Final answer:
The heat and light from stars are produced by the fusion of hydrogen into helium, a process that happens under extreme conditions in the star's core.
Step-by-step explanation:
The heat and light from most stars, including our own Sun, are produced by nuclear fusion, specifically the fusion of hydrogen to form helium. This process occurs under extreme pressure and temperature conditions at the core of the star, where hydrogen nuclei, or protons, combine to create helium in a series of reactions known as the proton-proton chain. This fusion process releases considerable energy, which manifests as the star's radiance and warmth. It's interesting to note that while other processes like radioactive decay, gravitational compression, and electromagnetism play roles in various cosmic phenomena, they are not the primary mechanisms generating heat and light in stable, main-sequence stars.