The galaxy is made up of gases called nebulae. The nebula gas clouds begin to shrink as the gravitational force between the atoms of the gases moving slowly in space increases as the cold atomic gas clouds move closer and closer together due to the higher gravitational force.
All particles contract towards the center and form a strong bond that starts hot due to excessive pressure.
This temperature will continue to rise to several million degrees Celsius. At this temperature, the nuclear reaction, i.e., the nuclear reaction, begins. This is when the star is born.
Nebula
Star formation:
Its color varies depending on the temperature of the star. The color changes to red, yellow, white, and long as the temperature rises. When the blue color comes, it means that the destruction of the star begins.
The capital that illuminates a star is the heat and light emitted uncontrollably during nuclear reactions.
During nuclear fusion, four hydrogen atoms combine to form a helium atom. Thus, supernatural energy is exposed.
During each fusion, a certain number of atoms are lost. This mass is converted into more thermal energy and is lost.
The formation of helium with hydrogen will continue for billions of years.
Larger galaxies lose fuel faster than others. Thus the larger galaxy will have a shorter lifespan.
Smaller galaxies will continue to react for a long time. Its lifespan will be longer.
Destruction of the star:
The reaction of helium with hydrogen continues. When hydrocarbons are depleted over time, this level indicates that the star's destruction has begun.
The helium atoms then combine to form mass atoms of carbon, oxygen, and ion.
As this reaction occurs at a higher temperature, the temperature of the star rises further. This heat makes the star size many times larger than the initial size.
This reaction occurs at the inner center of the star so that the outside begins to cool. But the interior will be of great terrible heat.
The position of this giant red star is called the Red Giant. It is very luminous. Its diameter will be more than fifty million kilometers.
That is, the larger our sun touches our earth, the larger it will be.
The galaxy will further collapse, scattering its contents into space. The material on the outside will be losing a little bit. Again these form a small nebula around the star.
This stage is called the white dwarf, where the size of the star decreases and forms a small white glowing star with a higher density. I.e., called the white dwarf star. Its surface is boiling. The reason is that after the stagnant star, it will start to change permanently.
Combustion products are found in exhaustion. This phenomenon is called a supernova. Maybe if it had been the biggest star, it would have finally exploded terribly.
Scattered into particles and pushed into space. When pushed like that, electromagnetic waves are formed. At the center will be a small neutron star. But today, the weight of the tiny neutron star is much higher than in India.
Eventually, it turns into a black hole. This continuous reaction will cause the star to disappear billions of years later.
When viewed through a telescope, each star is visible as white, yellow, red, and elongated. This color will determine its age. Every star is a sun.
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