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Astrometrical observations of Pluto-Charon system with the automated telescopes of Pulkovo observatory

机译:普尔科沃天文台自动望远镜对冥王星-Charon系统的天文观测

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The space probe "New Horizons" was launched on 19th of January 2006 in order to study Pluto and its moons. Spacecraft performed close fly-by to Pluto on 14th of July 2015 and obtained the most detailed images of Pluto and its moon until this moment. At the same time, observation obtained by the ground based telescopes may also be helpful for the research of such distant system. Thereby, the Laboratory of observational astrometry of Pulkovo Observatory of RAS made a decision to reprocess observations obtained during last decade. More than 350 positional observations of Pluto-Charon system were carried out with the mirror astrograph ZA-320M at Pulkovo and Maksutov telescope MTM-500M near Kislovodsk. These observations were processed by means of software system APEX-II developed in Pulkovo observatory and numerical simulations were performed to calculate the differences between positions of photocenter and barycenter of Pluto-Charon system. (c) 2016 Elsevier Ltd. All rights reserved.
机译:为了研究冥王星及其卫星,“新视野号”太空探测器于2006年1月19日发射升空。航天器于2015年7月14日飞近冥王星,获得了冥王星及其月球最详细的图像。同时,地面望远镜的观测也可能对这种遥远系统的研究有所帮助。因此,RAS普尔科沃天文台的观测天文实验室决定重新处理过去十年中获得的观测结果。利用普尔科沃的天文望远镜ZA-320M和基斯洛沃茨克附近的马克苏托夫望远镜MTM-500M对冥王星-Charon系统进行了350多次位置观测。这些观测结果是通过在普尔科沃天文台开发的软件系统APEX-II处理的,并进行了数值模拟,以计算冥王星-Charon系统的光心和重心位置之间的差异。 (c)2016 Elsevier Ltd.保留所有权利。

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