The tectonics of Ganymede (original) (raw)

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• Published: 28 January 1982

Nature volume 295, pages 290–293 (1982)Cite this article

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Abstract

The surface of Ganymede, the largest icy jovian satellite, is composed of two distinct terrain types showing abundant evidence of global-scale tectonics. There is geological evidence consistent with the formation of younger bright terrain by the emplacement of relatively clean ice into rift zones developed in the more silicate-rich dark terrain.

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Author notes

1. S. W. Squyres
   Present address: NASA Ames Research Center, Moffett Field, California, 94035, USA
2. M. L. Allison
   Present address: Department of Geology and Geography, University of Massachusetts, Amherst, Massachusetts, 01002, USA

Authors and Affiliations

1. Department of Geological Sciences, Brown University, Providence, Rhode Island, 02912, USA
   E. M. Parmentier, J. W. Head & M. L. Allison
2. Laboratory for Planetary Studies, Cornell University, Ithaca, New York, 14853, USA
   S. W. Squyres

Authors

1. E. M. Parmentier
2. S. W. Squyres
3. J. W. Head
4. M. L. Allison

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Parmentier, E., Squyres, S., Head, J. et al. The tectonics of Ganymede.Nature 295, 290–293 (1982). https://doi.org/10.1038/295290a0

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• Received: 13 July 1981
• Accepted: 17 November 1981
• Issue date: 28 January 1982
• DOI: https://doi.org/10.1038/295290a0

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