Star

Main Sequence Star

A stable star fusing hydrogen into helium in its core.

The longest, most stable phase of a star's life. The Sun is a G-type main sequence star. About 90% of all observed stars are on the main sequence.

Overview

The longest, most stable phase of a star's life. The Sun is a G-type main sequence star. About 90% of all observed stars are on the main sequence.

See also