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1. Stars

   Linked via "mass-luminosity relation"

   The primary mechanism sustaining main-sequence stars is the fusion of hydrogen into helium. For solar-mass stars, this occurs predominantly via the Proton-Proton (pp) Chain-chain/). More massive stars utilize the more temperature-sensitive Carbon-Nitrogen-Oxygen (CNO) Cycle-cycle/) [3].
   The lifespan of a star (astronomical object)/) is inversely proportional to its initial […