The mass range for neutron stars is:

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The mass range for neutron stars is typically between 1.4 to 3 solar masses. This is because neutron stars are formed from the collapsed cores of massive stars, which typically have a mass range of 8 to 20 solar masses. During the collapse, the outer layers of the star are blown away, leaving behind a highly compressed core consisting mostly of neutrons. This core can be as small as 10 km in diameter, but contains the mass of 1.4 to 3 solar masses, resulting in an extremely dense and compact object. The mass range for neutron stars is typically between 1.4 to 3 solar masses. This is because neutron stars are formed from the collapsed cores of massive stars, which usually have a mass of around 8-20 solar masses. The collapse of the core during a supernova results in a highly dense object with a mass of around 1.4 times that of the sun, which is the minimum mass required for a stable neutron star to form. While some neutron stars can have a slightly higher or lower mass than this range, the majority fall within the 1.4-3 solar mass range.

The Mass Range for Neutron Stars Is