nontronite Archives

Colorized HiRISE map of the western edge of Jezero crater with rover traverse. The colors of the traverse indicate the location of different science campaigns with green showing the Crater Floor campaign (Section 2.1), orange showing the Fan Front campaign (Section 2.2), blue showing the Upper Fan campaign (Section 2.2), and pink showing the Margin Unit campaign (Section 2.4). Black arrows indicate the location of two investigations on boulders (Section 2.3). Planetary Instrument for X-ray Lithochemistry (PIXL) scans are indicated by either a square, triangle, or circle, indicating data collected on a natural surface target, an abrasion patch, or an abrasion patch where a sample was also collected, respectively. Sols associated with the triangles and circles indicate when the rover was at that location. The location of Three Forks Depot is shown by a star for reference. Journal of Geophysical Research: Planets

Astrogeology, Atmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Biosignatures & Paleobiology, Caves, Craters, Mountains, Subsurface, Lava Tubes, Desert Worlds, Fossils & Paleontology, Habitable Zones, Imaging & Spectroscopy, Mars, Missions & Hardware, Robotics/Rovers/UAVs, Status Report

Multiple Episodes of Fluid Alteration in Jezero Crater Indicated by MIST Mineral Identifications in PIXL XRF Data

by Keith CowingSeptember 23, 2025September 23, 2025

The Mineral Identification by Stoichiometry (MIST) algorithm can identify mineral species in geochemical data sets. MIST is applied to X-ray fluorescence chemical analyses from the Planetary Instrument for X-ray Lithochemistry […]

Mineralogical map of Jezero crater explored by the Perseverance rover. This mineral map was created from near-infrared (1-2.6 µm) CRISM imagery (Parente et al., 2021) using recently developed technologies (Itoh et al., 2021; Saranathan et al., 2021) and overlain on High Resolution Imaging Science Experiment (HiRISE ) imagery. The basaltic rocks at the landing site are dominated by the minerals olivine (red) and pyroxene (tan). Further west, in regions called the Western Fan and Margin Unit, sedimentary rocks predominate. Smectite clay minerals rich in iron and magnesium (light to dark blue tones) and carbonate rich in magnesium and iron (green-yellow tones) were formed through aqueous processes. Unusual iron phosphate and iron sulfide minerals were found at the Bright Angel and Masonic Temple sites near Neretva Vallis (Hurowitz et al., 2025). Other iron phosphate minerals were observed at the Onahu site in the Western Fan region. Credit M. Parente

Analog Studies, Arctic / Antarctic / Alpine, Biosignatures & Paleobiology, Caves, Craters, Mountains, Subsurface, Lava Tubes, Habitable Zones, Mars, Missions & Hardware, Origin & Evolution of Life, Planetary Protection & Biosafety, Press Release, Robotics/Rovers/UAVs

Perseverance Rover Uncovers Clues To Ancient Martian Chemistry

by Keith CowingSeptember 11, 2025

NASA’s Perseverance Rover spent three years exploring the floor of Jezero Crater, located just north of the Martian equator.

nontronite

Multiple Episodes of Fluid Alteration in Jezero Crater Indicated by MIST Mineral Identifications in PIXL XRF Data

Perseverance Rover Uncovers Clues To Ancient Martian Chemistry

Astrobiology Graduate Conference (AbGradCon) 2026

Lava World Recon: Juno Measures Subsurface Temperature Of Io

Mars Curiosity Blog Sols 4961-4967: Approaching a Break in the Rock Record?

Segment-level Thermal Sensitivity Analysis For Exo-Earth Coronagraphy With Segmented Space Telescopes

Decoding Animal Communication With AI