
I'm wondering how one can calculate blackbody temperatures for planets in multiple star systems. I know the BB temperature equation is:
Tb = [278.3 * (L^0.25)]/(D^0.5)
(where L is luminosity in Sols, D is distance in AU). But how do you incorporate the effect of another star at a varying distance in there? It's definitely not just a case of calculating separate Tb's using the L and D of each star and adding the results together. And I don't think it's a case of adding or averaging the L and D values before taking the roots...
Let's say we have a planet orbiting an G2 V star (luminosity: 1 sol) at 1 AU, with a K0V star (luminosity: 0.3 Sols) orbiting the G2V at 5 AU (I think that's stable...). So the K0V companion varies between 4 and 6 AU from the planet. How do I determine by how much the companion raises the BB temperature of the planet?
Any ideas?