Observatorio de I+D+i UPM

Descripción
In this paper we present new variables to describe the orbital motion of a celestial body in the Solar System. The motion is the solution of a perturbed two-body problem, where the main perturber can be the Sun or any planet. Two sets of generalized orbital elements are proposed for positive and negative values of the total energy, respectively. The former is the subject of the paper [1], while the latter is here presented for the first time. Numerical tests for perturbed geocentric motion and close encounters with a planet show that the new coordinates are very efficient when compared with both regularized and Cowell?s methods.
Internacional	Si
Nombre congreso	6th International Conference on Astrodynamics Tools and Techniques (ICATT)
Tipo de participación	960
Lugar del congreso	Darmstadt, Alemania
Revisores	No
ISBN o ISSN
DOI
Fecha inicio congreso	14/03/2016
Fecha fin congreso	17/03/2016
Desde la página	1
Hasta la página	9
Título de las actas	Publicación en linea: https://indico.esa.int/indico/event/111/session/30/contribution/111/material/slides/0.pdf

Esta actividad pertenece a memorias de investigación

• Autor: Claudio Bombardelli (UPM)
• Autor: Davide Amato . (UPM)
• Autor: Giulio Baù (Università di Pisa, Pisa, Italia)
• Autor: Andrea Milani (Università di Pisa, Pisa, Italia)

• Creador: Grupo de Investigación: Dinámica Espacial (SDG-UPM)
• Departamento: Física Aplicada a Las Ingenierías Aeronáutica y Naval