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Overview of the Mars Pathfinder mission and assessment of landing site predictionsChemical analyses returned by Mars Pathfinder indicate that some rocks may be high in silica, implying differentiated parent materials. Rounded pebbles and cobbles and a possible conglomerate suggest fluvial processes that imply liquid water in equilibrium with the atmosphere 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 approximately 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.
Document ID
20040172834
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Golombek, M. P.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Cook, R. A.
Economou, T.
Folkner, W. M.
Haldemann, A. F.
Kallemeyn, P. H.
Knudsen, J. M.
Manning, R. M.
Moore, H. J.
Parker, T. J.
Rieder, R.
Schofield, J. T.
Smith, P. H.
Vaughan, R. M.
Date Acquired
August 22, 2013
Publication Date
December 5, 1997
Publication Information
Publication: Science
Volume: 278
Issue: 5344
ISSN: 0036-8075
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Other
Keywords
unmanned
long duration
Mars Pathfinder Project
Flight Experiment

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