ARO309 - Astronautics and Spacecraft Design
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Transcript of ARO309 - Astronautics and Spacecraft Design
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ARO309 - Astronautics and Spacecraft Design
Winter 2014
Try LamCalPoly Pomona Aerospace Engineering
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Lambert’s Solution
Chapter 5
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Introductions
• This chapter only covers the basic concept of determining an orbit from some observation
• In practice, this is not referred to as orbit determination
• Space OD is actually a statistical estimation or filtering method (example: Kalman Filter)
• We will only cover Lambert’s problem (Section 5.3) from this Chapter
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Lambert’s Problem
• Given 2 positions on an orbit r1 and r2 and Δt, what are the velocities at those two points, v1 and v2.
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Lambert Fit• Steps to find v1 and v2:
1. Find the magnitude of r1 and r2
2. Decide if the orbit is prograde or retrograde
3. Compute the following
4. Compute Δθ
for prograde for retrograde
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Lambert Fit5. Compute the function
6. Find z by iterating using Newton’s method until convergence
you can start with z0 = 0 (or positive z0 if an elliptical orbit), where
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Lambert Fitwhere
7. Note: the sign of the converged z tells you the orbit type:
z < 0 Hyperbolic Orbitz = 0 Parabolic Orbitz > 0 Elliptical Orbit
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Lambert Fit8. Compute the function y(z) using the converged z
9. Compute f, g, fdot, gdot
10. Compute
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Example 5.2 (Text Book)
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Example 5.2 (Text Book)
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Example 5.2 (Text Book)