Planetary Science News

NASA’s Perseverance Rover Records Sound of Martian Dust Devil

Perseverance’s Navigation Camera (Navcam) observations of the direct dust devil encounter: the Navcam scene (the average background image, top panel) and each dust devil image processed to dust amount (five lower panels), masking out only the truly indeterminate areas (gray); the color scale ranges from optical depth, τ = 0 at the bottom (blue) to τ = 0.12 at the top (yellow), and is linear in between; the areas with low signal-to-noise ratio are masked out, and the images also show non-random noise (banding from instrument electronics during readout); the grid on the scene image (top panel) is 5  degrees in local level azimuth and elevation; the darker gray contours are elevation=0 degrees and azimuth=165 degrees. Image credit: Murdoch et al., doi: 10.1038/s41467-022-35100-z.
Dec 13, 2022 by News Staff

Dust devils — convective vortices loaded with dust — are common at the surface of Mars, particularly at Jezero crater, the landing site of NASA’s Perseverance rover. They are indicators of atmospheric turbulence and are an important lifting mechanism for the Martian dust cycle. Perseverance’s Navigation Camera (Navcam) observations of the direct dust devil encounter: the Navcam scene (the average background image, top panel) and each...

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An artist’s impression of an active mantle plume -- a large blob of warm and buoyant rock -- rising from deep inside Mars and pushing up Elysium Planitia, a plain within the planet’s northern lowlands. Image credit: Adrien Broquet & Audrey Lasbordes.

Planetary Scientists Find Evidence for Active Mantle Plume on Mars

Dec 6, 2022 by News Staff

Elysium Planitia, a flat-smooth plain just north of the Martian equator, is underlain by an 4,000-km-diameter active mantle plume, according to new research...

An illustration of an asteroid on its way to ancient Mars. Image credit: M. Kornmesser / ESO / Nathan Owen-Price / Sci.News.

Chicxulub-Like Asteroid Caused Megatsunami on Early Mars

Dec 1, 2022 by News Staff

The Chicxulub-like asteroid crash landed in shallow ocean waters in the Martian region of Chryse Planitia 3.4 billion years ago (Hesperian period) and...

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.

Early Martian Ocean Was Over 300 Meters Deep, New Research Suggests

Nov 18, 2022 by News Staff

An analysis of chromium isotopes in Martian meteorites suggests that approximately 4.5 billion years ago, there was enough water for the entire planet...

A spiral-shaped dust storm is visible in this image taken by the High Resolution Stereo Camera (HRSC) imager on ESA’s Mars Express spacecraft. This image, taken on May 26, 2019, depicts the formation of a spiral shape whose main arm is approximately 2,000 km in length. A granular pattern of dust cells is visible in the storm, formed by a process called closed-cell convection. This type of convection is also responsible for some cloud patterns on Earth. Image credit: ESA / DLR / FU Berlin.

Martian Springtime Dust Storms Churn Up Surprisingly Earth-Like Cloud Patterns: Study

Nov 16, 2022 by News Staff

Using images obtained by two orbiting spacecraft, NASA’s Mars Reconnaissance Orbiter and ESA’s Mars Express, planetary researchers analyzed textured...

Bonsor et al. present distinct observational evidence from white dwarf planetary systems for planetesimal formation occurring during the first few hundred thousand years after cloud collapse in exoplanetary systems. Image credit: NASA / JPL-Caltech.

Stars and Building Blocks of Their Planets ‘Grow Up’ Together, New Study Suggests

Nov 15, 2022 by News Staff

The timing and locations of formation of planetesimals — the building blocks of planets — are crucial to the understanding of planet formation....

This image, taken by Mars Express’ High Resolution Stereo Camera (HRSC) on April 5, 2022, shows the Terra Sirenum region on Mars. Image credit: ESA / DLR / FU Berlin / CC BY-SA 3.0 IGO.

Mars Express Sees Craters and Fractures in Terra Sirenum

Oct 31, 2022 by News Staff

This new image from the High Resolution Stereo Camera (HRSC) aboard ESA’s Mars Express orbiter shows a diverse region southeast of the Pickering crater...

Boulder-size blocks of water ice can be seen around the rim of an impact crater in the Amazonis Planitia regionon Mars, as viewed by the High-Resolution Imaging Science Experiment (HiRISE) aboard NASA’s Mars Reconnaissance Orbiter. Image credit: NASA / JPL-Caltech / University of Arizona.

Meteoroid Impact on Mars Excavated Large Chunks of Water Ice, Planetary Scientists Say

Oct 28, 2022 by News Staff

On December 24, 2021, NASA’s InSight lander recorded a magnitude 4 marsquake with a distinct signature rippling across the surface of Mars. In a pair...

Benjamin Cardenas & Michael Lamb show definitive evidence of a roughly 3.5-billion-year-old shoreline with substantial sedimentary accumulation, at least 900 m thick, that covered hundreds of thousands of square kilometers. Image credit: Benjamin Cardenas / Penn State.

New Evidence for Northern Ocean on Early Mars

Oct 28, 2022 by News Staff

A major question in Mars history is whether the planet had an ocean in its northern hemisphere. New research provides evidence for a northern ocean or...

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

Chances of Finding Ancient Bacteria on Mars are Better than Previously Expected: Study

Oct 27, 2022 by Natali Anderson

Radiation resistance of microbes is a key parameter in considering survivability of microbes over geologic times on the frigid, arid surface of Mars that...

NASA’s Cassini spacecraft in orbit around Saturn. Image credit: NASA / JPL-Caltech.

Cassini Sheds New Light on Saturn’s Rings

Oct 19, 2022 by News Staff

The Ultraviolet Imaging Spectrograph instrument onboard NASA’s Cassini spacecraft observed 41 solar occultations by Saturn’s rings. Now, planetary...

Review of the mechanisms proposed in the literature to explain the emplacement of liquid reservoirs invoked to correspond to a variety of geological features at Europa’s surface. Image credit: Lesage et al., doi: 10.3847/PSJ/ac75bf.

Shallow Lakes in Europa’s Crust Could Erupt, Planetary Scientists Say

Oct 13, 2022 by News Staff

In the search for life beyond Earth, subsurface bodies of water in the outer Solar System are some of the most important targets. That’s why NASA and...

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.

Mars was Habitable for Methanogenic Microorganisms 3.7 Billion Years Ago, Study Suggests

Oct 10, 2022 by News Staff

The subsurface of Mars during the Noachian period was likely to have been habitable for microorganisms that feed on hydrogen and produce methane, according...

These images shows Jupiter’s icy moons Ganymede and Europa with Jupiter in the background. Image credit: ESO / King & Fletcher / NASA / ESA / A. Simon, NASA’s Goddard Space Flight Center / M.H. Wong, University of California, Berkeley / OPAL Team.

SPHERE Helps Determine Surface Compositions of Europa and Ganymede

Oct 10, 2022 by Natali Anderson

Astronomers using the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) instrument on ESO’s Very Large Telescope have imaged Jupiter’s...

This look at the complex, ice-covered surface of Europa came from Juno during a close pass on September 29, 2022. The spacecraft had only a two-hour window to collect it, racing past the moon with a relative velocity of about 23.6 km per second (14.7 miles per second). Image credit: NASA / JPL-Caltech / SWRI / MSSS.

Juno Flyby Reveals Stunning New Image of Europa

Sep 30, 2022 by News Staff

This new image of Jupiter’s moon Europa, captured during NASA’s Juno spacecraft’s closest approach on September 29, 2022, shows a region near the...

A panning-view of Jupiter’s upper atmospheric temperatures, 1,000 km (621 miles) above the cloud tops; the auroral region (near the northern pole, in yellow/white) appears to have shed a massive, planetary-scale wave of heating towards the equator. Image credit: NASA / ESA / Hubble / A. Simon / NASA’s Goddard Space Flight Center / J. Schmidt / O’Donoghue et al., doi: 10.5194/epsc2022-373.

Huge Heat Wave Spotted in Upper Atmosphere of Jupiter

Sep 23, 2022 by News Staff

The high-temperature planetary-scale-sized structure is at least 130,000 km (80,778 miles) long, according to a new study led by JAXA scientists. A panning-view...

This image of the asteroid Ryugu was captured by the Optical Navigation Camera - Telescopic (ONC-T) on JAXA’s Hayabusa-2 spacecraft on June 26, 2018, from a distance of 13.7 miles (22 km). Image credit: JAXA / University of Tokyo / Kochi University / Rikkyo University / Nagoya University / Chiba Institute of Technology / Meiji University / Aizu University / AIST.

Asteroid Ryugu’s Parent Body Formed in Outer Solar System, New Analysis Suggests

Sep 23, 2022 by News Staff

Samples of the near-Earth asteroid (162173) Ryugu were brought to Earth by JAXA’s Hayabusa-2 spacecraft. This image of the asteroid Ryugu was captured...

This image shows ‘frosted cupcake’ clouds in the atmosphere of Jupiter. The image was taken at a nominal altitude of 13,536.3 km above Jupiter’s cloud tops. image credit: NASA / JPL-Caltech / SwRI / MSSS / Gerald Eichstädt.

Juno Spots ‘Frosted Cupcake’ Clouds on Jupiter

Sep 22, 2022 by News Staff

Intensity data of visible light seen by a camera can be plotted as a 3D elevation landscape. The new computer animation, created by citizen scientist and...

Phosphorus in the form of orthophosphate (e.g., HPO4-2) is likely abundant in the subsurface ocean of Saturn’s moon Enceladus; a soda or alkaline ocean (containing NaHCO3 and/or Na2CO3) inside of Enceladus interacts geochemically with a rocky core; modeling indicates that this interaction promotes the dissolution of phosphate minerals, making orthophosphate readily available to possible life in the ocean; because phosphorus is an essential ingredient for life, this finding bolsters mounting evidence for habitability within this small Saturnian moon. Image credit: Southwest Research Institute.

Subsurface Ocean of Enceladus is Rich in Phosphorus, Suggests Study

Sep 20, 2022 by News Staff

Enceladus is one of the prime targets in the search for life in our Solar System. Observations made by NASA’s Cassini spacecraft show that this small...

These craters were formed by a meteoroid impact on Mars on September 5, 2021, the first to be detected by NASA’s InSight lander; taken by NASA’s Mars Reconnaissance Orbiter, this enhanced-color image highlights the dust and soil disturbed by the impact in blue in order to make details more visible to the human eye. Image credit: NASA / JPL-Caltech / University of Arizona.

NASA’s InSight Lander Detects Seismic and Acoustic Waves from Meteoroid Impacts on Mars

Sep 20, 2022 by News Staff

The Seismic Experiment for Internal Structure (SEIS) seismometer on NASA’s InSight lander picked up vibrations and sounds from four space rocks that...

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