Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...428..247d&link_type=abstract
Astronomy and Astrophysics, v.428, p.247-253 (2004)
Astronomy and Astrophysics
Astrophysics
3
Comets: General, Oort Cloud, Planets And Satellites: General
Scientific paper
In long-term Monte Carlo simulations of the dynamics of the Oort cloud planetary perturbations cannot be taken directly into account. To do this we propose a simple approximation: estimating the Solar System transparency coefficient P measuring the probability for a comet to be removed from the cloud by planetary perturbations during a single perihelion passage. We estimated the value of this coefficient from the observed and artificial cometary samples. We excluded nongravitational forces fom our calculations. We obtained P≅0.25 for inner cloud comets and P≅0.5 for the outer and most active part of the cloud. The dependency of P on the comet observability limit OL is also presented for various cometary samples.
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