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The main fuel for stars is hydrogen.
When a Star runs out of fuel, it will expand into what is known as a "Red Giant". Massive stars will become "Red Supergiants". This phase will last until the star exhausts its remaining fuel. At this point, the pressure of the nuclear reaction is not strong enough to equalize the force of gravity and the star will collapse. Go to related link to read more about Stars... ;)
Yes we can say, life span of small stars are slower than bigger one because in the small star the nuclear fusion takes place at the moderate rate but massive stars require large amount of energy and therefore nuclear fusion consume all it's fuel in short Time As compare to small stars also mechanism of nuclear fusion in both case followed by different ways
The primary fuel for all stars is hydrogen
Massive stars evolve the fastest.Massive stars must supply more energy to prevent collapse under their own gravity. This energy is supplied by the nuclear reactions in the core of the star. more massive stars need to burn their nuclear fuel at a much greater rate than smaller stars in order to produce enough energy to balance their much greater gravity. Therefore, massive stars will burn their fuel faster and quicker evolve from their position on the main sequence
The main fuel for stars is hydrogen.
When stars "age", they spend their fuel source in a nuclear reaction (usually nuclear fusion).
The next possible nuclear fuel is actually Thorium, but will likely remain Uranium
In the nucleus of the fuel material, such as uranium-235
This part is the core of the nuclear reactor containing the nuclear fuel.
In nearly all stars, hydrogenis the most abundant element and it is consumed in a nuclear reaction that power stars.
Most stars process Hydrogen using nuclear fusion and turn it into Helium.
No, stars with the most hydrogen have the shortest lives. The more massive a star is, the faster it burns its fuel, and the sooner the core is depleted.
Nuclear fuel is the fuel used to produce nuclear energy.
The stars are powered by nuclear fusion, so this is widespread. Nuclear fission is more unusual and probably only occurs in certain planets where there is a lot of uranium.
When they run out of thermonuclear fuel in their cores. What fuel this would be varies, as more massive stars can fuse heavier elements. The absolute upper limit is iron, as fusing it absorbs energy.
Some massive stars reach a supernova state once they have exhausted all their nuclear fuel.