Radial transport and nebular thermal processing of millimeter-sized solids in the Solar protoplanetary disk inferred from Cr-Ti-O isotope systematics of chondrules

Fukuda, Kohei; Hibiya, Yuki; Kastelle, Craig R.; Suzuki, Katsuhiko; Iizuka, Tsuyoshi; Yamashita, Katsuyuki; Helser, Thomas E.; Kita, Noriko T.

doi:https://doi.org/10.1111/maps.14276

Radial transport and nebular thermal processing of millimeter-sized solids in the Solar protoplanetary disk inferred from Cr-Ti-O isotope systematics of chondrules

Fukuda, Kohei; Hibiya, Yuki; Kastelle, Craig R. et al.

Meteoritics and Planetary Science, 2024, 59(12), 3282-3304

アクセス数:732件（2025-08-14 19:19 集計）

固定URL: https://hdl.handle.net/11094/98411

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タイトル	Radial transport and nebular thermal processing of millimeter-sized solids in the Solar protoplanetary disk inferred from Cr-Ti-O isotope systematics of chondrules
著者	NRID 1000080963462 1000080963462 ORCID 0000-0002-8883-9251 0000-0002-8883-9251 researchmap permalink koheifukuda koheifukuda 著者名 Fukuda, Kohei
	NRID 1000030867536 1000030867536 著者名 Hibiya, Yuki
	著者名 Kastelle, Craig R.
	NRID 1000070251329 1000070251329 著者名 Suzuki, Katsuhiko
	NRID 1000070614569 1000070614569 著者名 Iizuka, Tsuyoshi
	NRID 1000050322201 1000050322201 著者名 Yamashita, Katsuyuki
	著者名 Helser, Thomas E.
	著者名 Kita, Noriko T.
内容	Fukuda K., Hibiya Y., Kastelle C.R., et al. Radial transport and nebular thermal processing of millimeter-sized solids in the Solar protoplanetary disk inferred from Cr-Ti-O isotope systematics of chondrules. Meteoritics and Planetary Science, (2024); https://doi.org/10.1111/maps.14276.
抄録	Understanding the material transport and mixing processes in the Solar protoplanetary disk provides important constraints on the origin of chemical and isotopic diversities of our planets. The limited extent of radial transport and mixing between the inner and outer Solar System has been suggested based on a fundamental isotopic dichotomy between non-carbonaceous (NC) and carbonaceous (CC) meteorite groups. The limited transport and mixing could be further tested by tracing the formation regions of individual meteoritic components, such as Ca-Al-rich inclusions (CAIs) and chondrules. Here, we show further evidence for the outward transport of CAIs and chondrules from the inner and subsequent thermal processing in the outer region of the protoplanetary disk based on the petrography and combined Cr-Ti-O isotope systematics of chondrules from the Vigarano-like (CV) carbonaceous chondrite Allende. One chondrule studied consists of an olivine core that exhibits NC-like Ti and O, but CC-like Cr isotopic signatures, which is enclosed by a pyroxene igneous rim with CC-like O isotope ratios. These observations indicate that the olivine core formed in the inner Solar System. The olivine core then migrated into the outer Solar System and experienced nebular thermal processing that generated the pyroxene igneous rim. The nebular thermal processing would result in Cr isotope exchange between the olivine core and CC-like materials, but secondary alteration effects on the parent body are also responsible for the CC-like Cr isotope signature. By combining previously reported Cr-Ti-O isotope systematics of CV chondrules, we show that some CV chondrules larger than ~1 mm would have formed in the inner Solar System. The accretion of the millimeter-sized, inner Solar System solids onto the CV carbonaceous chondrite parent body would require their very early migration into the outer Solar System within the first 1 million years after the Solar System formation.
出版者	John Wiley and Sons Inc
収録物名	Meteoritics and Planetary Science
巻(号)	59(12)
ページ	3282-3304
刊行年月	2024-10-27
言語	英語
ハンドルURL	https://hdl.handle.net/11094/98411
PISSN	10869379
関連情報 (isIdenticalTo)	DOI (出版社版) https://doi.org/10.1111/maps.14276
アクセス権	open access
権利情報	This article is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.
出版タイプ	Version of Record
カテゴリ	学術雑誌論文 Journal Article

資源タイプ	学術雑誌論文
ローカル資源タイプ	学術雑誌論文
DCTERMS.bibliographicCitation	Meteoritics and Planetary Science. 2024, 59(12), p. 3282-3304
DC.title	Radial transport and nebular thermal processing of millimeter-sized solids in the Solar protoplanetary disk inferred from Cr-Ti-O isotope systematics of chondrules
DC.creator	Fukuda, Kohei
	Hibiya, Yuki
	Kastelle, Craig R.
	Suzuki, Katsuhiko
	Iizuka, Tsuyoshi
	Yamashita, Katsuyuki
	Helser, Thomas E.
	Kita, Noriko T.
DC.publisher	John Wiley and Sons Inc
DC.language' scheme='DCTERMS.RFC1766	英語
DCTERMS.issued' scheme='DCTERMS.W3CDTF	2024-10-27
DC.identifier	https://doi.org/10.1111/maps.14276
DC.description	Fukuda K., Hibiya Y., Kastelle C.R., et al. Radial transport and nebular thermal processing of millimeter-sized solids in the Solar protoplanetary disk inferred from Cr-Ti-O isotope systematics of chondrules. Meteoritics and Planetary Science, (2024); https://doi.org/10.1111/maps.14276.
DCTERMS.abstract	Understanding the material transport and mixing processes in the Solar protoplanetary disk provides important constraints on the origin of chemical and isotopic diversities of our planets. The limited extent of radial transport and mixing between the inner and outer Solar System has been suggested based on a fundamental isotopic dichotomy between non-carbonaceous (NC) and carbonaceous (CC) meteorite groups. The limited transport and mixing could be further tested by tracing the formation regions of individual meteoritic components, such as Ca-Al-rich inclusions (CAIs) and chondrules. Here, we show further evidence for the outward transport of CAIs and chondrules from the inner and subsequent thermal processing in the outer region of the protoplanetary disk based on the petrography and combined Cr-Ti-O isotope systematics of chondrules from the Vigarano-like (CV) carbonaceous chondrite Allende. One chondrule studied consists of an olivine core that exhibits NC-like Ti and O, but CC-like Cr isotopic signatures, which is enclosed by a pyroxene igneous rim with CC-like O isotope ratios. These observations indicate that the olivine core formed in the inner Solar System. The olivine core then migrated into the outer Solar System and experienced nebular thermal processing that generated the pyroxene igneous rim. The nebular thermal processing would result in Cr isotope exchange between the olivine core and CC-like materials, but secondary alteration effects on the parent body are also responsible for the CC-like Cr isotope signature. By combining previously reported Cr-Ti-O isotope systematics of CV chondrules, we show that some CV chondrules larger than ~1 mm would have formed in the inner Solar System. The accretion of the millimeter-sized, inner Solar System solids onto the CV carbonaceous chondrite parent body would require their very early migration into the outer Solar System within the first 1 million years after the Solar System formation.
DC.rights	This article is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.
DC.format	98411
citation_title	Radial transport and nebular thermal processing of millimeter-sized solids in the Solar protoplanetary disk inferred from Cr-Ti-O isotope systematics of chondrules
citation_author	Fukuda, Kohei
	Hibiya, Yuki
	Kastelle, Craig R.
	Suzuki, Katsuhiko
	Iizuka, Tsuyoshi
	Yamashita, Katsuyuki
	Helser, Thomas E.
	Kita, Noriko T.
citation_publisher	John Wiley and Sons Inc
citation_language	英語
citation_date	2024-10-27
citation_journal_title	Meteoritics and Planetary Science
citation_volume	59
citation_issue	12
citation_firstpage	3282
citation_lastpage	3304
citation_doi	https://doi.org/10.1111/maps.14276
citation_public_url	https://hdl.handle.net/11094/98411

Radial transport and nebular thermal processing of millimeter-sized solids in the Solar protoplanetary disk inferred from Cr-Ti-O isotope systematics of chondrules

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