Stability boundaries of clathrate hydrates and thermodynamic conditions of celestial bodies (IMAGE)

Okayama University

Stability boundaries of clathrate hydrates and thermodynamic conditions of celestial bodies

Caption

Dissociation pressures of various clathrate hydrates across a range of cryogenic temperatures. The upper regions of each curve indicate stable boundaries of the clathrate hydrates. (Similar colors have been used to designate the guest species in the dissociation curves of clathrate hydrates and the thermodynamic condition in each celestial body.)

Credit

2021 Hideki Tanaka, Okayama Univ.

Usage Restrictions

None

License

Licensed content

Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.