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Tim Kendall's Extreme Astrophysics

JAXA/Akatsuki imaging of the night-side of Venus

23 Oct 2016, 15:02 UTC
JAXA/Akatsuki imaging of the night-side of Venus
(200 words excerpt, click title or image to see full post)

Image courtesy JAXA. Recent newspaper coverage has drawn attention to the Japanese space mission and results have been published in the Geophysical Research Letters:

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 prograde 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 0.715 Gya. These results demonstrate the role rotation and topography play in understanding the climatic history of Venus-like exoplanets discovered in the present epoch.

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