Did a Complex Carbon Cycle Operate in the Inner Solar System?

Solids in the interstellar medium consist of an intimate mixture of silicate and carbonaceous grains. Because 99% of silicates in meteorites were reprocessed at high temperatures in the inner regions of the Solar Nebula, we propose that similar levels of heating of carbonaceous materials in the oxyg...

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Detalles Bibliográficos
Autores principales: Nuth, Joseph A., Ferguson, Frank T., Hill, Hugh G. M., Johnson, Natasha M.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2020
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7555641/
https://www.ncbi.nlm.nih.gov/pubmed/32947938
http://dx.doi.org/10.3390/life10090206

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7555641/
https://www.ncbi.nlm.nih.gov/pubmed/32947938
http://dx.doi.org/10.3390/life10090206

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