How tidal heating in Io drives the galilean orbital resonance locks View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1979-06

AUTHORS

Charles F. Yoder

ABSTRACT

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. More... »

PAGES

767-770

Journal

TITLE

Nature

ISSUE

5716

VOLUME

279

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/279767a0

DOI

http://dx.doi.org/10.1038/279767a0

DIMENSIONS

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