Helium is formed in the core of the star (like the sun) by the nuclear fusion of hydrogen isotopes.
False. A star is born when hydrogen starts to fuse into helium.
A "red giant" star can fuse both hydrogen (in the star's outer shells) and helium (in the core).
As a star ages, it fuses hydrogen into helium in its core. Therefore, helium becomes more abundant in older stars compared to younger stars.
As a star exhausts its hydrogen fuel and increases in temperature and pressure, it needs to start fusing helium to produce energy and maintain equilibrium against the inward force of gravity. This process is necessary to sustain the star's energy output and prevent collapse.
Helium. A low mass star does not have enough mass to generate the heat needed to fuse helium.
Hydrogen and helium
converting hydrogen into helium
A star's nuclear fusion reaction converts hydrogen into helium, and generates energy through this process. A "new" star has a fairly low percentage of helium, but over the course of billions of years, it fuses the hydrogen "fuel" into helium "ash".
All of them, that's how a star gets to be "old" ... it converts its hydrogen into helium.
A star that is mainly fusing hydrogen into helium.
Hydrogen and helium are the most abundant elements in a star.
The next nuclear fusion cycle after helium fusion in a massive star is carbon fusion. This process involves fusing helium nuclei to form carbon. Carbon fusion typically occurs in the core of a massive star after helium fusion is completed.