| Agemegos |
02-08-2010 07:59 PM |
Re: [Space] Binary star trojans
Quote:
Originally Posted by lexington
(Post 930529)
Physics isn't my strong suit but I'm fairly certain you can't orbit any Lagrange point, given that it isn't exerting a pull on objects near it.
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Well, it turns out that there are orbits for a test mass in a two-body system that have the same period as the orbit of the two main bodies but which aren't similar to the orbits of the main bodies about the barycentre. In the co-rotating frame of reference these look like loops (often distorted loops) around empty points. There is a family of such "halo orbits" around L1, L2, and L3, which are truly periodic, and there are so-called "Lissajous orbits" around all of the L points, though those are only quasi-periodic and not really stable.
Look up "horseshoe orbit" and "tadpole orbit".
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