Here's a couple screen capture of starting out in olive orbits and eventually leaving earth's Hill Sphere. Same orbits, different zooms.
Quote from: Hop_David on 05/19/2015 08:16 amHere's a couple screen capture of starting out in olive orbits and eventually leaving earth's Hill Sphere. Same orbits, different zooms.Is the place where the paths of the pellets diverge so greatly near the SEL-1 point? Or SE-L2?
I think that mass for energy storage is likely to be prohibitive, the vehicle will simply shut down propulsion when in the dark, this could significantly increase the time needed to spiral out, but the spiral out is an unmanned flight, almost no amount of time is too much, the only thing were worried about is Van-Allen radiation induced degradation of the vehicle, primarily the solar system.
The plots below show a "quick path" home from EML-2. The total elapsed time is 10.8 days. The total delta-v is 583 m/s. The trajectory departs EML-2 with a 55 m/s burn at an angle of 148.5 degrees from the line between the Earth and Moon. It travels in the general direction of the Moon, looping around a bit until it reaches an apolune at 6.6 days. There a 158 m/s retrograde burn leads to a deep perilune at 8.3 days. A 370 m/s burn at perilune leads to a trajectory that intersects the Earth at a relative speed of 11,134 m/s.
Quote from: sdsds on 05/27/2015 04:45 pmFiguring out the "control law" that would make that thrust always be in the optimal direction seems like quite a challenge, though!Bounded momentum model on the combined two body (Earth Moon) projective gradient.
Figuring out the "control law" that would make that thrust always be in the optimal direction seems like quite a challenge, though!
Quote from: Space Ghost 1962 on 05/27/2015 06:02 pmQuote from: sdsds on 05/27/2015 04:45 pmFiguring out the "control law" that would make that thrust always be in the optimal direction seems like quite a challenge, though!Bounded momentum model on the combined two body (Earth Moon) projective gradient.That's easy for you to say! I think by optimal you might mean, "has greatest effect" on energy, looking at something like the Jacobi integral.
Decreasing the energy would effectively put the particle down into one of the wells of the effective potential. This would be going "always down hill" on the energy manifold. That gets someplace with optimal efficiency. I don't see how to make certain that someplace is the place we want to go.
For planar motion there is a four-dimensional phase space, (x, y, vx, vy). Consider starting at (x1, y1, vx1, vy1) with the desire to get to (x2, y2, vx2, vy2). I don't see an easy solution to that!
As for orbits being reversible?