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

被引:196
作者
Golombek, MP
Cook, RA
Economou, T
Folkner, WM
Haldemann, AFC
Kallemeyn, PH
Knudsen, JM
Manning, RM
Moore, HJ
Parker, TJ
Rieder, R
Schofield, JT
Smith, PH
Vaughan, RM
机构
[1] UNIV CHICAGO, ENRICO FERMI INST, CHICAGO, IL 60637 USA
[2] UNIV COPENHAGEN, NIELS BOHR INST, DK-1168 COPENHAGEN, DENMARK
[3] US GEOL SURVEY, ASTROGEOL TEAM, MENLO PK, CA 94025 USA
[4] MAX PLANCK INST CHEM, D-55128 MAINZ, GERMANY
[5] UNIV ARIZONA, LUNAR & PLANETARY LAB, TUCSON, AZ 85721 USA
关键词
D O I
10.1126/science.278.5344.1743
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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 similar to 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.
引用
收藏
页码:1743 / 1748
页数:6
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