Here’s the video: https://www.youtube.com/watch?v=hSeXeez5dv8

Here’s the video: https://www.youtube.com/watch?v=lDxnFge00Vc

Elon Musk has big ambitions to colonize Mars by 2050, and a new scientific discovery could make those dreams a reality.

A team of scientists have proposed an ‘innovative’ way to warm the Red Planet by more than 18 degrees Fahrenheit in just a matter of months, which they believe would be enough to sustain human life.

They proposed injecting large quantities of Martian dust into the atmosphere to improve its ability to trap heat, just like water vapor and carbon dioxide do on Earth.

Shooting about 10 liters of dust, consisting of iron and aluminum, per second for at least a decade could warm the planet from -85F to 86F.

A groundbreaking new discovery suggests that Elon Musk’s dream of terraforming Mars might not be as far-fetched as people think.

Musk himself has said that he plans to use the natural resources on Mars to ‘terraform’ its existing atmosphere and make the planet warmer, wetter and overall more like Earth.

The idea of being stuck in space might sound like the plot of the latest science fiction blockbuster. But it has become a reality for Suni Williams and Butch Wilmore – two unlucky astronauts who are potentially stuck on the International Space Station (ISS) until 2025, despite only expecting to be there for eight days. Although the views might be out of this world, the ISS is far from the ideal destination for an impromptu eight-month trip. With little spare room and zero gravity, even simple tasks like eating or going to the toilet can be extremely difficult. And whether it’s in their phone box-sized bedrooms or on the vacuum-powered toilet, the astronauts aboard the orbiting station can often be cramped, smelly, and uncomfortable.

This study suggests he may be onto something.

‘It’s not that often you get some really quite new, innovative idea for terraforming,’ Colin McInnes, a space engineer at the University of Glasgow not involved with the work, told Science Magazine.

‘The gap between where Mars is and where Mars could be for habitability is narrower than we might think,’ he added.

The researchers’ approach is actually based on the same atmospheric mechanism that’s driving climate change here on Earth: the greenhouse effect.

Currently, Mars’ atmosphere is so thin that heat from the sun easily escapes the planet’s surface.

The microscopic size and spherical shape of Martian dust mean that it isn’t great at absorbing radiation or reflecting heat back down to the surface.
But the research team believes they could use the iron and aluminum in the dust to engineer nine-micrometer-long rods.

That’s roughly twice the size of a Martian dust particle, but smaller than a speck of glitter.

Currently, the surface of Mars is a freezing, barren desert. But scientists have come up with a simple way to warm up the Red Planet.

Terraforming Mars’ atmosphere would bring us one step closer to establishing a human colony on the red planet.

When the researchers tested how their particles would absorb heat radiation and reflect it down to the planet’s surface, they found ‘unexpectedly huge effects,’ Samaneh Ansari, a Ph.D. student at Northwestern University and the study’s lead author, told Science Magazine.

This approach would require about two million tons of particles per year, but manufacturing them would be relatively easy because the ingredients are right there on Mars.

That sets this new approach apart from previous schemes to globally warm the Red Planet.

By comparison, this method would be roughly 5,000 times more efficient, the researchers claimed.

This strategy would still take decades, but it seems logistically easier than any other ideas proposed so far.

Warming up Mars would be a critical first step towards making this planet a suitable home for humans, or any other life form for that matter.

It would free up the little water that’s frozen in polar ice caps beneath the planet’s surface, and make Mars a more suitable place for agriculture and out own bodies.

Mars’ atmosphere is too thin to trap heat at the surface. Scientists want to inject it with engineered dust to make it more insulating.

This is all great news for Musk. But warming up Mars is just one step down a long road he’ll need to travel before he can colonize the Red Planet.

Even with this new atmosphere, humans still wouldn’t be able to breathe the air on Mars because it doesn’t contain enough oxygen.

Plus, the air pressure on Mars is 150 times lower than on Earth, which would cause human blood to boil.

Musk will have to solve these problems and more before he builds a bustling Martian metropolis. But this new research brings him a little bit closer to realizing his dream.

Source: https://www.msn.com/en-za/news/other/humans-closer-to-living-on-mars-with-new-theory-to-terraform-planet/ar-AA1oC7jL?ocid=msedgdhp&pc=U531&cvid=0d319a90373241dcabc4adfd85339b2f&ei=32

Here’s the video: https://www.youtube.com/watch?v=COaWZtI7r_Y

Here’s the video: https://www.youtube.com/watch?v=kx4UzkzjERM&t=214s

On September 24, 2023, NASA’s OSIRIS-REx spacecraft dropped a capsule to Earth containing pristine carbonaceous regolith collected from the near-Earth asteroid Bennu. These samples were obtained after the probe took an impressive, seven-year roundtrip journey through the solar system and back.

Since these space rock pieces arrived (approximately 120 grams of sample, to be precise) scientists have highly anticipated an analysis of the specimens that can tell us what molecules lie within Bennu. They’ve been hoping to find clues about the history of our solar system, seeing as Bennu should’ve been present when our cosmic neighborhood was coming together, and prebiotic molecules that might provide insights into the origin of life on Earth. It’s possible, many experts speculated, that these samples could host the seeds of other essential ingredients, such as water, that could have contributed to Earth’s habitability if they ended up on our planet, too.

"The sample we returned is the largest reservoir of unaltered asteroid material on Earth right now," Dante Lauretta, co-lead author of the paper and principal investigator for OSIRIS-REx at the University of Arizona, Tucson, said in a statement.

While initial studies did indeed indicate the OSIRIS-REx samples exhibited evidence of carbon and water, perhaps even more remarkable is the team’s recent, and unexpected, discovery of magnesium-sodium phosphate. This is an ionic compound composed of the magnesium cation (Mg2+), sodium cation (Na?) and phosphate anion (PO43-).

On Earth, magnesium-sodium phosphate can be found in certain minerals and geological formations. According to a NASA press release, however, its presence on Bennu surprised the research team because it wasn’t seen in the OSIRIS-REx probe’s remote sensing data prior to sample collection. The team says its presence "hints that the asteroid could have splintered off from a long-gone, tiny, primitive ocean world."

"The presence and state of phosphates, along with other elements and compounds on Bennu, suggest a watery past for the asteroid," said Lauretta. "Bennu potentially could have once been part of a wetter world. Although, this hypothesis requires further investigation."

The OSIRIS-REx spacecraft obtained a sample of Bennu’s regolith on October 20, 2020 using its Touch-and-Go Sample Acquisition Mechanism (TAGSAM), which comprises a specialized sampler head situated on an articulated arm. Bennu is a small B-type asteroid, which are relatively uncommon carbonaceous asteroids. "[Bennu] was selected as the mission target in part because telescopic observations indicated a primitive, carbonaceous composition and water-bearing minerals," stated the team in their paper.

Further analysis on the samples revealed the prevailing component of the regolith sample is magnesium-bearing phyllosilicates, primarily serpentine and smectite — types of rock typically found at mid-ocean ridges on Earth. A comparison of these serpentinites with their terrestrial counterparts provides possible insights into Bennu’s geological past. "Offering clues about the aqueous environment in which they originated," wrote the team.

While Bennu’s surface may have been altered by water over time, it still preserves some of the ancient characteristics scientists believe were present during the early solar system’s days. Bennu’s surface materials still contain some original features from the cloud of gas and dust from which our solar system’s planets formed — known as the protoplanetary disk.

The team’s study also confirmed the asteroid is rich in carbon, nitrogen and some organic compounds — all of which, in addition to the magnesium phosphate, are essential components for life as we know it on Earth.

"These findings underscore the importance of collecting and studying material from asteroids like Bennu — especially low-density material that would typically burn up upon entering Earth’s atmosphere," said Lauretta. "This material holds the key to unraveling the intricate processes of solar system formation and the prebiotic chemistry that could have contributed to life emerging on Earth."

In addition to the important scientific discoveries made during this mission, it underscores the significance of sample return in unraveling the geological and geochemical intricacies of asteroids like Bennu, and their implications for the formation and evolution of the solar system.

"The data we have presented here are only the tip of the iceberg: there is likely more about the sample that we do not know than we do know," concluded the scientists.

The paper about these results was published on June 26 in the journal Meteoritics & Planetary Science.

Source: https://www.space.com/nasa-osiris-rex-sample-return-phosphate-ocean-world?utm_term=AF536F6D-055D-443A-91F7-FD448D0CCA73&lrh=4cd1bd23c622eeb1274411ac3b55b43215b8c098a20f14a3285c9e8ae13a98ca&utm_campaign=58E4DE65-C57F-4CD3-9A5A-609994E2C5A9&utm_medium=email&utm_content=48248DFA-EB74-4B4A-B41E-0744E07D5CC2&utm_source=SmartBrief

New research suggests the timing of human gestation is not a compromise between the size of a woman’s hips and the size of a baby’s head. Instead, it’s determined by a woman’s energy limits.

Have you ever wondered why women stay pregnant for nine months? For decades, anthropologists have explained the timing of human gestation and birth as a balance between two constraints: the size of a women’s hips and the size of a newborn’s brain. But new research says that’s not the case. Instead, the timing of childbirth occurs when women’s bodies can no longer keep up with the energy demands of pregnancy. That happens at around nine months, Holly Dunsworth of the University of Rhode Island and colleagues report online August 27 in the Proceedings of the National Academy of Sciences.

The traditional explanation of gestation length is known as the obstetric dilemma. The hypothesis suggests that the width of the pelvis, and thus the width of the birth canal, is limited by the demands of efficient upright walking. But as brain size expanded over hominid evolution, heads got bigger. To make sure a baby’s head could fit through the birth canal, gestation decreased and babies were born at an earlier stage of development; today, newborns enter the world with the least developed brain of all primates at less than 30 percent adult size.

Dunsworth and her colleagues wanted to see if they could find any actual evidence to support the obstetric dilemma. First, they considered gestation length. Traditionally, human gestation has been considered short when looking at how much additional growth the brain needs to reach adult size. But such a measure is unfair when compared to other primates since humans have abnormally large brains, the researchers say. Instead, Dunsworth’s team compared gestation length to maternal body size and found humans actually have relatively long pregnancies—37 days longer than would be expected for a typical primate our size. Our gestation is also relatively extended compared with chimpanzees or gorillas, suggesting pregnancies got longer, not shorter, in hominids.

The team also looked for evidence that widening the pelvis to accommodate bigger brained babies would make walking less efficient. Researchers have assumed that broadening the hips would increase the force needed by hip muscles to walk and run, thus making locomotion less energy efficient. But one recent study shows the dimensions of the hips don’t actually affect the muscle’s required force, calling into question the long-held belief that wider hips would interfere with women’s walking. Furthermore, the team calculated how much wider the hips would have to be if humans were born with the same brain development as chimps (40 percent adult size). All that would be needed is a three-centimeter increase. Women’s hips already vary by three or more centimeters, the researchers say, suggesting that hip size really doesn’t limit gestation.

Instead, gestation is determined by energy. Studies of mammals show that during pregnancy females reach their species’ “metabolic ceiling,” the upper limit of the amount of energy they can expend. In humans, the metabolic ceiling is 2 to 2.5 times the baseline amount of energy needed during rest. Dunsworth and her colleagues say women reach that limit by their sixth month of pregnancy. Then at nine months, the energy demands of a fetus go beyond this metabolic threshold. “Extending gestation even by a month would likely require metabolic investment beyond the mother’s capacity,” the team writes.

But even though hip size doesn’t appear to limit the size of a baby’s head, women around the world often have trouble delivering babies because of the tight fit of the head going through the birth canal. One possible explanation is that childbirth has only become problematic recently in human evolution. Changes in diet that have led to increased energy consumption may be allowing women to produce bigger babies, and natural selection hasn’t had enough time to broaden the hips. Figuring out why modern childbirth is so difficult, and dangerous, is an area that needs further research.

Source: https://www.smithsonianmag.com/science-nature/timing-of-childbirth-evolved-to-match-womens-energy-limits-18018563/

Here’s the video: https://www.youtube.com/watch?v=LVU-hwZgnuA

Some species of pterosaurs flew by flapping their wings while others soared like vultures, demonstrates a new study published in the Journal of Vertebrate Paleontology.

It has long been debated whether the largest pterosaurs could fly at all.

However, "remarkable" and "rare" three-dimensional fossils of two different large-bodied azhdarchoid pterosaur species—including one new to science—have enabled scientists to hypothesize that not only could the largest pterosaurs take to the air, but their flight styles could differ too.

The new findings are led by experts from the University of Michigan, in the US; the Natural Resources Authority and Yarmouk University, in Jordan; and the Saudi Geological Survey, in Saudi Arabia.

Their paper details how these fossils—which date back to the latest Cretaceous period (approximately 72 to 66 million years ago)—were remarkably three-dimensionally preserved within the two different sites that preserve a nearshore environment on the margin of Afro-Arabia, an ancient landmass that included both Africa and the Arabian Peninsula.

The research team used high-resolution computed tomography (CT) scans to then analyze the internal structure of the wing bones.

"The dig team was extremely surprised to find three-dimensionally preserved pterosaur bones. This is a very rare occurrence," explains lead author Dr. Kierstin Rosenbach, from the Department of Earth and Environmental Sciences of the University of Michigan.

"Since pterosaur bones are hollow, they are very fragile and are more likely to be found flattened like a pancake, if they are preserved at all.

"With 3D preservation being so rare, we do not have a lot of information about what pterosaur bones look like on the inside, so I wanted to CT scan them.

"It was entirely possible that nothing was preserved inside, or that CT scanners were not sensitive enough to differentiate fossil bone tissue from the surrounding matrix."

Luckily, though, what the team uncovered was "remarkable," via "exciting internal structures not only preserved, but visible in the CT scanner."

CT scans reveal one soars, one flaps
Newly collected specimens of the already-known giant pterosaur, Arambourgiania philadelphiae, confirm its 10-meter wingspan and provide the first details of its bone structure. CT images revealed that the interior of its humerus, which is hollow, contains a series of ridges that spiral up and down the bone.

This resembles structures in the interior of wing bones of vultures. The spiral ridges are hypothesized to resist the torsional loadings associated with soaring (sustained powered flight that requires launch and maintenance flapping).

The other specimen analyzed was the new-to-science Inabtanin alarabia, which had a five-meter wingspan. The team named it after the place where it was excavated—near a large grape-colored hill, called Tal Inab. The generic name combines the Arabic words "inab," for grape, and "tanin" for dragon. "Alarabia" refers to the Arabian Peninsula.

Inabtanin is one of the most complete pterosaurs ever recovered from Afro-Arabia, and the CT scans revealed the structure of its flight bones was completely different from that of Arambourgiania.

Dr. Kierstin Rosenbach assessing the Arambourgiania humerus with the Inabtanin material in the background. Credit: Dr. Kierstin Rosenbach
The interior of the flight bones were crisscrossed by an arrangement with struts that match those found in the wing bones of modern flapping birds.

This indicates it was adapted to resist bending loads associated with flapping flight, and so it is likely that Inabtanin flew this way—although this does not preclude occasional use of other flight styles too.

"The struts found in Inabtanin were cool to see, though not unusual," says Dr. Rosenbach. "The ridges in Arambourgiania were completely unexpected, we weren’t sure what we were seeing at first. Being able to see the full 3D model of Arambourgiania’s humerus lined with helical ridges was just so exciting."

What explains this difference?
The discovery of diverse flight styles in differently-sized pterosaurs is "exciting," the experts state, because it opens a window into how these animals lived. It also poses interesting questions, like to what extent flight style is correlated with body size and which flight style is more common among pterosaurs.

"There is such limited information on the internal bone structure of pterosaurs across time, it is difficult to say with certainty which flight style came first," Dr. Rosenbach adds. "If we look to other flying vertebrate groups, birds and bats, we can see that flapping is by far the most common flight behavior. Even birds that soar or glide require some flapping to get in the air and maintain flight.

"This leads me to believe that flapping flight is the default condition, and that the behavior of soaring would perhaps evolve later if it were advantageous for the pterosaur population in a specific environment; in this case the open ocean."

Co-author Professor Jeff Wilson Mantilla, Curator at Michigan’s Museum of Paleontology, and Dr. Iyad Zalmout, from the Saudi Geological Survey, found these specimens in 2007 at sites in the north and south of Jordan.

Professor Jeff Wilson Mantilla says the "variations likely reflect responses to mechanical forces applied on the pterosaurs’ wings during flight."

Enabling further study of vertebrate flight
Concluding, Dr. Rosenbach states, "Pterosaurs were the earliest and largest vertebrates to evolve powered flight, but they are the only major volant group that has gone extinct. Attempts to-date to understand their flight mechanics have relied on aerodynamic principles and analogy with extant birds and bats.

"This study provides a framework for further investigation of the correlation between internal bone structure and flight capacity and behavior, and will hopefully lead to broader sampling of flight bone structure in pterosaur specimens."

Source: https://phys.org/news/2024-09-pterosaurs-soar-flight-capability-giants.html

Discovering life beyond Earth may well start with a sniff, a whiff of some chemical that scientists struggle to explain without invoking a strange, shadowy microbe. That first step has happened on Mars and on a few distant moons, and now, scientists suggest, on Venus.

A team of astronomers announced today (Sept. 14) that it has spotted the chemical fingerprint of phosphine, which scientists have suggested may be tied to life, in the clouds of the second rock from the sun. The finding is no guarantee that life exists on Venus, but researchers say it’s a tantalizing find that emphasizes the need for more missions to the hot, gassy planet next door.

"The interpretation that it’s potentially due to life, I think, is probably not the first thing I would go for," Victoria Meadows, an astrobiologist at the University of Washington who was not involved in the new research, told Space.com.

But it is an intriguing detection, she said, and one that emphasizes how we overlook our neighbor. "We have some explaining to do," she continued. "This discovery especially is just another reminder of how much more we have yet to learn about Venus."

The new research builds on the idea that, although the surface of Venus endures broiling temperatures and crushing pressures, conditions are much less harsh high up in the clouds. And scientists have realized that Earth’s own atmosphere is full of tiny life. Suddenly, microbes in the sweet spot of Venus’s atmosphere, where temperatures and pressures mimic those on Earth, don’t seem quite so outlandish.

The discovery
The scientists behind the new research wanted to look for phosphine. Researchers have recently wondered whether the chemical could be a good biosignature, a compound astronomers target in looking for life. It should break down quickly in atmospheres that are rich in oxygen, like those of Earth and Venus, and on Earth, when it isn’t being made by human industrial processes, it seems to be found near certain kinds of microbes.

Jane Greaves, an astronomer at the University of Cardiff in the U.K. and lead author of the new research, realized that she could use a telescope she knew well to check for it in the atmosphere of Venus, she told Space.com.

"Looking for it in Venus might be really peculiar, but it’s not hard to do and it wouldn’t take that many hours of telescope time," Greaves said she thought at the time. "Why not give it a go?" So on five separate mornings in June 2017, the astronomers used the James Clerk Maxwell Telescope in Hawaii to stare at Venus.

And then the observations sat around on a computer for a year and a half, Greaves said, without her managing to find time to study them.

"I thought, well, just before we throw this away, I’ll have a final go at [analyzing the data]," she said. "There was this line and it just wouldn’t go away, and it seemed like it wasn’t imaginary anymore. I was just completely stunned."

That line is one stripe of a spectrum, a chemical barcode that scientists can read in a telescope’s observations of light. Each chemical has its own unique fingerprint of lines and blank spaces; match enough lines and you can identify a mystery substance.

But the observations in the new research focus on only one of the lines in phosphine’s barcode, Meadows said, so she isn’t quite convinced the new findings represent a conclusive identification of phosphine.

"Until we can go and get another piece of that barcode … we can’t discriminate between which kind of barcode we’re looking at," Meadows said. "I think they make a good case for it being phosphine in there, but I think they don’t have what I would consider a slam-dunk detection yet."

The researchers haven’t tackled that aspect yet, but Greaves and her colleagues did arrange to use the Atacama Large Millimetre/submillimetre Array (ALMA) in March 2019 to look for the chemical again and make sure the detection wasn’t just a telescopic hiccup.

A new image of Venus shows the view ALMA had during its observations for the new research.

A new image of Venus shows the view ALMA had during its observations for the new research. (Image credit: ALMA (ESO/NAOJ/NRAO), Greaves et al.)
ALMA gathered a few hours of data, which also revealed more phosphine than the scientists expected — not a huge amount in the grand scheme of things, but about 20 particles out of every billion, according to the research.

"I was braced for disappointment, but it was amazing," Greaves said.

That abundance is significantly more phosphine than she had expected to see. The way the telescopes’ observations work, the chemical must have been more than 30 miles (50 kilometers) above the Venusian surface. That’s about the same altitude at which a different recent paper with some shared co-authors suggests microbial life could survive in spore form.

So Greaves and her colleagues set to work considering what might have created all that phosphine: Perhaps volcanoes erupting or lightning striking, or perhaps meteors melting in the atmosphere or winds pulling particles off the planet’s surface. But none of these explanations seemed sufficient to them.

As usual, struggling to make more conventional explanations check out does not mean that scientists think they’ve found life. But the possibility of tiny Venusian bugs has gradually become more plausible — and researchers focused on our neighboring world say that’s important, whether or not there’s actual life to find.

"Either it’s a mistaken identity but we don’t know what the chemical is, or some strange chemistry that we are not aware of — or biology," Sanjay Limaye, an atmospheric scientist at the University of Wisconsin, Madison, who wasn’t involved in the new research, told Space.com. "It’s a question of if it looks like a duck, quacks like a duck, walks like a duck, do you call it life or not? We won’t know until we go there and find out."

As tantalizing as the detection of phosphine on Venus may be, scientists not involved with the new research worry that it makes a few big leaps, even before the massive potential implications of a detection of life.

Some were unconvinced that phosphine was a reliable fingerprint of living organisms. The single phosphorus molecule surrounded by three hydrogen molecules is, on Earth, a rarity and short-lived: some industrial processes produce it, and it’s affiliated with some types of bacteria living in particularly strange environments. It quickly transforms in Earth’s oxygen-rich atmosphere and should in that of Venus as well, which is intriguing for scientists looking for alien breath. But the excitement about phosphine may well be premature.

"The phosphine link to the biological world is very, very faint and needs to be corroborated simply by going to the lab and doing experiments," Tetyana Milojevic, a biochemist at the University of Vienna not involved in the new research, told Space.com.

She argues that phosphine has only been found near microbes, not produced by it, and that the compound seems to be released by the chemical decay of biological material. So before scientists can use phosphine as a potential biosignature, they need to get into the lab and really understand whether and how microbes produce phosphine, a process that scientists eyeing Mars completed for methane long ago.

Alas, those experiments aren’t quite as simple for phosphine, Matthew Pasek, an astrobiologist and geochemist at the University of South Florida who has worked on phosphorus cycling issues but was not involved in the new research, told Space.com. "Phosphine is kind of nasty, so we don’t like playing with it, so we don’t actually understand how it gets made through natural processes very well," Pasek said. "It’s always been kind of relegated to the background of phosphorus chemistry."

Greaves said that she’s confident phosphine is a biosignature on Earth, but does hope that the scientific community can take on these sorts of lab experiments and otherwise build on her team’s work.

The idea of phosphine as a biosignature may have another fatal flaw. Venus is now the fourth planet where scientists have detected phosphine: two gas giants and Earth. The new detection shows phosphine levels on Venus about equal to those on Jupiter and Saturn. But that’s significantly more abundant — 1,000 times more abundant — than on Earth, Pasek said.

"For the one place that it is likely biological, there’s a lot less of it even there," he said. "So it’s kind of weird that if it is biology on Venus, that’s a whole lot of phosphine that is generating for weird reasons."

It is Venus, after all — our mysterious neighbor.

Greaves and her colleagues plan to continue studying Venus from the ground, although she said that the coronavirus pandemic has interfered with those observations. Meadows said she hopes for analysis that would cover some of those other lines in the phosphine barcode. And of course some of the phosphine investigations can be done right here in laboratories.

But the details of this massive puzzle aren’t likely the sort of thing that can be seen clearly from the surface of Earth. And spacecraft tend to zip around Venus, keeping a safe distance from its hostile environments. Designing machinery that can withstand its clouds and surface is so difficult that no spacecraft has ventured into the atmosphere in decades.

"It should implore NASA and other space agencies to look at Venus as a target for astrobiology investigation, which means they should pump some money into the development of capable aerial platforms," Limaye said of the new research.

There’s no shortage of ideas to choose from when it comes to dreamed-of Venus missions that could tackle the atmosphere, whether your taste runs to more traditional designs or unorthodox options like blimps, balloons or commercially built spacecraft.

"It’s time to figure out Venus," James Garvin, a planetary scientist at NASA’s Goddard Space Flight Center in Maryland, who wasn’t involved in the new research but is the principal investigator on a Venus atmospheric probe mission that NASA is evaluating, told Space.com. "If we ignore it too long, we could be missing the forest for the trees, and that would never be good."

He thinks engineering has caught up with the challenges of the Venusian atmosphere.

"The time is ripe for thinking about what the atmosphere is telling us within itself. It’s just this beautiful laboratory next door that has been tough enough that we’ve ignored it for 35 years," Garvin said. "The atmosphere is kind of calling us, whispering in the night, ‘Hey, I may have something that you should think about.’ And we haven’t been."

The research is described in a paper published today (Sept. 14) in the journal Nature Astronomy.

Source: https://www.space.com/venus-clouds-possible-life-chemical-discovery.html