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The CNO cycle is a series of nuclear fusion reactions which convert four hydrogen nuclei to a helium nucleus, releasing energy in the process. The CNO cycle dominates the nuclear reactions in stars with more than three times the mass of the Sun.
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CNO cycleWikipedia, the free encyclopedia - Cite This Source The CNO cycle (for carbon-nitrogen-oxygen), or sometimes Bethe-Weizsäcker- cycle, is one of two fusion reactions by which stars convert hydrogen to helium, ...
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CNO cycle/process -- a reaction involving carbon, nitrogen, and oxygen (C, N, and O) that fuses hydrogen into helium and releases energy. The process begins with a hydrogen nucleus fusing with a carbon nucleus.
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CNO CycleOne way that a star converts hydrogen into helium. During the CNO cycle, carbon, nitrogen, and oxygen catalyze the nuclear reaction, so the total number of carbon, nitrogen, and oxygen nuclei remains the same.
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CNO cycle - (n.) A nuclear- fusion-reaction sequence in which hydrogen nuclei are combined to form helium nuclei, and in which other nuclei, such as isotopes of carbon, oxygen, and nitrogen, appear as catalysts or by-products.
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CNO Cycle - The series of reactions by means of which massive stars fuse hydrogen into heliumCollision Fragment - A satellite which probably is a fragment of a larger satellite broken apart by a collision with a meteoroid ...
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CNO cycleA series of nuclear reactions in which carbon is used as a catalyst to transform hydrogen into helium. co-creation theory ...
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Study the CNO cycle reactions shown in Figure 11-9 and the reaction list in the inset box. Things on the left side of the arrows are inputs to the reactions. Things on the right side are outputs.
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There is another set of reactions in the Sun called the CNO cycle because they involve carbon, nitrogen and oxygen. This cycle was thought to be the main source of the Sun's energy.
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Larger stars, whose crushing weight generates even higher temperatures at their cores, utilize a more complex fusion process called the " CNO cycle.
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1938 - Hans Bethe and Carl von Weizsacker detail the proton-proton chain and CNO cycle in stars 1939 - Rupert Wildt realizes the importance of the negative hydrogen ion for stellar opacity ...
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See also: Cycle, Energy, Hydrogen, Mass, Helium
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