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- Q232976 subject Q6453069.
- Q232976 subject Q7007336.
- Q232976 subject Q7163675.
- Q232976 abstract "In classical mechanics, the two-body problem is to determine the motion of two point particles that interact only with each other. Common examples include a satellite orbiting a planet, a planet orbiting a star, two stars orbiting each other (a binary star), and a classical electron orbiting an atomic nucleus (although to solve the electron/nucleus 2-body system correctly a quantum mechanical approach must be used).The two-body problem can be re-formulated as two one-body problems, a trivial one and one that involves solving for the motion of one particle in an external potential. Since many one-body problems can be solved exactly, the corresponding two-body problem can also be solved. By contrast, the three-body problem (and, more generally, the n-body problem for n ≥ 3) cannot be solved in terms of first integrals, except in special cases.".
- Q232976 thumbnail Orbit5.gif?width=300.
- Q232976 wikiPageExternalLink Two-BodyProblem.html.
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- Q232976 wikiPageWikiLink Q6453069.
- Q232976 wikiPageWikiLink Q6604.
- Q232976 wikiPageWikiLink Q7007336.
- Q232976 wikiPageWikiLink Q7163675.
- Q232976 wikiPageWikiLink Q7858690.
- Q232976 wikiPageWikiLink Q809690.
- Q232976 wikiPageWikiLink Q822938.
- Q232976 comment "In classical mechanics, the two-body problem is to determine the motion of two point particles that interact only with each other.".
- Q232976 label "Two-body problem".
- Q232976 depiction Orbit5.gif.