Stars don't "burn" chemically like a fire.
The energy they release is obtained by fusing light elements into heavier elements.
In doing that they convert mass into energy as Einstein described with the equation E=mc2.
A high mass star explodes as a supernova, leaving behind a neutron star or a black hole. Neither of those is capable of nuclear fusion.
The small dense remains of a high-mass star are called neutron stars or black holes, depending on the mass of the star. Neutron stars are formed when the core collapses under its own gravity, while black holes are formed when the core collapses into a singularity.
A high mass star's core collapses when nuclear fusion ceases and gravitational pressure overwhelms the radiation pressure supporting the core. This collapse leads to a rapid increase in temperature and pressure, triggering a supernova explosion.
When a large star collapses in a supernova, it can produce either a neutron star or a black hole, depending on the mass of the original star. A neutron star forms when the core of the star collapses but the outer layers are ejected, while a black hole forms when the core collapses completely.
When a star collapses to half its size, its gravitational field at the surface increases. This is because the gravitational force is directly proportional to the mass of the star and inversely proportional to the square of the distance from the center of the object. As the star collapses, its mass remains the same but the distance to its center decreases, leading to a stronger gravitational field at its surface.
High mass.
Because all the material that could rekindle it has run out - there is none left.
The small dense remains of a high-mass star are called neutron stars or black holes, depending on the mass of the star. Neutron stars are formed when the core collapses under its own gravity, while black holes are formed when the core collapses into a singularity.
After a high mass star explodes, the leftover material forms a remnant called a neutron star or a black hole. If the core of the star is less than about 3 times the mass of the Sun, it collapses to form a neutron star. If the core is more massive, it collapses further, causing the gravitational collapse to form a black hole.
A high mass star's core collapses when nuclear fusion ceases and gravitational pressure overwhelms the radiation pressure supporting the core. This collapse leads to a rapid increase in temperature and pressure, triggering a supernova explosion.
r0ck s1ide
it is a type of mass movement called a landslide or a landslump.
The mass remains the same, the star becomes more and more dense as the volume decreases
it is a type of mass movement called a landslide or a landslump.
When a large star collapses in a supernova, it can produce either a neutron star or a black hole, depending on the mass of the original star. A neutron star forms when the core of the star collapses but the outer layers are ejected, while a black hole forms when the core collapses completely.
When a single high mass star explodes, it undergoes a supernova event. The core collapses inwards and then rebounds explosively, sending out a shockwave that ejects the outer layers of the star into space. This explosion can outshine an entire galaxy for a short period of time.
A star of similar mass to the sun dies and collapses, forming a white dwarf which cools, forming a black dwarf.A mass of dust and gas too small to ignite fusion collapses, forming a brown dwarf which cools, forming a black dwarf.
When a star collapses to half its size, its gravitational field at the surface increases. This is because the gravitational force is directly proportional to the mass of the star and inversely proportional to the square of the distance from the center of the object. As the star collapses, its mass remains the same but the distance to its center decreases, leading to a stronger gravitational field at its surface.