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AAE450 Spring 2009 Analysis of Trans-Lunar Spiral Trajectory [Levi Brown] [Mission Ops] February 12, 2009 1.

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Presentation on theme: "AAE450 Spring 2009 Analysis of Trans-Lunar Spiral Trajectory [Levi Brown] [Mission Ops] February 12, 2009 1."— Presentation transcript:

1 AAE450 Spring 2009 Analysis of Trans-Lunar Spiral Trajectory [Levi Brown] [Mission Ops] February 12, 2009 1

2 AAE450 Spring 2009 [Levi Brown] [Mission Ops] Spiral Transfer 2 Equations of Motion (EOM)s : r: distance from central body to spacecraft (s/c) μ: Gravitational parameter (G*M) θ: Angle of rotation T: Thrust from engine m: Mass of spacecraft Assumes: Two body problem Point mass central body/spacecraft Coplanar Transfer to Moon Thrust is in Force of gravity in the Circular lunar orbit Constant thrust Created Code: Input s/c mass, thrust levels, time of flight (TOF) Integrate EOMs for spiral outward to moon’s sphere of influence (r ≈ 3.2 x 10 5 km) “Turn off” Earth’s gravity and “turn on” Moon Determine velocity and position relative to moon (integrate with a “braking” thrust) Output history of s/c position and velocity

3 AAE450 Spring 2009 [Levi Brown] [Mission Ops] 3 Results Limiting Case: 1 Year TOF Inputs: m o = 595.4 kg (Latest OTV Mass) TOF out = 356 days TOF in ≈7 days (Keep low spiral time) Results: Required T out = 109.5 mN Required T in = 93.5 mN Perilune Altitude ≈ 8.0 km Perilune Velocity = 2.3 km/s Note: Code uses physics to determine s/c motion and is independent of engine properties Can we produce this much thrust for this amount of time with a s/c of this mass? ΔV is dependent on engine characteristics because of low thrust Will use this code iteratively with propulsion to determine if mission can be completed for a given system

4 AAE450 Spring 2009 Back-up Slides [Levi Brown] [Mission Ops] 4

5 AAE450 Spring 2009 [Levi Brown] [Mission Ops] Case 1 Spiral Out 5

6 AAE450 Spring 2009 [Levi Brown] [Mission Ops] Case 1 Spiral In 6

7 AAE450 Spring 2009 [Levi Brown] [Mission Ops] 7 Spacecraft Radius for Lunar Spiral

8 AAE450 Spring 2009 [Levi Brown] [Mission Ops] 4 Other Future Work: Work with descent group Many possibilities for altitude and velocity for descent What works best? Should we try to circularize orbit more first? Look at effects of varying departure orbit (higher LEO, GTO) Add in 3 rd body effect Have both Earth and Moon gravity in both integrations More efficient thrusting Is it more efficient to thrust in velocity direction?

9 AAE450 Spring 2009 [Levi Brown] [Mission Ops] 4 Notes on iteration with propulsion: DeltaV is caused by 2 factors (gravity and thrust) For impulse type maneuvers, it is assumed that the thrusting is instantaneous This means that the deltaV between two points on a trajectory is only caused by gravity Because code indicates an initial mass, a constant thrust, and a TOF, it was determined that the best method of calculating deltaV was through the equations for the engine The current mass was based off of our initial deltaV assumption of 8 km/s The sizing equations take a deltaV and various specifications for a particular engine Using the deltaV and specifications, parameters such as TOF, propellant mass, mass flow rate, initial mass, and thrust are produced. If we fix a TOF, we can vary deltaV until the TOF match and then find the mass and thrust required for that engine Then use the trajectory code to determine if we can reach the moon If not, vary the deltaV and do it again


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