Paper:	Collinear Lagrange Point Solutions in the Circular Restricted Three-Body Problem with Radiation Pressure using Fortran
Volume:	394, Astronomical Data Analysis Software and Systems (ADASS) XVII
Page:	734
Authors:	Stenborg, T.N.
Abstract:	The effects of radiation pressure in the circular restricted three-body problem displace the Lagrangian equilibrium points from their classical locations. Components of Newton-Raphson solutions to displaced collinear Lagrange points are presented here. Using Fortran 95, solution convergence for valid approximate zeros (0.07 for r2 at L1, L2 and 1 for r1 at L3) and radiation pressure relevant to asteroidal dust particles (β = 0.2), was explored quantitatively.

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