Empirical model of area-to-mass ratio variations of Fengyun 2D Deb
- Paper number
IAC-18,A6,IP,43,x45279
- Author
Dr. Polina Levkina, Russian Federation, Institute of Astronomy, Russian Academy of Sciences (RAS)
- Coauthor
Dr. Nail Bakhtigaraev, Russian Federation, Institute of Astronomy, Russian Academy of Sciences (RAS)
- Coauthor
Dr. Vadim Chazov, Russian Federation, Sternberg Astronomical Institute of Moscow Lomonosov State University
- Year
2018
- Abstract
Orbital motion of space debris objects highly susceptible to difficult-to-predict non-gravitational perturbations. Area-to-mass ratio value can be calculated directly from observations and is a variable value that depends on the rotation parameters of the object. Knowledge of the area-to-mass ratio variations can improve the prediction accuracy of the orbital elements. The small-sized fragment of space debris 2006-053D Fengyun 2D Deb has been observed since 2007. This fragment moves in libration orbit around the Eastern stable point at longitude 75E with amplitude of 24 degrees and a period of 750 days. An empirical model of the area-to-mass ratio of this fragment was created using the results of 12-week sessions of observations at the Terskol observatory from 2009 to 2014. Area-to-mass ratio varies from 0.04 to 0.22 m$^2$/kg. The model was composed of four curves on the interval of a single period (392 days). Each curve is a section of a sinusoid with a period of 196 days. The model of area-to-mass ratio was developed using a numerical–analytical theory of satellite motion. Observations of Fengyun 2D Deb in 2015-2017 with the telescope Zeiss–2000 of Terskol observatory and at the telescope Zeiss–1000 of Sanglokh observatory have confirmed the validity of the model of area-to-mass ratio variations (the model was not improved by observations after 2014). This research supported by grant of the President of the Russian Federation No. MK-6640.2018.2.
- Abstract document
- Manuscript document
IAC-18,A6,IP,x45279.pdf (🔒 authorized access only).
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