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Periodic Orbits Around the Triangular Points with Prolate Primaries Cover

Periodic Orbits Around the Triangular Points with Prolate Primaries

Artificial Satellites
Volume 58 (2023): Issue 1 (March 2023)
By: Nihad Abd El Motelp and  Mohamed Radwan  
Open Access
|Apr 2023

Figures & Tables

Figure 1.a.

The variation of short-period frequency versus mass parameter μ for different values of the plorate triaxiality
The variation of short-period frequency versus mass parameter μ for different values of the plorate triaxiality

Figure 1.b.

The variation of long-period frequency versus mass parameter μ for different values of the plorate triaxiality parameter
The variation of long-period frequency versus mass parameter μ for different values of the plorate triaxiality parameter

Figure 2.a.

Eccentricity effect on the short-period frequency
Eccentricity effect on the short-period frequency

Figure 2.b.

Eccentricity effect on the long-period frequency
Eccentricity effect on the long-period frequency

Figure 3.a.

The variations of s2 versus mass parameter μ for different values of semi-major axis (a = 0.90, 0.95, 0.99), with fixed values of Aσ = −0.004, Aγ = −0.006, and e = 0.06
The variations of s2 versus mass parameter μ for different values of semi-major axis (a = 0.90, 0.95, 0.99), with fixed values of Aσ = −0.004, Aγ = −0.006, and e = 0.06

Figure 3.b.

The variations of s1 versus the mass parameter μ for different values of the semimajor axis (a = 0.90, 0.95, 0.99), with fixed plorateness triaxiality coefficients Aγ = −0.006, Aσ = −0.004, and e = 0.06
The variations of s1 versus the mass parameter μ for different values of the semimajor axis (a = 0.90, 0.95, 0.99), with fixed plorateness triaxiality coefficients Aγ = −0.006, Aσ = −0.004, and e = 0.06

Figure 4.a.

Comparing the long-period frequency for some selected cases with the classical case
Comparing the long-period frequency for some selected cases with the classical case

Figure 4.b.

Comparing the short-period frequency for some selected cases with the classical case
Comparing the short-period frequency for some selected cases with the classical case

Figure. 5.a.

Comparing the eccentricity of long period motion in the classical with a selected perturbed case.
Comparing the eccentricity of long period motion in the classical with a selected perturbed case.

Figure 5.b.

Comparing the eccentricity of short-period motion in the classical with a selected perturbed case.
Comparing the eccentricity of short-period motion in the classical with a selected perturbed case.
DOI: https://doi.org/10.2478/arsa-2023-0001 | Journal eISSN: 2083-6104 | Journal ISSN: 1509-3859
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Language: English
Page range: 1 - 13
Submitted on: May 17, 2022
Accepted on: Feb 2, 2023
Published on: Apr 15, 2023
Published by: Polish Academy of Sciences, Space Research Centre
In partnership with: Paradigm Publishing Services
Publication frequency: 4 issues per year
Keywords:
restricted three-body problem,
triangular points,
prolate triaxial,
periodic orbits
Related subjects:
Geosciences,
Geosciences, other

© 2023 Nihad Abd El Motelp, Mohamed Radwan, published by Polish Academy of Sciences, Space Research Centre
This work is licensed under the Creative Commons Attribution 4.0 License.

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