Observations of high-elliptical space objects in the INASAN Zvenigorod Observatory

Authors

  • Bakhtigaraev N.S. Institute of Astronomy, Russian Academy of Science, Moscow, Russian Federation
  • Kostyuk N.D. Institute of Astronomy, Russian Academy of Science, Moscow, Russian Federation
  • Chazov V.V. Sternberg State Astronomical Institute, Moscow State University, Moscow, Russian Federation

UDC

629.78:52-13

Abstract

The camera VAU in the Zvenigorod Observatory was upgraded in 2009. The central guide of a triaxial mount of camera VAU was replaced by wide angle telescope "Santel-500", produced by A.V. Sankovitch in "Santel-M" company. The telescope equipped with a CCD-receiver FLI PL-9000 (3056 × 3056 pixels). Characteristics of the new telescope (aperture 0.5 m, the focal length 1.25 m, field of view 2.8 sq.deg) are providing successful observations of high-elliptical near-earth space objects. For example, in 2013, during 88 nights of observations carried out more than 45 thousands of definition of positions and star magnitudes for 850 high-orbit space objects, which are primarily used for the maintenance of the Catalogue of space objects in the of Space Surveillance System of the Russian Federation. The main attention is paid to the observations of space debris. Efforts were successful sessions observations of several "Molniya" type satellites before their reentering to the atmosphere. Observatory successfully participated in the optical ballistic following of Anik G1 satellite launch. The results of observations are discussed.

Keywords:

space debris, observations of high-elliptical space objects

Author Infos

Nail S. Bakhtigaraev

канд. физ.-мат. наук, доцент, старший научный сотрудник Института астрономии РАН

e-mail: nail@inasan.ru

Natalya D. Kostyuk

канд. физ.-мат. наук, старший научный сотрудник Института астрономии РАН

e-mail: kostyuk@inasan.ru

Vadim V. Chazov

д-р физ.-мат. наук, старший научный сотрудник Государственного астрономического института им. П.К. Штернберга Московского государственного университета

e-mail: vadimchazov@yandex.ru

References

  1. Бахтигараев Н.С., Костюк Н.Д., Чазов В.В. Наблюдения спутника Молния 3-39 в Звенигородской обсерватории ИНАСАН и определение времени падения // Вестник СибГАУ. 2011. Вып. 6 (39). С. 183-185.
  2. Kouprianov V. Distinguishing features of CCD astrometry of faint GEO objects // Advances in Space Research. 2008. Vol. 41. P. 1029-1038.
  3. Бахтигараев Н.С., Чазов В.В. Информационное обеспечение космических экспериментов на основе численно-аналитической теории движения искусственных спутников Земли // Космические исследования. 2005. Т. 43. №5. С. 386-389.
  4. Шилин В., Хуторовский З. Сопровождение, определение времени прекращения существования и района возможного падения обломков космических аппаратов "Молния-1-92" и "Молния-3-53". М.: ОАО "МАК "Вымпел"", 2013. Рукопись. 30 с. [URL]: http://vimpel.ru/images/stories/skkp/__.doc (дата обращения 12.12.2013)

Issue

Pages

38-42

Submitted

2013-12-12

Published

2013-12-30

How to Cite

Bakhtigaraev N.S., Kostyuk N.D., Chazov V.V. Observations of high-elliptical space objects in the INASAN Zvenigorod Observatory. Ecological Bulletin of Research Centers of the Black Sea Economic Cooperation, 2013, no. 4, pp. 38-42. (In Russian)