Planetary Science News

This image comprises data gathered by ESA’s Mars Express on November 8, 2020, during orbit 21,305. Image credit: ESA / DLR / FU Berlin / CC BY-SA 3.0 IGO.

Mars Express Spots Festive Silhouettes near Martian South Pole

Dec 18, 2020 by News Staff

The wings of an angelic figure, complete with halo, can be seen sweeping up and off the top of the frame in a new image from ESA’s Mars Express spacecraft,...

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’ Subsurface Ocean Has Various Energy Sources for Microbial Life, Study Suggests

Dec 17, 2020 by News Staff

In a study published this month in the journal Icarus, planetary researchers from the United States and Germany modeled chemical processes in the subsurface...

Rendering of Gale Lake some 3.5 billion years ago, when Mars was warmer and much wetter. Image credit: Evan Williams / NASA / Mars Reconnaissance Orbiter HIRISE project.

Martian Brines May Not Be as Widespread as Previously Thought

Dec 11, 2020 by News Staff

In a new study published in the Planetary Science Journal, a team of U.S. scientists combined experimentally verified data on brine evaporation rates along...

A fragment of the Tagish Lake meteorite. Image credit: Mike Zolensky, NASA’s Johnson Space Center.

Scientists Find Precursor of Prebiotic Chemistry in Three Meteorites

Dec 8, 2020 by News Staff

An international team of researchers has detected a polyheterocyclic organic molecule called hexamethylenetetramine in three carbonaceous meteorites: Murchison,...

The young Mars would have had enough water to cover its entire surface in a liquid layer about 140 m deep, but it is more likely that the liquid would have pooled to form an ocean occupying almost half of Mars’s northern hemisphere, and in some regions reaching depths greater than 1.6 km. Image credit: M. Kornmesser / ESO / N. Risinger, skysurvey.org.

Study: Early Mars Likely Had Energy Source for Underground Life

Dec 3, 2020 by News Staff

According to a new study published in the journal Science Advances, the Martian subsurface would have been the most habitable region for simple life forms...

This artist’s impression shows how Mars may have looked about 4 billion years ago. Image credit: M. Kornmesser / ESO.

Curiosity Finds Deposits from Megafloods in Martian Crater

Nov 23, 2020 by News Staff

NASA’s Curiosity rover has found a series of symmetrical, 10-m- (33-foot-) high gravel ridges — sedimentologic evidence of ancient giant floods...

This artist’s concept depicts the dry environment seen at Mars today versus the early Martian environment. Image credit: Simon Fraser University.

Global and Regional Dust Storms Cause Mars to Lose Water

Nov 13, 2020 by News Staff

Mars was once a wet planet, but it has lost most of its water through reactions that produce hydrogen. In standard models, molecular hydrogen produced...

These illustrations show three versions of a rocky planet with different amounts of internal heating from radioactive elements. The middle planet is Earth-like, with plate tectonics and an internal dynamo generating a magnetic field. The top planet, with more radiogenic heating, has extreme volcanism but no dynamo or magnetic field. The bottom planet, with less radiogenic heating, is geologically ‘dead,’ with no volcanism. Image credit: Melissa Weiss.

Internal Heating from Radioactive Elements May Be Crucial to Planet Habitability, Study Says

Nov 12, 2020 by News Staff

The thermal evolution of rocky planets depends on the heat input from three long-lived radiogenic elements: potassium, thorium, and uranium. Concentrations...

This artist’s conception of Europa shows a hypothesized cryovolcanic eruption, in which briny water from within the icy shell blasts into space. Image credit: Justice Blaine Wainwright.

Europa’s Plumes May Originate from Near-Surface Brine Reservoirs, Not Global Ocean

Nov 11, 2020 by News Staff

Europa, the sixth of Jupiter’s moons and the fourth largest, has a subsurface ocean covered by an icy shell. Despite evidence for plumes on the icy moon,...

Water Present on All Rocky Planets, Martian Meteorite Study Suggests

Nov 10, 2020 by News Staff

Water may emerge in connection with the formation of terrestrial planets, according to a new analysis of a Martian meteorite called North West Africa (NWA)...

This illustration of Jupiter’s moon Europa shows how its icy surface may glow on its nightside. Image credit: NASA / JPL-Caltech.

Europa’s Icy Surface Glows in the Dark, New Study Suggests

Nov 10, 2020 by News Staff

Jupiter’s icy moon Europa is bombarded by a constant and intense blast of radiation from the gas giant. Different salty compounds on the moon’s surface...

This colorized radar image, taken by NASA’s Cassini orbiter on February 15, 2005, shows a 60-km (37-mile) wide crater on Titan. The appearance of the crater and the extremely bright (hence rough) blanket of material surrounding it is indicative of an origin by impact, in which a hypervelocity comet or asteroid, in this case, roughly 5-10 km (3-6 miles) in size, slammed into the surface of the moon. The bright surrounding blanket is debris, or ejecta, thrown out of the crater. The asymmetric appearance of this ejecta blanket could be an effect of atmospheric winds associated with the impact itself. Although clearly formed by impact, the feature lacks a central peak, suggesting that it has been eroded or otherwise modified after formation. Rainfall, wind erosion, and softening of the solid material in which the crater formed are all possible processes that might have altered this impact feature. Image credit: NASA / JPL-Caltech / ASI.

Cassini Finds Organics and Water Ice in Titan’s Impact Craters

Nov 6, 2020 by News Staff

Using the spectral data collected by the Visual and Infrared Mapping Spectrometer (VIMS) onboard NASA’s Cassini spacecraft, a team of researchers has...

This image shows a triple crater in Noachis Terra, Mars. The largest crater measures 45 km across, and the smallest 28 km. There are also signs of other sizeable craters, such as the round patches of sunken surface seen to the top right and bottom left. This image comprises data gathered by ESA’s Mars Express using its High Resolution Stereo Camera (HRSC) on August 6, 2020. This image was created using data from the nadir and color channels of the HRSC. The nadir channel is aligned perpendicular to the surface of Mars, as if looking straight down at the surface. North is to the right. Image credit: ESA / DLR / FU Berlin / CC BY-SA 3.0 IGO.

Mars Express Spots Triple Crater on Red Planet

Nov 3, 2020 by News Staff

ESA’s Mars Express orbiter has spotted three overlapping craters in Noachis Terra, an extensive landmass in the southern hemisphere of Mars. This image...

Juno Observes Sprites and Elves in Upper Atmosphere of Jupiter

Oct 30, 2020 by News Staff

NASA’s Juno spacecraft has been in orbit around Jupiter since 2016. One of its instruments is the ultraviolet spectrograph (UVS), which is primarily...

A false-color view of Titan, a moon of Saturn surrounded by a thick orange haze. Image credit: NASA / JPL / University of Arizona / University of Idaho.

Cyclopropenylidene Detected in Atmosphere of Titan

Oct 28, 2020 by News Staff

Using high sensitivity spectroscopic observations from the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have detected a small cyclic...

A fragment of the Hamburg meteorite found on Strawberry Lake near Hamburg, Michigan, the United States. Image credit: Heck et al., doi: 10.1111/maps.13584.

Scientists Find Organic Compounds in Hamburg Meteorite

Oct 28, 2020 by News Staff

An international team of researchers has found extraterrestrial hydrocarbons, sulfurized and nitrogen-containing compounds in the Hamburg meteorite, which...

When the Moon had a magnetic field, it would have been shielded from incoming solar wind, as shown in this illustration. Image credit: NASA.

Moon’s Ancient Magnetosphere May Have Helped Early Earth Retain Its Atmosphere

Oct 15, 2020 by News Staff

Solar storms strip a planet’s atmosphere over time, and only a strong magnetosphere would be able to provide maximum protection. Lunar samples gathered...

Pluto’s Mountains are Capped with Methane Frost: Study

Oct 14, 2020 by News Staff

The bright frosts observed in 2015 in the equatorial region of Cthulhu on Pluto are mostly made of methane-rich ice, according to new research. This image,...

This oblique color view from the HiRISE instrument onboard NASA’s Mars Reconnaissance Orbiter shows a lithified field of sand dunes within Melas Chasma, Valles Marineris. The large degree of preserved morphology for many of these paleodunes reveals important information regarding the acting wind regime and climate prior to their cementation. Image credit: NASA / JPL / University of Arizona.

One-Billion-Year-Old Sand Dunes Spotted on Mars

Oct 12, 2020 by News Staff

Planetary researchers have mapped and characterized ancient sand dune fields in the canyons of Valles Marineris on Mars. Their discovery offers new insights...