QUOTE (djellison @ May 4 2006, 01:32 PM)
There's an equation to calculate the aparant magnitude ( i.e. those values ) from the absolute magnitude ( the mag of an object at a standard distance ) which we know for the sun.
Time for a shameless plug for my
brightness calculator again: setting albedo, diameter and distances (star to X, viewer from X) will give you, Rem31, a good estimate to the brightness of bodies that are fully lit by the Sun.
To calculate the Sun's brightness at different ranges, Doug's right:
Apparent Magnitude = 2.5*log10(
dist^2) - 26.73
dist is in AU. The figure -26.73 is the Sun's Absolute Magnitude.
Andy (edited the link)