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Meltwater is hydro-fracking Greenland’s ice sheet through millions of hairline cracks – destabilizing its internal structure

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Meltwater is hydro-fracking Greenland's ice sheet through millions of hairline cracks – destabilizing its internal structure

Richard Bates and Alun Hubbard kayak a meltwater stream on Greenland's Petermann Glacier, towing an ice radar that reveals it's riddled with fractures.
Nick Cobbing.

Alun Hubbard, University of Tromsø

I'm striding along the steep bank of a raging white- torrent, and even though the canyon is only about the width of a highway, the 's flow is greater than that of London's Thames. The deafening roar and rumble of the cascading water is incredible – a humbling reminder of the raw power of nature.

As I round a corner, I am awestruck at a completely surreal sight: A gaping fissure has opened in the riverbed, and it is swallowing the water in a massive whirlpool, sending up huge spumes of spray. This might sound like a computer-generated scene from a blockbuster action – but it's real.

Alun Hubbard discusses the mechanics of moulins and rappels into one in the second half of this introduction to the Greenland ice sheet.

A moulin is forming right in front of me on the Greenland ice sheet. Only this really shouldn't be here – current scientific understanding doesn't accommodate this reality.

As a glaciologist, I've spent 35 years investigating how meltwater affects the flow and stability of glaciers and ice sheets.

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This gaping hole that's opening up at the surface is merely the beginning of the meltwater's journey through the guts of the ice sheet. As it funnels into moulins, it bores a complex network of tunnels through the ice sheet that extend many hundreds of meters down, all the way to the ice sheet bed.

When it reaches the bed, the meltwater decants into the ice sheet's subglacial drainage system – much like an urban stormwater network, though one that is constantly evolving and backing up. It carries the meltwater to the ice margins and ultimately ends up in the ocean, with major consequences for the thermodynamics and flow of the overlying ice sheet.

Scenes like this and new research into the ice sheet's mechanics are challenging traditional thinking about what happens inside and under ice sheets, where observations are extremely challenging yet have stark implications. They suggest that Earth's remaining ice sheets in Greenland and Antarctica are far more vulnerable to climate warming than models predict, and that the ice sheets may be destabilizing from inside.

NASA's GRACE satellites capture Greenland's ice loss from 2002-2021.

This is a tragedy in the making for the half a billion people who populate vulnerable coastal regions, since the Greenland and Antarctic ice sheets are effectively giant frozen freshwater reservoirs locking up in excess of 65 meters (over 200 feet) of equivalent global sea level rise. Since the 1990s their mass loss has been accelerating, becoming both the primary contributor to and the wild card in future sea level rise.

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How narrow cracks become gaping maws in ice

Moulins are near-vertical conduits that capture and funnel the meltwater runoff from the ice surface each summer. There are many thousands across Greenland, and they can grow to impressive sizes because of the thickness of the ice coupled with the exceptionally high surface melt rates experienced. These gaping chasms can be as large as tennis courts at the surface, with chambers hidden in the ice beneath that could swallow cathedrals.

But this new moulin I've witnessed is really far from any crevasse fields and melt lakes, where current scientific understanding dictates that they should form.

A helicopter sitting on the ice sheet looks tiny next to the gaping moulin, where a meltwater stream pours into the ice sheet.
High rates of meltwater discharge combined with a thick and gently sloping ice sheet in Western Greenland gives rise to monster holes like this moulin.
Alun Hubbard

In a new paper, Dave Chandler and I demonstrate that ice sheets are littered with millions of tiny hairline cracks that are forced open by the meltwater from the rivers and streams that intercept them.

Because glacier ice is so brittle at the surface, such cracks are ubiquitous across the melt zones of all glaciers, ice sheets and ice shelves. Yet because they are so tiny, they can't be detected by satellite remote sensing.

Under most conditions, we find that stream-fed hydrofracture like this allows water to penetrate hundreds of meters down before freezing closed, without the crack's necessarily penetrating to the bed to form a full-fledged moulin. But, even these partial-depth hydrofractures have considerable impact on ice sheet stability.

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As the water pours in, it damages the ice sheet structure and releases its latent heat. The ice fabric warms and softens and, hence, flows and melts faster, just like warmed-up candle wax.

Alun Hubbard using a rappelling rope lowers himself from the top of the ice sheet into a huge hold with water pouring down the sides. The hole appears to be as wide as a two-lane road.
Alun Hubbard rappels into a moulin in October 2019, a point in the year when surface melt should have ceased but hadn't.
Lars Ostenfeld / Into the Ice

The stream-driven hydrofractures mechanically the ice and transfer heat into the guts of the ice sheet, destabilizing it from the inside. Ultimately, the internal fabric and structural integrity of ice sheets is becoming more vulnerable to climate warming.

Emerging processes that speed up ice loss

Over the past two decades that scientists have tracked ice sheet melt and flow in earnest, melt have become more common and more intense as global temperatures rise – further exacerbated by Arctic warming of almost four times the global mean.

The ice sheet is also flowing and calving icebergs much faster. It has lost about 270 billion metric tons of ice per year since 2002: over a centimeter and a half (half an inch) of global sea-level rise. Greenland is now, on average, contributing around 1 millimeter (0.04 inches) to the sea level budget annually.

A 2022 study found that even if atmospheric warming stopped now, at least 27 centimeters – nearly 1 foot – of sea level rise is inevitable because of Greenland's imbalance with its past two decades of climate.

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Understanding the risks ahead is crucial. However, the current generation of ice sheet models used to assess how Greenland and Antarctica will respond to warming in the future don't account for amplification processes that are being discovered. That means the models' sea-level rise estimates, used to inform Intergovernmental Panel on Climate Change (IPCC) reports and policymakers worldwide, are conservative and lowballing the rates of global sea rise in a warming world.

Two people stand inside an ice cave with light coming from a large hole above.
Daniela Barbieri and Alun Hubbard explore the contorted englacial plumbing deep inside a Greenland moulin.
Lars Ostenfeld / Into the Ice

Our new finding is just the latest. Recent studies have shown that:

In the last months, other papers also described previously unknown feedback processes underway beneath ice sheets that computer models currently can't include. Often these processes happen at too fine a scale for models to pick up, or the model's simplistic physics means the processes themselves can't be captured.

Two such studies independently identify enhanced submarine melting at the grounding line in Greenland and Antarctica, where large outlet glaciers and ice streams drain into the sea and start to lift off their beds as floating ice shelves. These processes greatly accelerate ice sheet response to climate change and, in the case of Greenland, could potentially double future mass loss and its contribution to rising sea level.

Greenland's ice loss through meltwater and calving of glaciers has contributed nearly 10 centimeters (4 inches) to global sea-level rise since 1900. The chart shows sea level rise from all sources through 2018.
NASA's Goddard Space Flight Center/PO.DAAC

Current climate models lowball the risks

Along with other applied glaciologists, “structured expert judgment” and a few candid modelers, I contend that the current generation of ice sheet models used to inform the IPCC are not capturing the abrupt changes being observed in Greenland and Antarctica, or the risks that lie ahead.

Ice sheet models don't include these emerging feedbacks and respond over millennia to strong-warming perturbations, leading to sluggish sea level forecasts that are lulling policymakers into a false sense of security. We've a long way since the first IPCC reports in the early 1990s, which treated polar ice sheets as completely static entities, but we're still short of capturing reality.

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As a committed field scientist, I am keenly aware of how privileged I am to work in these sublime environments, where what I observe inspires and humbles. But it also fills me with foreboding for our low-lying coastal regions and what's ahead for the 10% or so of the world's population that lives in them.The Conversation

Alun Hubbard, Professor of Glaciology, Arctic Five Chair, University of Tromsø

This article is republished from The Conversation under a Creative Commons license. Read the original article.

The Conversation

Playing with the kids is important work for chimpanzee mothers

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theconversation.com – Zarin Machanda, Assistant Professor of Anthropology and Biology, Tufts – 2024-05-08 08:01:53

Chimp mothers take on the critical role of playmate with their young.

Kris Sabbi

Zarin Machanda, Tufts University and Kris Sabbi, Harvard University

Wild chimpanzees have been studied for more than 60 years, but they continue to delight and surprise observers, as we found during the summer of 2017 in Kibale National Park in Uganda.

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We were observing young chimpanzees' play to better understand how they grow up. For most group-living animals, play is an integral component of . Beyond just fun, social play allows them to practice critical physical and social skills they will need later in life.

But that summer, we realized that it wasn't just the young ones playing. Adults were joining in on play more often than we had seen before, especially with each other. Watching fully grown female chimpanzees tickling each other and laughing surprised even the most veteran researchers of our .

Two moms with babies play with one another on small trees, and two other young chimpanzees join in.

What made this so unusual was not that adult chimpanzees were playing at all, but that they were doing it so frequently. A behavior that we typically might see once every or two became something that we saw every day and sometimes lasted for hours.

So what had changed that summer? For us, as primatologists, this is where the fun began.

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Why would adults play in the first place?

Scientists tend to think the main reason play declines with age is that individuals essentially grow out of it as they master motor and social skills and shift toward more adult behaviors. By this logic, adults only rarely play because they no longer need to. The situation is different for domesticated species like dogs because the process of domestication itself preserves juvenile behaviors like playfulness into adulthood.

Neither of these reasons would explain why our adult chimpanzees were shoving babies out of the way to play with each other that summer. Instead of asking why adults would play, we had to ask what might, in other circumstances, stop them from playing. And for this, we had to go back to the basics of primatology and consider the effects of food on behavior.

The summer of 2017 was notable because there was an unusually high seasonal peak of a lipstick-red fruit called Uvariopsis, a favorite and calorie-rich chimpanzee food. During the months when these fruits are ripe and plentiful, chimpanzees spend more time hanging out together in larger groups.

This sort of energy surplus has been linked to rigorous activities, such as hunting among monkeys. We wondered whether fruit abundance might be linked to social play as well. Perhaps adult play is constrained because grown chimpanzees just don't usually have the extra time and energy to devote to it.

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Female chimpanzee sits with her infant on a tree branch.

Gathering enough food to eat is a critical task.

Kris Sabbi

When life gets in the way of play

To test this idea, we turned to the long-term of the Kibale Chimpanzee Project, extracting nearly 4,000 observations of adult play over 10 years.

Whether tussling with a young chimpanzee or playing chase with another adult, the frequency of adult play was strongly correlated with the amount of ripe fruit in the diet in any given month. When the forest was full of high-quality food, adult chimpanzees played a lot.

But when their prized fruits dwindled, their playful sides all but disappeared – that is, except for mothers.

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A surprising sex difference

Among chimpanzees, males are much more social than females. Males invest a lot of time developing friendships, and, in turn, they reap the rewards of those bonds: higher dominance rank and more sex. For females, the high energetic costs of pregnancy and lactation mean socializing at the cost of sharing food that they need for themselves and their offspring.

We expected that play, as a social behavior, would follow other social patterns, with males playing more and being able to afford to play even when food abundance was low. To our surprise, we found the opposite. Females played more, especially during months with less fruit – because mothers kept playing with their babies even when all other chimpanzees had stopped.

A hidden cost of motherhood

Chimpanzees in multimale, multifemale societies that exhibit what researchers call fission-fusion. In other words, the whole social group is rarely, if ever, all together. Instead, chimpanzees break up into temporary subgroups called parties that individuals move among throughout the day.

When food is scarce, parties tend to be smaller, and mothers are often alone with just their young. This strategy reduces feeding competition with group mates. But it also leaves mothers as the only social partners for their offspring. Mothers' time and energy that might be devoted toward other daily tasks, such as feeding and rest, go toward play instead.

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A chimpanzee mom tussles playfully with her young daughter while her infant nurses.

Not only did our study reveal this previously unknown cost of motherhood, but it also highlighted how important play must be for these young chimpanzees that their mothers accept this cost.

You might be curious about how chimpanzee fathers fit in here. Chimpanzees mate promiscuously, so males do not know which offspring are theirs. Mothers are left to bear the costs of parenthood on their own.

An ape connection

Child development researchers know that play, and especially play with parents, is critically important for human social development. In fact, caregivers of young might be reading this in between bouts of play with their little ones right now.

Chimpanzees and people enjoy some of the same kinds of physical play, like playing airplane.

Since chimpanzees are one of our closest living relatives, these kinds of behavioral similarities between our species are not uncommon.

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But not all primate parents reckon with costly play. In fact, there are almost no records of monkey mothers playing with their babies at all. Most other primate species, such as baboons and capuchins, don't go their separate ways during the day, so babies can play with each other and moms can catch a break.

Whether maternal play is a product of fission-fusion grouping or the developmental needs of offspring still needs to be tested directly. But the responsibility to play with your little ones certainly resonates with many human parents who experienced a sudden shift to become their children's main play partners when COVID-19 interrupted normal activities.

So on this Mother's Day, consider raising a glass to also celebrate these amazing – and tired – chimpanzee moms.The Conversation

Zarin Machanda, Assistant Professor of Anthropology and Biology, Tufts University and Kris Sabbi, Fellow in Human Evolutionary Biology, Harvard University

This article is republished from The Conversation under a Creative Commons license. Read the original article.

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Everyday life and its variability influenced human evolution at least as much as rare activities like big-game hunting

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theconversation.com – Cara Wall-Scheffler, Professor and Chair of Biology at Seattle Pacific University and Affiliate Assistant Professor of Anthropology, University of Washington – 2024-05-08 07:35:48

Collecting water and caring for kids are necessities.

Three Lions/Hulton Archive via Getty Images

Cara Wall-Scheffler, University of Washington

Think about taking a walk: where you need to go, how fast you need to move to get there, and whether you need to bring something along to carry the results of your errand.

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Are you going on this walk with someone else? Does walking with a friend change your preparation? If you're walking with a child, do you remember to bring an extra sweater or a snack? You probably did – because people intuitively vary their plan depending on their current needs and situations.

In my research as an anthropologist, I've focused on the evolution of human walking and running because I love the flexibility people bring to these behaviors. Humans in all kinds of environments across and time vary how far they go, when they go and what they go for – whether food, water or friends – based on a multitude of factors, season, daylight, rituals and .

Anthropologists split their studies of human activity into two broad categories: what people need to do – including eat, keep their kids alive and so on – and what solutions they come up with to accomplish these needs.

How people keep their children alive is a key issue in my research because it has a direct impact on whether a population survives. It turns out that kids stay alive if they're with adults. To this end, it is a human universal that women carry heavy loads every day, including kids and their food. This needs-based behavior seems to have been an important part of our evolutionary history and explains quite a few aspects of human physiology and female morphology, such as women's lower center of mass.

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woman in exercise gear running away from camera, showing back down to sneakers

Women are built for endurance. What needs-based behaviors drove this evolutionary path?

Robert Decelis/Stone via Getty Images

The solutions to other key problems, like specifically which food women will be carrying, vary across time and space. I suggest that these variations are as integral to explaining human biology and culture as the needs themselves.

Impacts of uncommon activities

Evolutionary scientists often focus on how beneficial heritable traits get passed on to offspring when they a survival advantage. Eventually a trait can become more common in a population when it provides a useful solution.

For example, researchers have made big claims about how influential persistence hunting via endurance running has been on the way the human body evolved. This theory suggests that taking down prey by running them to exhaustion has led to humans' own abilities to long distances – by increasing humans' ability to sweat, strengthening our head and making sure our lower limbs are light and elastic.

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But persistence hunting occurs in fewer than 2% of the recorded instances of hunting in one major ethnographic database, making it an extremely rare solution to the need to find food. Could such a rare and unusual form of locomotion have had a strong enough impact to select for the suite of adaptive traits that make humans such excellent endurance athletes ?

Maybe persistence hunting is actually a fallback strategy, providing a solution only at key moments when survivorship is on the edge. Or maybe these capabilities are just side effects of the loaded walking done every day. I think a better argument is that the ability to predict how to move between common and uncommon strategies has been the driver of human endurance capacity.

man in traditional clothing stands beside canoe with two children in it on shoreline

Hunting big game is only one way to get food – this Inuit man and children are out to find eggs.

George Rinhart/Corbis via Getty Images

Everyday life's influence on evolution

Hunting itself, especially of large mammals, is hardly ubiquitous, despite how frequently it is discussed. For example, anthropologists tend to generalize that people who lived in the Arctic even up to a hundred years ago consumed only animal meat hunted by men. But actually, the original ethnographic work reveals a far more nuanced picture.

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Women and children were actively involved in hunting, and it was a strongly seasonal activity. Coastal fishing, berry picking and the use of plant materials were all vital to Arctic people's day-to-day sustenance. Small family groups used canoes for coastal foraging for part of the year.

During other seasons, the whole community participated in hunting large mammals by herding them into dangerous situations where they were more easily killed. Sometimes family groups were together, and sometimes large communities were together. Sometimes women hunted with rifles, and sometimes children ran after caribou.

The dynamic nature of daily life means that the relatively uncommon activity of hunting large terrestrial vertebrates is unlikely to be the main behavior that helps humans solve the key problems of food, water and keeping children alive.

Anthropologist Rebecca Bliege Bird has investigated how predictable food is throughout the day and the year. She's noted that for most communities, big game is rarely caught, especially when a person is hunting alone. Even among the Hadza in Tanzania, generally considered a big-game hunting community, a hunter acquires 0.03 prey per day on average – essentially 11 animals a year for that person.

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Bird and others clearly argue that the planning and flexible coordination done by females is the crucial aspect of how humans survive on a daily basis. It's the daily efforts of females that allow people to be spontaneous a few times a year to accomplish high-risk activities such as hunting – persistence or otherwise. Therefore it is female flexibility that allows communities to survive between the rare big-game opportunities.

girl, older woman and middle-aged women laughing with their arms around each other

Roles and identities shift across the life span.

Jose Luis Pelaez Inc/DigitalVision via Getty Images

Changing roles and contributions

Some anthropologists argue that in some parts of the world, behavior varies more for cultural reasons, like what tools you make, than for environmental ones, such as how much daylight there is during winter. The importance of culture means that the solutions vary more than the needs.

One of the aspects of culture that varies is the role assigned to specific genders. Varying gender roles are related to the distribution of labor and when people take on certain solution-based tasks. In most cultures, these roles change across a female's life span. In American culture, this would be like a grandparent going back to college to hone a childhood passion in order to take on a new job to send their grandchildren to college.

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In many places, females go from youth when they might carry their siblings and firewood, to early parenthood where they might go hunting with a baby on their back, to older parenthood where they might carry water on their head, a baby on their back and tools in their hands, to postmenopausal periods when they might carry giant loads of mangoes and firewood to and from camp.

Even though always load carrying, our capacity to plan and change our behavior for diverse environments is part of what drives Homo sapiens' , which means that the behavior of females across their different life stages has been a major driver of this capability.The Conversation

Cara Wall-Scheffler, Professor and Chair of Biology at Seattle Pacific University and Affiliate Assistant Professor of Anthropology, University of Washington

This article is republished from The Conversation under a Creative Commons license. Read the original article.

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Exoplanet WASP-69b has a cometlike tail – this unique feature is helping scientists like me learn more about how planets evolve

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theconversation.com – Dakotah Tyler, Ph.D. Candidate in Astrophysics, of California, Los Angeles – 2024-05-08 07:35:12

WASP-69b closely orbits its sun.

W. M. Keck Observatory/Adam Makarenko

Dakotah Tyler, University of California, Los Angeles

Located 163 light-years from Earth, a Jupiter-sized exoplanet named WASP-69b offers astrophysicists a window into the dynamic processes that shape planets across the galaxy. The star it orbits is baking and stripping away the planet's atmosphere, and that escaped atmosphere is being sculpted by the star into a vast, cometlike tail at least 350,000 miles long.

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I'm an astrophysicist. My research team published a paper in the Astrophysical Journal describing how and why WASP-69b's tail formed, and what its formation can illuminate about the other types of planets astronomers tend to detect outside of our solar system.

A planet with a gaseous cloud around it in the shape of a tail, orbiting around a sun.

Artist's interpretation of an aerial view of the exoplanet WASP-69b on its 3.8-day orbit around its host star. Its atmosphere is being stripped away and sculpted into a long cometlike tail that trails the planet.

W. M. Keck Observatory/Adam Makarenko

A universe filled with exoplanets

When you look up at the night sky, the you see are suns, with distant worlds, known as exoplanets, orbiting them. Over the past 30 years, astronomers have detected over 5,600 exoplanets in our Milky Way galaxy.

It isn't easy to detect a planet light-years away. Planets pale in comparison, in both size and brightness, to the stars that they orbit. But despite these limitations, exoplanet researchers have uncovered an astonishing variety – everything from small rocky worlds barely larger than our own moon to gas giants so colossal that they've been dubbed “super-Jupiters.”

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However, the most common exoplanets astronomers detect are larger than Earth, smaller than Neptune, and orbit their stars more closely than Mercury orbits our Sun.

These ultra-common planets tend to fall into one of two distinct groups: super-Earths and sub-Neptunes. Super-Earths have a radius that's up to 50% larger than Earth's radius, while sub-Neptunes typically have a radius that's two to four times larger than Earth's radius.

A diagram showing the relative sizes of exoplanet categories, with Gas Giants by far the largest, the Neptune-like (or sub-Neptunes), super-Earths and terrestrial rocky planets.

Sub-Neptunes, or Neptune-like planets, look at lot like a super-Earth, but with a thick atmosphere.

NASA-JPL/Caltech

Between those two radius ranges, there's a gap, known as the “Radius Gap,” in which researchers rarely find planets. And, Neptune-sized planets that complete orbits around their stars in less than four days are exceedingly rare. Researchers call that gap the “Hot Neptune Desert.”

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Some underlying astrophysical processes must be preventing these planets from forming – or surviving.

Planet formation

As a star forms, a large disk of dust and gas forms around it. In that disk, planets can form. As young planets gain mass, they can accumulate significant gas atmospheres. But as the star matures, it starts to emit high amounts of energy in the form of ultraviolet and X-ray radiation. This stellar radiation can bake away the atmospheres that the planets have accumulated in a called photoevaporation.

Rings of gas and dust rotating around a hot bright core.

A planet-forming disk.

ALMA (ESO/NAOJ/NRAO)

However, some planets resist this process. More massive planets have stronger gravity, which helps them hold onto their original atmospheres. Additionally, planets that are farther away from their star aren't hit with as much radiation, so their atmospheres erode less.

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So, maybe a significant portion of super-Earths are actually the rocky cores of planets that had their atmospheres completely stripped, while sub-Neptunes were massive enough to retain their puffy atmospheres.

As for the Hot Neptune Desert, most Neptune-sized planets simply are not massive enough to completely resist the stripping power of their star if it orbits too closely. In other words, a sub-Neptune orbiting its star in four days or fewer will quickly lose its entire atmosphere. When observed, the atmosphere has already been lost and what remains is a bare rocky core – a super-Earth.

To put this theory to the test, research teams like mine have been collecting observational evidence.

WASP-69b: A unique laboratory

Enter WASP-69b, a unique laboratory for studying photoevaporation. The name “WASP-69b” from the way it was discovered. It was the 69th star with a planet, b, found in the Wide Angle Search for Planets survey.

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Despite being 10% larger than Jupiter in radius, WASP-69b is actually closer to the mass of much lighter Saturn – it's not very dense, and it has only about 30% the mass of Jupiter. In fact, this planet has about the same density as a piece of cork.

This low density results from its ultra-close 3.8-day orbit around its star. Being so close, the planet receives an immense amount of energy, which causes it to heat up. As gas heats, it expands. Once the gas expands enough, it begins to escape the planet's gravity for good.

When we observed this planet, my colleagues and I detected helium gas escaping WASP-69b rapidly – about 200,000 tons per second. This translates to the mass of the Earth lost every years.

Over the star's lifetime, this planet will end up losing a total atmospheric mass equivalent of nearly 15 times the mass of Earth. This sounds like a lot, but WASP-69b is approximately 90 times Earth's mass, so even at this extreme rate, it will only ever lose a small fraction of the total amount of gas from which it is comprised.

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The cometlike tail of WASP-69b

Perhaps most striking is the discovery of WASP-69b's extended helium tail, which my team detected trailing behind the planet for at least 350,000 miles (about 563,000 kilometers). Strong stellar winds, which are a constant flow of charged particles emitted from stars, sculpt tails like this. These particle winds ram into the escaping atmosphere and shape it into a cometlike tail behind the planet.

WASP-69b's escaping atmosphere.

Our study is actually the first to suggest that WASP-69b's tail was so extensive. Past observations of this system suggested the planet had only a modest tail or even no tail at all.

This difference likely comes down to two main factors. For one, each research group used different instruments to make their observations, which could result in varying detection levels. Or, there could be actual variability in the system.

A star like our Sun has a magnetic activity cycle, called the “solar cycle.” The Sun's lasts for 11 years. During peak activity years, the Sun has more flares, sunspots and changes to the solar wind.

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To complicate things even more, each cycle is unique – no two solar cycles are the same. Solar scientists are still to better understand and predict our Sun's activity. Other stars have their own magnetic cycles, but scientists just don't have enough data to understand them yet.

So the variability observed for WASP-69b may from the fact that every time it gets observed, the host star is behaving differently. Astronomers will have to continue to observe this planet more in the future to get a better idea of exactly what's going on.

Our direct look at WASP-69b's mass loss tells exoplanet researchers like me more about how planetary evolution works. It gives us real-time evidence for atmospheric escape and supports the theory that hot Neptunes and Radius Gap planets are hard to find because they just aren't massive enough to retain their atmospheres. And once they lose them, all that is left to observe is a rocky super-Earth core.

The WASP-69b study highlights the delicate balance between a planet's composition and its stellar , shaping the diverse planetary landscape we observe . As astronomers continue to probe these distant worlds, each discovery brings us closer to understanding the complex tapestry of our universe.The Conversation

Dakotah Tyler, Ph.D. Candidate in Astrophysics, University of California, Los Angeles

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This article is republished from The Conversation under a Creative Commons license. Read the original article.

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