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What actually happens to the types of stars is that the low mass will turn into a white dwarf and the medium mass will turn into a black dwarf and reproduce a nebula
Mass decides a stars ultimate fate.
Mass. Higher mass stars, while having more fuel to burn, counterintuitavely have shorter lifespans, as they are able to bring more of that mass to temperatures capable of supporting fusion.
Yes, all stars run on a limited suppliy of fuel - mainly hydrogen. Some stars burn it very quickly but reach high temperatures, while other lower mass stars burn their fuel more slowly, lasting for longer, but burn at cooler temperatures.
In order to prevent stars collapsing under their own gravity, some outward pressure must exist. this is supplied by the energy released by 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. the difference in required reaction rates is actually greater than the difference in mass, consequently the more massive a star is, the faster it expends its fuel.
White dwarf. High mass stars become neutron stars or black holes.
What actually happens to the types of stars is that the low mass will turn into a white dwarf and the medium mass will turn into a black dwarf and reproduce a nebula
What actually happens to the types of stars is that the low mass will turn into a white dwarf and the medium mass will turn into a black dwarf and reproduce a nebula
Stars with a huge mass will consume its fuel faster. in the end it becomes a supernova and soon after (in star-time) it will implode. Depending on its mass, it might become a super-massive black hole or a little dwarf where only one teaspoon of its mass will weigh in at many tons.
Exactly what happens depends on the mass of the star. Low mass stars first expand into giants, then shrink to white dwarfs. Stars with a little more mass than the Sun end up as neutron stars; stars with considerably more mass with the sun end up as black holes.
When the star runs out of fuel. Most stars burn (fuse, actually) hydrogen. When this runs out, what happens next depends on the mass of the star... heavier stars can fuse heavier elements for a short time, but lower mass stars simply collapse into white dwarfs.
Stars with more than about 80% of the Sun's mass behave like the Sun. They should eventually become red giant stars then white dwarf stars. Stars with mass of between about 8% and 80% of the Sun's mass are red dwarf stars. Below that come the "brown dwarfs, which aren't really true stars at all. The red dwarfs cannot fuse helium, so they simply become "white dwarf" stars when they have used up all their hydrogen "fuel".
The more the mass the shorter their life cycle (the more quickly they use their fuel)
Mass decides a stars ultimate fate.
The size (diameter) of a star can change over its lifetime; sometimes within hours.What really matters is the star's MASS. The most massive stars will produce a lot of radiation, and thus use up their fuel very quickly. After that: Stars up to about 1.4 solar masses will end up as white dwarves. Above that, stars up to somewhere between 2 and 3 solar masses will end up as neutron stars. Above that, stars end up as black holes. The "mass" refers to whatever mass remains once the star uses up its fuel. For instance, a supernova explosion may remove a large part of the star's mass. Likewise, massive stars may lose a lot of mass during their lifetime, through their stellar wind.
Low, medium, or high what, exactly? The Sun is estimated to be around percentile 85 with respect to brightness. That means that some stars are brighter than the Sun, but 85% of all stars are less bright than the Sun. I guess the situation with mass would be similar, since brightness greatly depends on mass.
Stars with less mass live much longer. Stars with greater mass get hotter, and have more pressure in their core; as a result, they use up their fuel much faster.