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Io After Galileo: A New View of Jupiter’s Volcanic Moon

Jupiter’s moon Io is the Solar System’s most exotic satellite. Active volcanism on Io was discovered from observations by the Voyager 1 spacecraft in 1979, confirming a possibility suggested from theoretical studies of Io’s orbit. Our knowledge of Io’s volcanism, composition, and space environment w...

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Detalles Bibliográficos
Autores principales: Lopes, Rosaly M. C, Spencer, John R
Lenguaje:eng
Publicado: Praxis Publishing Ltd, Chichester, UK 2007
Materias:
Acceso en línea:https://dx.doi.org/10.1007/978-3-540-48841-5
http://cds.cern.ch/record/1338800
Descripción
Sumario:Jupiter’s moon Io is the Solar System’s most exotic satellite. Active volcanism on Io was discovered from observations by the Voyager 1 spacecraft in 1979, confirming a possibility suggested from theoretical studies of Io’s orbit. Our knowledge of Io’s volcanism, composition, and space environment were significantly increased as a result of observations by the Galileo spacecraft from 1996 through 2001. The end of the Galileo mission in 2003 makes this an ideal time to summarize the new results in a book as no book has ever been written about Jupiter’s volcanic moon, Io.