Tag Archive for Mars

Maurice et al. find that the speed of sound is slower on Mars than on Earth and that, mostly, a deep silence prevails. Image credit: Maurice et al., doi: 10.1038/s41586-022-04679-0.

Perseverance Characterizes Acoustic Environment of Mars

Apr 4, 2022 by News Staff

NASA’s Perseverance rover first recorded Martian sounds on February 19, 2021, the day after its arrival. These sounds fall within the human audible spectrum,...

This image shows Utopia Planitia, a plain that fills one of three major basins in the northern hemisphere of Mars. Image credit: ESA / DLR / FU Berlin / CC BY-SA 3.0 IGO.

Mars Express Sees Fascinating Ice-Related Features in Utopia Planitia

Mar 31, 2022 by News Staff

Utopia Planitia, a large lava plain in the northern hemisphere of Mars, has a diameter of roughly 3,300 km (2,051 miles) — just under twice the north-south...

NASA’s Perseverance rover acquired this image on April 22, 2021, using its left Mastcam-Z camera. Image credit: NASA / JPL-Caltech / MSSS.

NASA Extends Flight Operations of Mars Helicopter Ingenuity

Mar 21, 2022 by News Staff

NASA’s Ingenuity mission will support the science campaign of the agency’s Perseverance rover exploring the ancient river delta of Jezero Crater until...

This MAHLI image shows a tighter view of the flower-like rock artifact. Image credit: NASA / JPL-Caltech / MSSS.

NASA’s Curiosity Rover Finds ‘Coral’ on Mars

Mar 3, 2022 by Enrico de Lazaro

The Mars Hand Lens Imager on NASA’s Curiosity Mars rover has imaged a flower-like rock artifact in the Gale crater on Mars. This image from the MAHLI...

This image from ESA’s Trace Gas Orbiter shows a giant impact crater in Acidalia Planitia on Mars. Image credit: ESA / CaSSIS / CC BY-SA 3.0 IGO.

Trace Gas Orbiter Spots ‘Tree Stump’ Crater on Mars

Feb 2, 2022 by News Staff

ESA’s Trace Gas Orbiter (TGO) has spotted an ice-rich impact crater in Acidalia Planitia, a Martian plain between the Tharsis volcanic province and Arabia...

This image from the Context Camera onboard NASA’s Mars Reconnaissance Orbiter shows Bosporos Planum on Mars; the white specks are salt deposits found within a dry channel; the largest impact crater in the scene is nearly 1.5 km (one mile) across. Image credit: NASA / JPL-Caltech / MSSS.

Water Flowed on Martian Surface as Recently as Two Billion Years Ago, Study Suggests

Jan 27, 2022 by News Staff

It’s commonly believed that Martian liquid water evaporated about 3 billion years ago, but a duo of planetary scientists from Caltech and Johns Hopkins...

Mattei et al. studied the antifreeze properties of exotic salts that exist on Mars. Image credit: NASA / JPL-Caltech / USGS / SwRI.

Brine-Ice Mixtures Exist beneath Martian South Polar Cap: Study

Jan 26, 2022 by News Staff

In 2018, the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) instrument onboard ESA’s Mars Express orbiter found evidence of liquid...

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.

Study: Frequency of Asteroid Impacts in Inner Solar System Constant over Past 600 Million Years

Jan 21, 2022 by News Staff

Using a novel crater detection algorithm, which automatically counts the visible impact craters from a high-resolution image, a team of planetary researchers...

A selfie taken by NASA’s Mars rover Curiosity on Sol 2291 (January 15, 2019) at the ‘Rock Hall’ drill site, located on Vera Rubin Ridge. Image credit: NASA / JPL-Caltech / MSSS.

Curiosity’s Samples from Martian Crater Strongly Depleted in Carbon-13, Researchers Say

Jan 18, 2022 by News Staff

An analysis of carbon isotopes in sediment samples taken by NASA’s Curiosity rover from Gale crater, Mars, leave planetary researchers with three plausible...

Possible scenarios of terrestrial planet formation: in the classic Wetherill-type model of oligarchic growth, the terrestrial planets formed by mutual collisions among Moon- to Mars-sized planetary embryos after the gas disk dissipated and accreted only a small fraction of CC planetesimals, which were scattered inward during Jupiter’s growth and/or putative migration; alternatively, the terrestrial planets may have formed within the lifetime of the gas disk by efficiently accreting ‘pebbles’ from the outer Solar System, which drift sunward through the disk due to gas drag; the two models differ in the amount of outer solar system material accreted by the terrestrial planets, which may be quantified using nucleosynthetic isotope anomalies. Image credit: Burkhardt et al., doi: 10.1126/sciadv.abj7601.

Earth and Other Terrestrial Planets Formed from Inner Solar System Material, Study Suggests

Dec 28, 2021 by News Staff

Two fundamentally different processes of rocky planet formation exist, but it is unclear which one built the Earth and other terrestrial solar system planets....

Trace Gas Orbiter Finds Water Ice in Martian Polar Crater

Dec 27, 2021 by News Staff

ESA’s Trace Gas Orbiter has returned a stunning image of a 4-km- (2.5-mile) wide crater located in Vastitas Borealis, the largest lowland region of Mars. The...

Mars; the center of the scene shows the entire Valles Marineris canyon system. Image credit: NASA Goddard Space Flight Center.

ESA’s Trace Gas Orbiter Finds Water in Martian Canyon System

Dec 17, 2021 by News Staff

Planetary researchers using the Fine Resolution Epithermal Neutron Detector (FREND) instrument onboard ESA’s Trace Gas Orbiter (TGO) have found evidence...

The Mastcam-Z instrument on NASA’s Perseverance rover took this image of Ingenuity on December 1, 2021, when the rotorcraft was about 295 m (970 feet) away. Image credit: NASA / JPL-Caltech / ASU / MSSS.

Ingenuity Helicopter Completes Its Seventeenth Flight on Mars

Dec 16, 2021 by News Staff

On December 5, 2021, NASA’s Ingenuity helicopter successfully flew to a new destination located very close to its original airfield, Wright Brothers...

Curiosity used its navigation cameras to capture panoramas of this scene at two times of day. Image credit: NASA / JPL-Caltech.

Curiosity Team Releases Stunning Panorama of Martian Landscape

Nov 26, 2021 by News Staff

Members of NASA’s Curiosity rover mission team have combined two versions of the black-and-white images of Martian mountains from different times of...

This artist’s impression shows NASA’s InSight lander in Homestead Hollow, a small impact crater; the r SEIS seismometer is the light-colored hemisphere on the ground in front of the lander; the ground beneath it consists of a sandy regolith layer on top of alternate layers of sediments (yellow-orange colors) and basaltic rocks, i.e. former lava flows (brown colors). Image credit: Géraldine Zenhäusern / ETH Zürich.

Mars Has Multi-Layered Subsurface, New Study Says

Nov 24, 2021 by News Staff

Using seismic data collected by the SEIS (Seismic Experiment for Interior Structure) instrument aboard NASA’s InSight (Interior Exploration using Seismic...

Organic and inorganic biomorphs (small abiotic structures that bear a morphological resemblance to living or fossil microbes): (a) asteroidal trichites radiating from central magnetite grains in a natural volcanic glass; (b) organic microspheres obtained from RNA and quartz mixtures under diagenetic conditions; (c) amphiphilic spherical and tube-like vesicles formed by mixed fatty acids and 1-alkanols (C10-C15) in 10 mM CaCl2; (d) coacervate microdroplets prepared in water by mixing PDDA with ATP; (e, f ) chain-forming and twinning proteinoid microspheres obtained by heating mixtures of amino acids; (g, h) apatite particles formed by double diffusion in gelatin mimicking dividing cells and raised polygonal features in embryos; (i) rod-shaped silica particles formed on the walls of basalt fractures injected with supercritical CO2; (j) cryogenic opal filaments and sheets formed in rapidly freezing silica-rich fluids; (k) cryogenic carbonate segmented filaments obtained by freezing of silica-rich alkaline brines; (l) rod-shaped apatite particles forming within organic films in sediments; (m) fluoroapatite particle precipitated in the presence of citrate, mimicking dividing coccoid cells. Image credit: McMahon & Cosmidis, doi: 10.1144/jgs2021-050.

Martian Rocks May Contain Numerous Types of False Biosignatures, Astrobiologists Say

Nov 22, 2021 by News Staff

In a new paper published in the Journal of the Geological Society, University of Edinburgh’s Dr. Sean McMahon and University of Oxford’s Dr. Julie...

Levin et al suggest that we could have more in common with our extraterrestrial neighbors than initially thought. Image credit: Fernando Ribas.

Astrobiologists Call for New Framework in Search for Extraterrestrial Life

Nov 8, 2021 by News Staff

The question of whether we are alone in the Universe has been a source of wonder for humanity for millennia or more. Advances in planetary sciences, astronomy,...

This artist’s concept depicts NASA’s Mars rover Perseverance on the surface of the Red Planet. Image credit: NASA / JPL-Caltech.

NASA’s Perseverance Rover Records Martian Sounds

Oct 20, 2021 by News Staff

NASA’s Perseverance rover carries two microphones which are directly recording sounds on Mars, including wind gusts, rover wheels crunching over gravel,...

Perseverance Finds Ancient Delta-Lake System, Flood Deposits in Martian Jezero Crater

Oct 8, 2021 by News Staff

Planetary scientists have analyzed images taken by the Mastcam-Z camera and the Remote Micro-Imager of the SuperCam instrument on NASA’s Perseverance...

Valley networks and paleolake outlet canyons on Mars: (a) distribution of analyzed valley networks (black) and paleolake outlet canyons (white); gray shading indicates the combined latitude (poleward of ±30°) and age (younger than Early Hesperian) mask used for volume calculations; (b and c) examples of the early Martian landscape dissected by both valley networks (black) and paleolake outlet canyons (white); paleolake basin extents shown by semi-transparent white polygons. Image credit: Goudge et al., doi: 10.1038/s41586-021-03860-1.

Lake Breach Floods Eroded Surface of Early Mars, Study Says

Sep 30, 2021 by News Staff

Massive floods from overflowing crater lakes were responsible for eroding at least 24% of the volume of incised valleys on early Mars, according to new...

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