Abstract
The classical treatment of implied differences on the orbital ellipticelements from the errors involved at an initial epoch is not possible toapply if we consider a long interval of integration, because there is atemporal variation for all the partial derivatives of the elements withrespect to all the variations in the initial ones. We propose asemi-analytical method to compute these partial derivatives by solving a setof initial value problems which are obtained from the planetary Lagrangeequations and their partial derivatives with respect to all the variationsin the initial elements.
Similar content being viewed by others
References
Bretagnon, P. and Francou, G.: 1988, 'Planetary theories in rectangular and spherical variables VSOP87 solutions', Astron. Astrophys. 202, 309–315.
Brouwer D. and Clemence G.: 1961, Methods of Cellestial Mechanics, Academic Press.
Fricke W.: 1982, 'Determination of the Equinox and Equator of the FK5', Astron. Astrophys. 107, 13–16.
I. T. A.: 1991, 'Ephemeris of Minor Planets', Academy of Sciences of the URSS.
Levallois, J. J.: 1969, Géodésie Générale, Vol IV. Éditions Eyrolles.
Simon, J. L.: 1987, 'Calcul des dérivées premières et secondes des équations de Lagrange par analyse harmonique', Astron. Astrophys. 175, 303–308.
Yeomans D. K. et al.: 1990 'Report of the IAU commision', 20 system transition commitee, International Astronomical Union.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Marco, F., Lopez, J. & Martinez, M. Temporal Variations of Perturbed Elliptic Elements: A Semi-Analytical Approach. Celestial Mechanics and Dynamical Astronomy 68, 193–198 (1997). https://doi.org/10.1023/A:1008286427471
Issue Date:
DOI: https://doi.org/10.1023/A:1008286427471