期刊
ICARUS
卷 150, 期 2, 页码 288-296出版社
ACADEMIC PRESS INC
DOI: 10.1006/icar.2000.6581
关键词
moon; impact processes; planetary formation; satellites; accretion
We describe a scaling relationship that can be used to characterize the results of numerical smooth particle hydrodynamic (SPH) experiments of potential satellite-forming impacts. The relationship is used to interpret and summarize data from 41 such SPH simulations, all employing an impactor-to-target mass ratio of 3:7, but with a variety of total masses and angular momenta, The results can be utilized to infer other classes of impacts beyond those simulated to date that are plausible Moon-forming candidates. (C) 2001 Academic Press.
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