This is a kind of supplementary video for how to consider which gases can phase change and how or why. This is more of a things to know and gleaned from information from the stationpedia and compared to the planet's atmospheric conditions.
We will go over each planet/moon and talk about how the atmosphere affects them, and also if there is anything to take advantage of when pressurizing the atmosphere.
0:00 Intro and Moon (by extension also Mimas)
Moon and Mimas have no atmosphere, the vacuum means they will radiate energy out.
9:53 Mars
composed of a thin atmosphere of CO2, N, O, and Pollutants. It ranges from 20C daytime to -40C Nighttime
16:47 Europa
Composed of a decent atmosphere of O. It ranges from -140C daytime to -150C nighttime. Additional note if you enclose and warm up this cold atmosphere to room temp, you will have 100kpa of atmosphere in your enclosure.
22:50 Vulcan
Very hot, you have an atmosphere of Volatiles, CO2, and Pollutants. It gets to at least 650C daytime and 127C nighttime. This is hot that uninsulated liquid tanks can lead to rapid evaporation and bursting. You can condense the nighttime pollutants to use for cooling.
[Last footage before I wiped this save I was doing the Let's Play on ): ]
33:36 Venus
Quite hot with a thick atmosphere of CO2 and some Pollutants and N. There is no variance in temperature of 460C except during a storm it gets down to 360C where you can condense water. Even so this place is hot and the main challenge is getting cool.