Abstract

This research studies the orbital dynamics of space debris in near-earth orbit and calculates its respective lifetime. The orbital dynamics of space debris is closely examined in near-earth orbit whereby (apogee altitude ha=1200 km and perigee altitude hp=200 km). In addition, the lifetime of the space debris is calculated using the influence of the friction force exerted on the atmospheric particles with debris dimensions measuring between (1-10 cm). In this study, the Drag Thermospheric Models (DTM78 and DTM94) are used because of their dependence on solar and geomagnetic activities, and pulsed lasers are utilized to interact with Aluminum 2024 particles which are frequently employed in the structure of spacecraft and aerospace designs. A numerical analysis program (NaP1) was built to calculate the lifetime of space debris and its time of return to the atmosphere. It is then integrated with a second numerical analysis program (NaP2) developed using the Lax-Wendroff finite difference method to simulate the laser material interaction model. A high-power Nd:YAG laser was applied to produce shock wave pressure in the target. The results show that the maximum peak pressure occurs at 50 μm depth and then slowly decays, the peak pressure increases with the increase of the laser intensity, and the optimum value of the momentum coupling coefficient (Cm) for the aluminum debris of size range (1-10 cm) is 6.5 dyn.s/j.

Highlights

  • Thin-film is called a layer or several layers of material atoms that do not intersect with.Space debris is defined as man -made objects or parts of in space, which do not serve any useful purpose

  • This research studies the orbital dynamics of space debris in near earth orbit

  • The lifetime of the space debris is calculated using the influence of the friction force exerted on the atmospheric particles with debris dimensions measuring between (1 and 10 cm)

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Summary

INTRODUCTION

Thin-film is called a layer or several layers of material atoms that do not intersect with. In more than 50 years of spaceflight, over 30,000 t of satellites and rockets have been sent to space. About half of the tractable objects are fragments from explosions or from the backup of satellites or rockets bodies [6, 7]. These debris which are 1 to 10 cm in size are very dangerous because they are difficult to see and yet can punch a big hole in space craft. A few years ago, a detailed project study were undertaken by Phipps and co-workers to propose a high-energy laser system called ORION

Lifetime and Atmospheric Drag Theory
Laser Material Interaction Theory
D D u C 2 du dP
Reentry of Space Debris Theory
Lax-Wendroff Method
Results of laser material interaction and Reentry Model
CONCLUSIONS
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