Between about 8 and 100 times the mass of the Sun.
Most stars fall within a mass range of approximately 0.1 to 100 times the mass of our Sun. This range includes most of the stars in the universe, from low-mass stars like red dwarfs to high-mass stars like blue giants.
High mass stars have a faster rate of burning compared to low mass stars. This is because high mass stars have more gravitational pressure in their cores, leading to faster nuclear reactions and higher energy output. This results in a shorter lifespan for high mass stars compared to low mass stars.
There are more low mass stars. this is for two reasons:- # the star forming process generates more low mass stars # High mass stars burn out very quickly and explode as supernovas and thus over time there are less and less of them.
They produce light.
Low and high mass stars are indirectly related; high mass stars evolve faster and have shorter lifespans compared to low mass stars. This is because high mass stars burn through their fuel at a faster rate due to their higher core temperature and pressure.
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.
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.
High mass adult stars are classified as supergiants or giants, while low mass adult stars are classified as main sequence stars. This classification is based on the mass of the star and where it falls on the Hertzsprung-Russell diagram.
White dwarfs are the remnants of dead low to medium mass stars, which is the mass range of the majority of stars.
high mass has shortest life (stars right?)
Stars are classified based on their mass, with low-mass stars typically having less than about 0.8 solar masses, while high-mass stars can exceed 8 solar masses. The sun has a mass of approximately 1 solar mass, serving as a reference point. Low-mass stars burn their fuel slowly and can have lifespans of billions of years, whereas high-mass stars burn quickly and may only last a few million years before ending their lives in supernovae.
High-mass stars might become black holes, if the remaining matter (after the supernova explosion) is sufficiently large.