Rare gas studies of twenty-four antarctic chondrites

The concentrations of rare gases and isotopic compositions of He, Ne and Ar were determined in twenty-four antarctic meteorites by rare gas mass spectrometry. No significant difference is found in cosmic-ray irradiation and thermal histories between antarctic and non-antarctic chondrites, except a d...

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Bibliographic Details
Main Authors: Nobuo Takaoka, Kazuo Saito, Yoshio Ohba, Keisuke Nagao
Format: Report
Language:English
Published: Department of Earth Sciences, Faculty of Science, Yamagata University/Department of Earth Sciences, Faculty of Science, Yamagata University/Department of Earth Sciences, Faculty of Science, Yamagata University/Department of Fundamental Science, Okayama University of Science 1981
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Online Access:https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=1220
http://id.nii.ac.jp/1291/00001220/
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=1220&item_no=1&attribute_id=18&file_no=1
Description
Summary:The concentrations of rare gases and isotopic compositions of He, Ne and Ar were determined in twenty-four antarctic meteorites by rare gas mass spectrometry. No significant difference is found in cosmic-ray irradiation and thermal histories between antarctic and non-antarctic chondrites, except a discovery of extremely long irradiation age of 92 m.y. for the Yamato-74035 (L6) chondrite. The Yamato-75028 chondrite contains high concentrations of solartype rare gases. On the basis of rare gas data, two groups of paired meteorites were identified; they are Yamato-75097,-75102,-75108 and -75271,and Allan Hills-77015,-77167 and -77260.