in stars and fusion bombs.
During nuclear fusion, hydrogen atoms are fused into helium atoms. This process releases a large amount of energy in the form of heat and light. It is the same process that powers the sun and other stars.
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 and helium are formed in Sun.
Essentially yes; the sun's energy comes from nuclear fusion with hydrogen being converted to helium.
Nuclear fusion in sun is followed by proton proton chain reaction during this reaction hydrogen fused to form helium the main products of this reaction according to nuclear equation is - positron, neutrino, gamma ray photons, isotopes of hydrogen and helium
- hydrogen nuclei waiting to be fused into helium and - helium which has been fused from hydrogen nuclei
99.993 % into Helium, .007 % into energy.
Nuclear fusion, in which hydrogen-1 is fused into helium-4.
The sun's light is the result of a nuclear fusion reaction by which hydrogen is fused into helium.
The ratio of hydrogen to helium in the sun has been decreasing over time as hydrogen is being converted into helium through nuclear fusion reactions in the sun's core. This process is gradually shifting the composition of the sun more towards helium.
We understand that hydrogen atoms are fused into helium in the sun's core.
Hydrogen is fused into helium in the core of stars through a process called nuclear fusion. This occurs under extreme temperatures and pressures, allowing hydrogen atoms to combine to form helium, releasing a tremendous amount of energy in the form of radiation.
Within our Sun, hydrogen is fused into helium at very high temperatures. This is how the Sun is powered.
During nuclear fusion, hydrogen atoms are fused into helium atoms. This process releases a large amount of energy in the form of heat and light. It is the same process that powers the sun and other stars.
All stars- including our sun- are an ongoing nuclear fusion reaction- hydrogen is fused into helium. The hydrogen is consumed in that reaction.
The sun consists of hydrogen and helium atoms. The hydrogen atoms combine in a process called nuclear fusion, releasing energy and creating helium atoms.
In the sun, hydrogen atoms fuse together to form helium through a process called nuclear fusion. This process releases energy in the form of light and heat, which is what sustains the sun's brightness and temperature.