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Mission Design for the CubeSat OUFTI-1

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CHAPTER 7.ATTITUDE CONTROL SYSTEMwhere C s is <strong>the</strong> solar constant, c <strong>the</strong> speed of light, R <strong>the</strong> reflectivityfactor, r sk <strong>the</strong> vector from <strong>the</strong> center of mass to <strong>the</strong> k’th surface elementA k , n k <strong>the</strong> outward surface normal and S <strong>the</strong> unit vector from satellite tosun.We pose R = 0.6, in a simplified scalar expression and we have:T SP,max = C sc A (1 + R) cos(i) (c SP − c GC ) = 2.06 · 10 −9 Nm (7.11)where i = 0 ◦ is incidence angle of sun and c SP − c GC = √ 0.02 2 + 0.02 2<strong>the</strong> distance between <strong>the</strong> center of mass and <strong>the</strong> center of solar pressure,projected on <strong>the</strong> surface.It’s usually cyclic when <strong>the</strong> satellite turns around <strong>the</strong> earth or arounditself (constant only <strong>for</strong> sun-oriented vehicles) and depends mainly from<strong>the</strong> surface properties and from <strong>the</strong> spacecraft geometry.• Aerodynamic drag: generated by <strong>the</strong> aerodynamic drag acting on <strong>the</strong> facein a point non coinciding with <strong>the</strong> gravity center.T A = 1 2 ρv2 c D∑rsk ×(n T k ˆV)ˆVAk (7.12)where c D is <strong>the</strong> drag coefficient, r sk <strong>the</strong> vector from <strong>the</strong> center of mass to<strong>the</strong> k’th surface element A k , n k <strong>the</strong> outward surface normal, ˆV <strong>the</strong> unitvector of velocity and V <strong>the</strong> module of <strong>the</strong> velocity vector.With c D = 2 and at <strong>the</strong> perigee we have:T A = 1 2 ρv2 Ac D (c A − c GC ) = 1.84 · 10 −7 Nm (7.13)where c A <strong>the</strong> center of aerodynamic <strong>for</strong>ce.Variable <strong>for</strong> inertially oriented vehicle, it depends from <strong>the</strong> altitude andon <strong>the</strong> geometry.• Magnetic field: generated by <strong>the</strong> coupling between <strong>the</strong> earth magneticfield and <strong>the</strong> satellite residual dipole.T M = D × B (7.14)where B is <strong>the</strong> earth magnetic field and D <strong>the</strong> residual dipole. For <strong>the</strong>moment we are not able to estimate it.Galli Stefania 67 University of Liège

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