Final answer:
Once a star reaches the main-sequence stage, it generates internal energy through hydrogen fusion, creating helium.
Step-by-step explanation:
Once a star reaches the main-sequence stage of its life, it derives its energy by converting hydrogen into helium through nuclear fusion in its core. This process can maintain the star's equilibrium for a long time, keeping it on the main sequence. So, the correct answer is option a: The star is generating internal energy by hydrogen fusion, creating helium.