Studying the Evolution of the Exterior Zone of Oort's Cometary Cloud by Numerical Modelling

Details Studying the Evolution of the Exterior Zone of Oort's Cometary Cloud by Numerical Modelling Studying the Evolution of the Exterior Zone of Oort's Cometary Cloud by Numerical Modelling

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987atsir1478....5c&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1478/FEB, 1987

Astronomy and Astrophysics

Astronomy

Scientific paper

Differential equations of cometary motions in the Oort's cloud are studied by the Runge-Kutta numerical integration method taking into account different kinds of perturbations. It is shown that (1) the gravitational field of the Galaxy increases the dimensions of Oort's cloud, but at the same time it presses this cloud. (2) The exterior zone of Oort's cloud is destroyed after one encounter of the Solar System with any star or interstellar H2-cloud.

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