The sun produces energy by fusing hydrogen atoms into helium atoms. This is a nuclear fusion that occurs at the sun's core.
Two hydrogen nucleus on fussion produce helium nucleus but it should be kept in mind that sun contains plasma (dissociated atoms as ions and electrons) not the atoms.
Yes it does. It produces helium by fusing hydrogen
Helium atoms
Hydrogen
helium
Hydrogen, but its not burning, its fusing.
Three-quarters of the Sun's mass is hydrogen. How many hydrogen atoms are in the Sun?
Helium.
Yes. It will eventually. The sun has enough hydrogen in its core to remain as a main sequence star for about 5 billion years. After that it will alternate between fusing helium in its core and hydrogen in a shell around the core for about 2 billions. Then it will shed its outer layers and leave behind a degenerate remnant called a white dwarf.
under extreme heat and pressure - it happens on the sun all the time!
Yes it does. It produces helium by fusing hydrogen
The sun is fusing hydrogen atoms together, turning them into helium.
At the age the sun is now it is still fusing hydrogen into helium.
The fusing of hydrogen atoms into helium.
The sun's energy (and that of all other stars) comes from nuclear fusion. The nuclei of hydrogen atoms (ie protons) fuse together to produce helium and release energy.
Our sun gets energy from fusing hydrogen atoms with neutrons to form helium atoms.
Inside the Sun, it is mainly hydrogen-1 fusing into helium-4.
Nuclear reaction inside the Sun is fusing of Hydrogen to Helium and release out thermal energy.
Hydrogen: the mutual fusing of H atoms into Helium, with consequent release of energy.
sun have H2 atoms so by fussion process H atoms produce hydrogen bomb and then blast and light will produce .
The sun produce energy during the nuclear fusion process when hydrogen atoms are converted into helium atoms in the core of the sun. When the sun runs out of hydrogen it will "start to die".
The sun is a star, fusing hydrogen atoms in its inner most layers to produce electromagnetic energy. A Protostar is basically a clump of interstellar matter/dust that may be coalescing due to gravitation to form a star but its center has not yet achieved a high enough temperature for hydrogen fusion to begin.