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Abstract <p>Within the framework of the two-body problem with variable masses, the dependencies of the heliocentric distances of planets and its orbital elements on changes in the mass of the Sun are determined. Using the variability of the Sun’s mass as a perturbing factor, differential equations for orbital elements were numerically solved. The results obtained were applied to five planets of the Solar System.</p>

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Dependence of Heliocentric Distances of Planets on Changes in the Mass of the Sun

  • 期刊论文

  • 发表日期：

    2025年12月1日

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  • S. A. Gasanov,
  • A. G. Mammadli,
  • R. T. Mammadov

摘要

Abstract

Within the framework of the two-body problem with variable masses, the dependencies of the heliocentric distances of planets and its orbital elements on changes in the mass of the Sun are determined. Using the variability of the Sun’s mass as a perturbing factor, differential equations for orbital elements were numerically solved. The results obtained were applied to five planets of the Solar System.