NASA Scientists Explore Venus Habitable Climate Scenarios at NCCS

By Keith Cowing
Press Release
September 1, 2020
Filed under
NASA Scientists Explore Venus Habitable Climate Scenarios at NCCS
Left: This simulation combines imagery from NASA’s Magellan and Pioneer missions and coloration from the Soviet Venera 13 and 14 spacecraft, revealing that Venus is currently a bone-dry planet. Right: Observations suggest that Venus may have had water oceans like these in its distant past, so NASA scientists used a climate model to explore a variety of land-sea and other configurations that could have made the planet habitable. Images by NASA/Jet Propulsion Laboratory-Caltech (left) and NASA (right).

NASA Goddard Institute for Space Studies (GISS) scientists leveraged NASA supercomputing resources for several months to model a hypothetical climate history for Venus over the past 4.2 billion years.

The modeling helped the scientists explore whether the planet had an Earth-like climate for a long period.

The planetary science community agrees that Venus and Earth form as rocky planets with similar geochemical make-ups and large quantities of water. From there, leading theories about Venus’s history diverge onto two distinct paths.

This graph represents Venus’s possible climate history over several billion years (Ga). The three dots mark the 1-bar-surface-pressure atmospheres modeled at those points in time. Figure adapted from M.J. Way and A.D. Del Genio, J. Geophys. Res.

Along path one, Venus initially has an atmosphere of carbon dioxide (CO2) and steam water and a magma ocean that lasts up to 100 million years. With a highly active Sun producing much more X-ray and ultraviolet photons than now, sunlight reaching Venus efficiently splits the steam water molecules into hydrogen (H2) and oxygen (O). Give this process 100 million years, and all the H2 escapes into space and the magma ocean absorbs all the O. Once the magma ocean cools, Venus has an atmosphere with no water left and a dry surface.

Along path two, Venus has the same CO2/steam water atmosphere, but its magma ocean lasts only a few million years. Under this much shorter timeframe most of the steam water gets preserved. When the short-lived magma ocean cools, the atmospheric steam condenses onto Venus’s surface as a liquid water ocean.

The GISS modeling team follows path two. Expanding on previous studies of this theory, the researchers ran 45 different simulations with the ROCKE-3D model–an adaptation of the GISS Model E2 Earth general circulation model.

The GISS Venus model simulated varied topographies (taken from NASA Magellan mission radar maps), land-sea configurations, soil types, surface pressures, atmospheric compositions, amounts of sunlight (insolation), and planet rotation rates. The spatial resolution for all simulations was 1,513 by 1,210 kilometers (940 by 750 miles).

Each simulation ran on 44 computing cores of the NASA Center for Climate Simulation (NCCS) Discover supercomputer. Run-times ranged from a few hours for 8-orbit simulations to 2 months for 3,000-orbit simulations. These simulations collectively covered epochs in Venus’s past, present, and future.

Output data totaling 13 terabytes was initially stored in Discover online disk and then migrated into NCCS mass storage. The researchers used the NCCS DataPortal to help distribute their results.

“NCCS supercomputing resources allowed us to run a wide suite of simulations in a modest amount of time,” said GISS research scientist Michael Way. “We also benefited from their excellent compiler and library support and their ability to keep the supercomputers running efficiently over many contiguous months with few shutdowns. It is a remarkable resource that our group treasures!”

The new GISS simulations showed that, if Venus had liquid surface water early on, then the planet could have had habitable conditions for nearly 3 billion years. The scientists also speculated that Venus could have evolved into its current hothouse state after large-scale resurfacing from volcanic eruptions released enough CO2 to dry up the surface water. Indeed, there is evidence that volcanic activity continues on Venus, as published in a recent study by Swiss Federal Institute of Technology and University of Maryland, College Park researchers.

Way and his colleagues will be exploring both areas in future simulations at NCCS. “We wish to look more closely at the very early evolution of Venus–the first few 100 million years–to better understand if water could condense on the surface or not,” Way said. “We also plan to investigate if it is possible for Venus to go into a runaway greenhouse state, as it is in today, from the clement state we propose.”

This visualization of Simulation 28 shows surface air temperature (Celsius) 2.9 billion years ago for a hypothetical Venus having a nitrogen (N2)-dominated atmosphere with .25-bar surface pressure and an Earth topography with a 310-meter deep ocean. It was the most Earth-like of the 45 simulations, even allowing for the possibility of snow at higher elevations. Figure from M.J. Way and A.D. Del Genio, J. Geophys. Res. Planets.


Way, M.J., and A.D. Del Genio, 2020: Venusian Habitable Climate Scenarios: Modeling Venus Through Time and Applications to Slowly Rotating Venus-Like Exoplanets. J. Geophys. Res. Planets, 125, 5, e2019JE006276, doi:10.1029/2019JE006276.
How Long Was Venus Habitable?,” EOS, 5/8/20.
Model Suggests Toxic Transformation on Venus,” Scientific American, August 2020.


Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻