作者: R. I. Gumerov , I. M. Khamitov , L. A. Hudkova , N. V. Maigurova , G. I. Pinigin
DOI: 10.3103/S0884591315060021
关键词: Geocentric coordinates 、 Near-Earth object 、 Orbital elements 、 Declination 、 Physics 、 Dynamic method 、 Asteroid 、 Telescope 、 Astronomy 、 Right ascension
摘要: We report the results of analysis data volume containing 13834 topocentric positions 231 asteroids obtained from observations at Russian–Turkish RTT-150 telescope (TUBITAK (Scientific and Technological Research Council Turkey), Turkey) in 2004–2013. The were calculated with differential reduction method ICRS system use reference catalogs UCAC series. observational program covered main-belt closely encountering other near-Earth (NEA). For main belt asteroids, mean-square error one position was 84 68 mas right ascension declination, respectively, while it 160 120 mas, for NEAs. asteroid widens arc groundbased these bodies, which is important evaluating their orbital elements a higher accuracy. Moreover, periods close encounters yield valuable material to solve problem on accurate estimation masses dynamic method. It has been shown that supplementing input dataset here-reported decreases estimates perturbing mass parameters perturbed bodies.