Orateur
Dr
Piotr A. Dybczyński
(Astronomical Observatory Institute, faculty of physics, A.Mickiewicz Univ., Poznań, Poland)
Description
Galactic and stellar perturbations are important factors when studying the
past and future motion of the observed Oort spike comets. Since our
knowledge on the Solar System Galactic environment is continuously
increasing it is necessary to upgrade our methods and computer codes for
taking into account these perturbations in a proper way. I will report our
preparations to incorporate new and hopefully revolutionary data from the
Gaia mission into our dynamical model of the cometary orbit evolution.
Some test results will also be presented.
Auteur principal
Dr
Piotr A. Dybczyński
(Astronomical Observatory Institute, faculty of physics, A.Mickiewicz Univ., Poznań, Poland)
