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Check out some of the weird rocks that have turned up on Mars

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As the Mars rover Perseverance crested the top of Witch Hazel Hill, its operators back on Earth expected amazing things. This area on the western rim of the Jezero crater, along an ancient river delta that Perseverance has been exploring since it landed in 2021, is thought to contain some of the oldest rocks on the planet’s surface. The light-toned, layered materials promise a record of a wetter time, possibly one that hosted life.

The team did not expect what they found on March 11: a dark rock resembling a clutch of frog’s eggs. Dubbed St. Paul’s Bay, the rock looks nothing like its neighbors. Where it came from and how it formed are a mystery. More

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  • 163 Shares99 Views

    in Space & Astronomy

    Check out some of the weird rocks that have turned up on Mars

    As the Mars rover Perseverance crested the top of Witch Hazel Hill, its operators back on Earth expected amazing things. This area on the western rim of the Jezero crater, along an ancient river delta that Perseverance has been exploring since it landed in 2021, is thought to contain some of the oldest rocks on the planet’s surface. The light-toned, layered materials promise a record of a wetter time, possibly one that hosted life.

    The team did not expect what they found on March 11: a dark rock resembling a clutch of frog’s eggs. Dubbed St. Paul’s Bay, the rock looks nothing like its neighbors. Where it came from and how it formed are a mystery. More

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    A new iron compound hints ‘primordial’ helium hides in Earth’s core

    Scientists have coaxed one of the universe’s most stubborn elements into a new compound.

    Formed under intense pressures, the newly discovered compound packs helium atoms into crystalline iron, researchers report February 25 in Physical Review Letters. The compound joins a short list of materials that incorporate the normally unreactive element and suggests that helium from the early solar system could be stored in the iron that makes up Earth’s core.

    Helium is one of the least reactive elements on the periodic table. Like the other noble gases, helium doesn’t gain or lose electrons easily and so does not normally form chemical compounds. But under extremely high pressures, helium can interact with a few other elements, including nitrogen and sodium — and now iron, research shows.

    An iron-helium compound, shown here in artificial color using a technique called secondary ion mass spectrometry, forms under high temperature and pressure. Blue and black areas mark the background, while the orange and red area represents the sample. ©2025 Hirose et al. CC-BY-ND

    To make the new iron compound, physicist Kei Hirose of the University of Tokyo and his colleagues squeezed iron and helium together in a diamond anvil cell, a high-pressure device that subjected the elements to pressures greater than 50,000 Earth atmospheres and temperatures above 1,000 degrees Celsius. This compression formed crystals containing both iron and helium.

    The volume of the crystal formed was larger than that of a crystal of pure iron at the same pressure, the team found. The researchers attributed this increase to helium ions packing into interstitial sites, the tiny spaces between iron atoms in the crystal. But the helium atoms don’t bond directly to iron — they’re too unreactive, even at extreme conditions. More

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    Uranus emits more heat than previously thought

    Uranus emits more energy than it gets from the sun, two new studies report — a discovery that contradicts findings from the venerable Voyager spacecraft.

    When Voyager 2 sped past Uranus on January 24, 1986, the spacecraft detected no significant excess heat from the planet, making it seemingly unique among the sun’s giant worlds. However, new observations from space- and ground-based telescopes reveal that Uranus does in fact radiate more energy than sunlight provides, two research teams report in work submitted to arXiv.org in late February. More

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    Juno reveals dozens of lava lakes on Jupiter’s moon Io

    Jupiter’s moon Io, the most volcanically active body in the solar system, is littered with hundreds of erupting volcanoes. High-resolution images now reveal several dozen lava lakes, researchers report in the February Journal of Geophysical Research: Planets. These lakes are far larger than their analogs on Earth, and their structure sheds light on how magma moves beneath the surface of Io. 

    Io’s volcanism — probably present over the moon’s entire 4.6-billion-year existence — was discovered when the Voyager spacecraft flew by in 1979. The volcanic activity is caused by the intense gravitational pulls of Jupiter and nearby moons, which deform Io by tens of meters. “This squeezing is heating the body,” says Alessandro Mura, a planetary scientist at Italy’s National Institute for Astrophysics in Rome. More

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    A private mission to Venus aims to look for signs of life

    BOSTON —Droplets of Venus’ clouds may someday come to Earth. Researchers are testing a device that can gather mist from our planetary neighbor’s atmosphere and deliver it to scientists so they can test the samples for signs of life.

    Venus is not an obvious place to look for life. Its globe-spanning cloud decks are made of sulfuric acid, “a feature that was long believed to be sterile for any organic chemistry,” said MIT planetary scientist Iaroslav Iakubivskyi in a Feb. 15 talk at a meeting of the American Association for the Advancement of Science.

    But in the last few years, lab experiments by Iakubivskyi and colleagues have suggested that sulfuric acid can support the organic chemistry that gives rise to stable nucleic and amino acids — the building blocks of DNA and proteins. Together, the data suggest that “rather than being a disruptive force, sulfuric acid might actually serve as a potential solvent for life-essential molecules,” he said. “Still, we have to go to Venus to test it.”

    A future mission to Venus could include floating a cloud-catching device from a giant balloon in the planet’s sulfuric acid atmosphere, as shown in this illustration.W. Buchanan

    Iakubivskyi’s team is working with the private spaceflight company Rocket Lab on a series of Venus probes called the Morning Star Missions. The first, a probe that will fall through Venus’ atmosphere and measure the sizes of sulfuric acid droplets, is slated to launch in 2026. A later mission would use a two-ton rocket to launch samples into Venus’ orbit to be picked up by a spacecraft returning to Earth. If successful, Morning Star would be the first private mission to another planet.

    Inspired by fog-catching plants in the Atacama desert, the team built a prototype cloud catcher from four layers of wire mesh. The wires can be charged to ionize atmospheric droplets and attract them to the mesh. More

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    A weird ice that may form on alien planets has finally been observed

    A strange type of ice thought to dwell deep in the oceans of alien planets has finally been proven to exist.

    For the first time, researchers have directly observed a sort of hybrid phase of water called plastic ice, which forms at high temperatures and pressures and exhibits traits of both solid ice and liquid water. The observations, reported February 12 in Nature, may help researchers better understand the internal architecture and processes of other worlds in our solar system and beyond, some of which might be habitable. More

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    The moon’s two grand canyons formed in less than 10 minutes

    A giant impact 3.8 billion years ago sent a curtain of rock flying away from a point near the moon’s south pole. When that curtain fell, its rocks plunged up to 3.5 kilometers into the lunar surface with energies 130 times greater than the global inventory of nuclear weapons, new calculations show.

    And that’s how a hailstorm of boulders carved out two gargantuan canyons on the moon in less than 10 minutes.

    “They landed in a staccato fashion, bang-bang-bang-bang-bang,” says planetary geologist David Kring of the Lunar and Planetary Institute in Houston, who reports the finding February 4 in Nature Communications. More

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    Ancient rocks reveal when rivers began pouring nutrients into the sea

    Rivers may have operated on a global scale around 3.5 billion years ago.

    The new find comes courtesy of ancient rocks in China and South Africa. A change in rock chemistry around that time provides the earliest known chemical evidence for the weathering of Earth’s continents and the subsequent delivery of nutrients from land to ocean, geobiologist Kurt Konhauser and colleagues report December 12 in Geology.

    Water chips away at rocks on land, removing minerals and washing them away. “As soon as you get weathering, you’ve got a nutrient influx to the oceans, which can lead to … life thriving in coastal waters,” says Konhauser, of the University of Alberta in Edmonton, Canada. More