  The values of the phase integral q were determined for asteroids using (i) a
numerical integration of the brightness phase functions over a wide phase-angle
range and (ii) the relations between q and the G parameter of the HG-function
and q and the G1, G2 parameters of the HG1G2-function. The phase-integral
values for asteroids of different albedo range from 0.34 to 0.54 with an
average value of 0.44. These values can be used for the determination of the
Bond albedo of asteroids. Estimates for the phase-integral values using the G1
and G2 parameters are in very good agreement with the available observational
data. We recommend using the HG1G2-function for the determination of the phase
integral. Comparison of the phase integrals of asteroids and planetary
satellites shows that asteroids have systematically lower values of q.
