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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.
What else can I help you with?
What is the order of radius for 1 solar mass white dwarf 1 solar mass star 1.5 solar mass neutron star and 1 solar mass black hole from smallest to largest?
1 solar mass black hole (smallest) 1 solar mass white dwarf 1 solar mass star 1.5 solar mass neutron star (largest)
What determines whether a very massive star will become a neutron?
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.
What would happen if more mass was added to a 1.4-solar-mass neutron star?
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.
What is the average density of a neutron star that has the same mass as the sun?
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.
What is the significance of 3 solar masses in a star's fate?
After a high-mass star explodes as supernova and leaves a core behind, the core would become a neutron star or a black hole. If the core is less than 3 solar masses, it would become a neutron star; if the mass exceeds 3 solar masses, the core would continue to collapse, forming a black hole.
What is the order of radius for 1 solar mass white dwarf 1 solar mass star 1.5 solar mass neutron star and 1 solar mass black hole from smallest to largest?
1 solar mass black hole (smallest) 1 solar mass white dwarf 1 solar mass star 1.5 solar mass neutron star (largest)
Which of these objects has the largest radius 1. a 1.2 solar mass white dwarf 2. a 1.5 solar mass neutron star 3. a 3 solar mass blackhole?
Answer is 1
What determines whether a very massive star will become a neutron?
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.
What would happen if more mass was added to a 1.4-solar-mass neutron star?
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.
How do you find the neutron of the elements?
Atomic Mass of element - the number the protons.
Mass of a neutron?
Neutron has mass nearly 1,840 times the mass of the electron.
Is the mass of a neutron the same as?
The mass of neutron is similar to the mass of proton, but not equal !
What has mass of 3.4 solar masses?
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.
What is the average density of a neutron star that has the same mass as the sun?
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.
What forms from a supernova?
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).
What is the significance of 3 solar masses in a star's fate?
After a high-mass star explodes as supernova and leaves a core behind, the core would become a neutron star or a black hole. If the core is less than 3 solar masses, it would become a neutron star; if the mass exceeds 3 solar masses, the core would continue to collapse, forming a black hole.
What is the approximate atomic mass of a neutron?
The relative mass of a neutron compared with a proton is one.
