Modified Newtonian dynamics — where it appears
Named by 2 essays across one field — each of them below, with the objects they name alongside it.
Also named here as radial acceleration relation — the same set of essays touches all of them, so they are one junction rather than several.
One acceleration, and every galaxy's missing mass
Plot the acceleration measured at each radius of a rotation curve against the acceleration its stars and gas would produce there, for every galaxy at once, and the points fall on a single curve. Where the discrepancy begins is set not by a radius or a mass but by an acceleration.
A galaxy born without a halo
When two galaxies collide, some of the gas flung out along their tidal tails condenses into new dwarf galaxies. Debris launched from a disc cannot take the dark halo with it, so these dwarfs should rotate at the speed their own gas and stars allow and no faster. The relation that predicts every ordinary galaxy's rotation from its baryons says they should rotate twice as fast. One rotation curve decides between a halo and a law — except that the inclination of a lumpy young disc can move the answer by more than the difference.
Named alongside it
The objects these essays reach for when they reach for this one.
Dark matter haloRadial acceleration relationRotation curveBaryonThe baryonic Tully–Fisher relationDynamical massEscape velocityFeedbackGalaxy interactionInclinationMass discrepancyTidal tail