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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...
Uloženo v:
| Hlavní autor: | |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
The Royal Society Publishing
2014
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| On-line přístup: | 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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