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Helium is formed in the core of the star (like the sun) by the nuclear fusion of hydrogen isotopes.

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Is star is born when helium and oxygen combine true or false?

False. A star is born when hydrogen starts to fuse into helium.


What star in the life cycle of stars fuses hydrogen and helium?

A "red giant" star can fuse both hydrogen (in the star's outer shells) and helium (in the core).


What chemical is more abundant the older a star is?

As a star ages, it fuses hydrogen into helium in its core. Therefore, helium becomes more abundant in older stars compared to younger stars.


Why must a star convert helium after it has converted all of its hydrogen to helium?

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.


What element does a low mass star stop at and why?

Helium. A low mass star does not have enough mass to generate the heat needed to fuse helium.


What are the main gases if a star?

Hydrogen and helium


How does a a star get its energy?

converting hydrogen into helium


Why would an older main sequense star be composed of a higher percentage of helium than a young main sequence star?

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".


What old-main-sequence star will be composed of a higher percentage of helium than a young main-sequene star?

All of them, that's how a star gets to be "old" ... it converts its hydrogen into helium.


What is the defeniton of main sequence star?

A star that is mainly fusing hydrogen into helium.


What elements are in the the star Sirius?

Hydrogen and helium are the most abundant elements in a star.


Which nuclear fusion cycle is the next one to begin after helium fusion ends in a massive 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.