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 per...
Although Venus is often referred to as the most Earth-like of the terrestrial planets, its runaway ...
A one-dimensional climate model is used to study the response of an Earth-like atmosphere to large i...
International audienceEarth has had oceans for nearly four billion years (1) and Mars had lakes and ...
Present-day Venus is an inhospitable place with surface temperatures approaching 750 K and an atmosp...
Present-day Venus is an inhospitable place with surface temperatures approaching 750K and an atmosph...
Using a modern three-dimensional general circulation coupled atmosphere/ocean model [1] we recently ...
Venus today is inhospitable at the surface, its average temperature of 750 K being incompatible to t...
Little is known about the early evolution of Venus and a potential habitable period during the first...
Little is known about the early evolution of Venus and a potential habitable period during the first...
Planetary rotation rate is a key parameter in determining atmospheric circulation and hence the spat...
International audienceA detailed characterization of the formation and evolution of Venus is a key l...
Venus is in the spotlight of the public and scientific community after the selection of 3 missions: ...
Although Venus is often referred to as the most Earth-like of the terrestrial planets, its runaway ...
A one-dimensional climate model is used to study the response of an Earth-like atmosphere to large i...
International audienceEarth has had oceans for nearly four billion years (1) and Mars had lakes and ...
Present-day Venus is an inhospitable place with surface temperatures approaching 750 K and an atmosp...
Present-day Venus is an inhospitable place with surface temperatures approaching 750K and an atmosph...
Using a modern three-dimensional general circulation coupled atmosphere/ocean model [1] we recently ...
Venus today is inhospitable at the surface, its average temperature of 750 K being incompatible to t...
Little is known about the early evolution of Venus and a potential habitable period during the first...
Little is known about the early evolution of Venus and a potential habitable period during the first...
Planetary rotation rate is a key parameter in determining atmospheric circulation and hence the spat...
International audienceA detailed characterization of the formation and evolution of Venus is a key l...
Venus is in the spotlight of the public and scientific community after the selection of 3 missions: ...
Although Venus is often referred to as the most Earth-like of the terrestrial planets, its runaway ...
A one-dimensional climate model is used to study the response of an Earth-like atmosphere to large i...
International audienceEarth has had oceans for nearly four billion years (1) and Mars had lakes and ...