Into heavier elements like carbon and oxygen.
A "Main Sequence" star.
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A main sequence star.
All stars do this.
A "red giant" star can fuse both hydrogen (in the star's outer shells) and helium (in the core).
Oops ! No. The statement is going along pretty good until the end.The star actually fuses hydrogen into helium .
All stars are composed mostly of hydrogen. The star fuses hydrogen into helium. The helium cannot escape the start until the end of the star's life cycle. Thus a middle-aged, medium sized star will be comprised of hydrogen and helium. As the star ages, it may start to fuse helium at its core into carbon. At this point it will likely expand into a red giant star, and thus would no longer be yellow.
well the sun gets its name by just spiningb a star so its a star . comment please
A "main-sequence star" is one that fuses hydrogen into helium. Eventually, the star will run out of this specific type of fuel - in other words, it won't have enough hydrogen (at least, near its core) to continue this process.
A "red giant" star can fuse both hydrogen (in the star's outer shells) and helium (in the core).
For about 90% of a star's existence, it fuses hydrogen into helium, producing lots of heat. When the hydrogen starts to become depleted and the helium "ash" starts building up, the star may expand into a red giant, in which it fuses helium into carbon and heavier elements.
Oops ! No. The statement is going along pretty good until the end.The star actually fuses hydrogen into helium .
All stars are composed mostly of hydrogen. The star fuses hydrogen into helium. The helium cannot escape the start until the end of the star's life cycle. Thus a middle-aged, medium sized star will be comprised of hydrogen and helium. As the star ages, it may start to fuse helium at its core into carbon. At this point it will likely expand into a red giant star, and thus would no longer be yellow.
well the sun gets its name by just spiningb a star so its a star . comment please
A red dwarf fuses hydrogen into helium, just like any star, albeit at a very conservative rate.
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".
because the star burns and fuses hydrogen and helium (like the sun) making heat an light
A star is made up of Hydrogen and Helium, (the Helium coming from the fusion of Hydrogen atoms). When a star goes super nova, it is so hot that it fuses together gases so rapidly that it creates all of the elements on the periodic table.
A "main-sequence star" is one that fuses hydrogen into helium. Eventually, the star will run out of this specific type of fuel - in other words, it won't have enough hydrogen (at least, near its core) to continue this process.
Normal "main sequence" stars fuse hydrogen into helium during most of the star's life. The core of a star gets so hot that the hydrogen atoms begin to fuse together. As hydrogen only has 1 proton when if fuses with another hydrogen atom it has 2 protons so has become helium.
Nuclear fusion is the process that provides energy to the stars.The star fuses hydrogen to form helium this is a process that gives out a lot of energy,stars which are more passive than our sun then it fuses the helium atoms to form carbon.