Bifurcations of plane to 3D periodic orbits in the restricted three-body problem with oblateness

被引:4
作者
Perdios, EA [1 ]
Kanavos, SS [1 ]
Markellos, VV [1 ]
机构
[1] Univ Patras, Dept Engn Sci, GR-26110 Patras, Greece
关键词
Periodic Orbit; Numerical Technique; Mass Parameter; Basic Family; Vertical Stability;
D O I
10.1023/A:1001831319656
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider the bifurcation of 3D periodic orbits from the plane of motion of the primaries in the restricted three-body problem with oblateness. The simplest 3D periodic orbits branch-off at the plane periodic orbits of indifferent vertical stability. We describe briefly suitable numerical techniques and apply them to produce the first few such vertical-critical orbits of the basic families of periodic orbits of the problem, for varying mass parameter mu and fixed oblateness coefficent A(1) = 0.005, as well as for varying A(1) and fixed mu = 1/2. The horizontal stability of these orbits is also determined leading to predictions about the stability of the branching 3D orbits.
引用
收藏
页码:75 / 87
页数:13
相关论文
共 9 条
[1]  
Henon M., 1970, Periodic orbits, stability and resonances, P349
[2]  
HENON M, 1973, ASTRON ASTROPHYS, V28, P415
[3]  
HENON M, 1965, ANN ASTROPHYS, V28, P992
[4]  
Markellos V. V., 1981, Investigating the universe, P321
[5]   STABILITY PARAMETERS OF PERIODIC-SOLUTIONS [J].
MARKELLOS, VV .
ASTROPHYSICS AND SPACE SCIENCE, 1976, 43 (02) :449-458
[6]  
ROBIN IA, 1983, DYNAMICAL TRAPPING E, V213
[7]   STATIONARY SOLUTIONS AND THEIR CHARACTERISTIC EXPONENTS IN RESTRICTED 3-BODY PROBLEM WHEN MORE MASSIVE PRIMARY IS AN OBLATE SPHEROID [J].
SHARMA, RK ;
RAO, PVS .
CELESTIAL MECHANICS, 1976, 13 (02) :137-149
[8]  
Szebehely V., 1967, THEORY ORBITS
[9]  
ZAGOURAS C, 1977, ASTRON ASTROPHYS, V59, P79