As far as we know, the sun will never become a neutron star. it will eventually become a Red Giant and then it will eventually become a white dwarf
sup.
Neither. Our Sun will turn into a red giant, and then cool to become a white dwarf.
The Sun will never leave behind a stellar remnant such as a neutron star, as it does not have enough mass to achieve the massive pressures required to make one. Our Sun will end up as a white dwarf stellar remnant.
No. it is not massive enough. When the sun dies it will become a white dwarf.
Approximately 1.4 times the mass of the sun, known as the Chandrasekhar limit, is required for a star to become a neutron star. If a star has a mass greater than this limit, it will likely undergo a supernova explosion and collapse into a neutron star.
No, unless it somehow acquires more mass. It requires more mass to become a neutron star.
sup.
Neither. Our Sun will turn into a red giant, and then cool to become a white dwarf.
The Sun will never leave behind a stellar remnant such as a neutron star, as it does not have enough mass to achieve the massive pressures required to make one. Our Sun will end up as a white dwarf stellar remnant.
No. it is not massive enough. When the sun dies it will become a white dwarf.
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.
No. Stars such as our sun become white dwarfs. Only stars 8-10 times the mass of the sun or more become neutron stars.
Approximately 1.4 times the mass of the sun, known as the Chandrasekhar limit, is required for a star to become a neutron star. If a star has a mass greater than this limit, it will likely undergo a supernova explosion and collapse into a neutron star.
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.
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.
No, our sun is not massive enough to become a neutron star. When our sun runs out of fuel, it will shed its outer layers and become a planetary nebula, leaving behind a dense core called a white dwarf.
a star of about sun's mass will become a white dwarf star and will fade slowly into a black dwarf. a star of sun's 1.4 to 3 time the mass of the sun will become a neutron star. a star of more than 3 times of mass of the sun will become a black hole. hopes its help!!