Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-18T05:26:09.807Z Has data issue: false hasContentIssue false

Io's Escaping Atmosphere: Continuing the Legacy of Surprise

Published online by Cambridge University Press:  03 November 2010

Nicholas M. Schneider*
Affiliation:
LASP, University of Colorado, Boulder CO 80309, USA email: nick.schneider@lasp.colorado.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The discovery of Io and her fellow Medicean Stars clearly altered the course of science as a whole. It is equally clear that the discovery of Io's tidal heating has altered the course of planetary science. One of the most directly observable consequences of Io's tidal heating is the prodigious escape of a ton per second of volcanically-supplied gases. I will review how studies of Io's escaping atmosphere since 1972 have advanced our deep understanding of Io itself, and helped formulate our perspective on planetary evolution in our solar system and beyond.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

Bergstralh, J. T., Matson, D. L., & Johnson, T. V. 1975, Astrophys. J. Lett., 196, L131CrossRefGoogle Scholar
Bigg, E. K. 1964, Nature, 203, 1008CrossRefGoogle Scholar
Binder, A. B. & Cruikshank, D. P. 1966, Astrophys. J., 144, 1240CrossRefGoogle Scholar
Brown, R. A. 1974, Exploration of the Planetary System, 65, 527CrossRefGoogle Scholar
Burger, M. H., Schneider, N. M., & Wilson, J. K. 2000, Geophys. Res. Lett., 27, 1081Google Scholar
Goldberg, B. A., Mekler, Y., Carlson, R. W., Johnson, T. V., & Matson, D. L. 1980, Icarus, 44, 305CrossRefGoogle Scholar
Goldberg, B. A., Garneau, G. W., & Lavoie, S. K. 1984, Science, 226, 512Google Scholar
Lellouch, E., Paubert, G., Moses, J. I., Schneider, N. M., & Strobel, D. F. 2003, Nature, 421, 45CrossRefGoogle Scholar
Macy, W. W. Jr. , & Trafton, L. M. 1975, Icarus, 25, 432CrossRefGoogle Scholar
Marois, C., Macintosh, B., Barman, T., Zuckerman, B., Song, I., Patience, J., Lafreniére, D., & Doyon, R. 2008, Science, 322, 1348CrossRefGoogle Scholar
Matson, D. L., Goldberg, B. A., Johnson, T. V., & Carlson, R. W. 1978, Science, 199, 531Google Scholar
Mendillo, M., Baumgardner, J., Flynn, B., & Hughes, W. J. 1990, Nature, 348, 312CrossRefGoogle Scholar
Mendillo, M., Wilson, J., Spencer, J., & Stansberry, J. 2004, Icarus, 170, 430CrossRefGoogle Scholar
Pilcher, C. B., Fertel, J. H., Smyth, W. H., & Combi, M. R. 1984, Astrophys. J., 287, 427Google Scholar
Schneider, N. M. & Bagenal, F. 2007, Io After Galileo: A New View of Jupiter's Volcanic Moon, 265Google Scholar
Schneider, N. M., Wilson, J. K., Trauger, J. T., Brown, D. I., Evans, R. W., & Shemansky, D. E. 1991, Science, 253, 1394Google Scholar
Smyth, W. H. & McElroy, M. B. 1978, Astrophys. J., 226, 336Google Scholar
Thomas, N., Bagenal, F., Hill, T. W., & Wilson, J. K. 2004, Jupiter. The Planet, Satellites and Magnetosphere, 561Google Scholar
Trafton, L., Parkinson, T., Macy, W. Jr, 1995, Astrophys. J. Lett., 190, L85CrossRefGoogle Scholar
Wilson, J. K. & Schneider, N. M. 1994, Icarus, 111, 31Google Scholar
Wilson, J. K. & Schneider, N. M. 1999, J. Geophys. Res., 104, 16567Google Scholar