A low temperature transfer of ALH84001 from Mars to Earth

被引:172
作者
Weiss, BP [1 ]
Kirschvink, JL
Baudenbacher, FJ
Vali, H
Peters, NT
Macdonald, FA
Wikswo, JP
机构
[1] CALTECH, Div Geol & Planetary Sci 17025, Pasadena, CA 91125 USA
[2] Vanderbilt Univ, Dept Phys & Astron, Stevenson Ctr 6301, Nashville, TN 37235 USA
[3] McGill Univ, Ctr Electron Microscopy, Dept Anat & Cell Biol, Montreal, PQ H3A 2B2, Canada
[4] McGill Univ, Dept Earth & Planetary Sci, Montreal, PQ H3A 2B2, Canada
关键词
D O I
10.1126/science.290.5492.791
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
The ejection of material from Mars is thought to be caused by Large impacts that would heat much of the ejecta to high temperatures. Images of the magnetic field of martian meteorite ALH84001 reveal a spatially heterogeneous pattern of magnetization associated with fractures and rock fragments. Heating the meteorite to 40 degreesC reduces the intensity of some magnetic features, indicating that the interior of the rock has not been above this temperature since before its ejection from the surface of Mars. Because this temperature cannot sterilize most bacteria or eukarya, these data support the hypothesis that meteorites could transfer Life between planets in the solar system.
引用
收藏
页码:791 / 795
页数:5
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