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Binary Asteroids: Secular Perturbations
1992
Symposium - International astronomical union
Preserved Fulltext
The motion of two small bodies orbiting each other whose barycenter is orbiting around a massive body is studied. The equations of motion are integrated considering the secular part of the disturbing function.
doi:10.1017/s0074180900091129
fatcat:ibcw6ui4azaq7j6jmgh7kk6orq