| Literature DB >> 9388167 |
M P Golombek1, R A Cook, T Economou, W M Folkner, A F 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.
Abstract
Chemical 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.Entities:
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Year: 1997 PMID: 9388167 DOI: 10.1126/science.278.5344.1743
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728