Reasons for change in artificial space objects own rotation

Authors

  • В. П. Єпішев Laboratory of space reserches, Uzhhorod National University, Ukraine
  • В. І. Кудак Laboratory of space reserches, Uzhhorod National University, Ukraine
  • В. І. Присяжний National space facilities control and test center, Ukraine
  • Д. М. Кожухов National space facilities control and test center, Ukraine
  • В. М. Періг Laboratory of space reserches, Uzhhorod National University, Ukraine
  • І. Ф. Найбауер Laboratory of space reserches, Uzhhorod National University, Ukraine

DOI:

https://doi.org/10.24144/2415-8038.2019.46.137-144

Keywords:

Period, Satellite, Rotation, Photometry, Light curve.

Abstract

Purpose. Photometry in conjunction with positional observations is currently the main method of controlling the operation of artificial space objects in orbit with which radio communication is lost. This paper presents an analysis oflong-range photometric observations of low-orbital artificial Earth satellites of various functionality class.

Methods. A methodological approach to determining the dynamic characteristics of the behavior of space objects in orbit using photometric information in the form of light curves is considered. It is based on studies of the characteristics of the object’s own rotation and their causes.

Results. 40 years of experience in such studies has made it possible to evaluate virtually all possible factors affecting its functional dynamics by changes in the light of an object. The paper presents six reasons for the occurrence of a satellite’s own rotation in the Earth’s orbit. They cover both natural factors and the effects of human intervention.

Conclusions. If the size and mass of the destabilized satellites are known, then this satellite can be used as an indicator of the course of physical processes in the Earth’s atmosphere at the height of the satellite’s orbit. The variants of finding the period of own rotation of the object in manual and automatic modes are described.

References

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Kudak V.I. Studying of the own rotation period changes of satellite ”Ajisai” on the interval 1986-2017 Kudak V.I., Perig V.M., Neubauer I.F. //Uzhhorod University Scientific Herald. Series Physics. — 2017, — Issue 41, — P. 140 – 145.

Lafler J. An RR Lyrae Star Survey with Ihe Lick 20-INCH Astrograph II. The Calculation of RR Lyrae Periods by Electronic Computer. Lafler, J., Kinman, T. D // The Astrophysical Journal Supplement Series, — 1965, — V.11, — P. 216 – 222.

Scargle J. D. Studies in astronomical time series analysis. II-Statistical aspects of spectral analysis of unevenly spaced data. /Scargle, J. D. //The Astrophysical Journal. — 1982. — V. 263, — P. 835 – 853.

Published

2019-11-27

Issue

Section

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