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Pressure–temperature evolution of primordial solar system solids during impact-induced compaction
Prior to becoming chondritic meteorites, primordial solids were a poorly consolidated mix of mm-scale igneous inclusions (chondrules) and high-porosity sub-μm dust (matrix). We used high-resolution numerical simulations to track the effect of impact-induced compaction on these materials. Here we sho...
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| Publicado no: | Nat Commun |
|---|---|
| Main Authors: | , , , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Nature Pub. Group
2014
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4268713/ https://ncbi.nlm.nih.gov/pubmed/25465283 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/ncomms6451 |
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