Why can changes in a quasar's brightness reveal its small size?
Shown are apparently normal, solitary galaxies (left), colliding galaxies (centre), and merging galaxies (right).
The observation that a quasar can change its brightness significantly over a short periodâsuch as a few daysâprovides a direct constraint on its physical size.
Because nothing can travel faster than the speed of light, a change in brightness across the entire object cannot occur faster than the time it takes for light to travel across it. If a quasarâs luminosity fluctuates on a timescale of a few days, the region producing that light cannot be larger than a few light-days across. This indicates that the energy-emitting region is extremely compact, roughly the size of our solar system, despite the object's immense luminosity.1