$H$_{2}$-H$_{2}$O demixing in Uranus and Neptune: Adiabatic structure models$

H$_{2}$-H$_{2}$O demixing in Uranus and Neptune: Adiabatic structure models

Demixing properties of planetary major constituents influence the interior structure and evolution of planets. Comparing experimental and computational data on the miscibility of hydrogen and water to adiabatic profiles suggests phase separation between these components occurs in the ice giants Uran...

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Veröffentlicht in:	arXiv.org 2024-10
Hauptverfasser:	Marina Cano Amoros, Nettelmann, Nadine, Tosi, Nicola, Baumeister, Philipp, Rauer, Heike
Format:	Artikel
Sprache:	eng
Schlagworte:	Adiabatic flow Constituents Demixing Miscibility Neptune Phase diagrams Phase separation Physics - Earth and Planetary Astrophysics Planetary evolution Planetary interiors Rocks Transition pressure Uranus Water Water masses
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H\(_{2}\)-H\(_{2}\)O demixing in Uranus and Neptune: Adiabatic structure models