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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Detalles Bibliográficos
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.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: National Academy of Sciences 2018
Materias:
Physical Sciences
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

Internet

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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