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Through measuring how much luminosity it is giving out, measuring the size of the star, and find out how hot the star is, we can categorize each star in a graph. Our sun just happens to be part of the main sequence of stars; the sun is not as big as a giant or a super giant star nor is it as small as a white dwarf so therefore the sun is in between.

Main sequence stars are more common because they are very stable so it wont change over a long course of time, unlike variable stars, which changes its size and luminosity. A variable star has a period of a day to a month. A period is how long it takes for the star to return to its starting point as it changes in a cycle.

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