Satellites of Mars: geologic history

P. Thomas, J. Veverka, James Bell, J. Lunine, D. Cruikshank

Research output: Chapter in Book/Report/Conference proceedingChapter

30 Scopus citations

Abstract

The small, irregularly shaped satellites of Mars, Phobos and Deimos, provide the most detailed view of the geomorphic forms and processes important on small solar system bodies. The satellites appear to be very similar in composition, strongly resembling carbonaceous asteroids; however, recent groundbased spectra suggest that their surfaces have little bound or interlayer water. Despite their similar compositions, sizes and environments, Phobos and Deimos have radically different surface features. Phobos is densely covered by craters that are nearly lunar in appearance; Deimos' craters are subdued and largely filled in by debris. Phobos shows only local downslope movement of regolith; Deimos has it on a global scale. -from Authors

Original languageEnglish (US)
Title of host publicationMars
EditorsH.H. Kieffer
PublisherUniversity of Arizona Press, Space Science Series
Pages1257-1282
Number of pages26
StatePublished - 1992
Externally publishedYes

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ASJC Scopus subject areas

  • Earth and Planetary Sciences(all)
  • Environmental Science(all)

Cite this

Thomas, P., Veverka, J., Bell, J., Lunine, J., & Cruikshank, D. (1992). Satellites of Mars: geologic history. In H. H. Kieffer (Ed.), Mars (pp. 1257-1282). University of Arizona Press, Space Science Series.