Properties of Bessel Function Solution to Kepler’s Equation with Application to Opposition and Conjunction of Earth–Mars

Author:

Ebaid Abdelhalim1,Al-Blowy Ahmed B.2

Affiliation:

1. Faculty of Science, Department of Mathematics, University of Tabuk, P.O. Box 741, Tabuk 71491, Saudi Arabia, E-mail:

2. Faculty of Science, Department of Mathematics , University of Tabuk , P.O. Box 741, Tabuk 71491, Saudi Arabia

Abstract

Abstract In this article, a simple approach is suggested to calculate the approximate dates of opposition and conjunction of Earth and Mars since their opposition on August 28, 2003 (at perihelion of Mars). The goal of this article has been achieved via using accurate analytical solution to Kepler’s equation in terms of Bessel function. The periodicity property of this solution and its particular values at specified times are discussed through some lemmas. The mathematical conditions of opposition and conjunction of the two planets are formulated. Moreover, the intervals of opposition and conjunction have been determined using the graphs of some defined functions. The calculations reveal that there are nine possible oppositions and conjunctions for Earth and Mars during 20 years started on August 28, 2003. The dates of such oppositions and conjunctions were approximately determined and listed in Tables. It is found that our calculations differ few days from the published real dates of Earth–Mars oppositions due to the neglected effects of the gravitational attraction of other planets in the Solar system on the motion of two planets. The period of 20 years can be extended for any number of years by following the suggested analysis. Furthermore, the current approach may be extended to study the opposition and conjunction of the Earth and any outer planet.

Publisher

Walter de Gruyter GmbH

Subject

Physical and Theoretical Chemistry,General Physics and Astronomy,Mathematical Physics

Reference10 articles.

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2. N. I. Ioakimids and K. E. Papadakis, Celest. Mech. Dyn. Astr. 35, 305 (1985).

3. N. M. Swerdlow, J. Hist. Astr. 31, 339 (2000).

4. L. Stumpf, Celest. Mech. Dyn. Astr. 74, 95 (1999).

5. M. Palacios, J. Comput. Appl. Math. 138, 335 (2002).

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