THE SIMULATION OF THE ORBITAL EVOLUTION OF A PASSIVE HIGH-ORBIT FRAGMENT WITH LARGE SURFACE AREA
Journal Title: Odessa Astronomical Publications - Year 2014, Vol 27, Issue 2
Abstract
The numerical integration of the motion equations of a passive high-orbit fragment with large surface area was performed accounting for the main gravitational perturbations of the Earth, Moon and Sun, as well as the solar radiation pressure. Based on the numerical model of motion in the near-Earth space that accounts for only the most powerful perturbations, a new method for de-orbiting artificial celestial bodies from high altitudes is suggested.
Authors and Affiliations
A. A. Bazyey
Keywords
Related Articles
- EP ID EP604342
- DOI -
- Views 82
- Downloads 0
PROBING AND IDENTIFYING NEW PHYSICS SCENARIOS AT INTERNATIONAL LINEAR COLLIDER
Many new physics scenarios are described bycontact-like effective interactions that can manifest themselves in e+e− collisions through deviations of the observables from the Standard Model predictions. If such a deviation...
THREE GIANTS – MEMBERS OF THE OPEN CLUSTER M 67
We determined the atmospheric parameters and chemical composition of the three giants, which are members of the open cluster M 67. The high resolution spectra (R = 60 000) were obtained with the echel...
THE PROPERTIS OF TIDAL FORCES IN THE KERR METRIC
The expression for the tidal forces of the two relativistic protons at a distance of the order of the Compton wavelength near a rotating black hole is found. The analysis shows that the tidal forces are dependent on the...
POSITIONAL CATALOGUES OF SATURN’S AND JUPITER’S MOONS
In the framework of the UkrVO national project (http://ukr-vo.org/) we have started the processing of photographic observations of Saturn’s (S1-S8) and Jupiter’s (J6-J8) moons. Observations were conducted during...
THE DAILY 110 MHZ SKY SURVEY (BSA FIAN): ON-LINE DATABASE, SCIENCE AIMS AND FIRST RESULTS OF DATA PROCESSING
From 2012 on radio telescope BSA FIAN multi beams diagram was started. It capable at July 2014 daily observing by 96 beams in declination -8 .. 42 degrees in the frequency band 109-111.5 MHz. The number of frequency band...