Algol or the Demon star is a star in the constellation Perseus.
It has an apparent magnitude (as seen from Earth) of 2.12 or an absolute magnitude of -0.15.
See related link for more information.
The absolute magnitude is -7.92
-6.02
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.
Brightness of stars (apparent and absolute magnitude) is measured by convention, taking an another star as a standard.
No, a star's absolute magnitude is a measure of its intrinsic brightness regardless of its distance from the observer. It is a standardized measure that allows for comparison of the brightness of stars at a set distance.
the brightness of a star
The absolute magnitude is -7.92
Absolute Brightness .
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.
If you mean infinite brightness, then nothing.
A fixed star, in Medusa's head, in the constellation Perseus, remarkable for its periodic variation in brightness.
-6.02
Energy output, as absolute brightness (magnitude) is taken at a standard distance of 10 parsecs.
Algol is a binary star system composed of two stars orbiting each other. The dimming and brightening of Algol occur when the dimmer star passes in front of the brighter star from our point of view, resulting in an eclipse. This regular change in brightness is known as an eclipsing binary system.
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.