Remnants of low mass stars include white dwarfs, neutron stars, and black holes, depending on the mass of the original star. White dwarfs are remnants of stars similar in mass to our Sun, while neutron stars and black holes are remnants of more massive stars. These remnants are formed after the star exhausts its nuclear fuel and undergoes a supernova explosion.
When a star dies, it can leave behind different types of stellar remnants depending on its mass. Some examples include white dwarfs, neutron stars, and black holes. White dwarfs are formed from the remnants of low to medium mass stars, neutron stars are formed from the remnants of massive stars, and black holes are formed from the remnants of the most massive stars.
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.
A collapsed star after using up its fuel is called a white dwarf, neutron star, or black hole, depending on its mass. White dwarfs are remnants of low to medium mass stars, neutron stars are remnants of massive stars, and black holes are formed when very massive stars collapse.
A collapsed star after using its fuel is called a white dwarf, neutron star, or black hole, depending on its mass. White dwarfs are remnants of low to medium-mass stars, while neutron stars are remnants of massive stars. Black holes are formed from the most massive stars and have gravitational pull strong enough to trap even light.
Massive stars become neutron stars, or black holes (depending on how much mass is left at the end of a star's lifetime).
White dwarfs are the remnants of dead low to medium mass stars, which is the mass range of the majority of stars.
When a star dies, it can leave behind different types of stellar remnants depending on its mass. Some examples include white dwarfs, neutron stars, and black holes. White dwarfs are formed from the remnants of low to medium mass stars, neutron stars are formed from the remnants of massive stars, and black holes are formed from the remnants of the most massive stars.
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.
A collapsed star after using up its fuel is called a white dwarf, neutron star, or black hole, depending on its mass. White dwarfs are remnants of low to medium mass stars, neutron stars are remnants of massive stars, and black holes are formed when very massive stars collapse.
Neutron stars and black holes.
A collapsed star after using its fuel is called a white dwarf, neutron star, or black hole, depending on its mass. White dwarfs are remnants of low to medium-mass stars, while neutron stars are remnants of massive stars. Black holes are formed from the most massive stars and have gravitational pull strong enough to trap even light.
Massive stars become neutron stars, or black holes (depending on how much mass is left at the end of a star's lifetime).
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.
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.
They produce light.
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.
Low and medium sized stars will end up as white dwarfs.