Category: Environment

From season to season and year to year, weather events that were once rare occurrences are now increasingly commonplace. After human kind has been through once in a century like the Covid pandemic that has killed over a million people, now the world is faced with yet another once in a century like catastrophic climatic conditions around the world. 

Soaring and record-breaking temperatures, hotter air holding more moisture, extreme weather getting wilder, melting glaciers, rising sea levels, wild fires, and floods that are inundating parts of the world that has proven 2022 to be yet another year that will go down in history.

Unprecedented heat waves have occurred recently from Delhi to the Pacific Northwest, and the number of these deadly events is expected to increase. New research from the University of Washington and Harvard University gives a range of heat impacts worldwide by the end of this century, depending on future emissions of greenhouse gases.

The study was published Aug. 25 in the open-access journal Communications Earth & Environment. “The record-breaking heat events of recent summers will become much more common in places like North America and Europe,” said lead author Lucas Vargas Zeppetello, who did the research as a doctoral student at the UW and is now a postdoctoral researcher at Harvard. “For many places close to the equator, by 2100 more than half the year will be a challenge to work outside, even if we begin to curb emissions.”

“Our study shows a broad range of possible scenarios for 2100,” he added. “This shows that the emissions choices we make now still matter for creating a habitable future.”

The study looks at a combination of air temperature and humidity known as the “heat index” that measures impact on the human body. A “dangerous” heat index is defined by the National Weather Service as 103 F (39.4 C). An “extremely dangerous” heat index is 124 F (51 C), deemed unsafe to humans for any amount of time.

“These standards were first created for people working indoors in places like boiler rooms — they were not thought of as conditions that would happen in outdoor, ambient environments. But we are seeing them now,” Vargas Zeppetello said.

Across the world “intense rain storms are getting more intense,” said Princeton University climate scientist Michael Oppenheimer. And he said mountains, like those in Pakistan, help wring extra moisture out as the clouds pass. The flooding has all the hallmarks of a catastrophe juiced by climate change, but it is too early to formally assign blame to global warming, several scientists told the media. 

At least 1,136 people have been killed since June and roads, crops, homes and bridges washed away across the country. This year’s record monsoon is comparable to the devastating floods of 2010 – the deadliest in Pakistan’s history – which left more than 2,000 people dead.

The “recent flood in Pakistan is actually an outcome of the climate catastrophe … that was looming very large,” said Anjal Prakash, a research director at India’s Bharti Institute of Public Policy. “The kind of incessant rainfall that has happened … has been unprecedented.”

“This year Pakistan has received the highest rainfall in at least three decades. So far this year the rain is running at more than 780% above average levels,” said Abid Qaiyum Suleri, executive director of the Sustainable Development Policy Institute and a member of Pakistan’s Climate Change Council. “Extreme weather patterns are turning more frequent in the region and Pakistan is not a exception.”

Pakistan’s Climate Minister Sherry Rehman said “it’s been a catastrophe of unprecedented proportions.” Pakistan “is considered the eighth most vulnerable country to climate change,” said Moshin Hafeez, a Lahore-based climate scientist at the International Water Management Institute. Its rain, heat and melting glaciers are all climate change factors scientists warned repeatedly about.

“Clearly, it’s being juiced by climate change,” said Jennifer Francis, a climate scientist at the Woodwell Climate Research Center in Massachusetts. There’s been a 400% increase in average rainfall in areas like Baluchistan and Sindh, which led to the extreme flooding, Hafeez said. At least 20 dams have been breached.

If the rains are a huge factor that impacted millions, the heat has been as relentless as the rain. In May, Pakistan consistently saw temperatures above 45 degrees Celsius (113 Fahrenheit). Scorching temperatures higher than 50 degrees Celsius (122 Fahrenheit) were recorded in places like Jacobabad and Dadu.

The extreme heat accelerates the long-term glacier melting then water speeds down from the Himalayas to Pakistan in a dangerous phenomena called glacial lake outburst floods. “We have the largest number of glaciers outside the polar region, and this affects us,” climate minister Rehman said. “Instead of keeping their majesty and preserving them for posterity and nature. We are seeing them melt.”

As per reports, the disaster is hitting a poor country that has contributed relatively little to the world’s climate problem, scientists and officials said. Since 1959, Pakistan has emitted about 0.4% of heat-trapping carbon dioxide, compared to 21.5% by the United States and 16.4% by China.

“Those countries that have developed or gotten rich on the back of fossil fuels, which are the problem really,” Rehman said. “They’re going to have to make a critical decision that the world is coming to a tipping point. We certainly have already reached that point because of our geographical location.”

UN Secretary General Antonio Guterres urged the world to come to Pakistan’s aid as he launched a $160m appeal to help the tens of millions affected in the disaster. He blamed “the relentless impact of epochal levels of rain and flooding”.

As global temperatures rise, the hottest temperatures — and the number of areas impacted by extreme heat — are also rising. That means more scorching hot days in more places.

Take the Texas cities of Austin and Houston, for example. Over the past 50 years, Austin has seen the number of days with temperatures above 100°F increase by one month, while Houston has recorded an additional month with temperatures above 95°F. In California, temperatures are estimated to have increased 3°F in the past century.

In recent years, California has become ground zero for meteorological turmoil. With record dry, hot conditions across the state, seasonal high winds (known as Diablo in Northern California and Santa Ana in the southern part of the state) caused destructive wildfires to grow and spread at an unprecedented rate.

When global temperatures rise, moisture evaporates from waterbodies and soil. Droughts in the U.S. and elsewhere in the world have become more severe and long-lasting thanks to climate change. The American West is currently in the midst of a mega drought that ranks among the worst in the past 1,200 years.

Hurricanes are growing more powerful as global temperatures rise because these storm systems draw their energy from warm ocean water. One of the most powerful storms to ever hit the United States struck the Gulf Coast in August 2020. Hurricane Katrina ripped into the Gulf Coast in August 2005, devastating entire cities and hitting communities like those in low-lying New Orleans parishes especially hard.

As the planet warms, ocean waters are also warming — and expanding. At the same time, warmer temperatures are causing land ice — think glaciers and ice caps — to melt, which is adding water to the world’s oceans. As a result, average global sea level has increased eight inches in the last 150 years.

Ice Melt from Greenland will raise sea level 10 inches

Greenland’s rapidly melting ice sheet will eventually raise global sea level by at least 10.6 inches (27 centimeters) — more than twice as much as previously forecast — according to a study published on August 29th.

That’s because of something that could be called zombie ice. That’s doomed ice that, while still attached to thicker areas of ice, is no longer getting replenished by parent glaciers now receiving less snow. Without replenishment, the doomed ice is melting from climate change and will inevitably raise seas, said study co-author William Colgan, a glaciologist at the Geological Survey of Denmark and Greenland.

“It’s dead ice. It’s just going to melt and disappear from the ice sheet,” Colgan said in an interview. “This ice has been consigned to the ocean, regardless of what climate (emissions) scenario we take now.” Study lead author Jason Box, a glaciologist at the Greenland survey, said it is “more like one foot in the grave.”

One of the study authors said that more than 120 trillion tons (110 trillion metric tons) of ice is already doomed to melt from the warming ice sheet’s inability to replenish its edges. When that ice melts into water, if it were concentrated only over the United States, it would be 37 feet (11 meters) deep.

The figures are a global average for sea level rise, but some places further away from Greenland would get more and places closer, like the U.S. East Coast, would get less. Although 10.6 inches may not sound like much, this would be over and above high tides and storms, making them even worse, so this much sea level rise “will have huge societal, economic and environmental impacts,” said Ellyn Enderlin, a geosciences professor at Boise State University, who wasn’t part of the study. “This is a really large loss and will have a detrimental effect on coastlines around the world,” said NYU’s David Holland who just returned from Greenland, but is not part of the study.

According to scientists, the year 2012 (and to a different degree 2019 ) was a huge melt year, when the equilibrium between adding and subtracting ice was most out of balance. If Earth starts to undergo more years like 2012, Greenland melt could trigger 30 inches (78 centimeters) of sea level rise, he said. Those two years seem extreme now, but years that look normal now would have been extreme 50 years ago. That’s how climate change works. Today’s outliers become tomorrow’s averages.”

By, Harvard University

Artistic reconstruction of the reptile adaptive radiation in a terrestrial ecosystem during the warmest period in Earth’s history. Image depicts a massive, big-headed, carnivorous erythrosuchid (close relative to crocodiles and dinosaurs) and a tiny gliding reptile at about 240 million years ago. The erythrosuchid is chasing the gliding reptile and it is propelling itself using a fossilized skull of the extinct Dimetrodon (early mammalian ancestor) in a hot and dry river valley.

Newswise — Just over 250 million years ago during the end of the Permian period and start of the Triassic, reptiles had one heck of a coming out party.

Their rates of evolution and diversity started exploding, leading to a dizzying variety of abilities, body plans, and traits, and helping to firmly establish both their extinct lineages and those that still exist today as one of the most successful and diverse animal groups the world has ever seen. For the longest time, this flourish was explained by their competition being wiped out by two of the biggest mass extinction events (around 261 and 252 million years ago) in the history of the planet.

A new Harvard-led study has rewritten that explanation by reconstructing how the bodies of ancient reptiles changed and by comparing it against millions of years of climate change.

Harvard paleontologist Stephanie Pierce’s lab shows that the morphological evolution and diversification seen in early reptiles not only started years before these mass extinction events but instead were directly driven by what caused them in the first place — rising global temperatures due to climate change.

“We are suggesting that we have two major factors at play — not just this open ecological opportunity that has always been thought by several scientists — but also something that nobody had previously come up with, which is that climate change actually directly triggered the adaptive response of reptiles to help build this vast array of new body plans and the explosion of groups that we see in the Triassic,” said Tiago R. Simões, a postdoctoral fellow in the Pierce lab and lead author on the study.

“Basically, [rising global temperatures] triggered all these different morphological experiments — some that worked quite well and survived for millions of years up to this day, and some others that basically vanished a few million years later,” Simões added.

In the paper, which published Friday in Science Advances, the researchers lay out the vast anatomical changes that took place in many reptile groups, including the forerunners of crocodiles and dinosaurs, in direct response to major climate shifts concentrated between 260 to 230 million years ago.

The study provides a close look at how a large group of organisms evolve because of climate change, which is especially pertinent today as temperatures continually rise. In fact, the rate of carbon dioxide released into the atmosphere today is about nine times what they were during the timeframe that culminated in the biggest climate change-driven mass extinction of all time 252 million years ago: the Permian-Triassic mass extinction.

“Major shifts in global temperature can have dramatic and varying impacts on biodiversity,” said  Stephanie E. Pierce, Thomas D. Cabot Associate Professor of Organismic and Evolutionary Biology and curator of vertebrate paleontology in the Museum of Comparative Zoology. “Here we show that rising temperatures during the Permian-Triassic led to the extinction of many animals, including many of the ancestors of mammals, but also sparked the explosive evolution of others, especially the reptiles that went on to dominate the Triassic period.”

The study involved close to eight years of data collection and took a heavy dose of camerawork, CT scanning, and loads of passport stamps as Simões traveled to more than 20 countries and more than 50 different museums to take scans and snapshots of more than 1,000 reptilian fossils.

With all the information, the researchers created an expansive dataset that was analyzed with state-of-the-art statistical methods to produce a diagram called an evolutionary time tree. Time trees reveal how early reptiles were related to each other, when their lineages first originated, and how fast they were evolving. They then combined it with global temperature data from millions of years ago.

Diversification of reptile body plans started about 30 million years before the Permian-Triassic extinction, making it clear these changes weren’t triggered by the event as previously thought. The extinction events did help put them in gear though.

The dataset also showed that rises in global temperatures, which started at about 270 million years ago and lasted until at least 240 million years ago, were followed by rapid body changes in most reptile lineages. For instance, some of the larger cold-blooded animals evolved to become smaller so they could cool down easier; others evolved to life in water for that same effect. The latter group included some of the most bizarre forms of reptiles that would go on to become extinct such as a giant, long-necked marine reptile once thought to be the Loch Ness monster, a tiny chameleon-like creature with a bird-like skull and beak, and a gliding reptile resembling a gecko with wings. It also includes the ancestors of reptiles that still exist today like turtles and crocodiles.

Smaller reptiles, which gave rise to the first lizards and tuataras, went on a different path than their larger reptile brethren. Their evolutionary rates slowed down and stabilized in response to the rising temperatures. The researchers believe it was because the small-bodied reptiles were already better adapted to the rising heat since they can more easily release heat from their bodies compared to larger reptiles when temperatures got hot very quickly all-around Earth.

The researchers say they are planning to expand on this work investigating the impact of environmental catastrophes on evolution of organisms with abundant modern diversity, such as the major groups of lizards and snakes.

Newswise — The way rivers function is significantly affected by how much sediment they transport and where it gets deposited. River sediment — mostly sand, silt, and clay — plays a critical ecological role, as it provides habitat for organisms downstream and in estuaries. It is also important for human life, resupplying nutrients to floodplain agricultural soils, and buffering sea level rise caused by climate change by delivering sand to deltas and coastlines. However, these functions are under threat: in the past 40 years, humans have caused unprecedented, consequential changes to river sediment transport, according to a new Dartmouth study published in Science.

Using satellite images from NASA Landsat and digital archives of hydrologic data, Dartmouth researchers examined changes in how much sediment is carried to the oceans by 414 of the world’s largest rivers from 1984 to 2020.

“Our results tell a tale of two hemispheres. The north has seen major reductions in river sediment transport over the past 40 years, while the south has seen large increases over the same period,” says lead author Evan Dethier, a post-doctoral fellow at Dartmouth. “Humans have been able to alter the world’s biggest rivers at rates that are unprecedented in the recent geologic record.” Dethier says. “The amount of sediment rivers carry is generally dictated by natural processes in watersheds, like how much rain there is or whether there are landslides or vegetation. We find that direct human activities are overwhelming these natural processes, and even outweighing the effects of climate change.”

The findings show that massive 20th century dam building in the global hydrologic north — North America, Europe/Eurasia and Asia — has reduced global in river suspended sediment delivery to the oceans by 49% relative to pre-dam conditions. This global reduction has occurred despite major increases in sediment delivery from the global hydrologic south — South America, Africa and Oceania. There, sediment transport has increased on 36% of its rivers in the region due to major land use change.

The changes to sediment transport in the south have been driven mainly by intensive land use changes, most of which are associated with deforestation. Notable examples include logging in Malaysia; alluvial gold mining in South America and sub-Saharan Africa; sand mining in Bangladesh and India; and palm oil plantations across much of Oceania. (In prior research, Dethier found that artisanal gold mining in Peru is associated with increases in suspended sediment levels).

In the north, dam building has been the dominant agent of change for rivers in the past several centuries.

“One of the motivations for this research has been the global expansion of building large dams,” says co-author Francis Magilligan, a professor of geography and the Frank J. Reagan ’09 Chair of Policy Studies at Dartmouth, who studies dams and dam removal. “In the U.S. alone, there are more than 90,000 dams listed in the National Inventory of Dams.” Magilligan says, “One way to think about this is that we, as a nation have been building on average, one dam per day, since the signing of the Declaration of Independence.”

Rivers are responsible for creating floodplains, sandbars, estuaries, and deltas due to the sediment that they transport. However, once a dam is installed, that supply of sediment, including its nutrients, is often shut off.

In the U.S. and other countries in the Northern Hemisphere, however, many dams are more than a half-century- old and fewer dams are being built in the 21st century. Recent declines in sediment transport are relatively minimal, as a result. Dam building in Eurasia and Asia in the past 30 years, especially in China, has driven ongoing reductions in global sediment transport.

“For low lying countries (countries that live at, near or below sea level) in delta regions, sediment supply from rivers has in the past, been able to help offset the effects of sea level rise from climate change,” says Magilligan “but now you’ve got the double drivers of declining sediment from dam construction and rising sea levels.” He says, “This is particularly worrisome for densely populated places like Vietnam, where sediment supply has been reduced significantly by dam activity along the Mekong River.”

The results in the north are striking and could foreshadow future changes to come for the south, as the study reports that there are more than 300 dams planned for large rivers in South America and Oceania. The Amazon River carries more sediment than any other river in the world and is a major target for these dams.

“Rivers are pretty sensitive indicators of what we’re doing to the surface of the Earth — they are sort of like a thermometer for land use change,” says co-author Carl Renshaw, the Evans Family Distinguished Professor of Earth Sciences at Dartmouth. “Yet, for rivers in the Northern Hemisphere, dams are now blocking that signal for sediment coming to the ocean.” Renshaw says that, “It’s well-established that there’s a soil loss crisis in the U.S. but we just don’t see it in the sediment export record because it’s all getting stuck behind these dams, whereas, we can see the signal for rivers in the global south.”

Dethier says, “In many cases throughout the world, we have built our environment around rivers and the way that they operate, for use in agriculture, industry, recreation and tourism, and transportation, but when human activity suddenly disrupts the way rivers function, it may become difficult to adapt in real-time to such impacts.”

How dams retain sediment and how land use is increasing downstream erosion are principles which the researchers hope can be used to help inform planning decisions and land use and environmental management policies in riparian and coastal zones in the future.

By, Dartmouth College

Two Catholic priests, both astrophysicists from the Vatican Observatory, have suggested a radically new mathematical approach to studying the initial moments following the Big Bang that gave birth to our universe.

Little is known about the first seconds of the universe’s existence, and one of the deeper puzzles is accounting for the role gravity played in those early moments. The Rev. Gabriele Gionti, a Jesuit, and the Rev. Matteo Galaverni, a priest in the Diocese of Reggio Emilia-Guastalla in Northern Italy, set out to propose a new technique that explains how gravity might have behaved as the cosmos expanded rapidly at its inception.

Their research, published in the prestigious Physical Review D journal on April 15, proposes an alternative to the Jordans-Brans-Dicke theory of gravitation, which solves difficulties with Albert Einstein’s general theory of relativity in describing gravity after the Big Bang, but which has its own inconsistencies.

Einstein’s theory works well in explaining the way matter behaves on a large scale but clashes with the way quantum physics describes the gravity among the smallest observable particles. For years, Gionti has attempted to reconcile the two.

The priests’ work is “a tassel within this search that the scientific community has been conducting for many years on quantum gravity, meaning that gravity is capable of affecting (matter) even at a very, very small scale,” said Galaverni in a Zoom interview conducted by RNS with the two priests on Thursday (May 5).

“We realized that within limits, when the gravitational constant is very high, it’s possible for the speed of light to go to zero, meaning that nothing propagates because gravity is too high,” said Gionti.

“This might be a way to explain what happened after the Big Bang,” he said. In layman’s terms, Gionti said, “It’s like being in a theater, and until now we have seen the musicians and the orchestra with our eyes. Now with gravitational waves we can also hear the music. This is revolutionizing and will revolutionize the next decades of astronomy,” he added.

Gionti clarified that their “research is based on a very speculative and theoretical mathematical approach,” which will have to be tested in its physical and observable consequences.

They wrote their theory at the Specola Vaticana, the Vatican Observatory in Castel Gandolfo, the pope’s summer residence, drawing up their abstract calculations both on computers and  blackboards as they compared and discussed their ideas.

Pope Leo XIII created the Specola in 1918 “in a time of modernism where society accused the church of obscurantism,” Gionti said. The Vatican trials against astronomers and thinkers like Galileo Galilei and Giordano Bruni in the 16th century had pegged the Catholic Church as a “determined opponent to scientific progress,” he explained.

“The Vatican created the Vatican observatory for priests, nuns and religious to prove to the world that the church directly contributed to science by providing it with an astronomical observatory that worked scientifically like all other observatories,” Gionti said.

Gionti and Galaverni’s work stands on the shoulders of great scientists as well as on the work of religious people. It was a diocesan priest from Belgium, Georges Lemaître, who first theorized the Big Bang in the early 20th century. Numerous priests and religious contributed to today’s understanding of gravity and astronomy. The Jesuit Angelo Secchi laid out the principles for how we classify stars today from the roof of the Church of St. Ignatius in Rome.

Science and religion are “two complementary approaches that must be respected in their diversity,” Galaverni said, who added that studying the universe is “not something that proves my faith, it’s something that enriches it.”

“Science also teaches me a certain humility in looking at the universe and recognizing our smallness and seeing the greatness of God in this,” he added. While studying the laws of physics and nature, the universe seems harmonious and well-ordered, he said, adding that “for someone of faith it’s an easy step to recognize in this order the footprint of God.”

Their work has been well received by their scientific peers, “but we are not finished yet. There are other questions that we haven’t answered,” Gionti said.

It’s not the end of the world. It only seems that way. Climate change is going to get worse, but as gloomy as the latest scientific reports are, including today’s from the United Nations, scientist after scientist stresses that curbing global warming is not hopeless. The science says it is not game over for planet Earth or humanity. Action can prevent some of the worst if done soon, they say.

After decades of trying to get the public’s attention, spur action by governments and fight against organized movements denying the science, climate researchers say they have a new fight on their hands: doomism. It’s the feeling that nothing can be done, so why bother. It’s young people publicly swearing off having children because of climate change.

University of Maine climate scientist Jacquelyn Gill noticed in 2018 fewer people telling her climate change isn’t real and more “people that we now call doomers that you know believe that nothing can be done.” Gill says it is just not true. “I refuse to write off or write an obituary for something that’s still alive,” Gill told The Associated Press, referring to the Earth. “We are not through a threshold or past the threshold. There’s no such thing as pass-fail when it comes to the climate crisis.”

“It’s really, really, really hard to walk people back from that ledge,” Gill said. Doomism “is definitely a thing,” said Wooster College psychology professor Susan Clayton, who studies climate change anxiety and spoke at a conference in Norway last week that addressed the issue. “It’s a way of saying ‘I don’t have to go to the effort of making changes because there’s nothing I can do anyway.’”

Gill and six other scientists who talked with The Associated Press about doomism aren’t sugarcoating the escalating harm to the climate from accumulating emissions. But that doesn’t make it hopeless, they said.

“Everybody knows it’s going to get worse,” said Woodwell Climate Research Center scientist Jennifer Francis. “We can do a lot to make it less bad than the worst case scenario.”

The United Nation’s Intergovernmental Panel on Climate Change just issued its third report in six months. The first two were on how bad warming is and how it will hurt people and ecosystems, with today’s report focusing on how the extent of disruption depends on how much fossil fuels are burned. It shows the world is still heading in the wrong direction in its fight to curb climate change, with new investments in fossil fuel infrastructure and forests falling to make way for agriculture.

“It’s not that they’re saying you are condemned to a future of destruction and increasing misery,” said Christiana Figueres, the former U.N. climate secretary who helped forge the 2015 Paris climate agreement and now runs an organization called Global Optimism. “What they’re saying is ’the business-as-usual path … is an atlas of misery ’ or a future of increasing destruction. But we don’t have to choose that. And that’s the piece, the second piece, that sort of always gets dropped out of the conversation.”

United Nations Environment Program Director Inger Andersen said with reports like these, officials are walking a tightrope. They are trying to spur the world to action because scientists are calling this a crisis. But they also don’t want to send people spiraling into paralysis because it is too gloomy.

“We are not doomed, but rapid action is absolutely essential,” Andersen said. “With every month or year that we delay action, climate change becomes more complex, expensive and difficult to overcome.”

“The big message we’ve got (is that) human activities got us into this problem and human agency can actually get us out of it again,” James Skea, co-chair of Monday’s report, said. “It’s not all lost. We really have the chance to do something.”

Monday’s report details that it is unlikely, without immediate and drastic carbon pollution cuts, that the world will limit warming to 1.5 degrees Celsius (2.7 degrees Fahrenheit) since pre-industrial times, which is the world’s agreed upon goal. The world has already warmed 1.1 degrees Celsius (2 degrees Fahrenheit). And earlier IPCC reports have shown that after 1.5 degrees, more people die, more ecosystems are in trouble and climate change worsens rapidly.

“We don’t fall over the cliff at 1.5 degrees,” Skea said, “Even if we were to go beyond 1.5 it doesn’t mean we throw up our hands in despair.”

IPCC reports showed that depending on how much coal, oil, and natural gas is burned, warming by 2100 could be anywhere from 1.4 to 4.4 degrees Celsius (2.5 to 7.2 degrees Fahrenheit) above pre-industrial times, which can mean large differences in sickness, death and weather disasters.

While he sees the increase in doom talk as inevitable, NASA climate scientist Gavin Schmidt said he knows first-hand that people are wrong when they say nothing can be done: “I work with people and I’m watching other people and I’m seeing the administration. And people are doing things and they’re doing the right things for the most part as best they can. So I’m seeing people do things.”

Pennsylvania State University climate scientist Michael Mann said scientists used to think Earth would be committed to decades of future warming even after people stopped pumping more carbon dioxide into the air than nature takes out. But newer analyses in recent years show it will only take a few years after net zero emissions for carbon levels in the air to start to go down because of carbon being sucked up by the oceans and forests, Mann said.

Scientists’ legitimate worries get repeated and amplified like in the kids game of telephone and “by the time you’re done, it’s ‘we’re doomed’ when what the scientist actually said was we need to reduce or carbon emissions 50% within this decade to avoid 1.5 (degrees of) warming, which would be really bad. Two degrees of warming would be far worse than 1.5 warming, but not the end of civilization,” Mann said.

Mann said doomism has become far more of a threat than denialism and he believes that some of the same people, trade associations and companies that denied climate change are encouraging people who say it is too late. Mann is battling publicly with a retired University of Arizona ecologist, Guy McPherson, an intellectual leader of the doom movement.

McPherson said he’s not part of the monetary system, hasn’t had a paycheck in 13 years, doesn’t vote and lived off the grid for a decade. He said all species go extinct and humans are no exception. He publicly predicted humanity will go extinct in 2026, but in an interview with The Associated Press said, “I’m not nearly as stuck on 2026,” and mentioned 2030 and changes to human habitat from the loss of Arctic summer sea ice.

Woodwell’s Francis, a pioneer in the study of Arctic sea ice who McPherson said he admires, said while the Arctic will be ice free by the summer by 2050, McPherson exaggerates the bad effects. Local Arctic residents will be hit hard, “the rest of us will experience accelerated warming and sea-level rise, disrupted weather patterns and more frequent extreme weather. Most communities will adapt to varying degrees,” Francis said. “There’s no way in hell humans will go extinct by 2026.”

Humans probably can no longer prevent Arctic sea ice from disappearing in the summer, but with new technology and emissions cuts, Francis said, “we stand a real chance of preventing those (other) catastrophic scenarios out there.”

Psychology professor Clayton said “no matter how bad things are, they can always be worse. You can make a difference between bad and worse… That’s very powerful, very self-affirming.

Could the Earth be one of the trillions of experiments God is running throughout the universe? If so, will it be a failed experiment?

Humankind’s sacred Scriptures, written in prescientific times, often portray the Earth and humanity as the center of the universe. Recent scientific discoveries have suggested that this is not so. It is time to update our theological imaginations.

I spent New Year’s weekend bingeing on NOVA’s five-part series on astronomy, “Universe Revealed,” which premiered in October. It beautifully describes the findings of NASA’s astronomical satellites, including the Hubble Space Telescope, the Chandra X-ray Observatory and the Fermi Gamma Ray Space Telescope.

We have learned that our Milky Way is one of 2 trillion known galaxies in the universe. Our galaxy alone has 200 billion stars and most of these stars appear to have planets. The probability of intelligent life somewhere in our galaxy or in another galaxy is high, given these numbers.

Why would God create such a huge universe with so many possible sources of life if he did not want thousands of species to bloom? Do we think that God has so little imagination that we are the only possibility he could come up with?

This is humbling for the human species, which thinks that it is the most important thing in the universe. It means that we are just one of God’s many children — and probably not the most important. We may be in our infancy in comparison with our siblings in other parts of the universe.

A Hubble photo shows but a small portion of one of the largest seen star-birth regions in the galaxy, the Carina Nebula. Towers of cool hydrogen laced with dust rise from the wall of the nebula. Captured here are the top of a three-light-year-tall pillar of gas and the dust that is being eaten away by the brilliant light from nearby bright stars. Photo courtesy of NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)

Perhaps the universe is incredibly huge so that God could provide “social distance” between all his experiments so that they would not cross-contaminate.

As for us, God has granted us a very beautiful and rich planet, made from star dust. He has given us intelligence with which we have gained great power for both good and evil.

And yet he appears to have included a fail-safe in the human experiment: If we do not evolve morally, we will destroy ourselves before we can reach the stars and pollute the rest of the universe.

The human experiment can fail, and if so our failure will not be God’s failure. God gives us every chance, but we can blow it. That is what we call free will. But he has other experiments running throughout the universe, and some of them will succeed.

On the other hand, we may also succeed and join our other siblings in the universe in discovering God’s plan for uniting himself with the cosmos

Pope Benedict XVI described the risen Christ as the next step in human evolution. That evolution is a spiritual consciousness that puts service above domination, puts generosity above greed and puts love above self-indulgence.

Pierre Teilhard de Chardin, the Jesuit paleontologist, had a similar vision of the universe, infused with the Spirit, evolving into the Cosmic Christ. Do we want to be part of that evolution or will we fight it?

Perhaps we do have a special place in the universe. Perhaps like Bethlehem, Earth is a backwater in the universe that has something worth sharing. I hope so. But unless our spiritual development matches our scientific development, the human experiment will fail.

Efforts are about to get under way to drill a core of ice in Antarctica that contains a record of Earth’s climate stretching back 1.5 million years. A European team will set up its equipment at one of the highest locations on the White Continent, for an operation likely to take four years. The project aims to recover a near-3km-long cylinder of frozen material.

Scientists hope this ice can help them explain why Earth’s ice ages flipped in frequency in the deep past.

“Beyond EPICA”, as the project is known, is a follow-up to a similar venture at the turn of the millennium called simply EPICA (European Project for Ice Coring in Antarctica).

The new endeavour will base itself a short distance away from the original at Little Dome C, an area located roughly 40km from the Italian-French Concordia Station, on the east Antarctic plateau

At an altitude of 3,233m above sea level and over 1,000km from the coast, Little Dome C will be an inhospitable place to work. Even in summer, temperatures won’t get much above -35C.

The camp where the drill team will base itself was set up in the 2019/20. This coming season will largely be about putting in the necessary drilling infrastructure. But the technicians do aim to at least start on their core quest by getting down beyond the first 100m.

This should take the borehole past the lightly compacted snow layers, or firn, into the impervious ice layers that are the real interest for scientists. The deep ice in Antarctica contains tiny bubbles of air. These little gas pockets are a direct snapshot of the historic atmosphere.

Scientists can read off the levels of carbon dioxide and other heat-trapping components, such as methane.

Analysing the atoms in the water-ice molecules encasing the gases also gives an indication of the temperature that persisted at the time of the snowfall that gave rise to the ice.

The previous ice core showed temperature and carbon dioxide moving in lock-step

When researchers drilled the original EPICA core, they uncovered a narrative of past climate temperature and atmospheric carbon dioxide stretching back 800,000 years.

It’s become one of the key climate data-sets of recent decades.

It showed that CO2 and temperature moved in lock-step. Whenever the Earth went into an ice age and temperature fell, the concentration of greenhouse gases in the atmosphere would also decline. And when the climate warmed back up again, the CO2 rose in parallel.

These cycles occurred roughly every 100,000 years – a phasing that is most likely linked to slight shifts in the eccentricity of Earth’s orbit (a larger or smaller ellipse) around the Sun.

But it is recognised from an alternative record of past climate, which has been deciphered from ocean sediments, that deeper back in time the ice age cycle was much shorter – at about every 41,000 years.

That is a period probably dominated by the way the Earth tilts back and forth on its axis. But why the switch occurred, no-one is really sure. The new Beyond Epica core may contain some clues if its ices can extend the climate narrative back to 1.5 million years ago.

“We believe this ice core will give us information on the climate of the past and on the greenhouse gases that were in the atmosphere during the Mid-Pleistocene Transition (MPT), which happened between 900,000 and 1.2 million years ago,” said team-leader Carlo Barbante, the director of the Institute of Polar Sciences of the National Research Council of Italy.

“During this transition, climate periodicity between ice ages changed from 41,000 to 100,000 years: the reason why this happened is the mystery we hope to solve.” Beyond EPICA camp was set up during the 2019/20 Antarctic summer season.

To achieve an 800,000-year record, the original EPICA project drilled to a depth of 2,774m. The bedrock at Little Dome C is just over 2,800m down. The extra 700,000 years being sought by the new project should be in the additional metres of layered ice.

“We already have the 800,000 years of ice, so much of the first few years of drilling will simply be a repeat of ice we already have,” explained Robert Mulvaney from the British Antarctic Survey.

“In practice, with many new PhD students coming online, and new groups getting involved, and new analytical techniques always being developed, we will make good use of the ice younger than 800,000 years.

“We will also use the younger ice to ensure our techniques are working well by the time we get to the deep ice, where we only get one chance to get all the analyses right,” he told BBC News.

Beyond EPICA is funded by the European Union. UK scientists are allowed to participate because the money comes from a period when Britain was still a part of the 27-member-state bloc.

It’s easy to be brand loyal to the moon. We’ve only got the one, after all, unlike Jupiter and Saturn, where you’d have dozens to choose from. Here, it’s luna or nada. Or not. The fact is, there’s another sorta, kinda moon in a sorta, kinda orbit around Earth that was discovered only in 2016. And according to a new study in Nature, we may at last know how it was formed.

The quasi-moon—named Kamo’oalewa, after a Hawaiian word that refers to a moving celestial object—is not much to speak of, measuring less than 50 m (164 ft) across. It circles the Earth in a repeating corkscrew-like trajectory that brings it no closer than 40 to 100 times the 384,000 km (239,000 mi.) distance of our more familiar moon. Its odd flight path is caused by the competing gravitational pulls of the Earth and the sun, which continually bend and torque the moonlet’s motions, preventing it from achieving a more conventional orbit.

“It’s primarily influenced just by the sun’s gravity, but this pattern shows up because it’s also—but not quite—on an Earth-like orbit. So it’s this sort of odd dance,” says graduate student Ben Sharkey of the Lunar and Planetary Laboratory at the University of Arizona, the lead author of the paper.

None of this means that Kamo’oalewa has to have especially exotic origins. The solar system is littered with asteroids, some of which are captured by the gravity of other planets and become more conventional—if fragmentary—moons. Others don’t orbit other planets in the common way but fall into line in front of them or behind them and pace them in their orbits around the sun, like the flocks of so-called Trojan asteroids that precede and trail Jupiter.

Either way, Kamo’oalewa was bound to get attention because its composition posed a stubborn mystery. Asteroids tend to reflect brightly in certain infrared frequencies, but Kamo’oalewa just doesn’t. It’s dimmer somehow—clearly made of different stuff, which suggests a different origin.

To investigate the mystery, Sharkey, under the guidance of his PhD adviser, planetary scientist Vishnu Reddy, first turned to a NASA-run telescope in Hawaii routinely used for studying Earth-vicinity asteroids. But even through the usually reliable instrument, the infrared signature seemed too faint. Instead they switched to a University of Arizona-run monocular telescope that, as Sharkey says, could “squeeze every last ounce of photons out of that object.”

That produced better, clearer results, but still they were incomplete. The rock was made of common silicates like other asteroids, but they were common only in their general composition, not in their infrared signature, which remained stubbornly off.

At last, the answer suggested itself. If Kamo’oalewa was behaving like a sort of quasi-moon, perhaps it was an artifact of the actual moon. Earlier in Sharkey’s PhD program, one of his advisers published a paper on lunar samples brought back by the Apollo 14 mission in 1971. When Sharkey compared the data he was getting in his telescope with what the earlier geologists came up with in the rock lab, the results matched perfectly. The kind of space-weathering lunar silicates undergo when they’re still on the surface of the moon precisely accounted for the differences in the infrared reflectivity between common asteroids and Kamo’oalewa.

“Visually, what you’re seeing is weathered silicate,” says Sharkey. “The eons of exposure to space environment and the micrometeorite impacts, it’s almost like a fingerprint and it’s hard to miss.”

How Kamo’oalewa shook free of our lunar companion is no mystery. The moon’s been getting bombarded by space rocks for billions of years, resulting in all manner of lunar debris getting ejected into space (nearly 500 bits of which have made it to the surface of the Earth as meteorites). Kamo’oalewa is one such piece of lunar rubble that spiraled away from the moon. But rather than landing on Earth or simply tumbling off into the void, it found itself a quasi-satellite in its own right.

“We see thousands of craters on the moon, so some of this lunar ejecta has to be sticking around in space,” says Sharkey. Kamo’oalewa won’t stick around all that long, as its current trajectory is not entirely stable. According to estimates from Sharkey and others, the object will remain an earthly companion for only about 300 more years—nothing at all on the cosmic clock—after which it will break free of its current gravitational chains and twirl off into the void. Originally a part of the moon, then a companion of Earth, it will spend the rest of its long life traveling on its own.

On November 19, stargazers can enjoy a partial lunar eclipse which will also be the last lunar eclipse of the year. This will also be the longest eclipse in 580 years.

On November 19, stargazers can enjoy a partial lunar eclipse which will also be the last lunar eclipse of the year. The last time such a lengthy partial eclipse occurred was on February 18, 1440, and the next time a similar one will occur on February 8, 2669.

A partial lunar eclipse occurs when the Earth comes between the Sun and the Moon, but not in a perfect line. A small part of the moon gets covered by the Earth’s shadow and we can see a reddish Moon. It is also called the frost moon or beaver moon. Full moons in November earned this name as this is the time of first snowfall and frost, and beavers start building their dams or traps.

The partial lunar eclipse will be visible from North America, South America, Eastern Asia, Australia, and the Pacific Region.

In India, a small part of Arunachal Pradesh and Assam will experience the partial eclipse, and those from Uttar Pradesh, Bihar, Jharkhand can see the end part of the penumbral eclipse. A penumbral lunar eclipse takes place when the Moon, Sun, and Earth are imperfectly aligned and the Moon moves through the outer part of Earth’s shadow called the penumbra.

Dr Debiprosad Duari, Director, Research & Academic at MP Birla Planetarium, Kolkata explains: “The partial eclipse will start around 12:48 IST and will end at 16:17 IST. The duration of the partial eclipse hence will be for 3hrs 28 minutes and 24 seconds, making it the longest eclipse of the 21st century and the longest in almost last 600 years.”

“The penumbral eclipse preceding and succeeding the umbral partial eclipse will begin at around 11:32 IST and end at 17:33 IST. At the maximum partial eclipse, at around 14:34 IST, 97% of the Moon will be covered by the Earth’s shadow and the Moon may appear to be blood red in colour, which happens when the red part of the sunlight passes through the Earth’s atmosphere get least deflected and falls on the Moon giving it a reddish tinge.”

The next total lunar eclipse will be on May 16, 2022, but it will not be visible from India. India will experience a total lunar eclipse on November 8, 2022.

Newswise — ITHACA, N.Y. – More than 99.9% of peer-reviewed scientific papers agree that climate change is mainly caused by humans, according to a new survey of 88,125 climate-related studies.

The research updates a similar 2013 paper revealing that 97% of studies published between 1991 and 2012 supported the idea that human activities are altering Earth’s climate. The current survey examines the literature published from 2012 to November 2020 to explore whether the consensus has changed.

“We are virtually certain that the consensus is well over 99% now and that it’s pretty much case closed for any meaningful public conversation about the reality of human-caused climate change,” said Mark Lynas, a visiting fellow at the Alliance for Science at Cornell University and the paper’s first author.

“It’s critical to acknowledge the principal role of greenhouse gas emissions so that we can rapidly mobilize new solutions, since we are already witnessing in real time the devastating impacts of climate-related disasters on businesses, people and the economy,” said Benjamin Houlton, Dean of the College of Agriculture and Life Sciences at Cornell and a co-author of the study, “Greater than 99% Consensus on Human Caused Climate Change in the Peer-Reviewed Scientific Literature,” which published Oct. 19 in the journal Environmental Research Letters.

In spite of such results, public opinion polls as well as opinions of politicians and public representatives point to false beliefs and claims that a significant debate still exists among scientists over the true cause of climate change. In 2016, the Pew Research Center found that only 27% of U.S. adults believe “almost all” scientists agreed climate change is due to human activity, according to the paper. A 2021 Gallup poll pointed to a deepening partisan divide in American politics on whether Earth’s rising observed temperatures since the Industrial Revolution were primarily caused by humans.

“To understand where a consensus exists, you have to be able to quantify it,” Lynas said. “That means surveying the literature in a coherent and non-arbitrary way in order to avoid trading cherry-picked papers, which is often how these arguments are carried out in the public sphere.”

In the study, the researchers began by examining a random sample of 3,000 studies from the dataset of 88,125 English-language climate papers published between 2012 and 2020. They found only four out of the 3,000 papers were skeptical of human-caused climate change. “We knew that [climate skeptical papers] were vanishingly small in terms of their occurrence, but we thought there still must be more in the 88,000,” Lynas said.

Co-author Simon Perry, a United Kingdom-based software engineer and volunteer at the Alliance for Science, created an algorithm that searched out keywords from papers the team knew were skeptical, such as “solar,” “cosmic rays” and “natural cycles.” The algorithm was applied to all 88,000-plus papers, and the program ordered them so the skeptical ones came higher in the order. They found many of these dissenting papers near the top, as expected, with diminishing returns further down the list. Overall, the search yielded 28 papers that were implicitly or explicitly skeptical, all published in minor journals.

If the 97% result from the 2013 study still left some doubt on scientific consensus on the human influence on climate, the current findings go even further to allay any uncertainty, Lynas said. “This pretty much should be the last word,” he said.

Support for the Alliance for Science is provided by the Bill and Melinda Gates Foundation.

Newswise — While analyzing some of the world’s oldest coloured gemstones, researchers from the University of Waterloo discovered carbon residue that was once ancient life, encased in a 2.5 billion-year-old ruby.

The research team, led by Chris Yakymchuk, professor of Earth and Environmental Sciences at Waterloo, set out to study the geology of rubies to better understand the conditions necessary for ruby formation. During this research in Greenland, which contains the oldest known deposits of rubies in the world, the team found a ruby sample that contained graphite, a mineral made of pure carbon. Analysis of this carbon indicates that it is a remnant of early life.

“The graphite inside this ruby is really unique. It’s the first time we’ve seen evidence of ancient life in ruby-bearing rocks,” says Yakymchuk. “The presence of graphite also gives us more clues to determine how rubies formed at this location, something that is impossible to do directly based on a ruby’s colour and chemical composition.”

The presence of the graphite allowed the researchers to analyze a property called isotopic composition of the carbon atoms, which measures the relative amounts of different carbon atoms. More than 98 per cent of all carbon atoms have a mass of 12 atomic mass units, but a few carbon atoms are heavier, with a mass of 13 or 14 atomic mass units.

“Living matter preferentially consists of the lighter carbon atoms because they take less energy to incorporate into cells,” said Yakymchuk. “Based on the increased amount of carbon-12 in this graphite, we concluded that the carbon atoms were once ancient life, most likely dead microorganisms such as cyanobacteria.”

The graphite is found in rocks older than 2.5 billion years ago, a time on the planet when oxygen was not abundant in the atmosphere, and life existed only in microorganisms and algae films.

During this study, Yakymchuk’s team discovered that this graphite not only links the gemstone to ancient life but was also likely necessary for this ruby to exist at all. The graphite changed the chemistry of the surrounding rocks to create favourable conditions for ruby growth. Without it, the team’s models showed that it would not have been possible to form rubies in this location.

The study, Corundum (ruby) growth during the final assembly of the Archean North Atlantic Craton, southern West Greenland, was recently published in Ore Geology Reviews. A companion study, The corundum conundrum: Constraining the compositions of fluids involved in ruby formation in metamorphic melanges of ultramafic and aluminous rocks, was published in the journal Chemical Geology in June.

Newswise — In 1973, a scientist stumbled upon a strange tree in the Amazon rainforest, unlike anything he’d ever seen. It was about 20 feet tall, with tiny orange fruits shaped like paper lanterns. He collected samples of the plant’s leaves and fruits, but all the scientists he showed them to wound up scratching their heads– not only were they unable to identify the plant as a species that had previously been described by scientists, but they couldn’t even declare it a new species, because they couldn’t tell what family it belonged to. But in a new study in the journal Taxon, scientists analyzed the plant’s DNA and determined where it belongs in the family tree of trees, finally giving it a name meaning “Mystery of Manu,” after the park in Peru it came from.

“When I first saw this little tree, while out on a forest trail leading from the field station, it was the fruit — looking like an orange-colored Chinese lantern and juicy when ripe with several seeds — that caught my attention,” says Robin Foster, the scientist who originally collected the mystery plant in Peru’s Manu National Park, a retired curator at Chicago’s Field Museum and now a researcher with the Smithsonian Tropical Research Institute. “I didn’t really think it was special, except for the fact that it had characteristics of plants in several different plant families, and didn’t fall neatly into any family.  Usually I can tell the family by a quick glance, but damned if I could place this one.”

Foster wasn’t the only one who couldn’t figure it out. Nancy Hensold, a botanist at the Field Museum, remembers him showing her a dried specimen of the plant more than 30 years ago. “I came to work at the Field Museum in 1990, and Robin showed me this plant. And I tried to get it identified using little fine technical characters like boiling up the ovaries of the flowers and taking pictures of the pollen, and after all that, we still didn’t know,” she recalls. “It really bugged me.”

The mystery plant sat in the Field Museum’s herbarium, a library of dried plant specimens, for years, but Hensold and her colleagues didn’t forget about it. “When you have a plant no one can put in a family, it can fall through the scientific cracks. I felt for it,” she says. The team eventually got a grant to study the plant, funded by the Field Museum’s Women’s Board, and the search was on.

The team attempted to analyze the plant’s DNA using the dried specimens, but when that didn’t work, they enlisted the help of Patricia Álvarez-Loayza, a scientist who works in the Manu National Park and has spent years monitoring the forest there, to find a fresh specimen of the plant. She did, and when the researchers back at the Field analyzed it in the museum’s Pritzker DNA Laboratory, they were shocked by what they found. “When my colleague Rick Ree sequenced it and told me what family it belonged to, I told him the sample must have been contaminated. I was like, no way, I just couldn’t believe it,” recalls Hensold.

The DNA analysis revealed that the mystery plant’s closest relatives were in the Picramniaceae family, which was a big deal to the botanists because it didn’t look anything like its closest relatives, at least at first glance. “L​​ooking closer at the structure of the tiny little flowers I realized, oh, it really has some similarities but given its overall characters, nobody would have put it in that family,” says Hensold. The researchers sent specimens to Wayt Thomas, a curator emeritus at The New York Botanical Garden and an expert in Picramniaceae. “When I opened the package and looked at the specimens, my first reaction was, ‘What the heck?’ These plants didn’t look like anything else in the family,” says Thomas, the lead author of the paper in Taxon. “So I decided to look more carefully–once I looked really carefully at the tiny, 2-3 milimeter long flowers, things fell into place.” With the DNA finally revealing what family the plant belonged to, the researchers were able to give it a formal scientific name, Aenigmanu alvareziae. The genus name, Aenigmanu, means “mystery of Manu,” while the species name is in honor of Patricia Álvarez-Loayza, who collected the first specimens used for the genetic analysis. (It’s worth noting that while Aenigmanu alvareziae is new to scientists, it has long been used by the Indigenous Machiguenga people.)

The researchers say that finally getting a scientific classification for Aenigmanu alvareziae could ultimately help protect the Amazon rainforest in the face of deforestation and climate change. “Plants are understudied in general. Especially tropical forest plants. Especially Amazon plants.  And especially plants in the upper Amazon. To understand the changes taking place in the tropics, to protect what remains, and to restore areas that have been wiped out, plants are the foundation for everything that lives there and the most important to study,” says Foster.  “Giving them unique names is the best way to organize information about them and call attention to them. A single rare species may not by itself be important to an ecosystem, but collectively they tell us what is going on out there.”

New scientific research conducted by archaeologists has uncovered what they believe are the oldest known human footprints in North America. Research done at the White Sands national park in New Mexico discovered the ancient footprints, with researchers estimating that the tracks were between 21,000 and 23,000 years old, reported Science.

The prints were buried in layers of soil in the national park, with scientists from the US Geological Survey analyzing seeds embedded in the tracks to calculate the age of the fossils. Researchers also determined that the dozen footprints found belonged to a variety of people, mostly children and teenagers. Previously, scientists had widely assumed that the earliest appearance of humans in the Americas was 11,000 to 13,000 years ago because of stone spears found throughout North America and associated with what is known as the Clovis culture.

“The evidence is very convincing and extremely exciting,” says Tom Higham, an archaeological scientist and radiocarbon-dating expert at the University of Vienna to Nature. “I am convinced that these footprints genuinely are of the age claimed.” The new research was conducted by experts from White Sands national park, the National Park Service, US Geological Survey, Bournemouth University, University of Arizona and Cornell University.

“The paper makes a very compelling case that these footprints are not only human, but they’re older than 20,000 years,” said Spencer Lucas, a palaeontologist at the New Mexico Museum of Natural History & Science in Albuquerque to Nature. “That’s a gamechanger.”

A new study has now pointed out that these changes in the Arctic region induced by anthropogenic global warming have disrupted a wind system called Stratospheric Polar Vortex (SPV). In the recent past, the Arctic region has warmed rapidly and studies have shown that the temperatures in the region have risen about twice as fast as global temperatures. This phenomenon is termed Arctic amplification and multiple factors including increased greenhouse gas emissions and atmospheric transport of heat to the region play important roles. Recently, researchers from India and Brazil noted that this Arctic warming was behind the heatwaves in India. The warming was found to have an impact on the frequency and intensity of heat waves. Though very counterintuitive, there have also been a few studies stating that this Arctic warming has propelled the cold winter spells in North America.

A new study has now pointed out that these changes in the Arctic region induced by anthropogenic global warming have disrupted a wind system called Stratospheric Polar Vortex (SPV). This stretching of SPV can lead to extreme cold events in parts of Asia and North America. The report published Friday in Science adds that this SPV disruption was behind the February 2021 Texas cold wave. “The SPV consists of strong westerly winds from 10km to 50km above the surface. It peaks at around 50 m/s on average near 50km and is strongest in mid-winter, however, on occasion it can weaken, and sometimes the winds reverse direction entirely,” explains one of the authors Prof. Chaim Garfinkel in an email to indianexpress.com. He is the Head of the Graduate Program in Atmospheric Science at Hebrew University, Israel. He adds that these stretching events almost certainly occurred before greenhouse gas emissions began increasing, but the current emissions are leading to an increase in the occurrence of these types of events.

Lead author Judah Cohen told theguardian.com: “When the polar vortex is nice and circular, that’s a sign all the cold air is bottled up over the Arctic…When it stretches like this, a piece of it goes into Asia and a piece of it goes towards eastern North America. So that’s what we’re seeing. And that was what happened with the Texas cold wave.” A reversal of the polar vortex is known to bring warm winter temperatures in Southern Asia. When asked if the disruption can have an effect on India, Dr Cohen told indianexpress.com that the polar vortex stretching events are associated with relatively cold temperatures in Central and East Asia but there are no strong signals in India. “If anything these events might slightly favour relatively mild temperatures,” he adds.

The team is currently studying the various dynamics of this disruption. “Our modelling work needs to be elaborated to explore stronger forcings that might occur by the end of the century,” adds Prof. Garfinkel. The team writes that by identifying the precursor pattern to these stretching events, we can extend the warning lead time of cold extremes in Asia, Canada, and the United States. “Preparing for only a decrease in severe winter weather can compound the human and economic cost when severe winter weather does occur,” concludes the report.

The Government of India have given approval for signing of a MoU between the Geological Survey of India (GSI) and Florida International University, the US, for cooperation in the field of geology.

Chaired by Prime Minister Narendra Modi, the Cabinet gave its approval for signing the MoU between the GSI, under the Ministry of Mines, and the varsity’s board of trustees on behalf of its Department of Earth and Environment, a government statement said. The identified area of cooperation between the two participants would include development of geological knowledge, research regarding geologic and tectonic environment of post collisions magmatism in India-Asia collisional margin, geologic history and tectonics of the Eastern Himalayan Syntaxis and developing cooperative projects in the fields of regional geological, geochemical, petrological and multi-isotopic studies related to the evolution of post collisional magmatic belts.

The MoU will provide an institutional mechanism between Geological Survey of India (GSI) and the Florida International University (FIU) on cooperation in the field of Geology.The objectives of the MoU are to understand the geologic and tectonic environment of the generation and emplacement of post-collisional magmatism in India-Asia Collision margin in particular and to construct a model of post-collisional magma genesis in continental collision zones in general and to construct the geologic and tectonics of the Eastern Himalayan Syntaxis.

The identified area of cooperation between the two Participants will be as follows:

• Development of the geological knowledge, research regarding geologic and tectonic environment of post collisions magmatism in India-Asia collisional margin, geologic history and tectonics of the Eastern Himalayan Syntaxis.
• Developing cooperative projects in the fields of regional geological, geochemical, petrological and multi-isotopic studies related to the evolution of post collisional magmatic belts.

Heatwaves and the heavy rains that cause flooding have become more intense and more frequent since the 1950s in most parts of the world, and climate change is now affecting all inhabited regions of the planet. Drought is increasing in many places and it is more than 66% likely that numbers of major hurricanes and typhoons have risen since the 1970s.

“If there was still a need for a proof that climate changes is caused by human activities, then this is the report that provides it,” said Prof Corinne Le Quéré of the University of East Anglia. And the consequences of humanity’s massive act of atmospheric interference are now clear: what is hot today will become hotter tomorrow; extreme floods will become more frequent, wildfires more dangerous and deadly droughts more widespread. In short, things can only get worse.

“Our future climate could well become some kind of hell on Earth,” said Prof Tim Palmer, of Oxford University. Or, as Prof Dave Reay, executive director of Edinburgh University’s Climate Change Institute, put it: “This is not just another scientific report. This is hell and high water writ large.”

Certainly the numbers outlined in the report were stark and strikingly emphatic in comparison with past, far more cautious, IPCC offerings. As it makes clear, humans have pumped around 2,400bn tonnes of carbon dioxide into the atmosphere since 1850, creating concentrations of the gas that have not been seen on Earth in the last 2 million years.

And the consequences of humanity’s massive act of atmospheric interference are now clear: what is hot today will become hotter tomorrow; extreme floods will become more frequent, wildfires more dangerous and deadly droughts more widespread. In short, things can only get worse.

Indeed, by the end of the century they could become threatening to civilisation if emissions are allowed to continue at their present rate. “That might seem like a long way away but there are millions of children already born who should be alive well into the 22nd century,” added Prof Jonathan Bamber of Bristol University, another report author.

In fact, they could become utterly catastrophic with the occurrence of world-changing events – such as continent-wide forest die-backs or collapsing Antarctic ice sheets, says Prof Andrew Watson of Edinburgh University. “The IPCC report gives a comprehensive update on the knowns of climate change, and that makes for grim reading. But it also makes the point that climate models don’t include ‘low probability-high impact’ events, such as drastic changes in ocean circulation, that also become more likely the more the climate is changed. These ‘known unknowns’ are scarier still.”

The new IPCC report is certainly a very different, uncompromising document compared with previous versions, as meteorologist Keith Shine of Reading University pointed out. “I was heavily involved in IPCC’s first assessment report back in 1990. We weren’t even sure then that observed climate change was due to human activity. The IPCC now says the evidence is ‘unequivocal’. That means there is no hiding place for policymakers.”

A crucial system of currents in the Atlantic Ocean that helps control temperatures in the Northern Hemisphere and has implications for the entire planet’s weather systems is showing signs of instability due to human-made climate change, scientists say.  Its collapse would have dire consequences for our weather and life on Earth.

The Atlantic Meridional Overturning Circulation (AMOC) — which the Gulf Stream is a major part of — helps maintain the energy balance in the Atlantic Ocean. It is often described as a “conveyor belt” that takes warm surface water from the tropics and distributes it to the north Atlantic. The colder, saltier water then sinks and flows south.

A study, published Thursday in Nature and Climate Change, warned of “an almost complete loss of stability of the AMOC over the course of the last century. Researchers say it could be close to a collapse from a strong circulation to a weak circulation, though the threshold for such a collapse is still uncertain.

Scientists have warned for years that the circulation is weakening. Heavy rain and melting ice sheets are making the water in the North Atlantic Ocean less salty, which makes it lighter and less likely to sink. If the water in this region becomes too light, the entire circulation could be disrupted.

Global weather patterns are critically linked to the circulation and its transport of heat and nutrients around the planet. A collapse of this system would result in significant and abrupt changes, including fast sea level rise, more extreme winters in Western Europe and disruptions to monsoon systems in the tropics.

It could also have a cascading effect and destabilize other components of the Earth’s climate system, including the Antarctic ice sheet and the Amazon rainforest.

This scenario was the premise for the 2004 climate science fiction film “The Day After Tomorrow,” in which a series of extreme weather disasters strike after climate change caused the AMOC to collapse.

The circulation is weaker than it has been in around 1,000 years, scientists had previously said, but they did not know whether it had actually been destabilized or undergoing natural changes. This week’s study used eight datasets looking at surface temperatures and salinity in the North Atlantic over a period of 150 years, and found global warming was driving the destabilization.

“The difference is crucial,” the study’s author, Niklas Boers from the Potsdam Institute for Climate Impact Research, told CNN in an email.

“Imagine a chair, which can be either shifted (with all four legs remaining on the ground) or tilted. Both change the position of the chair (corresponding to the change in mean AMOC strength), but in the first case the stability of the chair won’t be affected, while in the latter case there exists a critical point. If we tilt the chair just slightly further, it will fall down. My results suggest that what is happening to the AMOC is more likely to be a tilting than only a shifting, so the AMOC has moved toward the critical threshold at which it may collapse,” he said.

Boers added that he himself was surprised by his findings that the AMOC had been destabilized and was “moving toward its critical threshold, at which it could abruptly collapse.”

A collapse of the circulation would mean significant cooling in Europe, Beors said, “but maybe more concerning is the effect of an AMOC collapse on the tropical monsoon systems of South America, Western Africa, and India; especially in Western Africa, an AMOC collapse could lead to permanent drought conditions.”

Boers recognizes in his study that he and other scientists still don’t know if and when the current might collapse, but he called on the world to reduce greenhouse gas emissions “as much and as quickly as possible.”

“Every gram of extra greenhouse gas in the atmosphere will increase to the probability of an AMOC collapse in the future, so emitting as little as possible, both on individual but of course also on collective and international level, is the key.”

The study comes ahead of a major report by the UN’s International Panel on Climate Change on Monday, which has been years in the making and is expected to provide the most conclusive look yet at the extent of human-made climate change. It will also likely paint a picture of what the future could look like, depending on what action the world takes to reduce its greenhouse gas emissions.

Newswise — New research led by the University of Bristol demonstrates that a decline in the concentration of atmospheric CO2 played a major role in driving Earth’s climate from a warm greenhouse into a cold icehouse world around 34 million years ago. This transition could be partly reversed in the next centuries due to the anthropogenic rise in CO2.

Between 40 and 34 million years ago, Earth’s climate underwent a major climatic transition. Before 40 million years ago, during the Eocene, Antarctica was covered by lush forests, but by 34 million years ago, in the Oligocene, these forests had been replaced by thick continental ice sheets, as we know Antarctica today. The main driver of this greenhouse to icehouse transition is widely debated, and little information is available about how climate changed on land. An international team led by Dr Vittoria Lauretano and Dr David Naafs at the University of Bristol used molecular fossils preserved in ancient coals to reconstruct land temperature across this transition.

The team used a new approach based on the distribution of bacterial lipids preserved in ancient wetland deposits. It was developed as part of the ERC-funded project, The Greenhouse Earth System (TGRES), which also funded this study. The TGRES PI and paper co-author Rich Pancost, from the University’s School of Chemistry, explained: ‘These compounds originally comprised the cell membranes of bacteria living in ancient wetlands, with their structures changing slightly to help the bacteria adapt to changing temperature and acidity. Those compounds can then be preserved for tens of millions of years, allowing us to reconstruct those ancient environmental conditions.’

To reconstruct temperature change across the greenhouse to icehouse transition, the team applied their new approach to coal deposits from the southeast Australian Gippsland Basin. These remarkable deposits span over 10 million years of Earth history and have been extensively characterised by collaborators on the study from the University of Melbourne, Dr. Vera Korasidis and Prof. Malcolm Wallace.

The new data show that land temperatures cooled alongside the ocean’s and by a similar magnitude of about 3C. To explore causes of that temperature decline, the team conducted climate model simulations, Crucially, only simulations that included a decline in atmospheric CO2 could reproduce a cooling consistent with the temperature data reconstructed from the coals.

These results provide further evidence that atmospheric CO2 plays a crucial role in driving Earth’s climate, including the formation of the Antarctic ice sheet.

Heat waves. Floods. Wildfires. It’s been a destructive summer so far, and forecasts for droughts, fires and hurricanes are looking downright bleak.

We know that climate change is to blame. But how exactly is global warming driving dangerous weather?

Lauren Sommer and Rebecca Hersher from NPR’s climate team broke down the details in a conversation with Morning Edition’s Noel King.

The country is experiencing yet another heat wave this week. Is it just us or is this summer unusual?

It’s not just our memories — this past June was the hottest June recorded in the U.S. in more than a century, about four degrees hotter on average. Heat waves (like in the Pacific Northwest) can be deadly, and many cities are just realizing now how underprepared they are to deal with them.

What’s the connection between these extreme heat events and climate change?

There’s been about two degrees Fahrenheit of warming so far worldwide. The number sounds small, but it’s enough to “profoundly shift the statistics of extreme heat events,” according to Dr. Radley Horton, a climate scientist at Columbia University. He says these “dangerous thresholds of really high temperature and high humidity” could potentially happen twice as often as they have in the past.

What does this mean for wildfires?

About 95% of the West is in drought right now, and there’s a clear cycle where heat dries out land and vegetation. So when wildfires do happen, they burn hotter and even create their own weather systems in which huge pyrocumulus clouds can generate lightning strike — in turn causing even more fires.

What does a hotter Earth have to do with flash flooding?

It’s been a wild few weeks for flash flood disasters, from Central China to western Europe to Mumbai to Arizona. These fast-moving waters have killed hundreds of people, but they’re not a surprise to climate scientists, who have been sounding the alarms for years.

Even though these floods happened around their world, their root cause was the same: extreme rain. And it’s getting more common as the Earth gets warmer (hot air + hot water = more moisture in the air).

Plus, as the planet heats up, some climate models show winds in the upper atmosphere slowing down in certain places, which would mean that extreme weather would linger there longer.

Scientists are working hard to predict how common these disasters will be in the years to come. After all, lives are on the line.

Astronomers have discovered the largest known comet, and it’s about a thousand times more massive than others.  Comet Bernardinelli-Bernstein, so named because it was found by University of Pennsylvania department of physics and astronomygraduate student Pedro Bernardinelli and Professor Gary Bernstein, is between 62 to 124 miles (100 to 200 kilometers) across. The team announced the discovery in June. This unusual comet will make itsclosest approach to our sun in 2031, but you’ll likely need a large amateur telescope to see it.  The giant comet, also known as C/2014 UN271, is from the outskirts of our solar system and has been making its way toward our sun for millions of years. This is also the most distant comet to be discovered on its inbound journey, which will provide scientists a chance to observe and study it for years to come.

Comet Bernardinelli-Bernstein was found in six years of data collected by the Dark Energy Camera, which is located on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile. The data collected by this camera feeds into The Dark Energy Survey, a collaboration of more than 400 scientists across seven countries and 25 institutions. The camera, also known as DECam, is helping to map 300 million galaxies across the night sky — but it also captures glimpses of comets and trans-Neptuinan objects, or icy celestial bodies that reside along the outskirts of the solar system, beyond Neptune’s orbit.

Bernardinelli and Bernstein used algorithms at the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign to identify trans-Neptunian objects. During their work, the astronomers traced 32 detections to one object. Comets are icy relics that were kicked out of the solar system when the giant planets formed and migrated to their current configurations. As comets approach our sun during their orbits, their ices evaporate, creating their signature appearance.

Comets include a nucleus, or the solid “dirty snowball” at its center. Comas are the gaseous clouds that form around the nucleus as the comet’s ices evaporate. The evaporating gas and dust is pushed behind the comet as well, creating two tails illuminated by sunlight. These tails can be hundreds or even millions of miles in length. Images of the object taken between 2014 and 2018 did not show a cometary tail. But within the past three years, the object grew a tail, which officially makes it Comet Bernardinelli-Bernstein.

Observations made using the Las Cumbres Observatory network of telescopes around the globe helped confirm the status of the active comet. “Since we’re a team based all around the world, it just happened that it was my afternoon, while the other folks were asleep. The first image had the comet obscured by a satellite streak, and my heart sank. But then the others were clear enough and gosh: there it was, definitely a beautiful little fuzzy dot, not at all crisp like its neighbouring stars!” said Michele Bannister, astronomer at the University of Canterbury in New Zealand, in a statement.

The comet’s journey started over 3.7 trillion miles (6 trillion kilometers) away from the sun, or 40,000 astronomical units. The distance between Earth and the sun is one astronomical unit. For reference, Pluto is 39 astronomical units from the sun. The comet came from the OortCloud of objects, an isolated group of icy objects that are more distant than anything else in our solar system. Scientists believe this is where comets come from, but they have never actually observed an object within the OortCloud.

The OortCloud is located between 2,000 and 100,000 astronomical units from the sun. Eventually, NASA spacecraft like Voyager 1 and 2, as well as New Horizons will reach the OortCloud. But by the time they do, their power sources will have been dead for centuries. Comet Bernardinelli-Bernstein is currently about 1.8 billion miles (3 billion kilometers) away — about the distance of Uranus from the sun– and at its closest point in 2031, it will be just a bit more than Saturn’s distance to the sun.

“We have the privilege of having discovered perhaps the largest comet ever seen — or at least larger than any well-studied one — and caught it early enough for people to watch it evolve as it approaches and warms up,” Bernstein said in a statement. “It has not visited the planets in more than 3 million years.” This unusual opportunity to study an inbound comet will allow astronomers a chance to better understand the origin and composition of the comet. It may be just one of many giant comets originatingin the OortCloud.

Biologists from the Central University of Punjab have discovered a new species of moss in Continental Antarctica. The species has been named Bryumbharatiensis after one of the remotest Indian research stations in the desert continent of Antarctica. Coincidentally, the name also pays tribute to the Hindu Deity Bharati, who is the Goddess of learning. Presenting our discovery of Bryumbharatiensis, a new species of moss from Antarctica named after Goddess Saraswati (Bharati)! BBC featured a detailed story on the discovery. @narendramodi@PMOIndia@EduMinOfIndiahttps://t.co/Igbqkf53jW — Felix Bast (@ExaltFibs) July 12, 2021

The plant was first discovered growing on some rocks near the research station by Dr. Felix Bast, a polar and marine biologist who heads the Department of Botany in the Central University of Punjab. He was part of the Indian Antarctic Expedition 2016-17. With the rising earth temperature, Antarctica has been fast losing large amounts of its ice cover. With areas that were once perennially frozen now slowly being thawed and melting away for the first time in millions of years, patches of green have appeared on what was once a frigid wasteland. Thus, increasing the likelihood of discovering new species of plants and microbes that were previously frozen deep under the thick ice sheets. So, in 2017, a team of biologists from Punjab University had gone to the Indian research station as a part of a six month long expedition, specifically to collect samples and examine the plant life.

After it was first discovered, samples were brought back by Dr. Bast to the university, where it was extensively researched upon by a group researchers including Wahid Ul Rahman, a fourth-year PhD student at CUPB and Kirti Gupta, the head of the Botany Department at DAV College in Bathinda. The identification and classifying of new species is a laborious process and it took over five years of careful study of the DNA sequencing of the plant, for scientists to confirm the existence of Bryumbharatiensis. A paper was then published in the journal of Asia-Pacific Biodiversity – a leading international journal by the team, describing the discovery of the moss.

It is yet unknown how the moss survived the rock and ice that makes up close to 99 percent of the Antarctic landmass. Plants require amongst other things, sunlight, water, and several minerals including nitrogen, phosphorus and potassium to survive. It was discovered that this moss grows primarily in areas inhabited by large numbers of penguins. Penguin excrement is an excellent source of nitrogen and it has been theorized that it is used by the moss as a form of manure.

Antarctica being at the very bottom of the Southern Hemisphere faces an interesting phenomenon where the entire continent experiences six whole months of continuous sunlight during the summers and the six months of winter are spent in constant darkness. Scientists think that the moss dries up, not entirely unlike a seed and remains dormant during the winter months. And when the sun comes out in September it germinates by absorbing the water from the melted snow. Over a hundred different moss species have been previously been found in the Antarctic. This particular moss is native to Eastern Antarctica and monumentally, the first and only plant species discovered in last four decades of the Indian Antarctic Mission.

The sequoia tree slab is an invitation to begin thinking about a vast timescale that includes everything from fossils of armored amoebas to the great Tyrannosaurus rex. PaleobotanistScott Wing hopes that he’s wrong. Even though he carefully counted each ring in an immense, ancient slab of sequoia, the scientist notes that there’s always a little bit of uncertainty in the count. Wing came up with about 260, but, he says, it’s likely a young visitor may one day write him saying: “You’re off by three.” And that would a good thing, Wing says, because it’d be another moment in our ongoing conversation about time.

The shining slab, preserved and polished, is the keystone to consideration of time and our place in it in the “Hall of Fossils—Deep Time” exhibition at the Smithsonian’s National Museum of Natural History. The fossil greets visitors at one of the show’s entrances and just like the physical tree, what the sequoia represents has layers.

Each yearly delineation on the sequoia’s surface is a small part of a far grander story that ties together all of life on Earth. Scientists know this as Deep Time. It’s not just on the scale of centuries, millennia, epochs, or periods, but the ongoing flow that goes back to the origins of our universe, the formation of the Earth, and the evolution of all life, up through this present moment. It’s the backdrop for everything we see around us today, and it can be understood through techniques as different as absolute dating of radioactive minerals and counting the rings of a prehistoric tree. Each part informs the whole.

In decades past, the Smithsonian’s fossil halls were known for the ancient celebrities they contained. There was the dinosaur hall, and the fossil mammal hall, surrounded by the remains of other extinct organisms. But now all of those lost species have been brought together into an integrated story of dynamic and dramatic change. The sequoia is an invitation to begin thinking about how we fit into the vast timescale that includes everything from fossils of armored amoebas called forams to the great Tyrannosaurus rex.

Exactly how the sequoia fossil came to be at the Smithsonian is not entirely clear. The piece was gifted to the museum long ago, “before my time,” Wing says. Still, enough of the tree’s backstory is known to identify it as a massive tree that grew in what’s now central Oregon about 16 million years ago. This tree was once a long-lived part of a true forest primeval. There are fossils both far older and more recent in the recesses of the Deep Time displays. But what makes the sequoia a fitting introduction to the story that unfolds behind it, Wing says, is that the rings offer different ways to think about time. Given that the sequoia grew seasonally, each ring marks the passage of another year, and visitors can look at the approximately 260 delineations and think about what such a time span represents.

Wing says, people can play the classic game of comparing the tree’s life to a human lifespan. If a long human life is about 80 years, Wing says, then people can count 80, 160, and 240 years, meaning the sequoia grew and thrived over the course of approximately three human lifespans—but during a time when our own ancestors resembled gibbon-like apes. Time is not something that life simply passes through. In everything—from the rings of an ancient tree to the very bones in your body—time is part of life.

The record of that life—and even afterlife—lies between the lines. “You can really see that this tree was growing like crazy in its initial one hundred years or so,” Wing says, with the growth slowing as the tree became larger. And despite the slab’s ancient age, some of the original organic material is still locked inside. “This tree was alive, photosynthesizing, pulling carbon dioxide out of the atmosphere, turning it into sugars and into lignin and cellulose to make cell walls,” Wing says. After the tree perished, water carrying silica and other minerals coated the log to preserve the wood and protect some of those organic components inside. “The carbon atoms that came out of the atmosphere 16 million years ago are locked in this chunk of glass.”

And so visitors are drawn even further back, not only through the life of the tree itself but through a time span so great that it’s difficult to comprehend. A little back of the envelope math indicates that the tree represents about three human lifetimes, but that the time between when the sequoia was alive and the present could contain about 200,000 human lifetimes. The numbers grow so large that they begin to become abstract. The sequoia is a way to touch that history and start to feel the pull of all those ages past, and what they mean to us. “Time is so vast,” Wing says, “that this giant slab of a tree is just scratching the surface.”

(Riley Black is a freelance science writer specializing in evolution, paleontology and natural history who blogs regularly for Scientific American.)

Newswise — According to the World Health Organization, about 785 million people around the world lack a clean source of drinking water. Despite the vast amount of water on Earth, most of it is seawater and freshwater accounts for only about 2.5% of the total. One of the ways to provide clean drinking water is to desalinate seawater. The Korea Institute of Civil Engineering and Building Technology (KICT) has announced the development of a stable performance electrospun nanofiber membrane to turn seawater into drinking water by membrane distillation process. Membrane wetting is the most challenging issue in membrane distillation. If a membrane exhibits wetting during membrane distillation operation, the membrane must be replaced. Progressive membrane wetting has been especially observed for long-term operations. If a membrane gets fully wetted, the membrane leads to inefficient membrane distillation performance, as the feed flow through the membrane leading to low-quality permeate.

A research team in KICT, led by Dr. Yunchul Woo, has developed co-axial electrospun nanofiber membranes fabricated by an alternative nano-technology, which is electrospinning. This new desalination technology shows it has the potential to help solve the world’s freshwater shortage. The developed technology can prevent wetting issues and also improve the long-term stability in membrane distillation process. A three-dimensional hierarchical structure should be formed by the nanofibers in the membranes for higher surface roughness and hence better hydrophobicity.

The co-axial electrospinning technique is one of the most favorable and simple options to fabricate membranes with three-dimensional hierarchical structures. Dr. Woo’s research team used poly(vinylidene fluoride-co-hexafluoropropylene) as the core and silica aerogel mixed with a low concentration of the polymer as the sheath to produce a co-axial composite membrane and obtain a superhydrophobic membrane surface. In fact, silica aerogel exhibited a much lower thermal conductivity compared with that of conventional polymers, which led to increased water vapor flux during the membrane distillation process due to a reduction of conductive heat losses.

Most of the studies using electrospun nanofiber membranes in membrane distillation applications operated for less than 50 hours although they exhibited a high water vapor flux performance. On the contrary, Dr. Woo’s research team applied the membrane distillation process using the fabricated co-axial electrospun nanofiber membrane for 30 days, which is 1 month.

The co-axial electrospun nanofiber membrane performed a 99.99% salt rejection for 1 month. Based on the results, the membrane operated well without wetting and fouling issues, due to its low sliding angle and thermal conductivity properties. Temperature polarization is one of the significant drawbacks in membrane distillation. It can decrease water vapor flux performance during membrane distillation operation due to conductive heat losses. The membrane is suitable for long-term membrane distillation applications as it possesses several important characteristics such as, low sliding angle, low thermal conductivity, avoiding temperature polarization, and reduced wetting and fouling problems whilst maintaining super-saturated high water vapor flux performance.

Dr. Woo’s research team noted that it is more important to have a stable process than a high water vapor flux performance in a commercially available membrane distillation process. Dr. Woo said that “the co-axial electrospun nanofiber membrane have strong potential for the treatment of seawater solutions without suffering from wetting issues and may be the appropriate membrane for pilot-scale and real-scale membrane distillation applications.”

The Korea Institute of Civil Engineering and Building Technology (KICT) is a government sponsored research institute established to contribute to the development of Korea’s construction industry and national economic growth by developing source and practical technology in the fields of construction and national land management. This research was supported by an internal grant (20200543-001) from the KICT, Republic of Korea. The outcomes of this project were published in the international journal, Journal of Membrane Science, a renowned international journal in the polymer science field (IF: 7.183 and Rank #3 of the JCR category) in April 2021.

Newswise — Our universe is expanding, but our two main ways to measure how fast this expansion is happening  have resulted in different answers. For the past decade, astrophysicists have been gradually dividing into two camps: one that believes that the difference is significant, and another that thinks it could be due to errors in measurement. If it turns out that errors are causing the mismatch, that would confirm our basic model of how the universe works. The other possibility presents a thread that, when pulled, would suggest some fundamental missing new physics is needed to stitch it back together. For several years, each new piece of evidence from telescopes has seesawed the argument back and forth, giving rise to what has been called the ‘Hubble tension.’

Wendy Freedman, a renowned astronomer and the John and Marion Sullivan University Professor in Astronomy and Astrophysics at the University of Chicago, made some of the original measurements of the expansion rate of the universe that resulted in a higher value of the Hubble constant. But in a new review paper accepted to the Astrophysical Journal, Freedman gives an overview of the most recent observations. Her conclusion: the latest observations are beginning to close the gap.   That is, there may not be a conflict after all, and our standard model of the universe does not need to be significantly modified.

Universal questions

The rate at which the universe is expanding is called the Hubble constant, named for UChicago alum Edwin Hubble, SB 1910, PhD 1917, who is credited with discovering the expansion of the universe in 1929. Scientists want to pin down this rate precisely, because the Hubble constant is tied to the age of the universe and how it evolved over time. A substantial wrinkle emerged in the past decade when results from the two main measurement methods began to diverge. But scientists are still debating the significance of the mismatch.

One way to measure the Hubble constant is by looking at very faint light left over from the Big Bang, called the cosmic microwave background. This has been done both in space and on the  ground with facilities like the UChicago-led South Pole Telescope. Scientists can feed these observations into their ‘standard model’ of the early universe and run it forward in time to predict what the Hubble constant should be today; they get an answer of 67.4 kilometers per second per megaparsec.

The other method is to look at stars and galaxies in the nearby universe, and measure their distances and how fast they are moving away from us. Freedman has been a leading expert on this method for many decades; in 2001, her team made one of the landmark measurements using the Hubble Space Telescope to image stars called Cepheids. The value they found was 72.  Freedman has continued to measure Cepheids in the years since, reviewing more telescope data each time; however, in 2019, she and her colleagues published an answer based on an entirely different method using stars called red giants. The idea was to cross-check the Cepheids with an independent method.

Red giants are very large and luminous stars that always reach the same peak brightness before rapidly fading. If scientists can accurately measure the actual, or intrinsic, peak brightness of the red giants, they can then measure the distances to their host galaxies, an essential but difficult part of the equation. The key question is how accurate  those measurements are. The first version of this calculation in 2019 used a single, very nearby galaxy to calibrate the red giant stars’ luminosities. Over the past two years, Freedman and her collaborators have run the numbers for several different galaxies and star populations. “There are now four independent ways of calibrating the red giant luminosities, and they agree to within 1% of each other,” said Freedman. “That indicates to us this is a really good way of measuring the distance.”

“I really wanted to look carefully at both the Cepheids and red giants. I know their strengths and weaknesses well,” said Freedman. “I have come to the conclusion that that we do not require fundamental new physics to explain the differences in the local and distant expansion rates. The new red giant data show that they are consistent.”  University of Chicago graduate student Taylor Hoyt, who has been making measurements of the red giant stars in the anchor galaxies, added, “We keep measuring and testing the red giant branch stars in different ways, and they keep exceeding our expectations.”

The value of the Hubble constant Freedman’s team gets from the red giants is 69.8 km/s/Mpc—virtually the same as the value derived from the cosmic microwave background experiment. “No new physics is required,” said Freedman.The calculations using Cepheid stars still give higher numbers, but according to Freedman’s analysis, the difference may not be troubling. “The Cepheid stars have always been a little noisier and a little more complicated to fully understand; they are young stars in the active star-forming regions of galaxies, and that means there’s potential for things like dust or contamination from other stars to throw off your measurements,” she explained. To her mind, the conflict can be resolved with better data.

Kicking the tires

Next year, when the James Webb Space Telescope is expected to launch, scientists will begin to collect those new observations. Freedman and collaborators have already been awarded time on the telescope for a major program to make more measurements of both Cepheid and red giant stars. “The Webb will give us higher sensitivity and resolution, and the data will get better really, really soon,” she said. But in the meantime, she wanted to take a careful look at the existing data, and what she found was that much of it actually agrees. “That’s the way science proceeds,” Freedman said. “You kick the tires to see if something deflates, and so far, no flat tires.”

Some scientists who have been rooting for a fundamental mismatch might be disappointed. But for Freedman, either answer is exciting.  “There is still some room for new physics, but even if there isn’t, it would show that the standard model we have is basically correct, which is also a profound conclusion to come to,” she said. “That’s the interesting thing about science: We don’t know the answers in advance. We’re learning as we go. It is a really exciting time to be in the field.”

On Jan. 5, 2020, astrophysicists heard a chirp from a distant part of the cosmos, some 900 million light-years away. The fleeting sound was unlike any they’d heard before and was caused by a great ripple in space-time — a gravitational wave — that spread out across the universe from over 900 million light-years away, washing over the Earth and pinging detectors. Chirp.  Then, 10 days later, they heard another, similar sound. A cosmic twin. Gravitational waves had once again pinged Earth’s detectors. Chirp.

After careful analysis, the two signals have been identified as emanating from extreme, never-before-seen events in deep space: the collision between a black hole and a neutron star. The pair of collisions (or, less poetically, “mergers”) are detailed in a new study published in the Astrophysical Journal Letters on Tuesday, featuring over 1,000 scientists from the LIGO/Virgo and KAGRA collaborations, a multinational effort to hunt for gravitational waves. The two newly described events are named GW200105 and GW200115, for the dates they were discovered, and provide the first definitive evidence of an elusive merger.

Prior to the dual detection, astronomers had only found black holes merging with black holes and neutron stars merging with neutron stars.”We’ve been waiting and expecting, at some stage, to detect a system with one of each,” said Susan Scott, an astrophysicist at Australian National University and a member of OzGrav and the LIGO collaboration. Now they have. Over the last two years, there had been suggestions that a collision between a neutron star and a black hole may have been spotted — but one of the objects appeared a little unusual. It was too big to be a neutron star and too small to be a black hole. The unknown object remains a mystery, which means GW200105 and GW200115 will go down in history.

“These are the first really confident detections of the merger of a neutron star with a black hole,” adds Rory Smith, an astrophysicist at Monash University in Australia and a member of the LIGO collaboration. There is huge excitement among scientists with the first confirmed detection of a neutron star-black hole (NS-BH) collision being reported. This ground breaking discovery of gravitational waves from a pair of NS-BH mergers was published in the Astrophysical Journal Letters on Tuesday. Professor SomakRaychaudhury, Director of Inter University Centre for Astronomy and Astrophysics (IUCAA), told the media that the development was expected for a long time but was not confirmed. A new analysis was done to reconfirm this discovery which has now been published in the international journal, said Raychoudhury.

Until now, the LIGO-Virgo collaboration (LVC) of gravitational waves detectors has only been able to observe collisions between pairs of black holes or neutron stars. For the first time, in January 2020, the network of detectors made the discovery of gravitational waves from a pair of NS-BH mergers. According to the IUCAA director, the technique used here to detect the signal is called matched filtering. “This was also used for the first discovery of gravitational waves. It may be recalled that this was developed at IUCAA in the 1990s by Sanjeev Dhurandhar and others,” he said. “Basically, we have been detecting binary black hole mergers and binary neutron star mergers (until now). This is a hybrid collision,” according to scientists at the Laser Interferometer Gravitational-wave Observatory, India (LIGO-India).

When contacted, DrTarunSouradeep, spokesperson of LIGO-India, said that researchers from LIGO-India have contributed to this major discovery. “This is an ongoing effort and the reason to make the detector network stronger is to discover a newer kind of phenomenon,” said Souradeep. This is a clear indication of neutron star and black hole merger, Prof Rajesh Nayak from the Center of Excellence in Space Sciences, IISER, Kolkata said.

Summer’s officially here! Longest day in the Northern Hemisphere is June 21st. Technically, the summer solstice occurs when the sun is directly over the imaginary Tropic of Cancer, or 23.5°N latitude. It’s also known as the northern solstice because it occurs when the sun is directly over the Tropic of Cancer in the Northern Hemisphere. This year, it occurred at 9:02 am IST on June 21st.Zenith Furthest Away from the Equator. A solstice happens when the sun’s zenith is at its furthest point from the equator. On the June solstice, it reaches its northernmost point and the Earth’s North Pole tilts directly towards the sun, at about 23.4 degrees.

“Solstice” (Latin: “solstitium”) means sun-stopping. The point on the horizon where the sun appears to rise and set, stops and reverses direction after this day. On the solstice, the sun does not rise precisely in the east, but rises to the north of east and sets to the north of west, meaning it’s visible in the sky for a longer period of time. Although the June solstice marks the first day of astronomical summer, it’s more common to use meteorological definitions of seasons, making the solstice midsummer or midwinter.

Solstices in Culture

Over the centuries, the June solstice has inspired countless festivals, midsummer celebrations and religious holidays. One of the world’s oldest evidence of the summer solstice’s importance in culture is Stonehenge in England, a megalithic structure which clearly marks the moment of the June solstice. In the Southern Hemisphere, where the June solstice is known as the shortest day of the year, it marks the first day of astronomical winter, but the middle of winter in meteorological terms.

Midnight Sun or Polar Night?

On the June solstice, the midnight sun is visible (weather permitting) throughout the night, in all areas from just south of the Arctic Circle to the North Pole.

Sunrise and Sunset Times

On the other side of the planet, south of the Antarctic Circle there’s Polar Night, meaning no Sunlight at all, on the June solstice.

Solstice Dates Vary

Even though most people consider June 21 as the date of the June solstice, it can happen anytime between June 20 and June 22, depending on which time zone you’re in. June 22 solstices are rare – the last June 22 solstice in UTC time took place in 1975 and there won’t be another one until 2203. The varying dates of the solstice are mainly due to the calendar system – most western countries use the Gregorian calendar which has 365 days in a normal year and 366 days in a Leap Year.

A tropical year is the time it takes the Earth to orbit once around the Sun. It is around 365.242199 days long, but varies slightly from year to year because of the influence of other planets. The exact orbital and daily rotational motion of the Earth, such as the “wobble” in the Earth’s axis (precession of the equinoxes), also contributes to the changing solstice dates. The 23.4° tilt in the Earth’s axis causes varying amounts of sunlight to reach different regions during its year-long orbit around the Sun. Today, the North Pole is tipped more towards the Sun than on any other day of the year. However, that does not mean more heat or that the Earth is any closer to the Sun, per common misconceptions.

Summer solstices happen twice each year (once in each hemisphere). Summer solstice for the Northern Hemisphere = Winter solstice for the Southern Hemisphere, and vice-versa. Also, during Equinoxes (vernal and autumnal), the Sun shines directly on the Equator and the length of day and night are nearly equal in either hemisphere. More key dates for 2021 (Northern Hemisphere): Autumn Equinox: Thursday, September 23, Winter Solstice: Tuesday, December 21.

Newswise — Woods Hole, MA — An innovative underwater robot known as Mesobot is providing researchers with deeper insight into the vast mid-ocean region known as the “twilight zone.” Capable of tracking and recording high-resolution images of slow-moving and fragile zooplankton, gelatinous animals, and particles, Mesobot greatly expands scientists’ ability to observe creatures in their mesopelagic habitat with minimal disturbance. This advance in engineering will enable greater understanding of the role these creatures play in transporting carbon dioxide from the atmosphere to the deep sea, as well as how commercial exploitation of twilight zone fisheries might affect the marine ecosystem.

In a paper published June 16 in Science Robotics, Woods Hole Oceanographic Institution (WHOI) senior scientist Dana Yoerger presents Mesobot as a versatile vehicle for achieving a number of science objectives in the twilight zone.  “Mesobot was conceived to complement and fill important gaps not served by existing technologies and platforms,” said Yoerger. “We expect that Mesobot will emerge as a vital tool for observing midwater organisms for extended periods, as well as rapidly identifying species observed from vessel biosonars. Because Mesobot can survey, track, and record compelling imagery, we hope to reveal previously unknown behaviors, species interactions, morphological structures, and the use of bioluminescence.”

Co-authored by research scientists and engineers from WHOI, MBARI (Monterey Bay Aquarium Research Institute), and Stanford University, the paper outlines the robot’s success in autonomously tracking two gelatinous marine creatures during a 2019 research cruise in Monterey Bay. High-definition video revealed a “dinner plate” jellyfish “ramming” a siphonophore, which narrowly escaped the jelly’s venomous tentacles. Mesobot also recorded a 30-minute video of a giant larvacean, which appears to be nearly motionless but is actually riding internal waves that rise and fall 6 meters (20 feet). These observations represent the first time that a self-guided robot has tracked these small, clear creatures as they move through the water column like a “parcel of water,” said Yoerger.

“Mesobot has the potential to change how we observe animals moving through space and time in a way that we’ve never been able to do before,” said KakaniKatija, MBARI principal engineer. “As we continue to develop and improve on the vehicle, we hope to observe many other mysterious and captivating animals in the midwaters of the ocean, including the construction and disposal of carbon-rich giant larvacean ‘snot palaces.’”

Packaged in a hydrodynamically efficient yellow case, the hybrid robot is outfitted with a suite of oceanographic and acoustic survey sensors. It may be piloted remotely through a fiberoptic cable attached to a ship or released from its tether to follow pre-programmed missions or autonomously track a target at depths up to 1,000 meters (3,300 feet). This autonomous capability will one day enable Mesobot to follow a target animal for over 24 hours without human intervention, which is enough time to observe its migration from the midwater twilight zone to the surface and back. Future studies with Mesobot could provide researchers with valuable insight into animal behavior during diel vertical migration, known as “the greatest migration on Earth” because of the vast number and diversity of creatures that undertake it each night.

“By leveraging the data we’ve collected using Mesobot, and other data that we’ve been curating for 30-plus years at MBARI, we hope to integrate smarter algorithms on the vehicle that uses artificial intelligence to discover, continuously track, and observe enigmatic animals and other objects in the deep sea,” Kakani said. The design, construction, and initial testing for Mesobot was funded by the U.S. NSF program for Ocean Technology and Interdisciplinary Coordination (OTIC). The research in this paper was supported by the David and Lucile Packard Foundation and WHOI’s Ocean Twilight Zone (OTZ) Project, funded as part of The Audacious Project housed at TED.

See more Mesobot here: https://youtu.be/5hjZtBvsmVY

The WMO report predicts an increased chance of tropical cyclones in the Atlantic Ocean, that Africa’s Sahel and Australia will likely be wetter, and that the southwest of Northern America is likely to be drier.

There is now a 40% chance that global temperatures will temporarily reach 1.5℃ above pre-industrial levels in the next five years — and these odds are rising, a U.N. report said on Wednesday.This does not yet mean that the world would already be crossing the long-term warming 1.5-degree threshold set by the Paris Climate Accord, which scientists warn is the ceiling to avoid the most catastrophic effects of climate change. The Paris Accord target looks at temperature over a 30-year average, rather than a single year.

But it does underscore that “we are getting measurably and inexorably closer” to that threshold, said U.N. World Meteorological Organization (WMO) Secretary-General Petteri Taalas in a statement. Taalas described the study as “yet another wakeup call” to slash greenhouse gas emissions.Every year from 2021 through 2025 is likely to be at least 1℃ warmer, according to the study. The report also predicts a 90% chance that at least one of those years will become the warmest year on record, topping 2016 temperatures.

In 2020 – one of the three warmest years on record – the global average temperature was 1.2 degrees Celsius above the pre-industrial baseline, according to an April WMO report.”There’s a little bit of up and down in the annual temperatures,” said Gavin Schmidt, director of NASA’s Goddard Institute for Space Studies in New York City. “But these long term-trends are unrelenting.””It seems inevitable that we’re going to cross these boundaries,” Schmidt said, “and that’s because there are delays in the system, there is inertia in the system, and we haven’t really made a big cut to global emissions as yet.”

Almost all regions are likely to be warmer in the next five years than in the recent past, the WMO said. The WMO uses temperature data from multiple sources including NASA and the National Oceanic and Atmospheric Administration (NOAA).Weather that was once unusual is now becoming typical. Earlier this month, for example, NOAA released its updated “climate normals,” which provide baseline data on temperature and other climate measures across the United States. The new normals — updated every 10 years — showed that baseline temperatures across the United States are overwhelmingly higher compared with the past decade.

Temperatures shifts are occurring both on average and in temperature extremes, said Russell Vose, chief of the climatic analysis and synthesis branch at NOAA’s National Centers for Environmental Information. Over the next five years, these extremes are “more likely what people will notice and remember,” he said.Warming temperatures also affect regional and global precipitation. As temperatures rise, evaporation rates increase and warmer air can hold more moisture. Climate change also can shift circulation patterns in the atmosphere and ocean.

The WMO report predicts an increased chance of tropical cyclones in the Atlantic Ocean, that Africa’s Sahel and Australia will likely be wetter, and that the southwest of Northern America is likely to be drier.The projections are part of a recent WMO effort to provide shorter-range forecasts of temperature, rainfall and wind patterns, to help nations keep tabs on how climate change may be disrupting weather patterns.Looking at marine and land heat waves, ice sheets melting, ocean heat content rising, and species migrating toward colder places, “it’s more than just temperature,” Vose said. “There are other changes in the atmosphere and in the ocean and in the ice and in the biosphere that all point to a warming world.”

There’s a 40% chance that the world will get so hot in the next five years that it will temporarily push past the temperature limit the Paris climate agreement is trying to prevent, meteorologists said. A new World Meteorological Organization forecast for the next several years also predicts a 90% chance that the world will set yet another record for the hottest year by the end of 2025 and that the Atlantic will continue to brew more potentially dangerous hurricanes than it used to.For this year, the meteorologists say large parts of land in the Northern Hemisphere will be 1.4 degrees (0.8 degrees Celsius) warmer than recent decades and that the U.S. Southwest’s drought will continue.

The 2015 Paris climate accord set a goal of keeping warming to a few tenths of a degree warmer from now. The report said there is a 40% chance that at least one of the next five years will be 1.5 degrees Celsius (2.7 degrees Fahrenheit) higher than pre-industrial times — the more stringent of two Paris goals. The world is already 1.2 degrees Celsius (2.2 degrees Fahrenheit) warmer than pre-industrial times. Last year, the same group forecasted a 20% chance of it happening.

The doubling of the odds is due to improvements in technology that show it has “actually warmed more than we thought already,” especially over the lightly-monitored polar regions, said Leon Hermanson, a climate scientist at the United Kingdom’s Met Center who helped on the forecast. “It’s a warning that we need to take strong action,” Hermanson said.

Pennsylvania State University climate scientist Michael Mann, who wasn’t part of the report, said he is “almost certain” the world will exceed that Paris warming threshold at least once in the next few years. But he said one or two years above 1.5 degrees Celsius (2.7 degrees Fahrenheit) isn’t as worrisome as when the overall trend of temperatures stays above that level. Mann said that won’t happen probably for decades and could still be prevented.

Newswise — Washington, DC– The cause of Earth’s deepest earthquakes has been a mystery to science for more than a century, but a team of Carnegie scientists may have cracked the case.New research published in AGU Advances provides evidence that fluids play a key role in deep-focus earthquakes–which occur between 300 and 700 kilometers below the planet’s surface. The research team includes Carnegie scientists Steven Shirey, Lara Wagner, Peter van Keken, and Michael Walter, as well as the University of Alberta’s Graham Pearson.

Most earthquakes occur close to the Earth’s surface, down to about 70 kilometers. They happen when stress builds up at a fracture between two blocks of rock–known as a fault–causing them to suddenly slide past each other.However, deeper into the Earth, the intense pressures create too much friction to allow this kind of sliding to occur and the high temperatures enhance the ability of rocks to deform to accommodate changing stresses. Though theoretically unexpected, scientists have been able to identify earthquakes that originate more than 300 kilometers below the surface since the 1920s.

“The big problem that seismologists have faced is how it’s possible that we have these deep-focus earthquakes at all,” said Wagner. “Once you get a few tens of kilometers down, it becomes incredibly difficult to explain how we are getting slip on a fault when the friction is so incredibly high.”

Ongoing work over the past several decades has shown us that water plays a role in intermediate-depth earthquakes–those that occur between 70 and 300 kilometers below Earth’s surface. In these instances, water is released from minerals, which weakens the rock around the fault and allows the blocks of rock to slip. However, scientists didn’t think this phenomenon could explain deep-focus earthquakes, largely because it was believed that water and other fluid-creating compounds couldn’t make it far enough down into the Earth’s interior to provide a similar effect.This thinking changed for the first time when Shirey and Wagner compared the depths of rare deep-Earth diamonds to the mysterious deep-focus earthquakes.

“Diamonds form in fluids” explained Shirey, “if diamonds are there, fluids are there.”The diamonds themselves indicated the presence of fluids, however, they also brought samples of the deep-Earth to the surface for the scientists to study. When diamonds form in the Earth’s interior, they sometimes capture pieces of mineral from the surrounding rock. These minerals are called inclusions and they may make your jewelry less expensive, but they are invaluable to Earth scientists. They are one of the only ways scientists can study direct samples of our planet’s deep interior.

The diamond’s inclusions had the distinct chemical signature of similar materials found in oceanic crust. This means that the water and other materials weren’t somehow created deep in the Earth’s interior. Instead, they were carried down as part of a sinking oceanic plate.Said Wagner: “The seismology community had moved away from the idea that there could be water that deep. But diamond petrologists like Steve were showing us samples and saying ‘No, no, no. There’s definitely water down here’ So then we all had to get together to figure out how it got down there.”

To test the idea, Wagner and van Keken built advanced computational models to simulate the temperatures of sinking slabs at much greater depths than had been attempted before. In addition to the modeling, Walter examined the stabilities of the water-bearing minerals to show that under the intense heat and pressures of the Earth’s deep interior, they would, indeed, be capable of holding on to water in certain conditions. The team showed that even though warmer plates didn’t hold water, the minerals in the cooler oceanic plates could theoretically carry water to the depths we associate with deep-focus earthquakes.

To solidify the study the team compared the simulations to real-life seismological data. They were able to show that the slabs that could theoretically carry water to these depths were also the ones experiencing the previously unexplained deep earthquakes.This study is unusual in applying four different disciplines–geochemistry, seismology, geodynamics, and petrology–to the same question, all of which point to the same conclusion: water and other fluids are a key component of deep-focus earthquakes.

“The nature of deep earthquakes is one of the big questions in geoscience,” said Shirey. “We needed all four of these different disciplines to come together to make this argument. It turned out we had them all in-house at Carnegie.”The authors thank the Carnegie Institution for Science and the University of Alberta for continuing support. Diamond research is supported by the Deep Carbon Observatory and the U.S. National Science Foundation.

The Carnegie Institution for Science (carnegiescience.edu) is a private, nonprofit organization headquartered in Washington, D.C., with three research divisions on both coasts. Since its founding in 1902, the Carnegie Institution has been a pioneering force in basic scientific research. Carnegie scientists are leaders in the life and environmental sciences, Earth and planetary science, and astronomy and astrophysics.