CaltechAUTHORS
Published January 31, 1992 | Version public
Journal Article Metadata-only

Lunar Impact Basins and Crustal Heterogeneity: New Western Limb and Far Side Data from Galileo

Creators

  • 1. ROR icon NOIRLab
  • 2. ROR icon Brown University
  • 3. ROR icon Arizona State University
  • 4. ROR icon Astrogeology Science Center
  • 5. ROR icon German Aerospace Center
  • 6. ROR icon Jet Propulsion Lab
  • 7. ROR icon Itres (Canada)
  • 8. ROR icon United States Geological Survey
  • 9. ROR icon Planetary Science Institute
  • 10. ROR icon RAND Corporation
  • 11. ROR icon University of Hawaii at Manoa
  • 12. ROR icon Cornell University
  • 13. ROR icon University of Arizona
  • 14. ROR icon California Institute of Technology
  • 15. ROR icon National Aeronautics and Space Administration

Abstract

Multispectral images of the lunar western limb and far side obtained from Galileo reveal the compositional nature of several prominent lunar features and provide new information on lunar evolution. The data reveal that the ejecta from the Orientale impact basin (900 kilometers in diameter) lying outside the Cordillera Mountains was excavated from the crust, not the mantle, and covers pre-Orientale terrain that consisted of both highland materials and relatively large expanses of ancient mare basalts. The inside of the far side South Pole-Aitken basin (>2000 kilometers in diameter) has low albedo, red color, and a relatively high abundance of iron- and magnesium-rich materials. These features suggest that the impact may have penetrated into the deep crust or lunar mantle or that the basin contains ancient mare basalts that were later covered by highlands ejecta.

Additional Information

© 1992 American Association for the Advancement of Science. 30 August 1991; accepted 11 December 1991. We thank the Galileo Project Office, the National Aeronautics and Space Administration, and numerous individuals who participated in the mission planning and initial data analysis for help and support including T. Becker, L. Bolef, H. Breneman, E. Dejong, E. Fischer, L. Gaddis, P. Helfenstein, H. Hoffmann, R. Jaumann, J. Moersch, S. Murchie, J. Oberst, J. Plutchak, M. Robinson, D. Rudy, R. Sullivan, J. Sunshine, L. Wainio, and D. Williams. Helpful comments on earlier drafts of this manuscript were provided by P. Pinet, S. Murchie, J. Sunshine, E. Fischer, and an anonymous reviewer.

Additional details

Identifiers

Eprint ID
38434
DOI
10.1126/science.255.5044.570
Resolver ID
CaltechAUTHORS:20130510-152958369

Related works

Describes
10.1126/science.255.5044.570 (DOI)
http://www.jstor.org/stable/info/2876822 (URL)

Funding

NASA

Dates

Created
2013-05-10
Created from EPrint's datestamp field
Updated
2021-11-09
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Caltech Custom Metadata

Caltech groups
Division of Geological and Planetary Sciences (GPS)