Figure 1 from Habitable Zones around Main-sequence Stars: Dependence on Planetary Mass

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Habitable Zones around Main-sequence Stars: Dependence on Planetary Mass

Authors: Ravi Kumar Kopparapu, Ramses M. Ramirez, James SchottelKotte, James F. Kasting, Shawn Domagal-Goldman, and Vincent Eymet

Kopparapu et al. 2014 The Astrophysical Journal Letters 787 L29.

Provider: AAS Journals

Caption: Figure 1.

Variation in radiative fluxes and planetary albedo as a function of background N₂ partial pressure (panels (a) and (c)) and planetary mass (panels (b) and (d)). The top row is for the inner edge and the bottom row is for the outer edge of the HZ.

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