Oxygen Isotopes in Several Yamato Meteorites

Oxygen isotopic compositions (^<18>O/^<16>O and ^<17>O/^<16>O) of five Yamato meteorites have revealed that Yamato-7303 (m), -74190,-74191,and -7308 (l), -74013 can be classified as L ordinary chondrites and differentiated meteorites, respectively. The former three meteorites...

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Bibliographic Details
Main Authors: Naoki Onuma, Robert N. Clayton, Toshiko K. Mayeda, Keizo Yanai
Format: Report
Language:English
Published: Department of Chemistry, The University of Tsukuba/The Enrico Fermi Institute, The University of Chicago/The Enrico Fermi Institute, The University of Chicago/National Institute of Polar Research 1978
Subjects:
Yamato
Memoirs of National Institute of Polar Research
Polar Research
Online Access:https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=890
http://id.nii.ac.jp/1291/00000890/
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=890&item_no=1&attribute_id=18&file_no=1
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Summary:Oxygen isotopic compositions (^<18>O/^<16>O and ^<17>O/^<16>O) of five Yamato meteorites have revealed that Yamato-7303 (m), -74190,-74191,and -7308 (l), -74013 can be classified as L ordinary chondrites and differentiated meteorites, respectively. The former three meteorites may have been derived from one parent body, and the latter two meteorites are from another parent body in the solar system.

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