the closest a fluid body can orbit to its primary without
being pulled apart by tidal forces. A solid body may survive
within the Roche limit if the tidal forces do not exceed its
structural strength. The Roche limit is calculated with the
equation
RL = 2.456*R*(p'/p)^(1/3)
where p' is the density of the planet, p is the density of the
moon, and R is the radius of the planet.