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Chondrules reveal large-scale outward transport of inner Solar System materials in the protoplanetary disk

Dynamic models of the protoplanetary disk indicate there should be large-scale material transport in and out of the inner Solar System, but direct evidence for such transport is scarce. Here we show that the ε(50)Ti-ε(54)Cr-Δ(17)O systematics of large individual chondrules, which typically formed 2...

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Detalles Bibliográficos
Autores principales:	Williams, Curtis D., Sanborn, Matthew E., Defouilloy, Céline, Yin, Qing-Zhu, Kita, Noriko T., Ebel, Denton S., Yamakawa, Akane, Yamashita, Katsuyuki
Formato:	Online Artículo Texto
Lenguaje:	English
Publicado:	National Academy of Sciences 2020
Materias:	Physical Sciences
Acceso en línea:	https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7519341/ https://www.ncbi.nlm.nih.gov/pubmed/32900966 http://dx.doi.org/10.1073/pnas.2005235117

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