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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...

Disgrifiad llawn

Wedi'i Gadw mewn:
Manylion Llyfryddiaeth
Cyhoeddwyd yn:Geochim Cosmochim Acta
Prif Awduron: Larsen, K.K., Schiller, M., Bizzarro, M.
Fformat: Artigo
Iaith:Inglês
Cyhoeddwyd: 2016
Pynciau:
Mynediad Ar-lein: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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