Nuclear Fission In Sun

• Suns major amount of energy comes out of fission, this type of fission comes when hydrogen atoms in the core of sun starts to hit each other, resulting to the formation of helium, releasing vast amount of energy

• Hydrogen atoms just does not collide like that and turn into lithium. This is a very long process inside the sun, this process is called stellar process

Stellar Process

• This process occurs when multiple hydrogen atoms collide together, making the atoms release insane amount of heat and energy, this cause the creation of helium atoms

• Usually Steller process occurs when hydrogen converts to helium and goes on till carbon, neon or iron. Usually at iron it stops as iron does not release energy

• Iron cant release energy thus it absorbs them, in huge planets when fission occurs it stops till iron and starts absorbing energy like a black hole

Sufficient Fuel

• Because the Sun is so massive and contains so much hydrogen, it can sustain these fusion reactions for billions of years.

Nuclear Fission - Particle Study

• Nuclear fission occurs when the nucleus splits into half, this releases tones of energy and heat

• The nucleus of particular atoms may be really unstable like uranium and etc, to get the fission process started when there is a neutron hitting the nucleus it breaks and spreads into multiple small uranium atoms

High Temperature And Pressure

• Fusion requires extremely high temperatures (millions of degrees) and pressures to overcome the repulsion between positively charged nuclei.

• This explains why fusion is not easy to replicate on Earth—achieving and containing these conditions is a massive engineering challenge.

Energy Radiation

• The energy produced in the Sun’s core travels outward, eventually reaching Earth in the form of sunlight (electromagnetic radiation).

• Only a tiny fraction of the Sun’s total output reaches Earth, yet it is still the driving force behind our climate, weather, and most life processes.