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oxygen-burning process

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Again, gravitational pressure takes over and compresses the central core, increasing its density and temperature until the oxygen-burning process can start.
ชื่อเอกสารscb_mt_enth_2020 scb_mt_enth_2020
The oxygen-burning process is a set of nuclear fusion reactions that take place in massive stars that have used up the lighter elements in their cores.
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After a few years the star consumes all its neon and the core ceases producing fusion energy and contracts. Again, gravitational pressure takes over and compresses the central core, increasing its density and temperature until the oxygen-burning process can start.
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During neon burning, oxygen and magnesium accumulate in the central core while neon is consumed. After a few years the star consumes all its neon and the core ceases producing fusion energy and contracts. Again, gravitational pressure takes over and compresses the central core, increasing its density and temperature until the oxygen-burning process can start.
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The oxygen fuel within the core of the star is exhausted after 0.01–5 years, depending on the star's mass and other parameters. The silicon-burning process, which follows, creates iron, but this iron cannot react further to create energy to support the star. During the oxygen-burning process, proceeding outward, there is an oxygen-burning shell, followed by a neon shell, a carbon shell, a helium shell, and a hydrogen shell.
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Essentially, the oxygen (O) atom is stripped from the additional water (steam) to oxidize CO to CO. This oxidation also provides energy to maintain the reaction. Additional heat required to drive the process is generally supplied by burning some portion of the methane.
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6 sinne gevind in 5 ms. Hulle kom uit baie bronne en word nie nagegaan nie.