Given the cumulative distributions of asteroid absolute magnitudes and
geometric albedos, we derive the corresponding cumulative size distri
bution. The inversion problem entails a one-dimensional integral equat
ion whose kernel is not separable from the unknown size distribution.
Assuming the size and geometric albedo to be independent, the size dis
tribution enters the well-known Fredholm integral equation of the firs
t kind. We solve the integral equation analytically for discretely dis
tributed geometric albedos. As an application, we then compute the siz
e distribution of Earth-crossing asteroids assuming the population has
light-scattering properties similar to C- and S-class asteroids. If t
he assumed proportion of brighter asteroids is increased, the total nu
mber of asteroids larger than a given size is decreased. The size dist
ribution is rather insensitive to the geometric albedos assigned to th
e C- and S-class asteroids.