Uranian satellites (Veiga+, 1995)

Details Uranian satellites (Veiga+, 1995) Uranian satellites (Veiga+, 1995)

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat..41130557v&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/113/557. Originally published in: 1995A&AS..113..557V

Astronomy and Astrophysics

Astronomy

Solar System, Planets, Astrometric Data

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. (1 data file).

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