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Article #4167Re: Finding Lagrange's Libration Points
From: Henry Spencer
Date: Fri, 20 Jan 1989 18:08
Date: Fri, 20 Jan 1989 18:08
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In article <11854@dartvax.Dartmouth.EDU> dalex@eleazar.dartmouth.edu (Dave Alexander) writes: >So if L1, L2, and L3 are loci of unstable equilibrium, how can we expect >an object to librate or oscillate about any of them? You can't, and it won't, without help. An object *precisely* at one of those points, with *no* perturbations, would stay there, but in the real world, that doesn't work. There are trajectories near those points -- so-called "halo orbits" -- which are *almost* stable, requiring only very slight corrections to maintain. ISEE-3 was in a halo orbit around the Earth-Sun L1 point for some years, to study the solar wind "upwind" of Earth. -- Allegedly heard aboard Mir: "A | Henry Spencer at U of Toronto Zoology toast to comrade Van Allen!!" | uunet!attcan!utzoo!henry henry@zoo.toronto.edu
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Newsgroups: sci.astro,sci.space Path: arc1-ca.pugleaf.net!utzoo!henry From: henry@utzoo.uucp (Henry Spencer) Subject: Re: Finding Lagrange's Libration Points Message-ID: <1989Jan20.180839.7800@utzoo.uucp> Organization: U of Toronto Zoology References: <1989Jan18.044744.18328@sq.uucp> <11854@dartvax.Dartmouth.EDU> Date: Fri, 20 Jan 89 18:08:39 GMT