Lunar accretion from an impact-generated disk

被引：0
|
作者：
Shigeru Ida
Robin M. Canup
Glen R. Stewart
机构：
[1] Tokyo Institute of Technology,Department of Earth and Planetary Sciences
[2] LASP,undefined
[3] University of Colorado,undefined
来源：
Nature | 1997年 / 389卷
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摘要：
Although the mechanism by which the Moon was formed is currently unknown, several lines of evidence point to its accretion from a circumterrestrial disk of debris generated by a giant impact on the Earth. Theoretical simulations show that a single large moon can be produced from such a disk in less than a year, and establish a direct relationship between the size of the accreted moon and the initial configuration of the debris disk.
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页码：353 / 357
页数：4
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