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.
High mass.
The major difference is that a low-mass star lives much longer. The reason for this is that a high-mass star gets hotter, is much brighter, and uses up its fuel much faster. The difference can be quite dramatic, with some stars being millions of times brighter than others. Also, assuming the star doesn't acquire additional mass, a low-mass star will end up as a white dwarf, while more massive stars will end up as a neutron star, or in the case of the most massive stars, a black hole.
The color of a star is mainly related to the star's surface temperature. This is only remotely related to the star's mass; for example, high-mass stars can either be very hot (blue) or not-so-hot (red), depending on the phase in the star's life.
The mass of a star affects the lifespan of the star. The less the mass, the longer life span of the star. More massive stars burn up their fuel more quickly than the smaller stars. As the massive stars begin to burn the fuel and become smaller, the life span increases.
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.
High mass.
A high-mass star will use up its fuel faster than a low-mass one. Depending on the amount of mass that remains at the end of its life, it may convert to a neutron star, or to a black hole.
The life span of a star is determined by its mass. More massive stars burn through their fuel faster and have shorter life spans, while less massive stars have longer life spans. The life span of a star can be estimated using the mass-luminosity relation and the star's initial mass.
The Sun is a medium mass star in main sequence.
The major difference is that a low-mass star lives much longer. The reason for this is that a high-mass star gets hotter, is much brighter, and uses up its fuel much faster. The difference can be quite dramatic, with some stars being millions of times brighter than others. Also, assuming the star doesn't acquire additional mass, a low-mass star will end up as a white dwarf, while more massive stars will end up as a neutron star, or in the case of the most massive stars, a black hole.
The major difference is that a low-mass star lives much longer. The reason for this is that a high-mass star gets hotter, is much brighter, and uses up its fuel much faster. The difference can be quite dramatic, with some stars being millions of times brighter than others. Also, assuming the star doesn't acquire additional mass, a low-mass star will end up as a white dwarf, while more massive stars will end up as a neutron star, or in the case of the most massive stars, a black hole.
The major difference is that a low-mass star lives much longer. The reason for this is that a high-mass star gets hotter, is much brighter, and uses up its fuel much faster. The difference can be quite dramatic, with some stars being millions of times brighter than others. Also, assuming the star doesn't acquire additional mass, a low-mass star will end up as a white dwarf, while more massive stars will end up as a neutron star, or in the case of the most massive stars, a black hole.
The major difference is that a low-mass star lives much longer. The reason for this is that a high-mass star gets hotter, is much brighter, and uses up its fuel much faster. The difference can be quite dramatic, with some stars being millions of times brighter than others. Also, assuming the star doesn't acquire additional mass, a low-mass star will end up as a white dwarf, while more massive stars will end up as a neutron star, or in the case of the most massive stars, a black hole.
The major difference is that a low-mass star lives much longer. The reason for this is that a high-mass star gets hotter, is much brighter, and uses up its fuel much faster. The difference can be quite dramatic, with some stars being millions of times brighter than others. Also, assuming the star doesn't acquire additional mass, a low-mass star will end up as a white dwarf, while more massive stars will end up as a neutron star, or in the case of the most massive stars, a black hole.
A high mass star will leave behind either a neutron star of a black hole.
High mass.
no the sun is a medium mass star.