Absolute magnitudes of stars generally range from 10 to +17.

For the objects brighter than absolute magnitude 9.0 the population is probably complete.

With an absolute magnitude of 5.2, it is probably dwarf planet.

Absolute Magnitude is also a collection of sixteen stories taken from the magazine between 1993 and 1997.

However, in 1994 after only two issues the name was changed to Absolute Magnitude.

He also computed the absolute magnitude of the entire galaxy.

From another source the absolute magnitude is about 8.0.

The lower an object's absolute magnitude, the higher its luminosity.

This star is similar to our own Sun, being only slightly larger and brighter in absolute magnitude.

A single supemova can reach a maximum absolute magnitude of -17.

When the visual and absolute magnitudes are known, the distance to the star can be measured.

The absolute magnitudes of galaxies can be much lower (brighter).

In terms of gamma rays, the burst had an absolute magnitude around 29.

Reports indicate that the object is about 74 metres wide and has an absolute magnitude of 23.28.

The configurations will be entirely different, and Sol's absolute magnitude is not great.

The primary has an absolute magnitude of 2.6 and is of spectral class F0.

Its absolute magnitude was determined to be 11.5.

The term "significant" does not imply a judgment about the absolute magnitude or educational relevance of changes in student performance.

Absolute magnitude is a measure of a star's absolute brightness.

From this the star's absolute magnitude is estimated.

Its absolute magnitude - or intrinsic brightness - of 0.5 was the sixth highest in recorded history.

VB 10 has an extremely low luminosity with an absolute magnitude of nearly 19, making it very difficult to see.

Objects with well established orbits include (in order of the absolute magnitude):

The apparent magnitude is 8 and absolute magnitude is 4.

That is to say, it gives the approximate absolute magnitude of a vector given the real and imaginary parts.