Binary Asteroids: Secular Perturbations

R. Vilhena De Moraes, S. M. G. Winter
1992 Symposium - International astronomical union  
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