What is the core temperature requirement for helium fusion via the triple-alpha process in a Sun-sized star?

Answer

About $10^8$ K

For a star around the Sun's mass, sufficient core contraction is achieved when the temperature reaches about $10^8$ Kelvin, which allows the triple-alpha process to fuse helium into carbon and oxygen.

What is the core temperature requirement for helium fusion via the triple-alpha process in a Sun-sized star?

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