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...

詳細記述

書誌詳細

出版年:	The Planetary Science Journal
主要な著者:	H. W. Horn, V. Prakapenka, S. Chariton, S. Speziale, S.-H. Shim
フォーマット:	論文
言語:	英語
出版事項:	IOP Publishing 2023-01-01
主題:	Planetary science Planet formation Exoplanet evolution Exoplanets Exoplanet formation Planetary interior
オンライン･アクセス:	https://doi.org/10.3847/PSJ/acab03