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Modelling Large Body Impacts

Published online by Cambridge University Press:  25 April 2016

Helen Pongracic
Helen Pongracic*
Affiliation:
Department of Mathematics, Monash University
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Abstract

Hypervelocity impacts are considered to be the main mechanism for the production of craters on the surfaces of planets and moons. Two- and three-dimensional numerical simulations for the first few seconds of large-body impacts will be discussed. Both normal and oblique impacts will be considered, with particular emphasis being placed on the distribution of impact products.

Type
Theoretical
Information
Publications of the Astronomical Society of Australia , Volume 7 , Issue 2 , 1987 , pp. 136 - 138
Copyright
Copyright © Astronomical Society of Australia 1987

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