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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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| Publié dans: | Proc Natl Acad Sci U S A |
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| Auteurs principaux: | , , , , , , , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
National Academy of Sciences
2020
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| Sujets: | |
| Accès en ligne: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7519341/ https://ncbi.nlm.nih.gov/pubmed/32900966 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.2005235117 |
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