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
A spectral line refers to the distinct lines in a spectrum that correspond to specific wavelengths of light emitted or absorbed by atoms or molecules. For example, astronomers analyze the spectral lines of distant stars to determine their composition and temperature.
Large cool stars are classified as either K or M type stars on the spectral classification scale, with M stars being cooler and redder than K stars. These stars are part of the main sequence on the Hertzsprung-Russell diagram and have surface temperatures lower than 5,000 K.
Gliese does not have a specific color as it is a designation for a star within the Gliese catalog of nearby stars. The color of a star is determined by its temperature, with hotter stars appearing bluer and cooler stars appearing redder.
They are the same.
spectral analysis of light of stars help us
Large cool stars are classified as either K or M type stars on the spectral classification scale, with M stars being cooler and redder than K stars. These stars are part of the main sequence on the Hertzsprung-Russell diagram and have surface temperatures lower than 5,000 K.
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.
Gliese does not have a specific color as it is a designation for a star within the Gliese catalog of nearby stars. The color of a star is determined by its temperature, with hotter stars appearing bluer and cooler stars appearing redder.
Distant Stars was created in 1981.
Distant Stars has 352 pages.
The distance to nearby stars can be measured using the parallax effect. Astronomers observe the apparent shift in position of a star against the background of more distant stars as the Earth orbits the Sun, allowing them to calculate the star's distance based on the angle of the shift.
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.
Nearby stars appear to change their position against the distant background in an annual cycle, because of the Earth's changing position 'across' its orbit. This apparent shift is called the star's "parallax".
Spectroscopy is the systematic study of spectra and spectral lines. Spectral lines are used to provide evidence about the chemical composition of distant objects. So the answer to your question is through spectroscopy.. not spectrometry like the previous editor posted.