Doing this calculation a bit more precisely, I used:
Solar constant
WP: 1361 W/m^2
Stefan–Boltzmann constant
WP: 5.670373*10^(-8) W/m^2/K^4
Astronomical unit
WP: 149597870700 m
For a surface at 1 AU whose normal direction points at the Sun, and whose absorption and emission albedos are the same, I find a temperature of 394 K or 121 C.
The Earth does not get nearly that hot, so one has to do the calculation more carefully. Doing the calculation for a sphere, assuming a constant temperature over it, one gets 1/sqrt(2) * the previous number. For the Earth, that is 279 K or 6 C. The Earth's actual average temperature is around 15 C.
For 1.45 AU, the two numbers are 54 C and -42 C. The latter number is about right for Philae's current temperature.