Helium atoms
Oxygen is produced through repeated hydrogen fusion in stars. One such process would start with the hydrogen atoms fusing to form helium. And then the helium would fuse to form beryllium. That in turn would fuse to create oxygen.
hydrogen,All stars are composed primarily of hydrogen. Stars can also contain some other elements such as helium, but hydrogen accounts for the majority of a star's composition.
nebula
A nuclear reaction - either fusion or fission - is required to turn matter into energy.
Hydrogen and helium. It's better to ask which two ELEMENTS make up the bulk of the stars, since ALL elements in a star are in the gaseous state.
Stars produce energy by fusing hydrogen into helium through a process called nuclear fusion. This fusion reaction releases a tremendous amount of energy in the form of light and heat, which powers the star and allows it to shine.
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.
Nuclear fusion, usually by fusing hydrogen-1 to helium-4.
Stars like our sun and hydrogen bombs produce energy through nuclear fusion.
Nuclear fusion, usually by fusing hydrogen-1 to helium-4.
No. The hydrogen in the universe was formed during the Big Bang. Stars consume hydrogen, fusing it into helium.
No. Standard sized young Stars are made up of hydrogen atoms fusing themselves into helium atoms and giving off lots of Energy.
technically speaking, stars are first made of Hydrogen. The moment the star comes to life, it starts fusing together Hydrogen atoms, forming helium. when a star is nearing the end of its life, it starts fusing together helium and keeps on fusing until there is nothing more to fuse. then, the star dies.
Oops ! No. The statement is going along pretty good until the end.The star actually fuses hydrogen into helium .
The main source of energy for stars is nuclear fusion, where hydrogen atoms combine to form helium. This process releases a tremendous amount of energy in the form of light and heat, which is what allows stars to shine and emit heat.
Helium is an important element in stars as it is a byproduct of nuclear fusion, the process that powers a star. In the core of a star, hydrogen atoms fuse to form helium, releasing energy in the process. This energy generation is what allows stars to shine and sustain their existence.
The main sequence stars are stars that fuse hydrogen, so the stars that have left the main sequence are the ones that have basically run out of hydrogen. They are the Red Giant stars, Supergiant stars and White Dwarf stars.