What is the main sequence in stars?
The main sequence is a phase in a star's life where it fuses hydrogen into helium in its core.
How long do stars stay in the main sequence?
Stars can spend millions to billions of years in the main sequence, depending on their mass.
What happens after the main sequence?
After the main sequence, stars evolve into red giants or supergiants, depending on their mass.
Can you give examples of main sequence stars?
Sure! Our Sun is a G-type main sequence star, while Sirius is an A-type main sequence star.
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