I have no idea about this thing, but since Mars is on the table, why not Venus? It has comparatively better gravity and a big enough surface. Also, maybe we can harvest its atmosphere and use it elsewhere. I'm not talking about small colonies but terraforming the whole planet. Secondary question: What would be the benefits of Venus over Mars.

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    $\begingroup$ Well there is the length of a Venusian day; which is nearly 117 Earth days. That means almost 60 days of continuous sunlight with twice the intensity of that at Earth's distance from the Sun, then almost 60 days of night cooling down by radiating all that heat into space. So that has to be factored into your definition of a "habitable surface". $\endgroup$
    – uhoh
    Commented Nov 4, 2017 at 9:58
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    $\begingroup$ And I guess there's no way that can be solved. Or is there? $\endgroup$
    – harsh99
    Commented Nov 4, 2017 at 13:15
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    $\begingroup$ 4 billion years ago, Venus had a much thinner atmosphere and temperatures in the range needed for liquid water. The Sun was 30% less bright back then though. $\endgroup$
    – Hobbes
    Commented Nov 5, 2017 at 10:26
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    $\begingroup$ Without an atmosphere, during the day the surface of Venus will be hotter than that of our Moon due to the shorter distance to the Sun and the longer Venusian day. But the difference between night and day temperatures will be higher than that with the Venusian atmosphere. $\endgroup$
    – Uwe
    Commented Nov 5, 2017 at 16:28
  • $\begingroup$ Increasing Venus' Rotation:If we strike Venus (at the right angle) with meteorites or just have these meteorites 'flyby' Venus tuging at the planet, we can increase Venus' rotation. Anton Petrov explains this very well at: youtube.com/watch?v=dNL07o-Wk04&t=440s $\endgroup$
    – johnM
    Commented Oct 29, 2022 at 4:15

4 Answers 4


There's several advantages and disadvantages to Venus compared to Mars terraforming and colonization:


  • Venus's gravity is ~0.9 G which is very similar to Earth's
  • Venus is closer to the earth with less communication lag and more frequent launch windows (around every 600 days instead of 800 days to mars)
  • At high altitudes, temperatures are in manageable ranges (75C-27C)
  • At same high altitudes, air pressures are OK for humans meaning you'd only need a respirator and no pressure suit (but maybe thermal control)
  • The atmosphere is mostly carbon dioxide which could be used for plants Venus Atmosphere


  • Venus's atmosphere contains sulfur dioxide which is bad for humans and plants
  • Venus's atmosphere contains almost no oxygen and water will be hard to come by
  • With current technology the corrosive conditions of the surface can't be survived for very long meaning it would be extremley difficult to transport materials from the surface. This means all materials would have to be brought to the planet. The surface is under extreme pressure, temperature, and chemical conditions. On mars, the surface can easily be mined for resources including water.

Surface of venus The surface of venus


As for terraforming efforts, talking about "harvesting the atmosphere" is so far out of our reach currently that making guesses is borderline fantasy however given "magical future technology" we'd have to worry about a couple things:

  1. Removing toxic chemicals from the atmosphere
  2. Reduce carbon dioxide content and increase nitrogen and oxygen content
  3. Figure out how to cool the planet (shoot hot gas into space?)
  4. Figure out how to keep the planet cool (large orbital mirrors between the sun and venus?
  5. Figure out how to make the surface non-toxic

Basically, you'd need to redo and remove a large part of the atmosphere and then redo the entire surface (or a large part of it) and install some sort of planetary thermal management system.

I think terraforming Mars is much more realistic as you don't have many of the problems that you have with venus:

  1. Raising the temperature of mars will release frozen water which will form an atmosphere. This could be achieved by detonating nukes in the icecaps, pointing large mirrors at mars, or redirecting asteroids with 'good chemistry' to impact mars
  2. Reestablish Mars' magnetic field. This could be done by positioning a bunch of magnet-equipped satellites at good positions between the sun and Mars (some scientists say this is feasible with current technology Mars magnetic shield




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    $\begingroup$ Nice answer! Is "caustic" used correctly here? Perhaps "corrosive" is better? $\endgroup$
    – uhoh
    Commented Nov 19, 2017 at 9:11
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    $\begingroup$ bases are caustic, acids are corrosive. So Sulfuric clouds are corrosive, not caustic. $\endgroup$ Commented Oct 25, 2018 at 3:34

Yes it would.

Currently on the surface the temperature is 467 °C, the air pressure 90 atmosphere, and there is no direct sunlight. 4 billion years ago Venus was like the Earth with liquid water on the surface. A runaway greenhouse effect may have been caused by the evaporation of the surface water and subsequent rise of the levels of other greenhouse gases. Unlike Earth though, Venus lacks a magnetosphere. So what kept the atmosphere from blowing away like that of Mars? It's ionosphere. This separates the atmosphere from outer space and the solar wind. This ionised layer excludes the solar magnetic field, giving Venus a distinct magnetic environment. This is considered Venus's induced magnetosphere. Lighter gases, including water vapour, are continuously blown away by the solar wind through the induced magnetotail.

There is no realistic way to change it's atmosphere though, but there is a way to live on Venus. Balloon like ships that float at about 50km high. Venus city

Despite the harsh conditions on the surface, the atmospheric pressure and temperature at about 50 km to 65 km above the surface of the planet is nearly the same as that of the Earth, making its upper atmosphere the most Earth-like area in the Solar System, even more so than the surface of Mars. Due to the similarity in pressure and temperature and the fact that breathable air (21% oxygen, 78% nitrogen) is a lifting gas on Venus in the same way that helium is a lifting gas on Earth, the upper atmosphere has been proposed as a possible location for both exploration and colonization.


Terraforming either planet "quickly" (within say 1000 years) would require extreme measures massively beyond our present technology or economic capabilities.

For Mars you will need to bring in large amounts of hydrogen, and probably nitrogen, from somewhere else. Ceres might be a promising source for hydrogen (water), Titan might be the best source for nitrogen in the kind of quantities needed. If you can figure out how to ship those to Mars in the kind of vast quantities needed, everything else you need is probably relatively simple. You need to add energy to the system as well, but mirrors or impacts (of your incoming hydrogen and nitrogen) probably do that. Eventually (within the first million years, say) you'll need to deal with preventing the light gasses being lost to space again.

For Venus, you need to get a lot of $CO_2$ out of the atmosphere and cool things down. Simply blocking sunlight from reaching Venus at all (with a really big mirror) will do that in a few centuries. Then you need to bury the $CO_2$ ice under something (one SF writer proposed cracking some of it to $O_2$ and carbon in the form of diamond, and just plating a few meters of diamond over the $CO_2$ ice to hold it down). Then you end up with a nitrogen/oxygen atmosphere. You would probably use more mirrors to get a suitable day-night cycle.

There are much slower, but less "exotic" methods for both planets relying on microorganisms to extract gases from the crust of Mars, or condense carbon and oxygen out of the atmophere of Venus, but they take millenia.


The atmosphere high above in somewhat habitable zones could be harvested, by man, robot, or whatever, but not for some end goal like terraforming, but for a short term goal: experiments, and/or deuterium and or other resource collection. As for usable energy without need for solar panels, Venus has electric field, and turbines could run crazy with all that surface heat. Think of earth, we'd save a lot of desalination energy if the oceans didnt have salt, but we don't go terraforming the ocean to rid it of salt, for example, by blasting salt to space (nevermind that would take much energy). Its about economics today, we simply desalinate. Similarly, Venus would not be to colonize but to mine, much like an asteroid, for the foreseeable future.


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