High gravitational compression (in stars) or mechanical compression (in weapons) forces two hydrogen atoms together in nuclear fusion. Recall that the only places we see nuclear fusion happeing (so far) are in stars and in fusion weapons. In the star, the thermal energy in which these reactions is happeing is enormous. It's super hot inside the star, and the hydrogen nuclei (two protons) are forced together because of the gravitational compression. Heck, they wouldn't normally want to get anywhere near each other, let alone fuse to become a heavier particle. But the extreme gravity and extreme thermal energy there allow this to happen.
In a nuclear fusion weapon, we use a fission device to create the mechanical compression (in place of the star's gravity) to force hydrogen nuclei together to get them to fuse. The fission device also creates the thermal energy needed. This is the simple explanation of this fundamental nuclear reaction. Links can be found below to learn more.
In the core of the sun, nuclear fusion occurs where hydrogen atoms combine to form helium. This process releases large amounts of energy in the form of heat and light. The sun's gravity plays a crucial role in maintaining the high temperature and pressure needed for nuclear fusion to take place.
The two gases associated with nuclear fusion are deuterium and tritium. When these two isotopes of hydrogen fuse together, they form helium and release a large amount of energy in the process.
Hydrogen fusion occurs in stars to create helium. This process, known as nuclear fusion, involves the fusion of hydrogen nuclei to form helium nuclei, releasing large amounts of energy in the process.
It's called the proton-proton cycle. It's the source of the sun's energy. Also called nuclear fusion.
In the Sun, hydrogen nuclei are fused together to form helium in a process called nuclear fusion. This fusion process releases a large amount of energy in the form of light and heat, which powers the Sun and sustains its brightness.
Hydrogen is what gets fused together to form Helium.
hydrogen fusion
In the core of the sun, nuclear fusion occurs where hydrogen atoms combine to form helium. This process releases large amounts of energy in the form of heat and light. The sun's gravity plays a crucial role in maintaining the high temperature and pressure needed for nuclear fusion to take place.
Stars get their energy from nuclear fusion - mainly, hydrogen to helium.Stars get their energy from nuclear fusion - mainly, hydrogen to helium.Stars get their energy from nuclear fusion - mainly, hydrogen to helium.Stars get their energy from nuclear fusion - mainly, hydrogen to helium.
Nuclear Fusion
This is a fusion process, the nuclear reaction that powers our Sun. Hydrogen and hydrogen isotopes come together to make helium
The nuclear fusion uses Hydrogen to produce Helium. The fusion also releases a lot of energy, which is what causes the explosion.
During the solar nuclear reaction, hydrogen nuclei (protons) bond together to form helium nuclei through a process called nuclear fusion. This fusion involves the conversion of hydrogen into helium, releasing a large amount of energy in the form of light and heat.
Nuclear fusion of hydrogen into helium.
The two gases associated with nuclear fusion are deuterium and tritium. When these two isotopes of hydrogen fuse together, they form helium and release a large amount of energy in the process.
Hydrogen fusion occurs in stars to create helium. This process, known as nuclear fusion, involves the fusion of hydrogen nuclei to form helium nuclei, releasing large amounts of energy in the process.
It's called the proton-proton cycle. It's the source of the sun's energy. Also called nuclear fusion.