Diamond formation from methane hydrate under the internal conditions of giant icy planets

Hydrocarbon chemistry in the C–O–H system at high pressure and high temperature is important for modelling the internal structure and evolution of giant icy planets, such as Uranus and Neptune, as their interiors are thought to be mainly composed of water and methane. In particular, the formation of...

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Detalles Bibliográficos
Autores principales: Kadobayashi, Hirokazu, Ohnishi, Satoka, Ohfuji, Hiroaki, Yamamoto, Yoshitaka, Muraoka, Michihiro, Yoshida, Suguru, Hirao, Naohisa, Kawaguchi-Imada, Saori, Hirai, Hisako
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2021
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8047023/
https://www.ncbi.nlm.nih.gov/pubmed/33854182
http://dx.doi.org/10.1038/s41598-021-87638-5

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8047023/
https://www.ncbi.nlm.nih.gov/pubmed/33854182
http://dx.doi.org/10.1038/s41598-021-87638-5

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