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Applied Mathematics and Nonlinear Sciences
Volumen 2 (2017): Edición 2 (July 2017)
Acceso abierto
Investigation of the effect of albedo and oblateness on the circular restricted four variable bodies problem
Abdullah A. Ansari
Abdullah A. Ansari
| 12 dic 2017
Applied Mathematics and Nonlinear Sciences
Volumen 2 (2017): Edición 2 (July 2017)
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Publicado en línea:
12 dic 2017
Páginas:
529 - 542
Recibido:
09 feb 2017
Aceptado:
12 dic 2017
DOI:
https://doi.org/10.21042/AMNS.2017.2.00044
Palabras clave
Albedo, Oblate body
,
Triangular equilibrium points
,
Stationary Points
,
Poincaré surface of sections
,
Basins of Attraction
© 2017 Abdullah A. Ansari, published by Sciendo
This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 3.0 License.
Fig. 1
Configuration of the problem in CRFVBP with the effect of oblateness and Albedo.
Fig. 2
The locations of lagrangian points during in-plane motion (i.e. ξ≠0, η≠0, ζ = 0) in five cases: (a). Third primary is placed at one of the lagrangian points of the classical circular restricted three-body problem (points with blue color), (b). Variation of masses (points with green color), (c). Solar radiation pressure (points with red color), (d). Albedo effect (points with black color), (e). Oblateness effect (points with magenta color).
Fig. 3
The locations of lagrangian points during out of plane motion (i.e. ξ ≠ 0, η = 0, ζ ≠ 0) in five cases: (a). Third primary is placed at one of the lagrangian points of the classical circular restricted three-body problem (points with blue color), (b). Variation of masses (points with green color), (c). Solar radiation pressure (points with red color), (d). Albedo effect (points with black color), (e). Oblateness effect (points with magenta color).
Fig. 4
The locations of lagrangian points during out of plane motion (i.e.ξ = 0, η ≠ 0, ζ ≠ 0) in five cases: (a). Third primary is placed at one of the lagrangian points of the classical circular restricted three-body problem (points with blue color), (b). Variation of masses (points with green color), (c). Solar radiation pressure (points with red color), (d). Albedo effect (points with black color), (e). Oblateness effect (points with magenta color).
Fig. 5
Poincaré surface of sections for five cases: (a). Third primary is placed at one of the lagrangian points of the classical circular restricted three-body problem (with blue color), (b). Variation of masses (with green color), (c). Solar radiation pressure (with red color), (d). Albedo effect (with black color), (e). Oblateness effect (with magenta color). (i) Poincaré surface of sections in ξ−ξ′-plane, (ii) Poincaré surface of sections in η−η′-plane, (iii) Zoomed part of figure (ii) near the origin.
Fig. 6
(a): The basin of attraction for the case when third primary is placed at one of the lagrangian points of the classical circular restricted three- body problem. (b): Zoomed image of (a) near the lagrangian configuration.
Fig. 7
(a): The basin of attraction for the variable mass case. (b): Zoomed image of (a) near the lagrangian configuration.
Fig. 8
(a): The basin of attraction for the solar radiation pressure case. (b): Zoomed image of (a) near the lagrangian configuration.
Fig. 9
(a): The basin of attraction for the Albedo case. (b): Zoomed image of (a) near the lagrangian configuration.
Fig. 10
(a): The basin of attraction for the oblateness case. (b): Zoomed image of (a) near the lagrangian configuration.
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