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.
      (more)