Planetary Science News

Glein et al. found evidence for hydrothermal or metamorphic activity deep within the icy dwarf planets Eris and Makemake. Image credit: Southwest Research Institute.

Webb Finds Evidence of Hydrothermal Processes in Interiors of Eris and Makemake

Feb 15, 2024 by News Staff

The icy dwarf planets Eris and Makemake have surfaces bearing methane ice of unknown origin. According to an analysis of data from the NASA/ESA/CSA James...

A topographic map of the Eridania region of Mars; volcanic structures described by Michalski et al. are classified by morphology and morphometrics. Image credit: Michalski et al., doi: 10.1038/s41550-023-02191-7.

Early Mars was Tectonically and Volcanically Active, Study Suggests

Feb 12, 2024 by News Staff

The relatively well-preserved ancient crust of Mars provides a natural window into early planetary evolution not available on Earth. Mars has generally...

The JunoCam instrument aboard NASA’s Juno spacecraft imaged Io, the most geologically active body in our Solar System, on February 3, 2024, from a distance of about 7,904 km (4,911 miles). Image credit: NASA / SwRI / MSSS.

NASA’s Juno Orbiter Captures Stunning Images of Jupiter’s Moon Io

Feb 9, 2024 by Natali Anderson

On February 3, 2024, NASA’s Juno spacecraft made a second close flyby of Io, the fifth of Jupiter’s moons and the third largest. Like the previous...

Mimas’ surface, like the surfaces of most of the other major Saturnian moons without atmospheres, is not pure ice but contains some dark impurities; the relatively dark markings appear along the lower portion of the walls of the 130-km-wide Herschel Crater (the peak in the middle of the crater is about as tall as Mount Everest; the impact that made it likely almost destroyed the moon) and some of the smaller craters; scientists interpret this darkening as evidence for the gradual concentration of impurities from evaporating icy materials in areas where the dark impurities slide slowly down the crater wall. Image credit: NASA / JPL / Space Science Institute.

Saturn’s Moon Mimas Harbors Global Ocean beneath Its Icy Shell, Study Suggests

Feb 7, 2024 by News Staff

From detailed analysis of Mimas’ orbital motion based on data from NASA’s Cassini mission, planetary researchers from Sorbonne Université, Nantes...

Predicted areas of slope instability in the south polar region of the Moon; the image is centered on Shackleton crater; locations of proposed Artemis III landing regions are shown (blue boxes); the model predicts that large portions of the interior walls of Shackleton crater are susceptible to landslides (inset), as are portions of the interior crater walls in the Nobile Rim 1 region. Image credit: Watters et al., doi: 10.3847/PSJ/ad1332.

Earth’s Moon is Shrinking, New Modeling Study Suggests

Jan 29, 2024 by News Staff

Earth’s Moon shrank more than 46 m (150 feet) in circumference as its core gradually cooled over the last few hundred million years, according to a paper...

This image shows a height map of the Martian surface, with lowest land in blue and highest in white. Image credit: ESA.

Mars Express Finds New Evidence for Ice-Rich Layered Deposits in Medusae Fossae

Jan 22, 2024 by News Staff

Over 15 years ago, ESA’s Mars Express spacecraft studied the Medusae Fossae Formation, revealing enigmatic deposits up to 2.5 km deep. From those early...

A map of the titanium abundances of the Moon’s surface, obtained from NASA’s Clementine spacecraft; the red parts indicate extremely high concentrations compared to terrestrial rocks. Image credit: Lunar and Planetary Institute.

Scientists Solve Major Puzzle in Moon’s Geology

Jan 15, 2024 by News Staff

New research from the University of Bristol sheds light on the origin of titanium-rich basaltic magmas on the Moon. A map of the titanium abundances of...

Venus in real colors, processed from Mariner 10 images. Image credit: Mattias Malmer / NASA.

Combination of Two Minerals Can Explain Mysterious UV Absorber in Clouds of Venus

Jan 8, 2024 by Enrico de Lazaro

The clouds of Venus are believed to be composed of sulfuric acid and minor constituents including iron-bearing compounds. Respective concentrations of...

Summary of the fate of simple and complex organics on Titan’s surface. Image credit: Yu et al., doi: 10.1029/2023GL106156.

‘Magic Islands’ on Titan’s Hydrocarbon Lakes Are Floating Chunks of Porous Organic Solids

Jan 8, 2024 by Enrico de Lazaro

Titan, the largest moon of Saturn, has a unique atmosphere that transforms simple gases like methane and nitrogen into more complex organic compounds....

Enceladus’ tiger stripes are known to be spewing ice from the moon’s icy interior into space, creating a cloud of fine ice particles over the moon’s south pole and creating Saturn’s mysterious E-ring. Evidence for this has come from NASA’s Cassini spacecraft that orbited Saturn from 2004 to 2017. Pictured here, a high resolution image of Enceladus is shown from a close flyby. Tiger stripes are visible in false-color blue. Image credit: NASA / ESA / JPL / SSI / Cassini Imaging Team.

Enceladus’ Surface May Contain Relatively High Abundances of Pristine Organic Material

Dec 21, 2023 by News Staff

Enceladus, the sixth-biggest moon of Saturn, presents a remarkable opportunity in our Solar System for searching for evidence of extraterrestrial life,...

Illustration of plume activity on Enceladus. Image credit: Peter et al., doi: 10.1038/s41550-023-02160-0.

Planetary Researchers Detect Hydrogen Cyanide in Plume of Enceladus

Dec 17, 2023 by News Staff

Using data from NASA’s Cassini mission, planetary scientists have detected several compounds of strong importance to the habitability of Saturn’s icy...

Molecular hydrogen points to hydrothermal activity in an ocean beneath the icy surface of Enceladus. Image credit: NASA / JPL-Caltech.

Ice Plumes of Saturn’s Icy Moon Enceladus May Hold Amino Acids, Study Suggests

Dec 5, 2023 by News Staff

Enceladus is a prime target in the search for life in the Solar System, identified by NASA as the second-highest priority site for a flagship mission in...

This image, taken with the NASA/ESA Hubble Space Telescope on August 30, 2006, shows the dwarf planet Eris (center) and its moon Dysnomia. Image credit: NASA / ESA / M. Brown, California Institute of Technology.

New Research Sheds Light on Internal Structure of Dwarf Planet Eris

Dec 4, 2023 by Natali Anderson

The trans-Neptunian dwarf planet Eris is tidally locked to its small moon Dysnomia. Recently obtained bounds on the mass of Dysnomia demonstrate that Eris...

ESA Astronaut Captures Stunning Images of Rare Thunder Phenomenon

Dec 1, 2023 by News Staff

As part of the Thor-Davis experiment on the International Space Station (ISS), ESA astronaut Andreas Mogensen has captured images of a phenomenon called...

This image of the Martian horizon was captured by the THEMIS camera on NASA’s Mars Odyssey orbiter. Image credit: NASA / JPL-Caltech / ASU.

Mars Odyssey Beams Back Magnificent Images of Martian Horizon

Nov 29, 2023 by News Staff

In an operation that took mission scientists three months to plan, NASA’s Mars Odyssey orbiter captured a series of panoramic images that showcases the...

An artist’s rendition of the hot-Jupiter exoplanet TOI-1789b. Image credit: Sci-News.com.

Scientists Recreate Extraterrestrial Atmospheric Hazes in the Lab

Nov 27, 2023 by News Staff

The NASA/ESA/CSA James Webb Space Telescope has begun its scientific mission, which includes the atmospheric characterization of transiting exoplanets....

This image shows an artist’s impression of what nightglow might look like to an astronaut in the polar winter regions of Mars at night. Image credit: NASA / JPL-Caltech /Cornell University / Arizona State University / E.W. Knutsen.

ESA’s Trace Gas Orbiter Observes Green Atmospheric Nightglow on Mars

Nov 13, 2023 by News Staff

The atmospheric nightglow is observed on Earth. On Mars, it was something expected, yet never observed in visible light until now. This image shows an...

This illustration depicts findings that Jupiter’s atmospheric winds penetrate the planet in a cylindrical manner and parallel to its spin axis. The most dominant jet recorded by NASA’s Juno is shown in the cutout: the jet is at 21 degrees north latitude at cloud level, but 3,000 km below that, it’s at 13 degrees north latitude. Image credit: NASA / JPL-Caltech / SSI / SWRI / MSSS / ASI / INAF / JIRAM / Björn Jónsson / CC BY 3.0.

Atmospheric Winds Penetrate Jupiter in Cylindrical Manner, Planetary Researchers Say

Nov 9, 2023 by News Staff

The violent nature of Jupiter’s atmosphere has long been a source of fascination for scientists. NASA’s Juno spacecraft has had a ringside seat to...

Astronomers Directly Detect Atomic Oxygen on Venus

Nov 8, 2023 by News Staff

Atomic oxygen is produced on the dayside of Venus by photolysis of carbon dioxide and carbon monoxide. Atomic oxygen is a key species in the mesosphere...