Dust plays a key role in many Earth system processes and is ubiquitous in the Martian
atmosphere. Various intensive field campaigns, laboratory analyses, space-based remote …

Decades of space exploration reveal that Mars has been reshaped by volcanism throughout
its history. The range of observed volcanic landforms shows that effusive and explosive …

Combining U–Pb ages with Lu–Hf data in zircon provides insights into the magmatic history
of rocky planets. The Northwest Africa (NWA) 7034/7533 meteorites are samples of the …

Subsurface reflectors in radar sounder data from the Mars Advanced Radar for Subsurface
and Ionospheric Sounding instrument aboard the Mars Express spacecraft indicate …

Long-lived hydrothermal systems are prime targets for astrobiological exploration on Mars.
Unlike magmatic or impact settings, radiogenic hydrothermal systems can survive for> 100 …

Much has been discovered about volcanism on Mars over the past fifty years of space
exploration. Previous reviews of these discoveries have generally focused on the volcanic …

The ubiquitous eolian dust on Mars plays important roles in the current sedimentary and
atmospheric processes of the planet. The ChemCam instrument retrieves a consistent eolian …

Elysium Planitia includes several outflow channels that were likely carved by aqueous
erosion and subsequently infilled by younger lava flows, making Elysium Planitia the …

Abstract The extensive Medusae Fossae Formation (MFF) along the dichotomy boundary on
Mars has geologic features indicative of wind erosion of low‐density material. There is …

Abstract The Medusae Fossae Formation (MFF) is one of the largest unconformable
deposits on Mars. The origin of the MFF is unknown, but several formation processes have …