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What will a star that's 1000 times as massive as the sun ultimately become?
A star that is 1000 times as massive as the Sun will likely end its life in a supernova explosion, leaving either a neutron star or a black hole as a remnant, depending on the mass of the core after the explosion.
What is the difference between a nova a supernova and a neutron star?
A nova is a star which has a close companion star, and draws stellar material off of it's companion, occasionally flaring up very brightly in the process. A supernova is a massive and hot star to begin with, that tends to go through it's life cycle at high speed, and ending it's life in a cataclysmic explosion. Supernova remnants then collapse into a neutron star - a spinning, very hot pile of stellar ash, so dense that a teaspoonful of it would weigh thousands of tons. If the collapsed supernova star was big enough, it's gravity upon collapse is so intense than not even light can escape from it, and it becomes what is called a "Black Hole".
What is a very massive star?
The sun
Is your sun a supernova or a white dwarf?
Our Sun is currently a main sequence star. It is not a supernova, as supernovae are massive explosions that occur at the end of a star's life cycle, and it is not a white dwarf, which is a type of star that has exhausted its nuclear fuel and collapsed to a very dense state.
Is a star that burst very brightly and violently?
It sounds like you might be describing a supernova, which is an astronomical event where a star undergoes a powerful explosion, briefly outshining an entire galaxy before fading from view. Supernovae can result from the death of massive stars or from the interactions in binary star systems.
What star blows up in a super nova explosion?
That will happen to stars that are very massive.
What will a star that's 1000 times as massive as the sun ultimately become?
A star that is 1000 times as massive as the Sun will likely end its life in a supernova explosion, leaving either a neutron star or a black hole as a remnant, depending on the mass of the core after the explosion.
The final stage in the evolution of the most massive stars is an?
The final stage in the evolution of the most massive stars is a supernova explosion, where the star collapses and then rebounds in a powerful explosion. This explosion can lead to the formation of either a neutron star or a black hole, depending on the mass of the collapsing core.
What is the difference between a nova a supernova and a neutron star?
A nova is a star which has a close companion star, and draws stellar material off of it's companion, occasionally flaring up very brightly in the process. A supernova is a massive and hot star to begin with, that tends to go through it's life cycle at high speed, and ending it's life in a cataclysmic explosion. Supernova remnants then collapse into a neutron star - a spinning, very hot pile of stellar ash, so dense that a teaspoonful of it would weigh thousands of tons. If the collapsed supernova star was big enough, it's gravity upon collapse is so intense than not even light can escape from it, and it becomes what is called a "Black Hole".
What is a very massive star?
The sun
Is your sun a supernova or a white dwarf?
Our Sun is currently a main sequence star. It is not a supernova, as supernovae are massive explosions that occur at the end of a star's life cycle, and it is not a white dwarf, which is a type of star that has exhausted its nuclear fuel and collapsed to a very dense state.
What is a very small dense remnant of a supernova explosion composed mostly of neutrons?
A very small, dense remnant of a supernova explosion composed mostly of neutrons is called a neutron star. Neutron stars are formed when the core of a massive star collapses under gravity after it exhausts its nuclear fuel, leading to a catastrophic explosion. These stars are incredibly dense, with masses greater than that of the Sun compressed into a radius of about 10 kilometers. Their extreme density results in the formation of neutrons from protons and electrons, giving them their name and unique properties.
What is the explosion of a dying giant or supergiant star?
There are several different kinds. An explosion ON a star is usually called a "nova" (from the Latin for "new", because this results in the star brightening significantly, thus appearing to be a "new star"). The star itself usually survives, and the cycle will probably repeat several times. The explosion OF a very large star is called a "supernova", and again there are different kinds. Stars generally either do not survive this, or survive only in very changed form (as a neutron star or black hole).
The birth of a small star and a very massive star are the same but the end of their life is very different Describe the difference in the fate of a small star and a very massive star?
The difference between the death of a small star and a massive star is what the become afterwards. A small star will typically become a red dwarf while a large star will become a neutron star or a black hole.
What term is applied to stars that explode?
Stars that explode are referred to as supernovae. This explosive event occurs when a massive star reaches the end of its life cycle and undergoes a rapid and intense process of collapse and explosion. Supernovae release an incredible amount of energy and can briefly outshine an entire galaxy.
A very small dense star It forms after a huge massive star explodes and then collapses A teaspoon of it matter would weigh millions of tons?
The description matches that of a neutron star, which is formed after a supernova explosion of a massive star. Neutron stars are incredibly dense, with matter packed tightly together. Due to their high gravitational pull, a small amount of neutron star material would have an extremely high mass.
Is a star that burst very brightly and violently?
It sounds like you might be describing a supernova, which is an astronomical event where a star undergoes a powerful explosion, briefly outshining an entire galaxy before fading from view. Supernovae can result from the death of massive stars or from the interactions in binary star systems.
