Skip to main navigation Skip to search Skip to main content

Soils of eagle crater and Meridiani Planum at the opportunity Rover landing site

  • L. A. Soderblom
  • , R. C. Anderson
  • , R. E. Arvidson
  • , J. F. Bell
  • , N. A. Cabrol
  • , W. Calvin
  • , P. R. Christensen
  • , B. C. Clark
  • , T. Economou
  • , B. L. Ehlmann
  • , W. H. Farrand
  • , D. Fike
  • , R. Gellert
  • , T. D. Glotch
  • , M. P. Golombek
  • , R. Greeley
  • , J. P. Grotzinger
  • , K. E. Herkenhoff
  • , D. J. Jerolmack
  • , J. R. Johnson
  • B. Jolliff, C. Klingelhöfer, A. H. Knoll, Z. A. Learner, R. Li, M. C. Malin, S. M. McLennan, H. Y. McSween, D. W. Ming, R. V. Morris, J. W. Rice, L. Richter, R. Rieder, D. Rodionov, C. Schröder, F. P. Seelos IV, J. M. Soderblom, S. W. Squyres, R. Sullivan, W. A. Watters, C. M. Weitz, M. B. Wyatt, A. Yen, J. Zipfel
  • United States Geological Survey
  • Jet Propulsion Laboratory, California Institute of Technology
  • Washington University St. Louis
  • Cornell University
  • National Aeronautics and Space Administration
  • University of Nevada, Reno
  • Arizona State University
  • Lockheed Martin
  • The University of Chicago
  • Space Science Institute
  • Massachusetts Institute of Technology
  • Max Planck Institute for Chemistry
  • Johannes Gutenberg University Mainz
  • Harvard University
  • Ohio State University
  • Malin Space Science Systems
  • Stony Brook University
  • University of Tennessee
  • NASA Johnson Space Center
  • German Aerospace Center
  • Planetary Science Institute

Research output: Contribution to journalArticlepeer-review

139 Scopus citations

Abstract

The soils at the Opportunity site are fine-grained basaltic sands mixed with dust and sulfate-rich outcrop debris. Hematite is concentrated in spherules eroded from the strata. Ongoing saltation exhumes the spherules and their fragments, concentrating them at the surface. Spherules emerge from soils coated, perhaps from subsurface cementation, by salts. Two types of vesicular clasts may represent basaltic sand sources. Eolian ripples, armored by well-sorted hematite-rich grains, pervade Meridiani Planum. The thickness of the soil on the plain is estimated to be about a meter. The flatness and thin cover suggest that the plain may represent the original sedimentary surface.

Original languageEnglish
Pages (from-to)1723-1726
Number of pages4
JournalScience
Volume306
Issue number5702
DOIs
StatePublished - Dec 3 2004

Fingerprint

Dive into the research topics of 'Soils of eagle crater and Meridiani Planum at the opportunity Rover landing site'. Together they form a unique fingerprint.

Cite this