Carbon fusion is a stage towards the end of a star's life. See para below and link
Carbon burning starts when helium burning ends. During helium fusion, stars build up an inert core rich in carbon and oxygen. Once the helium density drops below a level at which He burning can be sustained, the core collapses due to gravitation. This decrease in volume raises temperature and density of the core up to the carbon ignition temperature. This will raise the star's temperature around the core allowing it to burn helium in a shell around the core. The star increases in size and becomes a red supergiant.
No, carbon dating does not use nuclear fusion. Carbon dating is a method used to determine the age of organic materials by measuring the remaining levels of a radioactive isotope called carbon-14. This process involves the decay of carbon-14, not nuclear fusion.
Carbon cannot be used as a nuclear fuel, either for fission or fusion.
First beryllium is formed, followed by carbon
Nuclear fusion (converting hydrogen-1 to helium-4), in the Sun. This is what powers the Sun.
Fusion is a type of
Carbon fusion requires much higher temperatures and pressures than ordinary hydrogen fusion.
In deuterium-tritium fusion, the result is helium-4. In helium fusion, carbon is produced.
No, carbon dating does not use nuclear fusion. Carbon dating is a method used to determine the age of organic materials by measuring the remaining levels of a radioactive isotope called carbon-14. This process involves the decay of carbon-14, not nuclear fusion.
When hydrogen stocks run out
Carbon is formed during the fusion process within stars. When the star can no longer sustain stable fusion, it explodes and scatters its constituent elements throughout the universe.
Same as all elements - in stars by nuclear fusion.
Carbon cannot be used as a nuclear fuel, either for fission or fusion.
First beryllium is formed, followed by carbon
hydrogen, helium and carbon
Thermonuclear fusion of hydrogen occurs during the red giant phase. Helium to carbon fusion, or dredge up, also occurs at this time.
Carbon is synthesized from the nuclear fusion that occurs inside stars. The mass of a large or massive star creates conditions that allows more fusion to occur than just hydrogen to helium.
the star collapses in on itself, and usually when the fusion stops it is in the last stages of its life as a giant or supergiant and forms a white dwarf made of the carbon left over from the second stage of helium to carbon fusion from the core of the star that takes place after the hydrogen to helium fusion. after the white dwarf is formed it will eventually cool off into a black dwarf which is basically a carbon corpse of a star