
Two planets (each having mass m) revolve around
a stationary star ( of mass M ) in a circle of radius
r. The two planets are always on opposite side of
the star (i.e. they are diametrically opposite and
always having separation 2r ). The orbital period T of the planets is of the form T= 2 π✓r^3/GM` What is the value of M`
a stationary star ( of mass M ) in a circle of radius
r. The two planets are always on opposite side of
the star (i.e. they are diametrically opposite and
always having separation 2r ). The orbital period




