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Multiple generations of grain aggregation in different environments preceded solar system body formation
The solar system formed from interstellar dust and gas in a molecular cloud. Astronomical observations show that typical interstellar dust consists of amorphous (a-) silicate and organic carbon. Bona fide physical samples for laboratory studies would yield unprecedented insight about solar system fo...
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| Veröffentlicht in: | Proc Natl Acad Sci U S A |
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| Hauptverfasser: | , , , , , , , , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
National Academy of Sciences
2018
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| Schlagworte: | |
| Online Zugang: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6042113/ https://ncbi.nlm.nih.gov/pubmed/29891720 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1720167115 |
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