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  • A long-ago reshuffling of the giant planets in our solar system may have been instrumental in giving Earth its moon.

    For decades, planetary scientists have hypothesized that Jupiter, Saturn, Uranus and Neptune were born much closer to the sun and that gravitational interactions among those planets jolted them into their contemporary trajectories (SN: 5/10/22). But the timing of that “giant planet orbital instability” has been tricky to nail down.

    Now, an analysis of meteorite data suggests that the instability took place between 60 million and 100 million years after the solar system started forming, planetary scientist Alessandro Morbidelli reported October 5 in San Antonio at a meeting of the American Astronomical Society’s Division for Planetary Sciences. That timing also roughly coincides with when Earth’s moon is thought to have formed in the wake of a Mars-sized planet running into our own.

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    The instability of the giant planets “is related to a complete reshaping of the solar system, the formation of the cometary reservoirs, the sculpting of the asteroid belt,” says Morbidelli, of the Observatoire de la Côte d’Azur in Nice, France. “Understanding when it occurred means fixing a milestone in the history of the solar system.”

    The giant planet migration, first proposed by Morbidelli and colleagues in 2005, is a widely accepted hypothesis for explaining much about the solar system. In particular, the giant planets travel along slightly elongated orbits that are askew to one another. But observations of other planetary systems and computer simulations of planet formation suggest that giant planets, in general, form on closer-in orbits that are circular and coplanar. Using simulations, Morbidelli and others showed that if the giant planets in our solar system formed like that, they wouldn’t stay that way. Gravitational interactions would eventually knock the planets into the orbits they have today.

    At first, the team thought this instability occurred about 600 million years after the birth of the solar system. That timing meant the migration of the giant planets could also explain an apparent asteroid bombardment of the terrestrial planets — Mercury, Venus, Earth and Mars — as evidenced by craters on the moon and lunar rocks brought back by Apollo astronauts. More recent work, however, has cast doubt on the reality of this “lunar cataclysm.”

    Now, Morbidelli suspects the orbital instability came a lot earlier. His reasoning starts with a rare type of meteorite called EL enstatite chondrites.

    The mix of elements in these meteorites suggests they must be the remnants of a large rocky body, a few hundred kilometers across, born near the terrestrial planets in the dusty disk that once swirled around our sun.

    Then, in 2022, Morbidelli and colleagues showed that any of these enstatites that land on Earth today must come from a collection of bits and pieces in the asteroid belt between Mars and Jupiter. Those bits all broke off Athor, one of the many asteroids there, after it collided long ago with some other object in the belt. Altogether, that family of material adds up to an asteroid roughly 60 kilometers across — much smaller than the one thought to have birthed the enstatites in the first place. That means Athor must be only one piece of that larger rocky body, left over from a collision that destroyed it much closer to the sun.

    “The question is, which dynamical mechanism can allow the implantation of Athor in the asteroid belt?” Morbidelli said at the meeting.

    He tried computer simulations of several possibilities, but so far, only the giant planet instability seems capable of sending Athor to a stable orbit in the asteroid belt.

    This couldn’t have happened earlier than 60 million years after the birth of the solar system, Morbidelli said. Radioactive elements in the enstatite chondrites indicate their parent body was slowly cooling until then, which means it was still large. It hadn’t yet collided with one of the many other planetesimals stirred around by the forming terrestrial planets.

    On the other hand, simulations suggest the instability can’t have occurred later than about 100 million years after the solar system began. A study in 2018 concluded that if the giant planets migrated later, a pair of asteroids dubbed Patroclus-Menoetius, trailing Jupiter around the sun while orbiting each other, would have been pulled apart.

    That 60-million- to 100-million-year window makes the instability a prime suspect in the diversion of a hypothesized planet that hit Earth, creating the moon (SN: 3/15/23).  The timing “seems right,” says Matthew Clement, an astrophysicist at the Johns Hopkins Applied Physics Laboratory in Laurel, Md.  “Lots of things were happening in the solar system’s early history. However, dynamically speaking, we don’t have a whole lot of reason to believe that things changed much after the moon-forming impact.”

    But he cautions that Morbidelli’s estimate is based on “one data point, of the breakup of one asteroid, pieces of which serendipitously happened to get to Earth.”

    Still, “it’s nice that [the new result] is actually based on some real data, even if it’s indirectly, rather than just computer models,” says planetary scientist John Chambers. He has questions, though. “They suggest this happened when the formation of the terrestrial planets was more or less complete, apart maybe from the giant impact that formed the moon,” says Chambers, of the Carnegie Institution for Science in Washington, D.C. “But then there’s a good chance it would have messed up the orbits of the terrestrial planets and possibly led to some of them colliding,” which the current lineup of planets suggests did not happen.

    Both Chambers and Matthews have worked on scenarios in which the orbital instability occurred even earlier, just a few million years after the solar system began. That earlier time for the instability would help explain one of the outstanding riddles of the solar system: the relatively small size of Mars compared with Earth and Venus. That’s because the instability would have removed many objects from near the orbit of Mars before it could grow to the size of Earth or larger. The new result from Morbidelli’s team seems to exclude that solution.

    “I’m prepared to rely on the evidence,” Chambers says. But he isn’t convinced yet because many facets of the solar system’s present structure must be reconciled with any date for the giant planet instability.

    Clement agrees. “There’s problems if the instability happened at 500 million years. There’s still problems that we have to resolve if it happened when they say it happened,” he says. “And there’s still problems if it happened immediately after the planets formed, in the first few million years. This story is not done being told yet.” More

  • CHICAGO — The last key ingredient for life has been discovered on Saturn’s icy moon Enceladus.

    Phosphorus is a vital building block of life, used to construct DNA and RNA. Now, an analysis of data from NASA’s Cassini spacecraft reveals that Enceladus’ underground ocean contains the crucial nutrient. Not only that, its concentrations there may be thousands of times greater than in Earth’s ocean, planetary scientist Yasuhito Sekine reported December 14 at the American Geophysical Union’s fall meeting.

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    The essential element may abound on many other icy worlds too, holding promise for the search for alien life, said Sekine, of the Tokyo Institute of Technology.

    “We knew that Enceladus had most of the elements that are essential for life as we know it — carbon, hydrogen, nitrogen, oxygen and sulfur,” says Morgan Cable, an astrobiologist at the Jet Propulsion Laboratory in Pasadena, Calif., who was not involved in the research. “Now that [phosphorus] has been confirmed … Enceladus now appears to meet all of the criteria for a habitable ocean.”

    Many researchers consider Enceladus to be among the most likely places to house extraterrestrial life. It’s a world encased in ice, with an ocean of salty water hidden beneath (SN: 11/6/17). What’s more, in 2005 the Cassini spacecraft observed geysers blasting vapor and ice grains out of Enceladus’ icy shell (SN: 8/23/05). And in that space-faring spray, scientists have detected organic molecules.

    But until now, researchers weren’t sure if phosphorus also existed on Enceladus. On Earth’s surface, the element is relatively scarce. Much of the phosphorus is locked away in minerals, and its availability often controls the pace at which life can proliferate.

    So Sekine and colleagues analyzed chemical data, collected by the now-defunct Cassini, of particles in Saturn’s E ring, a halo of material ejected from Enceladus’ jets that wraps around Saturn.

    Some ice grains in the E ring are enriched in a phosphorus compound called sodium phosphate, the researchers found. They estimate that a kilogram of water from Enceladus’ ocean contains roughly 1 to 20 millimoles of phosphate, a concentration thousands of times greater than in Earth’s big blue ocean.

    At the floor of Enceladus’ subsurface ocean, phosphate may arise from reactions between seawater and a phosphate-bearing mineral called apatite, Sekine said, before being ejected through geysers into space. Apatite is often found in carbonaceous chondrites, a primitive, planet-building material (SN: 7/14/17).

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    But that’s not all. Many other icy ocean worlds may contain apatite as well, Sekine said. Similarly, they too could also carry high levels of phosphate in their oceans. That richness could be a boon for any potential alien organisms.

    Though the findings are promising, they give rise to a glaring conundrum, Sekine said. “If life exists [on] Enceladus, why [does] such [an] abundance of chemical energy and nutrients remain?” After all, here on Earth, any available phosphorus is rapidly scavenged by life.

    It’s possible that the moon is simply barren of life, Sekine said. But there’s another more hopeful explanation too. Life on frigid Enceladus, he said, may simply consume the nutrient at a sluggish pace. More

  • Innumerable stars reside within 1.6 light-years of the Milky Way’s central black hole. But this same crowded neighborhood has fewer red giants — luminous stars that are large and cool — than expected.
    Now astrophysicists have a new theory why: The supermassive black hole, Sagittarius A*, launched a powerful jet of gas that ripped off the red giants’ outer layers. That transformed the stars into smaller red giants or stars that are hotter and bluer, Michal Zajaček, an astrophysicist at the Polish Academy of Sciences in Warsaw, and colleagues suggest in a paper published online November 12 in the Astrophysical Journal.
    Today Sagittarius A* is quiet, but two enormous bubbles of gamma-ray-emitting gas rooted at the center of the Milky Way tower far above and below the galaxy’s plane (SN: 12/9/20). These gas bubbles imply the black hole sprang to life some 4 million years ago when something fell into it.
    At that time, a disk of gas around the black hole shot a powerful jet of material into its star-studded neighborhood, Zajaček and colleagues propose. “The jet preferentially acts on large red giants,” he says. “They can be effectively ablated by the jet.” The biggest and brightest red giants seem to be missing near the galactic center, Zajaček says.

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    Red giants are vulnerable because they are large and their envelopes of gas tenuous. A red giant forms from a smaller star after the star’s center gets so full of helium that it can no longer burn its hydrogen fuel there. Instead, the star starts to burn hydrogen in a layer around the center, which makes the star’s outer layers expand, causing its surface to cool and turn red. As a result, some red giants are more than a hundred times the diameter of the sun, making them easy pickings for the jet.
    Still, Zajaček says that as red giants orbit the black hole, they must pass through the jet hundreds or thousands of times before becoming hot, blue stars. The jet is most effective at removing red giants within 0.13 light-years of the black hole, the team calculates.
    “The idea is plausible,” says Farhad Yusef-Zadeh, an astronomer at Northwestern University in Evanston, Ill., who was not involved with the study.
    Tuan Do, an astronomer at UCLA, adds “it may take a combination of several of these kinds of mechanisms to fully explain the lack of the red giants.” In particular, he says, something other than a jet likely accounts for the paucity of red giants farther away from the black hole.
    One candidate, say Zajaček and Do, is a large disk of gas that circled the black hole a few million years ago. This disk spawned stars that now orbit the black hole in a single plane. These young stars exist as far as 1.6 light-years from the black hole, which is also the extent of the red giant gap. As red giants revolved around the black hole and repeatedly plunged through the disk, its gas may have torn off their outer layers, explaining another part of the galactic center’s red star shortage. More

  • It’s big. It’s beautiful. It looks a bit like a sparkly, starry, slightly smooshed Eye of Sauron.

    It’s the galaxy NGC 4632, and new radio telescope images suggest that it sports a rare “polar ring” — a halo of mostly hydrogen gas tilted about 90 degrees from the plane of the galaxy’s disk.

    These spectacular structures, which can also contain dust and stars, are thought to encircle only about 1 in 1,000 galaxies. But now it seems that many more — possibly 30 times as many — could be hiding in plain sight, researchers report in the November Monthly Notices of the Royal Astronomical Society.

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    “The implication would be that there are tons of these things out there, masquerading as normal galaxies,” says astronomer Ronald Buta of the University of Alabama in Tuscaloosa, who wasn’t involved in the new study.

    Astronomers are still puzzling out how any galaxies have polar rings at all. But they’re thought to form as galaxies grow, either by colliding with other galaxies or by gobbling up gas.

    “The rings give us clues about how [galaxies] can grow and evolve,” says astronomer Nathan Deg of Queen’s University in Kingston, Canada.

    Deg and colleagues spotted the ringlike structure around NGC 4632 — and one encircling another galaxy, NGC 6156 — in data from the WALLABY survey, a project that is scanning half of the southern sky with the ASKAP radio telescope in Western Australia.

    “It immediately strikes you that, hey, look, there’s something funny going on right here that kind of looks like a ring,” Deg says.

    It can be tough to tell rings from warped galactic disks, depending on how galaxies are oriented with respect to Earth. So the team used virtual reality visualizations to help distinguish the galaxies’ disks from the potential rings, and compared the real data with simulated observations of perfect polar rings viewed at different angles.

    The scientists report that the stunning structures sported by the two galaxies are indeed probably polar rings, with NGC 4632’s ring spanning roughly 60,000 light-years.

    And these two may have plenty of company. The fact that the team has already spotted two potential polar rings in the 592 galaxies included in these first bits of WALLABY data suggests that earlier estimates of the frequency of such structures were too low.

    The team’s simulations, which tested how polar ring galaxies look to telescopes when viewed at different angles, indicate a similar conclusion. Altogether, the observations and simulations suggest that as many as 3 percent of nearby galaxies could have overlooked rings, too.

    A fruit of these combined efforts is a striking composite image of NGC 4632’s starry disk, viewed in visible light, and the radio glow of its hydrogen halo. Hydrogen emits mostly radio light, so the structure is invisible in visible-light images of the galaxy previously taken by the Subaru Telescope in Hawaii. Larger telescopes taking closer looks, Deg says, might be able to spot stars in the halo too.

    Thanks to large surveys like WALLABY, Deg says, “we’re in an era where we can discover these and figure out the rings in a way that we never could before.” More

  • Though it looks like a smooth, solid, pale blue orb, there’s more going on beneath the clouds of Uranus than meets the eye.

    A polar cyclone has been spotted at the planet’s north pole, researchers report in the May 28 Geophysical Research Letters. Observed with radio telescopes, the find is the first direct evidence of a cyclone on Uranus. A previous spacecraft flyby hinted at a similar storm at the planet’s south pole.

    “It’s really exciting to see this polar structure come into view,” says Michael Roman, a planetary scientist at the University of Leicester in England who was not involved with the research. The observations “show a rather unique structure that we simply have never been able to study before.”

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    In 1986, NASA’s Voyager 2 spacecraft revealed winds at the center of Uranus’ south pole were moving faster than those in neighboring areas and were rotating. This evidence pointed to something dynamic like a cyclone occurring at the pole. But the spacecraft’s instruments weren’t sensitive enough to confirm the storm.

    In recent years, as the north pole of Uranus turned more toward Earth, scientists were able to probe the other side of the ice giant, where they spotted similar hints of a swirling storm. Using the Very Large Array radio observatory in New Mexico, planetary scientist Alex Akins and colleagues probed the temperature under the clouds for more atmospheric clues. “What we saw with the VLA was kind of the last piece of [evidence],” says Akins, of the Jet Propulsion Laboratory in Pasadena, Calif. 

    New thermal emission observations from 2021 and 2022 show a spot on the north pole where the gas beneath the clouds is warmer and drier than its surroundings, suggesting the presence of a low-pressure region in the midst of those spinning winds. “These contrasts look similar to what we see in hurricanes on Earth,” Akins says.

    Excluding Mercury, all the planets in our solar system have now been observed to host some kind of swirling air mass at their poles (SN: 10/14/08).

    Akins plans to continue to observe the cyclone to see how it changes. Previous observations from 2015 suggest it is growing stronger. Researchers wouldn’t expect Uranus’ atmospheric circulation to change on such a relatively short timescale, Akins says, so a continued strengthening of the storm would suggest there’s more to learn about how the planet’s atmosphere works.

    In 2022, experts brought together by the National Academies of Sciences, Engineering, and Medicine recommended NASA send a probe to Uranus (SN: 4/20/22). “The more we can learn about Uranus as we begin to plan a mission,” Roman says, “the better we can focus our planning for that mission.” More

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    A single beam of light runs AI with supercomputer power

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Space & Astronomy

  • America risks losing its role as a space science pioneer

  • Early views of a supernova’s first moments reveal a lopsided blast

  • How did Pluto capture its largest moon, Charon?

  • See the largest, most detailed radio image of the Milky Way yet

  • Some planets might home brew their own water

  • Astronomers saw a rogue planet going through a rapid growth spurt

  • See a 3-D map of stellar nurseries based on data from the Gaia telescope

Humans

  • Kissing may have evolved in an ape ancestor 21 million years ago

  • New Denisovan discovery could rewrite our family tree

  • We can finally hear the long-hidden music of the Stone Age

  • Vast Bronze Age city discovered in the plains of Kazakhstan

  • Ancient figurine may show sexual encounter between woman and goose

  • Neanderthals’ hefty noses weren’t well adapted to cold climates

  • Ancient silver goblet preserves oldest known image of cosmic creation

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