The CNO cycle is considered catalytic in stellar nucleosynthesis because carbon is regenerated during the process, allowing it to facilitate further reactions without being consumed. The reactions in the CNO cycle are faster than those in the proton-proton (P-P) chain due to larger cross sections, which enhance the likelihood of interactions. In contrast, the P-P chain involves a weak interaction to form a deuteron from two protons, a process that occurs extremely slowly, estimated at once every few billion years. The CNO cycle's weak interactions, particularly involving nuclei like ^15O and ^13N, occur on a much shorter timescale of minutes. This efficiency in the CNO cycle makes it a more effective mechanism for stellar nucleosynthesis compared to the P-P chain.