Astrometric observations of the Uranian satellites and a comparison with the theory.

Details Astrometric observations of the Uranian satellites and a comparison with the theory. Astrometric observations of the Uranian satellites and a comparison with the theory.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pshao..18....1q&link_type=abstract

Publ. Shaanxi Astron. Obs., Vol. 18, p. 1 - 4

Astronomy and Astrophysics

Astronomy

Uranus Satellites: Astrometry, Uranus Satellites: Orbit Theory

Scientific paper

The positions of the Uranian satellites from 7 photographic plates obtained with 1.0 m RCC telescope at the Yunnan Astronomical Observatory during the 1990 oppositions are given. These positions were compared with those calculated theoretically. The standard deviations of the observed-minus-calculated residuals referred to Titania are of the order of σα = 0″31, σδ = 0″33 and they are comparable with most of the precise observations found in the literature.

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