Stars that have more mass than the sun will end their lives as neutron stars.
If a star has a mass of 1.5 to 2 or 3 times that of the Sun, it will eventually collapse even more, forming a neutron star with a possible diameter of 20 kilometers. In neutron stars, the gravitational force has overcome the electrons' ability to resist compression and compelled them to combine with protons to form neutrons.
After its formation, a neutron star produces neither light nor heat on its own. From an initial temperature of 600,000 degrees Kelvin (1 million degrees Fahrenheit), its latent heat will gradually decrease over millions of years, putting an end to its life as the icy, dead remnant of a once-brilliant star.
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