Puck satellite Earth-based observations

被引:6
作者
Veiga, C. H.
Bourget, P.
机构
[1] Observ Nacl, BR-20921400 Rio De Janeiro, Brazil
[2] CNRS, Serv Aeron, F-91371 Verrieres Le Buisson, France
来源
ASTRONOMY & ASTROPHYSICS | 2006年 / 454卷 / 02期
关键词
planets and satellites : general; celestial mechanics; astrometry;
D O I
10.1051/0004-6361:20064977
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Puck, a faint satellite very close to Uranus' planet, was discovered by Voyager 2 Spacecraft images in 1986. Ever since then, few observations from Earth have been made. This prompted us to start a program of systematic observations of this satellite with the 1.6 m telescope at the Laboratrio Nacional de Astrofsica/MCT (Itajub, Brazil). The success of the observations is mainly due to the use of a Coronagraph developed at Observatrio Nacional/MCT (Rio de Janeiro, Brazil). This article presents astrometric positions obtained from Earth observations of Puck and of the five major Uranian satellites for four nights in 2004. Those positions are compared to the theoretically calculated positions from JPL Development Ephemeris. For Puck, the root mean square (rms) of the mean residual was found to be 84 milliarcseconds (mas). The stars' USNO-A2.0 catalog was used as a reference system for the astrometric calibration.
引用
收藏
页码:683 / 685
页数:3
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