TY - JOUR
T1 - Petrogenesis of the EET 92023 achondrite and implications for early impact events
AU - Yamaguchi, A.
AU - Shirai, N.
AU - Okamoto, C.
AU - Ebihara, M.
N1 - Funding Information:
We thank NASA/JSC for providing the sample of EET 92023, R. C. Greenwood, and J. A. Barrat for discussions. We also thank the reviewers, J. A. Barrat and S. McKibbin, and the associate editor K. Righter for constructive comments. This research was partly supported by a Grant-in-Aid for Scientific Research from the Ministry of Education, Science, and Technology, Japan, and NIPR, Research Project Funds, KP-6.
Publisher Copyright:
© The Meteoritical Society, 2017.
PY - 2017/4
Y1 - 2017/4
N2 - We report petrology and geochemistry of an achondrite EET 92023 and compare it with normal and anomalous eucrites. EET 92023 is an unbrecciated achondrite and shows a granular texture mainly composed of low-Ca pyroxene and plagioclase, petrologically similar to normal cumulate eucrites such as Moore County. However, this rock contains a significant amount of kamacite and taenite not common in unbrecciated, crystalline eucrites. EET 92023 contains a significant amount of platinum group elements (PGEs) (ca. 10% of CI), several orders of magnitude higher than those of monomict eucrites. We suggest that the metallic phases carrying PGEs were incorporated by a projectile during or before igneous crystallization and thermal metamorphism. The projectile was likely to be an iron meteorite rather than chondritic materials, as indicated by the lack of olivine and the presence of free silica. Therefore, the oxygen isotopic signature is indigenous, rather than due to contamination of the projectile material with different oxygen isotopic compositions. A significant thermal event involving partial melting and metamorphism after the impact event indicates that EET 92023 records early impact events which took place shortly after the crust formation on a differentiated protoplanet when the crust was still hot.
AB - We report petrology and geochemistry of an achondrite EET 92023 and compare it with normal and anomalous eucrites. EET 92023 is an unbrecciated achondrite and shows a granular texture mainly composed of low-Ca pyroxene and plagioclase, petrologically similar to normal cumulate eucrites such as Moore County. However, this rock contains a significant amount of kamacite and taenite not common in unbrecciated, crystalline eucrites. EET 92023 contains a significant amount of platinum group elements (PGEs) (ca. 10% of CI), several orders of magnitude higher than those of monomict eucrites. We suggest that the metallic phases carrying PGEs were incorporated by a projectile during or before igneous crystallization and thermal metamorphism. The projectile was likely to be an iron meteorite rather than chondritic materials, as indicated by the lack of olivine and the presence of free silica. Therefore, the oxygen isotopic signature is indigenous, rather than due to contamination of the projectile material with different oxygen isotopic compositions. A significant thermal event involving partial melting and metamorphism after the impact event indicates that EET 92023 records early impact events which took place shortly after the crust formation on a differentiated protoplanet when the crust was still hot.
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U2 - 10.1111/maps.12821
DO - 10.1111/maps.12821
M3 - Article
AN - SCOPUS:85011003025
SN - 1086-9379
VL - 52
SP - 709
EP - 721
JO - Meteoritics and Planetary Science
JF - Meteoritics and Planetary Science
IS - 4
ER -