What are stars? Stars are massive balls of glowing gas held together by gravity. The primary fuel of stars is hydrogen, which, through the process of nuclear fusion, gets converted into helium, releasing huge amounts of energy in the form of light and heat. This energy is what makes stars shine and supports them against gravitational collapse. Stars come in different sizes, colors, and stages of life, and their evolution is dictated by their mass. For example, more massive stars burn their fuel faster and have shorter lifespans compared to smaller stars.