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    Amateur astronomers’ images of a rare double aurora may unlock its secrets

    What happens when two different kinds of auroras get together? One spills the other’s secrets.

    Amateur astronomers have captured a strange combination of red and green auroras on camera, and physicists — who had never seen such a thing before — have now used these images to learn what may trigger the more mysterious part of the lightshow.

    Photographer Alan Dyer was in his backyard in Strathmore, Canada, when he saw the lights dancing overhead and started filming. “I knew I had something interesting,” says Dyer, who also writes about astronomy. What he didn’t know was that he had just made the most complete recording of this rare phenomenon.

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    At a glance, Dyer’s video looks like a celestial watermelon. The rind, a rippling green aurora, is well understood: It appears when the solar wind energizes protons trapped within Earth’s magnetic field, which then rain down and knock electrons and atoms around (SN: 12/10/03).  

    The swath of fruity magenta is more mysterious: Though scientists have known about these “stable auroral red arcs” for decades, there’s no widely accepted proof of how they form. One popular theory is that part of Earth’s magnetic field can heat up the atmosphere and, like proton rain, jostle particles.   

    But until now, researchers had never seen both of these red and green auroras side by side, says Toshi Nishimura, a space physicist at Boston University. “This strange combination,” he says, “was something beyond our expectations.”

    [embedded content]
    Alan Dyer’s footage of this rare double aurora, a time lapse captured over 33 minutes on October 12, 2021, is helping physicists tease out clues to what causes the red glow.

    Along with satellite observations, Dyer’s images and similar ones captured by other amateur astronomers in Canada and Finland show that the two phenomena are related, Nishimura’s team reports in the July JGR Space Physics. Thin rays in the red aurora are the smoking gun as to how. Those lines trace the paths of electrons as they fall along the Earth’s magnetic field. So just as proton rain triggers the green aurora, electron rain appears to trigger the red one, with the solar wind powering both at the same time. Since the electrons carry less energy than the protons, they make for a more reddish color. 

    But electron rain might not be the only way to produce these red glows, cautions Brian Harding, a space physicist at the University of California, Berkeley. Either way, he says, the results are exciting because they show what’s going on is more complicated than researchers thought.

    Those complications are important to understand. The auroras Dyer saw, though beautiful, are danger zones for radio communication and GPS systems (SN: 8/13/17). As Nishimura puts it: If you were driving under a subauroral red arc, your GPS might tell you to veer into a field.

    Until scientists better understand these red glows, they won’t be able to forecast space weather like they do normal weather, Harding explains. “You want to make sure that you can predict stuff like this,” he says.

    The new results would not have been possible without the citizen scientists who took the photos, Nishimura says. “This is a new way of doing research…. When they take more and more cool images, they find more and more things that we don’t know about.”

    According to Dyer, more photos are exactly what’s coming. “We can make a unique contribution to science,” he says.  After all, “you never know what’s going to appear.” More

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    A new look at the ‘mineral kingdom’ may transform how we search for life

    If every mineral tells a story, then geologists now have their equivalent of The Arabian Nights.

    For the first time, scientists have cataloged every different way that every known mineral can form and put all of that information in one place. This collection of mineral origin stories hints that Earth could have harbored life earlier than previously thought, quantifies the importance of water as the most transformative ingredient in geology, and may change how researchers look for signs of life and water on other planets. 

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    “This is just going to be an explosion,” says Robert Hazen, a mineralogist and astrobiologist at the Carnegie Institution for Science in Washington, D.C. “You can ask a thousand questions now that we couldn’t have answered before.”

    For over 100 years, scientists have defined minerals in terms of “what,” focusing on their structure and chemical makeup. But that can make for an incomplete picture. For example, though all diamonds are a kind of crystalline carbon, three different diamonds might tell three different stories, Hazen says. One could have formed 5 billion years ago in a distant star, another may have been born in a meteorite impact, and a third could have been baked deep below the Earth’s crust.

    Diamonds have the same carbon structure, but they can form in different ways. This particular gem originated deep within the Earth.Rob Lavinsky/ARKENSTONE

    So Hazen and his colleagues set out to define a different approach to mineral classification. This new angle focuses on the “how” by thinking about minerals as things that evolve out of the history of life, Earth and the solar system, he and his team report July 1 in a pair of studies in American Mineralogist. The researchers defined 57 main ways that the “mineral kingdom” forms, with options ranging from condensation out of the space between stars to formation in the excrement of bats. 

    The information in the catalog isn’t new, but it was previously scattered throughout thousands of scientific papers. The “audacity” of their work, Hazen says, was to go through and compile it all together for the more than 5,600 known types of minerals. That makes the catalog a one-stop shop for those who want to use minerals to understand the past.

    The compilation also allowed the team to take a step back and think about mineral evolution from a broader perspective. Patterns immediately popped out. One of the new studies shows that over half of all known mineral kinds form in ways that ought to have been possible on the newborn Earth. The implication: Of all the geologic environments that scientists have considered as potential crucibles for the beginning of life on Earth, most could have existed as early as 4.3 billion years ago (SN: 9/24/20). Life, therefore, may have formed almost as soon as Earth did, or at the very least, had more time to arise than scientists have thought. Rocks with traces of life date to only 3.4 billion years ago (SN: 7/26/21). 

    “That would be a very, very profound implication — that the potential for life is baked in at the very beginning of a planet,” says Zachary Adam, a paleobiologist at the University of Wisconsin–Madison who was not involved in the new studies.

    The exact timing of when conditions ripe for life arose is based on “iffy” models, though, says Frances Westall, a geobiologist at the Center for Molecular Biophysics in Orléans, France, who was also not part of Hazen’s team. She thinks that scientists need more data before they can be sure. But, she says, “the principle is fantastic.”

    The new results also show how essential water has been to making most of the minerals on Earth. Roughly 80 percent of known mineral types need H2O to form, the team reports.

    “Water is just incredibly important,” Hazen says, adding that the estimate is conservative. “It may be closer to 90 percent.”

    Some minerals would not form in certain ways without the influence of life. Photosynthesizing bacteria helped bring about the oxygen-rich conditions needed for this azurite (left), while the opalized ammonite (right) was created by the mineral opal filling the space where an ammonite shell used to be.Rob Lavinsky/ARKENSTONE

    Taken one way, this means that if researchers see water on a planet like Mars, they can guess that it has a rich mineral ecosystem (SN: 3/16/21). But flipping this idea may be more useful: Scientists could identify what minerals are on the Red Planet and then use the new catalog to work backward and figure out what its environment was like in the past. A group of minerals, for example, might be explainable only if there had been water, or even life.

    Right now, scientists do this sort of detective work on just a few minerals at a time (SN: 5/11/20). But if researchers want to make the most of the samples collected on other planets, something more comprehensive is needed, Adam says, like the new study’s framework.

    And that’s just the beginning. “The value of this [catalog] is that it’s ongoing and potentially multigenerational,” Adam says. “We can go back to it again and again and again for different kinds of questions.” 

    “I think we have a lot more we can do,” agrees Shaunna Morrison, a mineralogist at the Carnegie Institution and coauthor of the new studies. “We’re just scratching the surface.” More

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    50 years ago, a new theory of Earth’s core began solidifying

    How the Earth got its core – Science News, July 1, 1972

    In the beginning, scientists believe there was an interstellar gas cloud of all the elements comprising the Earth. A billion or so years later, the Earth was a globe of concentric spheres with a solid iron inner core, a liquid iron outer core and a liquid silicate mantle…. The current theory is that the primeval cloud’s materials accreted … and that sometime after accretion, the iron, melted by radioactive heating, sank toward the center of the globe…. Now another concept is gaining ground: that the Earth may have accreted … with core formation and accretion occurring simultaneously.

    Update

    Most scientists now agree that the core formed as materials that make up Earth collided and glommed together and that the process was driven by heat from the smashups. The planet’s heart is primarily made of iron, nickel and some oxygen, but what other elements may dwell there and in what forms remains an open question. Recently, scientists proposed the inner core could be superionic, with liquid hydrogen flowing through an iron and silicon lattice (SN: 3/12/22, p. 12). More

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    Samples of the asteroid Ryugu are scientists’ purest pieces of the solar system

    Samples of the asteroid Ryugu are the most pristine pieces of the solar system that scientists have in their possession.

    A new analysis of Ryugu material confirms the porous rubble-pile asteroid is rich in carbon and finds it is extraordinarily primitive (SN: 3/16/20). It is also a member of a rare class of space rocks known as CI-type, researchers report online June 9 in Science. 

    Their analysis looked at material from the Japanese mission Hayabusa2, which collected 5.4 grams of dust and small rocks from multiple locations on the surface of Ryugu and brought that material to Earth in December 2020 (SN: 7/11/19; SN: 12/7/20). Using 95 milligrams of the asteroid’s debris, the researchers measured dozens of chemical elements in the sample and then compared abundances of several of those elements to those measured in rare meteorites classified as CI-type chondrites. Fewer than 10 meteorites found on Earth are CI chondrites.

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    This comparison confirmed Ryugu is a CI-type chondrite. But it also showed that unlike Ryugu, the meteorites appear to have been altered, or contaminated, by Earth’s atmosphere or even human handling over time. “The Ryugu sample is a much more fresh sample,” says Hisayoshi Yurimoto, a geochemist at Hokkaido University in Sapporo, Japan.

    The researchers also measured the abundances of manganese-53 and chromium-53 in the asteroid and determined that melted water ice reacted with most of the minerals around 5 million years after the solar system’s start, altering those minerals, says Yurimoto. That water has since evaporated, but those altered minerals are still present in the samples. By studying them, the researchers can learn more about the asteroid’s history.   More

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    Ice at the moon’s poles might have come from ancient volcanoes

    Four billion years ago, lava spilled onto the moon’s crust, etching the man in the moon we see today. But the volcanoes may have also left a much colder legacy: ice.

    Two billion years of volcanic eruptions on the moon may have led to the creation of many short-lived atmospheres, which contained water vapor, a new study suggests. That vapor could have been transported through the atmosphere before settling as ice at the poles, researchers report in the May Planetary Science Journal.

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    Since the existence of lunar ice was confirmed in 2009, scientists have debated the possible origins of water on the moon, which include asteroids, comets or electrically charged atoms carried by the solar wind (SN: 11/13/09). Or, possibly, the water originated on the moon itself, as vapor belched by the rash of volcanic eruptions from 4 billion to 2 billion years ago.

    “It’s a really interesting question how those volatiles [such as water] got there,” says Andrew Wilcoski, a planetary scientist at the University of Colorado Boulder. “We still don’t really have a good handle on how much are there and where exactly they are.”

    Wilcoski and his colleagues decided to start by tackling volcanism’s viability as a lunar ice source. During the heyday of lunar volcanism, eruptions happened about once every 22,000 years. Assuming that H2O constituted about a third of volcano-spit gasses — based on samples of ancient lunar magma — the researchers calculate that the eruptions released upward of 20 quadrillion kilograms of water vapor in total, or the volume of approximately 25 Lake Superiors.

    Some of this vapor would have been lost to space, as sunlight broke down water molecules or the solar wind blew the molecules off the moon. But at the frigid poles, some could have stuck to the surface as ice.

    For that to happen, though, the rate at which the water vapor condensed into ice would have needed to surpass the rate at which the vapor escaped the moon. The team used a computer simulation to calculate and compare these rates. The simulation accounted for factors such as surface temperature, gas pressure and the loss of some vapor to mere frost.

    About 40 percent of the total erupted water vapor could have accumulated as ice, with most of that ice at the poles, the team found. Over billions of years, some of that ice would have converted back to vapor and escaped to space. The team’s simulation predicts the amount and distribution of ice that remains. And it’s no small amount: Deposits could reach hundreds of meters at their thickest point, with the south pole being about twice as icy as the north pole.

    The results align with a long-standing assumption that ice dominates at the poles because it gets stuck in cold traps that are so cold that ice will stay frozen for billions of years.

    “There are some places at the lunar poles that are as cold as Pluto,” says planetary scientist Margaret Landis of the University of Colorado Boulder.

    Volcanically sourced water vapor traveling to the poles, though, probably depends on the presence of an atmosphere, say Landis, Wilcoski and their colleague Paul Hayne, also a planetary scientist at the University of Colorado Boulder. An atmospheric transit system would have allowed water molecules to travel around the moon while also making it more difficult for them to flee into space. Each eruption triggered a new atmosphere, the new calculations indicate, which then lingered for about 2,500 years before disappearing until the next eruption some 20,000 years later.

    This part of the story is most captivating to Parvathy Prem, a planetary scientist at Johns Hopkins Applied Physics Laboratory in Laurel, Md., who wasn’t involved in the research. “It’s a really interesting act of imagination.… How do you create atmospheres from scratch? And why do they sometimes go away?” she says. “The polar ices are one way to find out.”

    If lunar ice was belched out of volcanoes as water vapor, the ice may retain a memory of that long-ago time. Sulfur in the polar ice, for example, would indicate that it came from a volcano as opposed to, say, an asteroid. Future moon missions plan to drill for ice cores that could confirm the ice’s origin.

    Looking for sulfur will be important when thinking about lunar resources. These water reserves could someday be harvested by astronauts for water or rocket fuel, the researchers say. But if all the lunar water is contaminated with sulfur, Landis says, “that’s a pretty critical thing to know if you plan on bringing a straw with you to the moon.” More

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    These are the first plants grown in moon dirt

    That’s one small stem for a plant, one giant leap for plant science.

    In a tiny, lab-grown garden, the first seeds ever sown in lunar dirt have sprouted. This small crop, planted in samples returned by Apollo missions, offers hope that astronauts could someday grow their own food on the moon.

    But plants potted in lunar dirt grew more slowly and were scrawnier than others grown in volcanic material from Earth, researchers report May 12 in Communications Biology. That finding suggests that farming on the moon would take a lot more than a green thumb.

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    “Ah! It’s so cool!” says University of Wisconsin–Madison astrobotanist Richard Barker of the experiment.

    “Ever since these samples came back, there’s been botanists that wanted to know what would happen if you grew plants in them,” says Barker, who wasn’t involved in the study. “But everyone knows those precious samples … are priceless, and so you can understand why [NASA was] reluctant to release them.”

    Now, NASA’s upcoming plans to send astronauts back to the moon as part of its Artemis program have offered a new incentive to examine that precious dirt and explore how lunar resources could support long-term missions (SN: 7/15/19).

    The dirt, or regolith, that covers the moon is basically a gardener’s worst nightmare. This fine powder of razor-sharp bits is full of metallic iron, rather than the oxidized kind that is palatable to plants (SN: 9/15/20). It’s also full of tiny glass shards forged by space rocks pelting the moon. What it is not full of is nitrogen, phosphorus or much else plants need to grow. So, even though scientists have gotten pretty good at coaxing plants to grow in fake moon dust made of earthly materials, no one knew whether newborn plants could put down their delicate roots in the real stuff.

    To find out, a trio of researchers at the University of Florida in Gainesville ran experiments with thale cress (Arabidopsis thaliana). This well-studied plant is in the same family as mustards and can grow in just a tiny clod of material. That was key because the researchers had only a little bit of the moon to go around.

    The team planted seeds in tiny pots that each held about a gram of dirt. Four pots were filled with samples returned by Apollo 11, another four with Apollo 12 samples and a final four with dirt from Apollo 17. Another 16 pots were filled with earthly volcanic material used in past experiments to mimic moon dirt. All were grown under LED lights in the lab and watered with a broth of nutrients. 

    Thale cress plants grown for 16 days in volcanic material from Earth (left) looked starkly different compared with seedlings nourished in moon dirt (right). Plants potted in samples returned by the Apollo 11 mission (right, top) fared worse than those planted in Apollo 12 samples (right, middle) or Apollo 17 samples (right, bottom).Tyler Jones, IFAS/UF

    “Nothing really compared to when we first saw the seedlings as they were sprouting in the lunar regolith,” says Anna-Lisa Paul, a plant molecular biologist. “That was a moving experience, to be able to say that we’re watching the very first terrestrial organisms to grow in extraterrestrial materials, ever. And it was amazing. Just amazing.”

    Plants grew in all the pots of lunar dirt, but none grew as well as those cultivated in earthly material. “The healthiest ones were just smaller,” Paul says. The sickliest moon-grown plants were tiny and had purplish pigmentation — a red flag for plant stress. Plants grown in Apollo 11 samples, which had been exposed on the lunar surface the longest, were most stunted.

    Paul and colleagues also inspected the genes in their mini alien Eden. “By seeing what kind of genes are turned on and turned off in response to a stress, that shows you what tools plants are pulling out of their metabolic toolbox to deal with that stress,” she says. All plants grown in moon dirt pulled out genetic tools typically seen in plants struggling with stress from salt, metals or reactive oxygen species (SN: 9/8/21).

    Apollo 11 seedlings had the most severely stressed genetic profile, offering more evidence that regolith exposed to the lunar surface longer — and therefore littered with more impact glass and metallic iron — is more toxic to plants.

    Future space explorers could choose the site for their lunar habitat accordingly. Perhaps lunar dirt could also be modified somehow to make it more comfortable for plants. Or plants could be genetically engineered to feel more at home in alien soil. “We can also choose plants that do better,” Paul says. “Maybe spinach plants, which are very salt-tolerant, would have no trouble growing in lunar regolith.”

    Barker isn’t daunted by the challenges promised by this first attempt at lunar gardening.  “There’s many, many steps and pieces of technology to be developed before humanity can really engage in lunar agriculture,” he says. “But having this particular dataset is really important for those of us that believe it’s possible and important.” More

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    NASA’s InSight lander has recorded the largest Marsquake yet

    Any Martians out there should learn to duck and cover.

    On May 4, the Red Planet was rocked by a roughly magnitude 5 temblor, the largest Marsquake detected to date, NASA’s Jet Propulsion Laboratory in Pasadena, Calif., reports. The shaking lasted for more than six hours and released more than 10 times the energy of the previous record-holding quake.

    The U.S. space agency’s InSight lander, which has been studying Mars’ deep interior since touching down on the planet in 2018 (SN: 11/26/18), recorded the event. The quake probably originated near the Cerberus Fossae region, which is more than 1,000 kilometers from the lander.

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    Cerberus Fossae is known for its fractured surface and frequent rockfalls. It makes sense that the ground would be shifting there, says geophysicist Philippe Lognonné, principal investigator of the Seismic Experiment for Interior Structure, InSight’s seismometer. “It’s an ancient volcanic bulge.”

    Just like earthquakes reveal information about our planet’s interior structure, Marsquakes can be used to probe what lies beneath Mars’ surface (SN: 7/22/21). And a lot can be learned from studying this whopper of a quake, says Lognonné, of the Institut de Physique du Globe de Paris. “The signal is so good, we’ll be able to work on the details.” More

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    Lava and frost may form the mysterious lumps on Jupiter’s moon Io

    On Jupiter’s moon Io, lava creeping beneath frost may give rise to fields of towering dunes.

    That finding, described April 19 in Nature Communications, suggests that dunes may be more common on other worlds than previously thought, though the lumps may form in odd ways.  

    “In some sense, these [other worlds] are looking more familiar,” says George McDonald, a planetary scientist at Rutgers University in Piscataway, N.J. “But the more you think about it, they feel more and more exotic.”

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    Io is a world crowded with erupting volcanoes, created when the gravitational forces of Jupiter and some of its other moons pull on Io and generate heat (SN: 8/6/14). Around 20 years ago, scientists reported another type of feature on Io’s dynamic surface — hummocky ridges. The features resemble dunes, but that couldn’t be the case, scientists reasoned, because Io’s atmosphere is too thin for winds to whip up a dunescape.

    But in recent years, dunelike features have been discovered on comet 67P (SN: 9/21/20) and Pluto (SN: 8/24/21), planetary bodies that also lack thick atmospheres. Inspired by those alien dunescapes, McDonald and his colleagues revisited the matter of Io’s mysterious lumps. All they needed was some type of airborne force to sculpt the moon’s dunes.

    On Earth, powerful explosions of steam occur when flows of molten rock encounter bodies of water. While water isn’t found on Io, sulfur dioxide frost is pervasive. So the scientists hypothesize that when lava slowly flows into and just under a frost layer, jets of sulfur dioxide gas could burst from the frost. Those jets could send grains of rock and other material flying and forming dunes.

    The researchers calculate that an advancing lava flow, buried under at least 10 centimeters of frost, could sublimate some of the frost into pockets of hot vapor. When enough vapor accumulates and the pressure becomes high enough to match or overcome the weight of the overlying frost, the vapor could burst out at velocities over 70 kilometers per hour. These bursts could propel grains with diameters from 20 micrometers to 1 centimeter in size, the team estimates.  

    Analyzing images of Io’s surface, collected by NASA’s now-defunct Galileo probe, revealed highly reflective streaks of material radiating outward over dunes in front of lava flows — possibly material newly deposited at the time by vapor jets.

    This image, taken by NASA’s now-defunct Galileo spacecraft, shows dunelike lumps on Jupiter’s third-largest moon Io. The dark area (lower left) is a lava flow, and the bright streaks that radiate outward may be evidence of material strewn by jets of vapor that burst from frost heated by the lava.JPL-Caltech/NASA, Rutgers Univ.

    What’s more, using the images to measure the hummocky features showed that their dimensions align with those of dunes on other planetary bodies. Some of the Ionian dunes are over 30 meters high, the team estimates.

    “I think a lot of [scientists] looked at those and thought, hey, these really could be dunes,” says Jani Radebaugh, a planetary scientist at Brigham Young University in Provo, Utah, who was not involved in the study. “But what’s exciting about it is that they’ve come up with a good physical mechanism to explain how it’s possible.”

    Io is typically thought of as a world of volcanoes. The possibility of dunes suggests that there might be more going on there than scientists thought, McDonald says. “It certainly adds a layer of complexity.” More