The Carbon Nitrogen Cycle (CNO) (sometimes called Bethe – Weizsacker cycle) is one of the two known sets of fusion reactions by which stars convert hydrogen to helium, the other being the proton–proton chain reaction (p–p cycle), which is more efficient at the Sun's core temperature. The CNO cycle is hypothesized to be dominant in stars that are more than 1.3 times as massive as the Sun. The required equations are:
\({ }_6^{12} C +{ }_1^1 H \rightarrow{ }_7^{13} N + Q _1 \)
\({ }_7^{13} N \rightarrow{ }_6^{13} C+\left({ }_1^0 {e}\right) + {Q}_2\)
\({ }_6^{13} C +{ }_1^1 H \rightarrow{ }_7^{14} N + Q _3 \)
\({ }_7^{14} N +1 H \rightarrow{ }_8^{15} O + Q _4 \)
\({ }_8^{15} O \rightarrow{ }_7^{15} N +\left({ }_1^0 e \right)+ Q _5 \)
\({ }_7^{15} N +1 H \rightarrow{ }_6^{12} C +{ }_2^4 He + Q _6\)
Overall reaction:
\(4_1^1 H \rightarrow{ }_2^4 He +2\left({ }_1^0 e \right)+ Q \quad\) where \(Q = Q _1+ Q _2+ Q _3+ Q _4+ Q _5+ Q _6\) and theoretically it is net energy released in Carbon - Nitrogen cycle.
It can be seen that carbon along with hydrogen and in final reaction carbon is the product. Thus, carbon act as a catalyst in the overall reaction.