期刊
ICARUS
卷 193, 期 2, 页码 637-640出版社
ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2007.09.002
关键词
extrasolar planets; satellites; dynamics; tides; solid body
Expressions for tidal dissipation in a body in synchronous rotation at arbitrary orbital eccentricity and obliquity are derived. The rate of tidal dissipation for a synchronously rotating body is compared to that in a body in asymptotic nonsynchronous rotation. (c) 2007 Elsevier Inc. All rights reserved.
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