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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4813

Title: Tidal disruption of viscous bodies
Authors: Sridhar, S.
Tremaine, S.
Issue Date: Jan-1992
Publisher: Elsevier B.V.
Citation: ICARUS, 1992, Vol.95, p86
Abstract: Tidal disruptions are investigated in viscous-fluid planetesimals whose radius is small relative to the distance of closest (parabolic-orbit) approach to a planet. The planetesimal surface is in these conditions always ellipsoidal, facilitating treatment by coupled ODEs which are solvable with high accuracy. While the disrupted planetesimals evolve into needlelike ellipsoids, their density does not decrease. The validity of viscous fluid treatment holds for solid (ice or rock) planetesimals in cases where tidal stresses are greater than material strength, but integrity is maintained by self-gravity.
Description: Restricted Access.
URI: http://hdl.handle.net/2289/4813
ISSN: 0019-1035
Alternative Location: http://dx.doi.org/10.1016/0019-1035(92)90193-B
http://adsabs.harvard.edu/abs/1992Icar...95...86S
Copyright: 1992 Elsevier B.V.
Appears in Collections:Research Papers (A&A)

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