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A neutron star is a very dense and compact object that is formed when a massive star runs out of fuel and collapses under its own gravity.
A neutron star can only form in the center of a star if the star is at least 8 times more massive than our Sun. As the star's core runs out of fuel, it collapses under its own gravity, causing the electrons and protons to combine and form neutrons. This process creates a neutron star.
A neutron star at the center of the Sun is incredibly small, with a diameter of only about 20 kilometers. This is smaller than the size of a city on Earth, but it contains the mass of about 1.4 times that of our Sun.
The temperature of a neutron star at the center of the Sun can reach up to a billion degrees Celsius. This extreme heat is caused by the collapse of the star's core and the release of energy during the formation of the neutron star.
No, we cannot see the neutron star at the center of the Sun because it is surrounded by layers of gas and plasma. However, scientists can indirectly study the presence of a neutron star through the effects it has on its surroundings, such as the gravitational pull it exerts on nearby objects.