Neutron stars beginning story
Neutron stars born by following the flow of events. Have a look at how?
Neutron stars beginning story
In nature, there is a simple process of birth and death for everything. Also, the star has the same process. A star's death depends on its scale. The larger the star, the faster its energy blows up. Lastly, death happens earlier for giant size stars. We will know here about the birth of the neutron star.
The simplest atom found in nature is hydrogen. In the center, there is a single proton surrounded by a single electron. The next atom is helium. Helium has two protons and two electrons.
The neutrons keep protons together like glue. Otherwise, protons want to move away from each other because of strong repulsion. The hydrogen atoms wish to run at a massive speed because of the force of gravitational force. For this run, the atoms conflict among themselves. At a point, they exceed the limit of motion. As a result, a hydrogen atom enters the nucleus of another hydrogen atom through a beating.
This way, a helium atom is born in the synthesis of four hydrogen atoms. The two protons move and generate two helium neutrons. The mass of the helium nucleus, which is two neutrons and two protons separately, is less than 0.007 percent. When the proton and neutrons create the helium nucleus together, the reduced mass transforms into energy. This process is nuclear fusion. From this reaction emerges the full power of the planets.
Atoms of helium continue to collect at the constellation's center. Because helium atoms are more substantial than hydrogen, mass in the middle of the star tends to concentrate further. The elevated density generates more heat in the core. By obtaining sufficient temperature and pressure to raise this fuel, helium starts producing carbon in the cycle of atomic fusion. Stars whose mass is one and a half times greater than that of the Sun cannot provide enough energy to generate helium gas. Its demise is terrible too.
Once the hydrogen is on its path of ending, the star's diameter starts to reduce because of gravitational strain. But those contractions produce intense heat, which allows the hydrogen cluster the power to continue the cycle of fusion. As the stars become larger, they begin to spread their heat energy out, allowing the temperature to decrease. This center is the last step in the evolution of the constellation. This condition name is 'white dwarf'.
The stars, which are at least ten times heavier than the Sun, named is 'supergiant.' These stars have tremendous energy that they can make silicon from oxygen fusion. This silicon can produce iron. In this, time the star near to death because it's creating energy less than its need able energy.
Hydrogen is forming helium in the constellation, at some depth, from helium to carbon and from there to oxygen. Deeper is the silicone, the main center, after which the silicon is turned to iron. This is the last stage of creating heavy atom for iron. The planets live on poor equilibriums. Atoms in the trillions trillion tons of mass plasma pull away from the center of gravity. Thanks to this strong desire, the hydrogen nucleus builds helium by fusion only when the atoms do not have enough space to flee.
Consequently, the released energy tries to pull itself out toward gravity. As long as these two are in balance, the stars remain stable. But as soon as the supercontinent star generates iron, and this iron cannot make any more atoms, the equilibrium begins to collapse. Instead, no more strength create to counter the immense force of gravity.
At the center of the constellation under the intense pressure of gravity, the electrons and protons turn into neutrons through fusion, which is again subjected to extreme stress. There is no more space between atoms. As a result, an iron sphere across the earth is shaped into a city by pressing.
However, this phenomenon does not just happen at the Iron Center; Pulls the entire constellation towards the center of gravity. The outer layer sits in the middle of the light frequency, four-quarters. At this great speed, when the iron pushes into the center, it creates a shock, bouncing off the outer layer into space. This phenomenon name is an eruption of the supernova that is visible throughout the galaxy. The part, which is alive in the center of this star is 'Neutron Star'. It is so large and thick that just one sugar cube can hold a billion tons of mass of neutron star.