We report results of an interdisciplinary project devoted to the 26 km‐diameter Ries crater
and to the genesis of suevite. Recent laboratory analyses of “crater suevite” occurring within …

More than 50 years of space and planetary exploration and concomitant studies of terrestrial
impact structures have demonstrated that impact cratering has been a fundamental process …

This article presents a current (as of September 2019) list of recommended ages for proven
terrestrial impact structures (n= 200) and deposits (n= 46) sourced from the primary …

Highly expanded Cretaceous–Paleogene (K-Pg) boundary section from the Chicxulub peak
ring, recovered by International Ocean Discovery Program (IODP)–International Continental …

Abstract The clay‐rich Glen Torridon region of Gale crater, Mars, was explored between sols
2300 and 3007. Here, we analyzed the diagenetic features observed by Curiosity, including …

We present the results of numerical modeling of the formation of the Ries crater utilizing the
two hydrocodes SOVA and iSALE. These standard models allow us to reproduce crater …

We modeled the differentiation of the South Pole–Aitken (SPA) impact melt sheet to
determine whether noritic lithologies observed within SPA formed as a result of the impact …

Abstract Northwest Africa 7533, a polymict Martian breccia, consists of fine‐grained clast‐
laden melt particles and microcrystalline matrix. While both melt and matrix contain medium …

Over the past few decades, it has become increasingly clear that the impact of interplanetary
bodies on other planetary bodies is one of the most ubiquitous and important geological …

Quantitative insights into the geochemistry and petrology of proximal impactites are
fundamental to understand the complex processes that affected target lithologies during and …