There are no neutron stars with 5 solar masses because one if a neutron star exceeds 3 solar masses, the neutrons inside would no longer be able to support the extreme gravity, so the neutron star would then collapse into a black hole.
A neutron star is prevented from further collapse by a force call neutron degeneracy pressure. Above 3 solar masses gravity will overcome this force and the stellar remnant will collapse completely to form a black hole.
A neutron star with a mass of 5 solar masses is usually not expected to exist because the pressure exerted by neutrons in such a massive object would likely be insufficient to counteract the force of gravity, leading to a collapse into a black hole. Neutron stars typically have masses between 1.4 to 2 times the mass of the Sun due to the balance between gravitational forces and neutron degeneracy pressure.
1 solar mass black hole (smallest) 1 solar mass white dwarf 1 solar mass star 1.5 solar mass neutron star (largest)
Whether a star will become a neutron star is determined by its mass. Generally, stars that are more than 8 solar masses (have a mass that is more than 8 times that of our Sun), but are less than 15 solar masses will become neutron stars when they die.
Adding more mass to a 1.4-solar-mass neutron star could potentially push it beyond the limits of neutron degeneracy pressure, causing it to collapse further. This could result in the formation of a black hole if the mass exceeds the Tolman-Oppenheimer-Volkoff (TOV) limit for neutron stars.
The average density of a neutron star with the same mass as the sun would be about 1 x 10^17 kg/m^3. Neutron stars are incredibly dense objects, as they are formed from the remnants of massive stars that have undergone supernova explosions.
A star with at least 3 solar masses has enough mass to end its life in a supernova explosion. This event can lead to the formation of a neutron star or a black hole, depending on the remaining mass after the explosion. The fate of the star is determined by its mass and the balance between gravitational collapse and nuclear fusion.
1 solar mass black hole (smallest) 1 solar mass white dwarf 1 solar mass star 1.5 solar mass neutron star (largest)
Answer is 1
Whether a star will become a neutron star is determined by its mass. Generally, stars that are more than 8 solar masses (have a mass that is more than 8 times that of our Sun), but are less than 15 solar masses will become neutron stars when they die.
Adding more mass to a 1.4-solar-mass neutron star could potentially push it beyond the limits of neutron degeneracy pressure, causing it to collapse further. This could result in the formation of a black hole if the mass exceeds the Tolman-Oppenheimer-Volkoff (TOV) limit for neutron stars.
Atomic Mass of element - the number the protons.
The average density of a neutron star with the same mass as the sun would be about 1 x 10^17 kg/m^3. Neutron stars are incredibly dense objects, as they are formed from the remnants of massive stars that have undergone supernova explosions.
Neutron has mass nearly 1,840 times the mass of the electron.
The mass of neutron is similar to the mass of proton, but not equal !
6.76294 × 1030kilograms is 3.4 solar masses. Also you can find out any solar mass if you just type the solar mass on google.
Depending on the mass of the original star it will either end up as a neutron star (< 20 solar masses) or a black hole (> 20 solar masses).
A star with at least 3 solar masses has enough mass to end its life in a supernova explosion. This event can lead to the formation of a neutron star or a black hole, depending on the remaining mass after the explosion. The fate of the star is determined by its mass and the balance between gravitational collapse and nuclear fusion.
The approximate atomic mass of a neutron is 1 unified atomic mass unit, which is equivalent to 1.008665 atomic mass units when considering the mass excess.