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Lunar-forming impacts: processes and alternatives

The formation of a protolunar disc by a giant impact with the early Earth is discussed, focusing on two classes of impacts: (i) canonical impacts, in which a Mars-sized impactor produces a planet–disc system whose angular momentum is comparable to that in the current Earth and Moon, and (ii) high-an...

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Bibliografski detalji
Glavni autor: Canup, R. M.
Format: Artigo
Jezik:Inglês
Izdano: The Royal Society Publishing 2014
Teme:
Online pristup:https://ncbi.nlm.nih.gov/pmc/articles/PMC4128262/
https://ncbi.nlm.nih.gov/pubmed/25114302
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2013.0175
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