Large impact cratering during lunar magma ocean solidification

Lunar impact basins formed during the magma ocean solidification should have formed almost unidentifiable topographic and crustal thickness signatures, thus may escape detection. This result allows for a higher impact flux in the earliest epoch of Earth-Moon evolution.

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Autores principales: K. Miljković, M. A. Wieczorek, M. Laneuville, A. Nemchin, P. A. Bland, M. T. Zuber
Formato: article
Lenguaje:EN
Publicado: Nature Portfolio 2021
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Acceso en línea:https://doaj.org/article/0e806c45c25943c29f2665154896bf41
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