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

Internet

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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