At that thermal equilibrium the surface temperature can be calculated using the S - B Law for any planet at a given level of solar input. (newclimatemodel.com)
In addition to global mean equilibrium surface temperature changes, local surface temperature changes have been identified by Gillett and Thompson (2003) as a result of ozone loss from the lower stratosphere. (ipcc.ch)
1 1 26 Equilibrium surface temperature less than -100 oC.» (realclimate.org)