The source craters of the martian meteorites: Implications for the igneous evolution of Mars

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 observations and modeling to constrain the source craters for several groups of martian meteorites. We compute that ejection-paired groups of meteorites are derived from lava flows within the top 26 m of the surface. We link ejection-paired groups to specific source craters and geologic units, providing context for these important samples, reconciling microscopic observations with remote sensing records, and demonstrating the potential to constrain the ages of their source geologic units. Furthermore, we show that there are craters that may have produced martian meteorites not represented in the world's meteorite collections that have yet to be discovered.

Authors

Institutions

Publication Details

Journal
Science Advances
Published
2024-08-16
DOI
https://doi.org/10.1126/sciadv.adn2378
Citations
16
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
5.30

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

The source craters of the martian meteorites: Implications for the igneous evolution of Mars

Anthony Lagain, Brandon Johnson, G. K. Benedix, Sean Wiggins et al.
16 citations
Science Advances
Astro and Planetary Science
5.30
article

The source craters of the martian meteorites: Implications for the igneous evolution of Mars

Anthony Lagain, Brandon Johnson, G. K. Benedix, Sean Wiggins, James R. Darling, L. L. Tornabene, E. L. Walton, J. S. Hamilton, H. J. Melosh, Alex I. Sheen, C. D. K. Herd, T. G. Sharp
article en
16 citations

Abstract

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 observations and modeling to constrain the source craters for several groups of martian meteorites. We compute that ejection-paired groups of meteorites are derived from lava flows within the top 26 m of the surface. We link ejection-paired groups to specific source craters and geologic units, providing context for these important samples, reconciling microscopic observations with remote sensing records, and demonstrating the potential to constrain the ages of their source geologic units. Furthermore, we show that there are craters that may have produced martian meteorites not represented in the world's meteorite collections that have yet to be discovered.

Science AdvancesVol. 10(33)
Western University (CA), Lawrence Livermore National Laboratory (US), Centre National de la Recherche Scientifique (FR), Planetary Science Institute (US), University of Alberta (CA), University of Toronto (CA), Curtin University (AU), Aix-Marseille Université (FR), Purdue University West Lafayette (US), Royal Ontario Museum (CA), Western Australian Museum (AU), Centre de Recherche et d’Enseignement de Géosciences de l’Environnement (FR), Institut de Recherche pour le Développement (FR), Arizona State University (US), University of Portsmouth (GB), Search for Extraterrestrial Intelligence (US), MacEwan University (CA)
University of Alberta, Science and Technology Facilities Council
Openalex Percentile: Top 4%
Astro and Planetary Science
5.30
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.