Morphological evidence for ancient channelized flows (fluvial and fluvial-like landforms)
exists on the surfaces of all of the inner planets and on some of the satellites of the Solar …

Orbiting and landed spacecrafts have provided vast amounts of data on fluvial and fluvial-
related landforms and sediments on Mars. One variant of these landforms consists of ridges …

We used imaging, laser altimeter and thermal infrared data to map a 0.5 by 0.5° area
containing the landing site of the Zhurong rover of the Tianwen‐1 mission. We analyzed the …

Gale Crater is filled by sedimentary deposits including a mound of layered deposits, Aeolis
Mons. Using orbital data, we mapped the crater infillings and measured their geometry to …

The Jezero crater open-basin lake contains two well-exposed fluvial sedimentary deposits
formed early in martian history. Here, we examine the geometry and architecture of the …

The landing site for the Curiosity rover is located at the distal end of the Peace Vallis fan in
Gale Crater. Peace Vallis fan covers 80 km2 and is fed by a 730 km2 catchment, which …

Sinuous ridges are important landforms on the surface of Mars that show promise for
quantifying ancient martian surface hydrology. Morphological similarity of these ridges to …

Sedimentary basins are the archives of ancient environmental conditions on planetary
surfaces, and on Mars they may contain the best record of surface water and habitable …

The paleo-meanders in the Aeolis Dorsa (AD) region show that meandering channels can
develop in the absence of vegetation. Three possible mechanisms other than vegetation …

Although there is little doubt that rivers once flowed on Mars' surface, how sustained and
frequent their flows were remains enigmatic. Understanding the hydrology of early Mars …