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Nuclear Fusion in a Giant Star involves Helium being fused into a hydrogen shell that surrounds the core, and Nuclear Fusion in a Main-Sequence star involves Hydrogen being fused into Helium to produce Energy inside of the core.

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8y ago
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6y ago

It is a fact that while a star plots on the main sequence line of the Hertzsprung-Russelldiagram, it is fusing the element HYDROGEN into the element helium to produce its energy output. The actual size of the star does not matter, the bigger stars just produce more energy than the smaller ones but they all sit on the main sequence line (just at opposite ends of it).

Once the star runs out of hydrogen in its core, the core shrinks further under gravity and gets hotter and denser and it reaches a point that causes the helium that it made earlier to fuse into heavier elements. This HELIUM fusion produces even more energy and the plot of the energy output profile is now no longer on the main sequence line. The extra energy makes the outer layers of the star inflate and the star enters it "giant" phase.

The larger the star, the less time it spends on the main sequence line because the larger it is the faster it fuses its hydrogen.

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12y ago

Fusion is much faster in giant stars causing them to burn out faster.

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Q: How does fusion differ for high mass stars and low mass stars?
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Related questions

How do stars convert mass to energy?

Nuclear Fusion


What is the fuel that runs fusion in stars?

Initially it is hydrogen. When that is spent, stars move to fusion of helium. There are also other fusion processes which take place: which process depends on the stars' mass.


What is the fuel the runs fusion in stars?

Initially it is hydrogen. When that is spent, stars move to fusion of helium. There are also other fusion processes which take place: which process depends on the stars' mass.


What is the differences between the main sequence stages for high and low mass stars?

(study island answer= all of these statements are true) Stars with masses less than 1.6 × 1029 kg become brown dwarfs because they are unable to reach high enough temperatures for hydrogen fusion to take place. Extremely massive stars are able to produce supernovas, or stellar explosions, when they cease to undergo nuclear fusion or when they undergo a sudden gravitational collapse. Low-mass stars develop more slowly than more massive stars; their lifetimes can last trillions of years as opposed to only a few million years.


What do high mass stars and low mass stars have in common?

They produce light.


What atoms powers the sun and other stars?

The fusion of atoms powers the sun and other stars


Materials of low mass fused together?

This is fusion not fission. In stars like our sun, hydrogen is turned into helium


Which stars have convective cores?

High-mass stars


What triggers nuclear fusion stars?

Fusion in stars are usually the result of gravity.Once a mass of hydrogen accumulates enough mass, the gravity of all that mass compresses the core of the star to the point that the hydrogen atoms there begin fusing into helium. The process then cascades outward, and the end result is a star.


What is made when stars die?

There are three types of stellar remnants. Low to medium mass stars will become white dwarfs. High mass stars will become neutron stars. Very high mass stars will become black holes.


What are both high mass and low mass adult stars classified as?

Main Sequence Stars


How do the numbers of low-mass stars compare with those of higher-mass stars in new star clusters?

In a newly formed star cluster stars with low masses must greaty out number stars with high masses. High mass stars are rare and low mass stars are extremely common.