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Collisional evolution of the mass-distribution spectrum of planetesimals II

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dc.contributor.author Matsui, Takafumi
dc.date.accessioned 2020-08-03T21:12:14Z
dc.date.available 2020-08-03T21:12:14Z
dc.date.issued 1979
dc.identifier.citation Proc. Lunar Planet. Sci. Conj. /0th (1979), p. 1881-1895. en
dc.identifier.uri https://hdl.handle.net/20.500.11753/1659
dc.description.abstract Conditions required for the early growth of planetesimals through their mutual collisions are investigated numerically with a Monte Carlo technique developed by the author. Four types of collisions (rebound, erosion, catastrophic break-up and coagulation) are taken into account. en
dc.format.extent Pages 1881-1895
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Pergamon Press en
dc.relation.ispartofseries LPI contribution ; no. 389
dc.subject Planets--Origin en
dc.title Collisional evolution of the mass-distribution spectrum of planetesimals II en
dc.type Book chapter en


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