Dynamic compression of water to conditions in ice giant interiors

Recent discoveries of water-rich Neptune-like exoplanets require a more detailed understanding of the phase diagram of H(2)O at pressure–temperature conditions relevant to their planetary interiors. The unusual non-dipolar magnetic fields of ice giant planets, produced by convecting liquid ionic wat...

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Detalles Bibliográficos
Autores principales: Gleason, A. E., Rittman, D. R., Bolme, C. A., Galtier, E., Lee, H. J., Granados, E., Ali, S., Lazicki, A., Swift, D., Celliers, P., Militzer, B., Stanley, S., Mao, W. L.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2022
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8758754/
https://www.ncbi.nlm.nih.gov/pubmed/35027608
http://dx.doi.org/10.1038/s41598-021-04687-6

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8758754/
https://www.ncbi.nlm.nih.gov/pubmed/35027608
http://dx.doi.org/10.1038/s41598-021-04687-6

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