How tidal heating in Io drives the galilean orbital resonance locks
about
The E ring of Saturn and satellite EnceladusStrong tidal dissipation in Io and Jupiter from astrometric observations.Thermal stress tectonics on the satellites of Saturn and UranusAccretional heating of the satellites of Saturn and UranusConvection in Io's asthenosphere: Redistribution of nonuniform tidal heating by mean flowsHigh heat flow from Enceladus' south polar region measured using 10–600 cm−1Cassini/CIRS dataTidal-tectonic processes and their implications for the character of Europa's icy crust
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How tidal heating in Io drives the galilean orbital resonance locks
description
article publié dans la revue scientifique Nature
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scientific article published in Nature
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wetenschappelijk artikel
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наукова стаття, опублікована в Nature в червні 1979
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name
How tidal heating in Io drives the galilean orbital resonance locks
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How tidal heating in Io drives the galilean orbital resonance locks
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type
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How tidal heating in Io drives the galilean orbital resonance locks
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How tidal heating in Io drives the galilean orbital resonance locks
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How tidal heating in Io drives the galilean orbital resonance locks
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How tidal heating in Io drives the galilean orbital resonance locks
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How tidal heating in Io drives the galilean orbital resonance locks
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Charles F. Yoder
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10.1038/279767A0
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1979-06-01T00:00:00Z
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1050131686