The Dynamical Complexity of Surface Mass Shedding from a Top-shaped Asteroid Near the Critical Spin Limit

The Dynamical Complexity of Surface Mass Shedding from a Top-shaped Asteroid Near the Critical Spin Limit
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接近临界自旋极限的顶形小行星表面质量脱落的动力学复杂性

DOI:
10.3847/1538-3881/aaccf7
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发表时间:
2018-07
期刊:
The Astronomical Journal
影响因子:
--
通讯作者:
Liu X.
Liu X.
中科院分区:
其他
文献类型:
--
作者:
Yu Y.;Michel P.;Hirabayashi M.;Schwartz S. R.;Zhang Y.;Richardson D. C.;Liu X.

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The regolith transport near the surface of an asteroid is inherently sensitive to the local topography. In this paper, conditions of surface mass shedding and the subsequent evolution of the shedding material are studied for the primary of 65803 Didymos,
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