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...
Published in: | Scientific Reports |
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Main Authors: | , , , , , , , , |
Format: | Text |
Language: | English |
Published: |
Nature Publishing Group UK
2021
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Subjects: | |
Online Access: | http://www.ncbi.nlm.nih.gov/pmc/articles/PMC8047023/ https://doi.org/10.1038/s41598-021-87638-5 |