THE BREAKUP OF A METEORITE PARENT BODY AND THE DELIVERY OF METEORITES TO EARTH

被引:25
作者
BENOIT, PH
SEARS, DWG
机构
[1] Cosmochemistry Group, Department of Chemistry and Biochemistry, University of Arkansas, Fayetteville
关键词
D O I
10.1126/science.255.5052.1685
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
Whether many of the 10,000 meteorites collected in the Antarctic are unlike those falling elsewhere is contentious. The Antarctic H chondrites, one of the major classes of stony meteorites, include a number of individuals with higher induced thermoluminescence peak temperatures than observed among non-Antarctic H chondrites. The proportion of such individuals decreases with the mean terrestrial age of the meteorites at the various ice fields. These H chondrites have cosmic-ray exposure ages of about 8 million years, experienced little cosmic-ray shielding, and suffered rapid postmetamorphic cooling. Breakup of the H chondrite parent body, 8 million years ago, may have produced two types of material with different size distributions and thermal histories. The smaller objects reached Earth more rapidly through more rapid orbital evolution.
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页码:1685 / 1687
页数:3
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