Planetary Science News

This is the first high-resolution, color image to be sent back by the Hazard Cameras (Hazcams) on the underside of NASA’s Perseverance Mars rover after its landing on February 18, 2021. Image credit: NASA / JPL-Caltech.

Perseverance Sends Back Its First Color Photos, Status Reports from Mars

Feb 22, 2021 by News Staff

Mission controllers at NASA’s Jet Propulsion Laboratory have received new images from the Perseverance rover as well as health reports from both the...

Perseverance’s first image (colorized) from Jezero Crater, Mars. Image credit: NASA’s Jet Propulsion Laboratory.

NASA’s Perseverance Rover Successfully Lands on Mars

Feb 19, 2021 by News Staff

After a 203-day journey, NASA’s car-sized Perseverance rover successfully landed in Jezero Crater on Mars on February 18, 2021. Confirmation of the successful...

This illustration shows NASA’s Mars 2020 spacecraft carrying the Perseverance rover as it approaches Mars. Image credit: NASA / JPL-Caltech.

NASA’s Perseverance Rover to Land on Mars Today: Watch Live

Feb 18, 2021 by News Staff

NASA’s Perseverance rover, with the Ingenuity helicopter attached to its belly, is on target to touch down gently in Jezero Crater on Mars around 3:55...

Artist’s impression depicting the separation of the Schiaparelli module from the Trace Gas Orbiter, and heading for Mars. Image credit: D. Ducros / ESA.

Trace Gas Orbiter Detects Hydrogen Chloride Gas in Atmosphere of Mars

Feb 17, 2021 by News Staff

The source of hydrogen chloride (HCl) in the atmosphere of Mars is recent surface volcanism, subsurface magmatic activity, or aerosol chemistry occurring...

HiRISE camera view of Krupac crater on Mars featuring gullies along the rim and recurring slope lineae lower down the crater wall. Image credit: NASA / JPL / University of Arizona.

New Research Reveals What Causes Landslides on Mars

Feb 4, 2021 by News Staff

On Mars, seasonal features known as recurring slope lineae (RSL) are prevalent on Sun-facing slopes. Previous studies have suggested RSL are related to...

The High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter captured this image of the larger of Mars’ two moons, Phobos, on March 23, 2008. The image was taken from a distance of about 6,800 km (about 4,200 miles). It is presented in color by combining data from the camera’s blue-green, red, and near-infrared channels. The illuminated part of Phobos seen in the image is about 21 km (13 miles) across. The most prominent feature is the large crater Stickney in the lower right. With a diameter of 9 km (5.6 miles), it is the largest feature on Phobos. Image credit: NASA / JPL-Caltech / University of Arizona.

Phobos May Contain Atmospheric Atoms from Ancient Mars

Feb 3, 2021 by News Staff

Martian atmospheric oxygen, carbon, nitrogen and argon ions have been escaping Mars for billions of years and could be preserved inside the uppermost hundreds...

An artistic rendering of Kraken Mare, a large liquid methane sea on Titan. Image credit: NASA’s John Glenn Research Center.

Titan’s Largest Methane Sea is Over 100 Meters Deep

Jan 21, 2021 by News Staff

Kraken Mare, a sea of liquid methane on Saturn’s moon Titan, is at least 100-m (330 feet) deep near its center, according to an analysis of data collected...

Hayabusa-2 image of the asteroid Ryugu as seen from a distance of 3.7 miles. A particularly large crater is visible near the center of the image. Image credit: JAXA / University of Tokyo / Kochi University / Rikkyo University / Nagoya University / Chiba Institute of Technology / Meiji University / University of Aizu / AIST.

Hayabusa-2 Reveals New Details about Asteroid Ryugu

Jan 6, 2021 by Enrico de Lazaro

The ancient parent body of the near-Earth ‘rubble pile’ asteroid Ryugu had likely dried out in some kind of heating event before the asteroid came...

Perspective view of chaotic terrain in Pyrrhae Regio, Mars. Image credit: ESA / DLR / FU Berlin / CC BY-SA 3.0 IGO.

Mars Express Spots Chaotic Terrain near Valles Marineris

Dec 31, 2020 by News Staff

The High Resolution Stereo Camera (HRSC) onboard ESA’s Mars Express orbiter has imaged a fascinating landscape near the major canyon system of Valles...

Hamilton et al. studied the composition of Almahata Sitta 202 to determine that it likely originated from a previously unknown parent asteroid. Image credit: Hamilton et al., doi: 10.1038/s41550-020-01274-z.

Almahata Sitta Meteorites Came from Ceres-Sized Asteroid, Study Shows

Dec 28, 2020 by News Staff

The parent body of the Almahata Sitta meteorites — space rocks that rained down on the Nubian Desert in Sudan in 2008 — is a 640 to 1,800 km-wide...

This image shows a suite of fluvial ridges on Mars (at –67.64 °E, 43.37 °S). Image credit: J. Dickson.

Planetary Researchers Create Map of Early Mars’ River Systems

Dec 24, 2020 by News Staff

Using data from the Context Camera aboard NASA’s Mars Reconnaissance Orbiter, planetary researchers have generated an 8-trillion-pixel global map of...

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...