Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10 5/3/83; site utzoo.UUCP Path: utzoo!henry From: henry@utzoo.UUCP (Henry Spencer) Newsgroups: net.space Subject: Re: Lagrange Points Message-ID: <5000@utzoo.UUCP> Date: Fri, 1-Feb-85 22:28:55 EST Article-I.D.: utzoo.5000 Posted: Fri Feb 1 22:28:55 1985 Date-Received: Fri, 1-Feb-85 22:28:55 EST References: <298@ho95b.UUCP>, <3347@alice.UUCP> Organization: U of Toronto Zoology Lines: 18 > L4 and L5 are only stable if the mass ratio of the two primary bodies > is large enough. I'd have to do some figgurin' to reconstruct the > limiting ratio, but as I remember, the Earth is just barely large > enough to make the Earth-Moon L4 and L5 stable. A corollary is that > the hotdog-shaped stable regions around the Earth-Moon Trojan points > aren't very large or `deep'. As I recall it, the threshold is about a 30:1 ratio. The Earth/Moon system has about an 80:1 ratio, I believe, which would make things a bit more favorable than Tom suggested. But I'd have to look all this up to be absolutely sure. Note to people wanting a simple explanation of why the ratio has to be in excess of a threshold: as far as I know, there isn't one. You just have to work through the math. -- Henry Spencer @ U of Toronto Zoology {allegra,ihnp4,linus,decvax}!utzoo!henry