I do believe that the stats aren't to be watched too closely (most of them are still pretty nonsense).
A neat little trick: Planet information is in Wollari's maps:
Obe IV[spoiler]Planet Type: Planet (Temperate)
Density: 4365.43 g/cm³ (almost thousand times as dense as the Earth)
Eccentricity: 0.162 (very circular, still significantly less circular than Earth's 0.01)
Escape Velocity: 14.374 km/s (Earth: 11.1 km/s)
Mass Dust: 1.424e+25 kg (about 2.5 times Earth)
Mass Gas: 1.954e+24 kg
Orbit Period: 1743 days (almost five standard years)
Orbit Radius: 3.241 AU (3.2 times further than Earth - and the Obe star is a hot F6 VI blue dwarf)
Pressure: 8.83 kPa (about the same as Earth's - at 55 km altitude, not breathable)
Radius: 9,200 km (little less than 1.5 times Earth's)
Surface Gravity: 11.228 m/s² (slightly higher than Earth)
Temperature: 299.13 K (slightly higher than Earth - due to thin athmosphere, assume runaway greenhouse effect and/or a very active volcanism/lots of uranium on the crust[/spoiler]
Well. If we run with those, the temperature is warm, likely you could still see live things there, algae and bacteria. I assume there's a whole lot of CO2 in the gas sphere, so a bit like the early Earth, except less light: The sun will not look like our sun, more like (bright?) star. Since it's pretty hot, I assume volcanic activity. Domed or covered farms with artificial athmosphere.
Or, make up your own stats. Specially the amount of heat compared to other stats make no sense, that thing is orbiting well beyond the asteroid belt distance, the sun isn't going to heat it up.