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Overview of the Mars Pathfinder Mission and assessment of landing site predictions

  • M. P. Golombek
  • , R. A. Cook
  • , T. Economou
  • , W. M. Folkner
  • , A. F.C. Haldemann
  • , P. H. Kallemeyn
  • , J. M. Knudsen
  • , R. M. Manning
  • , H. J. Moore
  • , T. J. Parker
  • , R. Rieder
  • , J. T. Schofield
  • , P. H. Smith
  • , R. M. Vaughan

Research output: Contribution to journalReview articlepeer-review

Abstract

Chemical analyses returned by Mars Pathfinder indicate that some rocks may be high in silica. Implying diffentiated parent materials. Rounded pebbles and cobbles and a possible conglomerate suggest fluvial processes that imply liquid water in equilibrium with the atmospher and thus a warmer and wetter past. The moment of inertia indicates a central metallic core of 1300 to 2000 kilometers in radius. Composite airborne dust particles appear magnetized by freeze-dried maghemite stain or cement that may have been leached from crustal materials by an active hydrologic cycle. Remote-sensing data at a scale of generally greater than ~1 kilometer and an Earth analog correctly predicted a rocky plain safe for landing and roving with a variety of rocks deposited by catastrophic floods that are relatively dust-free.

Original languageEnglish (US)
Pages (from-to)1743-1748
Number of pages6
JournalScience
Volume278
Issue number5344
DOIs
StatePublished - Dec 5 1997

ASJC Scopus subject areas

  • General

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