If you mean infinite brightness, then nothing.
The variable of distance is eliminated when discussing absolute brightness. Absolute brightness specifically refers to the inherent brightness of an astronomical object without the influence of its distance from the observer.
the brightness of a star
The absolute magnitude is -7.92
Absolute Brightness .
-6.02
Energy output, as absolute brightness (magnitude) is taken at a standard distance of 10 parsecs.
Stellar brightness refers to the amount of light emitted by a star as perceived from Earth, often quantified in terms of apparent magnitude and absolute magnitude. Apparent magnitude measures how bright a star appears from our viewpoint, while absolute magnitude represents its intrinsic brightness at a standard distance of 10 parsecs. Factors such as distance, size, temperature, and composition influence a star's brightness. Understanding stellar brightness helps astronomers categorize stars and study their properties and distances.
A star's brightness at a standard distance is referred to as its apparent magnitude. This standard distance is 10 parsecs (32.6 light-years) from Earth. Apparent magnitude allows astronomers to compare the brightness of stars as seen from Earth, regardless of their actual distance from us.
Anything that is not the measure of intrinsic brightness of a celestial object.
Absolute Brightness: How bright a star appears at a certain distance. Apparent Brightness: The brightness of a star as seen from Earth.
To compare the absolute brightness of star X with star Y, we need to know their distances from Earth and their intrinsic luminosities. Absolute brightness, or absolute magnitude, refers to how bright a star would appear at a standard distance of 10 parsecs. If we have both stars' absolute magnitudes, we can directly compare them; otherwise, we cannot accurately assess their brightness without additional information about their distances and luminosities.
The absolute magnitude of the main star in the Polaris system is -3.6