Analysis of errors in the motion of short-period comets

Details Analysis of errors in the motion of short-period comets Analysis of errors in the motion of short-period comets

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...41r&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, no. 5, p. 41-49.

Computer Science

Comets, Orbit Perturbation, Orbital Elements, Solar Orbits, Error Analysis, Orbital Mechanics, Solar System

Scientific paper

The rate of variation of the longitude of the ascending node and the argument of perihelion determined with observation data (O) is compared with the calculated data (C), with all known disturbance factors taken into account. Systematic errors (O-C), which can be caused by the existence of an unknown massive body near the southern pole of the ecliptic, according to Radzievskii's (1972, 1987) hypothesis, are found.

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