A Neutron Star
A star that has collapsed under gravity and is made of neutrons is called a neutron star. Neutron stars are extremely dense and have a strong gravitational pull due to the collapsed core of a massive star. They are the remnants of supernova explosions.
A very small, dense remnant of a supernova explosion composed mostly of neutrons is called a neutron star. Neutron stars are formed when the core of a massive star collapses under gravity after it exhausts its nuclear fuel, leading to a catastrophic explosion. These stars are incredibly dense, with masses greater than that of the Sun compressed into a radius of about 10 kilometers. Their extreme density results in the formation of neutrons from protons and electrons, giving them their name and unique properties.
A cold dead star is called a white dwarf. It is formed when a star has exhausted its nuclear fuel and collapsed under gravity, shrinking to a small, dense, and dim object.
An extremely dense dying star is called a neutron star. It is formed when a massive star collapses in a supernova explosion, leaving behind a core made mostly of neutrons. Neutron stars are incredibly dense, packing the mass of the sun into a sphere only about 12 miles in diameter.
The small dense remains of a high mass star are either a neutron star or a black hole, depending on the mass of the original star. Neutron stars are formed from the core collapse of a massive star and are incredibly dense, composed mainly of neutrons. Black holes are formed when the core collapse results in a singularity with infinite density and a gravitational pull so strong that not even light can escape.
a neutron!!! (:
a neutron! :)
A Neutron Star
A Neutron Star
That is called a neutron star, or a pulsar.
A neutron star.
When a collapsed core becomes so dense, it reaches a state known as neutron degeneracy, where neutrons can exist in close proximity due to the exclusion principle preventing them from occupying the same quantum states. This forms a neutron star, where the core is primarily composed of densely packed neutrons.
A star that has collapsed under gravity and is made of neutrons is called a neutron star. Neutron stars are extremely dense and have a strong gravitational pull due to the collapsed core of a massive star. They are the remnants of supernova explosions.
A collapsed core of a supernova that only contains neutrons is called a neutron star. Neutron stars are very dense, with a mass greater than the sun but compressed into a sphere only about 12 miles in diameter. They are supported by neutron degeneracy pressure, which prevents further collapse.
A neutron star is formed when a star collapses under gravity to the point where its electrons and protons combine to form neutrons. Neutron stars are extremely dense and have strong gravitational forces.
A neutron star is composed almost entirely of neutrons. They are supported against further collapse by quantum degeneracy pressure due to the Pauli exclusion principle. This principle states "that no two neutrons (or any other fermionic particles) can occupy the same place and quantum state simultaneously."
A very small, dense remnant of a supernova explosion composed mostly of neutrons is called a neutron star. Neutron stars are formed when the core of a massive star collapses under gravity after it exhausts its nuclear fuel, leading to a catastrophic explosion. These stars are incredibly dense, with masses greater than that of the Sun compressed into a radius of about 10 kilometers. Their extreme density results in the formation of neutrons from protons and electrons, giving them their name and unique properties.