Perturbation Effect of Outer Planet on the Orbits of Minor Planets at Different Orbital Elements
Keywords:
Minor planet, Keplerian orbit, Perturbations, Orbital elementsAbstract
The distribution of a small asteroid 2023 DW minor planet with different eccentricity to the ecliptic plane and with respect to the Jupiter orbit is studied. The variation in orbital elements must be analyzed to effectively study the changes in eccentricity, semi-major axis (SMA), and inclination for the minor planet. The magnitude and direction of these changes depend on the specific conditions, such as the proximity of other bodies and the physical properties of the minor planet. Over time, these forces can significantly alter the orbit, sometimes in predictable ways and sometimes in chaotic or unpredictable patterns.
References
[1] International Astronomical Union, “IAU 2006 General Assembly: Results of the IAU Resolution votes,” Press Release, Aug. 24, 2006. Accessed: May 5, 2008.
[2] International Astronomical Union, “IAU 2006 General Assembly: Resolutions 5 and 6,” Aug. 24, 2006. [Online]. Available: https://www.iau.org
[3] A. L. Berger, “Long-term variations of the Earth’s orbital elements,” Celestial Mechanics, vol. 15, pp. 53–74, 1977.
[4] A. K. Izzet, M. J. Hamwdi, and A. T. Jasim, “Analytical study of Earth tides on low-orbit satellites,” Iraqi Journal of Science, vol. 61, no. 2, pp. 453–461, 2020.
[5] M. J. Hamwdi, “Studying the change in inclination and semi-major axis of satellites for low Earth orbits,” Periodicals of Engineering and Natural Sciences, vol. 9, no. 2, pp. 500–509, Mar. 2021.
[6] D. D. McCarthy, IERS Conventions. Paris, France: Central Bureau of the IERS, Observatoire de Paris, IERS Technical Note No. 21, 1996.
[7] E. M. Standish, “The observational basis for JPL’s DE 200, the planetary ephemerides of the Astronomical Almanac,” Astronomy and Astrophysics, vol. 233, pp. 252–271, 1990.
[8] C. Froeschlé and C. Froeschlé, “Order and chaos in the solar system,” in Proc. 3rd Int. Workshop on Positional Astronomy and Celestial Mechanics, Cuenca, Spain, Oct. 17–21, 1994, pp. 155–171, A. López García et al., Eds. Valencia, Spain: Universitat de València, Observatorio Astronómico, 1996.
[9] C. D. Murray and S. F. Dermott, Solar System Dynamics. Cambridge, U.K.: Cambridge University Press, 1999.
[10] G. Beutler, Methods of Celestial Mechanics, vol. II: Application to Planetary Systems, Geodynamics and Satellite Geodesy. Berlin, Germany: Springer, 2005.
[11] P. K. Seidelmann, Ed., Explanatory Supplement to the Astronomical Almanac. Mill Valley, CA, USA: University Science Books, 1992.
[12] G. Beutler, Methods of Celestial Mechanics, vol. I: Physical, Mathematical, and Numerical Principles. Berlin, Germany: Springer, 2005.
[13] F. R. Moulton, An Introduction to Celestial Mechanics, 2nd rev. ed. New York, NY, USA: Dover Publications, 1970.
[14] N. O. Hasan, W. H. A. Zaki, and A. K. Izzet, “The effect of atmospheric drag force on the elements of low Earth orbital satellites at minimum solar activity,” NeuroQuantology, vol. 19, no. 9, pp. 24–37, Sep. 2021.
[15] D. A. Vallado, Fundamentals of Astrodynamics and Applications, 4th ed. Hawthorne, CA, USA: Microcosm Press, 2013.
Downloads
Published
How to Cite
Issue
Section
License
Copyright (c) 2026 Mayada Jasim Hamwdi Hamwdi

This work is licensed under a Creative Commons Attribution 4.0 International License.