1) Nuclear fusion occurs inside the core of stars where extreme pressure and heat cause hydrogen atoms to fuse together, forming helium and releasing energy. 2) The temperature in a star's core is over 15 million kelvins and the density is over 150 times greater than water, creating the conditions for nuclear fusion. 3) During nuclear fusion, the nuclei of hydrogen atoms combine to form helium, releasing a large amount of energy in the process. This energy flows outward from the core, balancing the inward force of gravity in the star.