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Thin H2-dominated Atmospheres as Signposts of Magmatic Outgassing on Tidally Heated Terrestrial Exoplanets

  • Authors: Rahul Arora, Sukrit Ranjan, Pranabendu Moitra, Ananya Mallik

Rahul Arora et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 8.

Colored curves show the equilibrium surface pressure from the outgassing–escape balance as a function of mantle redox state (ΔFMQ) for four ﹩{m}_{{{\rm{H}}}_{2}{\rm{O}}}﹩ (10.00%, 1.29%, 0.46%, 0.06%). Solid lines correspond to L 98-59,d; dashed lines correspond to TRAPPIST-1,f. The yellow box highlights the observationally relevant regime bounded below by 0.1 bar (detectability threshold for a visible atmosphere; J. De Wit & S. Seager 2013) and above by P100Myr. Here we fixed ﹩{\chi }_{{{\rm{CO}}}_{2}}﹩ = 600 ppm and χS = 1000 ppm using MORB volatile inventory (F. Gaillard & B. Scaillet 2014).

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