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Accretion timescales and style of asteroidal differentiation in an (26)Al-poor protoplanetary disk
The decay of radioactive (26)Al to (26)Mg (half-life of 730,000 years) is postulated to have been the main energy source promoting asteroidal melting and differentiation in the nascent solar system. High-resolution chronological information provided by the (26)Al−(26)Mg decay system is, therefore, i...
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| Publicat a: | Geochim Cosmochim Acta |
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| Autors principals: | , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
2016
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| Matèries: | |
| Accés en línia: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4950964/ https://ncbi.nlm.nih.gov/pubmed/27445415 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1016/j.gca.2015.10.036 |
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