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STABILITY OF CO2 ATMOSPHERES ON DESICCATED M DWARF EXOPLANETS

  • Authors: Peter Gao, Renyu Hu, Tyler D. Robinson, Cheng Li, and Yuk L. Yung

2015 The Astrophysical Journal 806 249.

  • Provider: AAS Journals

Caption: Figure 1.

The spectra of the Sun (WMO 1985; yellow) and GJ 436 (France et al. 2013; red) scaled such that the total flux of each is identical to the total flux received by Earth at 1 AU (∼1360 W m−2). The wavelengths at which photolysis of CO2, O2, O3, and H2O2 is most efficient are added for comparison (Tian et al. 2014).

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