Lazarus dF star
Number of posts : 3337 Registration date : 2008-06-12
| Subject: Ocean heat transport on M-dwarf planets 2nd January 2014, 5:42 am | |
| Hu and Yang (2013) "Role of ocean heat transport in climates of tidally locked exoplanets around M dwarf stars" http://dx.doi.org/10.1073/pnas.1315215111Ocean heat transport modifies the "eyeball" state to a more "lobster" shape, and may push the inner HZ boundary outward by making the runaway greenhouse transition easier. | |
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