HOW TIDAL HEATING IN IO DRIVES THE GALILEAN ORBITAL RESONANCE LOCKS

被引：154

作者：

YODER, CF

机构：

[1] Jet Propulsion Laboratory, California Institute of Technology, Pasadena

来源：

NATURE | 1979年 / 279卷 / 5716期

关键词：

D O I：

10.1038/279767a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Tidal heating in Io is the most likely energy source of its volcanic activity. Tidal dissipation in Io and Jupiter also controls the resonance configuration among the three inner satellites. The formation of the several resonance locks is described in detail in this article. This model sets limits on the Q values of both Io and Jupiter. © 1979 Nature Publishing Group.

引用

页码：767 / 770

页数：4

共 10 条

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