CCD astrometric observations of Uranian satellites.

Details CCD astrometric observations of Uranian satellites. CCD astrometric observations of Uranian satellites.

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26as..113..557v&link_type=abstract

Astronomy and Astrophysics Supplement, v.113, p.557

Astronomy and Astrophysics

Astrophysics

12

Astrometry, Satellites Of Uranus

Scientific paper

Astrometric positions of the five largest satellites are given for the oppositions of Uranus for the years 1989 to 1994. These positions were measured on 368 CCD frames obtained at the Cassegrain focus of a 1.6-m reflector. They are compared with the theoretically calculated positions from GUST86 (Laskar & Jacobson 1987). The observed minus calculated residuals referred to Oberon have standard deviations of the order of 0."05 for the three greatest Uranian satellites and 0.07" for Miranda. These residuals are comparable to the best available in the literature.

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