Oxygen isotopic compositions of some Yamato meteorites
Oxygen isotopic compositions are reported for eight Yamato meteorites, selected because of unusual compositions or textures. Y-791197 is confirmed to be of lunar origin; Y-74357,Y-75274,and Y-791493 are unusual achondrites possibly related to Lodran; Y-790981 is a slightly weathered ureilite; Y-7901...
Main Authors: | , , |
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Format: | Report |
Language: | English |
Published: |
Enrico Fermi Institute, The University of Chicago
1984
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Subjects: | |
Online Access: | https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=1730 http://id.nii.ac.jp/1291/00001730/ https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=1730&item_no=1&attribute_id=18&file_no=1 |
Summary: | Oxygen isotopic compositions are reported for eight Yamato meteorites, selected because of unusual compositions or textures. Y-791197 is confirmed to be of lunar origin; Y-74357,Y-75274,and Y-791493 are unusual achondrites possibly related to Lodran; Y-790981 is a slightly weathered ureilite; Y-790112 is a member of the Renazzo-class (CR) of the carbonaceous chondrites; Y-75097 is an L6 chondrite containing an achondritic inclusion with H-chondrite isotopic composition; Y-790269 is a badly weathered H-chondrite. |
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