Tag Archive for 'Mars Reconnaissance Orbiter'

Charalambous et al. associate a new 21.5-m Mars impact crater in the tectonically active Cerberus Fossae region with InSight’s seismic event, S0794a. Image credit: NASA / JPL-Caltech / University of Arizona.

Impact-Generated Marsquakes Can Reach Deeper into Red Planet than Previously Known

Feb 4, 2025 by News Staff

In a new study, planetary researchers used global and high-resolution orbital imaging to discover a fresh, 21.5-m (71-foot) impact crater that appeared...

Fawdon et al. created the most detailed geologic map of Oxia Planum, the landing site for ESA’s Rosalind Franklin rover on Mars. Image credit: Fawdon et al., doi: 10.1080/17445647.2024.2302361.

Scientists Create High-Resolution Geological Map of Oxia Planum

Mar 27, 2024 by News Staff

Using data from ESA’s ExoMars Trace Gas Orbiter and NASA’s Mars Reconnaissance Orbiter, planetary scientists have created the 1:30000 scale geological...

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...

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...

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...

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...

The detailed global map of hydrated mineral deposits on Mars; various landing sites and areas of interest are shown; Mawrth Vallis is an ancient water outflow channel that is rich in clays; Oxia Planum is another clay-rich region and has been selected as the landing site for ESA’s Rosalind Franklin rover; Meridiani Planum straddles the Martian equator and was the landing spot for NASA’s Mars Exploration Rover Opportunity in 2004; Valles Marineris is one of the largest canyons in the Solar System’ Gale crater and Jezero crater were the landing sites of NASA’s Curiosity and Perseverance rovers in 2012 and 2020, respectively. Image credit: ESA / Mars Express / NASA / Mars Reconnaissance Orbiter.

Planetary Scientists Create First Global High-Resolution Map of Martian Aqueous Minerals

Aug 23, 2022 by News Staff

The newly-released map shows the locations and abundances of secondary minerals formed through interaction with water on Mars. It is based on the analysis...

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...

This image, acquired by NASA’s Mars Reconnaissance Orbiter on October 1, 2020, shows several craters in Arabia Terra filled with layered rock. Image credit: NASA / Molly Wasser.

Early Mars Experienced Volcanic Supereruptions, Reseachers Say

Sep 16, 2021 by News Staff

Using high-resolution images from NASA’s Mars Reconnaissance Orbiter, planetary scientists have discovered 4-billion-year-old layered deposits containing...

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

Regional Dust Storms Enhance Martian Water Loss to Space: Study

Aug 17, 2021 by News Staff

Individual regional dust events can boost planetary water loss by a factor of five to ten and represent an important driver of atmospheric evolution on...

Visible images with sketch maps showing major geologic features within as-yet unnamed crater mapped by Boatwright & Head: (a) the 54-km-diameter crater in the southern highlands of Mars (20.3°S, 42.6°E); no inlet or outlet breaches are observed; ridge networks (blue) begin near the crater wall base, where they are coincident with upslope-facing scarps (dashed lines) and crater wall alcoves; ridges terminate in two paleolake basins (cyan and green); (b) morphology of the eastern ridge network transitions downslope from dense proximal ridges to more widely spaced medial ridges; several medial ridges then converge into a single trunk ridge; (c) the southern ridge network terminates at three separate points along the margin of basin II. One of the ridges also displays an anabranching morphology. Image credit: Boatwright & Head, doi: 10.3847/PSJ/abe773.

New Type of Paleolake Spotted on Mars

Mar 31, 2021 by News Staff

A 54-km- (33.5-mile) diameter Noachian-aged crater with neither inlet nor outlet channels is distinct from previously documented crater basin lakes on...

Hernández-Bernal et al. reveal the daily and seasonal behavior of the AMEC cloud, using new observations from the Visual Monitoring Camera on ESA’s Mars Express, along with data from other Mars orbiters. Image credit: ESA.

Martian Orbiters Observe Extremely Elongated Cloud over Arsia Mons Volcano

Mar 19, 2021 by News Staff

In September and October 2018, ESA’s Mars Express orbiter observed a spectacular water ice cloud — named the Arsia Mons Elongated Cloud (AMEC)...

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...

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 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...

Channel-forms preserved in sedimentary layers in Hellas Planitia on Mars. Image credit: NASA / JPL-Caltech / University of Arizona / Matt Balme.

Deep, Perennial or Semi-Perennial Rivers Flowed on Early Mars

May 7, 2020 by News Staff

While the present-day Martian surface is generally dry and cold, its sedimentary rocks contain compelling evidence for the former presence of liquid water....

This map shows near-surface water ice on Mars; cool colors represent less than one foot (30 cm) below the surface; warm colors are over two feet (60 cm) deep; sprawling brown zones on the map represent areas where a landing spacecraft would sink into fine dust; the outlined box represents the ideal region to send astronauts for them to be able to dig up water ice. Image credit: NASA / JPL-Caltech / ASU.

New Map Shows Near-Surface Water Ice on Mars

Dec 12, 2019 by News Staff

Using data from NASA’s Mars Reconnaissance Orbiter and Mars Odyssey orbiter, a team of planetary researchers have crated a map of the water ice depth...

The yellow-white cloud in the bottom-center of this image, taken on November 30, 2010 by NASA’s Mars Reconnaissance Orbiter, is a ‘dust tower’ -- a concentrated cloud of dust that can be lofted dozens of miles above the surface. The blue-white plumes are water vapor clouds. Image credit: NASA / JPL-Caltech / MSSS.

‘Dust Towers’ Spotted on Mars

Nov 28, 2019 by News Staff

NASA’s Mars Reconnaissance Orbiter observed a high number of ‘dust towers’ — concentrated clouds of dust that warm in sunlight and rise high...

This image from NASA’s Mars Reconnaissance Orbiter shows Jezero Crater on Mars, the landing site for NASA’s Mars 2020 mission. On ancient Mars, water carved channels and transported sediments to form fans and deltas within lake basins. Examination of spectral data acquired from orbit show that some of these sediments have minerals that indicate chemical alteration by water. Here in Jezero Crater delta, sediments contain clays and carbonates. Image credit: NASA / JPL-Caltech / MSSS / JHU-APL.

NASA’s Mars Reconnaissance Orbiter Finds Hydrated Silica in Jezero Crater

Nov 14, 2019 by News Staff

Using data from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) instrument aboard NASA’s Mars Reconnaissance Orbiter, researchers have...

Area of the study: (a) Valles Marineris, Mars, showing the location of the landslide in Coprates Chasma (white box); (b) stereo-derived DEMs; (c and d) study areas within which morphological and morphometric characterization is conducted; burgundy lines: topographic profiles, numbered from proximal to distal edge of the landslide deposit; blue lines: longitudinal ridges; (e) oblique view of the landslide object of the study; red lines represent topographic profiles, numbered from proximal to distal area (following flow direction). Image credit: Magnarini et al, doi: 10.1038/s41467-019-12734-0.

Planetary Researchers Analyze Structure of Giant Martian Landslide

Oct 25, 2019 by News Staff

Unusually large and long ridges documented in massive landslides across our Solar System are commonly associated with the presence of ancient ice layers....

12 3