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hydrogen, helium and carbon
Nuclear Fusion
Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.
Stars spend about 90% of their fusion lifetimes on the main sequence.
The main source of energy in the Sun and other stars is fusion of hydrogen atoms into helium atoms.
hydrogen, helium and carbon
Nuclear Fusion
Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.
No. That's precisely the main difference between planets and stars - that stars can have nuclear fusion, planets not.
Stars spend about 90% of their fusion lifetimes on the main sequence.
No. Stars are only in the main sequence when they are fusing hydrogen.
The main process is nuclear fusion of hydrogen to form helium.
In main sequence stars, it is thermonuclear fusion of hydrogen into helium.
The thing the "main sequence" stars have in common is that they get their energy from the fusion of hydrogen (hydrogen-1 is converted into helium-4).
The main source of energy in the Sun and other stars is fusion of hydrogen atoms into helium atoms.
No elements were formed in the big bang. After quite some time, hydrogen began to form, and it is the main constituent of stars. The main by-product of nuclear fusion in stars is helium.
Main Sequence