Bounds on Rotation Periods of Disrupted Binaries in the Full 2-Body Problem

Details Bounds on Rotation Periods of Disrupted Binaries in the Full 2-Body Problem Bounds on Rotation Periods of Disrupted Binaries in the Full 2-Body Problem

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cemda..89..127s&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, v. 89, Issue 2, p. 127-140 (2004).

Astronomy and Astrophysics

Astronomy

6

Asteroids, Full 2-Body Problem, Gravitational Potentials, Rotation

Scientific paper

Constraints on the final rotation rates of a Hill unstable binary in the
full 2-body problem are derived and analyzed. Application of these
constraints are made to the problem of a constant density body spun to
disruption. This analysis has relevance to the evolution of asteroid
spin rates.

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