble Space Telescope to study auroras — stunning light shows in a planet's atmosphere — on the poles of the largest planet in the solar system, Jupiter. This observation program is supported by measurements made by NASA's Juno spacecraft, currently on its way to Jupiter.
Jupiter, the largest planet in the solar system, is best known for its colorful storms, the most famous being the Great Red Spot. Now astronomers have focused on another beautiful feature of the planet, using Hubble's ultraviolet capabilities.
The extraordinary vivid glows shown in the new observations are known as auroras. They are created when high-energy particles enter a planet's atmosphere near its magnetic poles and collide with atoms of gas. As well as producing beautiful images, this program aims to determine how various components of Jupiter's auroras respond to different conditions in the solar wind, a stream of charged particles ejected from the sun.
This observation program is perfectly timed as NASA's Juno spacecraft is currently in the solar wind near Jupiter and will enter the orbit of the planet in early July 2016. While Hubble is observing and measuring the auroras on Jupiter, Juno is measuring the properties of the solar wind itself; a perfect collaboration between a telescope and a space probe.
“These auroras are very dramatic and among the most active I have ever seen”, said Jonathan Nichols from the University of Leicester, U.K., and principal investigator of the study. “It almost seems as if Jupiter is throwing a firework party for the imminent arrival of Juno.” Read more: go.nasa.gov/294QswK
Credits: NASA, ESA, and J. Nichols (University of Leicester)
The central regions of many glittering galaxies, our own Milky Way included, harbor cores of impenetrable darkness -- black holes with masses equivalent to millions, or even billions, of suns. What's more, these supermassive black holes and their host galaxies appear to develop together, or "co-evolve." Theory predicts that as galaxies collide and merge, growing ever more massive.
Researchers have developed a new method for detecting and measuring one of the most powerful, and most mysterious, events in the Universe - a black hole being kicked out of its host galaxy and into intergalactic space at speeds as high as 5000 kilometers per second.
"When the detection of gravitational waves was announced, a new era in astronomy began, since we can now actually observe two merging black holes," said study co-author Christopher Moore, a Cambridge University PhD student who was also a member of the team which announced the detection of gravitational waves earlier this year. "We now have two ways of detecting black holes, instead of just one - it's amazing that just a few months ago, we couldn't say that. And with the future launch of new space-based gravitational wave detectors, we'll be able to look at gravitational waves on a galactic, rather than a stellar, scale."
The method, developed by researchers from the University of Cambridge, could be used to detect and measure so-called black hole superkicks, which occur when two spinning supermassive black holes collide into each other, and the recoil of the collision is so strong that the remnant of the black hole merger is bounced out of its host galaxy entirely. Their results are reported in the journal Physical Review Letters.
Earlier this year, the LIGO Collaboration announced the first detection of gravitational waves - ripples in the fabric of spacetime - coming from the collision of two black holes, confirming a major prediction of Einstein's general theory of relativity and marking the beginning of a new era in astronomy. As the sensitivity of the LIGO detectors is improved, even more gravitational waves are expected to be detected - the second successful detection was announced in June.
As two black holes circle each other, they emit gravitational waves in a highly asymmetric way, which leads to a net emission of momentum in some preferential direction. When the black holes finally do collide, conservation of momentum imparts a recoil, or kick, much like when a gun is fired. When the two black holes are not spinning, the speed of the recoil is around 170 kilometres per second. But when the black holes are rapidly spinning in certain orientations, the speed of the recoil can be as high as 5000 kilometres per second, easily exceeding the escape velocity of even the most massive galaxies, sending the black hole remnant resulting from the merger into intergalactic space.
The Cambridge researchers have developed a new method for detecting these kicks based on the gravitational wave signal alone, by using the Doppler Effect. The Doppler Effect is the reason that the sound of a passing car seems to lower in pitch as it gets further away. It is also widely used in astronomy: electromagnetic radiation coming from objects which are moving away from the Earth is shifted towards the red end of the spectrum, while radiation coming from objects moving closer to the Earth is shifted towards the blue end of the spectrum. Similarly, when a black hole kick has sufficient momentum, the gravitational waves it emits will be red-shifted if it is directed away from the Earth, while they will be blue-shifted if it's directed towards the Earth.
"If we can detect a Doppler shift in a gravitational wave from the merger of two black holes, what we're detecting is a black hole kick," said study co-author Davide Gerosa, a PhD student from Cambridge's Department of Applied Mathematics and Theoretical Physics. "And detecting a black hole kick would mean a direct observation that gravitational waves are carrying not just energy, but linear momentum as well."
Detecting this elusive effect requires gravitational-wave experiments capable of observing black hole mergers with very high precision. A black hole kick cannot be directly detected using current land-based gravitational wave detectors, such as those at LIGO. However, according to the researchers, the new space-based gravitational wave detector known as eLISA, funded by the European Space Agency (ESA) and due for launch in 2034, will be powerful enough to detect several of these runaway black holes. In 2015, ESA launched the LISA Pathfinder, which is successfully testing several technologies which could be used to measure gravitational waves from space.
The researchers found that the eLISA detector above will be particularly well-suited to detecting black hole kicks: it will be capable of measuring kicks as small as 500 kilometres per second, as well as the much faster superkicks. Kick measurements will tell us more about the properties of black hole spins, and also provide a direct way of measuring the momentum carried by gravitational waves, which may lead to new opportunities for testing general relativity.
The Daily Galaxy via University of Cambridge and NASA/JPL
Image credit top of page: ligo.caltech.edu
“Red dwarfs the dim bulbs of the cosmos have received scant attention by SETI scientists in the past,” SETI Institute engineer Jon Richard said last week in a news release announcing the initiative. “That's because researchers made the seemingly reasonable assumption that other intelligent species would be on planets orbiting stars similar to the sun.”
“This may be one instance in which older is better,” said astronomer Seth Shostak of California-based SETI, a private, non-profit organization which stands for Search for Extraterrestrial Intelligence. “Older solar systems have had more time to produce intelligent species.” A super-Earth known as Kapteyn b that orbits an 11.5 billion-year-old red dwarf, for example, makes the star and the planet 2.5 times older than Earth (image below).The srtistic representation shows the potentially habitable world Kapteyn b with the globular cluster Omega Centauri in the background. It is believed that the Omega Centauri is the remaining core of a dwarf galaxy that merged with our own galaxy billions of years ago bringing Kapteyn's star along. (PHL @ UPR Arecibo, Aladin Sky Atlas).
The SETI Institute belives that planetary systems orbiting red dwarfs — dim, long-lived stars that are on average billions of years older than our sun — are worth investigating for signs of advanced extraterrestrial life. The star that's closest to our sun, Proxima Centauri, is a red dwarf. A variety of observing efforts, including Cornell's Pale Red Dot initiative, are looking for habitable planets around Proxima Centauri (shown above).
The two-year project involves picking from a list of about 70,000 red dwarfs and scanning 20,000 of the nearest ones, along with the cosmic bodies that circle them using the SETI Institute's Allen Telescope Array in the High Sierras of northern California, a group of 42 antennas that can observe three stars simultaneously.
“We'll scrutinize targeted systems over several frequency bands between 1 and 10 GHz,” said SETI scientist Gerry Harp. “Roughly half of those bands will be at so-called ‘magic frequencies' — places on the radio dial that are directly related to basic mathematical constants. It's reasonable to speculate that extraterrestrials trying to attract attention might generate signals at such special frequencies.”
For a long time, scientists ruled out searching around red dwarfs because habitable zones around the stars are small, and planets orbiting them would be so close that one side would be constantly facing the star, making one side of the planet very hot and the other quite cold and dark.
But more recently, scientists have learned that heat could be transported from the light side of the planet to the darker side, and that much of the surface could be amenable to life.
“In addition, exoplanet data have suggested that somewhere between one sixth and one half of red dwarf stars have planets in their habitable zones, a percentage comparable to, and possibly greater than, for Sun-like stars,” said the statement.
The brightest of Red Dwarfs are a tenth as luminous as the sun, and some are just 0.01 percent as bright, but account for three-quarters of all stars, with 6 percent or more of all red dwarfs having potentially habitable, Earth-sized planets.
The Daily Galaxy via SETI Institute, and AFP
Image credits: NASA/Chandra X-Ray Space Observatory
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Food is an important element of Basque life. In the Ostatua Kitchen tent at the Smithsonian's 2016 Folklife Festival, chefs from two Basque culinary schools (Escuela Superior de Hostelería de Artxanda and Escuela Superior de Hostelería de Gamarra) will showcase regional cooking and drinks with cooking demonstrations and workshops. In the baserria (the farmstead), cheesemakers will share the art of producing the Basque's unique cheese, and visitors will learn how people from a villager in Alava process salt from natural springs, using traditional methods to produce environmentally sustainable gourmet salt.
The post Basque Country & Cheese appeared first on Smithsonian Insider.
Traditional Basque dancers at the 2016 Smithsonian Folklife Festival on the National Mall in Washington, D.C. (Flickr photo by Victoria Pickering)
On a bright, hot summer morning on the National Mall in Washington, D.C. the air was filled with more than just humidity. From inside the Smithsonian's Arts & Industries Building floated melodic strains of music from the diverse cultures of California and the Basque country, which is in the Pyrenees on the border between France and Spain.
Martha Gonzalez is doing double-duty during the Folklife Festival, playing with the band Quetzal and with the FandangObon group. Today she danced on the tarima platform with her son jarocho group. You can find them each day at the Sounds of California Stage & Plaza. (Photo by Walter Larrimore, Ralph Rinzler Folklife Archives)
Musicians were performing to kick off the 2016 Smithsonian Folklife Festival, with themes this year covering “Basque: Innovation by Culture” and “Sounds of California.”
Speakers at the opening ceremony alluded to ideas of inclusion, acceptance, and understanding. They often reminded the audience that we are all human, and much is shared among us despite superficial differences.
Salar Nader is a master of the tablas. He, along with rubâb player Homayoun Sakhi, performed in the opening ceremony and again in the afternoon at the Sounds of California Stage & Plaza. (Photo by Ronald Villasante, Ralph Rinzler Folklife Archives)
Michael Mason, Director of Smithsonian's Center for Folklife and Cultural Heritage, opened the ceremony by paraphrasing a quote from American poet and activist Muriel Rukeyser. “The world is not made of atoms, but of stories,” Mason said. He encouraged the crowd to listen to the stories being told at the festival, and to be brave enough to share their own.
Demonstration of a rural Basque sportthe object is to cut 6 slices of no more than 3 centimeters thick, as fast as possible. At the 2016 Smithsonian Folklife Festival on the National Mall. (Flickr photo by Victoria Pickering)
Smithsonian Secretary David Skorton began his remarks, “When we open up the newspapers every day, don't we need to see more things like the Folklife Festival?” The audience responded with cheers and applause. “Every day of this festival is magic, and we need this magic right now,” he said.
Richard Kurin, Smithsonian acting provost and undersecretary for museums and research, also stressed the ideas of knowledge, respect, and diversity. He decried ignorance and echoed President Barack Obama's remarks on immigration reform when he said, “We've all come from somewhere.”
U.S. Representative John Garamendi (D-Calif.) talked about his grandparents immigrating to the U.S. from the Basque country. “That's the story of America,” he said.
Irati Anda and Xabier Paya are bertsolariak, Basque poets who improvise songs on given topics. In today's “Berto Workshop,” they sang about arriving in Washington, their favorite sports, and Xabi's amuma (grandmother). (Photo by Maureen Spagnolo, Ralph Rinzler Folklife Archives)
The Folklife Festival, located on the National Mall between 4th and 7th Streets, is filled with concerts, music performances, craftsmen, language workshops, and cuisine. The Arts & Industries Building is host to the Folklife Festival Marketplace, where visitors can buy artisan products, books and clothing, and get a break from the heat.
FandangObon got the audience circling around the Sounds of California Stage & Plaza with a mix of Japanese and Mexican dance traditions. Want to join in? You have no choice! Just dance! (Photo by Francisco Guerra, Ralph Rinzler Folklife Archives)
The 2016 Smithsonian Folklife Festival runs this year from June 29-July 4 and July 7-10. Admission is free. Festival hours are from 11 a.m. to 5 p.m. each day, with special evening events beginning at 6:30 p.m. For more information: http://www.festival.si.edu.
he day evening with an evening concert by Basque accordion virtuoso Kepa Junkera. Dancers from Aukeran and visitors joined in kalejira, the Basque festival tradition of “going around singing and dancing.” Photo by Josh Weilepp, Ralph Rinzler Folklife Archives
The post Basque culture, California music thrill at 2016 Folklife Festival appeared first on Smithsonian Insider.
enclosed in thick white frames, the images have a tactile quality that seems to hold hundreds of overlapping layers within its borders.
The post megan geckler explores materiality & chaos in illusive scanner prints appeared first on designboom | architecture & design magazine.
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Getting food from the farmer to the shop costs just 4 percent of all its lifetime emissions. Ten times as much carbon is emitted in refrigerating British food as in air-freighting it from abroad, and fifty times as much is emitted by the customer traveling to the shops. A New Zealand lamb, shipped to England, requires one-quarter as much carbon to get on a London plate as a Welsh lamb; a Dutch rose grown in a heated greenhouse and sold in London, has six times the carbon footprint of a Kenyan rose grown under the sun using water recycled through a fish farm, using geothermal electricity and providing employment to Kenyan women.
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Many people around the world rely on fish not just for protein but for critical micronutrients like iron and zinc. So declining fisheries pose major risks for global health, scientists warn.
Trujillo is the second largest city in Peru with slightly less than 800,000 residents in its urban area. España Avenue - the circular road that is visible at the center of this Overview - contains the city's monument area and also traces the historic outline of the defensive wall that was constructed around the city in 1786. /// Source imagery: @dailyoverview (at Trujillo, Peru)
Scott Sumner is a monetary economist who studies the Great Depression and runs the blog The Money Illusion. He also used his knowledge 20th century economics to help fix the 2007-2009 recession. “Most of the discussion was missing the point,” Sumner says in this film by Ian Reid. “Other economists were looking at interest rates. They assumed money was easy. But commodity prices, stock prices, real estate prices, every other asset market was signaling money was too tight.”
This film was produced by Distant Moon and the Mercatus Center at George Mason University.
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George Ellery Hale Scientist of the Day
George Ellery Hale, an American astrophysicist, was born June 29, 1868.
Edward Lhuyd Scientist of the Day
Edward Lhuyd, a Welsh naturalist, died June 30, 1709, at about age 49 (we don't know his date of birth).
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The Hubble Space Telescope has captured new images of Jupiter's glowing aurora swirling around one of the planet's poles, as part of a wider observation programme of the gas giant.…
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Physicists have created a novel simulation which allows users to watch how the colour of a galaxy changes over time as it evolves.…
When McLaren inaugurated its present range of roadgoing supercars with the MP4-12C in 2010, it presented that car as the ultimate expression of form following function. Designed entirely for performance, the 12C was shaped by the wind tunnel and McLaren was proud of that fact. I'm here to state the obvious by denouncing that extremist approach to design as wrongheaded, and the car reminding me of that fact is the 1939 BMW 328 Mille Miglia Touring Coupé that I saw at Goodwood last week.
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Barbara Wolfe and Jason Fletcher at the University of Wisconsin-Madison found children from lower income families have lower non-cognitive skills than children from richer families.
British people are now bored of Brexit and have returned to using the Internet for what it was made for pornography.…
A well-known radio source has turned out not to be the galaxy it's been classified as for 20 years, but a surprisingly quiet black hole.…
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Pictured is the vorticity at the surface of the ocean with red indicating clockwise rotation and blue indicating counter-clockwise rotation. Many small coherent eddies are visible. These eddies can rotate in either direction and can endure for a year or more. The sharp boundary between the broad red and blue regions is a fast-moving, meandering jet, analogous to the North Atlantic Gulf Stream. This was done by a numerical simulation of an idealized, wind-driven ocean basin calculated on massively parallel computers at the San Diego Supercomputer Center.
Image credit: Jeffrey B. Weiss, University of Colorado Boulder
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According to new research, ocean acidification makes it harder for sea snails to escape from their sea star predators. The findings suggest that by disturbing predator-prey interactions, ocean acidification could spur cascading consequences for food web systems in shoreline ecosystems.
Image credit: Brittany Jellison/UC Davis
It will now prioritize posts from friends and family — potentially bad news for media companies relying on Facebook for traffic. The company has been under pressure to defend its political neutrality.
What if cars weren't mass produced? Local Motors, a small-batch auto manufacturer, relies on an online design community and a "co-creation" business model to bring new vehicles to market, really fast.
Some doctors are finding that virtual travel — to Venice, a Hawaiian beach or Africa — can open new worlds to people confined by low mobility, dementia or depression.
Joshua Browder was fed up with parking tickets so he made a robot to help people challenge fines. The robot chats with people in London and New York, asks them what happened and writes an appeal.
photography by francie posted a photo:
"The monarch butterfly (Danaus plexippus) is a milkweed butterfly (subfamily Danainae) in the family Nymphalidae. It may be the most familiar North American butterfly."
By Matthew Mulrennan
This post by Matt Mulrennan originally appeared in National Geographic's Ocean Views.
Our ocean remains the greatest mystery on planet Earth. The ocean takes up 70% of our blue planet, yet we've only explored 5% of it. The ocean suffers from many urgent grand challenges - we don't know enough about the ocean, too much pollution is going in, and too many fish and other animals are coming out.
Thankfully, ocean-related technology is riding the innovation wave, and we're seeing some really amazing breakthroughs in ocean health and exploration.
This World Oceans Day, we're celebrating eight amazing innovations that are helping to save our ocean.
Please share your favorite ocean innovations with #TeamOcean.
8. Snotbot
The "Snotbot" can hover above a whale to collect mucus from a whale's blow to gain valuable biological information like stress hormones, without stressing the animal.
Unmanned Aerial Vehicles (UAVs) and drones are improving biological research, monitoring coastal waters to scan for illegal activity and enforcing marine protected areas. They can also be used to make epic videos of a stampeding 'megapod' of dolphins.
7. Fishface
Fishface by the Nature Conservancy is an affordable fish identification tool being used for population assessments in Indonesia.
The technology that automatically tags you in a picture on Facebook is being applied to counting and describing fish stocks. Facial recognition and visual computing software are revolutionizing the process of counting fish and fisheries managers are using this information to make fisheries more sustainable.
6. Whale Alert App
The Whale Alert 2.0 App alerts mariners about the potential presence of whales to avoid deadly ship strikes, a leading cause of death for these protected species.
Whale Alert provides recommended routes to avoid whales and allows you to report when whales are in distress, such as being entangled in fishing gear. New innovative apps allow people to track marine debris, check fisheries regulations, visualize pollution and contribute observations to citizen science.
5. SkySails
Cargo ships with high altitude sails, like SkySails, can save 10-30% on daily fuel use.
About 90% of all global trade uses large cargo ships. The fuels burned by the global shipping fleet are a major contributor to climate change and ocean acidification, which are already harming marine life. But green shipping initiatives are saving fuel through improved hull design, breakthrough propellers, and simply slowing down ships.
4. Global Fishing Watch
Global Fishing Watch is a platform to monitor global fishing activity run by SkyTruth, Oceana and Google. It pools together historical data from a satellite-based vessel monitoring system and uses an algorithm to assess where fishing has occurred.
With advancement in tools like this for global fisheries monitoring, the writing is on the wall for taking down lots of illegal 'pirate' fishers. Argh.
3. Saildrone
Saildrone is an autonomous wind-propelled sailing vessel that can conduct scientific missions independently in rough weather for months.
95% of the ocean is still largely unexplored, and unmanned vessels are transforming oceanography by cutting down on expensive research ships that cost upwards of $50,000 per day to operate. Increasing autonomy for ocean exploration is a goal of the $7 million Shell Ocean Discovery XPRIZE, and team registration is still open!
2. Edible Six-Pack Rings
Saltwater Brewery has developed an edible and biodegradable six-pack ring out of wheat and barley from their brewing process. Nom.
There are 5 trillion pieces of plastics in the ocean causing $13 billion per year in damage to marine ecosystems. To solve ocean plastic pollution globally requires disruptive "moonshot" technologies in materials design for more benign packaging products, a circular economic approach that never allows plastics to become waste, as well as basic waste management in more cities and countries to stop the leakage of plastics into the ocean.
1. Live Dives
The Fish Eye Project is broadcasting a live SCUBA dive online today June 8th. You can tune in and submit questions to the diver via #LiveDive.
We are the first humans that can watch things happening live in the ocean from our computers or phones, and interact with the divers and robots. This is great for ocean exploration, and expanding access to the ocean to exponentially more people. The cutting edge in this field is high-definition, 360-degree cameras propelling footage immediately into virtual reality headsets from hard to reach habitats like the deep-sea. These interactive technologies will hopefully usher in a wave, better yet a tsunami, of new ocean explorers and innovators.
Matthew Mulrennan is the lead of the Ocean Initiative at XPRIZE - a commitment to conduct five ocean XPRIZE competitions, and put us on a path to making the ocean healthy, valued and understood.
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Pseudoscorpion (Microbisium sp.) collected in Gros Morne National Park, Newfoundland and Labrador, Canada, and photographed at the Centre for Biodiversity Genomics (sample ID: BIOUG14077-A08; specimen record: http://www.boldsystems.org/index.php/Public_RecordView?processid=SSGBB1807-14; BIN: http://www.boldsystems.org/index.php/Public_BarcodeCluster?clusteruri=BOLD:AAB2507)
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El Niño conditions in 2015 and early 2016 altered rainfall patterns around the world. In the Amazon, El Niño reduced rainfall during the wet season, leaving the region drier at the start of the 2016 dry season than any year since 2002, according to NASA satellite data.
Wildfire risk for the dry season months of July to October this year now exceeds fire risk in 2005 and 2010, drought years when wildfires burned large areas of Amazon rainforest, said Doug Morton, an Earth scientist at NASA's Goddard Space Flight Center who helped create the fire forecast.
"Severe drought conditions at the start of the dry season set the stage for extreme fire risk in 2016 across the southern Amazon," Morton said.
The Amazon fire forecast uses the relationship between climate and active fire detections from NASA satellites to predict fire season severity during the region's dry season. Developed in 2011 by scientists at University of California, Irvine and NASA's Goddard Space Flight Center, the forecast model is focused particularly on the link between sea surface temperatures and fire activity. Warmer sea surface temperatures in the tropical Pacific (El Niño) and Atlantic oceans shift rainfall away from the Amazon region, increasing the risk of fires during dry season months.
Read more: go.nasa.gov/2937ADt
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Sorry NASA, but it turns out that a 1917 image on an astronomical glass plate from the Carnegie Institute Observatories' collection shows the first-ever evidence of a planetary system beyond our own Sun. This unexpected find was recognized in the process of researching an article about planetary systems surrounding white dwarf stars in New Astronomy Reviews.
Here's what happened: about a year ago, the review's author, Jay Farihi of University College London, contacted our Observatories' Director, John Mulchaey. He was looking for a plate in the Carnegie archive that contained a spectrum of van Maanen's star (shown above), a white dwarf discovered by Dutch-American astronomer Adriaan van Maanen in the very year our own plate was made.
The 1917 photographic plate spectrum of van Maanen's star from the Carnegie Observatories' archive is shown below. The pull-out box shows the strong lines of the element calcium, which are surprisingly easy to see in the century old spectrum. The spectrum is the thin, (mostly) dark line in the center of the image. The broad dark lanes above and below are from lamps used to calibrate wavelength, and are contrast-enhanced in the box to highlight the two "missing" absorption bands in the star.
Stellar spectra are recordings of the light emitted by distant stars. Spectra spread out all of the component colors of light, like a rainbow from a prism, and they can teach astronomers about a star's chemical composition. They can also tell them how the light emitted by a star is affected by the chemistry of the things it passes through before reaching us on Earth.
Stellar spectra images allowed 19th century astronomers to develop a system for classifying stars that is still used today. Modern astronomers use digital tools to image stars, but for decades, they would use glass photographic plates both to take images of the sky, and to record stellar spectra.
As requested, the Observatories located the 1917 plate, made by former Observatories Director Walter Adams at Mount Wilson Observatory, which was then part of Carnegie. Other than a notation on the plate's sleeve indicating that the star looked a bit warmer than our own Sun, everything seemed very ordinary.
However, when Farihi examined the spectrum, he found something quite extraordinary.
The clue was in what's called an "absorption line" on the spectrum. Absorption lines indicate "missing pieces," areas where the light coming from a star passed through something and had a particular color of light absorbed by that substance. These lines indicate the chemical makeup of the interfering object.
Carnegie's 1917 spectrum of van Maanen's star revealed the presence of heavier elements, such as calcium, magnesium, and iron, which should have long since disappeared into the star's interior due to their weight.
Only within the last 12 years has it become clear to astronomers that van Maanen's star and other white dwarfs with heavy elements in their spectra represent a type of planetary system featuring vast rings of rocky planetary remnants that deposit debris into the stellar atmosphere. These recently discovered systems are called "polluted white dwarfs." They were a surprise to astronomers, because white dwarfs are stars like our own Sun at the end of their lifetimes, so it was not at all expected that they would have leftover planetary material around them at that stage.
The image at the top of the page shows Camelopardalis, a binary star system with a white dwarf and its companion star, surrounded by shells of ionised gas (NASA/JPL-Caltech)
"The unexpected realization that this 1917 plate from our archive contains the earliest recorded evidence of a polluted white dwarf system is just incredible," Mulchaey said. "And the fact that it was made by such a prominent astronomer in our history as Walter Adams enhances the excitement."
Planets themselves have not yet been detected orbiting van Maanen's star, nor around similar systems, but Farihi is confident it is only a matter of time.
"The mechanism that creates the rings of planetary debris, and the deposition onto the stellar atmosphere, requires the gravitational influence of full-fledged planets," he explained. "The process couldn't occur unless there were planets there."
"Carnegie has one of the world's largest collections of astronomical plates with an archive that includes about 250,000 plates from three different observatories--Mount Wilson, Palomar, and Las Campanas," concluded Mulchaey. "We have a ton of history sitting in our basement and who knows what other finds we might unearth in the future?"
The Daily Galaxy via Carnegie Institute
Image credit: van Maanen's star H. Bond (STSci), R. Ciardullo (PSU), WFPC2, HST, NASA
The Universe is becoming gradually cleaner as more and more cosmic dust is being mopped up by the formation of stars within galaxies, an international team of astronomers has revealed. Peering back 12 billion years using the Herschel space telescope to produce far-infrared images of the sky, the team led by researchers at Cardiff University has been able to observe the very early formation of galaxies and compare them to galaxies that have formed much more recently.
Cosmic dust is comprised of tiny solid particles that are found everywhere in space between the stars. The dust and the gas in the universe is the raw material out of which stars and galaxies form. Though this blanket of material is key to the formation of stars and galaxies, it also acts as a sponge, absorbing almost half of the light emitted by stellar objects and making them impossible to observe with standard optical telescopes.
With the launch of the Herschel space telescope in 2009, researchers were provided with the perfect tool for probing this hidden universe. Owing to a collection of sensitive instruments, mirrors and filters, the Herschel telescope had the capacity to detect the dust through the far-infrared emission it emits, revealing the existence of stars and galaxies hidden by the dust.
Professor Steve Eales, a co-leader of the project from Cardiff University's School of Physics and Astronomy, said: "We were surprised to find that we didn't need to look far in the past to see signs of galaxy evolution. Our results show that the reason for this evolution is that galaxies used to contain more dust and gas in the past, and the universe is gradually becoming cleaner as the dust is used up."
Professor Haley Gomez, also of the School of Physics and Astronomy, presented the team's results today, 29 June, at the National Astronomy Meeting in Nottingham. After seven years of work analysing the images from the Herschel telescope, the team of over 100 astronomers have released a large catalogue of the sources of far-infrared radiation in this 'hidden universe'.
The team's survey of the sky, called the Herschel Astrophysical Terahertz Large Area Survey (Herschel ATLAS), has revealed the details of over half a million galaxies, many of which have been viewed as they were over 12 billion years ago, just shortly after the big bang.
The team are hopeful that this unprecedented catalogue of sources will be vital tools for astronomers wishing to understand the detailed history of galaxies and the wider cosmos.
"Before Herschel we only knew of a few hundred such dusty sources in the distant universe and we could only effectively 'see' them in black and white," said Loretta Dunne, a co-leader of project from Cardiff University's School of Physics and Astronomy, said: Herschel, with its five filters, has given us the equivalent of technicolour, and the colour of the galaxy tell us about their distances and temperatures. So we now have half a million galaxies we can use to map out the hidden star formation in the universe."
The Daily Galaxy via Cardiff University
"Robots really do dream. We can ask RobERt to dream up what he thinks a water spectrum will look like, and he's proved very accurate," says Ingo Waldmann of University College London. "This dreaming ability has been very useful when trying to identify features in incomplete data. RobERt can use his dream state to fill in the gaps."
Machine-learning techniques that mimic human recognition and dreaming processes are being deployed in the search for habitable worlds beyond our solar system. A deep belief neural network, called RobERt (Robotic Exoplanet Recognition), has been developed by astronomers at UCL to sift through detections of light emanating from distant planetary systems and retrieve spectral information about the gases present in the exoplanet atmospheres.
"Different types of molecules absorb and emit light at specific wavelengths, embedding a unique pattern of lines within the electromagnetic spectrum," explained Dr Waldmann, who leads RobERt's development team. "We can take light that has been filtered through an exoplanet's atmosphere or reflected from its cloud-tops, split it like a rainbow and then pick out the 'fingerprint' of features associated with the different molecules or gases. Human brains are really good at finding these patterns in spectra and label them from experience, but it's a really time consuming job and there will be huge amounts of data.
A neural network's dream of Earth, is shown above. Similar to RobERt dreaming of exoplanet spectra, this neural network was trained to dream in the style of a Monet painting.
We built RobERt to independently learn from examples and to build on his own experiences. This way, like a seasoned astronomer or a detective, RobERt has a pretty good feeling for what molecules are inside a spectrum and which are the most promising data for more detailed analysis. But what usually takes days or weeks takes RobERt mere seconds."
Deep belief neural networks, or DBNs, were developed more than a decade ago and are commonly used for speech recognition, Internet searches and tracking customer behaviour. RobERt's DBN has three layers of unit processors, or 'neurons'. Information is fed into a bottom layer of 500 neurons, which make an initial filter of the data and pass a subset up to the second layer. Here, 200 neurons refine the selection and pass data up to a third layer of 50 neurons to make the final identification of the gases most likely to be present.
To prepare RobERt for his challenge, Waldmann and colleagues at UCL created a total of 85,750 simulated spectra, covering five different types of exoplanet ranging from GJ1214b, a potential "ocean planet," to WASP-12, a hot Jupiter orbiting very close to its star. Each spectrum in the training set contained the fingerprint of a single gas species. RobERt's learning progress was tested at intervals during the training with 'control' spectra. At the end of the training phase, RobERt had a recognition accuracy of 99.7%.
"RobERt has learned to take into account factors such as noise, restricted wavelength ranges and mixtures of gases," said Waldmann. "He can pick out components such as water and methane in a mixed atmosphere with a high probability, even when the input comes from the limited wavebands that most space instruments provide and when it contains overlapping features."
RobERt's DBN can also be reversed so that instead of analysing data fed into the system, he can enter a 'dreaming state' in which he can generate full spectra based on his experiences.
The James Webb Space Telescope, due for launch in 2018, will tell as more about the atmospheres of exoplanets, and new facilities like Twinkle or ARIEL will be coming online over the next decade that are specifically tailored to characterising the atmospheres of exoplanets. The amount of data these missions will provide will be breathtaking. RobERt will play an invaluable role in helping us to analyse data from these missions and find out what these distant worlds are really like."
The Daily Galaxy via Royal Astronomical Society (RAS)
Image credit: Waldmann/UCL/Gatys
“Suppose there is a civilization like ours and suppose — unlike us, who are skittish about broadcasting our presence — they think it's important to be a beacon, an interstellar or extragalactic lighthouse of sorts,” says University of California Santa Barbara physicist, Philip Lubin.. “There is a photonics revolution going on on Earth that enables this specific kind of transmission of information via visible or near-infrared light of high intensity."
magine if we sent up a visible signal that could eventually be seen across the entire universe. Imagine if another civilization did the same. Recent photonics advances now allow us to be seen across the universe, with major implications for the search for extraterrestrial intelligence, says Lubin.
Looking up at the night sky — expansive and seemingly endless, stars and constellations blinking and glimmering like jewels just out of reach — it's impossible not to wonder: Are we alone? For many of us, the notion of intelligent life on other planets is as captivating as ideas come. Maybe in some other star system, maybe a billion light years away, there's a civilization like ours asking the exact same question.
The technology now exists to enable exactly that scenario, according to Lubin, whose new work applies his research and advances in directed-energy systems to the search for extraterrestrial intelligence (SETI). His recent paper “The Search for Directed Intelligence” appears in the journal REACH Reviews in Human Space Exploration.
“If even one other civilization existed in our galaxy and had a similar or more advanced level of directed-energy technology, we could detect ‘them' anywhere in our galaxy with a very modest detection approach,” said Lubin, who leads the UCSB Experimental Cosmology Group. “If we scale it up as we're doing with direct energy systems, how far could we detect a civilization equivalent to ours? The answer becomes that the entire universe is now open to us.
“Similar to the use of directed energy for relativistic interstellar probes and planetary defense that we have been developing, take that same technology and ask yourself, ‘What are consequences of that technology in terms of us being detectable by another ‘us' in some other part of the universe?'” Lubin added. “Could we see each other? Can we behave as a lighthouse, or a beacon, and project our presence to some other civilization somewhere else in the universe? The profound consequences are, of course, ‘Where are they?' Perhaps they are shy like us and do not want to be seen, or they don't transmit in a way we can detect, or perhaps ‘they' do not exist.”
The same directed energy technology is at the core of Lubin's recent efforts to develop miniscule, laser-powered interstellar spacecraft. That work, funded since 2015 by NASA (and just selected by the space agency for “Phase II” support) is the technology behind billionaire Yuri Milner's newsmaking, $100-million Breakthrough Starshot initiative announced April 12.
Lubin is a scientific advisor on Starshot, which is using his NASA research as a roadmap as it seeks to send tiny spacecraft to nearby star systems.
In describing directed energy, Lubin likened the process to using the force of water from a garden hose to push a ball forward. Using a laser light, spacecraft can be pushed and steered in much the same way. Applied to SETI, he said, the directed energy system could be deployed to send a targeted signal to other planetary systems.
“In our paper, we propose a search strategy that will observe nearly 100 billion planets, allowing us to test our hypothesis that other similarly or more advanced civilizations with this same broadcast capability exist,” Lubin said.
“As a species we are evolving rapidly in photonics, the production and manipulation of light,” he explained. “Our recent paper explores the hypothesis: We now have the ability to produce light extremely efficiently, and perhaps other species might also have that ability. And if so, then what would be the implications of that? This paper explores the ‘if so, then what?'”
Traditionally and still, Lubin said, the “mainstay of the SETI community” has been to conduct searches via radio waves. Think Jodie Foster in “Contact,” receiving an extraterrestrial signal by way of a massive and powerful radio telescope. With Lubin's UCSB-developed photonics approach, however, making “contact” could be much simpler: Take the right pictures and see if any distant systems are beaconing us.
“All discussions of SETI have to have a significant level of, maybe not humor, but at least hubris as to what makes reason and what doesn't,” Lubin said. “Maybe we are alone in terms of our technological capability. Maybe all that's out there is bacteria or viruses. We have no idea because we've never found life outside of our Earth.
The Daily Galaxy via ucsb.edu
Image credit top of page, NASA-WMAP
europeanspaceagency posted a photo:
Caves offer a dark and alien underground environment with many analogies to space. Deep underground, our senses are deprived of many sounds and natural light. The procedure for moving along a cave wall resembles spacewalking and cave explorers need to stay alert, take critical decisions both as an individual and as a team, just as in space.
The CAVES Cooperative Adventure for Valuing and Exercising course focuses on multicultural approaches to leadership, following orders, teamwork and decision-making.
Credits: ESAS.Sechi
Follow the #CAVES2016 campaign: blogs.esa.int/caves
Credits: ESA-S.Sechi
They have provided physical evidence to a famous story of heroism during the Holocaust — known before only through the testimony of the 11 Jews who escaped a Lithuanian massacre site.
The Obama administration's controversial proposal to revise human research rules is flawed and should be scrapped, says a report from the National Academies of Sciences, Engineering, and Medicine.
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Dating isn't dead, it has just evolved, argues the author Moira Weigel in her book Labor of Love: The Invention of Dating. In fact, how people seek romance is directly related to how the economy changes. In this video by The Atlantic, she explains how romance has moved from the private to the public realm, the significance of dating apps, and why love is still a worthwhile pursuit.
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In Guangzhou, China, millions of mosquitoes are born at the Sun Yat-Sen University-Michigan University Joint Center of Vector Control for Tropical Disease in the hopes of finding a way to fight Zika. The lab's mosquitos are infected with a strain of Wolbachia pipientis, a bacterium that inhibits Zika and and other viruses by preventing the fertilization of eggs. Researchers at the center release infected mosquitos on Shazai island to mate with wild females, stopping the next generation. The lab claims there is 99% suppression of the population of Aedes albopictus or Asia tiger mosquito, the type known to carry Zika virus, after the first year of tests.
marco18678 posted a photo:
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At the E.O. Wilson Biophilia Center in East Freeport, Florida, children are learning about nature by experiencing it firsthand.
Developed by Walton County conservationist M.C. Davis in 2009, the Center sits on the 50,000-acre Nokuse Plantation. Paul Arthur, president of Nokuse Education Inc. and director of E.O. Wilson Biophilia Center for the past five years, describes it as an environmental education center.
“Our ultimate goal is to teach future generations about the importance of conservation, preservation, and restoration of the ecosystem,” Arthur says. “We want every student to leave a little bit of a naturalist.”
Through two- or four-day programs, the Center provides children with a “complete learning experience” that aims to give them an in-depth understanding of the Florida Panhandle's longleaf pine ecosystem, while also exposing them to the idea of conservation more broadly.
The Center's lesson plan aligns with Florida state standards and is adjusted yearly. With over 700 pages of curriculum written by its staff, the Biophilia Center targets 4th and 7th grade students, as standardized testing occurs in 5th and 8th grade. The students come to the Center from schools in its five surrounding counties—Okaloosa, Walton, Bay, Holmes, and Washington.
Each year the Center educates 5,200 students and averages more than 100 students every school day. It places a lot of emphasis on experiential learning; over 20 hands-on activities comprise 75 percent of the overall curriculum. These activities—led by team members with nicknames like Bluegill Jill, Tree Frog Tess, and Pine Tree Paul (Arthur)—include surveying with lasers to analyze topography and slope, water quality testing, and a gopher tortoise simulation class.
“My number one goal is to get students outside,” Arthur says. “We want to immerse them into the environment out here so they get excited about it.”
Their methods are working. In 2014, Columbus State University doctorate candidate Michael Dentzau conducted a two-year study on the effectiveness of the Biophilia Center. Dentzau had 4th grade students draw pictures of Florida's environment before and after they went. According to Arthur, before visiting the Center, students had a warped view of the outdoors, drawing “snow-peaked mountains with giraffes, elephants, and gorillas.” Following their visits to the Center, the students' drawings changed drastically.
“Not only did they draw it [accurately], they started labeling it: loblolly pine, gopher tortoise, eastern indigo, wire grass, turkey oak,” Arthur explains. “That's what really blew us away.”
Dentzau also interviewed students five months after the visit. Much to the Center's delight, they still remembered what they had learned.
“These kids were rattling off information to him that was amazing,” Arthur said. “It was amazing to hear that what we do is effective.”
The Center continues to serve students in northwestern Florida and promote the values of conservationism to the local community as a whole. Arthur notes that the Center hopes to provide a “complete learning experience” so students learn more than just facts.
“People don't understand that when you mess with the food web it affects everything,” he says. “We want the students to understand how important it is that we maintain that balance for the biodiversity of the planet.”
Read more from Paul Arthur and the E.O. Wilson Biophilia Center on Voices for Biodiversity.
Jaime Gordon is a sophomore at Duke University. She plans to declare a major in Cultural Anthropology and a minor in Political Science, while also working on a minor in Japanese and a certificate in Policy Journalism. Born in Jamaica, but raised in the United States, Jaime has always had an interest in how the human experience differs across cultural lines. She wants to travel as much as possible in between her semesters as a full-time student. Though her particular interests are in East Asia and Francophone Europe, Jaime hopes to visit all seven continents in pursuit of novel experiences, artsy photos, and the world's best ice cream.
Read more: Whatsworking, Environment, Food Waste, Hunger, Boston, Reclaim, Hunger Relief, Lovin' Spoonfuls, Food Rescue, Impact News
The Hubble telescope has captured images of a rare tadpole galaxy glittering with bursts of star formation, swimming in the black pond of space.…
Scientists are worried about how Britain's departure from the European Union would hurt the continent's mega-projects and its researchers. Scientific collaboration "should know no borders," says one.
Our thoughts are with the people of Istanbul today, following a gruesome terrorist attack that took place yesterday at the city's main airport. Istanbul is the largest metropolitan area in Turkey, with a population of more than 14 million people. This Overview was captured at night from the @iss. (at Istanbul, Turkey)
Small, poor towns in Texas were flooded with oil and gas workers just a few years ago, bringing a rush of business and prosperity to local economies. Then, seemingly just as soon as they appeared, they were gone again as oil prices tanked across the globe. This short film goes inside Dimmit County, where locals and experts are wondering whether any part of this short-lived success can be salvaged.
Van Alen Sessions is presented by Van Alen Institute with The Atlantic andCityLab. Season Two, “Power Lines,” is directed and produced by Kelly Loudenberg. The series is made possible with support from the National Endowment for the Arts, and is supported, in part, by public funds from the New York City Department of Cultural Affairs in partnership with the City Council. Connect with Van Alen Institute on vanalen.org.
select mixes by genre: | ![]() | ![]() | ![]() | ![]() |
00:00 | rhythm doctor | intro | truelove |
00:39 | grand larceny | body workin | b2 |
03:32 | rich pinder | hat play | d-vine |
07:26 | man without a clue | morning funk mix | clueless |
11:01 | roter lewis | get out of my life | nite grooves |
14:21 | juliet sikora | larry's garage | kitt ball |
19:15 | clio | dangerous | truesoul |
25:40 | be as deep | music makes me happy | plastic people |
32:22 | disk nation | saxophonists | cruise |
35:09 | rene amesz | like it deep | tiger |
41:34 | diskode | burp | moulton |
44:46 | move d | jus house | uzuri |
49:07 | lenny kiser | this time | moulton |
53:37 | soledrifter | soul groove | large |
57:35 | joi resh | here we go | kaleydo |
64:38 | rafa barrios | daledalehey | intec |
67:43 | alan de lanier | dance | mycrazything |
71:49 | soul divine | secret love | stereo flava |
74:54 | manuel sahagun | the 3rd advice | development |
81:13 | kerri chandler | mommy whats a record | downtown |
86:16 | kink | pocket piano | running back |
91:39 | x-press 2 | give it | skint |
My Planet Experience posted a photo:
The Griffon Vulture is a large raptor, inhabitant of the steep cliffs and rocky areas offering numerous cavities where it will nest.
The main cause of the rapid decline in the griffon vulture population is the consumption of poisoned baits set out by people. Wildlife conservation efforts have attempted to increase awareness of the lethal consequences of using illegally poisoned baits through education about the issue. It is very highly vulnerable to the effects of potential wind energy development and electrocution has been identified as a threat.
The flight of the Griffon Vulture is a real show of virtuosity. It soars during long moments, moving scarcely the wings, in an almost unperceivable and measured way.
© www.myplanetexperience.com
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Chevron sending up massive flares in Richmond is not the only sign things are getting hot for the oil giant on the run from a $11 billion verdict.
On June 19th, Chevron's Richmond refinery erupted a torrent of flames and black smoke into the air and terrified local residents. The community remembers all too well when 15,000 people were sent to the hospital when that same refinery exploded in 2012. Unfortunately, since then the public hospital in Richmond has closed. They can't afford another explosion as the closest public emergency room services are now thirty to forty minutes away in Oakland.
But that's not the only thing "on fire" at Chevron lately. Similar to the company's claims that it needs massive flares to burn off excess gas, Chevron claims there's "nothing to see here" as it tries to sell off US $5 billion in assets in its Burnaby oil refinery in British Columbia. But the company's actions and track record tell a different story. Realizing it was going to lose in its legal battle and be forced to accept responsibility for deliberately dumping 18 billion gallons of toxic waste into the Ecuadorian Amazon, Chevron instead sold off all its assets and fled that country. It's been a corporate criminal on the run ever since, but the law is finally catching up with Chevron in Canada.
In September, the Ecuadorian plaintiffs bolstered by a unanimous decision in their favor by Canada's Supreme Court will begin their trial to seize Chevron's Canadian assets to cover its US $11 billion debt to the affected communities in Ecuador.
Chevron currently holds approximately US $15 billion of assets in Canada, almost all of which is at risk due to this enforcement action. Chevron refuses to acknowledge its full liability to the SEC and to its shareholders, and this latest move may give a clue as to why. Unable to replicate its customary racist attacks against Ecuador's judiciary and legal system, Chevron has to dream up new methods in Canada.
The Ecuadorians have defeated Chevron in every single legal contest which has considered the evidence of their crimes in Ecuador (Chevron's singular victory a retaliatory RICO SLAPP suit in the US notoriously forbade any evidence of contamination in its proceedings and is still under appeal). The writing is on the wall in Canada, and Chevron is trying to slip out quietly and escape justice once again.
To make matters worse for the oil giant, a recent U.S. Supreme Court decision on the use of RICO may preemptively doom its defense before the Second Circuit Court of Appeals in New York. As respected appellate attorney Deepak Gupta wrote, the Supreme Court decision "further limits private RICO actions by requiring proof of a quantifiable, redressable and domestic injury something Chevron has steadfastly refuse to identify." The decision also made clear that the RICO statute could not be used to attack a final judgment from a foreign court, as Chevron has tried to do in the Ecuador case. Aaron Page, a U.S. lawyer for the Ecuadorians called it a "nail in the coffin" of Chevron's RICO case. He added, "Now, the Supreme Court has ruled you can't bring a RICO case, even a legitimate one, based on harm that took place abroad. This is another example of why Chevron's RICO case should have been thrown out on day one."
Bottom line on these developments: no matter how desperate it gets, Chevron can't hide its actions in Canada or its pollution in Ecuador or Richmond.
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Puma has collaborated with Designworks — BMW's for-hire design agency — to make a new shoe that pays homage to one of the stranger concept cars of the last decade.
The X-CAT DISC takes styling cues from BMW's GINA Light Visionary Model that debuted in 2008, a roadster with a seamless, silvery fabric pulled taut over a substructure where you'd normally expect metal panels. The car was ridiculous in all the ways you want a true concept car to be: when the swing doors opened, the cloth simply bunched up; when the headlights weren't needed, they disappeared behind cloth "eyelids." Whether you liked the design, you had to give credit to BMW for doing something radically different.
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LG's materials and components subsidiary, LG Innotek, has developed a new type of flexible, textile pressure sensor. The company has yet to commercialize the technology, but says it could be used in a number of industries, including healthcare and car manufacturing. The company points out that current pressure sensors are all inflexible and stiff, whereas LG's new design is made from a flexible, elastic material that means they can be seamlessly integrated into other products. It also detects pressure across the whole of its exterior — not just in specific points.
The company mentions a number of possible use cases for the pressure sensors, including:
Bacon infused vodka may not be everyone's cup of tea, but selling this improbable beverage in Oklahoma could land you in hot water.…
Read more: Nasa, Gif, Sls Test, Nasa Rocket Test, Rocket Booster, Space Launch System, Orion Spacecraft, Orion, Science News
The Public Accounts Committee has advised the UK government to take a more evidence-based approach when deciding spending on science projects, according to a report published today.…
The National Park Service is racing to record soundscapes each park that capture nature for the ear. "If we start to lose sounds of wilderness, we start to lose a piece of us," one scientist says.
Full Text:
Camera-equipped smartphones, laptops and other devices make it possible to share ideas and images with anyone, anywhere, often in real-time. But in our cameras-everywhere culture, the risks of accidentally leaking sensitive information are growing. Computer scientists at Duke University have developed software that helps prevent inadvertent disclosure of trade secrets and other restricted information within a camera's field of view by letting users specify what others can see.
Image credit: Duke University
Full Text:
There are reasons to be interested in the other worlds even if they couldn't possibly harbor life. The hot, rocky planets, for example, offer rare and precious clues to the character and evolution of the early Earth. Numerical models show these exoplanets can change their chemistry by vaporizing rock-forming elements in steam atmospheres that are then partially lost to space.
Image credit: NASA
Will it be a hamburger or hummus wrap for lunch? When customers saw indications of a meal's calorie content posted online, they put fewer calories in their cart, a study finds.
Can a computer write a sonnet that's indistinguishable from what a person can produce? A contest at Dartmouth attempted to find out. With our online quiz, you too can give it a try.
1968 Belgian poster for THE PRODUCERS (Mel Brooks, USA, 1967)
Designer: unknown
Poster source: Posteritati
Happy 90th Birthday Mel Brooks!
The National Air and Space Museum will reopen the “Boeing Milestones of Flight Hall” July 1 in conjunction with the museum's 40th anniversary. The two-year renovation of the hall was made possible by a gift from Boeing. Several of the museum's most iconic artifacts will remain on view, and new ones have been added. The installation will also introduce GO FLIGHT, a digital experience designed to allow visitors to make connections with and between artifacts and to share the national collection beyond the walls of the museum.
A ceremony at 8:30 p.m. will celebrate the anniversary and reopening. “All Night at the Museum” will begin at 9 p.m. and will include activities throughout the night concluding at 10 a.m. July 2. To learn more, visit http://airandspace.si.edu/events/40th-birthday/.
This video shows the Smithsonian's Digitization Program Office 3D scanning three Milestones of Flight Aircraft at the National Air and Space Museum: Spirit of St. Louis, Bell X-1 and SpaceShipOne. Look for these models soon on http://3d.si.edu for viewing and download! #SIx3D and in the newly opened “Boeing Milestones of Flight Hall.”
The post Air and Space Museum's “Boeing Milestones of Flight Hall” Reopens July 1! appeared first on Smithsonian Insider.
Smithsonian staff scientist, Carlos Jaramillo (shown here), and Bruce McFadden from the Florida Museum of Natural History led a 5 year project to collect fossils from and understand the geology of the Panama Canal expansion earthworks. (Photo by Sean Mattson, STRI staff photographer)
The Smithsonian Tropical Research Institute (STRI) celebrated with Panama the completion of the Panama Canal expansion project on June 26, 2016. The $5.6 billion engineering effort allows ships with triple the carrying-capacity of current vessels to transit the canal. The enterprise gave Smithsonian scientists unique opportunities to study two global-scale experiments: a natural, intercontinental land bridge bisected by a man-made, inter-oceanic pathway. They studied fossils, invasive species, whale migration routes, environmental services and changing climate.
STRI staff scientist Carlos Jaramillo along with Bruce McFadden, curator of vertebrate paleontology at the Florida Museum of Natural History, led the five-year Panama Canal Paleontology Project funded by the U.S. National Science Foundation to salvage fossils uncovered by the earthmovers. The fossils reveal ancient migrations of flora and fauna between North and South America and include new species such as Panamacebus transitus, the earliest monkey found in North America. Excavations expose an unusually complete view of the geology of the isthmus' formationthis record of global transformation of ocean currents, weather patterns and ecosystems would otherwise have remained buried under rock and rainforest.
The canal expansion reopens questions about whether exotic species will cross the freshwater corridor to establish themselves on the other side, potentially disrupting the existing ocean ecosystems. Former STRI director Ira Rubinoff argued in the 1960s that maintaining a freshwater bridge between oceans sharply reduced the risk of invasions likely with a sea-level canal, since most marine organisms cannot withstand abrupt changes in salinity. Staff scientist Mark Torchin asks if exotic speciesand their parasites — will be helped or hindered by increased ship traffic arriving daily from around the world.
Nearly 17,000 commercial vessels cross the Gulf of Panama each year. Staff scientist Hector Guzman's studies of humpback whale migration led the government of Panama to propose a “traffic separation scheme” to the International Maritime Organization. Ships in the Bay of Panama now reduce their speed and come into the Pacific entrance to the Canal through a narrow shipping lane. Researchers expect this to reduce the probability of collisions between ships and whales by 95 percent.
Catalina Pimiento was able to do her Ph.D. thesis at the University of Florida, excavating teeth of the largest shark ever, from the Panama Canal expansion earthworks. (STRI photo)
To study the Canal's freshwater heartbeat scientists turn to its source — the surrounding forests. The Republic of Panama established Soberania National Park and additional protected areas to conserve the forested watersheds that supply the canal with its lifeblood. At the Agua Salud project located near Soberania, staff scientist Jefferson Hall and colleagues ask how native tree species in lowland tropical forests regulate water flow through soil, help maintain biodiversity and store carbon. The project recently collaborated with the BIO Program of the Inter-American Development Bank to produce the free, online publication, Managing Watersheds for Ecosystem Services in the Steepland Neotropics.
“Climate change increases the likelihood of extreme weather, such as intense storms and droughts,” said Matthew Larsen, director of STRI. “We don't fully understand how the hydrologic and other natural systems in the Panama watershed will respond. STRI's ongoing scientific investigations help the Panama Canal Authority and land-use managers to better understand the range of future conditions.”
Last year's El Niño put the risk of water shortages in the canal into sharp relief. STRI monitoring stations throughout the region contribute to understanding such events. STRI maintains more than a dozen research facilities throughout Panama, including the Punta Galeta Marine Education Center near the Caribbean entrance to the canal and the Pacific-side Punta Culebra Nature Center. Both are open to the public, offering exhibits and educational tours.
STRI's presence in Panama has always been intertwined with the canal. From 1910 to 1912, the Smithsonian's Panama Biological Survey resulted in the first inventory of species and assessment of environmental conditions across the canal watershed. Panama's President Pablo Arosemena encouraged scientists to extend their survey throughout the country, creating an important baseline for understanding the wealth and diversity of the region's natural resources. The Barro Colorado Island research station was established in Lake Gatun, then newly flooded, in 1923. In 2016, along with Panama and the world, STRI looks forward to the fresh pulse that marks the completion of the canal expansion project.
The post Smithsonian celebrates Panama Canal expansion! appeared first on Smithsonian Insider.
By combining data from Chandra and several other telescopes, astronomers have identified the true nature of an unusual source in the Milky Way galaxy. This discovery implies that there could be a much larger number of black holes in the Galaxy that have previously been unaccounted for. For about two decades, astronomers have known about an object called VLA J213002.08+120904 (VLA J2130+12 for short). Although it is close to the line of sight to the globular cluster M15, most astronomers had thought that this source of bright radio waves was probably a distant galaxy.
Thanks to recent distance measurements with an international network of radio telescopes, including the EVN (European Very Long Baseline Interferometry Network) telescopes, the NSF's Green Bank Telescope and Arecibo Observatory, astronomers realized that VLA J2130+12 is at a distance of 7,200 light years, showing that it is well within our own Milky Way galaxy and about five times closer than M15. A deep image from Chandra reveals it can only be giving off a very small amount of X-rays, while recent VLA data indicates the source remains bright in radio waves.
This new study indicates that VLA J2130+12 is a black hole a few times the mass of our Sun that is very slowly pulling in material from a companion star. At this paltry feeding rate, VLA J2130+12 was not previously flagged as a black hole since it lacks some of the telltale signs that black holes in binaries typically display.
"Usually, we find black holes when they are pulling in lots of material. Before falling into the black hole this material gets very hot and emits brightly in X-rays," said Bailey Tetarenko of the University of Alberta, Canada, who led the study. "This one is so quiet that it's practically a stealth black hole."
This is the first time a black hole binary system outside of a globular cluster has been initially discovered while it is in such a quiet state.
Hubble observations identified VLA J2130+12 with a star having only about one-tenth to one-fifth the mass of the Sun. The observed radio brightness and the limit on the X-ray brightness from Chandra allowed the researchers to rule out other possible interpretations, such as an ultra-cool dwarf star, a neutron star, or a white dwarf pulling material away from a companion star.
In the graphic below, the images on the left show X-rays from Chandra and an optical image from Hubble of a large area around the source VLA J2130+12, including M15. The images on the right show the source VLA J2130+12 that is bright in radio waves, but can only be giving off a very small amount of X-rays. These pieces of information indicate the source contains a black hole with a few times the mass of the Sun.
Because this study only covered a very small patch of sky, the implication is that there should be many of these quiet black holes around the Milky Way. The estimates are that tens of thousands to millions of these black holes could exist within our Galaxy, about three to thousands of times as many as previous studies have suggested.
"Unless we were incredibly lucky to find one source like this in a small patch of the sky, there must be many more of these black hole binaries in our Galaxy than we used to think," said co-author Arash Bahramian, also of the University of Alberta.
There are other implications of finding that VLA J2130+12 is relatively near to us. "Some of these undiscovered black holes could be closer to the Earth than we previously thought," said Robin Arnason, a co-author from Western University, Canada "However there's no need to worry as even these black holes would still be many light years away from Earth."
Sensitive radio and X-ray surveys covering large regions of the sky will need to be performed to uncover more of this missing population. If, like many others, this black hole was formed in the plane of the Milky Way's disk, it would have needed a large kick at birth to launch it to its current position about 3,000 light years above the plane of the Galaxy.
The Daily Galaxy via International Center for Radio Astronomy Research
Image Credit: X-ray: NASA/CXC/Univ. of Alberta/B.Tetarenko et al; Optical: NASA/STScI; Radio: NSF/AUI/NRAO/Curtin Univ./J. Miller-Jones) and ALMA Observatory
Astronomers have long known that organic molecules form in diffuse gas clouds floating between stars. It is thought that as the Solar System formed 4.6 billion years ago, some of these organic molecules were transported from interstellar space to the planet forming disk. Later, these molecules played important roles in the chemical evolution resulting in the emergence of life on the Earth.
However, it is still unknown what kinds and quantities of organic molecules were actually supplied from interstellar space. Although radio astronomy observations during the last decade showed that saturated complex organic molecules, such as methanol (CH3OH) and methyl formate (HCOOCH3) [1], exist around Solar-type protostars, their distributions were too compact to be resolved with the radio telescopes available at the time.
With ALMA, an international team lead by Yoko Oya, a graduate student of Department of Physics, The University of Tokyo, and Nami Sakai, an associate chief scientist of RIKEN, studied the distribution of various organic molecules around a Solar-type protostar IRAS 16293-2422A at a high spatial resolution. They discovered a ring structure of complex organic molecules around the protostar. The radius of the ring is 50 times wider than the Earth's orbit. This size is comparable to the size of the Solar System, and the ring structure most likely represents the boundary region between infalling gas and a rotating disk structure around the protostar.
The observations clearly showed the distribution of large organic molecules methyl formate (HCOOCH3) and carbonyl sulfide (OCS). Apparently the distribution of methyl formate is confined in a more compact area around the protostar than the OCS distribution, which mainly traces the infalling gas. "When we measured the motion of the gas containing methyl formate by using the Doppler effect," said Oya "we found a clear rotation motion specific to the ring structure." In this way, they identified the rotating ring structure of methyl formate, although it is not resolved spatially. A similar ring structure is also found for methanol.
These saturated organic molecules are formed in interstellar space and are preserved on the surfaces of dust grains. Around the outer boundary of the disk structure, they evaporate due to shock generated by collisions of the disk and infalling material, and/or due to heating by the light from the baby star. This result is the first direct evidence that interstellar organic materials are indeed fed into the rotating disk structure that eventually forms a planetary system.
In 2014, the team found a similar ring structure of SO (sulfur monoxide) around another Solar-type protostar L1527. In this source, unsaturated complex organic molecules such as CCH and cyclic-C3H2 are very abundant in the infalling gas, while SO preferentially exists in the boundary between the infalling gas and the disk structure. Although the physical structure in L1527 is similar to that found in IRAS 16293-2422A, the chemical composition is much different. Saturated complex organic molecules are almost completely absent in L1527.
The present result, taken together with previous results on L1527, clearly demonstrates for the first time that the materials delivered to a planetary system differ from star to star. A new perspective on chemical composition is thus indispensable for a thorough understanding of the origin of the Solar System and the origin of life on the Earth.
The Daily Galaxy via National Institutes of Natural Sciences
A Southwest Research Institute-led team has discovered an elusive, dark moon orbiting Makemake, one of the "big four" dwarf planets populating the Kuiper Belt region at the edge of our solar system. The findings are detailed in the paper "Discovery of a Makemakean Moon," published in the June 27 issue of Astrophysical Journal Letters.
"Makemake's moon proves that there are still wild things waiting to be discovered, even in places people have already looked," said Dr. Alex Parker, lead author of the paper and the SwRI astronomer credited with discovering the satellite. Parker spotted a faint point of light close to the dwarf planet using data from Hubble's Wide Field Camera 3. "Makemake's moon -- nicknamed MK2 -- is very dark, 1,300 times fainter than the dwarf planet."
A nearly edge-on orbital configuration helped it evade detection, placing it deep within the glare of the icy dwarf during a substantial fraction of its orbit. Makemake is one of the largest and brightest known Kuiper Belt Objects (KBOs), second only to Pluto. The moon is likely less than 100 miles wide while its parent dwarf planet is about 870 miles across. Discovered in 2005, Makemake is shaped like football and sheathed in frozen methane.
"With a moon, we can calculate Makemake's mass and density," Parker said. "We can contrast the orbits and properties of the parent dwarf and its moon, to understand the origin and history of the system. We can compare Makemake and its moon to other systems, and broaden our understanding of the processes that shaped the evolution of our solar system."
With the discovery of MK2, all four of the currently designated dwarf planets are known to host one or more satellites. The fact that Makemake's satellite went unseen despite previous searches suggests that other large KBOs may host hidden moons.
Prior to this discovery, the lack of a satellite for Makemake suggested that it had escaped a past giant impact. Now, scientists will be looking at its density to determine if it was formed by a giant collision or if it was grabbed by the parent dwarf's gravity. The apparent ubiquity of moons orbiting KBO dwarf planets supports the idea that giant collisions are a near-universal fixture in the histories of these distant worlds.
The Daily Galaxy via Southwest Research Institute
"The dips found by Kepler are real. Something seems to be transiting in front of this star and we still have no idea what it is!" confirms German astronomer Michael Hippke. Even if aliens are not involved, Tabby's star remains "the most mysterious star in the universe" as Yale astronomer Tabetha Boyajian described it in a TED talk she gave last February.
The results of a new study make it far less likely that KIC 8462852, popularly known as Tabby's star, is the home of industrious aliens who are gradually enclosing it in a vast shell called a Dyson sphere. Media interest went viral last October when a group of astronomers from Pennsylvania State University released a preprint that cited KIC 8462852's "bizarre light curve" as "consistent with" a swarm of alien-constructed megastructures.
Public interest in the star, which sits about 1,480 light-years away in the constellation Cygnus, began last fall("Tabby") Boyajian and colleagues posted a paper on an astronomy preprint server reporting that "planet hunters" - a citizen science group formed to search data from the Kepler space telescope for evidence of exoplanets - had found unusual fluctuations in the light coming from the otherwise ordinary F-type star (slightly larger and hotter than the sun).
The most remarkable of these fluctuations consisted of dozens of uneven, unnatural-looking dips that appeared over a 100-day period indicating that a large number of irregularly shaped objects had passed across the face of the star and temporarily blocked some of the light coming from it.
The top panel of the graphic below shows four years of Kepler observations of the 12th-magnitude star KIC 8462852 in Cygnus. Several sporadic dips in its light output (normalized to 100%) hint that something is partially blocking its light. The portion highlighted in yellow, recorded in February to April 2013, is shown at three different scales along the bottom. The random, irregular shape of each dip could not be caused by a transiting exoplanet. (T. Boyajian & others / MNRAS).
The attention caused scientists at the SETI Institute to train its Alien Telescope Array on the star to see if they could detect any radio signals indicating the presence of an alien civilization. In November it reported finding "no such evidence" of signals with an artificial origin.
Then a study released in January by a Louisiana State University astronomer threw even more fuel on the fire of alien speculation by announcing that the brightness of Tabby's star had dimmed by 20 percent over the last century: a finding particularly difficult to explain by natural means but consistent with the idea that aliens were gradually converting the material in the star's planetary system into giant megastructures that have been absorbing increasing amounts of energy from the star for more than a century. That study has now been accepted for publication in the peer reviewed Astrophysical Journal.
However, a new study - also accepted for publication in the Astrophysical Journal - has taken a detailed look at the observations on which the LSU study was based and concluded there is no credible evidence that the brightness of the star been steadily changing over this period.
When the LSU study was posted on the physics preprint server ArXiv, it caught the attention of Vanderbilt doctoral student Michael Lund because it was based on data from a unique resource: Digital Access to a Sky Century @ Harvard. DASCH consists of more than 500,000 photographic glass plates taken by Harvard astronomers between 1885 and 1993, which the university is digitizing. Lund was concerned that the apparent 100-year dimming of Tabby's star might just be the result of observations having been made by a number of different telescopes and cameras that were used during the past century.
Lund convinced his advisor, Professor of Physics and Astronomy Keivan Stassun, and a frequent collaborator, Lehigh University astronomer Joshua Pepper, that the question was worth pursuing. After they began the study, the Vanderbilt/Lehigh group discovered that another team - German amateur astronomer Michael Hippke and NASA Postdoctoral Fellow Daniel Angerhausen - were conducting research along similar lines. So the two teams decided to collaborate on the analysis, which they wrote up and submitted to the Astrophysical Journal.
"Whenever you are doing archival research that combines information from a number of different sources, there are bound to be data precision limits that you must take into account," said Stassun. "In this case, we looked at variations in the brightness of a number of comparable stars in the DASCH database and found that many of them experienced a similar drop in intensity in the 1960's. That indicates the drops were caused by changes in the instrumentation not by changes in the stars' brightness."
The planet hunters first detected something unusual in the star's light curve in 2009. They found a 1 percent dip that lasted a week. This is comparable to the signal that would be produced by a Jupiter-sized planet passing in front of the star. But planets produce symmetric dips and the one they found was decidedly asymmetric, like something that would be produced by an irregular-shaped object like a comet.
The light from the star remained steady for two years, then it suddenly took a 15 percent plunge that lasted for a week.
Another two years passed without incident but in 2013 the star began flickering with a complex series of uneven, unnatural looking dips that lasted 100 days. During the deepest of these dips, the intensity of the light coming from the star dropped 20 percent. According to Boyajian it would take an object 1,000 times the area of the Earth transiting the distant star to produce such a dramatic effect.
"The Kepler data contains other cases of irregular dips like these, but never in a swarm like this," said Stassun.
Boyajian and her colleagues considered a number of possible explanations, including variations in the star's output, the aftermath of an Earth/Moon type planetary collision, interstellar clumps of dust passing between the star and earth, and some kind of disruption by the star's apparent dwarf companion. However, none of their scenarios could explain all of the observations. Their best explanation was a giant comet that fragmented into a cascade of thousands of smaller comets. (This hypothesis took a hit when the LSU study was announced because it could not explain a century-long dimming.)
The Kepler telescope is no longer collecting data in the Cygnus region, but Hippke reports that the mystery has captured the imagination of amateur astronomers around the world so thousands of them are pointing their telescopes at Tabby's star, snapping images and sending them to the American Association of Variable Star Observers in hopes of detecting further dips that will shed new light on this celestial mystery.
The Daily Galaxy via Vanderbilt University
"Unusual News" --From Around the Planet & Beyond (Sponsored Site)
europeanspaceagency posted a photo:
stronauts from five space agencies around the world are taking part in ESA's CAVES training course Cooperative Adventure for Valuing and Exercising human behaviour and performance Skills.
The two-week course prepares astronauts to work safely and effectively in multicultural teams in an environment where safety is critical.
As they explore the caves of Sardinia they will encounter caverns, underground lakes and strange microscopic life. They will test new technology and conduct science just as if they were living on the International Space Station. The six astronauts will rely on their own skills, teamwork and ground control to achieve their mission goals the course is designed to foster effective communication, decision-making, problem-solving, leadership and team dynamics.
This year is the first international space cooperation to involve astronauts from China, Russia, Japan, ESA and America, with cosmonaut Sergei Vladimirovich, ESA astronaut Pedro Duque, taikonaut Ye Guangfu, Japanese astronaut Aki Hoshide and NASA astronauts Ricky Arnold and Jessica Muir taking part.
After a week of training (pictured), the ‘cavenauts' will say goodbye to sunlight and spend six nights underground, setting up basecamp in the Sa Grutta cave in Sardinia, Italy.
Follow CAVES via twitter with #CAVES or on the CAVES blog .
Scientists have been trying to puzzle out for decades why the universe seems to weigh more than it should, and so far the answer points to dark matter—an invisible substance that they still don't clearly understand and is thought to exist in clumps throughout the universe. Dark matter, believed by physicists to outweigh all the normal matter in the universe by more than five to one, is by definition invisible. But, scientists at MIT and elsewhere have developed a new tool that could test to see if dark matter is detectable.
However, an exotic particle -a "dark photon"- that resembles a photon, but with mass, has been proposed by some theorists to explain dark matter — whose nature is unknown but whose existence can be inferred from the gravitational attraction it exerts on ordinary matter, such as in the way galaxies rotate and clump together.
“We're looking for a massive photon,” explains MIT physics professor Richard Milner. That may seem like a contradiction in terms: Photons, or particles of light, are known to be massless. If it does exist, that would represent a major discovery, Milner says. “It's totally beyond anything we understand about the physical world. A massive photon would be totally different” from anything allowed by the Standard Model, the bedrock of modern particle physics. "It's a tiny effect,” Milner adds, but “it can have enormous consequences for our theories and our understanding. It would be absolutely groundbreaking in physics.”
The experiment known as DarkLight, developed by MIT physics professor Peter Fisher and Milner in collaboration with researchers at the Jefferson National Accelerator Laboratory in Virginia and others, will look for evidence a massive dark photon with a specific energy postulated in one particular theory about dark matter, Milner says. If the planned experiment detects the A' particle, says Roy Holt, a distinguished fellow in the physics division at Argonne National Laboratory says, “it would signal that dark matter could actually be studied in a laboratory setting.”
Meanwhile, team of physicists at the University of California have uploaded on Arvix (the e-print archive with over 100,000 articles in physics) work done by a team in Hungary in 2015 that might have revealed the existence of this fifth force of nature. The Hungarian team, led by Attila Krasznahorkay, examined the possible existence of dark photons that work with dark matter. The Berkeley team has challenged the findings, suggesting that the new particle found by the Hungarian team was not a dark photon, but possibly a protophobic X boson, which might carry a super-short force which acts over just the width of an atomic nucleus.
To prove the existence of the theorized particle, dubbed A' (“A prime”), the Darklight experiment will use a particle accelerator at the Jefferson Lab that has been tuned to produce a very narrow beam of electrons with a megawatt of power. That's a lot of power, Milner says: “You could not put any material in that path,” he says, without having it obliterated by the beam. For comparison, he explains that a hot oven represents a kilowatt of power. “This is a thousand times that,” he says, concentrated into mere millionths of a meter.
The Jefferson Lab's Free Electron Laser, in Virginia, will bombard an oxygen target with a stream of electrons with one megawatt of power. This will be able to test for these massive photons at a mass-energy of up to 100 MeV. It is hoped that this hugely powerful beam of electrons will hit the target and create this theorized form of dark matter (A' particles). The dark matter, if it's created, will then immediately decay into two other particles that can be easily detected.
The MIT paper confirms that the new facility's beam meets the characteristics needed to definitively detect the hypothetical particle — or rather, to detect the two particles that it decays into, in precise proportions that would reveal its existence. Doing so, however, will require up to two years of further preparations and testing of the equipment, followed by another two years to collect data on millions of electron collisions in the search for a tiny statistical anomaly.
While DarkLight's main purpose is to search for the dark photon A' particle, it also happens to be well suited to addressing other major puzzles in physics, Milner says. It can probe the nature of a reaction, inside stars, in which carbon and helium fuse to form oxygen — a process that accounts for all of the oxygen that now exists in the universe.
“This is the stuff we're all made of,” Milner says, and the rate of this reaction determines how much oxygen exists. While that reaction rate is very hard to measure, Milner says, the DarkLight experiment could illuminate the process in a novel way: “The idea is to do the inverse.” Instead of fusing atoms to form oxygen, the experiment would direct the powerful beam at an oxygen target, causing it to split into carbon and helium. That, Milner says, would provide an indirect way of determining the stellar production rate.
In 2012, Simona Vegetti, a physics fellow at MIT, discovered an entire galaxy made of dark matter just outside the Milky Way. The dark galaxy may host a luminous galaxy made invisible by the dark matter. “The thing people like about dark matter is that it's been able to explain so many observations,” Vegetti said.
Because dark matter reflects no light, the galaxy is elusive. Vegetti worked with an international team of scientists including three from the U.S. and two from the Netherlands. Using the Keck Telescope in Hawaii, they detected the galaxy by studying ripples in the patterns of light rays from the Milky Way, a method known as gravitational lensing.
“It's a dark matter-dominated object,” Vegetti said, “So there might be stars but very little.”
There are thought to be more than 10,000 satellite galaxies attached to our Milky Way galaxy, but only 30 of them are visible, she said. The image above shows the Sagittarius Dwarf Galaxy, named for the constellation in which it is seen from the earth, in the process of colliding and merging with our own Milky Way. “The question becomes are these satellites missing because they don't exist or because they are purely dark? And that's one question we're trying to answer,” she said.
In the image at the top of the page, the bright source in the upper left is an active galaxy in the cluster, Abell 2142, six million light years across that contains hundreds of galaxies and enough gas to make a thousand more. It is one of the most massive objects in the universe.
The Daily Galaxy via MIT, Northwestern, and Physical Review Letters
Chris Forsyth captures Europe's overlooked underground spaces
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'je te pardonne' (I forgive you) is not intended as an homage, rather a search for humanity in the wake of tragedy.
The post monumental leila alaoui exhibition at galleria continua seeks to rediscover humanity appeared first on designboom | architecture & design magazine.
on the street-facing façade of a residential building, the artist has painted a brain-bending optical illusion that sees a wall seemingly penetrate a deep and dark abyss.
The post astro's brain-bending mural turns an apartment into an architectural wormhole appeared first on designboom | architecture & design magazine.
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Snowy Plover Fights for the Right to Exist.
Today's generation of fighter pilots could be the last of their breed, thanks to an AI system dubbed ALPHA that's proving unkillable in air combat.…
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Let's be honest, these are challenging times to be a conservationist, animal lover, nature fan, outdoorsman…a human. No matter the label, one thing that we all share in common is a desire to feel wonder: a wonder that often arises from experiences in the natural world.
Somehow, just knowing that incredible creatures are out there, moving through landscapes that revolve unperceivably slowly on their own dials, without regard or subservience to man's hand, connects us to something deeper. It allows us to believe that it will all be okay. That life was here before, and so will it be in the future. Eternity.
As such, it somehow seems like a sacrilege to validate the worthiness of nature—of a species—by weights and measures, dollars and cents. Too often we impatiently demand to know what good it does for us, the conquerors, the victors, to whom the spoils go daily. As if a row of decimal points could ever serve as the demarcation line between gold and garbage, your own mother on auction like a prize pig at the county fair.
I first discovered the rusty-patched bumble bee in a box on a museum shelf at Great Smoky Mountains National Park. I was there to look at the spectral array of bees that were native to the region. While I quickly scanned the collection like an eager child on Christmas morning, Becky Nichols, the park entomologist, drew my attention to one species that hadn't been seen in the Smokies for years.
It wasn't flashy or particularly outstanding in appearance. Even amongst bumble bees it seemed rather dull and unassuming. Only a hint of a fading rusty band, an oxidized kiss of orange on its abdomen, gave a clue to the origin of its common name. It was a species that was once abundant throughout the eastern US and into the upper Midwest, but then it wasn't; nearly winking out before most people even knew it existed.
There was a stuffed passenger pigeon in the same room, staring off into space with its glass eyes. This was once the most numerous bird on the continent, but we eliminated it before we even suspected such a thing was possible. I wondered if the rusty-patched bumble bee, like the passenger pigeon, was another ghost in the making.
It was at that moment that I knew that I had to see a living rusty-patched bumble bee. I wanted to hear the deep thrum of its wings and know, really know, what it was like to behold its presence. If there was ever a precious natural commodity, this was the currency that held the most value to me. This pivotal moment sent me off along the path of an incredibly journey, which culminated in many unexpected, insightful experiences, and a short film that will hopefully give others a sense of what we stand to lose if this species fades into extinction.
In the film, University of Wisconsin entomologist Dr. Claudio Gratton sites a provocative paper that looks at the economic value of native bees. Pollination services are often used as a reason to protect bees and other native pollinators. However, this paper suggests that a core group of bees are responsible for the majority of crop pollination. We have nearly 4,000 species of native bees in North America, none of which are protected under the Endangered Species Act. If crop pollination is our only justification for which species get graced with our approval to continue to exist, what happens to those that have no obvious value to us? Perhaps, as Dr. Gratton so elegantly puts it, this says more about how we value life in general than anything else.
If you'd like to speak up for the protection rusty-patched bumble, a species that has declined 87 percent in the past 15 years, please consider signing our petition requesting that the U.S. Fish and Wildlife Service place it under the care of the Endangered Species Act.
We spend so much time and effort trying to make life better for ourselves. The least we can do is make life possible for this bee.
Learn more at www.rustypatched.com.
Clay Bolt is a Natural History and Conservation Photographer specializing in the world's smaller creatures. He regularly partners with organizations such as the National Geographic Society, National Wildlife Federation, and the Xerces Society for Invertebrate Conservation. He is an Associate Fellow in the International League of Conservation Photographers (iLCP), president-elect of the North American Nature Photography Association (NANPA), and co-founder (2009) of the international nature and biodiversity photography project, Meet Your Neighbours. His current major focus is on North America's native bees and the important roles that they play in our lives. Clay lives in Bozeman, Montana where he is the communications lead for WWF's Northern Great Plains Program. Visit www.claybolt.com to learn more.
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The main line of inquiry should not focus on why the animal was shot, but rather what happened leading up to that unfortunate moment.
I can't help but wonder: What is the message conveyed by exposing a live animal as a mascot in front of a crowd?
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Every year, thousands of young women leave their Myanmar villages in search of work abroad—and many get stuck in forced labor. In this film by the Thomson Reuters Foundation, we hear some of their stories.
The Watts neighborhood of Los Angeles, California, is benefitting from the clean energy boom and all of the jobs that come with it. In this video, we go inside a solar installation training site to meet several women who are participating in the quest for clean energy and its economic benefits.
Van Alen Sessions is presented by Van Alen Institute with The Atlantic andCityLab. Season Two, “Power Lines,” is directed and produced by Kelly Loudenberg. The series is made possible with support from the National Endowment for the Arts, and is supported, in part, by public funds from the New York City Department of Cultural Affairs in partnership with the City Council. Connect with Van Alen Institute on vanalen.org.
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Saying that living organisms are algorithms is, in the very least, misleading and in strict terms, false.
There is no evidence that pure intellectual processes can form the basis for what makes us distinctly human.
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Check out this incredible drone shot of a road slicing through the forest near Pysht, Washington, USA. This one was captured and shared with us by @monascherie (at Pysht, Washington)
Read more: Gif, Motorcycle Accident, Motorbike Accident, I 94, Linda Leverty, Weird News News
There's an assumption that beauty and quality are connected by an unbreakable bond.
In my opinion, awareness, the feeling of self-efficiency, and responsibility are necessary ingredients for action and therefore for citizens' political participation.
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CBP Photography posted a photo:
ANZALDUAS, Texas Agriculture specialists with U.S. Customs and Border Protection, Office of Field Operations (OFO) at the Hidalgo/Pharr/Anzalduas Port of Entry have intercepted and seized an elephant skull that lacked proper ownership and exportation documentation, as required under U.S. and international law. Our CBP officers and agriculture specialists partner with the U.S. Fish and Wildlife Service (FWS) to enforce federal wildlife laws that protect vulnerable and endangered species.
Photo provided by U.S. Customs and Border Protection
Domenico Fontana Scientist of the Day
Domenica Fontana, an Italian engineer, died June 28, 1607, at about age 64.
A chemical camera sitting atop Curiosity, the Mars rover, has spotted signs that the Red Planet may have once had oxygen in its atmosphere, fuelling further speculation that it was once Earth-like.…
The recalled Jeep shifter that may have been involved in Star Trek actor Anton Yelchin's death is a straightforward example of how things get harder to use when you take controls out of hardware and put them into software. It's a UI problem, and an entirely avoidable one.
First things first: if you have a 2014 or 2015 Jeep Grand Cherokee or a 2012-2014 Dodge Charger or Chrysler 300, you should call your dealer right now and set up an appointment for the recall. According to my local dealer, the update takes 3.5 hours, and it patches the car's software to engage the emergency brake if the driver's door is opened when the car is in neutral. That's it. It's a software update that was finally accelerated in the past few weeks after a death,...
Will it be a hamburger or hummus wrap for lunch? When customers saw indications of a meal's calorie content posted online, they put fewer calories in their cart, a study finds.
¡Bong! [The following memo was found in a pilates studio in Shoreditch earlier this month, and forwarded to us anonymously. It is sourced to "BV Strategic Relations”, a highly secretive firm apparently registered in Panama, which describes itself as a "bespoke crisis management consultancy to governments”. The authenticity of the memo has been confirmed by to us by a representative of the firm, มาลัย (which means Garland of Flowers in Thai) - ed]…
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Mathias Appel posted a photo:
Reupload. Edited it a little differently.
Divers exploring the famous Antikythera shipwreck, 200 feet beneath the water's surface in Greece, have turned up a heavy object they think might have been a powerful weapon in the first century B.C.
Keep calm and carry on; artificial intelligence will not take all our jobs and achieve world domination, according to a report released by Forrester.…
Full Text:
Pictured here, the Cerro Tololo Inter-American Observatory's (CTIO) 4-meter Blanco Telescope is a silhouette against the Magellanic Clouds (at left) and the Milky Way, as seen from Cerro Tololo, Chile. CTIO provides qualified scientists with telescopes and related facilities for astronomical research in the Southern Hemisphere. CTIO has offices, labs and living quarters in the coastal city of La Serena, 482-kilometers north of Santiago. The observing facilities are on Cerro Tololo, a 2,194-meter mountain on the western slopes of the Andes Mountains, 64-kilometers inland from La Serena.
Image credit: Roger Smith/NOAO/AURA/NSF
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Strands of cow cartilage substitute for ink in a 3D bioprinting process that may one day create cartilage patches for worn out joints, according to a team of engineers. Cartilage is a good tissue to target for scale-up bioprinting because it is made up of only one cell type and has no blood vessels within the tissue. It is also a tissue that cannot repair itself. Once cartilage is damaged, it remains damaged.
Image credit: Ibrahim Ozbolat, Penn State University
The discovery of manganese oxides in Martian rocks might tell us that the Red Planet was once more Earth-like than previously believed. A new paper in Geophysical Research Letters reveals that NASA's Curiosity rover observed high levels of manganese oxides in Martian rocks, which could indicate that higher levels of atmospheric oxygen once existed on our neighboring planet. This hint of more oxygen in Mars' early atmosphere adds to other Curiosity findings--such as evidence of ancient lakes--revealing how Earth-like our neighboring planet once was.
"The only ways on Earth that we know how to make these manganese materials involve atmospheric oxygen or microbes," said Nina Lanza, a planetary scientist at Los Alamos National Laboratory and lead author on the study published in the American Geophysical Union's journal. "Now we're seeing manganese-oxides on Mars and wondering how the heck these could have formed."
Lanza uses the Los Alamos-developed ChemCam instrument that sits atop Curiosity to "zap" rocks on Mars and analyze their chemical make-up. This work stems from Los Alamos National Laboratory's experience building and operating more than 500 spacecraft instruments for national defense, giving the Laboratory the expertise needed to develop discovery-driven instruments like ChemCam. In less than four years since landing on Mars, ChemCam has analyzed roughly 1,500 rock and soil samples.
Microbes seem a far-fetched explanation for the manganese oxides at this point, said Lanza, but the idea that the Martian atmosphere contained more oxygen in the past than it does now seems possible. "These high-manganese materials can't form without lots of liquid water and strongly oxidizing conditions," said Lanza "Here on Earth, we had lots of water but no widespread deposits of manganese oxides until after the oxygen levels in our atmosphere rose due to photosynthesizing microbes."
In the Earth's geological record, the appearance of high concentrations of manganese is an important marker of a major shift in our atmosphere's composition, from relatively low oxygen abundances to the oxygen-rich atmosphere we see today. The presence of the same types of materials on Mars suggests that something similar happened there. If that's the case, how was that oxygen-rich environment formed?
"One potential way that oxygen could have gotten into the Martian atmosphere is from the breakdown of water when Mars was losing its magnetic field," said Lanza. "It's thought that at this time in Mars' history, water was much more abundant."
Yet without a protective magnetic field to shield the surface from ionizing radiation, that radiation started splitting water molecules into hydrogen and oxygen. Because of Mars' relatively low gravity, it wasn't able to hold onto the very light hydrogen atoms, but the heavier oxygen atoms remained behind. Much of this oxygen went into the rocks, leading to the rusty red dust that covers the surface today. While Mars' famous red iron oxides require only a mildly oxidizing environment to form, manganese oxides require a strongly oxidizing environment. These results suggest that past conditions were far more oxidizing (oxygen-rich) than previously thought.
"It's hard to confirm whether this scenario for Martian atmospheric oxygen actually occurred," Lanza added. "But it's important to note that this idea represents a departure in our understanding for how planetary atmospheres might become oxygenated." So far, abundant atmospheric oxygen has been treated as a so-called biosignature, or a sign of existing life.
The next step in this work is for scientists to better understand the signatures of non-biogenic versus biogenic manganese, which is directly produced by microbes. If it's possible to distinguish between manganese oxides produced by life and those produced in a non-biological setting, that knowledge can be directly applied to Martian manganese observations to better understand their origin.
The high-manganese materials were found in mineral-filled cracks in sandstones in the Kimberley region of Gale crater, which the Curiosity rover has been exploring for the last four years. But that's not the only place on Mars that abundant manganese has been found. The Opportunity rover, which has been exploring Mars since 2004, also recently discovered high-manganese deposits in its landing site thousands of miles from Curiosity, which supports the idea that the conditions needed to form these materials were present well beyond Gale crater. The ,image at the top of the page is an artist's concept of how the "lake" at Gale Crater on Mars may have looked millions of years ago. (credit Kevin Gill).
The Daily Galaxy via Los Alamos National Laboratory
Over the past two weeks, several milestones occurred that were key to a successful 35-minute burn of its rocket motor, which will place the robotic explorer into a polar orbit around the gas giant. "We have over five years of spaceflight experience and only 10 days to Jupiter orbit insertion," said Rick Nybakken, Juno project manager from NASA's Jet Propulsion Laboratory in Pasadena, California. "It is a great feeling to put all the interplanetary space in the rearview mirror and have the biggest planet in the solar system in our windshield."
On June 11, Juno began transmitting to and receiving data from Earth around the clock. This constant contact will keep the mission team informed on any developments with their spacecraft within tens of minutes of it occurring. On June 20, the protective cover that shields Juno's main engine from micrometeorites and interstellar dust was opened, and the software program that will command the spacecraft through the all-important rocket burn was uplinked.
One of the important near-term events remaining on Juno's pre-burn itinerary is the pressurization of its propulsion system on June 28. The following day, all instrumentation not geared toward the successful insertion of Juno into orbit around Jupiter on July 4 will be turned off.
"If it doesn't help us get into orbit, it is shut down," said Scott Bolton, Juno's principal investigator from the Southwest Research Institute in San Antonio. "That is how critical this rocket burn is. And while we will not be getting images as we make our final approach to the planet, we have some interesting pictures of what Jupiter and its moons look like from five-plus million miles away."
The mission optical camera, JunoCam, imaged Jupiter on June 21, 2016, at a distance of 6.8 million miles (10.9 million kilometers) from the gas giant. In the image, just to the right of center is Jupiter, with its distinctive swirling bands of orange, brown and white. To the left of Jupiter (from right to left) are the planet's four largest moons -- Europa, Io, Callisto and Ganymede. Juno is approaching over Jupiter's north pole, affording the spacecraft a unique perspective on the Jovian system. Previous missions that imaged Jupiter on approach saw the system from much lower latitudes, closer to the planet's equator.
JunoCam is an outreach instrument -- its inclusion in this mission of exploration was to allow the public to come along for the ride with Juno. JunoCam's optics were designed to acquire high-resolution views of Jupiter's poles while the spacecraft is flying much closer to the planet. Juno will be getting closer to the cloud tops of the planet than any mission before it, and the image resolution of the massive gas giant will be the best ever taken by a spacecraft.
All of Juno's instruments, including JunoCam, are scheduled to be turned back on approximately two days after achieving orbit. JunoCam images are expected to be returned from the spacecraft for processing and release to the public starting in late August or early September.
"This image is the start of something great," said Bolton. "In the future we will see Jupiter's polar auroras from a new perspective. We will see details in rolling bands of orange and white clouds like never before, and even the Great Red Spot.
Stunning new images and the highest-resolution maps to date of Jupiter at thermal infrared wavelengths shown above give a glowing view of Juno's target, a week ahead of the NASA mission's arrival at the giant planet. The maps reveal the present-day temperatures, composition and cloud coverage within Jupiter's dynamic atmosphere, and show how giant storms, vortices and wave patterns shape the appearance of the giant planet. The observations will be presented on Monday 27 June at the National Astronomy Meeting in Nottingham by
The high-resolution maps and images were created from observations with the European Southern Observatory's Very Large Telescope (VLT) in Chile, using a newly-upgraded thermal imager called VISIR. The observations were taken between February and June 2016 to characterise Jupiter's atmosphere ahead of Juno's arrival.
"We used a technique called 'lucky imaging', whereby individual sharp frames are extracted from short movies of Jupiter to 'freeze' the turbulent motions of our own atmosphere, to create a stunning new image of Jupiter's cloud layers," explained Leigh Fletcher of the University of Leicester. "At this wavelength, Jupiter's clouds appear in silhouette against the deep internal glows of the planet. Images of this quality will provide the global context for Juno's close-up views of the planet at the same wavelength."
Fletcher and his team have also used the TEXES spectrograph on NASA's Infrared Telescope Facility (IRTF) in Hawaii regularly to map Jupiter's changing appearance. The team made observations at many different wavelengths, optimised for different features and cloud layers in Jupiter's atmosphere, to create the first global spectral maps of Jupiter taken from Earth.
"These maps will help set the scene for what Juno will witness in the coming months. We have seen new weather phenomena that have been active on Jupiter throughout 2016.
These include a widening of one of the brown belts just north of the equator, which has spawned wave patterns throughout the northern hemisphere, both in the cloud layers and high above in the planet's stratosphere," said Dr Fletcher from the University of Leicester's Department of Physics and Astronomy. "Observations at different wavelengths across the infrared spectrum allow us to piece together a three dimensional picture of how energy and material are transported upwards through the atmosphere."
Both sets of observations were made as part of a campaign using several telescopes in Hawaii and Chile, as well as contributions from amateur astronomers around the world, to understand Jupiter's climate ahead of Juno's arrival. The ground-based campaign in support of Juno is led by Dr Glenn Orton of NASA's Jet Propulsion Laboratory. Once in orbit around Jupiter, Juno will skim just 5000 km above Jupiter's clouds once a fortnight - too close to provide global coverage in a single image. The Earth-based observations supplement the suite of advanced instrumentation on the Juno spacecraft, filling in the gaps in Juno's spectral coverage and providing the wider global and temporal context to Juno's close-in observations.
"The combined efforts of an international team of amateur and professional astronomers have provided us with an incredibly rich dataset over the past eight months," said Dr Orton. "Together with the new results from Juno, this dataset will allow researchers to characterise Jupiter's global thermal structure, cloud cover and distribution of gaseous species. We can then hope to answer questions like what drives Jupiter's atmospheric changes, and how the weather we see is connected to processes hidden deep within the planet."
The Daily Galaxy via NASA and ESO
europeanspaceagency posted a photo:
This NASA/ESA Hubble Space Telescope image reveals the iridescent interior of one of the most active galaxies in our local neighbourhood — NGC 1569, a small galaxy located about eleven million light-years away in the constellation of Camelopardalis (The Giraffe). This galaxy is currently a hotbed of vigorous star formation. NGC 1569 is a starburst galaxy, meaning that — as the name suggests — it is bursting at the seams with stars, and is currently producing them at a rate far higher than that observed in most other galaxies. For almost 100 million years, NGC 1569 has pumped out stars over 100 times faster than the Milky Way! As a result, this glittering galaxy is home to super star clusters, three of which are visible in this image — one of the two bright clusters is actually the superposition of two massive clusters. Each containing more than a million stars, these brilliant blue clusters reside within a large cavity of gas carved out by multiple supernovae, the energetic remnants of massive stars. In 2008, Hubble observed the galaxy's cluttered core and sparsely populated outer fringes. By pinpointing individual red giant stars, Hubble's Advanced Camera for Surveys enabled astronomers to calculate a new — and much more precise — estimate for NGC 1569's distance. This revealed that the galaxy is actually one and a half times further away than previously thought, and a member of the IC 342 galaxy group. Astronomers suspect that the IC 342 cosmic congregation is responsible for the star-forming frenzy observed in NGC 1569. Gravitational interactions between this galactic group are believed to be compressing the gas within NGC 1569. As it is compressed, the gas collapses, heats up and forms new stars.
More info here: spacetelescope.org/images/potw1626a/?utm_medium=social&am...
Credit: ESA/Hubble & NASA, Aloisi, Ford
Acknowledgement: Judy Schmidt
Scientists led by Durham University's Institute for Computational Cosmology ran the huge cosmological simulations that can be used to predict the rate at which gravitational waves caused by collisions between the monster black holes might be detected. The amplitude and frequency of these waves could reveal the initial mass of the seeds from which the first black holes grew since they were formed 13 billion years ago and provide further clues about what caused them and where they formed, the researchers said.
The research is being presented today (Monday, June 27, 2016) at the Royal Astronomical Society's National Astronomy Meeting in Nottingham, UK. It was funded by the Science and Technology Facilities Council, the European Research Council and the Belgian Interuniversity Attraction Poles Programme.
The study combined simulations from the EAGLE project - which aims to create a realistic simulation of the known Universe inside a computer - with a model to calculate gravitational wave signals.
Two detections of gravitational waves caused by collisions between supermassive black holes should be possible each year using space-based instruments such as the Evolved Laser Interferometer Space Antenna (eLISA) detector (image below) that is due to launch in 2034, the researchers said.
In February the international LIGO and Virgo collaborations announced that they had detected gravitational waves for the first time using ground-based instruments and in June reported a second detection.
As eLISA will be in space - and will be at least 250,000 times larger than detectors on Earth - it should be able to detect the much lower frequency gravitational waves caused by collisions between supermassive black holes that are up to a million times the mass of our sun.
Current theories suggest that the seeds of these black holes were the result of either the growth and collapse of the first generation of stars in the Universe; collisions between stars in dense stellar clusters; or the direct collapse of extremely massive stars in the early Universe.
As each of these theories predicts different initial masses for the seeds of supermassive black hole seeds, the collisions would produce different gravitational wave signals.
This means that the potential detections by eLISA could help pinpoint the mechanism that helped create supermassive black holes and when in the history of the Universe they formed.
Lead author Jaime Salcido, PhD student in Durham University's Institute for Computational Cosmology, said: "Understanding more about gravitational waves means that we can study the Universe in an entirely different way. These waves are caused by massive collisions between objects with a mass far greater than our sun. By combining the detection of gravitational waves with simulations we could ultimately work out when and how the first seeds of supermassive black holes formed."
Co- author Professor Richard Bower, of Durham University's Institute for Computational Cosmology, added: "Black holes are fundamental to galaxy formation and are thought to sit at the centre of most galaxies, including our very own Milky Way.
Discovering how they came to be where they are is one of the unsolved problems of cosmology and astronomy. Our research has shown how space based detectors will provide new insights into the nature of supermassive black holes."
Gravitational waves were first predicted 100 years ago by Albert Einstein as part of his Theory of General Relativity.The waves are concentric ripples caused by violent events in the Universe that squeeze and stretch the fabric of space time but most are so weak they cannot be detected.
LIGO detected gravitational waves using ground-based instruments, called interferometers, that use laser beams to pick up subtle disturbances caused by the waves. eLISA will work in a similar way, detecting the small changes in distances between three satellites that will orbit the sun in a triangular pattern connected by beams from lasers in each satellite.
In June it was reported that the LISA Pathfinder, the forerunner to eLISA, had successfully demonstrated the technology that opens the door to the development of a large space observatory capable of detecting gravitational waves in space.
The image at the top of the page, shows gas and stars in a slice of the EAGLE simulations at the present day. The intensity shows the gas density, while the color encodes the gas temperature. Researchers used the EAGLE simulations to predict the rate at which gravitational waves caused by collisions between supermassive black holes might be detected.
The Daily Galaxy via Durham University
Image credit: The EAGLE project/Stuart McAlpine
Land snail (Catinella avara) collected in Rouge National Urban Park, Ontario, Canada, and photographed at the Centre for Biodiversity Genomics (sample ID: BIOUG13756-C08; specimen record: http://www.boldsystems.org/index.php/Public_RecordView?processid=SSROB5543-14; BIN: http://www.boldsystems.org/index.php/Public_BarcodeCluster?clusteruri=BOLD:ACI3602)
After four years of semi-permanent and roving installations, the arts organization New Orleans Airlift is ready to build a permanent town…
the expressive collection of edibles sees three-dimensional, polygon mesh graphics form seemingly studded surfaces of watermelons, pineapples, cherries and grapes
The post neon nectar and studded skin form a sticky species of low-poly fruit appeared first on designboom | architecture & design magazine.
each of the artist's carefully-constructed photographs comprises countless images painstakingly pieced together over the course of several months.
The post catherine nelson's labyrinth landscapes submerge viewers in a fictional flood of flora appeared first on designboom | architecture & design magazine.
303
US one sheet for VOYAGE OF TIME (Terrence Malick, USA, 2016)
Designer: TBD
Poster source: Indiewire
Martin Puryear, “Drawing for Untitled,” 2009, about 2009, compressed charcoal on paper, Courtesy of the artist. © Martin Puryear, Courtesy Matthew Marks Gallery
From the repetition of vaguely familiar human shapes to his copious use of warm-colored woods and matte metals, Martin Puryear's sculptures are known for their high attention to craft and allusions to a common human experience.
Yet rarely has this Washington, D.C. native's art been displayed as a collection and never has it been shown together with the paper-based prints and sketches he still produces as part of his creative process.
Martin Puryear, “Maquette for Bearing Witness,” 1994, pine, Courtesy of the artist. © Martin Puryear, Courtesy Matthew Marks Gallery. (Photography by Jamie Stukenberg, Professional Graphics)
A new exhibition at the Smithsonian American Art Museum (SAAM) changes that dynamic, covering 50 years of the artist's labors for the first time in a way that gives a glimpse into his artistic approach and influences.
The Smithsonian is the final venue of “Martin Puryear: Multiple Dimensions,” an exhibition that opened first at its organizing museum, the Art Institute of Chicago, and then the Morgan Library and Museum in New York.
For SAAM, Karen Lemmey, the museum's curator of sculpture, chose to focus on the importance of Puryear's public art. Several of Puryear's most recent works happen to be public sculptures—“Big Bling” in New York's Madison Square Park, “Memorial to Slavery” commissioned by Brown University, and a monument for the Deichman Library in Oslo. All three, along with his older monument “Bearing Witness” for Federal Triangle, are referenced in the exhibition at SAAM.
Puryear's maquettes, which are small-scale models of a full-sized work, and drawings for “these monumental outdoor sculptures are never just preparatory models. Each one stands alone as a finished artwork while adding to our understanding of his creative process,” Lemmey says. “Seeing these models and drawings together in our exhibition gives us an opportunity to recognize continuities in commissions he completed at different times for sites around the world. His work often invites thought and discourse on important civic concerns, and what better place to do this than through public sculpture?”
Martin Puryear, “Maquette for Big Bling,” 2014, birch, plywood, maple, and 22k gold leaf, Courtesy of the artist. © Martin Puryear, Courtesy Matthew Marks Gallery. (Photograph by Jamie Stukenberg, Professional Graphics)
Puryear may be best known in his hometown of Washington, D.C. for “Bearing Witness,” a 40-foot-tall sculpture made of panels of hammered bronze standing guard outside the Ronald Reagan Building and International Trade Center. The exhibition features maquettes and drawings for several of his major outdoor public sculptures, including “Bearing Witness,” and the artist's new 40-foot-tall “Big Bling,” which debuted May 16 in Madison Square Park in New York City. That colossal work features a large, gold-leaf shackle and is on display throughout 2016.
Another large-scale work featured in the exhibition is “Vessel,” created from curving ship-sized timbers.
Puryear earned his undergraduate degree in fine arts at Catholic University in 1963, then joined the Peace Corps as a volunteer in Sierra Leone from 1964 to 1966. Without a camera in Sierra Leone, Puryear instead produced faithful drawings of villages and their inhabitants, which he sent along with letters home to family.
“For someone who is known for his public monuments, this exhibition is a rare opportunity to see some early drawings from the artist's personal collection made while he was in Sierra Leone, works he created for himself or for his family,” Lemmey says.
After the Peace Corps, Puryear began his training at the Swedish Royal Academy of Art in Stockholm. His works shift to become less of a mirror, and more of a lens through which he projects experiences in a way that evokes his memories and encounters.
“These prints show Puryear's origins before he became a sculptor,” says Joann Moser, who helped bring the exhibition to SAAM before she retired as the museum's senior curator of graphic arts and deputy chief curator. Despite a fire in 1977 that damaged or destroyed many of his early works, the pieces that survive show how some of Puryear's ideas got started.
Martin Puryear, “Bower,” 1980, Sitka spruce, pine, and copper tacks, Smithsonian American Art Museum, © 1980, Martin Puryear, Courtesy Matthew Marks Gallery
“Bower,” a bent-wood object from SAAM's collection on display only in Washington, echoes the shape of a Phrygian cap, a garment that dates from the fourth century B.C. that became popularized as a symbol of liberty during the French and American revolutions and at times was also a symbol adopted by abolitionists. While “Bower” was made in 1980, Puryear revisited the shape again nearly 20 years later, from 2001 to 2003, on three untitled prints, and again in 2012.
Martin Puryear, “Phrygian,” 2012, soft ground etching with spit bite, drypoint and aquatint on paper, laid down on paper (chine collé), Smithsonian American Art Museum. © 2012, Paulson Bott Press
“This exhibition provides an exciting look at the persistence and evolution of ideas in Puryear's work going back to the early 1960s,” Lemmey says. “I am particularly delighted to see ‘Bower,' one of Puryear's acknowledged masterpieces from the museum's collection, situated with works on paper from other collections so we can see how Puryear returned to latticework forms and ideas about shelter across the decades.”
Another form repeated often throughout Puryear's art is a kidney-shaped ellipse, sometimes looking more like a human head and neck, sometimes more like a teardrop. “Bearing Witness” and “Vessel” both recall this shape, as does “Big Bling” and a smaller, all-iron work, “Shackled,” where the shape appears as a negative space.
Martin Puryear, “Vessel,” 19972002, eastern white pine, mesh, and tar, Courtesy of the artist. © Martin Puryear, Courtesy Matthew Marks Gallery
Through the familiarity of the forms and materials he uses, Puryear aims to open up discourse about the meaning of the shapes he uses without dictating any concrete meaning.
“I tend not to tell people what they're looking at when they're in the presence of my work,” Puryear said at the dedication of his Madison Square Park piece. “I trust people's eyes. I trust their imagination. I trust my work to declare itself to the world.”
“Martin Puryear: Multiple Dimensions” is on view through Sept. 5, 2016.
The post New facets of Martin Puryear's inspiration explored in ‘Multiple Dimensions' at American Art appeared first on Smithsonian Insider.
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People want to take their country back. They want to have independence, in a sense. You see it with Europe, all over Europe. You're going to have more... many other cases where they want to take their borders back, they want to take their monetary back, they want to take a lot of things back. They want to be able to have a country again. So I think you're going to have this happen more and more... I think it's happening in the United States.
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New technology is being wheeled out for this year's Tour de France to scan bikes for hidden electric engines.…
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Despite having lost its biggest customer, being forced to invalidate thousands of test results, being placed under investigation by the US government for fraud, facing sanctions, having had a testing facility shut down, and having had its CEO's worth cut from $4.5bn to $0, "nothing's gone wrong with Theranos."…
Sarah-Louise Burns posted a photo:
The Portuguese artist Alexandre Farto, known as Vhils, has destroyed murals in over 50 countries across the world. By carving into walls that have been painted and graffitied over, he uncovers the slabs of color and texture that are already there in order to make massive portraits. “Why shouldn't I carve over those layers, expose the entrails of a building, and reflect on that process?” he says in this short documentary by Marina Watson Pelaez, Marzia Braggion, and Ricardo Vieira da Silva. “I continue to think that the biggest museums we have in the world are the streets.”
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Two weeks after the Orlando shooting, the LGBTQ communities in San Francisco and New York held their annual parades. Tight security and memorials made this year more somber than years' past, as marchers made sure Pulse victims were remembered with signs, photographs, and chants. Barbara Poma, the owner of Pulse, attended the New York City event. “Orlando and the world's gay community are strong and united,” she said. “We will not allow evil to prevail.”
Igor Karče (back and ...) posted a photo:
... taken from the top floor of the new Switch House at Tate Modern. London skyline for free.
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The red panda (Ailurus fulgens), also called lesser panda, is a mammal native to the eastern Himalayas and southwestern China.
[Facebook | 500px]
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Physicists have created simulations that predict the rate at which gravitational waves from the collision of monstrous supermassive black holes may be detected.…
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