Effect of the High-Order Resonances on the Orbital Evolution of Objects near Geostationary Orbit / Kuznetsov E. D.,Zakharova P. E.,Glamazda D. V.,Kudryavtsev S. O. // SOLAR SYSTEM RESEARCH. - 2014. - V. 48, l. 6. - P. 446-459.

ISSN/EISSN:

0038-0946 / 1608-3423

Type:

Article

Abstract:

The area-to-mass ratio of high-orbit space objects is estimated on the basis of positional observations from the SBG telescope at the Kourovka astronomical observatory of the Ural Federal University. The properties of regions where high-order resonances are located are analyzed. The position and sizes of the resonance zones depending on the area-to-mass ratio of objects are determined on the basis of numerical modeling. It is shown that a system transits through the high-order resonances due to secular perturbations of the semimajor axis under the Poynting-Robertson effect. The high-order resonances weakly influence the formation of the stochastic trajectories. The stochastic properties are mostly manifested in evolution of the semimajor axis of the orbit.

Author keywords:

SATELLITE; MOTION; PRESSURE

DOI:

10.1134/S0038094614060045

Web of Science ID:

ISI:000345092400006

Соавторы в МНС:

Другие поля

Поле	Значение
Month	NOV
Publisher	MAIK NAUKA/INTERPERIODICA/SPRINGER
Address	233 SPRING ST, NEW YORK, NY 10013-1578 USA
Language	English
EISSN	1608-3423
Keywords-Plus	SATELLITE; MOTION; PRESSURE
Research-Areas	Astronomy \& Astrophysics
Web-of-Science-Categories	Astronomy \& Astrophysics
Author-Email	eduard.kuznetsov@urfu.ru
Funding-Acknowledgement	Russian Foundation for Basic Research {[}13-02-00026-a]
Funding-Text	This work is partially supported by the Russian Foundation for Basic Research (project no. 13-02-00026-a).
Number-of-Cited-References	31
Usage-Count-Last-180-days	3
Usage-Count-Since-2013	18
Journal-ISO	Solar Syst. Res.
Doc-Delivery-Number	AT7BW