Looking up to the sky on a bright summer day - one could easily see the sun. That big ball of fire is the reason why we are all alive right now. But how did that ball of energy come about?
Stars like our sun was formed in space clouds called a nebula. A nebula is an enormous space cloud that is many light years across (a light year is the distance light travels within a year: which is nearly six trillion miles!).
These nebulae contains about 70% Hydrogen, 28% Helium and 2% of other elements.
In these nebulae, each particle of gas is so far a part that they don't even touch! But every now and then, a disturbance such as a supernova or irregularities in the nebula causes molecules to attract each other via gravity.
When this happens, the portion of the nebula that is disturbed starts collapsing unto itself bringing more and more molecules into close contact. As the size of the collapsing nebula decreases in size, it begins to rotate faster due to conservation of angular momentum. Angular momentum = mass x velocity x radius. Angular momentum has to stay the same and the mass does not change, therefore if the radius decreases, the velocity has to increase in order to keep angular momentum constant.
Now that the molecules are interacting more, the density, temperature, and pressure increases. The temperature increases because the kinetic energy of the molecules is converted to thermal energy. As the pressure increases, the pressure begins to counter the force of gravity.
A protostar becomes a star when it starts fuse hydrogen at its core. Fusion of hydrogen into helium occurs when core temperature reaches 10 million degrees kelvin or approximately 18 million degrees Fahrenheit. A star is stabilized by the forces nuclear fusion exerts and the forces of gravity. These two forces are opposing forces, therefore they must balance each other for the sun to stay in stasis. This state is called hydrostatic equilibrium.
Planets are created in the same way as the sun. The main difference is that planets do not have enough gravitational force to initiate fusion and they contain different composition of elements. For comparative purposes: by weight, the earth is mostly oxygen and silicon, and the sun is mostly hydrogen and helium.
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References:
Composition of Elements on Earth
How is a star born
Star Birth
Life Cycle of Stars
How do Stars Form and Evolve?
The Outer Planets
A Star is Born











