Extensive fields of sub-kilometre-to kilometre-scale mounds, cones, domes, shields, and
flow-like edifices cover large parts of the martian lowlands. These features have been …

One important scientific objective of China's first Mars mission (Tianwen‐1) is to investigate
the martian surface soil characteristics and water‐ice distribution. Layered ejecta craters …

The southern part of the smooth plain of Chryse Planitia on Mars hosts a large population of
kilometer‐sized (from~ 0.2 to~ 20 km) landforms spread over a wide area. Based on the …

Several ejecta deposits on Ceres display morphological characteristics not commonly
associated with dry ballistic emplacement. We characterized 30 examples of fluidized …

Impact craters are the dominant features on the Moon, and their degradation with time is the
most common geological process on this body. This work is aimed at detailed quantitative …

Inter-crater depressions on Mars, which may be host to candidate lakes, have not been
explored in much detail. Even if a small percentage of these depressions were actually filled …

Double‐layered ejecta (DLE) craters are distinctive among the variety of crater
morphologies observed on Mars, but the mechanism by which they form remains under …

Excess ice is widespread throughout the martian mid-latitudes, particularly in Arcadia
Planitia, where double-layer ejecta (DLE) craters also tend to be abundant. In this region, we …

Understanding the morphological characteristics of craters that are indicative of their
formation environment can provide insight into surface geology. Layered ejecta (LE) craters …

Thermal mixing below the spatial resolution of thermal infrared (TIR) instruments can
produce negatively sloped emissivity spectra at longer wavelengths that may inhibit …