The reddest stars are the stars that are considered the coolest. Blue light is more effectively scattered than Red light. This is called ``interstellar reddening".
spectral analysis of light of stars help us
Doug Fany answer: Parallax
Astronomers use a method called parallax to measure the distance to nearby stars. Astronomers can measure parallax by measuring the position of a nearby star with respect to the distant stars behind it. Then, they measure the same stars again six months later when the Earth is on the opposite side of its orbit.
They are the same.
Spectral analysis.
spectral analysis of light of stars help us
Doug Fany answer: Parallax
Astronomers use a method called parallax to measure the distance to nearby stars. Astronomers can measure parallax by measuring the position of a nearby star with respect to the distant stars behind it. Then, they measure the same stars again six months later when the Earth is on the opposite side of its orbit.
There are stars with spectral classes of O & B (e.g. Rigel) R136a1 is a star of the spectral class WN5h. Wolf Rayet stars have this kind of spectral type.
Typically the bigger and redder stars are the hottest.
No. K spectral type stars (which are orange) temperature is ranging from 5,000-3,500. A spectral type stars (which are blue-white) temperature is ranging from 7,500-11,000.
They are the same.
Distant Stars was created in 1981.
Distant Stars has 352 pages.
Actually, it doesn't matter what kind of galaxy it is, because it depends on what kind of stars are in it. If a galaxy has a lot of red giants, it will appear redder than a galaxy with mostly blue-white stars. Older galaxies might be redder than younger galaxies due to the fact that older stars appear redder.
Spectral class Y, which is typical of "brown dwarf" stars.
Spectral analysis.