The formation of impact craters is a highly dynamic and complex process that subjects the
impacted target rocks to numerous types of deformation mechanisms. Understanding and …

This study aims to assess the spatial and visible/near-infrared (VNIR) colour/spectral
capabilities of the 4-band Colour and Stereo Surface Imaging System (CaSSIS) aboard the …

We compiled a high‐resolution, global lunar impact crater database composed of 5,505
pristine craters≥~ 3 km. This database contains detailed morphometric data, and their …

Ceres is a partially differentiated dwarf planet, as confirmed by NASA's Dawn mission. The
Urvara basin (diameter~ 170 km) is its third-largest impact feature, enabling insights into the …

The Ries crater is a well‐preserved, complex impact crater that has been extensively used in
the study of impact crater formation processes across the solar system. However, its …

Most impacts occur at an angle with respect to the horizontal plane. This is primarily
reflected in the ejecta distribution, but at very low angle structural asymmetries such as …

The investigation of terrestrial impact structures is crucial to gain an in‐depth understanding
of impact cratering processes in the solar system. Here, we use the impact structure Jebel …

The ejecta blankets of impact craters in volatile‐rich environments often possess
characteristic layered ejecta morphologies. The so‐called double‐layered ejecta (DLE) …

The Ramgarh structure is a morphological landmark in southeastern Rajasthan, India. Its
200 m high and 3.5–4 km wide annular collar has provoked many hypotheses regarding its …

Comparing craters of identical diameter on a planet is an empirical method of studying the
effects of different target and impactor properties while holding total impact energy nearly …