Projectiles and the Kepler problem

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    Kepler Projectiles
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Homework Help Overview

The problem involves determining the initial velocity vector required to send a projectile from one point to another within the gravitational field of a celestial body, specifically addressing the time of flight and the uniqueness of the velocity vector.

Discussion Character

  • Exploratory, Conceptual clarification, Problem interpretation

Approaches and Questions Raised

  • Participants discuss the integration of time into the solution and the challenges associated with angular integration. There is mention of Lambert targeting as a potential approach, with questions about its relevance and resources for further reading.

Discussion Status

The discussion is ongoing, with participants exploring different methods and seeking clarification on Lambert targeting. Some guidance on resources has been provided, but there is no explicit consensus on the best approach yet.

Contextual Notes

Participants note that conservation principles may not be useful due to the time-dependent nature of the problem. There is also a reference to the complexity of the problem beyond the special case of circular orbits.

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Homework Statement



Within the gravitational field produced by a celestial body of mass M we want to send a projectile of mass m from (x1,y1) to (x2,y2). The M mass is placed at the origin of coordinates. If the flight time is T, what is the initial velocity vector that we have to give to the projectile? Is this vector unique?

Homework Equations



The usual equations of the Kepler problem, ie

[tex]l=mr^2\dot{\theta}[/tex]

[tex]E=\frac{1}{2}m\dot{r}^2+\frac{l^2}{2mr^2}-\frac{k}{r}[/tex]

[tex]r=\frac{\frac{l^2}{mk}}{1+\epsilon\cos\theta}[/tex]

Maybe the most relevant one is

[tex]dt=\frac{m}{l}r^2\,d\theta[/tex]

since this equation includes time explicitly.

The Attempt at a Solution



Using [tex]dt=\frac{m}{l}r^2\,d\theta[/tex] and the equation for the orbit I integrated from [tex]t=0[/tex] to [tex]t=T[/tex] but the angular integration, that although can be done analytically, it turns out to be quite difficult, so I think this is not the right way to go.

The special case of a circular orbit is solved easily but I think the problem has to be solved in general.

Thanks in advance!
 
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In this problem, conservation principles are not quite useful since they are time-independent. The main difficulty of this problem is to incorporate T into the solution of the problem.

Any ideas?
 
luisgml_2000 said:
Any ideas?
Lambert targeting.
 
Hi! Thanks for replying.

D H said:
Lambert targeting.

So my problem is about Lambert targeting? Can you tell me where I can read about it?

Thanks!
 
luisgml_2000 said:
So my problem is about Lambert targeting? Can you tell me where I can read about it?
[strike]As a starting point only, here is the wikipedia article on Lambert's problem: http://en.wikipedia.org/wiki/Lambert's_problem[/strike]

Fundamentals of Astrodynamics and Applications by David Vallado is an excellent reference. Some of the section regarding Lambert's problem is available at Google books: http://books.google.com/books?id=PJLlWzMBKjkC&pg=RA1-PA448#v=onepage&q=&f=false

Fundamentals of Astrodynamics by Bate, Mueller, and White also covers the topic.

Chapter 2 ("Guidance Algorithm") of http://dspace.mit.edu/bitstream/handle/1721.1/34137/67775726.pdf?sequence=1" does a nice job of describing Lambert's problem.


Edit:
Wikipedia reference struck. This is an example of why wikipedia is a lousy reference. The article has no references, is poorly written, and misses the very important concept of the "short way" versus the "long way".
 
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