Collisional evolution of the mass-distribution spectrum of planetesimals II

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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Documents the scientific research, meetings, and outreach products from the LPI.