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Why is why is there an upper limit to the mass of neutron stars?
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Why is there an upper limit to the mass of neutron stars?
There is an upper limit to the mass of neutron stars because if the neutron star is too massive, neutrons would be crushed by the gravity of the neutron star, and the neutron star would collapse into a black hole.
Why are neutron stars so heavy?
Neutron stars are so heavy because they are the compact core of a star that is 8 time the mass of our Sun. The most massive neutron stars possible are 3 times the mass of our Sun.
Do low mass and medium mass stars eventually become neutron stars?
Low and medium sized stars will end up as white dwarfs.
What are remnants of high mass star?
Neutron stars and black holes.
What is a low- meduim- mass star the becomes the end of its life?
White dwarf. High mass stars become neutron stars or black holes.
Why is there an upper limit to the mass of neutron stars?
There is an upper limit to the mass of neutron stars because if the neutron star is too massive, neutrons would be crushed by the gravity of the neutron star, and the neutron star would collapse into a black hole.
Why are neutron stars so heavy?
Neutron stars are so heavy because they are the compact core of a star that is 8 time the mass of our Sun. The most massive neutron stars possible are 3 times the mass of our Sun.
Do massive stars become neutron stars?
Some massive stars will become neutron stars. When massive stars die they will either become neutron stars or black holes depending on how much mass is left behind.
Will the sun turn into a neutron star?
No. It does not have enough mass. Only stars 8 times the mass of the sun or greater can become neutron stars. The sun will become a white dwarf.
Why is there an upper mass limit for main-sequence stars of about 100 solar masses?
Objects above this mass fuse hydrogen too rapidly and cannot stay together.
Do low mass and medium mass stars eventually become neutron stars?
Low and medium sized stars will end up as white dwarfs.
What is the remains of of high mass stars?
It can be a black hole or a Neutron Star
What are remnants of high mass star?
Neutron stars and black holes.
Could an average stars such as our sun become a neutron star?
No. Stars such as our sun become white dwarfs. Only stars 8-10 times the mass of the sun or more become neutron stars.
What is the difference between stars that become dwarf stars and stars that become neutron stars?
A star that becomes a white dwarf simply does not have the mass to become a neutron star. White dwarfs are the the remnants of a star very similar to our own sun in mass, where it takes a much more massive star to create a neutron star, Like the star Betelgeuse is a prime example of a star that does not have the mass to become a black hole but is massive enough to become a neutron star.
How are neutron stars formed?
Neutron stars are formed when stars with more than 8 times the mass of the Sun run out of fuel and explodes as a supernova. After the star explodes, the core of the star remains, the core would then become a neutron star or a black hole. If the core remain is less than 3 times the mass of the sun, it would become a neutron star.
What are the small dense remains of a high-mass star called?
Neutron stars
