Reaction between Hydrogen and Ferrous/Ferric Oxides at High Pressures and High Temperatures—Implications for Sub-Neptunes and Super-Earths

Sub-Neptune exoplanets may have thick hydrogen envelopes and therefore develop a high-pressure interface between hydrogen and the underlying silicates/metals. Some sub-Neptunes may convert to super-Earths via massive gas loss. If hydrogen chemically reacts with oxides and metals at high pressures an...

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Principais autores:	H. W. Horn, V. Prakapenka, S. Chariton, S. Speziale, S.-H. Shim
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2023-01-01
coleção:	The Planetary Science Journal
Assuntos:	Planetary science Planet formation Exoplanet evolution Exoplanets Exoplanet formation Planetary interior
Acesso em linha:	https://doi.org/10.3847/PSJ/acab03
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