The runaway greenhouse threshold of an Earth-sized planet varies with surface water distribution from about 130% to 180% of Earth's insolation, so the inner edge of the habitable zone depends on the planet's ocean coverage.
This GCM was developed for the modeling of the present Earth’s climate [Numaguchi, 1999] and was applied to the paleoclimate of Earth [Abe-Ouchi et al., 2013]
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Inner Edge of Habitable Zones for Earth-sized Planets with Various Surface Water Distributions
The runaway greenhouse threshold of an Earth-sized planet varies with surface water distribution from about 130% to 180% of Earth's insolation, so the inner edge of the habitable zone depends on the planet's ocean coverage.