the installation invites pedestrians and passersby to observe the trolleybus at its vanishing point, and capture a unique moment in time.
The post liudas parulskis' vanishing trolleybus blends into the urban landscape of vilnius, lithuania appeared first on designboom | architecture & design magazine.
the sculptural milieu of semi-nude sleeping figures includes the likes of taylor swift, kim kardashian, donald trump, george W. bush, rihanna, bill cosby, and west himself.
The post kanye west's ‘famous' nude celebrities exhibit at blum & poe gallery appeared first on designboom | architecture & design magazine.
Icelandic singer brings her 360-degree VR show to London's Somerset House, putting the universe of Vulnicura on display
Few will be surprised to learn that Björk admits she can be something of a control freak when it comes to her musical output.
“When I make my music I am a bit of a tyrant it is my world and people follow my vision,” she says with a giggle. “But with the visuals it's more of a collaboration.”
Related: Björk: Vulnicura review a sucker punch of a breakup album
Related: Björk: 'It's no coincidence that the porn industry has embraced virtual reality'
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Every year, participants in the Burning Man Festival descend on the playa of Nevada's Black Rock Desert to form a temporary city—a self-reliant community populated by performers, artists, free spirits, and more. An estimated 70,000 people from all over the world came to the 30th annual Burning Man to dance, express themselves, and take in the spectacle. Gathered below are some of the sights from this year, photographed once again by Reuters photographer Jim Urquhart.
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View of London from canary wharf
Leafhopper (Erythroneura vulnerata) collected in Thousand Islands National Park, Ontario, Canada, and photographed at the Centre for Biodiversity Genomics (sample ID: BIOUG20537-E04; specimen record: http://www.boldsystems.org/index.php/Public_RecordView?processid=CNTIC3917-15; BIN: http://www.boldsystems.org/index.php/Public_BarcodeCluster?clusteruri=BOLD:ACU6078)
Labrador sulphur (Colias nastes) collected in Churchill, Manitoba, Canada, and photographed at the Centre for Biodiversity Genomics (sample ID: 04HBL003042; specimen record: http://www.boldsystems.org/index.php/Public_RecordView?processid=LCH042-04; BIN: http://www.boldsystems.org/index.php/Public_BarcodeCluster?clusteruri=BOLD:ACE5358)
Scientists have discovered three giant planets in a binary star system composed of stellar ''twins'' that are also effectively siblings of our Sun. One star hosts two planets and the other hosts the third. The system represents the smallest-separation binary in which both stars host planets that has ever been observed. The findings, which may help explain the influence that giant planets like Jupiter have over a solar system's architecture.
New discoveries coming from the study of exoplanetary systems will show us where on the continuum of ordinary to unique our own Solar System's layout falls. So far, planet hunters have revealed populations of planets that are very different from what we see in our Solar System. The most-common exoplanets detected are so-called super-Earths, which are larger than our planet but smaller than Neptune or Uranus. Given current statistics, Jupiter-sized planets seem fairly rare--having been detected only around a small percentage of stars.
This is of interest because Jupiter's gravitational pull was likely a huge influence on our Solar System's architecture during its formative period. So the scarcity of Jupiter-like planets could explain why our home system is different from all the others found to date.
The new discovery from the Carnegie team is the first exoplanet detection made based solely on data from the Planet Finder Spectrograph--developed by Carnegie scientists and mounted on the Magellan Clay Telescopes at Carnegie's Las Campanas Observatory, shown at top of page. PFS is able to find large planets with long-duration orbits or orbits that are very elliptical rather than circular, including the new trio of planets discovered in this `"twin'" star study. This special capability comes from the long observing baseline of PFS; it has been taking observations for six years.
Led by Johanna Teske, the team included a number of Carnegie scientists from both the Department of Terrestrial Magnetism in Washington, DC, and the Carnegie Observatories in Pasadena, CA, as well as Steve Vogt of the University of California Santa Cruz.
"We are trying to figure out if giant planets like Jupiter often have long and, or eccentric orbits," Teske explained. "If this is the case, it would be an important clue to figuring out the process by which our Solar System formed, and might help us understand where habitable planets are likely to be found."
The twin stars studied by the group are called HD 133131A and HD 133131B. The former hosts two moderately eccentric planets, one of which is, at a minimum, about 1 and a half times Jupiter's mass and the other of which is, at a minimum, just over half Jupiter's mass. The latter hosts one moderately eccentric planet with a mass at least 2.5 times Jupiter's.
The two stars themselves are separated by only 360 astronomical units (AU). One AU is the distance between the Earth and the Sun. This is extremely close for twin stars with detected planets orbiting the individual stars. The next-closest binary system that hosts planets is comprised of two stars that are about 1,000 AU apart.
The system is even more unusual because both stars are "metal poor," meaning that most of their mass is hydrogen and helium, as opposed to other elements like iron or oxygen. Most stars that host giant planets are "metal rich." Only six other metal-poor binary star systems with exoplanets have ever been found, making this discovery especially intriguing.
Adding to the intrigue, Teske used very precise analysis to reveal that the stars are not actually identical "twins" as previously thought, but have slightly different chemical compositions, making them more like the stellar equivalent of fraternal twins.
This could indicate that one star swallowed some baby planets early in its life, changing its composition slightly. Alternatively, the gravitational forces of the detected giant planets that remained may have had a strong effect on fully-formed small planets, flinging them in towards the star or out into space.
"The probability of finding a system with all these components was extremely small, so these results will serve as an important benchmark for understanding planet formation, especially in binary systems," Teske explained.
The Daily Galaxy via Carnegie Institution for Science
In a video uploaded to YouTube on August 3rd (below), engineers from the Russian space agency, Roscosmos, proposed an orbiter and lander mission to Ganymede. The video suggests a launch could come in the next decade. Although the commentary is in Russian, the video appears to suggest that Ganymede may be as good a candidate or better for life than Europa.
In March of 2015, NASA's Hubble Space Telescope revealed the best evidence yet for an underground saltwater ocean on Ganymede, Jupiter's largest moon. The subterranean ocean is thought to have more water than all the water on Earth's surface. Identifying liquid water is crucial in the search for habitable worlds beyond Earth and for the search for life, as we know it.
"This discovery marks a significant milestone, highlighting what only Hubble can accomplish," said John Grunsfeld, recently retired assistant administrator of NASA's Science Mission Directorate at NASA Headquarters. "In its 25 years in orbit, Hubble has made many scientific discoveries in our own solar system. A deep ocean under the icy crust of Ganymede opens up further exciting possibilities for life beyond Earth."
Ganymede is the largest moon in our solar system and the only moon with its own magnetic field, shown above. The magnetic field causes aurorae, which are ribbons of glowing, hot electrified gas, in regions circling the north and south poles of the moon. Because Ganymede is close to Jupiter, it is also embedded in Jupiter's magnetic field. When Jupiter's magnetic field changes, the aurorae on Ganymede also change, "rocking" back and forth.
By watching the rocking motion of the two aurorae, scientists were able to determine that a large amount of saltwater exists beneath Ganymede's crust, affecting its magnetic field.
A team of scientists led by Joachim Saur of the University of Cologne in Germany came up with the idea of using Hubble to learn more about the inside of the moon. "I was always brainstorming how we could use a telescope in other ways," said Saur. "Is there a way you could use a telescope to look inside a planetary body? Then I thought, the aurorae! Because aurorae are controlled by the magnetic field, if you observe the aurorae in an appropriate way, you learn something about the magnetic field. If you know the magnetic field, then you know something about the moon's interior."
If a saltwater ocean were present, Jupiter's magnetic field would create a secondary magnetic field in the ocean that would counter Jupiter's field. This "magnetic friction" would suppress the rocking of the aurorae. This ocean fights Jupiter's magnetic field so strongly that it reduces the rocking of the aurorae to 2 degrees, instead of 6 degrees if the ocean were not present. Scientists estimate the ocean is 60 miles (100 kilometers) thick -- 10 times deeper than Earth's oceans -- and is buried under a 95-mile (150-kilometer) crust of mostly ice.
Scientists first suspected an ocean in Ganymede in the 1970s, based on models of the large moon. NASA's Galileo mission measured Ganymede's magnetic field in 2002, providing the first evidence supporting those suspicions. The Galileo spacecraft took brief "snapshot" measurements of the magnetic field in 20-minute intervals, but its observations were too brief to distinctly catch the cyclical rocking of the ocean's secondary magnetic field.
The new observations were done in ultraviolet light and could only be accomplished with a space telescope high above Earth's atmosphere, which blocks most ultraviolet light.
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The Daily Galaxy via Space Telescope Science Institute (STScI)
Image Credit: NASA/ESA and USGS Astrogeology Science Center/Wheaton/NASA/JPL-Caltech
In a newly melted part of Greenland, Australian scientists found the leftover structure from a community of microbes that lived on an ancient seafloor, according to a study in Wednesday's journal Nature. The team have found what they think is the oldest fossil on Earth, a remnant of life from 3.7 billion years ago when Earth's skies were orange and its oceans green.
The discovery shows life may have formed quicker and easier than once thought, about half a billion years after Earth formed . And that may also give hope for life forming elsewhere, such as Mars, said study co-author Martin VanKranendonk of the University of New South Wales and director of the Australian Center for Astrobiology.
"It gives us an idea how our planet evolved and how life gained a foothold," VanKranendonk said.
"It would have been a very different world. It would have had black continents, a green ocean with orange skies," he said. The land was likely black because the cooling lava had no plants, while large amounts of iron made the oceans green. Because the atmosphere had very little oxygen and oxygen is what makes the sky blue, its predominant color would have been orange, he said.
Scientists had thought it would take at least half a billion years for life to form after the molten Earth started to cool a bit, but this shows it could have happened quicker, he said. That's because the newly found fossil is far too complex to have developed soon after the planet's first life forms, he said.
In an outcrop of rocks that used to be covered with ice and snow which melted after an exceptionally warm spring, the Australian team found stromatolites (shown at top of the page surviving in Antarctica), which are intricately layered microscopic layered structures that are often produced by a community of microbes. The stromatolites were about .4 to 1.6 inches high (1 to 4 centimeters).
It "is like the house left behind made by the microbes," VanKranendonk said.
Scientists used the layers of ash from volcanoes and tiny zircon with uranium and lead to date this back 3.7 billion years ago, using a standard dating method, VanKranendonk said.
In this photo provided by Allen Nutman, a rock with the stromatolites, tiny layered structures from 3.7 billion years ago that are remnants from a community of microbes that used to be live there.
The dating seems about right, said Abigail Allwood , a NASA astrobiologist who found the previous oldest fossil, from 3.48 billion years ago, in Australia. But Allwood said she is not completely convinced that what VanKranendonk's team found once was alive. She said the evidence wasn't conclusive enough that it was life and not a geologic quirk.
"It would be nice to have more evidence, but in these rocks that's a lot to ask," Allwood said in an email.
The Daily Galaxy via AP and Nature
Image credit: (Laure Gauthiez/The Australian National University via AP)
"Ten billion years ago, galaxies like our Milky Way were much smaller, but they were forming stars 30 times faster than they are today," said Casey Papovich of Texas A&M University.
An international team of astronomers has charted the rise and fall of galaxies over 90 percent of cosmic history. Their work, which includes some of the most sensitive astronomical measurements made to date, is published by The Astrophysical Journal.
The FourStar Galaxy Evolution Survey (ZFOURGE) has built a multicolored photo album of galaxies as they grow from their faint beginnings into mature and majestic giants. They did so by measuring distances and brightnesses for more than 70,000 galaxies spanning more than 12 billion years of cosmic time, revealing the breadth of galactic diversity.
The team assembled the colorful photo album by using a new set of filters that are sensitive to infrared light and taking images with them with the FourStar camera at Carnegie's 6.5-meter Baade Telescope at our Las Campanas Observatory in Chile. They took the images over a period of 45 nights. The team made a 3-D map by collecting light from over 70,000 galaxies, peering all the way into the distant universe, and by using this light to measure how far these galaxies are from our own Milky Way.
The deep 3-D map also revealed young galaxies that existed as early as 12.5 billion years ago (at less than 10 percent of the current universe age), only a handful of which had previously been found. This should help astronomers better understand the universe's earliest days.
"Perhaps the most surprising result is that galaxies in the young universe appear as diverse as they are today," when the universe is older and much more evolved, said lead author Caroline Straatman, a recent graduate of Leiden University. "The fact that we see young galaxies in the distant universe that have already shut down star formation is remarkable."
But it's not just about distant galaxies; the information gathered by ZFOURGE is also giving the scientists the best-yet view of what our own galaxy was like in its youth.
"ZFOURGE is providing us with a highly complete and reliable census of the evolving galaxy population, and is already helping us to address questions like: How did galaxies grow with time? When did they form their stars and develop into the spectacular structures that we see in the present-day universe?" added Ryan Quadri, also of Texas A&M.
In the study's first images, the team found one of the earliest examples of a galaxy cluster, a so-called "galaxy city" made up of a dense concentration of galaxies, which formed when the universe was only three billion years old, as compared to the nearly 14 billion years it is today.
"The combination of FourStar, the special filters, Magellan, and the conditions at Las Campanas led to the detection of the cluster," said Persson, who built the FourStar instrument at the Carnegie Observatories in Pasadena. "It was in a very well-studied region of the sky--'hiding in plain sight.'"
The paper marks the completion of the ZFOURGE survey and the public release of the dataset, which can be found here: http://zfourge.tamu.edu/DR2016/data.html.
The Daily Galaxy via Carnegie Institution for Science
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This week, the ExoMars mission control team at ESA's centre in Darmstadt, Germany, is training to prepare for next month's arrival at the Red Planet.
Under the watchful eye of Flight Operations Director Michel Denis, the team was taken through a series of realistic simulations that rehearsed both ‘nominal' when everything goes as planned and ‘contingency' the opposite situations.
The team is actually a ‘team of teams' a number of spacecraft operations engineers working under the spacecraft operations manager, supported by diverse specialists from areas including flight dynamics, ground station operations, software and network support, and simulations and training as well as the ExoMars team from ESA's technical centre in the Netherlands.
Teams from the builder of the Mars orbiter, Thales Alenia Space France, and the builder of the Schiaparelli lander, Thales Alenia Space Italy, also took part in the ‘sim'.
Today, ExoMars has completed 80% of the 500 million km trip to Mars, and is 121 566 000 km from Earth. Schiaparelli is set to separate from its parent craft on 16 October and, three days later, will land on Mars as the orbiter fires its main engine to begin circling the planet.
Credit: ESA
"AlphaGo is not only a milestone in the quest of AI, but also an indication that IT now has entered a new era," said Fei-YueWang, at the Chinese Academy of Sciences and secretary general of the Chinese Association of Automation. The computer's win signaled a significant evolution of information technology (IT) and artificial intelligence (AI), according Wang, a professor at the Chinese Academy of Sciences. As the result, IT is no longer information or industrial technology, the New IT is Intelligent Technology. The world has entered the fifth era of intelligent technology.
The world's oldest board game still has a few moves to play. Go, a game of strategy and instinct considered more difficult to master than chess, was created roughly in the same era as the written word. The game is uniquely human - or, it was. Last year, a computer program called AlphaGo defeated an internationally ranked professional player.
In a recent editorial published in the IEEE/CAA Journal of Automatica Sinica, Wang argues that core principles of automation and Al must be rethought as the world navigates an IT paradigm shift.
Wang sketches the progress of robotic and neural machine-human interaction in a timeline of five "control" eras. Automation evolved from the pure mechanics of ancient water clocks and steam engines to the eventual development of electric circuits and transfer functions that gave way to power grids. Digital computers and microprocessors signaled the third shift and paved the way for the fourth - the Internet and the World Wide Web.
In the first four controls, physical and mental realities were approximated as accurately as possible and adjusted through the use of dual control theory. A machine with a set of conditions and a goal could succeed or fail. As the machine acts, it also investigates to learn what action may result in a better future outcome.
Between the physical and mental spaces, another reality in need of double control exists. Augmented, or artificial, reality bridges the gap of actuality and imagination. Pokémon GO is a prime example, as people navigate the physical world to find fictional creatures with only experience as a guide. The parameters and goals shift with each new exposure.
"In Control 5.0...only association revealed by data or experience is available, and causality is a luxury that is no longer attainable with limited resources for uncertainty, diversity, and complexity," Wang said.
Recognition of all three worlds and the dual learning roles of each, according to Wang, will be essential in the fifth era of intelligent technology.
The Daily Galaxy via Chinese Association of Automation
Image credit: Google
If humanity is to survive beyond the lifetime of our Sun, we must leave our Solar System and travel to the stars. If Proxima b is habitable, then it might be an ideal place to move. Perhaps we have just discovered a future home for humanity! But in order to know for sure, we must make many more observations, run many more computer simulations, and, hopefully, send probes to perform the first direct reconnaissance of an exoplanet. The challenges are huge, but Proxima offers a bounty of possibilities that fills me with wonder. Whether habitable or not, Proxima b offers a new glimpse into how planets and life fit into our universe.
The discovery of Proxima b is the biggest exoplanet discovery since the discovery of exoplanets. The planet is not much bigger than Earth and resides in the “habitable zone” of the Sun's nearest stellar neighbor. This planet may represent humanity's best chance to search for life among the stars. But is Proxima b habitable? Is it inhabited? These questions are impossible to answer at this time because we know so little about the planet. However, we can extrapolate from the worlds of our Solar System, as well as employ theoretical models of galactic, stellar, and planetary evolution, to piece together realistic scenarios for Proxima b's history.
The possibilities are varied and depend on phenomena usually studied by scientists in fields that are considered distinct, but an integrated perspective — an astrobiological perspective — can provide a realistic assessment of the possibility that life could have arisen and survived on the closest exoplanet.
As an astrobiologist and astronomer at the University of Washington, and a member of NASA's Virtual Planetary Lab, Roy Barnes has investigated the habitability of planets orbiting red dwarfs for years. His research involves building computer models that simulate how planetary interiors and atmospheres evolve, how stars change with time, and how planetary orbits vary. The discovery of Proxima b has me very excited, but being Earth-sized and in the habitable zone are just the first two requirements for a planet to support life, and the list of requirements is much longer for planets orbiting red dwarfs than for stars like our Sun.
If Proxima b is in fact habitable, meaning it possesses liquid water or even inhabited, meaning life is currently present, then it will have traversed a very different evolutionary path than Earth. This difference is frustrating, in that it will make our initial interpretations challenging, but also exciting, as it offers the chance to learn how Earth-sized planets evolve in our universe. Whether Proxima b is a sterile wasteland or teeming with life, we are now embarking on an unprecedented era of discovery, one that may finally provide an answer that age-old question “Are we alone?”.
What to make of Proxima b? It is at least as massive as Earth, and may be several times more massive. Its “year” is just over 11 days and its orbit may be circular or significantly elongated. Its host star is only 12% as massive as our Sun, 0.1% as bright, and it is known to flare. It may be joined to the stars Alpha Centauri A and B, 15,000 astronomical units (AU) away, by their mutual gravitational attraction.
All three stars contain substantially more heavy elements than our Sun, but we know very little of the composition of Proxima b, or how it formed. The new data point toward the presence of a second planet orbiting in the system with a period near 200 days, but its existence cannot be proven at this time. These are the facts we have and from them we must deduce whether Proxima b supports life.
Proxima b was detected via the radial velocity method, which does not provide a direct measurement of the planet's mass, only a minimum mass. So, the first question we'd like to answer is whether the planet's mass is low enough to be rocky like Earth. If the planet is much larger, it may be more like Neptune with a thick gaseous envelope. While we don't know where the dividing line between rocky and gaseous exoplanets is, models of planet formation and analyses of Kepler planets suggest the transition is between 5 and 10 times the mass of Earth. Only about 5% of allowed orbits place Proxima b's mass above 5 Earth masses, so it is very likely that this planet is in the rocky range.
The next question to ask is if the planet actually formed with water. Water consists of hydrogen and oxygen, the first and third most common elements in the galaxy, so we should expect it to be everywhere. Close to stars, however, where Proxima b resides, water is heated into its vapor phase while planets are forming, and hence it is difficult for planets to capture it. Planets that form at larger distances can gather more water, so if Proxima b formed farther out and moved to its current orbit later, it is more likely to be water-rich.
At this time, we don't know how the planet formed, but three scenarios seem most probable: 1) the planet formed where it is from mostly local material; 2) the planet formed farther out while the gas and dust disk that birthed the planetary system still existed, and forces from that disk drove the planet in to its present orbit; or 3) the planet formed elsewhere and some sort of system-wide instability rearranged the planets and b ultimately arrived in its current orbit.
The first method is how Earth and Venus formed, and so Proxima b may or may not possess significant water if it formed in this way. The second method produces planets that are very water-rich because water is more likely to be in its ice phase farther out in the disk and so the forming planet could easily gather it up. The third method is inconclusive as the planet could have come from an interior orbit and formed without water or farther out and be water-rich. We conclude that it is entirely possible that this planet has water, but we cannot be certain.
Next let's consider the clues from the stars themselves. Computer models of the evolution of our galaxy suggest that stars enriched in heavy elements like Proxima cannot form locally (25,000 light-years from the galactic center) as there just aren't enough heavy elements available. But closer to the galactic center, where star formation has been more vigorous and transpiring for longer, stars like Proxima are possible. Recent work has found that stars in our local solar neighborhood with compositions like Proxima must have formed at least 10,000 light-years closer to the galactic center. It would seem Proxima Centauri has wandered through our galaxy and this history may have played an important role in the evolution of Proxima b.
Computer models of the evolution of the Milky Way galaxy suggest Proxima Centauri has moved outward at least 10,000 light-years from where it formed, shown by the orange circle. The Sun and Earth probably formed near where they orbit today (blue circle), which is where we find Proxima Centauri, too.
The orbit of Proxima around Alpha Centauri A and B, assuming they are gravitationally connected, is large compared to other multiple star systems. In fact, it is so large that A and B's hold on Proxima is weak and the effects of the Milky Way galaxy have shaped Proxima's orbit significantly. The mass of the Milky Way as a whole causes Proxima's orbit to vary both in shape and orientation continuously.
Proxima is also susceptible to gravitational encounters from passing stars that can change its orbit. Recent simulations by Nate Kaib have found that these two effects can often lead to close passages between the stars in a multiple star system that disrupt their planetary systems. The disruption is often powerful enough to eject planets from the system and completely rearrange the orbits of the planets that remain.
New simulations by Russell Deitrick are revealing that this scenario is a real concern for Proxima, too; there is a significant probability that at some point in the past, Proxima swooped in close enough to Alpha Centauri A and B to cause its planetary system to break apart, hurling Proxima b's siblings into deep space. If such a disruption occurred, Proxima b may not have formed where we find it today because its orbit would have been affected by this disruption.
Even if Proxima is not currently bound to Alpha Cen A and B, it appears to be travelling with them, and it is very likely the stars formed from the same cloud of dust and gas. If they formed together, they should have similar compositions and nearly identical ages. Connecting their ages is important because it is very difficult to measure the ages of low mass stars like Proxima Centauri. Astronomers can estimate the age of Alpha Cen A via asteroseismology, the study of “starquakes.”
Stars bigger than the Sun vibrate with large enough amplitudes that brightness fluctuations can be observed, and careful monitoring of the pulsations can reveal a star's age. Recent work by Dr. Michaël Bazot has found that Alpha Cen A is between 3.5 and 6 billion years old. This range is larger than we would like, but Proxima is certainly old enough to support life, and Proxima b might even be about the same age as Earth!
Next we turn to clues from the Proxima Centauri planetary system. The vast majority of the energy used by life on Earth comes from our Sun, and small stars like Proxima can produce energy for trillions of years. The host star is almost as small as stars come, so for a planet to receive as much stellar energy as Earth, Proxima b must be about 25 times closer in than Earth is from the sun. This distance is where the habitable zone lies.
While Proxima is much dimmer than the Sun, it is still a thermonuclear explosion, and, everything else equal, life seems more likely at larger distances. And indeed the close-in orbit does produce numerous obstacles that life on Earth did not have to overcome. These include a long formation time for the star, short and energetic bursts of energy in UV and X-ray light, strong magnetic fields, larger starspots, larger coronal mass ejections, and gravitational tidal effects that cause rotational properties to change and frictional heating in oceans (if they exist) and the rocky interior.
The history of Proxima's brightness evolution has been slow and complicated. Stellar evolution models all predict that for the first one billion years Proxima slowly dimmed to its current brightness, which implies that for about the first quarter of a billion years, Proxima b's surface would have been too hot for Earth-like conditions. As Rodrigo Luger and Barnes recently showed, had our modern Earth been placed in such a situation, it would have become a Venus-like world, in a runaway greenhouse state that can destroy all of the planet's primordial water. This desiccation can occur because the molecular bonds between hydrogen and oxygen in water can be destroyed in the upper atmosphere by radiation from the star, and hydrogen, being the lightest of the elements, can escape the planet's gravity. Without hydrogen, there can be no water, and the planet is not habitable. Escaping or avoiding this early runaway greenhouse is the biggest hurdle for Proxima b's chances for supporting life.
Figure 2: Proxima Centauri's habitable zone has moved inward since it formed, which may mean that planet b lost its water shortly after it formed, when the system was 1—10 million years old. The habitable zone, shown in blue, doesn't arrive at the orbit of planet b until almost 200 million years after it formed. This early brightness may be the biggest obstacle for life to have gained a foothold on Proxima Centauri b.
As the star dims, the water destruction process halts, and so total desiccation is not inevitable. If some water remains, the atmosphere may also contain large quantities of oxygen leftover from the water vapor destruction. While having large amounts of water and oxygen may sound like a good recipe for life, it almost certainly is not. Oxygen is one of the most reactive elements, and its presence in the young atmosphere of Proxima b would likely prevent the development of pre-biotic molecules that require conditions with little oxygen to form. Life on Earth formed when no oxygen was present, and photosynthesis ultimately produced enough oxygen for it to become a major component of our atmosphere. Note that the destruction of only some water leads to the rather surprising possibility that the planet could possess oceans and an oxygen-rich atmosphere, but has been unable to support life!
Another intriguing possibility is that Proxima b started out more like Neptune and the early brightness and flaring eroded away a hydrogen-rich atmosphere to reveal a habitable Proxima below. Such a world was investigated by Rodrigo Luger, Barnes and others, and was found to be a viable pathway to avoid total desiccation. Essentially the hydrogen atmosphere protects the water. If Proxima b formed with about 0.1-1% of its mass in a hydrogen envelope, the planet would lose the hydrogen but not its water, potentially emerging as a habitable world after the star reached its current brightness.
This wide range of possible evolutionary pathways presents a daunting challenge as we imagine using space- and ground-based telescopes to search for life in the atmosphere of Proxima b. Nearly all the components of an atmosphere imprint their presence in a spectrum, so with our knowledge of the possible histories of this planet, we can begin to develop instruments and plan observations that pinpoint the critical differences.
For example, at high enough pressures, oxygen molecules can momentarily bind to each other and produce an observable feature in a spectrum. Crucially, the pressures required to be detectable are large enough to discriminate between a planet with too much oxygen, and one with just the right amount for life. As we learn more about the planet and the system, we can build a library of possible spectra from which to quantitatively determine how likely it is that life exists on Proxima b.
While the early brightness of the host star is the biggest impediment to life, other issues are also important. One of the original concerns for the habitability of planets orbiting red dwarfs was that they would become “tidally locked”, meaning that one hemisphere permanently faces the host star. This state is similar to the rotation of our Moon, in which the same tidal forces that raise waves in our ocean have caused the Moon to show only one face to Earth. Because it is so close to its star, Proxima b may be in this state, depending on the shape of its orbit.
For decades, astronomers were concerned that such a tidally locked planet would be uninhabitable because they believed the atmosphere would freeze and collapse to the surface on the permanently dark side. That possibility is now viewed as very unlikely because winds in the atmosphere will transport energy around the planet and maintain sufficient warmth on the backside to prevent this freeze out. Thus, as far as atmospheric stability is concerned, tidal locking is not a concern for this planet's potential habitability.
Although tidal locking is not very dangerous for life, it is possible for tides to provide large amounts of energy to the planet's atmosphere and interior. This energy is often called “tidal heating” and is a result of the deformation of the planet due to changes in the host star's gravitational force across the planet's diameter. For example, if the planet is on an elliptical orbit, when it is closer to the star, it feels stronger gravity than when it is farther away. This variation will cause the shape of the planet to change, and this deformation can cause friction between layers in the planet's interior, producing heat.
In extreme cases, tidal heating could trigger the onset of a runaway greenhouse like the one that desiccated Venus, independent of starlight. Proxima b is not likely to be in that state, but the tidal heating could still be very strong, causing continual volcanic eruptions as on Jupiter's moon Io, and/or raising enormous ocean waves. Based on the information we have now, we don't know the magnitude of tidal heating, but we must be aware of it and explore its implications.
The host star's short, high energy bursts, called flares, are also a well known concern for surface life on planets of red dwarfs. Flares are eruptions from small regions of the surfaces of stars that cause brief (hours to days) increases in brightness. Crucially, flares emit blasts of positively-charged protons, which have been shown by Antigona Segura and colleagues to deplete ozone layers that can protect life from harmful high-energy UV light.
Proxima flares far more often than our Sun and Proxima b is much closer to Proxima than Earth is to the Sun, so Proxima b is likely to have been subjected to repeated bombardments. If the atmosphere could develop a robust shield to these eruptions, such as a strong magnetic field that then flaring could be unimportant. Alternatively if it exists under just a few meters of water. Therefore, flares should not be considered fatal for life on Proxima b.
The concern over flaring naturally leads to the question of whether the planet actually does have a protective magnetic field like Earth's. For years, many scientists were concerned that such magnetic fields would be unlikely on planets like Proxima b because tidal locking would prevent their formation. The thinking went that magnetic fields are generated by electric currents moving in the planetary core, and the movement of charged particles needed to create these currents was caused by planetary rotation. A slowly rotating world might not transport the charged particles in the core rapidly enough to generate a strong enough magnetic field to repel the flares, and hence planets in the habitable zones of M dwarfs have no atmospheres.
However, more recent research has shown that planetary magnetic fields are actually supported by convection, a process by which hot material at the center of the core rises, cools, and then returns. Rotation helps, but Dr. Peter Driscoll and I recently calculated that convection is more than sufficient to maintain a strong magnetic field for billions of years on a tidally locked and tidally heated planet. Thus, it is entirely possible that Proxima b has a strong magnetic field and can deflect flares.
So is Proxima b habitable? The short answer is “It's complicated.” Our observations are few, and what we do know allow for a dizzying array of possibilities. Did Proxima b move halfway across the galaxy? Did it endure a planetary-system-wide instability that launched its sibling planets into deep space and changed its orbit? How did it cope with the early high luminosity of its host star? What is it made of? Did it start out as a Neptune-like planet and then become Earth-like? Has it been relentlessly bombarded with flares and coronal mass ejections? Is it tidally heated into an Io-like (or worse) state? These questions are central to unlocking Proxima's potential habitability and determining if our nearest galactic neighbor is an inhospitable wasteland, an inhabited planet, or a future home for humanity.
The last point is not as rhetorical as it might seem. Since all life requires an energy source, it stands to reason that, in the long term — by which I mean the loooong term — planets like Proxima b might be the ideal homes for life. Our Sun will burn out in a mere 4 billion years, but Proxima Centauri will burn for 4 trillion more. Moreover, if a “planet c” exists and slightly perturbs b's orbit, tidal heating could supply modest energy to b's interior indefinitely, providing the power to maintain a stable atmosphere.
The Daily Galaxy via PaleRedDot.org
“This galaxy cluster isn't just remarkable for its distance, it's also going through an amazing growth spurt unlike any we've ever seen,” said Tao Wang of the French Alternative Energies and Atomic Energy Commission (CEA) who led the NASA study.
A new record for the most distant galaxy cluster has been set using NASA's Chandra X-ray Observatory and other telescopes. This galaxy cluster may have been caught right after birth, a brief, but important stage of evolution never seen before.
The galaxy cluster is called CL J1001+0220 (CL J1001 for short) and is located about 11.1 billion light years from Earth. The discovery of this object pushes back the formation time of galaxy clusters the largest structures in the Universe held together by gravity by about 700 million years.
The core of CL J1001 contains eleven massive galaxies nine of which are experiencing an impressive baby boom of stars. Specifically, stars are forming in the cluster's core at a rate that is equivalent to over 3,000 Suns forming per year, a remarkably high value for a galaxy cluster, including those that are almost as distant, and therefore as young, as CL J1001.
The diffuse X-ray emission detected by Chandra and ESA's XMM-Newton Observatory comes from a large amount of hot gas, one of the defining features of a true galaxy cluster.
“It appears that we have captured this galaxy cluster at a critical stage just as it has shifted from a loose collection of galaxies into a young, but fully formed galaxy cluster,” said co-author David Elbaz from CEA. Previously, only these loose collections of galaxies, known as protoclusters, had been seen at greater distances than CL J1001.
The results suggest that elliptical galaxies in galaxy clusters like CL J1001 may form their stars during shorter and more violent outbursts than elliptical galaxies that are outside clusters. Also, this discovery suggests that much of the star formation in these galaxies happens after the galaxies fall onto the cluster, not before.
In comparing their results to computer simulations of the formation of clusters performed by other scientists, the team of astronomers found that CL J1001 has an unexpectedly high amount of mass in stars compared to the cluster's total mass. This may show that the build-up of stars is more rapid in distant clusters than simulations imply, or it may show that clusters like CL J1001 are so rare that they are not found in today's largest cosmological simulations.
“We think we're going to learn a lot about the formation of clusters and the galaxies they contain by studying this object,” said co-author Alexis Finoguenov of the University of Helsinki in Finland, “and we're going to be searching hard for other examples.”
The result is based on data from a large group of observatories in space and on the ground including Chandra, NASA's Hubble Space Telescope and Spitzer Space Telescope, ESA's XMM-Newton and Herschel Space Observatory, the NSF's Karl G. Jansky Very Large Array, the Atacama Large Millimeter/submillimeter Array (ALMA) , the Institut de Radioastronomie Millimetrique Northern Extended Millimeter Array (IRAM NOEMA), and ESO's Very Large Telescope.
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The Daily Galaxy via NASA's Chandra X-ray Observatory.
Don't miss this! Join Polygon's Charlie Hall as he mans an expedition to Alpha Centauri in Elite Dangerous, while space expert, Loren Grush, joins him to discuss last week's announcement that astronomers using European Southern Observatory (ESO) telescopes in Chile and other facilities have found clear evidence of a planet orbiting the closest star to Earth, Proxima Centauri may ultimately prove to be a habitable planet could that harbor an advanced technological civilization.
The long-sought world, designated Proxima b, orbits its cool red -dwarf parent star every 11 days and has a temperature suitable for liquid water to exist on its surface. This rocky world is a little more massive than the Earth and is the closest exoplanet to us -- and it may also be the closest possible abode for life outside the Solar System.
Red Dwarfs “may be one instance in which older is better,” said Seth Shostak, senior astronomer and director of California-based SETI. “Older solar systems have had more time to produce intelligent species.”
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I know it's true of every modern phone, but it's especially true of Sony's new pair of Xperia handsets: the camera will be the most important factor in deciding the fortunes of the Xperia XZ and Xperia X Compact. Introduced at IFA 2016 in Berlin today, Sony's Xperia XZ triples down on camera technology with a new laser autofocus, RGBC-IR white balance sensor, and its traditionally strong 23-megapixel imaging sensor. The Japanese company's new flagship even has a dedicated shutter button. And the Xperia X Compact is a smaller, less powerful vessel for that same upgraded camera system.
One of the reasons the camera is going to be so pivotal is that the rest of the specs are not all that impressive: the Xperia XZ has the Snapdragon 820,...
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There's new and detailed data on the impact of genetically modified crops on pesticide use. Those crops replaced insecticides, and, at first, some herbicides. But herbicide use has rebounded.
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In the last 30 years we've really moved into exceptional territory. Maintaining temperatures below the 1.5C guardrail requires significant and very rapid cuts in carbon dioxide emissions or co-ordinated geo-engineering. That is very unlikely. We are not even yet making emissions cuts commensurate with keeping warming below 2C.
Since the planet is our life support system -- we are essentially the crew of a largish spaceship -- interference with its functioning at this level and on this scale is highly significant. If you or I were crew on a smaller spacecraft, it would be unthinkable to interfere with the systems that provide us with air, water, fodder and climate control. But the shift into the Anthropocene tells us that we are playing with fire, a potentially reckless mode of behaviour which we are likely to come to regret unless we get a grip on the situation
Social disruption and economic consequences of such large sea level rise could be devastating. It is not difficult to imagine that conflicts arising from forced migrations and economic collapse might make the planet ungovernable, threatening the very fabric of civilization.
Climate change is real; it is happening right now. It is the most urgent threat facing our entire species, and we need to work collectively together and stop procrastinating.
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By Matthias Fiechter
The Pallas's cat is a small, little known wild cat species living in the steppes and mountains of Central Asia. Through a new research initiative “PICA” (Pallas's Cat International Conservation Alliance) launched earlier this year, conservationists are hoping to better understand this feline. The project is still in its early stages, but it has already produced some outstanding, rare footage of Pallas's cats, including video of wild cubs.
The footage (featured at the top of this post) was taken by a set of remote-sensor research cameras stationed in the Zoolon Mountains, in Mongolia's Gobi Gurvan Saikhan National Park. One sequence, shot during the night, shows three Pallas' cat cubs curiously examining the camera, while another snippet features an adult cat in broad daylight looking for signs of other animals.
First Footage of Pallas's Cat Cubs in This Part of Mongolia?
“This is the first footage of Pallas's cat cubs taken in this part of Mongolia as far as we know and is a valuable discovery from our project partners Snow Leopard Trust”, says David Barclay, Cat Conservation Officer at the Royal Zoological Society of Scotland (RZSS).
The cameras are part of the new international Pallas's cat conservation project, PICA, founded by the RZSS, Nordens Ark, a Swedish breeding center and zoo Nordens Ark, and U.S.-based conservation organization Snow Leopard Trust that aims to gather more information on the Pallas's cat, one of the world's least-studied felines.
“If we're hoping to conserve this mysterious cat, we need to first understand it, and we're hoping this study will bring valuable new insights.” — Emma Nygren, Nordens Ark
“We still don't know much about the Pallas's cat's behavior, or even it's true range,” says Emma Nygren, a conservation biologist at Nordens Ark who coordinates the research project. “If we're hoping to conserve this mysterious cat, we need to first understand it, and we're hoping this study will bring valuable new insights.”
The Snow Leopard Trust, which has been working in this part of Mongolia for more than a decade, is a technical and logistical partner in the project. “We're surveying these mountains for snow leopards anyway. The Pallas's cat shares the same habitat and is equally elusive, so it's a logical extension of our work to also look at them,” says Gustaf Samelius, Assistant Director of Science at the Snow Leopard Trust.
The study, which was made possible by the generous support of Fondation Segré, will continue for at least three years.
Matthias Fiechter is the Communications Manager for the Snow Leopard Trust, a Seattle, Washington-based charity with a mission to conserve the snow leopard and its mountain ecosystem through a balanced approach that considers the needs of local people and the environment.
More about the Pallas's Cat (IUCN Red List assessment and profile)
The Royal Zoological Society of Scotland was founded by visionary lawyer Thomas Gillespie in 1909 ‘to promote, facilitate and encourage the study of zoology and kindred subjects and to foster and develop amongst the people an interest in and knowledge of animal life'. The Society still exists to connect people with nature and safeguard species from extinction. Please visit here for information on all our conservation projects.
Nordens Ark is a Swedish non-profit foundation working to protect endangered species through conservation breeding and reintroduction programs as well as through research, field conservations programs and education. Nordens Ark was founded in 1989 and focus on applied conservation actions in Sweden as well as abroad. The foundation works with a wide range of species from snow leopards and Pallas's cats to Lesser White-fronted Geese and Lemur-leaf frogs.
The Snow Leopard Trust, based in Seattle, Washington, is a world leader in conservation of the endangered snow leopard, conducting pioneering research and partnering with communities as well as authorities in snow leopard habitat to protect the cat. Please go to www.snowleopard.org for more information about our research and conservation programs.
The National Geographic Big Cats Initiative funds research to save snow leopards and other big cats in the wild: Saving Snow Leopards in Upper Mustang, Nepal, by Predator-Proofing Livestock Corrals
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By Sarah Martin and Annie Reisewitz
The Department of Defense is taking action to be an environmental leader at defense facilities across the U.S.
Currently, the DOD, headed by the Defense Logistics Agency, is testing the use of biosynthetic motor oils on their non-tactical vehicle fleets. Several environmentally friendly lubricants companies have supplied bio-based motor oil to the DOD for demonstration projects across the U.S., including at Malmstrom Air Force Base in Montana. With nearly 40% of pollution in waterways coming from used motor oil, this is welcome news to help advance a new technology that need wider acceptance by large motor oil consumers.
Every year 10 billion gallons of liquid petroleum hydrocarbon, in the form of motor oil and other industrial lubricants, are released into the environment due to human activity. The majority of this coming in the form of silent oil spills, leaks from cars, and improper disposal of used oil—all contributing to the degradation of our environment and our water supply.
Almost all of the motor oils on the market today are made from refined petroleum. For years, the use of biosynthetic oils has been promoted as an environmentally friendly alternative but was long thought of as a “wouldn't that be nice” pie-in-the-sky idea that wouldn't work on a large scale in part due to the difficulty of using vegetable oils in high heat conditions like automotive engines. However, recent scientific advancements, including by the U.S. Department of Agriculture, have made this petroleum alternative dream very much a reality.
If the tests by the DOD shows that biosynthetic oils perform just as well, if not better, than the current oil being used, the switch to biosynthetic oils may be made Air Force and possibly DOD wide for use in their fleet of 200,000 vehicles in the future.
Increased availability of bio-based lubricant fluids would provide product source diversity; create additional options for government and commercial users as well as the average consumer; reduce dependence on oil imports; and decrease pollution in rivers and oceans.
Environmental as well as usability performance has become important to consumers and regulators. Today, these motor oils and lubricants made from non-toxic, environmentally friendly plant-based oils can protect us, and our environment and they are comparable to or better than petroleum oil when it comes to performance.
In the past, environmentally friendly lubricants have faced performance questions. But extensive testing has proven that biosynthetic oils not only exceed the most challenging environmental standards but also provide performance benefits not attainable with petroleum-based products alone.
This is just the beginning. Other federal agencies, such as the Department of Homeland Security's Law Enforcement Training School, are to begin testing biosynthetic oil later this year.
This large-scale change by the DOD would have widespread positive implications for our environment. While their testing will continue for the next 12-18 months there are steps that you can take to help reduce your environmental footprint. Ask your mechanic for a bio-based alternative the next time you go in for an oil change. According to the U.S. Environmental Protection Agency, just one gallon of motor oil can contaminate one million gallons of fresh water, so your small changes add up to a better environment.
About the authors:
Annie Reisewitz is a communications and marketing consultant for environmental and green technology initiatives. She manages the Silent Oil Spills public awareness campaign.
Sarah Martin has worked in environmental communications for the past several years. She works on the Silent Oil Spills campaign.
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London's famous houses of parliament and the London Eye as seen from the Thames shore. Today was a magical day in London. Although the sky wasn't orange or pink, it was a subtle blue. Beautiful for pictures.
Francis Aston Scientist of the Day
Francis William Aston, an English chemist turned physicist, was born Sep. 1, 1877.
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Thames
Photographs by Basia Irland
My name, Amstel, is derived from the old Dutch, Aeme-stelle, which means “water area.” In the 13th Century, a small fishing village, Amstelredam, was constructed near my mouth beside a dam. Today we know that town as Amsterdam. As early as the 11th Century, farmers began building dikes to try and keep me from flooding these low lands. In 1936 my mouth was filled in and sealed shut, so that today I end at Muntplein Square, although I remain connected to a body of water called the IJ by flowing underground through pipes. The IJ (an ancient Dutch word for water) used to be a bay, but currently is considered more of a lake. During the Dutch Golden Age in the 1600's Amsterdam was the wealthiest city in the world and one of the most important ports. My extensive system of canals, built during this time, is now on the UNESCO World Heritage List.
Looking along a canal toward the Zuiderke Church, built in 1611 (and once painted by Monet).
I flow south to north through this flat and low-lying city, which is the capital of the Netherlands. Parts of me are below sea level, and some of the land around me was reclaimed from the nearby sea or marshes. Dutch children must learn to swim at an early age and receive diplomas for that effort. Some dive from houseboats and swim in my water, careful to dodge the variety of boats that are found day and night, moving upon my body.
A boy dives into the Amstel River.
All kinds of boats ply the river and canals.
I have a beer named after me! The Amstel Brewery is located along my shore, as are other breweries, and my water is sometimes used in the production of these beers. Renowned artists have painted my portrait including Rembrandt van Rijn (1606-1669), Willim Witsen (1860-1923), and Piet Mondrian (1872-1944).
With the flat terrain, the inconvenience of driving a car, and over 400 kilometers (249 miles) of bike paths in Amsterdam, humans prefer to get around by bicycle. With well over a million bikes, it is no wonder so many two-wheelers are dredged out of my stomach each year.
Amsterdam is located on approximately ninety islands and linked by over 1,400 bridges that cross back and forth. Some of these bridges are especially wonderful at night, when their lights reflect on my dark water. One in particular, the Magere Brug, uses an Old Dutch design called a ‘double swipe'. In earlier times it was opened by hand, but now an electronic mechanism raises its two sections to let boats pass underneath to enter one of the many canals that traverse Amsterdam.
Magere Brug with the full moon.
Any visitor to this city will notice a lot of plastic trash floating on my surface, and there are currently attempts to clean up my 100 kilometers (60 miles) of canals. One such venture, Plastic Whale, is a company that fishes plastic bottles and other debris from my water and transforms the trash into material to make a boat that will be used to fish for more plastic. Boat Number Seven is constructed from over seven thousand plastic bottles that might otherwise have found their way out to sea.
Someone else who recycles trash from the canals is my dear friend, the meerkoet. These waterfowl use floating debris to create their unkempt nests, which are seen everywhere wedged amongst the houseboats. The meerkoet live on my surface, and enjoy tickling my ribs when they dive down to feed on plants. The monogamous pairs also eat aquatic insects, seeds, grass, and small animals, and they are one of my favorite playmates as I flow through Amsterdam.
A meerkoet and its nest in a boat tire.
A meerkoet nest built from river debris.
Fulbright Scholar, Basia Irland is an author, poet, sculptor, installation artist, and activist who creates global water projects. She is Professor Emerita, Department of Art and Art History, University of New Mexico, where she established the Arts and Ecology Program. Irland works with scholars from diverse disciplines building rainwater harvesting systems; connecting communities and fostering dialogue along the entire length of rivers; filming and producing water documentaries; and creating waterborne disease projects around the world. She lectures and exhibits internationally and is regularly commissioned to do artistic river restoration projects. Check out her work at basiairland.com
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Ampphire Photography 2016.
New London Pride - August 27th 2016.
Analyzing an event by breaking it down into details might seem like a good way to predict the outcome, but social science research suggests that when most of us do it, we make worse predictions.
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Rivers of lava from the volcano Kilauea leave a lava tube at a bench of new land at the Ka`ili`ili sea entry. The steam in the background is right at sea level and is caused by the boiling hot lava meeting the cool ocean water. With each wave, parts of these flows are covered by water, generating a blinding cloud of hot steam. Kilauea is the youngest and southeastern-most volcano on the big island of Hawaii. Topographically Kilauea, which is located on the southernmost flank of Mauna Loa, was thought to be an extension of its giant neighbor. However, research over the past few decades clearly shows that Kilauea has its own magma-plumbing system, extending to the surface from more than 60 kilometers deep in the Earth.
Image credit: ©Tom Pfeiffer
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Tasmanian devils are evolving in response to a highly lethal and contagious form of cancer. A National Science Foundation-funded researcher and an international team of scientists discovered that two regions in the genomes of Australia's iconic marsupials are changing in response to the rapid spread of devil facial tumor disease (DFTD), a nearly 100 percent fatal and transmissible cancer first detected in 1996. The Washington University study suggests some Tasmanian devil populations are evolving genetic resistance to DFTD that could help the species avoid extinction. Additionally, the genomic data will support future medical research exploring how animals evolve rapidly in response to cancer and other pathogens.
Image credit: Menna Jones, University of Tasmania
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That's what 76 percent said in a recent Kaiser Family Foundation survey. Half the respondents also said they'd be uncomfortable traveling to places in Florida where mosquitoes are spreading Zika.
Is being shy a boon or a burden? Should it be fought against? This sparkling cultural history ranges from Jane Austen to Silicon Valley
Joe Moran, like many of us, is shy. He is hopeless at small talk and feels he “should probably wear a badge that says: ‘Please do not expect sparkling conversation'”. Like most shy people, he has a dread of being boring. Thankfully Shrinking Violets, his “field guide” to shyness, exhibits all the sparkle and fluency on the page he might lack when chatting to strangers. Though he touches on his own experience, it's not a memoir, full of shaming revelations (of course it isn't): Moran says he prefers to hide “behind the human shield of people more interestingly and idiosyncratically shy than me”.
So he investigates the fifth Duke of Portland (1800-1879), who was so shy he communicated by posting notes into letter boxes inside his house, and asked the workers on his Welbeck Estate “to pass him as if he were a tree”. The duke is notable for spending a chunk of his vast fortune excavating grand, illuminated tunnels beneath his land so that when taking a walk he would never risk a meeting.
In the 80s, cardigan-wearing indie kids embraced the idea of being shy "as a personal and political philosophy"
As Hilary Mantel has said, the condition began to be regarded as "a pathology, not just an inconvenient character trait"
Continue reading...Across Africa, elephant poaching is happening on an industrial scale. Though elephant killing is down in Kenya and conservationists are hopeful, the battle to save the largest animals on the Earth is far from being won
In the Samburu National Reserve in northern Kenya, when the fierce heat of the sun has softened into a gentle evening glow, David Daballen and I climb into a jeep to find some elephants.
As we drive through the savannah, Daballen, a conservationist at Save the Elephants, points out family groups and individuals within them. “These are the Butterflies, this group is Storms, here are the Spices,” he says. We have been looking out for Cinnamon, the Spices' matriarch, and suddenly there she is: around 50 years old, huge and tuskless, having been born without any precious ivory. Close to her is Habiba, who was orphaned along with seven siblings when poachers killed their mother in 2011. The orphans were adopted by Cinnamon and the rest of the Spices.
They are a crucial part of the ecosystem, and an iconic species. Can you imagine them no longer existing?
Related: Elephants on the path to extinction - the facts
The rangers could hear the bull making death sounds a loud rumble
It's not like the battle has been won the threat is still very real but it's not on the scale of a few years ago
Elephants have a humbling effect on humans; they make us realise that perhaps we are not the masters of the universe
Related: Why the Guardian is spending a year reporting on the plight of elephants
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A USAF RC-135 Rivet Joint Taxiing at RAF Mildenhall during sunset
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Gorgeous August sunset over the Thames River in London, Ontario.
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New London Pride - August 27th 2016.
Tiny devices sent into the human body for diagnosing and treating diseases run on batteries that may contain toxic materials. Researchers have come up with a safer battery made of natural pigments.
A journalist wanted to tell the stories of two rape victims while protecting their identities. How would he do it?
The FBI and other government security agencies are protecting against cyberattacks that might affect the elections. Hackers tried to gain access to two state voter registration databases this summer.
There's lots of money to be made by turning a video game into a competitive sport, or eSport. There are millions of fans watching video game athletes compete for millions of dollars in prize money.
On Friday, news site Quartz reported that Facebook fired its "news curators" and replaced them with algorithms to compile the news that ends up on Facebook's "Trending" news section. Many users took note when a fake article about Fox News anchor Megyn Kelly was trending.
A trending hashtag on Twitter invites people to personify countries in Africa with various schoolyard archetypes.
Christine's Observations posted a photo:
London's famous houses of parliament and the London Eye as seen from the Thames shore. Today was a magical day in London. Although the sky wasn't orange or pink, it was a subtle blue. Beautiful for pictures.
I didn't realize how pervasive animal exploitation is in our culture.
Veganism is certainly about animals, but it doesn't mean we disrespect our own species along the way.
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How are dogs and wolves similar and different? In a word? Intensity. Take any behavior exhibited by even the most uninhibited dog, then turn it up to thirty-seven and you've got that same behavior in a wolf.
Put another way, dogs dig holes; wolves dig mines. Dogs might rip up your sofa, a wolf will reduce one to feathers,splinters, springs and bits of fabric no more than a one-inch square.
I like to call wolves "raw dogs", "proto-dogs", or "the blueprint". Even with captive bred wolves, they exhibit a broader and more complex range of behavior than what I've experienced with dogs.
Even primitive dog breeds (more "wolf like" dogs) seem to be less adept at solving problems and more inclined to look towards a human for help.
Wolves have around 33% more gray matter than a comparably sized domestic dog. In general, I've witnessed the ability among wolves and high content wolfdogs to solve problems quickly that stymy dogs until they give up.
Aqutaq [my wolf], for example is incredibly adept with a lead line. She fully understands the concept of the line and that it connects us in such a way that we must be on the same side of any tall obstacle. She might be sixteen feet in front of me and on the wrong side of a tree, yet she'll anticipate this issue, and alter course such that she moves to pass the tree on the side that matches mine.
If she becomes entangled while moving through brush, she also understands to retrace the path of the line to unwind it.
Physically, they're very similar, although domestic dogs can eat foods that contain many more carbohydrates as a result of their long-term association with people. Wolves are also only reproductively active once a year, whereas dogs can cycle multiple times. Pound for pound wolves are stronger, have better endurance, have a much greater bite force, and are faster than all but a very select few breeds of dog.
For those that are curious, in my life I've had many different breeds of domestic dogs including:
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I'd already got a couple of shots of the Eye on my walk around, however I realised the light had changed and managed to get back just in time to grab this shot in between the commuters who use the area.
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Tower Bridge in London on a beautiful sunny day
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Big Ben and Houses of parliament at dusk, London, UK
The European Space Agency's Sentinel-1A satellite has been hit by an unidentified flying object while in orbit. Panic not: the probe remains fully operational.…
Bodies of four male sea otters, a federally protected animal whose killing can be punishable with jail time, washed up on beaches over course of eight days
Federal and state officials are investigating the shooting deaths of California sea otters, after the bodies of four male otters were found washed up on beaches near Santa Cruz.
On Monday, the US Fish and Wildlife Service announced a $10,000 reward for information that will lead to the arrest and conviction of the person responsible for fatally shooting three sea otters that were found between 12-19 August.
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The slow decline of hearing in old age is frustrating and alienating. Tyler Trumbo's short documentary, The Sound Inside, follows three elderly people who are taking a lip-reading class to mitigate the effects that hearing loss will have on their lives. The film focuses heavily on sound design and mirrors the silence and muffled noises that have become these characters' realities. “When you can't hear, you don't know what you can't hear,” says one woman. “Without the hearing aid, suddenly I feel like I've dropped in a black hole. All I hear is the noise in my head.”
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i. A minimum population of 5,000
ii. At least 75 percent of the male main working population engaged in non-agricultural pursuits;
iii. A density of population of at least 400 persons per sq. km.
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Cat Wars calls for a massive assault on all free-ranging cats
“From a conservation ecology perspective, the most desirable solution seems clear—remove all free-ranging cats from the landscape by any means necessary.” (Cat Wars, pp. 152-153)
In the process of writing about an on-going war on wolves (please see, for example, “Defenders of Wildlife Supports Killing Wolves: Livestock Win,” “Defenders of Wildlife = Defenders of Livestock? Why Do They Support Killing Wolves in Washington?”, and links therein), I received a new book by bird advocate Dr. Peter Marra, head of the Smithsonian Migratory Bird Center, and writer Chris Santella, called Cat Wars: The Devastating Consequences of a Cuddly Killer.
Along with numerous other people, I've been wondering when killing “in the name of conservation” is going to stop. Some people think it's simply business as usual, and there aren't any workable non-lethal humane alternatives. Killing members of one species to save others of their species, or killing individuals of one species to save individuals of another species, is all well and good and that's the way it is. Some people say they don't like the killing but don't do much to stop it. Our human-dominated world presents numerous frustrating and complicated challenges. We're living in an epoch called the Anthropocene, the “age of humanity.” We're all over the place ― here, there, and everywhere ― and we're the cause for the unprecedented loss of other animals, their homes, and destructive climate change. Actually, we're living in the “rage of inhumanity” because there are far too many of us and we think we're the only show in town.
The move from wolves to cats was dishearteningly seamless. Simply put, the authors of Cat Wars are confirmed bird advocates and activists and foes of all free-ranging cats. To wit, their book calls for a no holds barred, one-sided war on cats, in which the authors conclude, “From a conservation ecology perspective, the most desirable solution seems clear—remove all free-ranging cats from the landscape by any means necessary.” (pp. 152-153; please click here for information on the phrase “by any means necessary”). The authors use the phrase “free-ranging” to refer to feral, outdoor, and community cats.
Many of the topics they consider need to be discussed under the general umbrella centering on the ethics of pet keeping, a topic considered in detail by Psychology Today writer Dr. Jessica Pierce in her book called Run, Spot, Run: The Ethics of Keeping Pets (for an interview with Dr. Pierce please see “Are You Ready to Give Another Animal the Best Life Possible?).
Clearly, the authors are not advocating removing free-ranging cats softly, nor are they advocating any form of euthanasia or mercy killing. Rather, they are advocating outright and unregulated removal “by any means necessary.” When I asked some people what this meant to them, answers ranged from trapping, snaring, poisoning, bludgeoning, and shooting. A number of people feared we would see violence “in the name of science.”
Lest anyone say that these are hysterical responses, one only has to read the very words that Marra and Santella wrote. It's not asking too much from people to write what they mean, and although the authors surely read through their manuscript many times as did reviewers and editors, the phrase “by any means necessary” remains. Cats are vilified and no attention is paid to the emotional lives of these sentient beings.
Even those who endorsed this book can't agree on what it's actually all about. The comments on the back cover range all over the place. For example, Jonathan Franzen calls the book a “compassionate handling of a highly fraught issue,” Ted Williams sees it as a “dispassionate examination of America's free-ranging cat debacle,” whereas Scott Weidensaul claims the authors offer “commonsense solutions to one of the most polarizing issues in avian conservation.” It seems as if they didn't read the same book. In my opinion, this book is thoroughly dispassionate, and I shudder when I think that the call for an all out war on free-ranging cats “by any means necessary” could refer to anything that could possibly be called “compassionate handling” or “commonsense solutions.”
Collateral damage: In addition, the authors don't seem to care much about what's called “collateral damage,” the harming and killing of non-target species. Some of the methods of removing they sanction are incredibly non-selective and it will not only be free-ranging cats who are harmed and killed. I'm sure dogs and as well as other animals, including cats who escape the confines of their home, will be among the slaughtered.
What Cat Wars is all about
The phrase “by any means necessary” is among the most reprehensible statements I've ever seen, and of course, in addition to it being morally repugnant, it is not based on science and it won't work. And, think about the horrific lesson it offers to youngsters. The authors totally ignore the cognitive and emotional lives of cats, and view them as mere disposable objects. I'm glad I'm not their dog, and I'm surely glad I'm not their cat. The suggestion to wage war on free-ranging cats essentially lays out what this sensationalist, fear-mongering, and one-sided book is all about. I suppose one might congratulate the authors for being so transparent about their dismissive attitude.
The description for Cat Wars, published by a prestigious university press, reads:
In 1894, a lighthouse keeper named David Lyall arrived on Stephens Island off New Zealand with a cat named Tibbles. In just over a year, the Stephens Island Wren, a rare bird endemic to the island, was rendered extinct. Mounting scientific evidence confirms what many conservationists have suspected for some time―that in the United States alone, free-ranging cats are killing birds and other animals by the billions. Equally alarming are the little-known but potentially devastating public health consequences of rabies and parasitic Toxoplasma passing from cats to humans at rising rates. Cat Wars tells the story of the threats free-ranging cats pose to biodiversity and public health throughout the world, and sheds new light on the controversies surrounding the management of the explosion of these cat populations.
This compelling book traces the historical and cultural ties between humans and cats from early domestication to the current boom in pet ownership, along the way accessibly explaining the science of extinction, population modeling, and feline diseases. It charts the developments that have led to our present impasse―from Stan Temple's breakthrough studies on cat predation in Wisconsin to cat-eradication programs underway in Australia today. It describes how a small but vocal minority of cat advocates has campaigned successfully for no action in much the same way that special interest groups have stymied attempts to curtail smoking and climate change.
Cat Wars paints a revealing picture of a complex global problem―and proposes solutions that foresee a time when wildlife and humans are no longer vulnerable to the impacts of free-ranging cats.
It's difficult for me to figure out why Princeton University Press would publish this book, not because it calls for a repulsive and outright war on cats, but rather because it lacks the scientific rigor that characterizes numerous other books they've published.
“Cat people” versus “bird people”: A false dichotomy
Early in Cat Wars there is a rather insidious attack on pro-cat people as not caring about the environment and wildlife, which is most likely completely untrue. On page 28 we read, “More and more people are valuing birds and swelling the ranks of bird-watchers. Likewise, there are more cat owners in America now than at any time in history. But far fewer people, it seems, can summon affection for both cats and wildlife—and empathy for those they perceive to be on the ‘other side.' As each side has swelled in numbers, the stage has been set for ‘bird people and ‘cat people' to square off, forgetting, perhaps, that they are all animal lovers in the first place.”
It's hard to imagine that people who favor removing free-ranging cats “by any means necessary” truly love them. When I hear this I always say, “I'm glad they don't love me.” Yet, in another essay, we're told that Dr. Marra claims to like cats.
Along these lines, the third chapter of this book is called “The Rise of Bird Lovers and Cat Lovers: The Perfect Storm.” This chapter is the authors' interpretation (read: “skewed”) of the history of “bird lovers” and “cat lovers.” It concludes by saying that “Many cat advocates will aggressively contest the damage that free-ranging felines inflict upon bird populations. They will likewise deny the diseases that free-ranging cats spread to other mammals and even humans. But their hearsay and denials pale in the light of evidence of cat impacts on islands and the emerging hard science on their impacts on mainlands.” Again, the myth is repeated and developed that cat advocates are misguided, dangerous, and delusional people.
In chapter 4, titled “The Science of Decline,” the authors write, “After forty-five years of bird population decline, it seems obvious that our currently available legal instruments are failing.” (p. 55) It recognizes that human activities are “largely responsible for the declines of bird species” (p. 56) and it is “difficult to identify with any precision the relative impact of a mortality factor, such as the free-ranging cat, to all birds that make these journeys over such large spatial areas and wide expanses of time—and most bird species (>75 percent) in North America migrate!” (my emphasis; p. 57) This comment hardly supports the authors' thesis that cats are responsible for a significant number of bird deaths.
The authors then go on to write about cats as dangerous vectors for disease (Chapter 5 is called “The Zombie Maker: Cats as Agents of Disease”), and they conclude, “Free-ranging cats clearly pose a significant threat to a number of wild animals … [the] solution is to remove them—once and for all—from the landscape.” (p. 94)
They also completely discount the use of Trap-Neuter Return (TNR) programs in their chapter 6 called “Trap-Neuter-Return: A Palatable Solution That Is No Solution At All.” For more on TNR programs please see “Key Scientific Studies on Trap-Neuter-Return” and “Evaluation of the effect of a long-term trap-neuter-return and adoption program on a free-roaming cat population” in which it is concluded, “A comprehensive long-term program of neutering followed by adoption or return to the resident colony can result in reduction of free-roaming cat populations in urban areas.”
Is the public really “blissfully unaware?”
In chapter 8 titled “A Landscape with Fewer Free-Ranging Cats: Better for Cats, Better for Birds, Better for People” we read, “From a conservation ecology perspective, the most desirable solution seems clear—remove all free-ranging cats from the landscape by any means necessary.” (p. 152-153) Any means possible, of course, opens the door for killing cats using incredibly brutal methods. In addition, the public is blamed for being “blissfully unaware” of the significance of the problems at hand (p. 153).
In this chapter we also read, “Perhaps the greatest obstacle to convincing humans to take greater responsibility for their pets and act more responsibly on behalf of their environment and the health of the greater society is the growing ignorance and indifference about the natural world.” (p. 166) This is a most insulting charge for which these authors offer absolutely no scientific support at all. It's just more blaming a public that is supposedly “blissfully unaware.”
Here are a few more snippets:
“It is abundantly clear that free-ranging cats are not the primary threat to the future of birds and other wildlife. Habitat destruction, climate change, and pollution all come to bear on the well-being of wildlife populations; if we as a society hope to maintain these species for future generations, we need to act on all fronts to stem the tide. In the same light, we must act on many different fronts to reduce the populations of free-ranging cats and reduce their impact on native animal populations, both as predators and as vectors of disease. No one solution will prove a silver bullet; only a multipronged strategy will begin to reduce the number of free-ranging cats in the wild. A landscape with no (or at least fewer) free-ranging cats is the only hope for mitigating the toll these animals take on native wildlife and diminishing the spread of disease from cats to human populations.” (p. 145-146)
“Perhaps the owners did not view the birds and mammals that fall prey to domestic cats as sentient beings but instead as playthings for their beloved companions.” (p. 149)
“There is little question that free-ranging cats—both the unowned and the owned pets allowed to roam freely outside—pose a pending ecological and public-health disaster.” (p. 170)
Note that the authors recognize the victims of cat attacks as sentient beings, but feel it's totally fine to kill other sentient beings such as the cats and other nonhumans who will fall prey to efforts to kill all free-ranging cats.
There will be blood: A conservation problem from hell
In a previous essay called “Thousands of Cormorants to be Killed: There Will be Blood” I wrote about an excellent piece by science writer Warren Cornwall called “There Will Be Blood,” and noted it is a must read for anyone interested in keeping up with current discussions and debates about the supposed need to kill animals of one species to save those of another species. At the beginning of his essay Mr. Cornwall writes, “The pressure to reach for a gun to help save one animal from another is stronger than ever. And it has triggered a conservation problem from hell.” He's right. Mr. Cornwall also notes that the history of conservation is “tinged with blood.” For example, noted conservationists John Audubon and Aldo Leopold were quite comfortable killing members of one species to save members of another species, and so too are many conservationists nowadays.
If some people, even very few, choose to follow Marra and Santella's advice to wage war on all free-ranging cats, there will indeed be blood, and an incredible amount of pain, suffering, and death.
What should the future of conservation look like? When will the killing stop?
Should we kill for conservation? Open discussions and debates about the vexing and daunting question that centers on asking if we should kill for conservation are much-needed as we head into a future where more and more species will become imperiled and endangered because of what we are doing to them and to their dwindling habitats. We choose to destroy their homes and then we choose to destroy them. There is something very wrong, disheartening, and disingenuous about this course of action and the ways in which we decide who lives and who dies.
We're going to have to make difficult choices in the future, and choosing not to kill in the name of conservation is a viable option that is now on the table. Do we really want to continue the bloody history of conservation strategies? Time will tell, but times truly are changing. However, you wouldn't know this from Cat Wars. I suppose teachers could use this book as an example of “conservation gone bad” and how not to solve the problems at hand.
Important lessons from compassionate conservation
While the authors briefly mention the rapidly growing international field of compassionate conservation that can reshape conservation ethics in the Anthropocene, they totally ignore its basic tenets, namely, “First do not harm” and the life of every individual animal matters (please also see “Compassionate Conservation Meets Cecil the Slain Lion,” “Compassionate Conservation: More than “Welfarism Gone Wild”,” and “Compassionate Conservation: A Discussion from the Frontlines With Dr. Marc Bekoff”). By paying careful attention to the ways in which other conflicts have been solved without harming and killing the animals, humane and non-lethal solutions will emerge to the satisfaction of all stakeholders. An excellent place to begin to look for such examples is on the homepage for The Centre for Compassionate Conservation.
Harness anger into positive action: The killing of all free-ranging cats truly is a murderous experiment, is ethically indefensible, and likely won't work. Even if it did work, it's morally repugnant and shouldn't be pursued. All in all, I don't see how Cat Wars will change anyone's mind about cats, because it is so sensationalist, one-sided, and so utterly anti-cat. My brief discussion here is only the tip of the iceberg of what is covered in this misleading and sensationalist book. If you disagree, please harness your anger into positive action.
Killing cats “in the name of science”: Readers and cats beware
On the one hand, really I didn't want to write this essay and surely didn't want to call attention to this unveiled diatribe against cats. On the other hand, I'm sure that with the title it has it will attract a good deal of attention. I hope people who choose to read Cat Wars will do so very carefully. It's sickening and disheartening in far too many places, but that's the price of admission. If you're looking for a fair and balanced account of the situation of hand, this is not the book to read. Even if you don't especially like cats, this book surely isn't “the cat's meow.” Indeed, if taken seriously, this book will lead to the loss of the wide range of vocalizations for which cats are well known as well of the lives of many other hapless and innocent individuals who are caught in the crossfire.
Returning to the authors' stance on all free-ranging cats, please keep in mind that the authors advocate removing cats “by any means necessary” ostensibly “in the name of science.” This is a thoroughly heartless conclusion that will undoubtedly lead to horrific pain, suffering, and death not only for cats, but also for other animals, because some people surely will appeal to science and say something like, “Scientists said it's ok to do this.” It is not.
Marc Bekoff's latest books are Jasper's Story: Saving Moon Bears (with Jill Robinson), Ignoring Nature No More: The Case for Compassionate Conservation, Why Dogs Hump and Bees Get Depressed: The Fascinating Science of Animal Intelligence, Emotions, Friendship, and Conservation, Rewilding Our Hearts: Building Pathways of Compassion and Coexistence, and The Jane Effect: Celebrating Jane Goodall (edited with Dale Peterson). The Animals' Agenda: Freedom, Compassion, and Coexistence in the Human Age (with Jessica Pierce) will be published in early 2017.
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