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Asymmetric shock heating and the terrestrial magma ocean origin of the Moon

One of the difficulties of the current giant impact model for the origin of the Moon is to explain the marked similarity in the isotopic compositions and the substantial differences in the major element chemistry. Physics of shock heating is analyzed to show that the degree of heating is asymmetric...

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Detalhes bibliográficos
Autor principal: KARATO, Shun-ichiro
Formato: Artigo
Idioma:Inglês
Publicado em: The Japan Academy 2014
Assuntos:
Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC3997809/
https://ncbi.nlm.nih.gov/pubmed/24621956
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.2183/pjab.90.97
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