Based on astronomical records, the reasons why there is main sequence are:
A star can be defined as a giant astronomical or celestial object that comprises a luminous sphere of plasma and it is bounded together by its own gravitational force.
Generally, a star is typically made up of two (2) main hot gases and these include the following:
A main sequence refers to a type of star that fuses hydrogen in its core and it has a stable balance of outward pressure as a result of core nuclear fusion and gravitational forces that are pushing inward.
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