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Oxygen Isotopes in AMMS and IDPS: Universality of Oxygen Isotope Systematics Of Crystalline Silicates in Comets

It has been suggested that the major source of crystalline silicates in comets is CR chondrule-like materials along with minor sources including O, R, CH-CB chondrite chondrule-like materials based on the comparisons of oxygen isotope systematics between cometary silicates and chondrules from various types of primitive chondrites [1-3]. However, cometary silicates used for these studies are from only two comets: Wild2 and a parent comet of U2-20GCA. It is uncertain that the oxygen isotope systematics represent that of crystalline silicates in all comets.
Document ID
20210026658
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
D Nakashima
(Tohoku University Sendai, Japan)
S Shimizu
(Tohoku University Sendai, Japan)
R Oike
(Tohoku University Sendai, Japan)
K Fukuda
(University of Wisconsin–Madison Madison, Wisconsin, United States)
M Zhang
(University of Wisconsin–Madison Madison, Wisconsin, United States)
N T Kita
(University of Wisconsin–Madison Madison, Wisconsin, United States)
M E Zolensky
(Johnson Space Center Houston, Texas, United States)
T Nakamura
(Tohoku University Sendai, Japan)
Date Acquired
January 11, 2022
Publication Date
March 7, 2022
Publication Information
Subject Category
Lunar And Planetary Science And Exploration
Meeting Information
Meeting: 54th Lunar and Planetary Science Conference
Location: woodlands tx
Country: US
Start Date: March 6, 2022
End Date: March 12, 2022
Sponsors: Lunar and Planetary Institute
Funding Number(s)
WBS: 191589.04.02.01.06
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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