Collisional evolution of mass-distribution spectrum of planetesimals

dc.contributor.author	Matsui, Takafumi
dc.date.accessioned	2020-05-11T20:15:18Z
dc.date.available	2020-05-11T20:15:18Z
dc.date.issued	1978
dc.identifier.uri	https://hdl.handle.net/20.500.11753/1521
dc.description.abstract	The early growth of planetesimals by mutual direct collisions is numerically simulated with a Monte Carlo technique to show how planetesimals with specific mass and velocity distributions evolve into a full-size planet. Four types of collisions are taken into into account: rebound, erosion, catastrophic break-up, and coagulation.	en
dc.description.statementofresponsibility	Takafumi Matsui
dc.format.extent	Pages 1-13
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Pergamon Press	en
dc.relation.ispartofseries	LSI contribution ; no. 331
dc.subject	Planets--Origin	en
dc.subject	Collisions (Astrophysics)	en
dc.title	Collisional evolution of mass-distribution spectrum of planetesimals	en
dc.type	Book chapter	en

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