The neutron star's density varies from below 1×109 kg/m3 in the crust increasing with depth to above 6×1017 or 8×1017 kg/m3 deeper insideThis density is approximately equivalent to the mass of the entire human population compressed into the size of a sugar cube.
Yes, the core of a high mass star will collapse under immense gravitational pressure during a supernova explosion, forming a neutron star. Neutron stars are incredibly dense and composed primarily of neutrons, hence the name.
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.
The singularity in a black hole, then comes the material in a neutron star.
No. Neutron stars are far MORE DENSE than the Sun's core. If the Sun were twice its actual mass, and if it were to collapse into a ball around 10 miles in diameter, THEN it would be as dense as a neutron star. Compared to a neutron star, the Sun is like a mist of hydrogen, a sort of fog.
Depends on the age of the neutron star. As a neutron star no longer has any method to produce heat, it will slowly cool over time. A young neutron star will have a core temperature of about 106 kelvin.
No, the density of a neutron star is much higher than that of a white dwarf. Neutron stars are composed mostly of densely packed neutrons, while white dwarfs are made of electron-degenerate matter. Neutron stars are some of the densest objects in the universe.
Yes, the core of a high mass star will collapse under immense gravitational pressure during a supernova explosion, forming a neutron star. Neutron stars are incredibly dense and composed primarily of neutrons, hence the name.
A dead star with the density of an atomic nuclei is called a neutron star. Neutron stars are incredibly dense and are composed mostly of tightly packed neutrons. They form when massive stars explode in a supernova and their cores collapse under gravity.
Strong is not a term used for a neutron star. If you mean density, then see related question.
See related questions
A typical neutron star - if there is a typical one - has the density of about 3.7×1017 to 5.9×1017 kg/m3. The Earth for comparison has a density of 5.515 g/cm3 To put that into perspective, a neutron star has the mass of the entire human population, squashed down to the size of a sugar cube, or one teaspoon (5 milliliters) of neutron star would have 900 times the mass of the Great Pyramid of Giza. Or imagine squeezing 50 million elephants into a thimble that is the density of a neutron star. Another way of understanding it, is:- if you were (you can't) standing on a neutron star, and you laid a sheet of paper down, the effort required to climb the edge of the paper would be the equivalent of climbing a 3,000 mile cliff on Earth!
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.
The singularity in a black hole, then comes the material in a neutron star.
I suggest you do some reading on both, to get an idea what a neutron star really is, and what a supergiant is. For a start, some differences are: their diameter; their density; the fact that a neutron star no longer produces any energy.
The density of a pulsar or neutron star is much greater than that of a white dwarf. A typical (if there is such a thing) neutron star has a density of between 8.4 × 1016 to 1 × 1018 kg/m3 whereas a white dwarf has a density of about 1 × 109 kg/m3
No. Neutron stars are far MORE DENSE than the Sun's core. If the Sun were twice its actual mass, and if it were to collapse into a ball around 10 miles in diameter, THEN it would be as dense as a neutron star. Compared to a neutron star, the Sun is like a mist of hydrogen, a sort of fog.
Depends on the age of the neutron star. As a neutron star no longer has any method to produce heat, it will slowly cool over time. A young neutron star will have a core temperature of about 106 kelvin.