ScienceDirect® Home Skip Main Navigation Links
You have guest access to ScienceDirect. Find out more.
 
Home
Browse
My Settings
Alerts
Help
 Quick Search
 Search tips (Opens new window)
    Clear all fields    
 
Font Size: Decrease Font Size  Increase Font Size
 Abstract - selected
Purchase PDF (736 K)

Article Toolbox
 
 
 
Related Articles in ScienceDirect
View More Related Articles
 
View Record in Scopus
 
doi:10.1016/0012-821X(69)90030-2    
How to Cite or Link Using DOI (Opens New Window)

Copyright © 1969 Published by Elsevier B.V.

Shock, reheating, and the gas retention ages of chondrites

Purchase the full-text article



References and further reading may be available for this article. To view references and further reading you must purchase this article.

G.J. Taylor1 and D. Heymann1

1Department of Geology, Rice University, Houston, Texas 77001, USA


Received 3 June 1969. 
Available online 14 October 2002.

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.


 
Home
Browse
My Settings
Alerts
Help
Elsevier.com (Opens new window)
About ScienceDirect  |  Contact Us  |  Information for Advertisers  |  Terms & Conditions  |  Privacy Policy
Copyright © 2008 Elsevier B.V. All rights reserved. ScienceDirect® is a registered trademark of Elsevier B.V.