Several past calculations of collision probabilities between pairs of
bodies on independent orbits have yielded inconsistent results. We rev
iew the methodologies and identify their various problems. Greenberg's
(1982) collision probability formalism (now with a corrected symmetry
assumption) is equivalent to Wetherill's (1967) approach, except that
it includes a way to avoid singularities near apsides. That method sh
ows that the procedure by Namiki and Binzel (1991) was accurate for th
ose cases where singularities did not arise.