Present-day Venus is an inhospitable place with surface temperatures 
approaching 750 K and an atmosphere 90 times as thick as Earth's. 
Billions of years ago the picture may have been very different. We have 
created a suite of 3-D climate simulations using topographic data from 
the Magellan mission, solar spectral irradiance estimates for 2.9 and 
0.715 Gya, present-day Venus orbital parameters, an ocean volume 
consistent with current theory, and an atmospheric composition estimated
 for early Venus. Using these parameters we find that such a world could
 have had moderate temperatures if Venus had a rotation period slower 
than ~16 Earth days, despite an incident solar flux 46 − 70% higher than
 Earth receives. At its current rotation period, Venus's climate could 
have remained habitable until at least 715 million years ago. These 
results demonstrate the role rotation and topography play in 
understanding the climatic history of Venus-like exoplanets discovered 
in the present epoch.
https://doi.org/10.1002/2016GL069790
https://doi.org/10.1002/2016GL069790
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