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.
A star's lifetime depends on its mass. More massive stars have shorter lifetimes, burning through their fuel faster, while less massive stars have longer lifetimes. Additionally, the composition of a star determines how it burns its fuel and influences its lifetime.
The main-sequence lifetime is a phase in a star's life when it fuses hydrogen into helium in its core. This phase typically lasts about 90% of a star's total fusion lifetime. After the main sequence, a star may continue to fuse other elements, depending on its mass, which will determine the total duration of its fusion lifetime.
an o-type blue star has a less length life than a g-type sun like star, this is because a the larger, hotter star, (the o-type blue star) uses its fuel (converting hydrogen into oxygen) quicker, so the correct answer to your question is the o-type blue star.
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.
The star 61 Cygni B is estimated to have a main sequence lifetime of approximately 10 billion years.
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.
A star's main fuel during its lifetime is hydrogen. Through nuclear fusion processes in the star's core, hydrogen is converted into helium, releasing vast amounts of energy in the form of light and heat. This fusion process sustains the star's energy output and keeps it shining bright.
The mass of the star. The bigger it is, the faster it will burn through its fuel supply.
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.