The Sun is classified as a main sequence star on the Hertzsprung-Russell diagram.
Main sequence stars, also known as dwarf stars, are the most common type of star in the universe. They are characterized by fusing hydrogen in their cores to produce energy. Main sequence stars are further classified into different spectral types, from O being the hottest and brightest to M being the coolest and dimmest. The Sun, being a G-type main sequence star, falls in the middle of this range.
The Sun is not classified as a supergiant star. Supergiants are extremely massive and luminous stars that are much larger than main sequence stars. They occupy the upper-right region of the Hertzsprung-Russell diagram.
Similarly, the Sun is not classified as a giant star. Giants are also more massive and luminous than main sequence stars but are smaller than supergiants. Giant stars are found in the upper-right region of the Hertzsprung-Russell diagram, just below the supergiants.
Lastly, the Sun is not classified as a white dwarf star either. White dwarfs are the remains of lower-mass stars that have exhausted their nuclear fuel. They are small and dense objects, typically about the size of Earth but with a mass similar to that of the Sun. White dwarfs are located in the lower-left region of the Hertzsprung-Russell diagram.
how is the sun classified on an hertzsprung russell diagram
as a main sequence star
as a supergiant star
as a giant star
as a white dwarf star
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