The pressure of the fusing gasses
Helium burning stars are called red giant stars. These stars have exhausted their core hydrogen fuel and have transitioned to fusing helium into heavier elements like carbon and oxygen.
Nearly 90 percent of all-stars are in the main-sequence phase of their life cycle. This is when they are fusing hydrogen into helium in their cores, a stable phase that can last for billions of years.
Nuclear fusion, usually by fusing hydrogen-1 to helium-4.
The majority of visible stars in the sky are main sequence stars, like our own Sun. These stars are in the stable phase of their life cycle where they are fusing hydrogen into helium in their cores.
Helium atoms
Any star that it fusing hydrogen into helium is classed as a main sequence star.
The pressure of the fusing gasses
No. A star is born when hydrogen stars fusing.
Balls of incandescent (fusing) hydrogen gas that was brought together by gravity.
No. Stars are only in the main sequence when they are fusing hydrogen.
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.
No. The hydrogen in the universe was formed during the Big Bang. Stars consume hydrogen, fusing it into helium.
Helium burning stars are called red giant stars. These stars have exhausted their core hydrogen fuel and have transitioned to fusing helium into heavier elements like carbon and oxygen.
Nearly 90 percent of all-stars are in the main-sequence phase of their life cycle. This is when they are fusing hydrogen into helium in their cores, a stable phase that can last for billions of years.
Nuclear fusion, usually by fusing hydrogen-1 to helium-4.
Because that is the period in a stars life when it is fusing hydrogen into helium See related question