Study of the Photo gravitational Circular Restricted Three Body Problem

Authors

  • Vikash Kumar  Research Scholar, University Department of Mathematics, B. R. A. Bihar University, Muzaffarpur, Bihar, India
  • Dr. K. B. Singh  P. G. Department of Physics, L. S. College, Muzaffarpur, B. R. A. Bihar University, Muzaffarpur, Bihar, India
  • & Dr. M. N. Haque  P. G. Department of Mathematics, M. S. College, Motihari, B. R. A. Bihar University, Muzaffarpur, Bihar, India

DOI:

https://doi.org//10.32628/IJSRST2215546

Keywords:

RTBP, CRTBP, Three Body Problem.

Abstract

In this chapter we will discuss the equation of motion of Photogravitational Circular Restricted Three Body Problem (in brief -PCR3BP) in which both the primaries are sources of radiation [1]. The three body problem studies the motion of three masses whose gravitational attraction have an effect on each other. The dynamics of the three-body problem are essentially different from those of two bodies, because in the latter case, an analytical solution may be found that admits orbits in the form of conic sections. This problem has been studied at great length and is the basis of most of today’s orbit planning and trajectory design for satellites.

References

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International Journal of Scientific Research in Science and Technology

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Published

2022-12-30

Issue

Volume 9, Issue 6, November-December-2022

Section

Research Articles

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How to Cite

[1]
Vikash Kumar, Dr. K. B. Singh, & Dr. M. N. Haque, " Study of the Photo gravitational Circular Restricted Three Body Problem, International Journal of Scientific Research in Science and Technology(IJSRST), Online ISSN : 2395-602X, Print ISSN : 2395-6011, Volume 9, Issue 6, pp.402-409, November-December-2022. Available at doi : https://doi.org/10.32628/IJSRST2215546