A star's "absolute magnitude" is a measure of its absolute (or real) brightness.
It is defined as the "apparent magnitude" the star would have at a standard distance of 10 parsecs, which is equal to 32.6 light years.
Depending on the type of supernova it can reach an absolute magnitude of −19.3 (or 5 billion times brighter than the Sun)
Quite low. Neutron stars are the crushed stellar "ash" that used to be a real star. They don't radiate much light, and are essentially invisible except for their gravity.
Apparent magnitude and absolute magnitude.
The term is "absolute magnitude".
Red giants.
No; the "magnitude" is how bright the star is. It can either mean:* The apparent magnitude = how bright it seems to us, * The absolute magnitude = how bright the star really is (i.e., how bright it would seem at a standard distance).
Apparent magnitude is the brightness of an object as seen from Earth without any atmosphere.Absolute magnitude is the brightness of an object as seen from a predetermined distance, depending on the object.For planets, the distance used is 1 AU (Astronomical Units). Stars and galaxies use 10 parsecs which is about 32.616 light years.The dimmer an object is the higher the positive value. The brighter an object is the higher the negative value.Examples:The Sun has an apparent magnitude of -26.74 but an absolute magnitude of 4.83Sirius has an apparent magnitude of -1.46 but an absolute magnitude of -1.42This means that from Earth, the Sun is a lot brighter, but if the Sun was replaced by Sirius, Sirius would be 25 times more luminous.See related links for more information
Constellations don't have an absolute magnitude. That is a property of individual stars.
The question is: Why is the apparent magnitude of some stars less than their absolute magnitude. Or: Why do some stars not look as bright as they really are ? The answer is: Because they're so far away from us.
The absolute magnitude is a measure of the star's luminosity hence the smaller the size the less the absolute magnitude.
Absolute magnitude
Apparent magnitude and absolute magnitude.
Most "yellow" stars fall into the classification of type G - the same as our Sun.They have an absolute magnitude of around 5.
Its absolute magnitude is -1.20.Its magnitude from our point of view is +3.65.
Absolute magnitude: they are extremely bright. Temperature: their surface temperature is fairly low.
The term is "absolute magnitude".
It is actually absolute magnitude, opposed to apparent magnitude which is how much light stars appear to give off.
The apparent magnitude is how bright the star appears to us, but stars are all at different distances so that a star that is really bright might look dim because it is very far away. So the absolute magnitude measures how bright the star would look if it was placed at a standard distance of 10 parsecs. When the absolute magnitude is greater than the apparent magnitude, it just means that it is closer than 10 pc. The brightest stars have absolute magnitudes around -7.
Mass and age.