Figure 3 from Evolved Climates and Observational Discriminants for the TRAPPIST-1 Planetary System

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Evolved Climates and Observational Discriminants for the TRAPPIST-1 Planetary System

Authors: Andrew P. Lincowski, Victoria S. Meadows, David Crisp, Tyler D. Robinson, Rodrigo Luger, Jacob Lustig-Yaeger, and Giada N. Arney

2018 The Astrophysical Journal 867 76.

Provider: AAS Journals

Caption: Figure 3.

Computed pre-main-sequence evolution of water loss and oxygen production for the TRAPPIST-1 planets assuming inefficient surface sinks. These results represent the maximum build-up of oxygen in the atmosphere. The maximum ocean inventory assumed was 20 Earth oceans, all of which may be lost for planets b, c, and d. Planet h may lose less than one ocean of water.

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