The absolute magnitude is the magnitude (brightness) an object would have at a standard distance - how bright would it look at a standard distance. For a star or galaxy, the standard distance of 10 parsecs is commonly used.
You look at the color of the light of the star and the "fraunhofer lines" which are teltale signs of the star's composition. You compare with theoretical models and other known stars of similar make-up, you thereby can know how bright it really shines (it's absolute magnitude)
M = m - 5 ((log10 DL) - 1)
For very large distances, redshift complicates might require a correction.
In astronomy, absolute magnitude measures a celestial object's intrinsic brightness as if all where viewed from the same distance. This distance is set at 1 AU for our Solar System. For greater distance's, galaxies etc. the value is 32.616 light years.
So our Sun has an Apparent magnitude (As viewed from Earth) of -26.74 (Negative values are the brightest) but it has an absolute magnitude of +4.83. Sirius for comparison has an absolute magnitude of +1.42 so would appear brighter if viewed from the same distance.
You can't because you don't have enough information. The difference between the star's
absolute magnitude and apparent magnitude depends on its distance from earth.
The absolute magnitude is a measure of the star's luminosity hence the smaller the size the less the absolute magnitude.
distance from earth
The absolute magnitude of Porrima is 3.04.
-3.64 is the absolute magnitude of Polaris.
VY Canis Majoris has an absolute magnitude of -9.4.
The absolute magnitude is a measure of the star's luminosity hence the smaller the size the less the absolute magnitude.
Apparent magnitude is the measure of how bright a star appears to be from our vantage point. Absolute magnitude is the measure of how bright a star would be if it were located 10 parsecs from earth.
Absolute magnitude and apparent magnitude are the same because they are both ways on how to measure the brightness of a star. Absolute magnitude is how bright is the star if we will see it in a 32.616 light-years distance while apparent magnitude is the brightness of it that we see on Earth.
distance from earth
You can measure it by using absolute magnitude.
Antares Absolute and Apparent Magnitude Absolute Magnitude~ -5.2 Apparent Magnitude~ +0.60
Meaning:A measure of how bright a star would be if it were seen from a standard distance.Sentence:The sun's Absolute Magnitude is 4.8.
No. The sun has an absolute magnitude of 4.83. By comparison, Betelgeuse has an absolute magnitude of -5.85. Lower numbers indicate a brighter star. In this case Betelgeuse is actually several thousand times brighter than the sun. The sun is the brightest star as measure by apparent magnitude, which is how bright a star looks from a given location and depends on both absolute magnitude and distance.
Its absolute magnitude is -7.92
The absolute magnitude of Porrima is 3.04.
The absolute magnitude of Betelgeuse is -6.05
Absolute magnitude refers to a measure of the real brightness of a star. In terms of absolute magnitude, a blue-violet star is classified as bright, while an orange-red star is classified as faint.