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The Sun lies near the middle of the main sequence.
In a young cluster the main sequence will be well-populated, but in an old cluster the heavier stars will have evolved away from the main sequence.
The star then reaches the main sequence, where it remains for most of its active life.
This spread is produced by stellar evolutionary effects and tends to broaden the main sequence.
The extent of the depopulation of the main sequence provides an index of age.
The giants lie above the main sequence in the upper right portion of the diagram.
As it continues to contract, it moves downward and to the left toward the main sequence.
By the time the star reaches the main sequence, it is still chemically homogeneous.
The white dwarf domain lies about 10 magnitudes below the main sequence.
Similar(2)
The majority of stars on a typical HR diagram lie along the main-sequence curve.
This forms a "knee" in the HR diagram, bending to the upper right from the main-sequence line.
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