Melting of Io by Tidal Dissipation
The dissipation of tidal energy in Jupiter's satellite Io is likely to have melted a major fraction of the mass. Consequences of a largely molten interior may be evident in pictures of Io's surface returned by Voyager I.
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| Veröffentlicht in: | Science (American Association for the Advancement of Science) 1979-03, Vol.203 (4383), p.892-894 |
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| container_end_page | 894 |
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| container_issue | 4383 |
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| container_title | Science (American Association for the Advancement of Science) |
| container_volume | 203 |
| creator | Peale, S. J. Cassen, P. Reynolds, R. T. |
| description | The dissipation of tidal energy in Jupiter's satellite Io is likely to have melted a major fraction of the mass. Consequences of a largely molten interior may be evident in pictures of Io's surface returned by Voyager I. |
| doi_str_mv | 10.1126/science.203.4383.892 |
| format | Article |
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| fulltext | fulltext |
| identifier | ISSN: 0036-8075 |
| ispartof | Science (American Association for the Advancement of Science), 1979-03, Vol.203 (4383), p.892-894 |
| issn | 0036-8075 1095-9203 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_733194392 |
| source | JSTOR Archive Collection A-Z Listing; American Association for the Advancement of Science |
| subjects | Artificial satellites Galilean satellites Jovian satellites Jupiter Liquids Mantle Melting Numerical eccentricity Orbital motion Solids |
| title | Melting of Io by Tidal Dissipation |
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