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. 2016 Jun 1;16(6):443–464. doi: 10.1089/ast.2015.1353

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© Aomawa L. Shields, et al., 2016; Published by Mary Ann Liebert, Inc.

This Open Access article is distributed under the terms of the Creative Commons Attribution Noncommercial License (http://creativecommons.org/licenses/by-nc/4.0/) which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and the source are credited.

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FIG. 10. — Surface temperature for a synchronous (left) and Earth-like (24 h) rotation rate for Kepler-62f, after a 65- to 100-year LMD Generic GCM simulation with 1 bar (top) and 3 bar (bottom) of CO₂ in the atmosphere. We assumed e = 0, VEP = 0°, and an obliquity of 0° for all four simulations.