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Re: [Phys-l] Fun orbital problem



On Jan 2, 2008, at 1:35 PM, Carl Mungan wrote:

Apropos of nothing in particular, here's a fun problem whose
solution may raise more questions in your mind:

Three particles interact only gravitationally, follow circular
orbits, and remain at all times collinear. The radii of two of the
orbits is unity. What is the radius of the third?

John Mallinckrodt
Cal Poly Pomona

I think this is a solution:

http://usna.edu/Users/physics/mungan/Scholarship/BinaryOrbit.pdf

but let me know if you had something else in mind.

1) Thanks for sharing, Carl.
2) The title of the above web-page is "Synchronous Orbit of a Satellite about a Binary Star." This is consistent with the way in which the problem is introduced. You wrote: "Two equal-mass stars circle each other a distance R apart. A much lighter third body is in line with them (but not between them) and orbits them synchronously. What is the radius x of its orbit?" . . .

3) After showing that x should be close to 1.2 you make the following statement: "What we have calculated here is the second/third Lagrange point (well known to be unstable) for an equal-mass astronomical system."

4) In my opinion (3) and (2) contradict each other. If the satellite was orbiting the binary stars synchronously then the state of the motion would be stable. The three objects would be always on the same line. If this were true (which is not the case) then the motion would be stable (would remain periodic cycle after cycle after cycle. But in (3) you say, that the state of motion is is known to be unstable.

5) Do agree that there is a contradiction? If so then how should it be resolved? This kind of questions belong to critical thinking, not to scholasticism.

6) How do you distinguish a stable state of motion from an unstable one?
_______________________________________________________
Ludwik Kowalski, a retired physicist
5 Horizon Road, apt. 2702, Fort Lee, NJ, 07024, USA
Also an amateur journalist at http://csam.montclair.edu/~kowalski/cf/