Mechanics of particles and systems Particle systems and celestial mechanics Problem
Euler's three-body problem
Builds on Newton's law of universal gravitationHamiltonian systemFirst integralIntegrable systemThree-body problem
Problem
Let be the gravitational constant, let and let . Two point masses and are fixed at the points and of . A particle at moves under their Newtonian attraction: where and are the distances from to the two fixed points. Given the initial position and velocity of the particle, determine its motion.
Remarks
The problem is also called the problem of two fixed centres. It is solved: Euler showed in 1760 that it can be integrated exactly. It is a Hamiltonian system with three degrees of freedom and three independent first integrals in involution, so it is an integrable system. They are the energy, the component of the angular momentum along the axis through the two centres, and a third integral found by separating variables. In prolate spheroidal coordinates , and the angle around the axis, the Hamilton–Jacobi equation separates, and the solution is given by elliptic integrals.
The problem differs from the three-body problem because the two centres do not move. It is used as an approximation for a satellite near an oblate planet and, in quantum mechanics, for the hydrogen molecule ion.
Reading path
To understand this page from the ground up, read these 49 pages in order. The foundations come first.
- Derivative concept
- Differential equation concept
- Euclidean space object
- Euclidean vector concept
- First integral concept
- Function concept
- Hamiltonian system concept
- Integrable system concept
- Interval concept
- Ordinary differential equation concept
- Velocity concept
- Fréchet derivative definition
- Cross product definition
- Ordinary differential equation definition
- Function of several variables concept
- Vector-valued function concept
- Lipschitz condition definition
- Classical mechanics concept
- n-body problem problem
- Limit of a function of several variables concept
- Momentum concept
- Partial derivative concept
- Solution of an ordinary differential equation definition
- Inertial frame of reference concept
- Three-body problem problem
- Continuity in R^n definition
- Differentiable function of several variables definition
- Partial derivative definition
- Initial value problem definition
- Newton's laws of motion statement
- Differentiable on an open set definition
- Gradient definition
- Higher partial derivatives definition
- Picard–Lindelöf hypotheses definition
- Iterated derivative definition
- Picard operator definition
- C^k function characterised by continuous derivatives statement
- Integral equation form of an initial value problem statement
- An iterate of the Picard operator is a contraction statement
- Vector field definition
- Picard–Lindelöf theorem statement
- Conservative vector field definition
- Classical mechanics definition
- Momentum definition
- Potential energy definition
- Angular momentum definition
- Central force definition
- Newton's law of universal gravitation statement
- Euler's three-body problem problem
Further reading
About this page
| Tag | FXPHA1T3NF |
|---|---|
| URI | m2://FXPHA1T3NF |
| Kind | problem |
| Writing | W0 stub |
| MSC | 70F07, 70H06, 70F15 |
| Status | This copy of the site has no build data. Run m2 status FXPHA1T3NF. |
| About | Three-body problem |
| Uses | Newton's law of universal gravitation, Hamiltonian system, First integral, Integrable system, Three-body problem |
| Same as | |
| Changed | 3 November 2026 |
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