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Cross-Posted from DeSmogBlog
Image Credit: Twitter
A DeSmog investigation has revealed the possibility that a front group supporting the controversial Dakota Access Pipeline (DAPL) — the Midwest Alliance for Infrastructure Now (MAIN) — may have created fake Twitter profiles, known by some as "sock puppets," to convey a pro-pipeline message over social media. And MAIN may be employing the PR services of the firm DCI Group, which has connections to the Republican Party, in order to do so.
DeSmog tracked down at least 16 different questionable Twitter accounts which used the #NoDAPL hashtag employed by protesters, in order to claim that opposition to the pipeline kills jobs, that those protesting the pipeline at the Standing Rock Sioux Tribe's encampment use violence, and that the pipeline does not pose a risk to water sources or cross over tribal land.
On September 13, people began to suspect these accounts were fake, calling them out on Twitter, and by September 14, most of the accounts no longer existed.
The Dakota Access Pipeline is set to carry oil obtained via hydraulic fracturing ("fracking") from the Bakken Shale basin in North Dakota across the Dakotas, Iowa, and Illinois. Its owner, Energy Transfer Partners (ETP), says it plans to talk to the Obama administration and "reiterate [its] commitment to bring the Dakota Access Pipeline into operation." It will do so despite the administration requesting that the company halt construction "voluntarily — particularly around the contested sacred tribal sites located 20 miles east and west of Lake Oahe and the Missouri River — until further notice."
In his memorandum announcing his company's plans to do so, ETP CEO Kelcy Warren espoused many of the same arguments that were deployed by the Twitter sock puppets, which calls into question whether his company helped spearhead the social media campaign behind the scenes in order to create the appearance of grassroots support, a technique known as "astroturfing."
In that memo, Warren said his company plans to engage more aggressively in the PR sphere.
"It has not been my preference to engage in a media/PR battle," wrote Warren. "However, misinformation has dominated the news, so we will work to communicate with the government and media more clearly in the days to come."
Vicki Granado, a spokesperson for the company, did not respond to a request for comment.
In the meantime, as all stakeholders in the debate await a definitive next move from the Obama administration, protests both on-site and nationwide have continued, with a militarized police presence at the Sacred Stone Camp intensifying. U.S. Sen. Bernie Sanders (I-VT) spoke at a September 13 Washington, DC protest against the pipeline, while U.S. Representatives Raul Grijalva (D-AZ) and Raul Ruiz (D-CA) that same day called for a congressional oversight investigation of the hotly contested permitting issues which have arisen in the ongoing saga over the pipeline's future.
With that backdrop, in came the "sock puppets" for their own September 13 day of action on Twitter — and with MAIN likely pulling the strings.
The sock puppet profiles had names such as Ashley Lovinggood, Garnett Vreeken, Yong Fetner, and Ying Baars, and all of the profile pictures featured women. Besides tweets promoting the Dakota Access Pipeline, what links all of the bogus profiles together is that they all "follow" (similar to "liking" a page on Facebook) the company Hootsuite.
Image Credit: Twitter
Hootsuite serves as a social media platform management tool which allows an administrator for many different social media accounts, such as Facebook and Twitter, to toggle quickly between accounts and send out posts in the form of tweets and other status updates. One of those accounts, that of Angla Dullea, formerly followed MAIN — and like all of the other pages — also followed Hootsuite; that is, until the account became suspended.
Dullea's profile photo bore an identical resemblance to the Twitter profile for Palma Mackerl, another bare-bones Twitter account.
Image Credit: Twitter
Dullea also retweeted a tweet from a group called Standing Rock Fact Checker, which on its website describes itself as a project of MAIN. The website also states it is "dedicated to promoting the truth" and battling "misinformation about the approved — and nearly complete — Dakota Access project." Five other suspicious Twitter profiles also shared Fact Checker tweets.
MAIN members include the South Dakota Petroleum and Propane Marketers Association, North Dakota Petroleum Council, Petroleum Marketers, Convenience Stores of Iowa, and others.
Reverse photo searches on Google revealed that the pictures used for other sock puppet profiles also appeared on a dermatologist website, a mail order bride website, and a hairstyle website featuring a photo of Eva Longoria, as well as images of Chinese model Crystal Wang Xi Ran, singer Keri Hilson, and the late singer Amy Winehouse.
Eva Longoria doppelgänger; Photo Credit: Twitter | Oliver Keyes
The use of political bots and sock puppets is nothing new and in fact, has become normalized by political factions worldwide, explained Norah Abokhodair of the Political Bots research program based at the University of Washington and Oxford University.
"There are many ways in which social bots can disrupt or influence online discourse, such as, spamming, phishing, distributed denial of service attacks (DDoS), or other nefarious activities," Abokhodair explained, pointing to examples such as the Syrian Civil War bots and bots used in Turkey. "They can also be deployed for sophisticated activities like astroturfing, misdirection (botnet that tries to get the audience to attend to other content by spamming the hashtag) and smoke screening (serves to hide or provide cover for or obscure some type of activity)."
MAIN was the only industry group to issue a press release in response to the Obama administration's September 9 announcement halting construction on a portion of the Dakota Access Pipeline. Its press release contained a statement attributed to spokesperson Craig Stevens. Stevens also recently did an interview with KVLY-TV, the NBC and CBS affiliate for Fargo, North Dakota. When on TV, however, he was billed as the "spokesperson for a pipeline sort of group, if you will" by segment host Chris Berg.
Despite the lack of disclosure by KVLY and Berg, it turns out that Craig Stevens actually works as Media Affairs and Crisis Management Lead for DCI Group. His DCI Group contact information is listed for MAIN's profile page on the website PR Newswire.
Image Credit: PR Newswire
DCI is a PR firm tied to the GOP and with roots in creating front groups on behalf of Big Tobacco, spearheading the modern Tea Party movement, and representing oppressive dictatorial regimes such as that of Burma and oil- and gas-soaked Azerbaijan. Stevens formerly worked for the George W. Bush presidential campaign, served as spokesperson for U.S. Secretary of Energy Samuel Bodman for the George W. Bush Administration, and also worked on Mitt Romney's 2012 Republican Party presidential campaign.
Jim Murphy, the political director for Donald Trump's Republican Party presidential campaign, formerly served as President and Managing Partner for DCI Group. Beyond the DCI Group connection, Continental Resources — whose founder and CEO Harold Hamm is one of Donald Trump's top energy advisers and a potential candidate for U.S. Secretary of Energy under a Trump presidency — said in a recent investor statement that a significant chunk of the company's Bakken oil will flow through Dakota Access.
Before DCI Group began working on Standing Rock-related projects for MAIN, it appears the PR firm LS2Group maintained the PR account for Dakota Access. A MAIN press release from November 2015 lists LS2's Kayla Day as the contact person and her LS2 work number is also listed, while metadata for the press release's PDF shows the document was last saved by former LS2 staffer Alex Shaner.
As DeSmog has previously revealed, LS2 also did PR work in support of TransCanada's Keystone XL pipeline. The group Iowa Citizens for Community Improvement published emails from 2014 (obtained via a public records request) showing LS2 also doing advocacy work in support of Dakota Access.
LS2's Day told DeSmog that LS2 still does some work on behalf of MAIN, but declined to comment further on how the work is divvied up between LS2 and DCI Group. Stevens was first listed as a spokesperson for MAIN in a September 6 press release, two days after the now-infamous dog biting incident took place at the protesting Standing Rock Siuox Tribe's Sacred Stone Camp. The Standing Rock Fact Checker website was registered the day before, and it also sent out its first tweet that same day.
Image Credit: WhoIs.net
Stevens declined to comment on who funds MAIN, referring to the membership list and confirming he was brought on in the past couple weeks to do PR work on behalf of the coalition, "as the whole public discussion has increased and been elevated" surrounding the pipeline. He also confirmed he runs the Fact Checker portal.
Asked about whether his firm or MAIN had anything to do with the sock-puppet tweets, Stevens denied he or MAIN had any involvement.
"It's frustrating to me because we're working to be respectful in tone and fact-based and any tactics like these are a distraction for what we're trying to do and that's to bring facts and contexts to this discussion," Stevens said. "I don't know about the tactics themselves and I don't know who or what is behind it, but as someone who's trying to get facts out and trying to be respectful in tone, it was incredibly frustrating that this was going on. As far as I know, and think I know, the MAIN Coalition had nothing to do with them."
However, noted environmental advocate and co-founder of climate group 350.org, Bill McKibben, doubts the authenticity of such claims from PR firms with a record like DCI, saying:
"There's a word for this kind of thing, and that word is: lying. The invention of fake people to make fake arguments perfectly exemplifies the tactics Big Oil has been reduced to. They can't win an argument on the merits, so they've given up trying. Instead, they literally make things up. The contrast with the steadfast straightforwardness of the tribes, and of the climate scientists, couldn't be more stark."
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California Gnatcatcher on Buckwheat at UCI Eco Preserve this morning.
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Guedelon Castle is a project started in 1997 by Michel Guyot and Maryline Martin in the Burgundy region of France. The castle is styled on typical French medieval chateau-fort, modeled on designs from the 13th century, and is being built using techniques and materials available to masons and builders 800 years ago. The Guedelon project has now become a tourist destination, and employs dozens of workers. The castle is due to be completed in 2023.
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Law enforcement agencies, NGOs, and business leaders gathered from across the world in Washington this week to share information and expertise and organize a concerted strategy to combat the global scourge of wildlife trafficking.
The unprecedented collaboration was heralded at the National Geographic Society's headquarters on Tuesday, at an event held against the backdrop of recent news of a catastrophic plunge in the last wild populations of African elephants and other species. The meeting also set the stage for CITES CoP17, a world wildlife conference in Johannesburg at the end of this month that will bring more than a hundred governments together to review the planet's biggest wildlife challenges and opportunities.
Stories From the Front Line: Exploring Global Law Enforcement in the New Age of Wildlife Trafficking — the title of the event hosted by the National Geographic Society and the U.S. Fish and Wildlife Service (USFWS) was attended also by officials and conservation experts from 11 African nations on the frontline of poaching of elephants, rhinos, and other iconic species.
The National Geographic/FWS event coincided with the publication of the October 2016 issue of National Geographic magazine, which features a report on the rhino horn trade and rhino farming in South Africa, written by Bryan Christy, the Society's wildlife crimes investigator.
Human-Wildlife Conflict Likely to Grow
The human population is expected to grow to nine billion people by 2050, one billion more in Africa alone in the next 35 years, said National Geographic Society President and CEO Gary E. Knell, at the opening of the event. “The chances of human-wildlife conflict are going to grow, whether we like it or not. We've got to come up with solutions, whether they're in Yellowstone National Park ecosystems, or whether it's in Gorongosa [National Park in Mozambique], or in Kenya or Cameroon. We have to find ways to find a balance and figure out ways to protect the natural habitats of wildlife, and at the same time protect the human needs for survival, food, housing, education, energy, and for all the things which we deserve in human rights.”
Bryan Christy's work on wildlife crime has been cited as one of ten ways National Geographic is changing the world, Knell said. Christy, head of the Society's Special Investigations Unit (SIU) team and 2014 NG Explorer of the Year, is an award-winning journalist and a true champion for wildlife and wild places, he added. “With dedication, courage and conviction [Christy] has already produced astounding results, exposing the criminals of wildlife trafficking and sharing these stories in print, television, digital media, Facebook. That's how we can make his work amplified. That work has put elephants and the illegal trade in elephants on the priority list of many countries, including our own, and has led to numerous Internet petitions and campaigns to stop the illegal ivory trade.”
Enforcement Is Key — But not Enough
David J. Hayes, Chair of the U.S. Wildlife Trafficking Alliance and Vice Chair of the President's Advisory Council on Wildlife Trafficking, said enforcement was key, both domestically in the U.S. and in Africa. “It is so fantastic that the FWS is training you all together to have an effective force,” he told the dozens of wildlife protection and law enforcement officers at the event. “But enforcement is not enough; we have to reduce the demand. As long as there are tremendous dollars chasing illegal products, it's going to be impossible for you guys to completely win,” he said.
Hayes said there was a need to develop international cooperation and public-private partnerships. “The government can't reduce demand by itself. We need all of civil society to come together. We need all of the big nonprofits in this space to not compete against each other, but to work together. And we need to recruit the corporate sector. We need new voices in this debate. We need companies that are being abused by traffickers, to step up, make sure that their supply chains are not being polluted by trafficked goods, and use their communications channels to deliver a broad message to consumers [to] ‘Watch out, don't buy this stuff. You may be the unwitting purchaser of it.'”
Hayes said the Advisory Council on Wildlife Trafficking went first to National Geographic to form a broad organization, “and with National Geographic, the World Wildlife Fund, the Wildlife Conservation Society, and the African Wildlife Foundation…we brought them under the U.S. Wildlife Trafficking Alliance banner. Then we went to the corporate world and said, we need your help…we're a nongovernmental temporary coalition bringing together the nonprofit community with the corporate community. We looked at leading companies in important sectors that traffickers were using. The e-commerce sector for example.”
Secret Sauce
The broad coalition of companies and NGOs under one umbrella speaks with one voice to help American consumers make better decisions, Hayes said.
But there's a secret sauce in this, he added. “You might say, why are you spending so much time in the U.S. consumer world when we know that the largest demand is coming from Southeast Asia. If we get global big name companies like Google, E-bay, Ralph Lauren, and others taking up this cause, communicating with their customers about the importance of this issue, that's going to affect international commerce, too. We're already seeing it happening. If we can get it done in the U.S., we think it will take fire globally as well.”
“All of society needs to help you do your job,” Hayes told the law enforcement gathering. “And with National Geographic's voice, with the impetus of companies and NGOs working together, we can address this issue and we must.”
Engagement Key to Success
“National Geographic's work gives us inspiration and helps us see what's possible in a world of challenge that often seems impossible,” Daniel M. Ashe, Director of the U.S. Fish and Wildlife Service, told the meeting. “If we are going to solve this crisis, this epidemic of wildlife trafficking, engaging people is the key ingredient in success.”
Photo Ark: A Reminder of What's at Stake
“Things like [the National Geographic project] Photo Ark with its 6,000 images, all of them a reminder of what's at stake,” was an example of engagement, Ashe said. “Iconic creatures like African elephant and black rhino and Sumatran tiger, but also the thousands of less charismatic creatures that form the foundation and the sinews that connect this global ecosystem on which we depend. The decline of all of these species, the great and small, the loved and obscure, is an ominous sign for the health of the planet and the billions of people that it sustains — and there will more people in the future, which reminds us that we need to do more and better.”
As we think about the future of prosecuting this effort, we can't just catch the poachers and the middlemen, Hayes added. “We have to go after the people who are making the money, so that we take wildlife trafficking from a high-profit, low-risk endeavor toward a lower profit, higher risk endeavor.”
Operation Crash
The success of Operation Crash [an ongoing nationwide criminal investigation led by the FWS Office of Law Enforcement, focusing on the illegal trade in rhinoceros horn and elephant ivory in response to international poaching and smuggling syndicates] was a key reason why the FWS was working to position senior agents around the globe to facilitate these efforts, Ashe said. The agency had recently selected a special agent to serve in Libreville, Gabon, joining five other attaches stationed in embassies in China, Thailand, Tanzania, Botswana, and Peru. “Hopefully before the end of the year, we will have attaches placed in three more key embassies around the world, because we've seen the tremendous value that these agents provide in improving our collaboration and information-sharing. They are dramatically expanding the reach and effectiveness of our law enforcement efforts and communication among law enforcement agencies across the globe,” Ashe said.
Long Time Coming
Introducing a panel discussion, Bryan Christy noted that the gathering of an international group of law enforcement officials had been a long time coming.
“Wildlife crime is organized crime…something that funds terrorist organizations operating in central Africa. It is violent…militarized…mechanized. And one of the advantages that it has is that law enforcement is not violent most of the time, not as well-funded, and, from the international perspective, not historically organized.
“You as law enforcement officers have restrictions that criminals don't; you have diplomatic restrictions on the ability cross borders, you have funding limitations, and you are outfitted with outdated technology occasionally. Criminals are not. Organized criminals are not, especially. So what's exciting to me about tonight is that this represents organized crime fighters.”
Christy noted that he had created the National Geographic Special Investigations Unit with specific goals: “To allow me to work on long investigations, give voice to the work that you do, have a platform for law-enforcement, and to profile endangered species and species we don't hear enough about — and then to empower communities on the ground, talk to journalists in developing countries where wildlife exists, and to law enforcement in those places.”
Following the Story No One Else Can Tell
“I tell law enforcement, if you share your story with me I will follow it,” Christy said. “I know you can't follow it…because of funding and so on. We have had great success doing that. And the success comes from sharing that story, sharing the work that you're doing, the work being done in other countries, pulling that together. And the impact can be pretty impressive.”
Panel Discussion
Five panelists joining Christy on the podium were Curtis Brown (Director of the Florida Fish & Wildlife Commission), Julius Kamwendwit Cheptei (Assistant Director, Kenya Wildlife Service Parks and Preserves), Mike Cenci (Deputy Chief, Washington State Department of Fish and Wildlife Law Enforcement Program), Christopher Fominyam Njoh Tangi (Director, Kimbi-Fungom National Park, Cameroon), and Timothy J. Santel (Resident Agent in Charge, Special Investigations Unit, U.S. Fish & Wildlife Service-Office of Law Enforcement).
Highlights of the Discussion
Curtis Brown: “It takes a lot of work, money and patience to allow for conservation work to happen, especially undercover work. It takes a long time for these cases to actually develop. And it costs a lot of money. So we appreciate everyone's support in that endeavor.
At a national association of conservation law enforcement chiefs meeting we will be trying to collaborate better, share information better, have better intelligence. We are going to get together and do a better job of sharing trafficking intelligence and work better together as investigators. Talking across borders is critical. Any time you share data it's always hard, but if you sit down and share information in conversation, that is valuable information.
Julius Kamwendwit Cheptei: Kenya is divided into eight conservation areas. One of those is the area I am responsible for, in the southern part of the country, 31,000 square kilometers, the equivalent of Israel. I have about 600 foot soldiers charged with the responsibility to ensure the survival of elephants, rhinos, and all other species. A big challenge is conflict between wildlife and community, but our primary responsibility is to ensure that wildlife survives.
Mike Cenci: We have 130 very dedicated Fish and Wildlife police officers and a small cadre of detectives that focus on trafficking and crimes related to natural resources. Some of you may be wondering what does this state agency have to do with the trafficking of species, particularly at the international level. Well, as a state, we've experienced our own natural resources being trafficked on a global scale. We're often the source…there's a lot of diversity in the Pacific Northwest…and our resources that are in relative abundance are highly valued worldwide, so we understand what some of these other nations are facing. If we are going to be concerned about our challenges, we have to show a lot of concern for their challenges. We know that wildlife trafficking is global and it requires a global response, and that requires that it be coordinated worldwide.
Chrstopher Fominyam Njoh Tangi: Responsible for the latest national park created in Cameroon (2015). We have a problem of bush meat, and our greatest problem is cross-border poaching from Nigeria. We also have a problem with the small trophy that comes out of our park, the buffalo horn, which is used as a drinking cup in our tradition. One of our greatest ways of handling wildlife crime is working with our local people. We have a lot of wildlife, but we need to do research to know what we have in the park. The park is enclaved, with no roads, so we have to work with the local people.
The wildlife criminals from Nigeria use the local people as their accomplices to get to what they want. We educate the local people to not be accomplices. In our culture, local people may take a little bush meat for their cultural use, but they may not sell it. But they always abuse this, so we have to discipline them. We have to work with them, get their support to track and find Nigerian trans-boundary poachers.
We don't have the technology, manpower, money, but we work with the local population. But what we hear from them is, “What is the alternative, if we don't work with these people who are paying us to show them where to get these animals, what are we going to do?” The challenge is to find partners who can come into these communities and help with alternative livelihoods, so they can have a better life and turn away from these poachers.
We must look at habitat to improve it. If the animals have a place to hide, they will outsmart the poachers by using the camouflage of the forest. Where we have deforested, the animals are exposed and can be shot from a long distance away. The restored forest is not friendly to poachers; more friendly to animals that can hide there. That's the planned aspect of our work…give animals places to hide and better security.
Tim Santel: We kicked off Operation Crash in 2011 with a team of special agents. I can say five years later, I am very proud of the results that our team put together. [Operation Crash is the centerpiece of Bryan Christy's rhino story in the October 2016 issue of National Geographic.] It is an extraordinary case that shows at multiple level the challenges for law enforcement and the impact of the U.S. Government.
John Webb, Member of the Federal Advisory Council on Wildlife Trafficking, and U.S. Department of Justice prosecutor (retired): We need well trained, well prepared investigators, and to be effective across borders requires those same investigators to cooperate among themselves. Two other important players in effective interdiction and enforcement: prosecutors and judges. How do we get that group of dedicated prosecutors that will take our effective investigations and turn them into successful prosecutions? How do we ensure that we have judges that take our cases seriously and are not corrupt? We have a trilogy of players, all of who must be on the same page for us to have effective wildlife crime fighting.
EAST SIDE SOL 2016 from Youth Speak Media Solutions on Vimeo.
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The Thames Barrier spans 520 metres across the River Thames near Woolwich, and it protects 125 square kilometres of central London from flooding caused by tidal surges. It has 10 steel gates that can be raised into position across the River Thames. When raised, the main gates stand as high as a 5-storey building and as wide as the opening of Tower Bridge. Each main gate weighs 3,300 tonnes.
The barrier is closed under storm surge conditions to protect London from flooding from the sea. It may also be closed during periods of high flow over Teddington Weir to reduce the risk of river flooding in some areas of west London including Richmond and Twickenham.
The Thames Barrier will then remain closed over high water until the water level downstream of the Thames Barrier has reduced to the same level as upstream. This is a managed process to provide for different circumstances, and takes about 5 hours. The Thames Barrier is then opened, allowing the water upstream to flow out to sea with the outward-bound tide.
Information taken from gov.uk website.
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I'm heading to San Francisco for DigitalGlobe's WorldView-4 satellite launch from Vandenberg Air Force Base on Friday! Here's a shot from their most advanced satellite currently in orbit, WorldView-3. The satellite was a remarkable 800 miles away over the Pacific Ocean when this Overview of Golden Gate Bridge, the Bay Bridge, and downtown San Francisco was captured. As you may have noticed, DigitalGlobe provides the raw imagery that makes Daily Overview possible, so we're super excited to see their constellation expanding!
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While Facebook, Google, and a few other companies have agreed to cover the costs of egg freezing for employees, the $10,000 to $15,000 cost isn't practical for most people. A new fertility clinic in New York City is promising to cut the cost by focusing solely on egg freezing. They promise a $4,990 “all-inclusive” price (though this does not include the costs of hormone treatments and egg storage, which are a few thousand more). Can specialization and competition actually drive down the price of this procedurewithout compromising safety? And should it? In this episode of If Our Bodies Could Talk, senior editor James Hamblin visits Extend Fertility to learn more about the idea.
Doctors have long thought that cat-scratch fever is no big deal, but an analysis finds that more people are getting sicker from it. Small children are especially at risk, as are people in the South.
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The man who might be president insists that climate change is an elaborate, "very expensive hoax," even possibly a "Chinese" one meant to undermine the American economy. It's "bullshit" and "pseudoscience" (on which, it seems, he's an expert). He's said this sort of thing numerous times, always mockingly, always dismissively. Only recently in his Phoenix speech on immigration, on his love of Mexicans, and on what suckers they'll be when it comes to paying for his future wall, he put it this way: "Only the out-of-touch media elites think the biggest problems facing America... it's not nuclear, and it's not ISIS, it's not Russia, it's not China, it's global warming." Those fools! They know nothing. They don't even know that there's a crucial footnote, a lone exception, to The Donald's climate change position: golf.
Though the heating of the planet via fossil fuels couldn't be more of a fantasy, while saving the coal industry, building pipelines, and reversing anything Barack Obama did in the White House to promote alternative energy systems will be the order of the day, it turns out that climate change does threaten one thing. And it's something crucial to human life as we know it: playing 18 holes on a coastal golf course. For that, protection is obviously in order. This is undoubtedly why the man with no fears about drowning coastal communities has, through his company Trump International Golf Links & Hotel Ireland, applied for permission to build "a coastal protection works to prevent erosion at his seaside golf resort in County Clare," based on... yep... the danger of rising sea levels. We're talking about "200,000 tons of rock distributed along two miles of beach." And if permission is finally granted, the result will surely be a "great wall," a "beautiful wall" that will not let a drop of sea water emigrate onto Irish soil.
One small hint for Mr. Trump, should he become president. From the Oval Office, he might consider granting similar wall-building exemptions to key parts of coastal Florida already experiencing a serious rise in what's called "sunny-day flooding." Such walls would protect crucial coastal properties like Mar-a-Lago, his top-of-the-line private club in Palm Beach, which could otherwise find itself "under at least a foot of water for 210 days a year because of tidal flooding" within three decades. It's that or develop a sport called aquatic golf.
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In a year of record-setting heat on a blistered globe, with fast-warming oceans, fast-melting ice caps, and fast-rising sea levels, ratification of the December 2015 Paris climate summit agreement -- already endorsed by most nations -- should be a complete no-brainer. That it isn't tells you a great deal about our world. Global geopolitics and the possible rightward lurch of many countries (including a potential deal-breaking election in the United States that could put a climate denier in the White House) spell bad news for the fate of the Earth. It's worth exploring how this might come to be.
The delegates to that 2015 climate summit were in general accord about the science of climate change and the need to cap global warming at 1.5 to 2.0 degrees Celsius (or 2.6 to 3.5 degrees Fahrenheit) before a planetary catastrophe ensues. They disagreed, however, about much else. Some key countries were in outright conflict with other states (Russia with Ukraine, for example) or deeply hostile to each other (as with India and Pakistan or the U.S. and Iran). In recognition of such tensions and schisms, the assembled countries crafted a final document that replaced legally binding commitments with the obligation of each signatory state to adopt its own unique plan, or “nationally determined contribution” (NDC), for curbing climate-altering greenhouse gas emissions.
As a result, the fate of the planet rests on the questionable willingness of each of those countries to abide by that obligation, however sour or bellicose its relations with other signatories may be. As it happens, that part of the agreement has already been buffeted by geopolitical headwinds and is likely to face increasing turbulence in the years to come.
That geopolitics will play a decisive role in determining the success or failure of the Paris Agreement has become self-evident in the short time since its promulgation. While some progress has been made toward its formal adoption -- the agreement will enter into force only after no fewer than 55 countries, accounting for at least 55% of global greenhouse gas emissions, have ratified it -- it has also encountered unexpected political hurdles, signaling trouble to come.
On the bright side, in a stunning diplomatic coup, President Obama persuaded Chinese President Xi Jinping to sign the accord with him during a recent meeting of the G-20 group of leading economies in Hangzhou. Together, the two countries are responsible for a striking 40% of global emissions. “Despite our differences on other issues,” Obama noted during the signing ceremony, “we hope our willingness to work together on this issue will inspire further ambition and further action around the world.”
Brazil, the planet's seventh largest emitter, just signed on as well, and a number of states, including Japan and New Zealand, have announced their intention to ratify the agreement soon. Many others are expected to do so before the next major U.N. climate summit in Marrakesh, Morocco, this November.
On the dark side, however, Great Britain's astonishing Brexit vote has complicated the task of ensuring the European Union's approval of the agreement, as European solidarity on the climate issue -- a major factor in the success of the Paris negotiations -- can no longer be assured. “There is a risk that this could kick EU ratification of the Paris Agreement into the long grass,” suggests Jonathan Grant, director of sustainability at PricewaterhouseCoopers.
The Brexit campaign itself was spearheaded by politicians who were also major critics of climate science and strong opponents of efforts to promote a transition from carbon-based fuels to green sources of energy. For example, the chair of the Vote Leave campaign, former Chancellor of the Exchequer Nigel Lawson, is also chairman of the Global Warming Policy Foundation, a think-tank devoted to sabotaging government efforts to speed the transition to green energy. Many other top Leave campaigners, including former Conservative ministers John Redwood and Owen Paterson, were also vigorous climate deniers.
In explaining the strong link between these two camps, analysts at the Economist noted that both oppose British submission to international laws and norms: “Brexiteers dislike EU regulations and know that any effective action to tackle climate change will require some kind of global cooperation: carbon taxes or binding targets on emissions. The latter would be the EU writ large and Britain would have even less say in any global agreement, involving some 200 nations, than in an EU regime involving 28.”
Keep in mind as well that Angela Merkel and François Hollande, the leaders of the other two anchors of the European Union, Germany and France, are both embattled by right-wing anti-immigrant parties likely to be similarly unfriendly to such an agreement. And in what could be the deal-breaker of history, this same strain of thought, combining unbridled nationalism, climate denialism, fierce hostility to immigration, and unwavering support for domestic fossil fuel production, also animates Donald Trump's campaign for the American presidency.
In his first major speech on energy, delivered in May, Trump -- who has called global warming a Chinese hoax -- pledged to “cancel the Paris climate agreement” and scrap the various measures announced by President Obama to ensure U.S. compliance with its provisions. Echoing the views of his Brexit counterparts, he complained that “this agreement gives foreign bureaucrats control over how much energy we use on our land, in our country. No way.” He also vowed to revive construction of the Keystone XL pipeline (which would bring carbon-heavy Canadian tar sands oil to refineries on the U.S. Gulf Coast), to reverse any climate-friendly Obama administration acts, and to promote the coal industry. “Regulations that shut down hundreds of coal-fired power plants and block the construction of new ones -- how stupid is that?” he said, mockingly.
In Europe, ultra-nationalist parties on the right are riding a wave of Islamaphobia, anti-immigrant sentiment, and disgust with the European Union. In France, for instance, former president Nicolas Sarkozy announced his intention to run for that post again, promising even more stringent controls on migrants and Muslims and a greater focus on French “identity.” Even further to the right, the rabidly anti-Muslim Marine Le Pen is also in the race at the head of her National Front Party. Like-minded candidates have already made gains in national elections in Austria and most recently in a state election in Germany that stunned Merkel's ruling party. In each case, they surged by disavowing relatively timid efforts by the European Union to resettle refugees from Syria and other war-torn countries. Although climate change is not a defining issue in these contests as it is in the U.S. and Britain, the growing opposition to anything associated with the EU and its regulatory system poses an obvious threat to future continent-wide efforts to cap greenhouse gas emissions.
Elsewhere in the world, similar strands of thinking are spreading, raising serious questions about the ability of governments to ratify the Paris Agreement or, more importantly, to implement its provisions. Take India, for example.
Prime Minister Narendra Modi of the Hindu nationalist Bharatiya Janata Party (BJP) has indeed voiced support for the Paris accord and promised a vast expansion of solar power. He has also made no secret of his determination to promote economic growth at any cost, including greatly increased reliance on coal-powered electricity. That spells trouble. According to the Energy Information Administration of the U.S. Department of Energy, India is likely to double its coal consumption over the next 25 years, making it the world's second largest coal consumer after China. Combined with an increase in oil and natural gas consumption, such a surge in coal use could result in a tripling of India's carbon dioxide emissions at a time when most countries (including the U.S. and China) are expected to experience a peak or decline in theirs.
Prime Minister Modi is well aware that his devotion to coal has generated resentment among environmentalists in India and elsewhere who seek to slow the growth of carbon emissions. He nonetheless insists that, as a major developing nation, India should enjoy a special right to achieve economic growth in any way it can, even if this means endangering the environment. “The desire to improve one's lot has been the primary driving force behind human progress,” his government affirmed in its emissions-reduction pledge to the Paris climate summit. “Nations that are now striving to fulfill this ‘right to grow' of their teeming millions cannot be made to feel guilty [about] their development agenda as they attempt to fulfill this legitimate aspiration.”
Russia is similarly likely to put domestic economic needs (and the desire to remain a great power, militarily and otherwise) ahead of its global climate obligations. Although President Vladimir Putin attended the Paris summit and assured the gathered nations of Russian compliance with its outcome, he has also made it crystal clear that his country has no intention of giving up its reliance on oil and natural gas exports for a large share of its national income. According to the Energy Information Administration, Russia's government relies on such exports for a staggering 50% of its operating revenue, a share it dare not jeopardize at a time when its economy -- already buffeted by European Union and U.S. sanctions -- is in deep recession. To ensure the continued flow of hydrocarbon income, in fact, Moscow has announced multibillion dollar plans to develop new oil and gas fields in Siberia and the Arctic, even if such efforts fly in the face of commitments to reduce future carbon emissions.
From Reform and Renewal to Rivalry
Such nationalistic exceptionalism could become something of the norm if Donald Trump wins in November, or other nations join those already eager to put the needs of a fossil fuel-based domestic growth agenda ahead of global climate commitments. With that in mind, consider the assessment of future energy trends that the Norwegian energy giant Statoil recently produced. In it is a chilling scenario focused on just this sort of dystopian future.
The second-biggest producer of natural gas in Europe after Russia's Gazprom, Statoil annually issues Energy Perspectives, a report that explores possible future energy trends. Previous editions included scenarios labeled “reform” (predicated on coordinated but gradual international efforts to shift from carbon fuels to green energy technology) and “renewal” (positing a more rapid transition). The 2016 edition, however, added a grim new twist: “rivalry.” It depicts a realistically downbeat future in which international strife and geopolitical competition discourage significant cooperation in the climate field.
According to the document, the new section is “driven” by real-world developments -- by, that is, “a series of political crises, growing protectionism, and a general fragmentation of the state system, resulting in a multipolar world developing in different directions. In this scenario, there is growing disagreement about the rules of the game and a decreasing ability to manage crises in the political, economic, and environmental arenas.”
In such a future, Statoil suggests, the major powers would prove to be far more concerned with satisfying their own economic and energy requirements than pursuing collaborative efforts aimed at slowing the pace of climate change. For many of them, this would mean maximizing the cheapest and most accessible fuel options available -- often domestic supplies of fossil fuels. Under such circumstances, the report suggests, the use of coal would rise, not fall, and its share of global energy consumption would actually increase from 29% to 32%.
In such a world, forget about those “nationally determined contributions” agreed to in Paris and think instead about a planet whose environment will grow ever less friendly to life as we know it. In its rivalry scenario, writes Statoil, “the climate issue has low priority on the regulatory agenda. While local pollution issues are attended to, large-scale international climate agreements are not the chosen way forward. As a consequence, the current NDCs are only partly implemented. Climate finance ambitions are not met, and carbon pricing to stimulate cost-efficient reductions in countries and across national borders are limited.”
Coming from a major fossil fuel company, this vision of how events might play out on an increasingly tumultuous planet makes for peculiar reading: more akin to Eaarth -- Bill McKibben's dystopian portrait of a climate-ravaged world -- than the usual industry-generated visions of future world health and prosperity. And while “rivalry” is only one of several scenarios Statoil's authors considered, they clearly found it unnervingly convincing. Hence, in a briefing on the report, the company's chief economist Eirik Wærness indicated that Great Britain's looming exit from the EU was exactly the sort of event that would fit the proposed model and might multiply in the future.
Climate Change in a World of Geopolitical Exceptionalism
Indeed, the future pace of climate change will be determined as much by geopolitical factors as technological developments in the energy sector. While it is evident that immense progress is being made in bringing down the price of wind and solar power in particular -- far more so than all but a few analysts anticipated until recently -- the political will to turn such developments into meaningful global change and so bring carbon emissions to heel before the planet is unalterably transformed may, as the Statoil authors suggest, be dematerializing before our eyes. If so, make no mistake about it: we will be condemning Earth's future inhabitants, our own children and grandchildren, to unmitigated disaster.
As President Obama's largely unheralded success in Hangzhou indicates, such a fate is not etched in stone. If he could persuade the fiercely nationalistic leader of a country worried about its economic future to join him in signing the climate agreement, more such successes are possible. His ability to achieve such outcomes is, however, diminishing by the week, and few other leaders of his stature and determination appear to be waiting in the wings.
To avoid an Eaarth (as both Bill McKibben and the Statoil authors imagine it) and preserve the welcoming planet in which humanity grew and thrived, climate activists will have to devote at least as much of their energy and attention to the international political arena as to the technology sector. At this point, electing green-minded leaders, stopping climate deniers (or ignorers) from capturing high office, and opposing fossil-fueled ultra-nationalism is the only realistic path to a habitable planet.
Michael T. Klare, a TomDispatch regular, is a professor of peace and world security studies at Hampshire College and the author, most recently, of The Race for What's Left. A documentary movie version of his book Blood and Oil is available from the Media Education Foundation. Follow him on Twitter at @mklare1.
Follow TomDispatch on Twitter and join us on Facebook. Check out the newest Dispatch Book, Nick Turse's Next Time They'll Come to Count the Dead, and Tom Engelhardt's latest book, Shadow Government: Surveillance, Secret Wars, and a Global Security State in a Single-Superpower World.
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U.S. users trying to take part in Samsung's unofficial recall find themselves winding through a network of stores and unclear guidelines. The government has yet to announce a formal recall.
You can nudge your kids' relationship with digital technology in a more healthful direction, but warning: It's going to require parents to change, too.
Uber is deploying a fleet of self-driving cars Wednesday in Pittsburgh. Employees will be in the front seats, but they will try to let technology do the driving. We went for a ride.
Video games are big business with high stakes for pro players. To help perform better, personal trainers are tailoring their services for gamers. Routines including yoga, weight lifting and cardio.
Joannes Jonston Scientist of the Day
Joannes Jonston, a Polish naturalist descended from a noble Scottish family, was born Sep. 15, 1603.
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A team of chemists has developed a method to yield highly detailed, 3-D images of the insides of batteries. The technique, based on magnetic resonance imaging, offers an enhanced approach to monitor the condition of these power sources in real time.
Image credit: Andrew J. Ilott and Alexej Jerschow, Chemistry Department, New York University
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Many kids rely on school for food their families can't afford. Two reports suggest one group is falling through the cracks: teens. Dogged by hunger, teens may try a wide range of strategies to get by.
Flood managers suspect August's big rainstorms and floods in Louisiana are becoming more common there and elsewhere because of climate change. One clue: Much of the damage was beyond the flood plain.
Full Text:
This is a vampire bat, named for its meals of blood. Scientists are discovering new links between vampire bats and rabies. Rabies will likely reach the Pacific Coast of Peru -- where the virus currently does not occur -- within four years. Researchers reported that the vector-borne virus, which is moving at a rate of 10 miles per year, is likely being carried by infected male vampire bats, and could arrive at the Peruvian coast by June 2020. Additional analyses showed that male bats, which leave their colonies upon reaching maturity, are using Andes Mountain corridors to carry the virus westward.
Image credit: D. Streicker
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Long weekends cooped up in a cramped sweaty workplace, grappling with unstable materials, your work critiqued by an harsh and judgemental boss.…
Doñana wetlands in Andalusia is home to thousands of species but has lost most of its natural water due to industry and faces ‘danger' listing by Unesco
A Spanish wetland home to 2,000 species of wildlife including around 6 million migratory birds is on track to join a Unesco world heritage danger list, according to a new report.
Doñana is an Andalusian reserve of sand dunes, shallow streams and lagoons, stretching for 540 square kilometres (209 square miles) where flamingoes feed and wild horses and Iberian lynx still roam.
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Rare fragile tree snail (Samoana fragilis) on dead coconut leaf.
To coincide with its tenth anniversary, this year Tent London and Super Brands London have been brought together under the new umbrella brand, London Design Fair.
It has also taken on an additional 3,500m2 space on the third floor of the Old Truman Brewery in east London, and will continue to run alongside London Design Festival as one of its design destinations.
One of several large trade shows to be found at London Design Festival, what is now London Design Fair will host the work of hundreds of product and furniture designers, with big brands and small outfits displaying side-by-side at the same venue. There are also some special projects and launches to be found…
Kit Miles and Moooi Carpets have designed the entrance to the foyer of the Old Truman Brewery this year, which will feature a colourful 150m2 carpet.
The carpet design is based on the “interplay of shadows and light”, and inspired by both Mediterranean and London architecture, according to the designers.
At 10 at Tent, ten now-established designers will show the pieces they originally debuted at Tent London, alongside their latest collections.
“This is a chance to take a moment and appreciate how far we've all come. Both the designers and the fair itself we've grown up together,' says London Design Fair founder and director, Jimmy MacDonald.
For another of this year's most promising new installations, the fair was invited to propose a project by the trade commission of the Trentino region of Italy. The result is Trentino Collaborations, which matches four British designers with Trentino-based manufacturers to create new retail products.
Max Lamb is working with a quarry company to produce granite furniture, Sebastian Cox is using a weaving technique from Trentino, Lucy Kurrein is designing leather upholstery and Giles Miller is making his first foray into natural stone tiles.
This year, India has been selected to host the first annual guest country pavilion. Co-curated by MacDonald, alongside London-based consultancy Tiipoi's founder, Spandana Gopal, This is India is designed to showcase a “renewed but intimate perspective on established and emerging design practices from India today”, according to the event organisers.
On the lineup are textile designers Leah Singh, Injiri and Safomasi, as well as industrial studio and manufacturers, Taama.
Look out for exhibition designer, Kangan Arora's installation too, featuring more than 500 hand-painted terracotta pots stacked into various colonnades and towers.
100% Norway will be returning to the London Design Fair for its 13th edition, curated by Max Fraser. It will include projects from a number of Norwegian designers, including Anderssen & Voll, Andreas Bergsaker and Vera & Kyte.
Other confirmed countries showing this year are China, Scotland Craft & Design, Swedish Design Pavilion, Nordic Design Collective, Portugal, Galicia and the Crafts Council of Italy.
London Design Fair takes place in the Old Truman Brewery, 91 Brick Lane, E1 6QL from 22-25 September. For more information, head here.
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The Natural History Museum has worked with Google to create an online visitor experience allowing people to virtually walk round galleries and see exhibits.
The new online platform is available at g.co/naturalhistory and uses Google indoor street view to enable virtual visitors to “walk through” galleries such as Hintze Hall, the Treasures gallery, Dinosaurs and others.
The project has been brought to life by the Google Cultural institute, a sub-organisation of Google which has so far created online archival resources for more than 1000 museums worldwide.
Amit Sood, director of the Google Cultural Institute, says: “Technology can be used not only to make museums' treasures accessible to people around the world, but also to create new experiences for museum-goers.”
The National History Museum platform contains nine virtual exhibitions, and more than 300,000 digital specimens such as the first T-Rex fossil ever found, a narwhal's skull and visuals of extinct mammoths.
It also includes an interactive timeline spanning natural history, and more than 80 million living creatures.
The street view uses gigapixel technology which allows for high resolution photography and video, and also incorporates Google Cardboard and YouTube 360 to provide viewers with virtual reality and 360° video experiences.
The platform also has a learning resource for teachers and students: Google Expeditions uses 360° panorama and 3D images to create interactive imagery, with annotations and descriptions for educational use.
The new online exhibition < g.co/naturalhistory > can be viewed for free on the web, and through the new Google Arts & Culture mobile app available on iOS and Android.
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“The London Design Festival has grown so much in its international importance; it is now one of the most important design events globally.
This year I am happy that my own area, south east London is represented with South East Makers club where I'm particularly looking forward to Ben Chatfield's talk on Saturday 24 September.
Tord Boontje, our neighbour on Charlotte Road and also at home in Brockley has organised Electro Craft. Made up of new and existing work, this show is about the craft of electronics and electronics made as craft.”
“19 Greek Street was the highlight of my London Design Festival last year, so I am really looking forward to this year's exhibition. In the midst of what can feel like a tsunami of consumerism, a gallery that champions the role of art and design to create a more ethical and sustainable future is a breath of fresh air.
From 24 September until 1 October 2016, this Soho townhouse will host “a multisensory experience [that] explores our connection with nature, with ourselves and our surroundings.” Events include design, art, books, tea, meditation and talks. I wouldn't miss it for the world.”
“LDF is a brilliant goad to exploring London, in particular seeing familiar spaces in a fresh guise. The one project currently on my list is the RIBA Regent Street Windows where artists, designers and visionaries transform the windows of iconic Regent Street shops.
It's not a part of London I'd regularly visit, but the promise of Design Haus Liberty's elegantly dangling light installations at Kate Spade is more than enough to get me there.
Their beads of light have the curious effect of being so sensual and luxurious that the formal architecture of Regent Street now provokes an erotic response!”
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Bill Burnett and Dave Evans introduced the Designing for Life course to Standford University in the US 15 years ago. Those that enrolled were younger students, mid-career professionals and retirees, who were all taught to “think like a designer.”
The basic idea is to encourage people to design a career and a life that is “meaningful, joyful and fulfilling” to help them reduce anxieties and reach clear goals.
The course has now been translated into a new book…
Choosing Happiness
Designing a career and a life requires not only that you have lots of options and good alternatives; it also requires the ability to make good choices and live into those choices with confidence, which means you accept them and don't second-guess yourself. Regardless of where you've started, what stage of life and career you are in, how great or dire you perceive your circumstances to be, we would bet our last dollar that there is one goal you all have in this life you are designing:
Happiness
Who doesn't want to be happy? We want to be happy, and we want our students to be happy, and we want you to be happy.
In life design, being happy means you choose happiness.
Choosing happiness doesn't mean you should click your heels together three times while wishing to go to your happy place. The secret to happiness in life design isn't making the right choice; it's learning to choose well.
You can do all the work of life design ideating and prototyping and taking action all leading to some really cool alternative life design plans, but this doesn't guarantee you will be happy and get what you want. Maybe you'll end up happy and getting what you want, and maybe you won't. We say “maybe” because being happy and getting what you want are not about future risks and unknowns or whether you picked the right alternatives; it's about how you choose and how you live your choices once they're made.
All of your hard work can be undone by poor choosing. Not so much by making the wrong choice (that's a risk, but, frankly, not a big one, and usually one you can recover from) as by thinking wrongly about your choosing. Adopting a good, healthy, smart life design choosing process is critical to a happy outcome. Many people are using a choosing model that cuts themselves off from their most important insights and actually prevents them from being happy with their choices after they've been made. We see it all the time, and studies agree: many people guarantee an unhappy outcome by how they approach this all-important design step of choosing.
On the flip side, choosing well almost guarantees a happy and life-giving outcome, while setting you up for more options and a better future.
The Life Design Choosing Process
In life design, the choosing process has four steps. First you gather and create some options, then you narrow down your list to your top alternatives, then finally you choose, and then, last but not least, you… agonise over that choice. Agonise over whether you've done the right thing. In fact, we encourage you to spend countless hours, days, months, or even decades agonising.
Just kidding. People can waste years agonising over the choices they've made, but agonising is a time suck. Of course we don't want you to agonise, and that is not the fourth step in the life design choosing process.
The fourth step in the process is to let go of our unnecessary options and move on, embracing our choice fully so that we can get the most from it.
We need to understand each of these choosing steps to appreciate the important difference between good choosing, which results in reliably happy outcomes and more future prospects, and bad choosing, which preconditions us for an unhappy experience.
Designing Your Life: Build a Life That Works for You, by Bill Burnett & Dave Evans is published by Penguin Random House on 15 September and is priced £14.99
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Futurecity, an initiative to regenerate urban spaces through art and culture, has curated an exhibition looking at the use of wit in design and branding.
Created by The Partners, and based on an updated version of Beryl McAlhone and David Stuart's celebrated graphic design book, A Smile in the Mind, the exhibition will explore how wit powers creative thinking among some of the world's biggest brands.
It is set to include original works from designers and artists including Noma Bar, Robert Brownjohn and Dominic Wilcox.
A Smile in the Mind will be go on display at The Gallery at Foyles, 107 Charing Cross Road, WC2H 0DT. For more information, head here.
Industrial designer Sebastian Bergne will be opening the doors of his Battersea studio to the public for this year's festival, showcasing some of his most famous designs from over the last 25 years in the place they were first created.
Highlights include the relaunched ring soap and lamp shade, as well as new products such as the Drop jug and Cubit beer glass.
25 Years of Editions will run Mon-Fri at 2 Ingate Place, SW8 3NS during LDF. For more information, head here.
Independent design magazine, Dirty Furniture and Italy-based The Shit Museum have teamed up to create an event exploring the potential of arguably our most primordial activity: poo.
Toilet Break features two exhibitions, including one called On the Go, featuring a new commission by Lukas Franciszkiewicz of London-Tokyo design studio Takram.
There will also be a series of talks, including one that will discuss whether gender-neutral toilets are the answer.
Toilet Break will take place at the Basement, 1 North Terrace, SW3 2BA from 17-25 September. For more information, head here.
Photography collective Rockarchive is collaborating with Brixton-based photo studio and gallery, Photofusion in an exhibition dedicated to the memory of one of the area's most famous residents: the late David Bowie.
As a visual celebration of Bowie's life and career, visitors can expect prints and images by music photographers including Ray Stevenson, Fernando Aceves, Mark Mawston and Steve Rapport, some of which are being shown in the UK for the first time.
Silhouettes and Shadows is running From 17-25 September at 17a Electric Lane, SW9 8LA. For more information, head here.
Coinciding with the Sir John Soane's Museum's seven-year restoration project, this year's festival will see the Regency kitchens open to the public for the first time
In a nod to the original use of the kitchens by Sir John Soane's servants, Below Stairs will showcase new or recent work from the likes of Edward Barber and Jay Osgerby, Jasper Morrison, Martino Gamper, and Paul Cocksedge in the reinstated space.
Each of the designers has been selected for their association with culinary and domestic design; Barber & Osgerby has designed ranges of tableware, day-to-day objects and a number of dining tables, while Martino Gamper considers himself part-chef, and part-designer.
Below Stairs will run from 13 September 2016 4 March 2017 at the Sir John Soane's Museum, 13 Lincoln's Inn Fields, WC2A 3BP. For more information, head here.
Be sure to check out these other exhibitions as well:
Show 13: Bare Minimum, by Viaduct
Designersblock London 2016, by Designersblock
London Design Festival at the V&A Engineering Season
All photos courtesy of London Design Festival 2016 supported by British Land.
The London Design Festival runs 17 25 September across various venues in London. For more information, head here.
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Online food delivery service Just Eat has rebranded, with the aim of adding “discovery” and “excitement” to the company.
The relaunch includes a new logo, app and marketing campaign, an updated website, and a new Chatbot function that can be used with Facebook Messenger.
The new visual identity aims to add a “burst of colour” to the brand, says Michael Zur-Szpiro, co-founder at venturethree.
It sees the old version of the logo italicised, and the clicking cursor icon has been removed from the centre of the “A” in “Eat”.
The red colour is retained, but used for the logotype itself, rather than the background.
A spectrum of colours has also been added underneath the logo, which will be used across delivery bikes, the website and the app. Delivery scooters will also carry lit-up delivery boxes.
The new Chatbot aims to “bring food discovery to life by engaging with customers to coach and inspire their food choices”, says Venturethree.
The feature will offer customers a selection of different restaurants they haven't previously ordered from, or help them order their regular choice.
An advertising campaign created by studio Karmarama accompanies the rebrand.
The new branding is being applied to online platforms, packaging, marketing material and to delivery staff apparel.
The new brand will be rolled out globally over the next 12 months.
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German poster for LA NOTTE (Michelangelo Antonioni, Italy, 1961)
Artist: Rolf Goetze
Poster source: Kinoart.net
A new restoration of LA NOTTE opens at Film Forum in New York today.
“Adult male western lowland gorilla named ‘Makumba' studied in the Primate Habituation Programme of WWF, eats ripe indoya fruit (“Trichoscypha acuminata”) in the Dzanga Sangha Protected Areas of Central African Republic.” (Photo by Christopher Whittier)
During the course of a year, a western gorilla in the Lossi Forest of Northern Congo stuffs its face with a profusion of fruit, including figs, mulberries, and the sour-sweet monkey fruit. It's a win-win situation for both animal and plant. The gorilla gets the energy from the sugar, and the plant gets its seeds dispersed—either dropped or ahm, dropped.
But there's one fruit you won't catch a western gorilla eating: Pentadiplantra brazzeana, a bean-sized berry that resembles a red plum, nicknamed l'oubli, meaning forgetfulness, because, as the story goes, the fruit tastes so sweet that in seeking it out, children may forget their mothers. So why don't these gorillas ingest what—judging by their sweetness—seem to be sugar-filled energy bombs?
New research suggests an answer: Because of two genetic mutations, both western gorillas and the closely related eastern gorillas don't taste the P. brazzeana fruit as sweet. The research was reported in the American Journal of Physical Anthropology.
It has been known since 1994 that the sweet component of P. brazzeana isn't sugar at all, but rather a sweet-tasting protein known as brazzein. It seems the plant has evolved to entice animals to eat its fruit, which packs the sweetness of a much larger, sugary fruit through only a bit of protein, while the gorillas appear to have evolved to not fall for the trick.
“Pentadiplandra brazzeana,”or oubli fruit.
“From an evolutionary standpoint, if the gorillas were eating a lot of the fruit but not obtaining the caloric benefit from it, it would give them a disadvantage over time because they wouldn't be getting the nutrition that they need. So by not eating it and eating other things, they're benefiting from [the mutations],” says Kristin Saltonstall, a co-author of the study from the Smithsonian Tropical Research Institute in Panama.
The researchers, including co-authors Brenda Bradley from George Washington University and her graduate student Elaine Guevara from GWU and Yale University, happened upon these findings while conducting a survey of variation in taste receptors for 57 primates and other animals. By looking at a particular protein called T1R3 found in taste buds and essential for tasting sweetness, the researchers saw that the T1R3 of many old world monkeys and apes is composed of the same amino acids, the protein's building blocks. These animals also are known to taste brazzein as sweet.
But since mice, who don't taste brazzein as sweet, have been shown in a 2004 study by a team at the Mount Sinai School of Medicine to have two different amino acids in key spots along the protein, Bradley and her team took note when they saw that western gorillas also have two different amino acids in the same spots. Eastern gorillas, who share ancestry with western gorillas 25-30 million years back, have the same swapped-out amino acids as western gorillas.
“You see these multiple mutations in gorillas, and they just happen to be (I'm using air quotes here) at those sites that would prevent them from being deceived. I think this is really interesting,” Bradley says.
Adult male western lowland gorilla ‘Makumba' eats ripe indoya fruit (“Trichoscypha acuminata”) in the Dzanga Sangha Protected Areas of Central African Republic. (Photo by Christopher Whittier)
Paulo Guimarães Jr., a coevolution researcher who was not involved in this study,
is fascinated by this “molecular evidence of potential coevolution,” he writes in an email. He has a few misgivings, though. “I missed some experimental manipulation exploring if and how gorillas avoid brazzein-rich fruits. Also, it is not clear to me why the ‘taster' phenotype was fixed in old world monkeys,” he continues.
Another way to think about the latter point is to ask, why haven't other old world monkeys and apes developed mutations in the same amino acids as eastern and western gorillas have? There certainly has been plenty of time—35 million years—for this to have happened.
“That's a question, perhaps, of historical contingency. Mutation is a random process. So it might be that mutations haven't happened,” Bradley says. Or it could be possible, she continues, that these other species get some benefit from the fruit, and so there wouldn't be strong selection for this particular mutation.
To say for sure, though, that the mutations indicate coevolutionary adaptations in response to brazzein's trickery, more work needs to be done on the natural ecology of flowering plants and their interaction with animal seed dispersers.
“We're not proving absolutely that it's an adaptation—it's really hard to prove that any trait is an adaptation that evolved via natural selection. The best we can do at this stage is say that it's a really interesting coincidence and something worth following up on,” Bradley says.
The post Gorillas Aren't Tricked By a Faux Sugary Fruit Thanks to a Mutation appeared first on Smithsonian Insider.
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NGC 3718, NGC 3729 and other galaxies shown above have been analyzed using machine learning algorithms that can be "taught" to recognize astrophysical similarities. The same technology is now being applied to cancer images, as well. Every day, NASA spacecraft beam down hundreds of petabytes of data, all of which has to be codified, stored and distributed to scientists across the globe. Increasingly, artificial intelligence is helping to "read" this data as well, highlighting similarities between datasets that scientists might miss.
For the past 15 years, the big data techniques pioneered by NASA's Jet Propulsion Laboratory in Pasadena, California, have been revolutionizing biomedical research. On Sept. 6, 2016, JPL and the National Cancer Institute (NCI), part of the National Institutes of Health, renewed a research partnership through 2021, extending the development of data science that originated in space exploration and is now supporting new cancer discoveries.
The NCI-supported Early Detection Research Network (EDRN) is a consortium of biomedical investigators who share anonymized data on cancer biomarkers, chemical or genetic signatures related to specific cancers. Their goal is to pool all their research data into a single, searchable network, with the goal of translating their collective work into techniques for early diagnosis of cancer or cancer risk.
In the time they've worked together, JPL and EDRN's efforts have led to the discovery of six new Food and Drug Administration-approved cancer biomarkers and nine biomarkers approved for use in Clinical Laboratory Improvement Amendments labs. The FDA has approved each of these biomarkers for use in cancer research and diagnosis. These agency-approved biomarkers have been used in more than 1 million patient diagnostic tests worldwide.
"After the founding of EDRN in 2000, the network needed expertise to take data from multiple studies on cancer biomarkers and create a single, searchable network of research findings for scientists," said Sudhir Srivastava, chief of NCI's Cancer Biomarkers Research Group and head of EDRN. JPL had decades of experience doing similar work for NASA, where spacecraft transmit hundreds of petabytes of data to be coded, stored and distributed to scientists across the globe.
Dan Crichton, the head of JPL's Center for Data Science and Technology, a joint initiative with Caltech in Pasadena, California, helped establish a JPL-based informatics center dedicated to supporting EDRN's big data efforts. In the renewed partnership, JPL is expanding its data science efforts to research and applying technologies for additional NCI-funded programs. Those programs include EDRN, the Consortium for Molecular and Cellular Characterization of Screen-Detected Lesions, and the Informatics Technology for Cancer Research initiative.
"From a NASA standpoint, there are significant opportunities to develop new data science capabilities that can support both the mission of exploring space and cancer research using common methodological approaches," Crichton said. "We have a great opportunity to perfect those techniques and grow JPL's data science technologies, while serving our nation.
Crichton said JPL has led the way when it comes to taking data from raw observations to scientific conclusions. One example: JPL often deals with measurements from a variety of sensors -- say, cameras and mass spectrometers. Both can be used to study a star, planet or similar target object. But it takes special software to recognize that readings from very different instruments relate to one another.
There's a similar problem in cancer research, where readings from different biomedical tests or instruments require correlation with one another. For that to happen, data have to be standardized, and algorithms must be "taught" to know what they're looking for.
Since the time of its founding, EDRN's major challenge has been access. Research centers all over the United States had large numbers of biomarker specimens, but each had its own way of labeling, storing and sharing their datasets. Ten sites may have high-quality specimens for study, but if their common data elements -- age of patient, cancer type and other characteristics - aren't listed uniformly, they can't be studied as a whole.
"We didn't know if they were early-stage or late-stage specimens, or if any level of treatment had been tried," Srivastava said. "And JPL told us, 'We do this type of thing all the time! That's how we manage our Planetary Data System.'"
As the network has developed, it has added members from dozens of institutions, including Dartmouth College's Geisel School of Medicine; Harvard Medical School's Massachusetts General Hospital; Stanford's NIST Genome-Scale Measurements Group; University of Texas' MD Anderson Cancer Center; and numerous others.
Christos Patriotis, program director at NCI's Cancer Biomarkers Research Group, said the network's members now include international researchers from the U.K., China, Japan, Australia, Israel and Chile.
"The more we expand, the more data we integrate," Patriotis said. "Instead of being silos, now our partners can integrate their findings. Each system can speak to the others."
As JPL and NCI's collaboration advances, next steps include image recognition technology, such as helping EDRN archive images of cancer specimens. Those images could be analyzed by computer vision, which is currently used to spot similarities in star clusters and other astrophysics research.
In the near future, Crichton said, machine learning algorithms could compare a CT scan with an archive of similar images, searching for early signs of cancer based on a patient's age, ethnic background and other demographics.
"As we develop more automated methods for detecting and classifying features in images, we see great opportunities for enhancing data discovery," Crichton said. "We have examples where algorithms for detection of features in astronomy images have been transferred to biology and vice-versa."
The Daily Galaxy via http://edrn.cancer.gov
Image credit: Catalina Sky Survey, U of Arizona, and Catalina Realtime Transient Survey, Caltech.
NASA Goddard Photo and Video posted a photo:
Dr. Holdren (left), Administrator Bolden (center) and Dr. Michele Gates (right) discuss the ARM mission during a live NASA TV briefing. Behind them is a mockup of robotic capture module for the Asteroid Redirect Mission.
More info: Asteroid Redirect Mission Update On Sept. 14, 2016, NASA provided an update on the Asteroid Redirect Mission (ARM) and how it contributes to the agency's journey to Mars and protection of Earth. The presentation took place in the Robotic Operations Center at NASA's Goddard Space Flight Center in Greenbelt, Maryland. Assistant to the President for Science and Technology Dr. John P. Holdren, NASA Administrator Charles Bolden and NASA's ARM Program Director, Dr. Michele Gates discussed the latest update regarding the mission. They explained the mission's scientific and technological benefits and how ARM will demonstrate technology for defending Earth from potentially hazardous asteroids. The briefing aired live on NASA TV and the agency's website. For more information about ARM go to www.nasa.gov/arm.
Credit: NASA/Goddard/Debbie Mccallum
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NASA Goddard Space Flight Center enables NASA's mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA's accomplishments by contributing compelling scientific knowledge to advance the Agency's mission.
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"Who would have thought that Pluto is a graffiti artist, spray-painting its companion with a reddish stain that covers an area the size of New Mexico?" asked Will Grundy, a New Horizons co-investigator from Lowell Observatory in Flagstaff, Arizona, and lead author of the paper. "Every time we explore, we find surprises. Nature is amazingly inventive in using the basic laws of physics and chemistry to create spectacular landscapes."
In June 2015, when the cameras on NASA's approaching New Horizons spacecraft first spotted the large reddish polar region on Pluto's largest moon, Charon, mission scientists knew two things: they'd never seen anything like it elsewhere in our solar system, and they couldn't wait to get the story behind it.
Over the past year, after analyzing the images and other data that New Horizons has sent back from its historic July 2015 flight through the Pluto system, the scientists think they've solved the mystery. As they detail this week in the international scientific journal Nature, Charon's polar coloring comes from Pluto itself as methane gas that escapes from Pluto's atmosphere and becomes "trapped" by the moon's gravity and freezes to the cold, icy surface at Charon's pole. This is followed by chemical processing by ultraviolet light from the sun that transforms the methane into heavier hydrocarbons and eventually into reddish organic materials called tholins.
NASA's New Horizons spacecraft captured the high-resolution, enhanced color view of Pluto's largest moon, Charon, shown below of the page just before closest approach on July 14, 2015. The image combines blue, red and infrared images taken by the spacecraft's Ralph/Multispectral Visual Imaging Camera (MVIC); the colors are processed to best highlight the variation of surface properties across Charon. Scientists have learned that reddish material in the north (top) polar region informally named Mordor Macula is chemically processed methane that escaped from Pluto's atmosphere onto Charon. Charon is 754 miles (1,214 kilometers) across; this image resolves details as small as 1.8 miles (2.9 kilometers).
"This study solves one of the greatest mysteries we found on Charon, Pluto's giant moon," said Alan Stern, New Horizons principal investigator from the Southwest Research Institute, and a study co-author. "And it opens up the possibility that other small planets in the Kuiper Belt with moons may create similar, or even more extensive 'atmospheric transfer' features on their moons."
The team combined analyses from detailed Charon images obtained by New Horizons with computer models of how ice evolves on Charon's poles. Mission scientists had previously speculated that methane from Pluto's atmosphere was trapped in Charon's north pole and slowly converted into the reddish material, but had no models to support that theory.
The New Horizons team dug into the data to determine whether conditions on the Texas-sized moon (with a diameter of 753 miles or 1,212 kilometers) could allow the capture and processing of methane gas. The models using Pluto and Charon's 248-year orbit around the sun show some extreme weather at Charon's poles, where 100 years of continuous sunlight alternate with another century of continuous darkness. Surface temperatures during these long winters dip to -430 Fahrenheit (-257 Celsius), cold enough to freeze methane gas into a solid.
"The methane molecules bounce around on Charon's surface until they either escape back into space or land on the cold pole, where they freeze solid, forming a thin coating of methane ice that lasts until sunlight comes back in the spring," Grundy said. But while the methane ice quickly sublimates away, the heavier hydrocarbons created from it remain on the surface.
The models also suggested that in Charon's springtime the returning sunlight triggers conversion of the frozen methane back into gas. But while the methane ice quickly sublimates away, the heavier hydrocarbons created from this evaporative process remain on the surface.
Sunlight further irradiates those leftovers into reddish material called tholins that has slowly accumulated on Charon's poles over millions of years. New Horizons' observations of Charon's other pole, currently in winter darkness and seen by New Horizons only by light reflecting from Pluto, or "Pluto-shine" confirmed that the same activity was occurring at both poles.
The Daily Galaxy via NASA
Image credit: NASA/JHUAPL/SwRI; image at top of page, http://www.solstation.com/stars/charon2.jpg
An experiment to explore the aftermath of cosmic dawn, when stars and galaxies first lit up the universe led by the University of California, Berkeley, called HERA, , the Hydrogen Epoch of Reionization Array, 240 radio dishes aimed at the southern sky near Carnarvon, South Africa, will explore the billion-year period after hydrogen gas collapsed into the first stars, perhaps 100 million years after the Big Bang, through the ignition of stars and galaxies throughout the universe. These first brilliant objects flooded the universe with ultraviolet light that split or ionized all the hydrogen atoms between galaxies into protons and electrons to create the universe we see today.
"The first galaxies lit up and started ionizing bubbles of gas around them, and soon these bubbles started percolating and intersecting and making bigger and bigger bubbles," said Aaron Parsons, a UC Berkeley associate professor of astronomy and principal investigator for HERA. "Eventually, they all intersected and you got this über bubble, leaving the universe as we observe it today: Between galaxies the gas is essentially all ionized."
That's the theory, anyway. HERA hopes for the first time to observe this key cosmic milestone and then map the evolution of reionization to about 1 billion years after the Big Bang.
"We have leaned a ton about the cosmology of our universe from studies of the cosmic microwave background, but those experiments are observing just the thin shell of light that was emitted from a bunch of protons and electrons that finally combined into neutral hydrogen 380,000 years after the Big Bang," he said. "We know from these experiments that the universe started out neutral, and we know that it ended ionized, and we are trying to map out how it transitioned between those two."
The 13.8-billion-year cosmic timeline shown above indicates the era shortly after the Big Bang observed by the Planck satellite, the era of the first stars and galaxies observed by HERA and the era of galaxy evolution to be observed by NASA's future James Webb Space Telescope.
"Before the cosmic dawn, the universe glowed from the cosmic microwave background radiation, but there weren't stars lighting up the universe," said David DeBoer, a research astronomer in UC Berkeley's Radio Astronomy Laboratory. "At some point the neutral hydrogen seeded the stars and black holes and galaxies that relit the universe and led to the epoch of reionization."
The HERA array, which could eventually expand to 350 telescopes, consists of radio dishes staring fixedly upwards, measuring radiation originally emitted at a wavelength of 21 centimeters the hyperfine transition in the hydrogen atom that has been red-shifted by a factor of 10 or more since it was emitted some 13 billion years ago. The researchers hope to detect the boundaries between bubbles of ionized hydrogen invisible to HERA and the surrounding neutral or atomic hydrogen.
By tuning the receiver to different wavelengths, they can map the bubble boundaries at different distances or redshifts to visualize the evolution of the bubbles over time.
"HERA can also tell us a lot about how galaxies form," Parsons said. "Galaxies are very complex organisms that feed back on themselves, regulating their own star formation and the gas that falls into them, and we don't really understand how they live, especially at this early time when flowing hydrogen gas ends up as complex structures with spiral arms and black holes in the middle. The epoch of reionization is a bridge between the cosmology that we can theoretically calculate from first principles and the astrophysics we observe today and try to understand."
UC Berkeley's partners in HERA are the University of Washington, UCLA, Arizona State University, the National Radio Astronomical Observatory, the University of Pennsylvania, the Massachusetts Institute of Technology, Brown University, the University of Cambridge in the UK, the Square Kilometer Array in South Africa and the Scuola Normale Superiore in Pisa, Italy.
Other collaborators are the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, the University of KwaZulu Natal, the University of Western Cape and Rhodes University, all in South Africa, and California State Polytechnic University in Pomona.
"Astronomers want to know what happened to the universe after it emerged from its so-called 'dark ages'," said Rich Barvainis, director of the National Science Foundation program that funds HERA. "HERA will help us answer that question, not by studying the primordial stars and galaxies themselves, but rather by studying how these objects changed the nature of intergalactic space."
The key to detecting these percolating bubbles of ionized gas from the epoch of reionization is a receiver that can detect radio signals from neutral hydrogen a million times fainter than nearby radio noise.
"The foreground noise, mostly synchrotron emission from electrons spiraling in magnetic fields in our own galaxy, is about a million times stronger than the signal," DeBoer said. "This is a real problem, because it's like looking for a firefly in front of an incredibly powerful searchlight. We are trying to see the firefly and filter out the searchlight."
The HERA collaboration expects eventually to expand to 330 radio dishes in the core array, each pointed straight up to measure radiation originally emitted some 13 billion years ago. Twenty outrigger dishes (not shown) are also planned, bringing the array up to 350 dishes total.
Previous experiments, such as the UC Berkeley-led Precision Array Probing the Epoch of Reionization (PAPER) in South Africa and the Murchison Widefield Array (MWA) in Australia, have not been sensitive enough to detect this signal, but with larger dishes and better signal processing, HERA should do the trick.
"HERA is a unique, next-generation instrument building on the heritage of PAPER," said Parsons, who helped build PAPER a decade ago when he was a graduate student working with the late UC Berkeley astronomer Donald Backer. "It is on the same site as PAPER, we are using a lot of the same equipment, but importantly we have brought together a lot more collaborators, including a lot of the U.S. team that has been working with MWA."
The strategy is to build a hexagonal array of radio dishes that minimizes the noise, such as radio reflections in the dishes and wires, that would obscure the signal. A supercomputer's worth of field programmable gate arrays will cross-correlate the signals from the antennas to finely map a 10-degree swath of southern sky centered at minus-30 degrees latitude. Using a technique adopted from PAPER, they will employ this computer processing power to eliminate the slowly varying noise across the wavelength spectrum 150-350 centimeters to reveal the rapidly varying signal from neutral hydrogen as they tune across the radio spectrum.
Astronomers have already discovered hints of reionization, Parsons said. Measurements of the polarization of the cosmic microwave background radiation show that some of the photons emitted at that early time in the universe have been scattered by intervening electrons possibly created by the first stars and galaxies. And galaxy surveys have turned up some very distant galaxies that show attenuation by intervening intergalactic neutral hydrogen, perhaps the last bit remaining before reionization was complete.
"We have an indication that reionization should have happened, and we are getting hints of when it might have ended, but we don't have anything telling us what is going on during it.," Parsons added. "That is what we hope to learn with HERA, the actual step-by-step process of how reionization happened."
Once astronomers know the reionization process, they can calculate the scattering of radiation from the era of recombination the cosmic background radiation, or CMB and remove some of the error that makes it hard to detect the gravitational waves produced by inflation shortly after the Big Bang.
"There is a lot of cosmology you can do with HERA," Parsons said. "We have learned so much from the thin shell of the CMB, but here we will be looking at a full three-dimensional space. Something like 80 percent of the observable universe can be mapped using the 21-centimeter line, so this opens up the next generation of cosmology."
Parsons and DeBoer compare HERA to the first experiment to detect the cosmic microwave background radiation, the Cosmic Background Explorer, which achieved its goal in 1992 and won for its leaders George Smoot of UC Berkeley and Lawrence Berkeley National Laboratory, and John Mather of NASA the 2006 Nobel Prize in Physics.
"Ultimately, the goal is to get to the point were we are actually making images, just like the CMB images we have seen," DeBoer said. "But that is really, really hard, and we need to learn a fair bit about what we are looking for and the instruments we need to get there. We hope that what we develop will allow the Square Kilometer Array or another big project to actually make these images and get much more science from this pivotal epoch in our cosmic history."
The Daily Galaxy via University of California - Berkeley
The majestic auroras have captivated humans for thousands of years, but their nature -- the fact that the lights are electromagnetic and respond to solar activity -- was only realized in the last 150 years. Thanks to coordinated multi-satellite observations and a worldwide network of magnetic sensors and cameras, close study of auroras has become possible over recent decades. Yet, auroras continue to mystify, dancing far above the ground to some, thus far, undetected rhythm.
Using data from NASA's Time History of Events and Macroscale Interactions during Substorms, or THEMIS, scientists have observed Earth's vibrating magnetic field in relation to the northern lights dancing in the night sky over Canada. THEMIS is a five-spacecraft mission dedicated to understanding the processes behind auroras, which erupt across the sky in response to changes in Earth's magnetic environment, called the magnetosphere.
These new observations allowed scientists to directly link specific intense disturbances in the magnetosphere to the magnetic response on the ground. A paper on these findings was published in Nature Physics on Sept. 12, 2016.
"We've made similar observations before, but only in one place at a time -- on the ground or in space," said David Sibeck, THEMIS project scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland, who did not participate in the study. "When you have the measurements in both places, you can relate the two things together."
Understanding how and why auroras occur helps us learn more about the complex space environment around our planet. Radiation and energy in near-Earth space can have a variety of effects on our satellites -- from disrupting their electronics to increasing frictional drag and interrupting communication or navigation signals. As our dependence on GPS grows and space exploration expands, accurate space weather forecasting becomes ever more important.
The artist's rendering below (not to scale) of a cross-section of the magnetosphere, with the solar wind on the left in yellow and magnetic field lines emanating from the Earth in blue. The five THEMIS probes were well-positioned to directly observe one particular magnetic field line as it oscillated back and forth roughly every six minutes. In this unstable environment, electrons in near-Earth space, depicted as white dots, stream rapidly down magnetic field lines towards Earth's poles. There, they interact with oxygen and nitrogen particles in the upper atmosphere, releasing photons and brightening a specific region of the aurora. (Emmanuel Masongsong/UCLA EPSS/NASA)
The space environment of our entire solar system, both near Earth and far beyond Pluto, is determined by the sun's activity, which cycles and fluctuates through time. The solar system is filled with solar wind, the constant flow of charged particles from the sun. Most of the solar wind is deflected from Earth by our planet's protective magnetosphere.
However, under the right conditions, some solar particles and energy can penetrate the magnetosphere, disturbing Earth's magnetic field in what's known as a substorm. When the solar wind's magnetic field turns southward, the dayside, or sun-facing side, of the magnetosphere contracts inward. The back end, called the magnetotail, stretches out like a rubber band. When the stretched magnetotail finally snaps back, it starts to vibrate, much like a spring moving back and forth. Bright auroras can occur during this stage of the substorm.
In this unstable environment, electrons in near-Earth space stream rapidly down magnetic field lines towards Earth's poles. There, they interact with oxygen and nitrogen particles in the upper atmosphere, releasing photons to create swaths of light that snake across the sky.
To map the auroras' electric dance, the scientists imaged the brightening and dimming aurora over Canada with all-sky cameras. They simultaneously used ground-based magnetic sensors across Canada and Greenland to measure electrical currents during the geomagnetic substorm. Further out in space, the five THEMIS probes were well-positioned to collect data on the motion of the disrupted field lines.
The scientists found the aurora moved in harmony with the vibrating field line. Magnetic field lines oscillated in a roughly six-minute cycle, or period, and the aurora brightened and dimmed at the same pace.
"We were delighted to see such a strong match," said Evgeny Panov, lead author and researcher at the Space Research Institute of the Austrian Academy of Sciences in Graz. "These observations reveal the missing link in the conversion of magnetic energy to particle energy that powers the aurora."
The brightening and dimming of the aurora corresponds to the motion of the electrons and magnetic field lines.
"During the course of this event, the electrons are flinging themselves Earthwards, then bouncing back off the magnetosphere, then flinging themselves back," Sibeck said.
When waves crash on the beach, they splash and froth, and then recede. The wave of electrons adopt a similar motion. The aurora brightens when the wave of electrons slams into the upper atmosphere, and dims when it ricochets off.
Before this study, scientists hypothesized that oscillating magnetic field lines guide the aurora. But the effect had not yet been observed because it requires the THEMIS probes to be located in just the right place over the ground-based sensors, to properly coordinate the data. In this study, scientists collected THEMIS data at a time when the probes were fortuitously positioned to observe the substorm.
THEMIS is a mission of NASA's Explorer program, which is managed by Goddard. University of California, Berkeley's Space Sciences Laboratory oversees mission operations. The all-sky imagers and magnetometers are jointly operated by UC Berkeley, UCLA, University of Calgary and University of Alberta in Canada.
The Daily Galaxy via NASA/Goddard Space Flight Center
Image top of page: http://www.outdoorfilms.cz/filmy/
The first catalog of more than a billion stars from ESA's Gaia satellite was published today the largest all-sky survey of celestial objects to date. On its way to assembling the most detailed 3-D map ever made of our Milky Way galaxy, Gaia has pinned down the precise position on the sky and the brightness of 1142 million stars.
"Today's release gives us a first impression of the extraordinary data that await us and that will revolutionize our understanding of how stars are distributed and move across our Galaxy," says Alvaro Giménez, ESA's Director of Science.
Launched 1000 days ago, Gaia started its scientific work in July 2014. This first release is based on data collected during its first 14 months of scanning the sky, up to September 2015.
"The beautiful map we are publishing today shows the density of stars measured by Gaia across the entire sky, and confirms that it collected superb data during its first year of operations," says Timo Prusti, Gaia project scientist at ESA.
The stripes and other artefacts in the image reflect how Gaia scans the sky, and will gradually fade as more scans are made during the five-year mission.
Transforming the raw information into useful and reliable stellar positions to a level of accuracy never possible before is an extremely complex procedure, entrusted to a pan-European collaboration of about 450 scientists and software engineers: the Gaia Data Processing and Analysis Consortium, or DPAC.
In addition to processing the full billion-star catalogue, the scientists looked in detail at the roughly two million stars in common between Gaia's first year and the earlier Hipparcos and Tycho-2 Catalogues, both derived from ESA's Hipparcos mission, which charted the sky more than two decades ago.
By combining Gaia data with information from these less precise catalogues, it was possible to start disentangling the effects of 'parallax' and 'proper motion' even from the first year of observations only. Parallax is a small motion in the apparent position of a star caused by Earth's yearly revolution around the Sun and depends on a star's distance from us, while proper motion is due to the physical movement of stars through the Galaxy.
In this way, the scientists were able to estimate distances and motions for the two million stars spread across the sky in the combined TychoGaia Astrometric Solution, or TGAS.
This new catalog is twice as precise and contains almost 20 times as many stars as the previous definitive reference for astrometry, the Hipparcos Catalog.
As part of their work in validating the catalogue, DPAC scientists have conducted a study of open stellar clusters groups of relatively young stars that were born together that clearly demonstrates the improvement enabled by the new data.
"With Hipparcos, we could only analyse the 3-D structure and dynamics of stars in the Hyades, the nearest open cluster to the Sun, and measure distances for about 80 clusters up to 1600 light-years from us," says Antonella Vallenari from the Istituto Nazionale di Astrofisica (INAF) and the Astronomical Observatory of Padua, Italy. "But with Gaia's first data, it is now possible to measure the distances and motions of stars in about 400 clusters up to 4800 light-years away.
For the closest 14 open clusters, the new data reveal many stars surprisingly far from the centre of the parent cluster, likely escaping to populate other regions of the Galaxy."
Many more stellar clusters will be discovered and analysed in even greater detail with the extraordinary data that Gaia continues to collect and that will be released in the coming years.
The new stellar census also contains 3194 variable stars, stars that rhythmically swell and shrink in size, leading to periodic brightness changes.
Many of the variables seen by Gaia are in the Large Magellanic Cloud, one of our galactic neighbours, a region that was scanned repeatedly during the first month of observations, allowing accurate measurement of their changing brightness.
Details about the brightness variations of these stars, 386 of which are new discoveries, are published as part of today's release, along with a first study to test the potential of the data.
"Variable stars like Cepheids and RR Lyraes are valuable indicators of cosmic distances," explains Gisella Clementini from INAF and the Astronomical Observatory of Bologna, Italy.
"While parallax is used to measure distances to large samples of stars in the Milky Way directly, variable stars provide an indirect, but crucial step on our 'cosmic distance ladder', allowing us to extend it to faraway galaxies."
This is possible because some kinds of variable stars are special. For example, in the case of Cepheid stars, the brighter they are intrinsically, the slower their brightness variations. The same is true for RR Lyraes when observed in infrared light. The variability pattern is easy to measure and can be combined with the apparent brightness of a star to infer its true brightness.
This is where Gaia steps in: in the future, scientists will be able to determine very accurate distances to a large sample of variable stars via Gaia's measurements of parallaxes. With those, they will calibrate and improve the relation between the period and brightness of these stars, and apply it to measure distances beyond our Galaxy. A preliminary application of data from the TGAS looks very promising.
"This is only the beginning: we measured the distance to the Large Magellanic Cloud to test the quality of the data, and we got a sneak preview of the dramatic improvements that Gaia will soon bring to our understanding of cosmic distances," adds Dr Clementini.
Knowing the positions and motions of stars in the sky to astonishing precision is a fundamental part of studying the properties and past history of the Milky Way and to measure distances to stars and galaxies, but also has a variety of applications closer to home for example, in the Solar System.
On 19 July 2016, Pluto passed in front of the faint star UCAC4 345-180315, offering a rare chance to study the atmosphere of the dwarf planet as the star first gradually disappeared and then reappeared behind Pluto (below).
This stellar occultation was visible only from a narrow strip stretching across Europe, similar to the totality path that a solar eclipse lays down on our planet's surface. Precise knowledge of the star's position was crucial to point telescopes on Earth, so the exceptional early release of the Gaia position for this star, which was 10 times more precise than previously available, was instrumental to the successful monitoring of this rare event.
Early results hint at a pause in the puzzling pressure rise of Pluto's tenuous atmosphere, something that has been recorded since 1988 in spite of the dwarf planet moving away from the Sun, which would suggest a drop in pressure due to cooling of the atmosphere.
These three examples demonstrate how Gaia's present and future data will revolutionize all areas of astronomy, allowing us to investigate our place in the Universe, from our local neighborhood, the Solar System, to Galactic and even grander, cosmological scales.
This first data release shows that the mission is on track to achieve its ultimate goal: charting the positions, distances, and motions of one billion stars about 1% of the Milky Way's stellar content in three dimensions to unprecedented accuracy.
"The road to today has not been without obstacles: Gaia encountered a number of technical challenges and it has taken an extensive collaborative effort to learn how to deal with them," says Fred Jansen, Gaia mission manager at ESA.
The Daily Galaxy via European Space Agency
Image credit: top of page, an all-sky view of stars in our Galaxy the Milky Way and neighboring galaxies, based on the first year of observations from ESA's Gaia satellite, from July 2014 to September 2015. Credit: ESA/Gaia/DPAC. Pluto image, B. Sicardy (LESIA, Observatoire de Paris, France), P. Tanga (Observatoire de la Côte d'Azur, Nice, France), A. Carbognani (Osservatorio Astronomico Valle d'Aosta, Italy), Rodrigo Leiva (LESIA, Observatoire de Paris)
europeanspaceagency posted a photo:
An all-sky view of stars in our Galaxy the Milky Way and neighbouring galaxies, based on the first year of observations from ESA's Gaia satellite, from July 2014 to September 2015.
This map shows the density of stars observed by Gaia in each portion of the sky. Brighter regions indicate denser concentrations of stars, while darker regions correspond to patches of the sky where fewer stars are observed.
The Milky Way is a spiral galaxy, with most of its stars residing in a disc about 100 000 light-years across and about 1000 light-years thick. This structure is visible in the sky as the Galactic Plane the brightest portion of this image which runs horizontally and is especially bright at the centre.
Darker regions across the Galactic Plane correspond to dense clouds of interstellar gas and dust that absorb starlight along the line of sight.
Many globular and open clusters groupings of stars held together by their mutual gravity are also sprinkled across the image.
Globular clusters, large assemblies of hundreds of thousands to millions of old stars, are mainly found in the halo of the Milky Way, a roughly spherical structure with a radius of about 100 000 light-years, and so are visible across the image.
Open clusters are smaller assemblies of hundreds to thousands of stars and are found mainly in the Galactic Plane.
The two bright objects in the lower right of the image are the Large and Small Magellanic Clouds, two dwarf galaxies orbiting the Milky Way. Other nearby galaxies are also visible, most notably Andromeda (also known as M31), the largest galactic neighbour to the Milky Way, in the lower left of the image. Below Andromeda is its satellite, the Triangulum galaxy (M33).
A number of artefacts are also visible on the image. These curved features and darker stripes are not of astronomical origin but rather reflect Gaia's scanning procedure. As this map is based on observations performed during the mission's first year, the survey is not yet uniform across the sky.
These artefacts will gradually disappear as more data are gathered during the five-year mission.
High resolution versions of the Gaia map, with transparent background, are available to download from: sci.esa.int/gaia/58209
An annotated version of this image is available here.
Credit: ESA/Gaia/DPAC
Acknowledgement: A. Moitinho & M. Barros (CENTRA University of Lisbon), on behalf of DPAC
How a community-supported collective of filmmakers wants to rewrite the rules of indie film.
To celebrate the recent release of ‘For the Love of Spock,' Adam Nimoy's documentary tribute to his father and the iconic character he…
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Chalcid wasp (Aprostocetus sp.) collected in Mingan Archipelago National Park Reserve, Quebec, Canada, and photographed at the Centre for Biodiversity Genomics (sample ID: BIOUG12652-A10; specimen record: http://www.boldsystems.org/index.php/Public_RecordView?processid=CNMIH1932-14 BIN: http://www.boldsystems.org/index.php/Public_BarcodeCluster?clusteruri=BOLD:ACW3983)
the large orange life rafts, anchored to the palace's windows, aim to draw attention to the fate of refugees who risk their lives daily.
The post ai weiwei to wrap the façade of florence's palazzo strozzi in rubber life boats appeared first on designboom | architecture & design magazine.
The European Space Agency [ESA] have released the most detailed map of the Milky Way galaxy to date, based on the first delivery of data from the ESA's Gaia probe, which was launched in 2013. The map represents 1% of the Milky Way's stars, but this map is at least 20 times more complete than any previous representations
Continue reading...The map, based on observations from the European Space Agency's Gaia probe, will transform what we know about the galaxy, say scientists
Astronomers have unveiled the most detailed map to date of the Milky Way, after charting the positions of more than 1bn stars with stunning precision.
The map, based on observations from the European Space Agency's Gaia probe, still only represents about 1% of the Milky Way's stars, but is already 20 times more complete than any previous observations of the night sky.
Continue reading...Victorian Society says 2016 list, featuring no structures in London or south-east, may reflect ‘vastly different financial climate'
From the former home of explorer Gertrude Bell to a landmark of the Grimsby skyline, seven of Britain's 10 most endangered historic buildings are in the north of England.
The annual list of once-celebrated structures, compiled by the Victorian Society, is dominated by “at-risk” buildings in the north and for the first time features none in London or the south-east.
Related: Lost in the Great Fire: which London buildings disappeared in the 1666 blaze?
Continue reading...From steamrooms suspended under remote Czech bridges to the Swedish robot sauna straight out of Star Wars, the spa experience is getting a guerilla makeover
An awkward grey creature stands on the edge of Frihamnen harbour in Gothenburg. It looks like a homemade robot elephant, cobbled together from industrial remains strewn around the dock. Clad in rusty sheets of corrugated steel, its truncated body stands on gawky little legs, lurching this way and that with cartoonish wonkiness.
“We wanted people to be curious about what this thing could be,” says Francesco Apuzzo of Raumlabor, the Berlin-based architectural collective behind this mysterious structure. It could be the chubby cousin of one of the laser-wielding AT-AT killing machines from Star Wars, but it has a more benign purpose. “People have to climb up the steps and only then do they discover the soft wooden interior of the sauna within.”
Related: Carnival of design
We're not sauna obsessives … but with everyone stripped of clothing, the sauna is ultimately a democratic space
Related: The naked truth about saunas | Andy Symington
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The hypocrisy from the majority members defending scientific freedom given their previous actions towards NOAA+Tom Karl is breathtaking
— Gavin Schmidt (@ClimateOfGavin) September 14, 2016
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Read more: Bernie Sanders, Climate Change, Obama, Environment, Native Americans, Activism, Oil and Gas, Green Energy, Dakota Access Pipeline, Politics News
In September, TU will be feeding you a heavy dose of stories about public lands. From the Golden Trout wilderness in California to the Green Mountains of Vermont, public lands are hugely important to wild and native fish. In most Western states, public lands comprise more than 70 percent of the available habitat for trout, and virtually all of the strongholds for native trout.
My father is the sixth generation of our family to grow up in Newark, NJ. Growing up, the closest public land we had was a local county park called Tuers, where I shot countless hours of hoop. Except for visiting family in Ireland, I didn't leave the Garden State until college in Vermont, and there discovered the Green Mountain National Forest. I spent many hours in that forest catching native brook trout.
After graduation I took a long, slow trip across the country with my dog, Gus, and a big box filled with Dinty Moore beef stew. Gus and I walked the Natchez Trace in Mississippi. We hiked the Smokies in Tennessee. We took pictures of fields of Black-eyed Susans in the Shenandoah. Swam in hot springs in Idaho and clamored over red rocks in Utah. Camped among the aspen in Colorado. Hiked old growth forests in Oregon, marveled at the coastal redwoods of California.
All those places share one thing. They are public lands that belong to us all. For now. In recent years, more than 50 short-sighted bills have been introduced in state legislatures to transfer, sell, or otherwise take away your birthright—the public lands that are managed for us by the U.S. Forest Service and the Bureau of Land Management. Not to be outdone, Congress has entertained similar proposals. Presidential candidates have campaigned on the issue. As much as we'd all like to think “that can't happen,” the fact is that there are well-heeled special interests dedicated to seeing that it does.
Those who seek this so called “transfer”—county supremacists, sagebrush rebels and their contemporary cicadian progeny—neglect an important fact. At no time did the Western federally managed public lands belong to the states. They were either ceded to the Union by Eastern states or acquired through treaty, conquest or purchase by the federal government acting on behalf of the citizens of the United States.
Public lands are the best idea America ever had. For those of us who want to fish and hunt, camp and hike without having to beg or buy permission, they are a godsend. The ham-handed dialogue about transferring or divesting public lands that drives the debate today is unhelpful and unproductive. To suggest that our land legacy—a legacy that a kid from New Jersey shares with a rancher in New Mexico—should be transferred or sold for a pittance is extreme and offensive.
For the next 30 days, tune into TU for a steady diet of stores about why public lands matter. Share the stories, video, and photos with your friends. Raise your voice and let your member of Congress and elected leaders in your state know that the public lands are a birthright that belongs to all of us, and we are not willing sellers.
-- 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.