Copyright © 1969 Published by Elsevier B.V.
Shock, reheating, and the gas retention ages of chondrites
Received 3 June 1969.
Abstract
In order to investigate shock and reheating effects in ordinary chondrites, 71 bronzite, 26 hypersthene and 6 amphoterite chondrites were examined by X-ray diffraction and 39 bronzite and 19 hypersthene chondrites were studied metallographically. In addition, the inert gas contents of 11 bronzites and 4 hypersthene chondrites were measured mass spectrometrically. We have found that virtually all chondrites with short gas retention ages (<2 b.y.) are substantially shocked and reheated, whereas those with ages >3 b.y. are not reheated to any appreciable extent, although they may be strongly shocked. We have concluded that the reheating observed in chondrites is generally related to shock and that these shock-induced reheating events took place before chondrites were ejected from their parent objects.






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- 60 Myr) can be solved by the hypothesis that kilometer-sized fragments of the parent asteroid were deflected by Mars into Earth-crossing orbits on a tume scale of ≈ 109 yr. Chondrites spalled off from such fragments by secondary collisions have lifetimes against planetary capture of 106–107 yr. The destruction lifetime of chondrites in the asteroid belt can be increased from 107 to ≈ 108 yr with a 10-fold reduction on the cross-section requirement.



