Uranian satellites in 1995/97 (Shen+, 2002)

Details Uranian satellites in 1995/97 (Shen+, 2002) Uranian satellites in 1995/97 (Shen+, 2002)

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33910775s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/391/775. Originally published in: 2002A&A...391..775S

Astronomy and Astrophysics

Astronomy

Planets, Positional Data

Scientific paper

In this paper, we publish measurements of 864 positions of the major satellites of Uranus made in 1995-1997 using CCD (1024"*1024") detectors attached to the 1.56-metre Astrometric Telescope at the Sheshan station near Shanghai. Analysis of the data as inter-satellite positions shows that the observations of Ariel, Umbriel, Titania and Mirand relative to Oberon have root-mean-square residuals of 0.03"-0.05", except for the innermost and faintest satellite Miranda, whose residuals exceeded 0.08" due to the proximity of Uranus. (2 data files).

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