Marina Cano Amoros

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O demixing in Uranus and Neptune: Adiabatic structure models

14 citations · 14 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.EP2024★ 14 cited

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

Marina Cano Amoros, Nadine Nettelmann, Nicola Tosi +2

Demixing properties of planetary major constituents influence the interior structure and evolution of planets. Comparing experimental and computational data on the miscibility of h…

astro-ph.EP2024

Atmospheric Helium Abundances in the Giant Planets

N. Nettelmann, M. Cano Amoros, N. Tosi +2

Noble gases are accreted to the giant planets as part of the gas component of the planet-forming disk. While heavier noble gases can separate from the evolution of the hydrogen-ric…

H2​-H2​O demixing in Uranus and Neptune: Adiabatic structure models

Atmospheric Helium Abundances in the Giant Planets

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