Ocean heat transport on M-dwarf planets

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Ocean heat transport on M-dwarf planets

Post by Lazarus on 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"

Ocean 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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