EQUILIBRIUM NONSYNCHRONOUS ROTATION OF TITAN

被引:13
作者
SEARS, WD
LUNINE, JI
GREENBERG, R
机构
[1] Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, Tucson
关键词
D O I
10.1006/icar.1993.1123
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A satellite on an eccentric orbit experiences a zero net tidal torque when the rotation is slightly faster than synchronous, if there is no significant permanent asymmetry. Calculations indicate that for Titan this period should be 15.82 to 15.93 days, depending on the tidal dissipation model. This range includes the period recently determined by radar observations. A water-ice highland plateau with a diameter of less than 180 km standing just above the expected hydrocarbon ocean is consistent with both the radar data and the asymmetry constraints. © 1993 by Academic Press, Inc.
引用
收藏
页码:259 / 262
页数:4
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