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Euler’s Forgotten Equation of the Center

DOI: 10.4236/ahs.2021.101005, PP. 44-52

Keywords: Euler’s Works on Astronomy, Equation of the Center, History of Orbital Calculations, Investigations on Planets’ Orbits, Astronomical Calculations, Keplerian Orbital Mechanics

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Abstract:

In a 1778 publication in Latin, titled Nova Methodvs Motvm Planetarvm Determinandi (New method to determine the motion of planets), Euler derives an equation of the center, which, apparently, has been forgotten. In the present work, the developments that led to Euler’s equation of the center are revisited, and applied to three planets of the Solar System. These are then compared with results obtained from an equation of center that has been proposed, showing good agreement for planets with not so high eccentricities. Nonetheless, Euler’s derivation was not influential, and since then, the resulting equation of the center has been neglected by scholars and by specialized publications alike.

References

[1]  Brower, D., & Clemence, G. M. (1961). Methods of Celestial Mechanics. New York: Academic Press.
[2]  Euler, L. (1778). Nova methodus motum planetarum determinandi. Acta Academiae Scientarum Imperialis Petropolitinae, 1781, 277-302.
[3]  Narrien, J. (1833). An Historical Account of the Origin and Progress of Astronomy. London: Baldwin and Cradock.
[4]  Roy, A. E. (2005). Orbital Motion (4th ed.). Bristol: IOP Publishing Ltd.
https://doi.org/10.1201/9781420056884
[5]  Smart, W. M. (1956). Textbook on Spherical Astronomy. London: Cambridge University Press.

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