Cavities on the equator of rotating asteroids
What is it about?
This is a study of the possible origin of the cavities found in small, rotating asteroids. We take a look especially at asteroid 2008 EV5 and DP107. We show that it is possible that the cavities observed in their equatorial regions were formed not by impacts, but by the ejection of a sizable piece of the original bodies.
Why is it important?
It provides a plausible explanation for these equatorial cavities and gives some evidence to the hypothesis that the secondary of a binary asteroid could have been formed by an important fission event that ejected a large, coherent piece and not by the slow re-acreation of ejected particles.
The following have contributed to this page: Dr Diego P Sánchez Lana
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