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...

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Bibliographic Details
Main Authors: Robert N. Clayton, Toshiko K. Mayeda, Keizo Yanai
Format: Report
Language:English
Published: Enrico Fermi Institute, The University of Chicago 1984
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
Description
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.