First let's assume the question is about a star's actual brightness not apparent brightness as seen from Earth.
There are in fact several possibilities.
The Hertzprung-Russell diagram is helpful here.
One possibility is red dwarfs and white dwarfs.
Of course there's large variation within these groups, but a red dwarf can certainly have a luminosity that's similar to a white dwarf.
If the question is about apparent brightness, then a distant luminous star can appear similar in brightness to a nearby faint star.
Blue Supergiants and Supergiants
Two ways are by temperature and brightness
Apparent magnitude and absolute magnitude.
No. Brighter distant stars can have the same apparent magnitude as fainter stars that are closer.(Absolute magnitude does not refer to actual brightness, but rather to what the brightness of a star would likely be at an arbitrary distance of 10 parsecs, rather than its actual distance.)
Alpha Centauri and the sun
Blue Supergiants and Supergiants
Two ways are by temperature and brightness
Two ways are by temperature and brightness
Apparent magnitude and absolute magnitude.
false
Their distance away from you and their intrinsic luminosity.
Two stars revolving around one another (around their center of mass, to be precise) are called a "binary star". There is no special name for the case that the brightness is unequal; this is actually the usual case.
Two factors that affect a star's apparent brightness are: 1.) The distance between the Earth and the star 2.) The absolute magnitude (the actual brightness) of the star Hope that helps :P
Yes. The prefix bi- means two.
No. Brighter distant stars can have the same apparent magnitude as fainter stars that are closer.(Absolute magnitude does not refer to actual brightness, but rather to what the brightness of a star would likely be at an arbitrary distance of 10 parsecs, rather than its actual distance.)
U.o.e.n.o it
About 97.7 (calculated as 2.55)