Abstract
In this article, we investigated the resonant curves of geo-centric satellite due to the rate of change in earth’s equatorial ellipticity parameter \((\dot{\gamma })\), moon’s angular velocity around the earth \((\dot{\vartheta })\), and angular velocity of bary-center \((\dot{\Theta })\) around the sun. We expressed the equations of the motion of the satellite in a spherical coordinate system using the earth’s potential. The system of equations are reduced into a second-order ordinary differential equation and determined its solution. From the solution, it is noted that resonance appears due to the frequencies \(\dot{\delta _{s0 }}\), \(\dot{\gamma }\), \(\dot{\Theta _0}\) and \(\dot{\vartheta _0}\) at ten resonant points \({\dot{\delta }_{s0}}={2\dot{\gamma }}\), \({\dot{\delta }_{s0}}={\dot{\gamma }}\), \({\dot{\delta }_{s0}}={2\dot{\Theta }_0}\), \({\dot{\delta }_{s0}}={\dot{\Theta }_0}\), \({\dot{\delta }_{s0}}=\frac{{2 \dot{\Theta }_0}}{3}\), \({\dot{\delta }_{s0}}=\frac{\dot{\Theta }_0}{2}\), \({\dot{\delta }_{s0}={2\dot{\vartheta _0}}}\), \({\dot{\delta }_{s0}={\dot{\vartheta _0}}}\), \({\dot{\delta }_{s0}=\frac{{2\dot{\vartheta _0}}}{3}}\), and \({\dot{\delta }_{s0}=\frac{{dot{\vartheta _0}}}{2}}\), where \({\dot{\delta }_{s0}}\), \({\dot{\Theta }_0}\) and \({\dot{\vartheta _0}}\) are the steady-state value of \({\dot{\delta }_{s}}\), \({\dot{\Theta }}\) and \({\dot{\vartheta }}\) respectively. We have drawn the resonant curves corresponding to the resonant points. From the graph, it is observed that the effect of earth’s equatorial ellipticity parameter on the resonant curves are very small. Also, we have shown the effect of eccentricity (e) and semi-major axes (a) on the oscillatory amplitudes \((A_i)\), where \(i=1,2,3\ldots 21\). Finally, we have analyzed the phase portrait by using Poincaré section method when the system is free from forces.
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Abbreviations
- (X, Y, Z):
-
Initial reference coordinate system of the sun and center of sun be its origin (Fig. 1)
- \((X', Y', Z')\) :
-
Initial reference coordinate system of the earth-moon system and the center of mass be its origin (Fig. 1)
- \((X'', Y'', Z'')\) :
-
Initial reference coordinate system of the earth and the center of earth be its origin (Fig. 1)
- (x, y, z):
-
Initial reference coordinate system with origin at the center of the earth and xy-plane in the earth’s equatorial plane (Fig. 1)
- \({{\vec {x}}_1}, \vec {y_1}, \vec {z_1} \) :
-
Unit vectors for the \((X, Y, Z), (X', Y', Z')\) and \((X'', Y'', Z'') \) coordinate systems
- \(a_{r_s}\) :
-
Acceleration component of satellite along the direction \(\vec {r_1}\)
- \(a_{\delta _s}\) :
-
Acceleration component of the satellite along the direction \(\vec {r_2}\)
- \(a_{\varphi _s}\) :
-
Acceleration component of satellite along the direction \(\vec {r_3}\)
- \(a_x, a_y, a_z\) :
-
Direction cosines of \(\vec {r_1}\)
- \(b_x, b_y, b_z\) :
-
Direction cosines of \(\vec {r_2}\)
- \(c_x, c_y, c_z\) :
-
Direction cosines of \(\vec {r}_3\)
- \(\vec {F}_{EM}\) :
-
Earth’s gravitational force on the moon
- \(\vec {F}_{SM}\) :
-
Sun’s gravitational force on the moon
- \(\vec {F}_{SE}\) :
-
Sun’s gravitational force on the earth
- \(\vec {F}_{ME}\) :
-
Moon’s gravitational force on the earth
- \(\vec {F}_{Ss}\) :
-
Sun’s gravitational force on the satellite
- \(\vec {F}_{Es}\) :
-
Earth’s gravitational force on the satellite
- \(\vec {F}_{Ms}\) :
-
Moon’s gravitational force on the satellite
- \(m_s\) :
-
Satellite’s mass
- \(M_M\) :
-
\(7.3476\times 10^{22}\) kg: Moon’s mass
- \(M_E\) :
-
\(5.972\times 10^{24}\) kg: Earth’s mass
- \(M_S\) :
-
\(1.989\times 10^{30}\) kg: Sun’s mass
- \(R_E\) :
-
6371 km: Earth’s radius
- \(R_S\) :
-
696340 km: Sun’s radius
- \(R_M\) :
-
1737.4 km: Moon’s radius
- \(g_E\) = \(9.8 \mathrm{{m/s}}^2\) :
-
Gravitational acceleration on the earth’s surface
- \(g_{S}\) = \(274 \mathrm{{m/s}}^2\) :
-
Gravitational acceleration on the sun’s surface
- \(g_M\) = \(1.62 \mathrm{{m/s}}^2\) :
-
Gravitational acceleration on the moon’s surface
- \(J_2\) = \(+1.08219\times 10^{-3}\) :
-
Earth’s oblateness coefficient
- \(J^{(2)}_2\) = \(-5.35\times 10^{-6}\) :
-
Earth’s equatorial ellipticity coefficient
- \(\gamma =\delta _s-\delta _E\) :
-
Earth’s equatorial ellipticity parameter
- \(\varphi _s\) :
-
Satellite’s latitude
- \(\delta _s\) :
-
Satellite’s longitude
- \(\vec {r_1}\), \(\vec {r_2}\), \(\vec {r}_3\) :
-
Unit vectors along the direction \(r_s, \delta _{s}\), and \(\varphi _s\)
- \(\vec {\rho _{Ss}}\) :
-
Be a vector from center of sun to the satellite
- \(\vec {\rho _{Ms}}\) :
-
Be a vector from center of moon to the satellite
- \(\vec {r_{SE}}\) :
-
Be a vector from center of sun to the center of earth
- \(\vec {r_{ME}}\) :
-
Be a vector from center of moon to center of the earth
- U :
-
Earth’s potential
- \(\Theta \) :
-
Angle between vector \(\vec {R}\) and \(\vec {x_1}\)
- \(\dot{\Theta }\) :
-
0.01720 rad/solar day = angular velocity of the earth-moon system around the sun
- \(\dot{\Theta _0}\) :
-
Steady-state value of \(\dot{\Theta }\)
- \(\delta _{s0}\) :
-
Steady-state value of \(\delta _s\)
- \(\delta _E\) :
-
Angular position of the minor axis of the earth’s equatorial section
- \(\dot{\delta }_E\) :
-
6.3004 rad/solar day = angular velocity of of earth
- \(\lambda \) :
-
\(23^027'\) = inclination angle of the equatorial plane to the plane of the ecliptic
- \(\mu \) :
-
Mass ratio of the earth-moon system
- \(\vartheta \) :
-
Angle between the vector \(-\vec {r_{ME}}\) and \(\vec {x_1}\)
- \(\dot{\vartheta }\) :
-
0.22998 rad/solar day = angular velocity of moon around the earth
- \(\dot{\vartheta _0}\) :
-
Steady-state value of \(\dot{\vartheta }\)
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We are thankful to the Center for Fundamental Research in Space Dynamic and Celestial Mechanics (CFRSC) for providing all facilities for this research work.
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Yadav, S., Kumar, V. & Aggarwal, R. Effect of Earth’s Equatorial Ellipticity on the Resonant Curve and Phase Portrait of Geo-centric Satellite Under the Gravitational Effect of the Earth–Moon–Sun System by Using Unperturbed Solution. Few-Body Syst 63, 41 (2022). https://doi.org/10.1007/s00601-022-01744-2
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DOI: https://doi.org/10.1007/s00601-022-01744-2