We consider the problem: given a collinear configuration of n bodies, find
the masses which make it central. We prove that for n less than or equal to
6, each configuration determines a one-parameter family of masses (after n
ormalization of the total mass). The parameter is the center of mass when n
is even and the square of the angular velocity of the corresponding circul
ar periodic orbit when n is odd. The result is expected to be true for any
n.