Serbian Astronomical Journal 2022 Issue 204, Pages: 51-63
https://doi.org/10.2298/SAJ2204051F
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Mercury and orbfit packages for numerical integration of planetary systems: implementation of the yarkovsky and yorp effects
Fenucci Marco (Department of Astronomy, Faculty of Mathematics, University of Belgrade, Belgrade, Serbia), marco_fenucci@matf.bg.ac.rs
Novaković Bojan (Department of Astronomy, Faculty of Mathematics, University of Belgrade, Belgrade, Serbia), bojan@matf.bg.ac.rs
For studies of the long-term evolution of small Solar System objects, it is
fundamental to add the Yarkovsky and Yarkovsky-O'Keefe-Radzievskii-Paddack
(YORP) effects in the dynamical model. Still, implementations of these
effects in publicly available N-body codes is either lacking, or the effects
are implemented using significantly simplified models. In this paper, we
present an implementation of the coupled Yarkovsky/YORP effects in the
mercury and orbfit N-body codes. Along with these two effects, we also
included the effects of non-destructive collisions and rotationally induced
breakups to model the asteroid spin state properly. Given the stochastic
nature of many incorporated effects, the software is suitable for
statistical dynamical studies. Here we primarily explained the scientific
aspect of the implementation, while technical details will be made freely
available along with the source codes.
Keywords: Minor planets, asteroids: general, Celestial mechanics, Planets and satellites: Dynamical evolution and stability
Project of the Serbian Ministry of Education, Science and Technological Development, Grant no. 451-03-68/2022-14/200104
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