摘要
本文发表的是我们于１９９０年在云南天文台利用１ｍＲＣＣ望远镜对天王星主要卫星进行照像观测的定位结果以及与理论计算值进行的比较分析．
The positions of the Uranian satellites from 7 photographic plates obtained with 1. 0m RCC telescope at the Yunnan Astronomical Observatory during the 1990 oppositions are given in this paper. 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 σa=0'. 31, σδ=0'. 33 and they are comparable with most of the precise observations found in the literatures.
出处
《陕西天文台台刊》
CSCD
1995年第6期1-4,共4页
Publications of The Shaanxi Astronomical Observatiory
基金
国家自然科学基金
中国科学院天文委员会基金
