Formation of meteorite hydrocarbons from thermal decomposition of siderite (FeCO3)

被引:104
作者
McCollom, TM [1 ]
机构
[1] Woods Hole Oceanog Inst, Woods Hole, MA 02543 USA
基金
美国国家科学基金会;
关键词
D O I
10.1016/S0016-7037(02)00945-6
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Thermal decomposition of siderite has been proposed as a source of magnetite in martian meteorites. Laboratory experiments were conducted to evaluate the possibility that this process might also result in abiotic synthesis of organic compounds. Siderite decomposition in the presence of water vapor at 300degreesC generated a variety of organic products dominated by alkylated and hydroxylated aromatic compounds. The results suggest that formation of magnetite by thermal decomposition of siderite on the precursor rock of the martian meteorite ALH84001 would have been accompanied by formation of organic compounds and may represent a source of extraterrestrial organic matter in the meteorite and on Mars. The results also suggest that thermal decomposition of siderite during metamorphism could account for some of the reduced carbon observed in metasedimentary rocks from the early Earth. Copyright (C) 2003 Elsevier Science Ltd.
引用
收藏
页码:311 / 317
页数:7
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