Vega is just over twice the mass of the Sun.
When a large star runs out of fuel, it undergoes a supernova explosion, where the core collapses and releases a huge amount of energy. The outer layers are expelled into space, forming a nebula, while the core either forms a neutron star or a black hole, depending on its mass.
Mass decides a stars ultimate fate.
It will probably explode as a supernova, leaving either a neutron star or black hole.
High mass.
Vega is just over twice the mass of the Sun.
Planet.
When a large star runs out of fuel, it undergoes a supernova explosion, where the core collapses and releases a huge amount of energy. The outer layers are expelled into space, forming a nebula, while the core either forms a neutron star or a black hole, depending on its mass.
After a large star like vv cephie there is a white dwarf.
The blue star gains a little more mass.
At the end of its life cycle, a large mass star undergoes a supernova explosion after exhausting its nuclear fuel. This explosion disperses the outer layers of the star into space, while the core collapses under gravity, potentially forming a neutron star or a black hole. The remnant can have a profound impact on its surroundings, enriching the interstellar medium with heavy elements and triggering the formation of new stars.
During last ages of life of a star, to find what happens in coming ages of life of star. It determines on its mass explained by chandrashekher that if the mass of given star is 2.42 times the mass of our sun then it explodes in the form of supernova. If the mass of given star is less than the 2.42 times the mass of our sun then it shrinks to become white dwarf.
it depends on the mass. If the star is small and it dies then it will turn into a red giant then a white dwarf. But if the star has enough mass and is bigger than any other star then it will collapse and turn into a black hole.
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.
The density will not be as large as one with the same mass which is spread over a smaller volume.
Mass decides a stars ultimate fate.
It stops at about 0.12 seconds.