Some Special Types of Orbits around Jupiter

This paper intends to show some special types of orbits around Jupiter based on the mean element theory, including stationary orbits, sun-synchronous orbits, orbits at the critical inclination, and repeating ground track orbits. A gravity model concerning only the perturbations of <inline-formula...

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Main Authors: Yongjie Liu, Yu Jiang, Hengnian Li, Hui Zhang
Format: Article
Language:English
Published: MDPI AG 2021-07-01
Series:Aerospace
Subjects:
Online Access:https://www.mdpi.com/2226-4310/8/7/183
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author Yongjie Liu
Yu Jiang
Hengnian Li
Hui Zhang
author_facet Yongjie Liu
Yu Jiang
Hengnian Li
Hui Zhang
author_sort Yongjie Liu
collection DOAJ
description This paper intends to show some special types of orbits around Jupiter based on the mean element theory, including stationary orbits, sun-synchronous orbits, orbits at the critical inclination, and repeating ground track orbits. A gravity model concerning only the perturbations of <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>J</mi><mn>2</mn></msub></mrow></semantics></math></inline-formula> and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>J</mi><mn>4</mn></msub></mrow></semantics></math></inline-formula> terms is used here. Compared with special orbits around the Earth, the orbit dynamics differ greatly: (1) There do not exist longitude drifts on stationary orbits due to non-spherical gravity since only <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>J</mi><mn>2</mn></msub></mrow></semantics></math></inline-formula> and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>J</mi><mn>4</mn></msub></mrow></semantics></math></inline-formula> terms are taken into account in the gravity model. All points on stationary orbits are degenerate equilibrium points. Moreover, the satellite will oscillate in the radial and North-South directions after a sufficiently small perturbation of stationary orbits. (2) The inclinations of sun-synchronous orbits are always bigger than 90 degrees, but smaller than those for satellites around the Earth. (3) The critical inclinations are no-longer independent of the semi-major axis and eccentricity of the orbits. The results show that if the eccentricity is small, the critical inclinations will decrease as the altitudes of orbits increase; if the eccentricity is larger, the critical inclinations will increase as the altitudes of orbits increase. (4) The inclinations of repeating ground track orbits are monotonically increasing rapidly with respect to the altitudes of orbits.
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spelling doaj.art-736d78b0ef1841d2b07acfa9c535ba852023-11-22T02:56:15ZengMDPI AGAerospace2226-43102021-07-018718310.3390/aerospace8070183Some Special Types of Orbits around JupiterYongjie Liu0Yu Jiang1Hengnian Li2Hui Zhang3State Key Laboratory of Astronautic Dynamics, Xi’an Satellite Control Center, Xi’an 710043, ChinaState Key Laboratory of Astronautic Dynamics, Xi’an Satellite Control Center, Xi’an 710043, ChinaState Key Laboratory of Astronautic Dynamics, Xi’an Satellite Control Center, Xi’an 710043, ChinaState Key Laboratory of Astronautic Dynamics, Xi’an Satellite Control Center, Xi’an 710043, ChinaThis paper intends to show some special types of orbits around Jupiter based on the mean element theory, including stationary orbits, sun-synchronous orbits, orbits at the critical inclination, and repeating ground track orbits. A gravity model concerning only the perturbations of <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>J</mi><mn>2</mn></msub></mrow></semantics></math></inline-formula> and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>J</mi><mn>4</mn></msub></mrow></semantics></math></inline-formula> terms is used here. Compared with special orbits around the Earth, the orbit dynamics differ greatly: (1) There do not exist longitude drifts on stationary orbits due to non-spherical gravity since only <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>J</mi><mn>2</mn></msub></mrow></semantics></math></inline-formula> and <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><msub><mi>J</mi><mn>4</mn></msub></mrow></semantics></math></inline-formula> terms are taken into account in the gravity model. All points on stationary orbits are degenerate equilibrium points. Moreover, the satellite will oscillate in the radial and North-South directions after a sufficiently small perturbation of stationary orbits. (2) The inclinations of sun-synchronous orbits are always bigger than 90 degrees, but smaller than those for satellites around the Earth. (3) The critical inclinations are no-longer independent of the semi-major axis and eccentricity of the orbits. The results show that if the eccentricity is small, the critical inclinations will decrease as the altitudes of orbits increase; if the eccentricity is larger, the critical inclinations will increase as the altitudes of orbits increase. (4) The inclinations of repeating ground track orbits are monotonically increasing rapidly with respect to the altitudes of orbits.https://www.mdpi.com/2226-4310/8/7/183mean element theoryorbit dynamicslongitude driftcritical inclinations
spellingShingle Yongjie Liu
Yu Jiang
Hengnian Li
Hui Zhang
Some Special Types of Orbits around Jupiter
Aerospace
mean element theory
orbit dynamics
longitude drift
critical inclinations
title Some Special Types of Orbits around Jupiter
title_full Some Special Types of Orbits around Jupiter
title_fullStr Some Special Types of Orbits around Jupiter
title_full_unstemmed Some Special Types of Orbits around Jupiter
title_short Some Special Types of Orbits around Jupiter
title_sort some special types of orbits around jupiter
topic mean element theory
orbit dynamics
longitude drift
critical inclinations
url https://www.mdpi.com/2226-4310/8/7/183
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AT yujiang somespecialtypesoforbitsaroundjupiter
AT hengnianli somespecialtypesoforbitsaroundjupiter
AT huizhang somespecialtypesoforbitsaroundjupiter