Add to ORKGThe general perturbations of the asteroids of the Flora group (975" < n < 1150", n - the mean daily motion) due to Jupiter have been automatically computed on an IBM 4341 computer with the Hansen method by manipulating Broucke's Symbolic Poisson Series Processor, and the results have been compared with that computed previously with the Bohlin group method
SIGLEAvailable from British Library Document Supply Centre- DSC:8670.19(RAE-TM-SPACE--384) / BLDSC -...
Series expansion of spherical functions for position perturbation theory of planetary syste
The main aim of this paper is the construction of a set of computational tools in order to improve t...
Published also as Astronomiska iakttagelser och undersökningar, band 10, n:o 1.Thesis (PH.D.)--Unive...
The classical disturbing function R is not suitable to most of the asteroids because in the integrat...
Earth Moon and Planets, 97, pp. 411-434, http://dx.doi.org./10.1007/s11038-006-9113-7International a...
The Hilda group is a collection of asteroids located in the asteroid belt between Mars and Jupiter t...
We present the first results based on the new analytical solution of planetary motion, VSOP2002b (Va...
Some aspects for efficient computation of the tidal perturbation due to the ellipticity effects of t...
In Nº 13 of the Information Bulletin for the Southern Hemisphere I have given an outline of this met...
One of the main problems in celestial mechanics is the construction of analytical theories of planet...
International audienceWe present the first results based on the new analytical solution of planetary...
The dynamical behaviours of spacecrafts moving around uniformly rotating asteroids are investigated ...
The short-periodic perturbations of asteroid elements are calculated by means of the fourth-degree a...
The methods for the computation of the perturbation spectrum of the classical orbit elements present...
SIGLEAvailable from British Library Document Supply Centre- DSC:8670.19(RAE-TM-SPACE--384) / BLDSC -...
Series expansion of spherical functions for position perturbation theory of planetary syste
The main aim of this paper is the construction of a set of computational tools in order to improve t...
Published also as Astronomiska iakttagelser och undersökningar, band 10, n:o 1.Thesis (PH.D.)--Unive...
The classical disturbing function R is not suitable to most of the asteroids because in the integrat...
Earth Moon and Planets, 97, pp. 411-434, http://dx.doi.org./10.1007/s11038-006-9113-7International a...
The Hilda group is a collection of asteroids located in the asteroid belt between Mars and Jupiter t...
We present the first results based on the new analytical solution of planetary motion, VSOP2002b (Va...
Some aspects for efficient computation of the tidal perturbation due to the ellipticity effects of t...
In Nº 13 of the Information Bulletin for the Southern Hemisphere I have given an outline of this met...
One of the main problems in celestial mechanics is the construction of analytical theories of planet...
International audienceWe present the first results based on the new analytical solution of planetary...
The dynamical behaviours of spacecrafts moving around uniformly rotating asteroids are investigated ...
The short-periodic perturbations of asteroid elements are calculated by means of the fourth-degree a...
The methods for the computation of the perturbation spectrum of the classical orbit elements present...
SIGLEAvailable from British Library Document Supply Centre- DSC:8670.19(RAE-TM-SPACE--384) / BLDSC -...
Series expansion of spherical functions for position perturbation theory of planetary syste
The main aim of this paper is the construction of a set of computational tools in order to improve t...