Collinear Lagrange Point Solutions in the Circular Restricted Three-Body Problem with Radiation Pressure using Fortran

Details Collinear Lagrange Point Solutions in the Circular Restricted Three-Body Problem with Radiation Pressure using Fortran Collinear Lagrange Point Solutions in the Circular Restricted Three-Body Problem with Radiation Pressure using Fortran

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..394..734s&link_type=abstract

Astronomical Data Analysis Software and Systems ASP Conference Series, Vol. 394, Proceedings of the conference held 23-26 Septem

Astronomy and Astrophysics

Astronomy

Scientific paper

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 r_2 at L_1, L_2 and 1 for r_1 at L_3) and radiation pressure relevant to asteroidal dust particles (β = 0.2), was explored quantitatively.

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