Abstract

In the present paper, we are concerned by some investigation on circular restricted three-body problem (CR3BP), where we assume that the primaries have variable masses and variable charges. Among the principal tools used in the present study, we cite the well known Meshcherskii transformation. We have derived the equations of motion and Jacobi integral which differ by variation constant k and charge q from the classical restricted three-body problem. More exactly, in this paper, we have drawn the equilibrium points, the zero-velocity curves, the periodic orbits, the surfaces and the basins of attraction for the different values of charge. We have found one equilibrium point when the charge is q=0.4 and three equilibrium points when its value is q=0.501. We also have drawn the periodic orbits for these two values of charge and found that they are periodic. We have also plotted the zero-velocity surfaces for these two values of charges and found a tremendous variation in these two surfaces. We notice that the Poincaré surfaces of section are shifting away from the origin, when we increase the value of charge. We also got different surfaces for the motion of infinitesimal body, with respect to the variations of charge. The basins of attraction have been drawn for these two values of charge by using Newton-Raphson iterative method. We also noticed that by increasing the values of charge, the basins of attraction are shrinking. For the stability of the equilibrium points that we have studied, we found that, among them, one is stable and three others are unstable.

Highlights

  • Many scientists have been extremely concerned by the study of the restricted three-body problem with diverse perturbations like, forms of the bodies, radiation pressure, variable mass, Pointing-Robertson drag, albedo, charged body, magnetic dipole, resonance and so on.Before the studies of the three-body problem, Jeans in [1] has been concerned by the study of the twobody problem with variable mass and Meshcherskii [2, 3] made some investigations on the mechanics of the bodies with variable mass

  • We have investigated the effect of the variation of charge in the circular restricted three-body problem with primaries having variable masses

  • We have derived the equations of motion and Jacobi integral which differ by variation constant k and charge q from the classical restricted three-body problem

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Summary

Introduction

Many scientists have been extremely concerned by the study of the restricted three-body problem with diverse perturbations like, forms of the bodies, radiation pressure, variable mass, Pointing-Robertson drag, albedo, charged body, magnetic dipole, resonance and so on. The basins of attraction in the restricted n-body problem have been an attractive subject for many other researchers. We have investigated, using Meshcherskii transformation, the circular restricted three-body problem, where the primaries are supposed to have variable masses and variable charges. In the numerical calculation section, we have drawn the equilibrium points, the zero-velocity curves, the periodic orbits, the surfaces for the different values of charge and the basins of attraction. Due to the radiation that they emit, stars have a variable mass and variable charge

Equations of motion
Locations of equilibrium points
Zero-velocity curves
Basins of attraction
Stability
Conclusion
Disclosure statement
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