Abstract
HYPOTHESES for the formation of the Earth–Moon system fall into one of three categories. The Moon was either (1) formed by fission from the Earth, (2) formed by accretion in Earth orbit, or (3) formed in solar orbit and then captured. We suggest that hypotheses (2) and (3) may be combined, with the result that many of the constraints on lunar origin are satisfied.
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CLARK, S., TURCOTTE, D. & NORDMANN, J. Accretional capture of the Moon. Nature 258, 219–220 (1975). https://doi.org/10.1038/258219a0
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DOI: https://doi.org/10.1038/258219a0
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