A low-acceleration modification associated with Mordehai Milgrom. For an isolated spherical system, , with at high and at low . An isolated point-like baryonic distribution then gives and a flat asymptotic galaxy rotation curve. The algebraic spherical relation is not a complete relativistic field theory and should not be assumed to hold vectorially for arbitrary mass distributions.[ref]
Mordehai Milgrom Created 2026-10-20 Updated 2026-11-05
Mordehai Milgrom proposed modified Newtonian dynamics as an alternative explanation of the discrepancy between visible mass and inferred gravitational effects in galaxies. The modification becomes important below a characteristic acceleration scale .
In the low-acceleration spherical limit, . For a circular orbit, substituting gives , independent of orbital radius. The same limiting rule therefore links a flat outer galaxy rotation curve with a relation between baryonic mass and orbital speed. These are consequences of the proposed dynamics, not a direct detection of the underlying mechanism.[ref]
Figure 1.
Portrait of Mordehai Milgrom
. Weizmann Institute of Science; Commons permission record VRT 2010112110015191. Public-domain release by Weizmann Institute of Science, worldwide, via Wikimedia Commons. Source.