The → total → brightness of a star or other astronomical object.
It is expressed in watts and represents the total amount of
→ energy that the object radiates each
→ second over all
wavelength regions of the → electromagnetic spectrum.
Because this quantity is independent of distance, it is an
→ intrinsic brightness.
See also:
→ absolute luminosity,
→ anomalous luminosity effect,
→ bolometric luminosity,
→ color-luminosity diagram,
→ Eddington luminosity,
→ H II region luminosity,
→ intrinsic luminosity,
→ luminosity class,
→ luminosity distance,
→ luminosity function,
→ luminosity problem,
→ luminosity-size relation,
→ mass-luminosity ratio,
→ mass-luminosity relation,
→ peak luminosity,
→ period-luminosity relation,
→ solar luminosity,
→ stellar luminosity,
→ wind luminosity.
See also: Verbal noun of → luminous.