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Kato, Yukako, Sekine, Toshimori, Kayama, Masahiko, Miyahara, Masaaki, Yamaguchi, Akira (2017) High-pressure polymorphs in Yamato-790729 L6 chondrite and their significance for collisional conditions. Meteoritics & Planetary Science, 52 (12) 2570-2585 doi:10.1111/maps.12957

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Reference TypeJournal (article/letter/editorial)
TitleHigh-pressure polymorphs in Yamato-790729 L6 chondrite and their significance for collisional conditions
JournalMeteoritics & Planetary Science
AuthorsKato, YukakoAuthor
Sekine, ToshimoriAuthor
Kayama, MasahikoAuthor
Miyahara, MasaakiAuthor
Yamaguchi, AkiraAuthor
Year2017 (December)Volume52
Issue12
PublisherWiley
DOIdoi:10.1111/maps.12957Search in ResearchGate
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Mindat Ref. ID334589Long-form Identifiermindat:1:5:334589:8
GUID0
Full ReferenceKato, Yukako, Sekine, Toshimori, Kayama, Masahiko, Miyahara, Masaaki, Yamaguchi, Akira (2017) High-pressure polymorphs in Yamato-790729 L6 chondrite and their significance for collisional conditions. Meteoritics & Planetary Science, 52 (12) 2570-2585 doi:10.1111/maps.12957
Plain TextKato, Yukako, Sekine, Toshimori, Kayama, Masahiko, Miyahara, Masaaki, Yamaguchi, Akira (2017) High-pressure polymorphs in Yamato-790729 L6 chondrite and their significance for collisional conditions. Meteoritics & Planetary Science, 52 (12) 2570-2585 doi:10.1111/maps.12957
In(2017, December) Meteoritics & Planetary Science Vol. 52 (12) Wiley

See Also

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Kato, Y., Sekine, T., Kayama, M., Miyahara, M., & Yamaguchi, A. (2017). High‐pressure polymorphs in Yamato‐790729 L6 chondrite and their significance for collisional conditions. Meteoritics & Planetary Science, 52(12), 2570-2585.
Kayama, Masahiro, Sekine, Toshimori, Tomioka, Naotaka, Nishido, Hirotsugu, Kato, Yukako, Ninagawa, Kiyotaka, Kobayashi, Takamichi, Yamaguchi, Akira (2018) Cathodoluminescence of high-pressure feldspar minerals as a shock barometer. Meteoritics & Planetary Science, 53 (7) 1476-1488 doi:10.1111/maps.13092
Tomioka, Naotaka, Miyahara, Masaaki (2017) High‐pressure minerals in shocked meteorites. Meteoritics & Planetary Science, 52 (9) 2017-2039 doi:10.1111/maps.12902
Kimura, M., Yamaguchi, A., Miyahara, M. (2017) Shock-induced thermal history of an EH3 chondrite, Asuka 10164. Meteoritics & Planetary Science, 52 (1) 24-35 doi:10.1111/maps.12738
Takenouchi, Atsushi, Mikouchi, Takashi, Kobayashi, Takamichi, Sekine, Toshimori, Yamaguchi, Akira, Ono, Haruka (2019) Fine‐structures of planar deformation features in shocked olivine: A comparison between Martian meteorites and experimentally shocked basalts as an indicator for shock pressure. Meteoritics & Planetary Science, 54 (9) 1990-2005 doi:10.1111/maps.13367
Li, Shaolin, Hsu, Weibiao (2018) The nature of the L chondrite parent body's disruption as deduced from high-pressure phases in the Sixiangkou L6 chondrite. Meteoritics & Planetary Science, 53 (10) 2107-2122 doi:10.1111/maps.13110
Ray, Dwijesh, Ghosh, S., Murty, S.V.S. (2017) On the possible origin of troilite-metal nodules in the Katol chondrite (L6-7) Meteoritics & Planetary Science, 52 (1) 72-88 doi:10.1111/maps.12742
Ozawa, Shin, Ohtani, Eiji, Miyahara, Masaaki, Suzuki, Akio, Kimura, Makoto, Ito, Yoshinori (2009) Transformation textures, mechanisms of formation of high-pressure minerals in shock melt veins of L6 chondrites, and pressure-temperature conditions of the shock events. Meteoritics & Planetary Science, 44 (11) 1771-1786 doi:10.1111/j.1945-5100.2009.tb01206.x
Takenouchi, Atsushi, Mikouchi, Takashi, Yamaguchi, Akira (2018) Shock veins and brown olivine in Martian meteorites: Implications for their shock pressure-temperature histories. Meteoritics & Planetary Science, 53 (11) 2259-2284 doi:10.1111/maps.13120
(2017) Meteoritics & Planetary Science, 52 (12) doi:10.1111/maps.2017.52.issue-12
Yamaguchi, Akira, Kimura, Makoto, Barrat, Jean‐Alix, Greenwood, Richard (2019) Compositional diversity of ordinary chondrites inferred from petrology, bulk chemical, and oxygen isotopic compositions of the lowest FeO ordinary chondrite, Yamato 982717. Meteoritics & Planetary Science, 54 (9) 1919-1929 doi:10.1111/maps.13351
 
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