Rubble Pile Asteroids: Stability of Equilibrium Shapes

Details Rubble Pile Asteroids: Stability of Equilibrium Shapes Rubble Pile Asteroids: Stability of Equilibrium Shapes

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1843h&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1843

Physics

1

Scientific paper

A new approach to derive limit equilibrium shapes for rubble-pile
asteroids with spin is given. Stability considerations are then
formulated. Stability constraints limit the equilibrium shapes
considerably, just as is the case for fluid bodies.

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