For positive masses and distinct positions, Newtonian gravitational field gives
Insert with . The separation numerator contributes a factor and the denominator , so
Hence the time-dependent equations are satisfied whenever
The fixed-shape condition is a Newtonian central configuration, and the resulting motion is a homothetic gravitational motion. It applies away from the collision scale ; a negative scale would require absolute values in the force scaling rather than the same positive-scale formula.
Multiplying the scalar equation by gives
Thus its first integral is for some real constant .
In the pair potential
differentiating a pair with respect to produces . Every pair incident on contributes exactly once, so . Moreover for . Differentiating with respect to at one proves the relevant Euler homogeneous function theorem identity directly:
Dot each fixed-shape equation with and sum to obtain
For a nontrivial collision-free configuration with at least two positive masses, and , and therefore . Positivity requires an interacting pair; an isolated one-particle system is the degenerate zero-force exception rather than a positive- gravitational configuration. Pairwise cancellation also gives , so the nondegenerate configuration has : its scaling origin is the centre of mass.
Finally, the system's kinetic energy is and its potential energy is . Consequently
This establishes the energy relation for every fixed configuration satisfying the algebraic condition, without assuming any particular particle arrangement.

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