Tag Archives: shaped

Hozier on the love and loss that shaped his new album, “Unreal Unearth” – CBS Mornings

  1. Hozier on the love and loss that shaped his new album, “Unreal Unearth” CBS Mornings
  2. Hozier Goes Through Hell and Tastes Ecstasy on ‘Unreal Unearth’ Rolling Stone
  3. Hozier – ‘Unreal Unearth’ album review: A beautiful, angst-filled journey through the nine circles of hell Far Out Magazine
  4. Hozier walks through hell but finds the light on ‘Unreal Unearth’ Entertainment Weekly News
  5. Hozier reflects on 10 years of “Take Me to Church,” processing the internal “janitorial work” of a breakup through music CBS News
  6. View Full Coverage on Google News

Read original article here

‘Reality’ Review: Sydney Sweeney Is Devastating as Reality Winner in Taut Thriller Shaped from FBI Transcript – Hollywood Reporter

  1. ‘Reality’ Review: Sydney Sweeney Is Devastating as Reality Winner in Taut Thriller Shaped from FBI Transcript Hollywood Reporter
  2. ‘Reality’ Review: Sydney Sweeney Is Outstanding as Whistleblower Reality Winner in a Clever, Gripping Docudrama Variety
  3. ‘Euphoria,’ ‘White Lotus’ Star Sydney Sweeney Consulted Real Life Whistleblower for Berlinale Title ‘Reality’: ‘This Is a Dream for an Actor’ Yahoo Entertainment
  4. ‘Reality’ Review: Sydney Sweeney Stuns in Fact-Based Single-Room Whistleblower Thriller IndieWire
  5. Sydney Sweeney On The “Honor” Of Speaking To Real Whistleblower For ‘Reality’ Role — Berlin Film Festival Deadline

Read original article here

Light shaped as a smoke ring that behaves like a particle

Light can be shaped into a structure resembling a twisted smoke ring. Credit: Y. Shen and Z. Zhu.

We can frequently find in our daily lives a localized wave structure that maintains its shape upon propagation—picture a smoke ring flying in the air. Similar stable structures have been studied in various research fields and can be found in magnets, nuclear systems, and particle physics. In contrast to a ring of smoke, they can be made resilient to perturbations. This is known in mathematics and physics as topological protection.

A typical example is the nanoscale hurricane-like texture of a magnetic field in magnetic thin films, behaving as particles—that is, not changing their shape—called skyrmions. Similar doughnut-shaped (or toroidal) patterns in 3D space, visualizing complex spatial distributions of various properties of a wave, are called hopfions. Achieving such structures with light waves is very elusive.

Recent studies of structured light revealed strong spatial variations of polarization, phase, and amplitude, which enable the understanding of—and open up opportunities for designing—topologically stable optical structures behaving like particles. Such quasiparticles of light with control of diversified topological properties may have great potential, for example as next-generation information carriers for ultra-large-capacity optical information transfer, as well as in quantum technologies.

As reported in Advanced Photonics, collaborating physicists from UK and China recently demonstrated the generation of polarization patterns with designed topologically stable properties in three dimensions, which, for the first time, can be controllably transformed and propagated in free space.

(a) The parameter-space sphere which represents spin: the longitude and latitude degrees (α and β) of a parametric 2-sphere are represented by hue color and its lightness (dark towards the south pole, where spin is down, and bright towards the north pole, where spin is up). Each point on a parametric 2-sphere corresponds to a closed iso-spin line located in a 3D Euclidean space. (b) The lines projected from the selected points of the same latitude β and different longitude α on the hypersphere (highlighted by the solid dots with the corresponding hue colors), form torus knots covering a torus (with different tori corresponding to different β). (c) The real-space visualization of a Hopf fibration as a full stereographic mapping from a hypersphere: torus knots arranged on a set of coaxially nested tori, with each torus corresponding to different latitude β of a parametric 2-sphere. The black circle corresponds to the south pole (spin down) and the axis of the nested tori corresponds to the north pole (spin up) in (a). (d) The 3D spin distribution in a hopfion, corresponding to the isospin contours in (c) with each spin vector colored by its α and β parameters of a parametric sphere in (a) as shown in the insert. (e, f) The cross-sectional view of the spin distribution in (d): (e) xy (z = 0) and (f) yz (x = 0) cross-sections show skyrmion-like structures with the gray arrows marking the vorticity of the skyrmions. Color scale is the same as that corresponding to the spin direction in (d). Credit: Shen et al., doi 10.1117/1.AP.5.1.015001

As a consequence of this insight, several significant advances and new perspectives are offered. “We report a new, very unusual, structured-light family of 3D topological solitons, the photonic hopfions, where the topological textures and topological numbers can be freely and independently tuned, reaching far beyond previously described fixed topological textures of the lowest order,” says Yijie Shen of University of Southampton in the UK, the lead author of the paper.

“Our results illustrate the immense beauty of light structures. We hope they will inspire further investigations towards potential applications of topological protected light configurations in optical communications, quantum technologies, light–matter interactions, superresolution microscopy, and metrology,” says Anatoly Zayats, professor at King’s College London and project lead.

This work provides a theoretical background describing the emergence of this family of hopfions and their experimental generation and characterization, revealing a rich structure of topologically protected polarization textures. In contrast to previous observations of hopfions localized in solid-state materials, this work demonstrates that, counterintuitively, an optical hopfion can propagate in free space with topological protection of the polarization distribution.

The robust topological structure of the demonstrated photonic hopfions upon propagation is often sought in applications.

This newly developed model of optical topological hopfions can be easily extended to other higher-order topological formations in other branches of physics. The higher order hopfions are still a great challenge to observe in other physics communities, from high-energy physics to magnetic materials. The optical approach proposed in this work may provide a deeper understanding of this complex field of structures in other branches of physics.

More information:
Yijie Shen et al, Topological transformation and free-space transport of photonic hopfions, Advanced Photonics (2023). DOI: 10.1117/1.AP.5.1.015001

Citation:
Photonic hopfions: Light shaped as a smoke ring that behaves like a particle (2023, January 19)
retrieved 20 January 2023
from https://phys.org/news/2023-01-photonic-hopfions-particle.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.



Read original article here

How the last 12,000 years have shaped what humans are today

Credit: Pixabay/CC0 Public Domain

While humans have been evolving for millions of years, the past 12,000 years have been among the most dynamic and impactful for the way we live today, according to an anthropologist who organized a special journal feature on the topic in the Proceedings of the National Academy of Sciences.

Our modern world all started with the advent of agriculture, said Clark Spencer Larsen, professor of anthropology at The Ohio State University.

“The shift from foraging to farming changed everything,” Larsen said.

Along with food crops, humans also planted the seeds for many of the most vexing problems of modern society.

“Although the changes brought about by agriculture brought plenty of good for us, it also led to increasing conflict and violence, rising levels of infectious diseases, reduced physical activity, a more limited diet, and more competition for resources,” he said.

Larsen is organizer and editor of a Special Feature published in the Jan. 17, 2023, issue of the journal Proceedings of the National Academy of Sciences. He is also author of the introduction to the section, titled “The past 12,000 years of behavior, adaptation, population, and evolution shaped who we are today.”

The Special Feature includes eight articles based mostly on bioarchaeology—the study of human remains and what they can tell scientists about changes in diet, behavior and lifestyle over the last 10 millennia or so. Larsen is co-author on two of these eight articles.

One message that connects all the articles is that the major societal issues of today have ancient roots, he said.

“We didn’t get to where we are now by happenstance. The problems we have today with warfare, inequality, disease and poor diets, all resulted from the changes that occurred when agriculture started,” Larsen said.

The shift from foraging to farming led humans, who had led a mostly transitory life, to create settlements and live a much more sedentary existence.

“That has had profound implications for virtually every aspect of our lives back then, now, and going forward,” he said.

Growing food allowed the world population to grow from about 10 million in the later Pleistocene Epoch to more than 8 billion people today.

But it came at a cost. The varied diet of foragers was replaced with a much more limited diet of domesticated plants and animals, which often had reduced nutritional quality. Now, much of the world’s population relies on three foods—rice, wheat and corn—especially in areas that have limited access to animal sources of protein, Larsen said.

Another important change in the diet of humans was the addition of dairy. In one article in the Special Feature, researchers examined dental calculus found in remains to show the earliest evidence of milk consumption dates to about 5,000 years ago in northern Europe.

“This is evidence of humans adapting genetically to be able to consume cheese and milk, and it happened very recently in human evolution,” he said. “It shows how humans are adapting biologically to our new lifestyle.”

As people began creating agricultural communities, social changes were occurring as well. Larsen co-authored one article that analyzed strontium and oxygen isotopes from tooth enamel of early farming communities from more than 7,000 years ago to help determine where residents were from. Results showed that Çatalhöyük, in modern Turkey, was the only one of several communities studied where nonlocals apparently lived.

“This was laying the foundation for kinship and community organization in later societies of western Asia,” he said.

These early communities also faced the problem of many people living in relatively cramped areas, leading to conflict.

In one article, researchers studying human remains in early farming communities across western and central Europe found that about 10% died from traumatic injuries.

“Their analysis reveals that violence in Neolithic Europe was endemic and scaling upward, resulting in patterns of warfare leading to increasing numbers of deaths,” Larsen writes in the introduction.

Research reported in this PNAS issue also reveals how these first human communities created the ideal conditions for another problem that is top-of-mind in the world today: infectious disease. Raising farm animals led to the common zoonotic diseases that can be transmitted from animals to people, Larsen said.

While the climate change crisis of today is unique in human history, past societies have had to deal with more short-term climate disasters, particularly long droughts.

In a perspective article co-authored by Larsen, the researchers noted that economic inequality, racism and other types of discrimination have been key factors in how societies have fared under these climate emergencies, and these factors will play a role in our current crisis.

Those communities with more inequality were most likely to experience violence in the wake of climate disasters, Larsen said.

What may be most surprising about all the changes documented in the Special Feature is how quickly they all occurred, he said.

“When you look at the six or so million years of human evolution, this transition from foraging to farming and all the impact it has had on us—it all happened in just a blink of an eye,” Larsen said.

“In the scale of a human lifespan it may seem like a long time, but it really is not.”

The research presented in the Special Feature also shows the amazing ability of humans to adjust to their surroundings.

“We are remarkably resilient creatures, as the last 12,000 years have shown,” he said.

“That gives me hope for the future. We will continue to adapt, to find ways to face challenges and to find ways to succeed. That is what we do as humans.”

More information:
Larsen, Clark Spencer, The past 12,000 years of behavior, adaptation, population, and evolution shaped who we are today, Proceedings of the National Academy of Sciences (2023). DOI: 10.1073/pnas.2209613120. doi.org/10.1073/pnas.2209613120

Provided by
The Ohio State University

Citation:
How the last 12,000 years have shaped what humans are today (2023, January 16)
retrieved 17 January 2023
from https://phys.org/news/2023-01-years-humans-today.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.



Read original article here

How a vanished Ice Age lake shaped the past and present of Missoula, Montana

Enlarge / Past shorelines left deposits that are still visible on the hills near the Missoula Valley.

Richard Forbes

Had the city of Missoula, Montana, existed thousands of years ago, it would have been under water.

During the last Ice Age, a sheet of ice 20 miles wide got stuck in the Idaho panhandle and blocked the Clark Fork River, creating glacial Lake Missoula. At its highest, the water level reached 4,250 feet above sea level—over 1,000 feet above the present city’s altitude. The ice sheet ultimately gave way to the pressure of the water, and glacial Lake Missoula drained catastrophically.

It’s estimated that the biggest flood discharge reached 386 million cubic feet per second. At that rate, it took the lake only a few days to drain, with its waters eventually reaching the Pacific Ocean.

The scariest thing is not the scale of this event—it’s that floods of this size happened multiple times. Thousands of years after that first flood, scientists finally pieced together whether it was a one-time deal by looking to the dirt for answers.

Signs of the past

In the fall of 1969, Rich Chambers drove southwest of Missoula along I-90 with his undergraduate adviser. They pulled over to the side of the road to look at a wall that ran 80 feet into the air. It was zebra-striped, with layers of dark and light sediments running horizontally up the slope.

Missoula is the second-biggest city in Montana, with a population of about 75,000, and it sits in a mountain valley. The University of Montana is known more for its forestry and law schools and less for the giant boulders sitting around campus or the lines on two mountains—visible from about anywhere on campus—that are remnants of the lake that once drowned the valley.

Chambers devoted his undergraduate and master’s work to glacial Lake Missoula, which formed behind the Cordilleran Ice Sheet between 14,000 and 21,000 years ago. The glacial lake would cover almost 3,000 square miles and hold as much water as Lake Ontario and Lake Erie combined.

Chambers’ adviser was David Alt, a well-renowned historian of glacial Lake Missoula. Something Alt wasn’t as familiar with, though, was the sediments left behind after the flood drained the lake—the sort of sediments that he and Chambers found themselves looking at off I-90.

“These are Lake Missoula sediments,” Alt said to Chambers as they stared at the zebra wall. “And nobody’s looking at them in detail.”

If there was to be anything new uncovered about the lake’s history, it would come from sediments like these. And there was some urgency in uncovering it—in the 1970s, there was a big back-and-forth brewing in the scientific community regarding how many times the lake may have drained and refilled.

Land of many lakes

Chambers started classifying Lake Missoula’s sediments and noticed two scales of zebra striping. On the large scale, he found about 40 alternating light and dark soil sequences up to several meters thick. These cycles, called rhythmites in geology-speak, are deposits where the light layers are made up of fine sand and silt deposited by rivers in the early stages of a lake’s filling, while the dark layers are made up of silt and clay that gather on the bottom of filled lakes.

Chambers then noticed that the dark layers had their own zebra stripes. The stripes-within-stripes at this scale are called varves, and they likely represented annual layers of sediment stacked on top of each other. The varves told geologists about the amount of time it took for the lake to fill. Assuming the varves represented annual stackings, Chambers said it took only an average of about 50 years for the lake to refill. Even though the lake’s depth decreased with each filling, that’s still a wild amount of water. At its peak, it was more than 500 cubic miles of water, about half the quantity held in Lake Michigan.

Zebra stripes in a deposit that once formed on the lake bottom.

Rich Chambers

Bit by bit, Chambers and Alt pieced together a picture of the area’s history. In a paper that Chambers and Alt co-authored, they suggested several decades might have passed between each lake draining and filling; in a different paper, Chambers concluded there was no evidence that the glacial lake had drained completely each time. He later argued that the last several lake drainages were less intense, which kept the floods from washing away deposits like the one seen at the roadcut on I-90.

That piece of land off the highway contains at least 800 years of history—and possibly more. It’s unclear how much sediment may have been removed from the record by subsequent floods. Each draining of glacial Lake Missoula could have taken with it evidence of earlier floods.

Read original article here

Above and beyond: key events in 2022 that shaped space exploration | Space

The year has been a blast in space exploration, from Nasa’s big step in returning to moon missions, to glimpses at the origins of the universe and hope that humanity could survive the doomsday scenario of an asteroid hurtling towards Earth.

These are the events that shaped 2022 in space advances:

Back to the moon

Nasa hadn’t sent a crew-capable spacecraft to the moon for half a century when Artemis 1 blasted off from Florida’s Cape Canaveral in November. Atop the mighty Space Launch System (SLS), the most powerful rocket in history, the unoccupied next-generation Orion capsule flew 1.3m miles on a 25-day flight to test the hardware and support systems for sending humans back to the lunar surface and beyond.

The Artemis I unmanned lunar rocket lifts off from Kennedy Space Center in Cape Canaveral, Florida. Photograph: Jim Watson/AFP/Getty Images

Orion splashed down in the Pacific Ocean on 11 December, 50 years to the day since two Apollo 17 astronauts became the last of only 12 moonwalkers in history. Mission managers are still assessing data from the Artemis mission but the program looks on track for a crewed lunar flyby in 2024 and a scheduled moon landing the year after.

A glimpse of creation

In July, the $10bn James Webb space telescope sent back the highest resolution images ever seen of distant galaxies as they were billions of years ago, promising astronomers a glimpse into the dawn of creation.

An image of Jupiter taken by James Webb space telescope, shows the planet’s weather patterns, tiny moons, altitude levels, cloud covers and auroras at the northern and southern poles. Photograph: Nasa/AFP/Getty Images

The stunning clear color pictures of the unseen universe were hailed by the Nasa chief, Bill Nelson, as a new era in astronomy, showcasing Webb’s ability to peer back 13.5bn years, close to the big bang. “We are going back almost to the beginning,” he said.

In November, Webb found two more galaxies, one that may have formed just 350m years after the big bang.

A moving occasion

In a “watershed moment for planetary defense” in September, Nasa crashed a multimillion-dollar, car-sized spacecraft into an asteroid the size of a football stadium and proved for the first time it could alter the orbit of a celestial body.

The Dart mission (Double Asteroid Redirection Test) was an unprecedented experiment of the space agency’s capacity to defend Earth from the doomsday scenario of a huge asteroid on a collision course.

The impact shortened the orbit of Dimorphos around the larger Didymos asteroid by about 32 minutes, to 11 hours and 23 minutes.

Private investigators

The first all-private crew of astronauts returned from the International Space Station (ISS) in April, the three wealthy paying guests joining a former space shuttle commander onboard the Axiom 1 flight on a SpaceX Falcon 9 rocket launched at Cape Canaveral.

Crew of the Ax-1 at a training session before the mission. Photograph: Axiom Space/AFP/Getty Images

The civilian astronauts, Larry Connor, Eytan Stibbe and Mark Pathy, paid an estimated $55m for the 17-day mission, during which they joined US and Russian crews aboard the ISS and conducted more than 25 research projects, incorporating regenerative medicine and space technology.

Former Nasa chief astronaut Peggy Whitson is slated to command Axiom 2 in May 2023.

Breath of fresh air

The potential for humans to one day live on the red planet came a step closer in August when researchers announced that a lunchbox-sized instrument named Moxie (Mars oxygen in-situ resource utilization experiment) had been generating breathable oxygen.

Technicians at Nasa’s jet propulsion laboratory lower the Moxie instrument into the belly of the Perseverance rover. Photograph: Nasa/JPL-Caltech/Reuters

Moxie, part of Nasa’s Perseverance astrobiology project on Mars, was successful in producing oxygen over seven experimental runs, in a variety of atmospheric conditions, day and night, through different Martian seasons. Each run produced at least 6g of oxygen an hour, similar to the rate of a modest tree on Earth.

Scaled-up versions of Moxie could become part of the Nasa Artemis program that aims to land humans on Mars in the 2030s.

Chinese space debris

China’s space program sparked global outrage in November when a chunk of a rocket used to deliver a module to its new Tiangong space station fell to Earth uncontrolled, triggering the closure of European airspace and hundreds of flight delays.

It was the second time in 2022 that parts of China’s Long March rockets had threatened populated areas, prompting calls from space experts for the “irresponsible” country to clean up its act. Chinese space debris has previously fallen on the Maldives and India.

China completed construction of Tiangong for a crew of three in 2022, and is already considering expansion.

Russia goes it alone

The Russian space agency Roscosmos announced in July it was to end its two-decade partnership with the US over the International Space Station, and planned to focus on building its own orbiting outpost.

Analysts linked the move to Russia’s invasion of Ukraine, as US-Russian tensions grew over the conflict. The announcement came barely three months after a crew of Russian cosmonauts boarded the ISS in the yellow and blue colors of the Ukraine flag.

Russia’s President Vladimir Putin reportedly replied “good” when Yuri Borisov, the newly appointed head of Roscosmos, told him Russia was out after fulfilling ISS obligations to 2024.

Commercial travelers

Boeing joined Elon Musk’s SpaceX in May as the only commercial companies to have docked their space vehicles at the International Space Station, a major step forward in its plans to ferry humans aboard its Starliner crew capsule.

SpaceX continues to dominate the commercial space market with two crewed missions to the ISS in 2022, among the 61 total launches it planned this year.

Boeing, a long-time partner of Nasa, has trailed SpaceX in development of a crew capsule. Its first crewed Starliner test flight has been delayed until no earlier than April 2023.

Read original article here

How Chewing Shaped Human Evolution

Humans spend about 35 minutes every day chewing. That adds up to more than a full week out of every year. But that’s nothing compared to the time spent masticating by our cousins: Chimps chew for 4.5 hours a day, and orangutans clock 6.6 hours.

The differences between our chewing habits and those of our closest relatives offer insights into human evolution. A study published Wednesday in the journal Science Advances explores how much energy people use while chewing, and how that may have guided — or been guided by — our gradual transformation into modern humans.

Chewing, in addition to keeping us from choking, makes the energy and nutrients in food accessible to the digestive system. But the very act of chewing requires us to expend energy. Adaptations to teeth, jaws and muscles all play a part in how efficiently humans chew.

Adam van Casteren, an author of the new study and a research associate at the University of Manchester in England, says that scientists haven’t delved too deeply into the energetic costs of chewing partly because compared with other things we do, such as walking or running, it’s a thin slice of the energy-use pie. But even comparatively small advantages can play a big role in evolution, and he wanted to find out if that might be the case with chewing.

To measure the energy that goes into chewing, Dr. van Casteren and his colleagues outfitted study participants with plastic hoods that look like “an astronaut’s helmet,” he said. The hoods were connected to tubes to measure oxygen and carbon dioxide from breathing. Because metabolic processes are fueled by oxygen and produce carbon dioxide, gas exchange can be a useful measure for how much energy something takes. The researchers then gave the subjects gum.

The participants didn’t get the sugary kind, though; the gum bases they chewed were flavorless and odorless. Digestive systems respond to flavors and scents, so the researchers wanted to make sure they were only measuring the energy associated with chewing and not the energy of a stomach gearing up for a tasty meal.

The test subjects chewed two pieces of gum, one hard and one soft, for 15 minutes each. The results surprised researchers. The softer gum raised the participants’ metabolic rates about 10 percent higher than when they were resting; the harder gum caused a 15 percent increase.

“I thought there wasn’t going to be as big a difference,” Dr. van Casteren said. “Very small changes in the material properties of the item you’re chewing can cause quite substantial increases in energy expenditure, and that opens up a whole universe of questions.”

Because chewing tougher food — or in this case, tougher gum — takes significantly more energy, these findings suggest that the metabolic costs of chewing may have played an important role in our evolution. Making food easier to process through cooking, mashing food with tools and growing crops optimized for eating might have dialed down the evolutionary pressure for us to be super-chewers. Our evolving chewing needs may have even shaped what our faces look like.

“One thing that we haven’t really been able to figure out is why the human skull is so funny-looking,” said Justin Ledogar, a biological anthropologist at East Tennessee State University, who was not involved with the study. Compared to our closest relatives, our facial skeletons are delicately built with jaws, teeth and chewing muscles that are all relatively small. “All this reflects a reduced reliance on forceful chewing,” he explained.

But he added that our flatter faces and shorter jaws let us bite more efficiently. “It makes the whole process of feeding just metabolically less costly,” Dr. Ledogar said. Humans developed ways to chew smarter, not harder. Dr. van Casteren, who hopes to continue his research using actual foods, says he’s excited by the prospect of learning more about how humans evolved.

“To know about the environmental and societal and dietary causes that led us to get here, it’s just infinitely interesting to me,” he said, because it enables humankind to “try and work out the foggy road ahead.”

Read original article here

Hubble Space Telescope images twisted galaxy shaped by a big neighbor

This fresh Hubble Space Telescope image looks like a gassy disaster unfolding deep in space.

The image shows the galaxy NGC 3718, which NASA officials say is a “highly disturbed spiral,” meaning its formation was disrupted. As the galaxy gets into the gravitational well from the neighboring galaxy NGC 3729, that galactic interaction pulls NGC 3718 into an S-shaped warp. The galaxies are separated by 150,000 light-years, with NGC 3729 not shown in this view from the Hubble Space Telescope.

“Hubble’s view of this portion of NGC 3718 shows the sinuous, twisting dust lane in detail as it sweeps by the core of the galaxy and curves into the surrounding gas,” NASA officials said in a May 24 statement (opens in new tab). “Both the galaxy’s gas and dust lane are similarly distorted into this unique configuration.” 

Related: The best Hubble Space Telescope images of all time!

NGC 3718 is also called Arp 214, recognizing its placement in the 1966 Atlas of Peculiar Galaxies, constructed by Halton Arp to look at galaxies with unusual structures.

The Hubble telescope was focusing on the nucleus of the galaxy, which is hard to see because of the amount of dust in the way. Infrared light allowed Hubble to peer through “as part of a study of the central regions of disk-shaped galaxies, with prominent bulges of stars in multiple environments,” NASA officials said.

The goals of the study included learning how supermassive black hole masses might be related to galactic “bulges” about the center, as well as how star formation happens throughout a galaxy.

A Hubble Space Telescope image of galaxy NGC 3718 (inset) compared with a Sloan Digital Sky Survey image of the region surrounding it (left). (Image credit: NASA, ESA, L. Ho (Peking University), and DSS; Image Processing: Gladys Kober (NASA/Catholic University of America))

NASA’s James Webb Space Telescope aims to extend Hubble’s generation of work by peering at galaxies close to the start of the universe. Webb is expected to start work this summer.

Some of Webb’s research will focus on matters such as galactic variety, mergers and collisions, as well as more details on galaxies’ relationships with supermassive black holes, according to NASA (opens in new tab).

Follow Elizabeth Howell on Twitter @howellspace (opens in new tab). Follow us on Twitter @Spacedotcom (opens in new tab) or Facebook. 



Read original article here

Changes in vegetation shaped global temperatures over last 10,000 years

Credit: Unsplash/CC0 Public Domain

Follow the pollen. Records from past plant life tell the real story of global temperatures, according to research from a climate scientist at Washington University in St. Louis.

Warmer temperatures brought plants—and then came even warmer temperatures, according to new model simulations published April 15 in Science Advances.

Alexander Thompson, a postdoctoral research associate in earth and planetary sciences in Arts & Sciences, updated simulations from an important climate model to reflect the role of changing vegetation as a key driver of global temperatures over the last 10,000 years.

Thompson had long been troubled by a problem with models of Earth’s atmospheric temperatures since the last ice age. Too many of these simulations showed temperatures warming consistently over time.

But climate proxy records tell a different story. Many of those sources indicate a marked peak in global temperatures that occurred between 6,000 and 9,000 years ago.

Thompson had a hunch that the models could be overlooking the role of changes in vegetation in favor of impacts from atmospheric carbon dioxide concentrations or ice cover.

“Pollen records suggest a large expansion of vegetation during that time,” Thompson said.

“But previous models only show a limited amount of vegetation growth,” he said. “So, even though some of these other simulations have included dynamic vegetation, it wasn’t nearly enough of a vegetation shift to account for what the pollen records suggest.”

In reality, the changes to vegetative cover were significant.

Early in the Holocene, the current geological epoch, the Sahara Desert in Africa grew greener than today—it was more of a grassland. Other Northern Hemisphere vegetation including the coniferous and deciduous forests in the mid-latitudes and the Arctic also thrived.

Thompson took evidence from pollen records and designed a set of experiments with a climate model known as the Community Earth System Model (CESM), one of the best-regarded models in a wide-ranging class of such models. He ran simulations to account for a range of changes in vegetation that had not been previously considered.

“Expanded vegetation during the Holocene warmed the globe by as much as 1.5 degrees Fahrenheit,” Thompson said. “Our new simulations align closely with paleoclimate proxies. So this is exciting that we can point to Northern Hemisphere vegetation as one potential factor that allows us to resolve the controversial Holocene temperature conundrum.”

Understanding the scale and timing of temperature change throughout the Holocene is important because it is a period of recent history, geologically speaking. The rise of human agriculture and civilization occurred during this time, so many scientists and historians from different disciplines are interested in understanding how early and mid-Holocene climate differed from the present day.

Thompson conducted this research work as a graduate student at the University of Michigan. He is continuing his research in the laboratory of climate scientist Bronwen Konecky at Washington University.

“Overall, our study emphasizes that accounting for vegetation change is critical,” Thompson said. “Projections for future climate change are more likely to produce more trustworthy predictions if they include changes in vegetation.”


Machine learning helps identify climatic thresholds that shape the distribution of natural vegetation


More information:
Alexander J. Thompson, Northern Hemisphere vegetation change drives a Holocene thermal maximum, Science Advances (2022). DOI: 10.1126/sciadv.abj6535. www.science.org/doi/10.1126/sciadv.abj6535
Provided by
Washington University in St. Louis

Citation:
Changes in vegetation shaped global temperatures over last 10,000 years (2022, April 15)
retrieved 16 April 2022
from https://phys.org/news/2022-04-vegetation-global-temperatures-years.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.



Read original article here

Record-breaking simulation hints at how climate shaped human migration



The early human species Homo heidelbergensis (skull shown) might have been able to spread across Earth because wetter, more migration-friendly weather conditions arose, according to a climate model.Credit: Javier Trueba/MSF/Science Photo Library

A colossal simulation of the past two million years of Earth’s climate provides evidence that temperature and other planetary conditions influenced early human migration — and possibly contributed to the emergence of the modern-day human species around 300,000 years ago.

The finding is one of many to come out of the largest model so far to investigate how changes in Earth’s movement have influenced climate and human evolution, published in Nature1 today. “This is another brick in the wall to support the role of climate in shaping human ancestry,” says Peter de Menocal, director of the Woods Hole Oceanographic Institution in Falmouth, Massachusetts.

The idea that climate might have a significant role in human evolution has been around since at least the 1920s2, when scientists started debating whether drier conditions had led early human ancestors to begin walking on two feet, to adapt to life on the savannah. But so far, researchers have struggled to provide strong evidence that climate played a part in shaping humanity.

Orbital influence

In the latest study, Axel Timmermann, a climate physicist at Pusan National University in South Korea, and his colleagues ran a climate model on a supercomputer for six months to reconstruct how temperature and rainfall might have shaped what resources were available to humans over the past few million years. Specifically, the researchers examined how long-term fluctuations in climate brought about by Earth’s astronomical movement might have created the conditions to spur human evolution.

The push and pull of other planets alters Earth’s climate by changing both the planet’s tilt, and the shape of its orbit. Over 41,000-year cycles, Earth’s tilt oscillates, affecting the intensity of seasons and changing how much rain falls over the tropics. And over 100,000-year cycles, Earth goes from having a more circular orbit — which brings more sunlight and longer summers — to having a more elliptical orbit, which reduces sunlight and can lead to periods of glacial formation.

Timmermann and his colleagues used a simulation that incorporated these astonomical changes, and then combined their results with thousands of fossils and other archaeological evidence to work out where and when six species of humans — including the early Homo erectus and the modern Homo sapiens — could have lived.

Movements and mixing

The study pumped out a dizzying amount of data, and Timmermann says that several interesting patterns emerged. For instance, the researchers’ analysis showed that an early human species, Homo heidelbergensis, started expanding its habitat around 700,000 years ago. Some scientists have thought that this species might have given rise to a slew of others across the globe, including Neanderthals (Homo neanderthalensis) in Eurasia and H. sapiens somewhere in Africa.

The model suggests that the distribution of H. heidelbergensis across the globe was possible because a more elliptical orbit created wetter climate conditions that allowed the species to migrate more widely. The simulation also showed that the most habitable regions, in terms of climate, shifted over time, and the fossil record tracked along with them.

“The global collection of skulls and tools is not randomly distributed in time,” Timmermann says. “It follows a pattern” that overlaps with climate change driven by Earth’s movement. “This is amazing to me — here is a pattern that nobody so far was able to see.”

One part of this pattern might provide fresh insight into where and how our own species emerged. Some genetic studies of modern-day hunter-gather groups in sub-Saharan Africa — who tend to be genetically isolated — suggest that H. sapiens is the outcome of a single evolutionary event in southern Africa. But other studies point to a more complex story, in which humanity began as a hotchpotch of many different groups of ancient Africans that, together, evolved into modern-day humans.

Timmermann and his colleagues say that their climate reconstruction favours the single-evolutionary-path hypothesis. The model suggests that our species evolved when H. heidelbergensis in southern Africa started losing liveable habitat during an unusually warm period. This population could have evolved into H. sapiens by adapting to the hotter, drier conditions.

But this finding is unlikely to end debate. “To make the case that a particular climate event led to a speciation event is really hard”, in part because of gaps in the fossil and genetic record, says Tyler Faith, a palaeobiologist at the University of Utah in Salt Lake City.

The same goes for many of the other patterns reported in the paper. “The people who’ve spent a career studying this will either be in violent agreement or disagreement with the propositions here,” de Menocal says. The model, however, is a “phenomenal accomplishment in and of itself” and “gives you a template to ask these questions”.

Most researchers that spoke to Nature say that more evidence will be needed to prove that astronomical cycles influenced the trajectory of human ancestry. “If solving the mystery of climate change and human evolution could be dealt with in one paper, it would have been done 40 years ago,” Faith says.

Which is why Timmermann and his colleagues are planning to run even larger models, including ones that integrate genetic data.

Read original article here