Hostname: page-component-cc8bf7c57-llmch Total loading time: 0 Render date: 2024-12-12T05:05:32.607Z Has data issue: false hasContentIssue false

On the Application of Hansen's Method of Partial Anomalies to the Calculation of Perturbations in Cometary Motions

Published online by Cambridge University Press:  14 August 2015

V. I. Skripnichenko*
Affiliation:
Institute for Theoretical Astronomy, Leningrad, U.S.S.R.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The main points of the method of partial anomalies are described. The method makes it possible to obtain analytical solutions for comets moving in orbits with high eccentricities. The method may be applied, in particular, to systems in which the orbits of the disturbed and disturbing bodies have points equidistant from the Sun. The method is applied to the calculation of the general perturbations by Saturn on P/Tuttle.

Type
Part II/General Methods of Orbit Theory
Copyright
Copyright © Reidel 1972 

References

Asten, E.: 1872, Mem. Acad. Imp. Sci. St. Petersb. 18, No. 10.Google Scholar
Brouwer, D. and Clemence, G. M.: 1961, Methods of Celestial Mechanics , Academic Press, New York and London.Google Scholar
Hansen, P. A.: 1856, Suppl. Compt. Rend. Acad. Sci. Paris 1, 121.Google Scholar
Nacozy, P. E: 1969, Astron. J. 74, 544.CrossRefGoogle Scholar
Porter, J. G.: 1961, Mem. Br. Astron. Assoc. 39, No. 3.Google Scholar
Skripnichenko, V. I.: 1970, Byull. Inst. Teor. Astron. 12, 16.Google Scholar