Galaxies: Types, Structure & Evolution

Tully-Fisher relation

/ TUH-lee FISH-er /

Here is a beautifully simple rule of thumb astronomers stumbled on: the faster a spiral galaxy spins, the brighter it is. Big bright spirals whirl fast; small dim ones turn slowly. This tight link between a spiral's rotation speed and its total luminosity is the Tully-Fisher relation, discovered by Brent Tully and Richard Fisher in 1977.

Quantitatively, a galaxy's luminosity climbs roughly as the fourth power of its rotation speed — double the rotation speed and the galaxy is something like sixteen times brighter. The rotation speed is easy to measure even for a faraway galaxy: the spinning gas broadens the galaxy's 21-centimeter radio line (or its optical lines), and the width of that line tells you how fast the disk turns, no matter how far away it is. The relation works because rotation speed traces total mass (mostly dark matter), and more massive galaxies hold more stars and so shine brighter — luminosity and mass march together.

The Tully-Fisher relation matters as a distance tool. Measure a spiral's rotation speed from its line width, and the relation hands you its true luminosity; compare that to how bright it looks, and the inverse-square law gives the distance — a standard-candle trick that reaches galaxies far beyond Cepheids. It is a key rung of the cosmic distance ladder and was historically important in measuring the expansion of the universe. Its tightness is also a clue that visible galaxies and their dark halos are deeply coupled.

Suppose a distant spiral's 21-cm line width says it rotates at about 220 km/s, the same as the Milky Way. Tully-Fisher then predicts a luminosity close to the Milky Way's; comparing that to how faint it appears yields a distance with no need to resolve individual stars.

Spin width in, true brightness out — a spiral becomes its own measuring rod.

Tully-Fisher works for rotating spirals, not for ellipticals, which lack orderly rotation; the elliptical counterparts are the fundamental plane and the Faber-Jackson relation. It also needs careful correction for the galaxy's tilt and for dust dimming.

Also called
TF relationTFR塔利-费希尔关系塔利-費希爾關係