And it could be again... I wish we would plan ahead and try a solar shield at L1. If we cooled the planet sufficiently, the CO2 would solidify and we could get to work processing it. Venus is far more interesting than the dusty little rock we keep probing. Sure, it may take a millenium, but the sooner we start, the sooner we finish.
Venus has lost almost all of its atmospheric hydrogen. Teraforming a planet like this to sustain life would be quite a challenge. Here's an excerpt from the wikipedia page ( https://en.wikipedia.org/wiki/Terraforming_of_Venus ) Difficulties include the fact that the production of organic molecules from carbon dioxide requires hydrogen, which is very rare on Venus. Because Venus lacks a protective magnetosphere, the u…
Venus has a magnetosphere, although not as strong as Earth's. The problem with Venus' atmosphere, AFAIK, is that the heavier carbon dioxide layer is so thick that reaches the limit of that magnetosphere and in doing so it pushes the lighter molecules like hydrogen or even water to be exposed to the mentioned solar wind. If enough of that atmospheric carbon gets somehow fixated, then the freed oxygen should act as a capture net for all the solar wind's incoming protons and form water molecules (which, being heavier than oxygen, should then sink into lower atmospheric layers).
P.S.: I assumed only "enough" of carbon taken out of the atmosphere, so enough carbon dioxide should be assumed as left there untouched, which now with newly available water molecules should result in bicarbonate, carbonic acid, and other goodies, thus preserve Venus' traditional acidic environment, so no worries there! ;)