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Unique igneous textures and shock metamorphism of the Northwest Africa 7203 angrite: Implications for crystallization processes and the evolutionary history of the angrite parent body

Cited 1 time in wos
Cited 1 time in scopus

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dc.contributor.authorHayashi, Hideyuki-
dc.contributor.authorMikouchi, Takashi-
dc.contributor.authorKim, Nak Kyu-
dc.contributor.authorPark, Changkun-
dc.contributor.authorSano, Yuji-
dc.contributor.authorTakenouchi, Atsushi-
dc.contributor.authorYamaguchi, Akira-
dc.contributor.authorKagi, Hiroyuki-
dc.contributor.authorBizzarro, Martin-
dc.date.accessioned2022-03-14T06:37:19Z-
dc.date.available2022-03-14T06:37:19Z-
dc.date.issued2022-01-
dc.identifier.urihttps://repository.kopri.re.kr/handle/201206/13263-
dc.description.abstractNorthwest Africa (NWA) 7203 is a quenched angrite, showing mineralogical features typically not present in other quenched angrites. NWA 7203 exhibits textures whose grain size varies from fine grains (<10 mu m) to coarse grains (similar to 3 mm), while other quenched angrites show only single-sized textures. Fine-grained and coarse-grained lithologies have nearly the same bulk compositions. Cooling rates were estimated to be similar to 80 degrees C h(-1) for fine-grained lithologies and similar to 1 degrees C h(-1) for coarse-grained lithologies. Mg-rich olivines (similar to Fo(64)) were found only in fine-grained lithologies. Crystallization of NWA 7203 started in the fine-grained lithologies with Mg-rich olivine grains acting as seeds for crystallization. Coarse-grained lithologies were subsequently formed under conditions of slower cooling. NWA 7203 shows clear shock metamorphic textures unlike other quenched angrites except for NWA 1670. We confirm that the oxygen isotopic ratios of NWA 7203 plot on the angrite fractionation line within uncertainty. However, the obtained Pb-Pb age of NWA 7203 is 4543 +/- 19 Ma, younger than the ages of other quenched angrites, which might be a result of disturbance by shock metamorphism. The finding of shock metamorphism of NWA 7203 suggests that some angrites might be derived from asteroids that remained large (>10 km in diameter) during the late heavy bombardment.en_US
dc.formatapplication/pdf-
dc.languageEnglishen_US
dc.language.isoenen_US
dc.subjectGeochemistry & Geophysicsen_US
dc.subject.classification기타(산소동위원소질량분석기)-
dc.titleUnique igneous textures and shock metamorphism of the Northwest Africa 7203 angrite: Implications for crystallization processes and the evolutionary history of the angrite parent bodyen_US
dc.title.alternative앵그라이트 NWA 7203의 화성 기원 조직과 충격 변성 특성 연구en_US
dc.typeArticleen_US
dc.identifier.bibliographicCitationHayashi, Hideyuki, et al. 2022. "Unique igneous textures and shock metamorphism of the Northwest Africa 7203 angrite: Implications for crystallization processes and the evolutionary history of the angrite parent body". <em>METEORITICS & PLANETARY SCIENCE</em>, 57(1): 105-121.-
dc.citation.titleMETEORITICS & PLANETARY SCIENCEen_US
dc.citation.volume57en_US
dc.citation.number1en_US
dc.identifier.doi10.1111/maps.13776-
dc.citation.startPage105en_US
dc.citation.endPage121en_US
dc.description.articleClassificationSCIE-
dc.description.jcrRateJCR 2020:48.864en_US
dc.subject.keywordMARTIAN METEORITEen_US
dc.subject.keywordPETROLOGYen_US
dc.subject.keywordSAHARA-99555en_US
dc.subject.keywordMINERALOGYen_US
dc.subject.keywordDORBIGNYen_US
dc.subject.keywordORIGINen_US
dc.subject.keywordAGESen_US
dc.identifier.localId2021-0360-
dc.identifier.scopusid2-s2.0-85121574502-
dc.identifier.wosid000733547300001-
Appears in Collections  
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