Comparing the roles of carbon dioxide at Venus, Earth and Mars
Here's a comparison of Venus, Earth and Mars and how they've processed their carbon dioxide inventories.
Earth-Venus-Mars Comparison
Venus is closer to the sun, so it started out hotter, so the greenhouse effect made it hot enough to to evaporate any water it may have had, increasing the greenhouse effect (water vapor is a powerful greenhouse gas) and baking carbon dioxide out of the rocks until it was all in the atmosphere, resulting in a roasting oven. The warming would raise the ceiling in the air at which water vapor turns into ice crystals. Once that ceiling was high enough, water molecules were able to float high enough to where energetic sunlight like ultraviolet rays could break it up, leaving Venus a dry planet blanketed in a hot carbon dioxide atmosphere.
Earth is further away, so the greenhouse effect didn't run away. Liquid water could exist and enable plenty of the carbon dioxide to get dissolved and converted to carbonate rocks like limestone. Water also enables plate tectonics by letting the plates
slide more easily at subduction zones, so the plate tectonics plays its part in
recycling the carbonates with volcanic activity. If Venus had any plate tectonics, it apparently locked up when the water was lost.
Mars is further away than Earth from the sun. Its smaller size made its interior cool down faster, locking up any plate tectonics it had. So the carbon dioxide that got incorporated into rocks when Mars had more water stayed locked up, so there isn't enough greenhouse effect to keep the planet warm.
Here, it says that Mars is colder than Earth would be if we moved Earth out to where Mars is. It's because Mars has only enough carbon dioxide to bump up the temperature by 5K.
Maybe we could engineer Mars someday to rearrange the rocks and atmosphere so we could live there. We might want to when the sun gets hotter as it ages. It's projected to go red giant in 5-7.5 billion years, but it'll be hot enough within a billion years to roast Earth. The extra heat will evaporate sea water, increase the greenhouse effect and bump up the ceiling of ice crystal formation. Once that is high enough, the water will get lost, drying out Earth.
I read the book
this page discusses, so I learned a lot about how the extra heat will roast Earth. Looks like a good idea to try moving to Mars even if it could be hard.