| Literature DB >> 28408771 |
M J Way1,2, Anthony D Del Genio1, Nancy Y Kiang1, Linda E Sohl1,3, David H Grinspoon4, Igor Aleinov1,3, Maxwell Kelley1, Thomas Clune5.
Abstract
Present-day Venus is an inhospitable place with surface temperatures approaching 750K 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.Entities:
Year: 2016 PMID: 28408771 PMCID: PMC5385710 DOI: 10.1002/2016GL069790
Source DB: PubMed Journal: Geophys Res Lett ISSN: 0094-8276 Impact factor: 5.576