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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...
Autores principales: | Ishii, Hope A., Bradley, John P., Bechtel, Hans A., Brownlee, Donald E., Bustillo, Karen C., Ciston, James, Cuzzi, Jeffrey N., Floss, Christine, Joswiak, David J. |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
National Academy of Sciences
2018
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6042113/ https://www.ncbi.nlm.nih.gov/pubmed/29891720 http://dx.doi.org/10.1073/pnas.1720167115 |
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