Taking the parameter b to vary along a monoparametric family of planar
curves, given in the form x = x(lambda, b), y = y(lambda, b) (lambda
being the parameter along each specific curve of the family), we deriv
e two equations to formulate the inverse problem of dynamics and find
all potentials creating, for adequate initial conditions, the given fa
mily. One of these equations offers the total energy on each specific
orbit traced under a known potential, the other equation relates merel
y potentials and orbital data. This later equation lends itself to ser
ies expansion solutions for small values of the parameter b. Two appli
cations to isotach and geometrically similar orbits are discussed as s
pecial cases and two examples are given to demonstrate the efficiency
and the indispensability of the new equations.