Category: Science

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.

A new report released this week by the National Oceanic and Atmospheric Administration (NOAA) shows that the United States is getting warmer and parts of it are getting wetter.

NOAA’s “new normals” set of data tracks changes in the U.S. climate over a 30-year period. The latest report is based on data from 1991 to 2020 and replaces the 1981 to 2010 report. It shows a small, but noticeable warming trend across much of the country, which is consistent with the majority of NOAA’s previous reports over the last 100 years.

“The changes in NOAA’s new report are only a degree or less but can still have a big impact, especially when much of the past century has seen steadily increasing temperatures, with the most pronounced changes occurring in the past several decades,” said Nick Bassill, a meteorologist at the University at Albany. “The unfortunate thing is that this does not make a bigger splash, even though it’s almost universally accepted that the new climate normals were going to come in warmer than the last report.”

“While some may dispute the exact amount the change is related to climate change vs. natural variability, it’s likely that this trend is driven in large part by climate change on a global scale.”

Bassill is the director of UAlbany’s Center of Excellence in Weather & Climate Analytics. He also works closely with the NYS Mesonet, which is headquartered at UAlbany, and includes a network of 126 standard weather observation stations across the state.
This new report will have a direct impact on New York’s weather and climate projections, according to Bassill.

“It’s likely that our NYS Mesonet stations will see a subtle, yet consistent, increase in expected average temperatures. Warmer temperatures, along with precipitation increases, are generally expected for the northeast U.S.”

About UAlbany’s Weather-Climate Enterprise: With close to 120 faculty, researchers and staff, UAlbany hosts the largest concentration of atmospheric, climate and environmental scientists in New York State, and one of the largest in the nation. Led by its Department of Atmospheric and Environmental Sciences and Atmospheric Sciences Research Center, UAlbany is also home to the NYS Center of Excellence Weather-Climate Business Analytics, the xCITE R&D laboratory, and the New York State Mesonet – the most advanced mesoscale weather observation system in the nation.

Newswise — The Antarctic ice sheet is much less likely to become unstable and cause dramatic sea-level rise in upcoming centuries if the world follows policies that keep global warming below a key 2015 Paris climate agreement target, according to a Rutgers coauthored study.

But if global warming exceeds the target – 2 degrees Celsius (3.6 degrees Fahrenheit) – the risk of ice shelves around the ice sheet’s perimeter melting would increase significantly, and their collapse would trigger rapid Antarctic melting. That would result in at least 0.07 inches of global average sea-level rise a year in 2060 and beyond, according to the study in the journal Nature.

That’s faster than the average rate of sea-level rise over the past 120 years and, in vulnerable coastal places like downtown Annapolis, Maryland, has led to a dramatic increase in days of extreme flooding.

Global warming of 3 degrees Celsius (5.4 degrees Fahrenheit) could lead to catastrophic sea-level rise from Antarctic melting – an increase of at least 0.2 inches per year globally after 2060, on average.

“Ice-sheet collapse is irreversible over thousands of years, and if the Antarctic ice sheet becomes unstable it could continue to retreat for centuries,” said coauthor Daniel M. Gilford, a post-doctoral associate in the Rutgers Earth System Science & Policy Lab led by coauthor Robert E. Kopp, a professor in the Department of Earth and Planetary Sciences within the School of Arts and Sciences at Rutgers University–New Brunswick. “That’s regardless of whether emissions mitigation strategies such as removing carbon dioxide from the atmosphere are employed.”

The Paris Agreement, achieved at a United Nations climate change conference, seeks to limit the negative impacts of global warming. Its goal is to keep the increase in global average temperature well below 2 degrees Celsius above pre-industrial levels, along with pursuing efforts to limit the increase to 1.5 degrees Celsius (2.7 degrees Fahrenheit). The signatories committed to eliminating global net carbon dioxide emissions in the second half of the 21st century.

Climate change from human activities is causing sea levels to rise, and projecting how Antarctica will contribute to this rise in a warmer climate is a difficult but critical challenge. How ice sheets might respond to warming is not well understood, and we don’t know what the ultimate global policy response to climate change will be. Greenland is losing ice at a faster rate than Antarctica, but Antarctica contains nearly eight times more ice above the ocean level, equivalent to 190 feet of global average sea-level rise, the study notes.

The study explored how Antarctica might change over the next century and beyond, depending on whether the temperature targets in the Paris Agreement are met or exceeded. To better understand how the ice sheet might respond, scientists trained a state-of-the-art ice-sheet model with modern satellite observations, paleoclimate data and a machine learning technique. They used the model to explore the likelihood of rapid ice-sheet retreat and the western Antarctic ice-sheet’s collapse under different global greenhouse gas emissions policies.

Current international policies are likely to lead to about 3 degrees Celsius of warming, which could thin Antarctica’s protective ice shelves and trigger rapid ice-sheet retreat between 2050 and 2100. Under this scenario, geoengineering strategies such as removing carbon dioxide from the atmosphere and sequestering (or storing) it would fail to prevent the worst of Antarctica’s contributions to global sea-level rise.

“These results demonstrate the possibility that unstoppable, catastrophic sea level rise from Antarctica will be triggered if Paris Agreement temperature targets are exceeded,” the study says. Gilford said “it’s critical to be proactive in mitigating climate change now through active international participation in reducing greenhouse gas emissions and by continuing to ratchet down proposed policies to meet the ambitious Paris Agreement targets.”

Rutgers coauthors include Erica Ashe, a post-doctoral scientist in the Rutgers Earth System Science & Policy Lab. Scientists at the University of Massachusetts Amherst, Pennsylvania State University, University of California Irvine, University of Bristol, McGill University, Woods Hole Oceanographic Institution and University of Wisconsin-Madison contributed to the study.

Global Temperature Report: April 2021

(New Reference Base, 1991-2020)

Global climate trend since Dec. 1 1978: +0.14 C per decade

 April Temperatures (preliminary)

Global composite temp.:  -0.05 C (-0.09 °F) below seasonal average

Northern Hemisphere: +0.05 C (+0.09 °F) above seasonal average

Southern Hemisphere: -0.15 C (-0.27 °F) below seasonal average

Tropics: -0.28 C (-0.50 °F) below seasonal average

 March Temperatures (final)

Global composite temp.:  -0.01 C (-0.02 °F) below seasonal average

Northern Hemisphere: +0.12 C (+0.22 °F) above seasonal average

Southern Hemisphere: -0.14 C (-0.25 °F) below seasonal average

Tropics: -0.29 C (-0.52 °F) below seasonal average

 Notes on data released May 3, 2021 (v6.0, with new reference base)

This is the period in the La Niña-induced cooling cycle where the global temperature typically reaches its coolest value.  NOAA again reports that the water temperatures in the tropical Pacific are still below average – about the same as March – but much warmer than last November and December.

The global departure from average of -0.05 °C (-0.09 °F) represents a slight cooling from March led by declines in the atmosphere’s temperature over the Northern Hemispheric land areas.   A key indicator of the next few months’ temperature is the tropical anomaly which in April was essentially the same as March.  This is an indication that this cool episode is likely bottoming-out around 0.4 °C cooler than last August to November.  Will the La Niña return next fall?  Will there be neutral conditions?  We are in the time of year called a forecast barrier beyond which it is difficult to predict what the next winter will see in terms of La Niña/El Niño/Neutral conditions.  The indicators will start showing their hand in the latter part of the northern summer.

The warmest grid cell, in terms of departure from average, was +3.7 °C (+6.7 °F) over the Bering Sea just north of the Rat Islands (part of the Aleutian chain).  Anomalous warmth centered there spread to the western conterminous US and eastward to the Russian coast.  Other areas of anomalous warmth were in NE Canada, western Russia southward to the Caspian Sea, the South Pacific and Argentina eastward into the South Atlantic.

The coldest departure from average was over the Baltic Sea just north of Poland at -3.2 °C (-5.8 °F).  This cool region stretched from the Arctic southward to the Mediterranean Sea.  Additional cool areas were found in north-central Canada, the African Sahel, India to western China, and several regions over the oceans, especially the southern oceans, primarily related to La Niña.

The conterminous US cooled from March’s warmth to -0.02 °C (-0.04 °F), almost exactly at the 30-year average.  As is often the case the average is a small residual of two contrasting areas – the West was warm and the East was cool.  Adding in Alaska’s above average temperature puts the 49-state average at +0.10 °C (+0.18 °F) – still very close to the average.  [We don’t include Hawaii in the US results because its land area is less than that of a satellite grid square, so it would have virtually no impact on the overall national results.]

New Reference Base Jan 2021.  As noted in the Jan 2021 GTR, the situation comes around every 10 years when the reference period or “30-year normal” that we use to calculate the departures is redefined.  With that, we have averaged the absolute temperatures over the period 1991-2020, in accordance with the World Meteorological Organization’s guidelines, and use this as the new base period.  This allows the anomalies to relate more closely to the experience of the average person, i.e. the climate of the last 30 years.  Due to the rising trend of global and regional temperatures, the new normals are a little warmer than before, i.e. the global average temperature for Januaries for 1991-2020 is 0.14 °C warmer than the average for Januaries during 1981-2010.  So, the new departures from this now warmer average will appear to be cooler, but this is an artifact of simply applying a new base period.  It is important to remember that changes over time periods, such as a trend value or the relative difference of one year to the next, will not change.  Think about it this way, all we’ve done is to take the entire time series and shifted it down a little.

To-Do List: There has been a delay in our ability to utilize and merge the new generation of microwave sensors (ATMS) on the NPP and JPSS satellites.  As of now, the calibration equations applied by the agency have changed at least twice, so that the data stream contains inhomogeneities which obviously impact the type of measurements we seek.  We are hoping this is resolved soon with a dataset that is built with a single, consistent set of calibration equations.   In addition, the current non-drifting satellite operated by the Europeans, MetOP-B, has not yet been adjusted or “neutralized” for its seasonal peculiarities related to its unique equatorial crossing time (0930).  While these MetOP-B peculiarities do not affect the long-term global trend, they do introduce error within a particular year in specific locations over land.

As part of an ongoing joint project between UAH, NOAA and NASA, Christy and Dr. Roy Spencer, an ESSC principal scientist, use data gathered by advanced microwave sounding units on NOAA, NASA and European satellites to produce temperature readings for almost all regions of the Earth. This includes remote desert, ocean and rain forest areas where reliable climate data are not otherwise available.  Drs. Danny Braswell and Rob Junod assist in the preparation of these reports.

The satellite-based instruments measure the temperature of the atmosphere from the surface up to an altitude of about eight kilometers above sea level. Once the monthly temperature data are collected and processed, they are placed in a “public” computer file for immediate access by atmospheric scientists in the U.S. and abroad.

The complete version 6 lower troposphere dataset is available here: http://www.nsstc.uah.edu/data/msu/v6.0/tlt/uahncdc_lt_6.0.txt

Archived color maps of local temperature anomalies are available on-line at: http://nsstc.uah.edu/climate/

Neither Christy nor Spencer receives any research support or funding from oil, coal or industrial companies or organizations, or from any private or special interest groups. All of their climate research funding comes from federal and state grants or contracts.

The global average temperature was about 1.2 degrees Celsius above pre-industrial levels despite the cooling effect of La Nina ocean-atmosphere phenomenon in 2020, the World Meteorological Organisation confirmed on Monday in its State of the Global Climate 2020 report. The Intergovernmental Panel on Climate Change (IPCC) had warned that a 1.5 degree C warming will mark a menacing milestone in the warming of the planet.

UN Secretary-General, Antonio Guterres who released the report on Monday said the UN is building a global coalition to reach net-zero emissions by 2050. “2020 was 1.2 degrees Celsius hotter than pre-industrial times. We are getting dangerously close to the 1.5-degree Celsius limit set by the scientific community. We are on the verge of the abyss. To avert the worst impacts of climate change, science tells us that we must limit global temperature rise to within 1.5 degrees of the pre-industrial baseline. That means reducing global greenhouse gas emissions by 45% from 2010 levels by 2030 and reaching net-zero emissions by 2050. We are way off track. This must be the year for action,” he said adding that all countries should phase out coal by 2040.

Last year was one of the three warmest years on record; the six years since 2015 have been the warmest on record and 2011-2020 was the warmest decade on record, the report highlighted adding that decrease in the annual growth rate of CO2 concentration due to the Covid 19 lockdown will be practically indistinguishable.

Globally averaged carbon dioxide (CO2) concentrations have already exceeded 410 parts per million (ppm), 148% of pre-industrial levels, and if the CO2 concentration follows the same pattern as in previous years, it could reach or exceed 414 ppm in 2021, according to the report.

“Developed countries must lead in phasing out coal — by 2030 in Organisation for Economic Cooperation and Development (OECD) countries, and 2040 elsewhere. No new coal power plants should be built.” Guterres also called for an agreement among all countries to follow a common direction of travel. “The United Nations is building a global coalition committed to net zero emissions – to cover all countries, cities, regions, businesses and financial institutions. Second, the next 10 years need to be a decade of transformation. Countries need to submit ambitious new NDCs — the nationally determined contributions to the Paris Agreement – which are their climate plans for the next 10 years,” he said.

The report comes ahead of the April 22-23 Virtual Leaders’ Summit on Climate convened by the United States of America. The Summit will have participation from 40 world leaders and one of its aims is “Galvanizing efforts by the world’s major economies to reduce emissions during this critical decade to keep the goal of limiting warming to 1.5 degree Celsius within reach,” according to the US department of state.

United States Special Presidential Envoy for Climate, John Kerry had met Prime Minister Narendra Modi and environment minister Prakash Javadekar earlier this month regarding increasing climate ambition ahead of COP 26 in Glasgow this November. Minister for Europe and Foreign Affairs of France, Jean-Yves Le Drian had also met Javadekar and said all countries should be on track to achieve carbon neutrality and start phasing out coal.

Javadekar had said India will not raise its climate ambition at the behest of or under pressure from developed countries. India has the right to develop and its poor have the right to grow and that countries should respect the principle of common but differentiated responsibilities (CBDR). (CBDR, a principle under the Paris Agreement requires richer countries to lead and take historical responsibility for the emissions caused in the past by them.)

According to Climatewatch’s net-zero tracker, 59 countries representing 54% of global emissions have announced net-zero targets. Only 6 parties have legislations on net-zero emissions. India is among 6 countries that are compliant with the Paris Agreement’s 2-degree target including Bhutan, Costa Rica and the Philippines according to Climate Action Tracker. 7 countries are “critically insufficient” and their pledges will lead to 4+degree C warming including the US and the Russian Federation.

Temperatures reached 38.0 degrees C at Verkhoyansk, Russian Federation on June 20, the highest recorded temperature anywhere north of the Arctic Circle. The Arctic minimum sea-ice extent in September 2020 was the second-lowest on record. The sea-ice retreat in the Laptev Sea was the earliest observed in the satellite era. Some 9.8 million people were displaced largely due to hydrometeorological hazards and disasters, and were recorded during the first half of 2020. Annual precipitation totals in monsoon in North America, Africa, South-West Asia and South-East Asia were unusually high in 2020. Monsoon seasonal totals in India were 109% of the long-term mean, the third-highest seasonal total after 1994 and 2019.

“2020 was one of the warmest years despite having a La Niña with cool waters in the east Pacific. La Niñas typically has a cooling effect on global temperatures, but this is now offset by global warming due to greenhouse gas emissions. As a result, La Niña years now are warmer than years with El Niño events of the past,” Roxy Mathew Koll, a climate scientist at the Indian Institute of Tropical Meteorology (IITM), Pune.

“International agreements on climate change aim to keep global warming within the safe range of 1.5C to 2C, but few people realise that the world’s average temperature is already more than a degree warmer than it was 200 years ago. Parts of the world like the Himalayas are warming even faster. This is a serious concern for India because climate change could have a compounding effect on existing scarcities, stresses and extreme events. For example, in 2020, even as we were fighting the Covid-19 pandemic, we also had to face Cyclone Amphan, which intensified rapidly in a warmer ocean. It is crucial that all countries invest in adaptation to climate impacts, especially to protect those who are most vulnerable to extreme events. At the same time, we need to accelerate policies and technologies to mitigate global greenhouse gas emissions as rapidly as possible,” said Ulka Kelkar, director of climate programme at the World Resources Institute, responding to the WMO report.

Google Earth users can now see the striking effect of climate change over the past four decades.  Google’s latest feature, Timelapse, is an eye opening, technical feat that provides visual evidence of how the Earth has changed due to climate change and human behavior. The tool takes the platform’s static imagery and turns it into a dynamic 4D experience, allowing users to click through timelapses that highlight melting ice caps, receding glaciers, massive urban growth and wildfires’ impact on agriculture.

Timelapse compiles 24 million satellite photos taken from 1984 to 2020, an effort Google (GOOG) said took two million processing hours across thousands of machines in Google Cloud. For the project, the company worked with NASA, the United States Geological Survey’s Landsat program — the world’s longest-running Earth observation program — the European Union’s Copernicus program and its Sentinel satellites, and Carnegie Mellon University’s CREATE Lab, which helped develop the technology behind Timelapse.

To explore Timelapse in Google Earth, users can type any location into the search bar to see it in motion, whether it’s a landmark or the neighborhood in which they grew up. Google said it removed elements such as clouds and shadows from the images, and computed a single pixel for every location on Earth for every year since 1984; ultimatel stitching them together into a timelapse video.

For example, it’s possible to see the Cape Cod coast slowly shifting south, agriculture growth in the middle of a desert in Al Jowf, Saudi Arabia, and the development of Songdo beach, a man-made beach in Busan, South Korea.

“Visual evidence can cut to the core of the debate in a way that words cannot and communicate complex issues to everyone,” said Rebecca Moore, a director of Google Earth, in a blog post on Thursday.

Google also created various guided tours through Voyager, its storytelling platform, around some of the broader changes seen in the imagery.

The company said it hopes governments, researchers, journalists, teachers and advocates will analyze the imagery, identity trends and share their findings.

“We invite anyone to take Timelapse into their own hands and share it with others — whether you’re marveling at changing coastlines, following the growth of megacities, or tracking deforestation,” Moore said. “Timelapse in Google Earth is about zooming out to assess the health and well-being of our only home, and is a tool that can educate and inspire action.”

The future life span of Earth’s oxygen-rich atmosphere is approximately one billion years, a new study reveals.

According to the study, published in the journal Nature Geoscience, Earth’s surface environment is highly oxygenated — from the atmosphere to the deepest reaches of the oceans, representing a hallmark of active photosynthetic biosphere.

However, the fundamental timescale of the oxygen-rich atmosphere on Earth remains uncertain, particularly for the distant future.

“For many years, the lifespan of Earth’s biosphere has been discussed based on scientific knowledge about the steadily brightening of the sun and global carbonate-silicate geochemical cycle,” said researcher Kazumi Ozaki, Assistant Professor at Toho University.

To examine how Earth’s atmosphere will evolve in the future, the team constructed an Earth system model which simulates climate and biogeochemical processes.

Because modelling future Earth evolution intrinsically has uncertainties in geological and biological evolutions, a stochastic approach was adopted, enabling the researchers to obtain a probabilistic assessment of the lifespan of an oxygenated atmosphere.

The team ran the model more than 400,000 times, varying model parameter, and found that Earth’s oxygen-rich atmosphere will probably persist for another one billion years before rapid deoxygenation renders the atmosphere reminiscent of early Earth before the Great Oxidation Event around 2.5 billion years ago.

“The atmosphere after the great deoxygenation is characterized by an elevated methane, low-levels of CO2 and no ozone layer. The Earth system will probably be a world of anaerobic life forms,” said Ozaki.

Earth’s oxygen-rich atmosphere represents an important sign of life that can be remotely detectable. However, this study suggests that Earth’s oxygenated atmosphere would not be a permanent feature, and that the oxygen-rich atmosphere might only be possible for 20-30 per cent of the Earth’s entire history as an inhabited planet, the researchers said.

Oxygen (and photochemical byproduct, ozone) is the most accepted biosignature for the search for life on the exoplanets, but if we can generalize this insight to Earth-like planets, then scientists need to consider additional biosignatures applicable to weakly-oxygenated and anoxic worlds in the search for life beyond our solar system, the team added. (IANS)

Dr. Huw Griffiths, marine biologist and lead author of the study, said that the stationary animals are like sponges and potentially several previously unknown species. The discovery appears to go against all previous theories of what kind of life could survive in such an extreme condition.(British Antarctic Survey)

Researchers accidentally discovered extreme life far underneath the ice shelves of the Antarctic during an exploratory survey, a recent study published in the journal Frontiers in Marine Science said. At a distance of 260km away from the open ocean, the researchers found out the existence of stationary animals attached to a boulder on the seafloor as they drilled through 900 metres of ice in the Filchner-Ronne Ice Shelf with their cameras lowered down.

Dr Huw Griffiths, marine biologist and lead author of the study, said that the stationary animals are like sponges and potentially several previously unknown species. In a video shared by the British Antarctic Survey, Griffiths said it was a surprising discovery because they never expected animals that “filter feed their food from the water column to be found this far from a source of food or daylight.”

“This discovery is one of those fortunate accidents that pushes ideas in a different direction and shows us that Antarctic marine life is incredibly special and amazingly adapted to a frozen world,” the biogeographer said in a separate statement.

The first-ever record of a hard substrate community deep beneath an ice shelf throws up more questions than it answers since the researchers don’t know how did they get there, what they have been eating or how long they have been there. The researchers are wondering whether these are the same species seen outside the ice shelf or are they new species. There are also few questions around the survival of these species in case the ice shelf collapses.

The discovery appears to go against all previous theories of what kind of life could survive in such an extreme condition. The dependence on drilling and cameras mean, according to Griffiths, the area underneath the giant floating ice shelves is probably one of the least known habitats on Earth. But getting up close with these animals and their environment remains a challenge for polar scientists.

“We have no idea what species these animals are. We don’t know how they are coping with these extreme conditions. And the only way we are going to be able to answer those questions is to come up with a new way of investigating their world,” added Griffiths.