An O star will stay on the main sequence for millions of years whereas a M star can stay on the main sequence for billions and billions of years.
It depends on its size. Smaller stars- main-sequence, red giant, planetary nebula, white dwarf, black dwarf Bigger stars- main-squence, red giant, supernova, neutron star.
hydrogen
Stars spend about 90% of their fusion lifetimes on the main sequence.
No. The less massive a star, the longer it will last. A main sequence star half the mass of the sun can be expected to last about 5 times longer.
For most of a star's life, the main fuel is protium (hydrogen-1), which is fused into helium-4.
Roughly 90% of a star's total lifetime is spent on the main sequence, where it fuses hydrogen into helium in its core. After this stage, the star will evolve off the main sequence and follow a different path, such as becoming a red giant or a supernova.
On the main sequence.
10¹¹ years
MAIN-SEQUENCE The average star spends 90% of its life as a hydrogen burning MS star.
Not exactly: Star formation is believed to be a slow process, compared to a human lifetime; scientists have, however, seen stars in different phases of their formation.
The mass of the star. The bigger it is, the faster it will burn through its fuel supply.
When a star is at the end of its lifetime its mass increases.