Math 2.0

Mechanics of particles and systems Definition

Central configuration

Builds on n-body problemCentre of massNewton's law of universal gravitation

Definition

Let n≥2n \ge 2, let G>0G > 0 be the gravitational constant, let m1,…,mn>0m_1, \ldots, m_n > 0 be masses and let d≥1d \ge 1. Let q1,…,qn∈ℝdq_1, \ldots, q_n \in \R^d be pairwise distinct positions with centre of mass c=1M∑imiqic = \frac{1}{M} \sum_i m_i q_i, where M=∑imiM = \sum_i m_i. The configuration (q1,…,qn)(q_1, \ldots, q_n) is a central configuration if there is a real number λ\lambda such that ∑j≠iGmj(qj−qi)∥qj−qi∥3=−λ (qi−c)for all i=1,…,n.\sum_{j \ne i} \frac{G m_j (q_j - q_i)}{\norm{q_j - q_i}^3} = -\lambda\, (q_i - c) \qquad \text{for all } i = 1, \ldots, n. The left side is the acceleration of body ii under Newton's law of gravitation.

Remarks

The constant λ\lambda is always positive. Central configurations are counted up to translation, rotation and scaling, since these maps send central configurations to central configurations. Equivalently, they are the critical points of the potential U=∑i<jGmimj/∥qi−qj∥U = \sum_{i < j} G m_i m_j / \norm{q_i - q_j} restricted to configurations with a fixed moment of inertia about the centre of mass.

Example: three equal masses m=1m = 1, with G=1G = 1, at the vertices of an equilateral triangle of side ss. Each body feels two pulls of size 1/s21/s^2 with an angle of 60∘60^\circ between them, so the total pull has size 3/s2\sqrt{3}/s^2 and points to the centre. The distance to the centre is s/3s/\sqrt{3}, so the condition holds with λ=3/s3\lambda = 3/s^3. By a result of Lagrange the equilateral triangle is central for any three positive masses.

Non-example: three unit masses on a line at 00, 11 and 33, with G=1G = 1, so c=4/3c = 4/3. The body at 00 has acceleration 1+1/9=10/91 + 1/9 = 10/9, which forces λ=5/6\lambda = 5/6. The body at 11 has acceleration −1+1/4=−3/4-1 + 1/4 = -3/4, which forces λ=−9/4\lambda = -9/4. No single λ\lambda works, so the configuration is not central.

These configurations give solutions of the n-body problem in which the shape stays similar to itself. In the plane, a rigid rotation with angular speed λ\sqrt{\lambda} about cc is a solution, called a relative equilibrium.

Reading path

To understand this page from the ground up, read these 50 pages in order. The foundations come first.

  1. Derivative concept
  2. Differential equation concept
  3. Euclidean space object
  4. Euclidean vector concept
  5. First integral concept
  6. Function concept
  7. Hamiltonian system concept
  8. Interval concept
  9. Ordinary differential equation concept
  10. Velocity concept
  11. Fréchet derivative definition
  12. Cross product definition
  13. Ordinary differential equation definition
  14. Function of several variables concept
  15. Vector-valued function concept
  16. Classical mechanics concept
  17. Lipschitz condition definition
  18. n-body problem problem
  19. Limit of a function of several variables concept
  20. Momentum concept
  21. Double integral concept
  22. Partial derivative concept
  23. Solution of an ordinary differential equation definition
  24. Inertial frame of reference concept
  25. Continuity in R^n definition
  26. Differentiable function of several variables definition
  27. Partial derivative definition
  28. Triple integral concept
  29. Initial value problem definition
  30. Newton's laws of motion statement
  31. Differentiable on an open set definition
  32. Gradient definition
  33. Higher partial derivatives definition
  34. Centre of mass concept
  35. Picard–Lindelöf hypotheses definition
  36. Iterated derivative definition
  37. Picard operator definition
  38. C^k function characterised by continuous derivatives statement
  39. Integral equation form of an initial value problem statement
  40. An iterate of the Picard operator is a contraction statement
  41. Vector field definition
  42. Picard–Lindelöf theorem statement
  43. Conservative vector field definition
  44. Classical mechanics definition
  45. Momentum definition
  46. Potential energy definition
  47. Angular momentum definition
  48. Central force definition
  49. Newton's law of universal gravitation statement
  50. Central configuration definition

Further reading

  1. Web https://en.wikipedia.org/wiki/Central_configuration
About this page
Tag7ZMAJ5RBEY
URIm2://7ZMAJ5RBEY
Kinddefinition
WritingW0 stub
MSC70F10, 70F15
DefinesCentral configuration
Usesn-body problem, Centre of mass, Newton's law of universal gravitation
Changed3 November 2026

Markdown · JSON · Edit on GitHub

What this page needs for W1

  • an inventory row: the row of the inventory that the node accounts for (0 of 1)
  • a source with a locator (0 of 1)

The writing levels say how complete the text of a page is. They do not measure its truth.

What links here

No page links to this page yet.