Abstract

By nodal regression and apsidal precession, the Earth flattering at satellite low Earth orbits (LEO) is manifested. Nodal regression refers to the shift of the orbit’s line of nodes over time as Earth revolves around the Sun. Nodal regression is orbit feature utilized for circular orbits to be Sun synchronized. A sun¬-synchronized orbit lies in a plane that maintains a fixed angle with respect to the Earth-Sun direction. In the low Earth Sun synchronized circular orbits are suited the satellites that accomplish their photo imagery missions. Nodal regression depends on orbital altitude and orbital inclination angle. For the respective orbital altitudes the inclination window for the Sun synchronization to be attained is determined. The apsidal precession represents major axis shift, respectively the argument of perigee deviation. The apsidal precession simulation, for inclination window of sun synchronized orbital altitudes, is provided through this paper.

Highlights

  • Orbital perturbation analyzes consider the satellite’s orbit behavior under real space-ambient circumstances compared with ideal orbit mathematical model defined by Kepler parameters

  • The aim of this paper is to conclude about the apsidal range which corresponds to inclination window for orbit Sun synchronization

  • The apsidal precession for circular orbits depends upon orbit inclination and orbit altitude

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Summary

INTRODUCTION

Orbital perturbation analyzes consider the satellite’s orbit behavior under real space-ambient circumstances compared with ideal orbit mathematical model defined by Kepler parameters. Due to the gravitational forces of the Sun, other celestial bodies and due to the Earth’s flattering at both poles the perturbations are caused. The Earth flattering is manifested by the nodal regression and apsidal precession. For satellites orbiting the Earth, the laws of celestial bodies’ movement are applied. This concept is applied for the apsidal precession analysis of the Sun synchronized low Earth orbiting (LEO) satellites. The nodal regression is considered and followed by terms the orbit Sun synchronization to be accomplished. Considering different initial low Earth orbit altitudes the inclination window for orbit Sun synchronization is determined. For the determined inclination window, the apsidal precession is simulated

NODAL REGRESSION
APSIDAL PRECESSION
CONCLUSIONS
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