Results of our detailed geological map** and interpretation of the nature and relative and
absolute model ages of units and structures in the SW portion of Utopia Planitia (20–45° N …

Passive degassing, or volatile release from persistent, non-eruptive volcanic activity, may
have contributed significantly to the Martian ice budget over the planet's history by providing …

The planet Mars is the most probable among the terrestrial planets in our solar system to
support human settlement or colonization in the future. The detection of water ice or liquid …

Abstract Hrad Vallis is an Amazonian‐age outflow channel located in the northwestern part
of the Elysium Volcanic Province of Mars. The formation of Hrad Vallis may have been …

Abstract The Central Elysium Planitia region contains evidence for large-scale, Late
Amazonian volcanic and fluvial activity, the youngest on Mars. The region consists of a …

Basaltic lava flows are common on the surface of the Earth and other terrestrial bodies.
However, inflation—including a combination of initially rapid molten core thickening and …

Mars is the most similar planet to the Earth in the solar system. Due to its diverse aqueous
history and the capability to preserve ancient life, Mars has been one of the major planets …

Abstract Hrad Vallis is a Martian outflow channel previously interpreted as a product of
aqueous outbursts from the subsurface, possibly involving mudflows associated with lahar …

This review summarizes the use of High Resolution Stereo Camera (HRSC) data as an
instrumental tool and its application in the analysis of geological processes and landforms …

Tianwen-1 is China's first independent Mars exploration mission. The rover “Zhurong”
landed in the southern Utopia Planitia where various landforms such as impact craters …