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When Belegeuse dies what kind of star will it be?
Betelgeuse is a type M Red Supergiant with a probable mass between 10 and 20 solar masses. Because of its mass it will continue to fuse elements until it reaches the iron phase at which time it will explode as a Type II supernova probably leaving behind a Neutron star of about a 20km radius.
What is the relationship between a supernova and a neutron star?
They both explode and some parts turn to meteors and some land on Earth. Though through out the whole thing people think super novas are alien spaceships from another galaxy. Astronomers study these novas and tell us the truth!
What remnant does a supernova leave?
Depending on the mass of the original star, it is either a black hole or a neutron star.
How long does a neutron star last after a supernova?
Nobody knows for sure, but billions of years. It would also depend on when the neutron star, no longer becomes a star. Is it when it stops radiating heat, or x-rays? The star or the remains will continue to be a physical property but will no longer radiate any energy.
Is a pulsar a white dwarf?
A pulsar is a type of neutron star, a collapsed core of an extremely massive star that exploded in a supernova. Whereas white dwarfs have incredibly high densities by earthly standards, neutron stars are even denser, cramming roughly 1.3 solar masses into a city-sized sphere.
What is the life cycle of the star Betelgeuse?
red giant, plantary nebula, white dwarf,black whole, red supergiant , supernova, neutron star
Will a neutron star eventually go supernova?
No. A neutron star is left behind after a supernova. However, some gamma ray bursts may result from a collision between neutron stars.
What is the differences between super nova and neutron star?
A supernova is when a massive star explodes. A neutron star is what can be formed after a supernova explosion. See related questions
What may the collapsed core of a supergiant star form?
What the core of the star will become is dependent of the mass of the supergiant star. Stars between about 3 and 10 solar masses will generally become neutron stars. Stars above 10 solar masses generally become black holes.
What can form after the supernova of a red giant?
After the supernova of a red giant, remnants such as a neutron star or a black hole can form, depending on the mass of the original star. If the star was especially massive, it may also result in a supermassive black hole or a hypernova explosion.
What happens during the life cycle of a starwith one stellar mass?
a star with 2-3 stellar masses would become a red supergiant then a supernova and then become a neutron star.
What is after super giant star?
After a supergiant star, the star can evolve into a supernova, which is a massive explosion that signals the end of the star's life. Depending on the mass of the star, it can then collapse into a neutron star or a black hole.
What can a super giant star explode into?
A supergiant star can explode into a supernova, where the outer layers are ejected into space. What remains may collapse into a neutron star or black hole, depending on the mass of the original star.
How does a star turns into a neutron star?
A star 8 time the mass of the Sun turns into a neutron star when it run out of fuel, become a supergiant, and undergo supernova explosion. After the explosion, a core remains. If the core is less than 3 Solar masses, it becomes a neutron star, or else it becomes a black hole.
What is the lifecycle of betelgeuse the star?
Betelgeuse is a red supergiant star currently in the late stages of its life. It is expected to explode as a supernova in the future, likely within the next 100,000 years. After the supernova event, it will leave behind either a neutron star or a black hole, depending on its initial mass.
What follows a supernova and has a neutral charge?
A neutron star
Was the first neutron star observed in a supernova remnant?
Yes, the first neutron star was observed in a supernova remnant. The object, named PSR B1919+21, was discovered in 1967 in the Crab Nebula, the remnant of a supernova that exploded in the year 1054 AD.
