Mars' crustal magnetic field holds information on the planet's interior evolution and exterior
processes that have modified the crust. Crustal magnetization records an ancient dynamo …

Seismic observations of impacts on Mars indicate a higher impact flux than previously
measured. Using six confirmed seismic impact detections near the NASA InSight lander and …

Physical materials from planetary bodies are crucial for understanding fundamental
processes that constrain the evolution of the solar system, as samples can be analyzed at …

The formation and differentiation of the crust of Mars in the first tens of millions of years after
its accretion can only be deciphered from incredibly limited records. The martian breccia …

Approximately 200 meteorites come from~ 10 impact events on the surface of Mars, yet their
pre-ejection locations are largely unknown. Here, we combine the results of diverse sets of …

Abstract The Cretaceous-Paleogene Boundary (KPB), the only known global impact ejecta
layer, resulted from the Chicxulub Impact Event (66 Ma). KPB is well-documented across the …

The goal of classifying shock metamorphic features in meteorites is to estimate the
corresponding shock pressure conditions. However, the temperature variability of shock …

Diaplectic feldspathic glass, commonly known as maskelynite, is a widely used impact
indicator, notably for shergottites, whose shock conditions are keys to their geochemistry …

Abstract The Mars Reconnaissance Orbiter and its Context Camera (CTX) have acquired
more than 100,000 separate panchromatic images that capture nearly the entire surface of …

Ejecta blankets around craters on a km-scale show stark differences in the ejecta mobility
(maximal extent of ejecta divided by the crater radius) with latitude and types of plains on …