Abstract
It has been shown (Heggie, 1974) that the equations of motion for the three-body problem may be cast into a form which is regular for collisions betweenany pair of bodies. The method proceeds by two stages, namely
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(i)
the introduction of redundant variables
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(ii)
the application of the KS-transformation.
The present contribution gives a different treatment of the first of these stages, and relates the redundant variables to those introduced by Broucke and Lass (1973).
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References
Broucke, R. and Lass, H.: 1973,Celes. Mech. 8, 5–10.
Goldstein, S.: 1950,Classical Mechanics, Addison-Wesley, London.
Heggie, D. C.: 1974,Celes. Mech. 10, 217–241.
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Heggie, D.C. Redundant variables for ‘global’ regularization of the three-body problem. Celestial Mechanics 14, 69–71 (1976). https://doi.org/10.1007/BF01247132
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DOI: https://doi.org/10.1007/BF01247132