Mars Geology Lunar Geology Martian Geology Mars Icy Moons Sedimentary Rocks Martian Surface Martian Rocks Surface Composition Asteroid Composition Impact Cratering Martian Surface Features Mineralogy Martian Terrain Asteroid Geology Impact Craters Surface Features Asteroids Impact Events Seismology Volcanic Activity Surface Processes Volcanism Europa's Surface Sedimentary Processes Volcanic Rocks Meteorites Impact Geology Seismic Activity Subsurface Oceans Hydrothermal Systems Lunar Surface Features Moon Geology Sedimentology Volcanology Volcanic Features Martian Subsurface Mars Exploration Geological Activity Lunar Regolith Martian Geography Cryovolcanism Lunar Surface Martian Soil Lunar Composition Planetary Formation Canyons Crater Formation Moon Icy Bodies Ice on Planets Planetary Evolution Metallic Objects Sand Ripples Magma Crystallization Geological Mechanisms Rock Types Mars Rocks Planet Composition Igneous Rocks Planetary Differentiation Lunar Surface Composition Rock Forming Elements Martian Surface Analysis Martian Surface Processes Martian Material Martian Landscape Martian Crust Sedimentary Structures Carbon Cycle Meteorite Analysis Fluvial Processes Surface Morphology Lava Planets Core Structure Erosion Processes Internal Processes Ceres Thermal Models Thermal History Chemical Alteration Planet Formation Extraterrestrial Terrain Martian Minerals Venusian Surface Saturn Water on Mars Magnetic Fields Remote Sensing Cratons Martian Lakes Subsurface Water Martian Water Cycle Marsquakes Mars Geological History Surface History Core-Mantle Interaction Lunar Formation Craters Zonation
A Science Advances analysis links the ferric oxides to brief oxidizing vapors from ancient impacts.