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...

Full description

Bibliographic Details
Published in:Scientific Reports
Main Authors: Kadobayashi, Hirokazu, Ohnishi, Satoka, Ohfuji, Hiroaki, Yamamoto, Yoshitaka, Muraoka, Michihiro, Yoshida, Suguru, Hirao, Naohisa, Kawaguchi-Imada, Saori, Hirai, Hisako
Format: Text
Language:English
Published: Nature Publishing Group UK 2021
Subjects:
Online Access:http://www.ncbi.nlm.nih.gov/pmc/articles/PMC8047023/
https://doi.org/10.1038/s41598-021-87638-5