Oscillatory motions for the restricted planar circular three body problem
Oscillatory motions for the restricted planar circular three body problem
复制标题
DOI:
10.1007/s00222-015-0591-y
复制
发表时间:
2012-07
影响因子:
3.1
通讯作者:
M. Guardia;Pau Martín;T. M. Seara
中科院分区:
文献类型:
--
作者:
M. Guardia;Pau Martín;T. M. Seara
The restricted planar elliptic three body problem models the motion of a massless body under the Newtonian gravitational force of the two other bodies, the primaries, which evolve in Keplerian ellipses. A trajectory is called oscillatory if it leaves every bounded region but returns infinitely often to some fixed bounded region. We prove the existence of such type of trajectories for any values for the masses of the primaries provided they make almost circular orbits.