Science ❯ Geology ❯ Planetary Geology
Jezero Crater Gale Crater Rock Analysis Rock Samples Mineralogy Mineral Analysis Sedimentary Rocks Water on Mars Subsurface Water Sedimentary Structures Geological Formations Marsquakes Gediz Vallis Carbon Cycle Rock Formations Subsurface Water Reservoirs Cheyava Falls Rock Impact Events Rock Composition Seismic Activity Subsurface Analysis Water History Cheyava Falls Neretva Vallis Oxia Planum Mars Noachian Period Noachian Period Carbon Deposits Mount Sharp Surface Processes Olivin-Mikrogabbro-Shergottit Spherules Water Activity Subsurface Water Detection Water Evidence Geomorphology Volcanism Mineral Composition Carbonate Rocks Carbonate Minerals Meteorite Composition Ancient Riverbeds Erosion and Sedimentation Rock Sample Analysis Ice Composition Ancient Martian Climate Mars Surface Analysis Core Structure Erosion Processes Aeolian Bedforms Ancient River Valleys Biosignatures Mineral Discovery Ancient Environments Bright Angel Formation Biomarkers River Deltas Boxwork Unit Boxwork Features Sedimentary Processes Sample Analysis Subglacial Lakes Sample Collection on Mars Ancient Habitability Sedimentary Features Boxwork Ridges Water Loss Mechanisms Chemical Signatures Seismic Measurements Seismic Studies on Mars Liquid Water Hydrological History Liquid Water in Mars Crust InSight Mission Water Reservoirs on Mars Carbon Dioxide Ice Mantle Processes Atmospheric Evolution Rover Findings Martian Rocks Martian Surface Water-Related Features Gediz Vallis Channel Sulfur Crystals Sulfur Discovery Sulfate-Rich Rock Studies Sedimentology Ancient Beaches Stratigraphy Curiosity Geological Observations
Peer-reviewed analysis of the rover’s deepest radar scans points to earlier long-lived surface water, expanding prospects for preserved biosignatures.