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Title: Radiation pressure torque and computational attitude modelling of space debris
Author: Virdee, Hira Singh
ISNI:       0000 0004 7226 0186
Awarding Body: UCL (University College London)
Current Institution: University College London (University of London)
Date of Award: 2017
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Human space activity in the past 50 years has led to a plethora of man-made space debris which pose an imminent threat to global space operations. The current models of space debris orbits are not sufficient for detailed orbit prediction or for accurate tracking. This uncertainty manifests itself in Conjunction Analysis (CA) with active spacecraft, which leads to excessive orbital manoeuvres which are both expensive and reduce the lifetime of satellites. Advances in orbit modelling will lead to better prediction of debris orbits and reduce the need for collision avoidance manoeuvres, as well as minimising the future pollution of the space environment through collisions. Most existing methods for analysing the orbits of space debris do not take into account the effects of tumbling, and the attitude-dependent nonconservative forces are generally neglected. This study models the torques and attitude motion of uncontrolled man-made objects in orbit about the Earth, which tumble due to a combination of natural influences of the near-Earth space environment and initial angular momentum acquired during debris formation. The modelling of space debris is a relatively new field and represents a huge new area of research. The two main branches of this thesis are (a) modelling the torques that induce spin for objects in orbit, and (b) modelling the effect of certain attitude-dependent non-conservative forces on spinning objects in orbit. The main torque modelled in this study is solar radiation pressure (SRP). Simulations of the radiation-induced torques are performed and the main mechanisms that lead to the tumbling of uncontrolled objects are analysed. A novel method of presenting attitude-dependent forces and torques on space objects, dubbed ”Torque Maps”, is presented. Radiation torques are caused by optical geometric asymmetry and can lead to oscillatory and secular changes in attitude. They are computed for one of the largest objects in orbit: Envisat, a defunct satellite with complex geometry. Further to these, simulations of objects spinning in orbit are used to calculate the effect of tumbling on orbital motion. The results show that the effects of nonconservative forces on tumbling objects lead to both periodic and secular variations in their orbital elements. This is contrary to previously popular assumption. Additionally, ideas for utilising modern developments in nanosatellite technology for validation of orbit prediction models are presented and calculations of the Lorentz force and its effect for uncontrolled objects are given.
Supervisor: Ziebart, M. Sponsor: Not available
Qualification Name: Thesis (Ph.D.) Qualification Level: Doctoral
EThOS ID:  DOI: Not available