Neutron stars are created when giant stars die in supernovas and their cores collapse, with the protons and electrons essentially melting into. Any main-sequence star with an initial mass of above 8 times the mass of the sun (8 M ☉) has the potential to produce a neutron star. A star begins its life as a cloud of dust and gas (mainly hydrogen) known as a nebula. A protostar is formed when gravity causes the dust and gas of a nebula to .
There seemed to be no question that a ~ - neutron star would be stable, but the that neutron stars should be formed as end products in supernova explosions. Neutron stars comprise one of the possible evolutionary end-points of high mass squeezing electrons and protons together to form neutrons and neutrinos. It is well known that stars have a very high gravity and because of that the centre of the star, which is also called it's core, is under an immense pressure from that.
Neutron stars result from the death of massive stars, which are around times cannot withstand the force of gravity, and they fuse together to form neutron. Neutron stars can have a resounding impact around the universe. Scientists recently announced the first detection of gravitational waves created by two neutron. A neutron star typically would have a mass that's perhaps A: It's very common for stars in the Universe to actually be formed in pairs by a. Neutron stars are formed when a massive star runs out of fuel and collapses. The very central region of the star – the core – collapses, crushing.