The calculus of apsidal precession frequencies of the planets is developed by means of a perturbation technique. A model of concentric rings (ring model), suitable for improving calculations, is introduced. Conclusive remarks concerning a comparison between the theoretical, the calculated and the observed data of the precession frequencies are performed

Calculation of Apsidal Precession via Perturbation Theory / Barbieri, L.; Talamucci, F.. - In: ADVANCES IN ASTROPHYSICS. - ISSN 2415-6450. - STAMPA. - 4:(2019), pp. 96-109. [10.22606/adap.2019.43003]

Calculation of Apsidal Precession via Perturbation Theory

Talamucci, F.
2019

Abstract

The calculus of apsidal precession frequencies of the planets is developed by means of a perturbation technique. A model of concentric rings (ring model), suitable for improving calculations, is introduced. Conclusive remarks concerning a comparison between the theoretical, the calculated and the observed data of the precession frequencies are performed
2019
4
96
109
Barbieri, L.; Talamucci, F.
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1174925
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