LagrangePointsL1ToL5:

Path: SC/Ephem

% Computes the position of Lagrange points in normalized rotating  
   coordinates with the origin at the joint center-of-mass.
   For a demo of the Earth Moon system type LagrangePointsL1ToL5
--------------------------------------------------------------------------
   Form:
   p = LagrangePointsL1ToL5( mu )
--------------------------------------------------------------------------

   ------
   Inputs
   ------
   mu             (1,1)  Ratio of smaller mass to total mass

   -------
   Outputs
   -------
   p              (2,5)  [L1, L2, L3, L4, L5]

--------------------------------------------------------------------------
   Reference: Szebehely, V., "Theory of Orbits", Academic Press, 1967, 
              pp. 134-138.
--------------------------------------------------------------------------

Back to the SC Module page