It is Nuclear fusion, and the energy released is directly proportional to the mass, as in Einstein's equation E=MC2. All stars in theory begin with Hydrogen, two H atoms are fused to form Helium, this continues until Iron, when it takes more energy to fuse the nuclei than is released, thus ending the life of the star
nucleur fusion
A star gets its energy from nuclear fusion reactions that occur in its core. These reactions fuse lighter elements, such as hydrogen, into heavier elements, releasing energy in the process. This energy is what fuels a star's brightness and heat.
Nuclear fusion. This is the process of fusing two atoms together to make a heavier one. Don't confuse this with nuclear fission, though. Fission is the process of splitting atoms apart (that is what we use for nuclear power plants.)
A star shines due to nuclear fusion in its core, where hydrogen atoms combine to form helium, releasing energy in the process. This energy radiates outwards, providing the star with heat and light. This process can last for billions of years until the star exhausts its nuclear fuel.
nuclear fusion
nuclear fusion
nuclear fusion
Nuclear fusion, of lighter elements onto heavier elements.
It is Nuclear fusion, and the energy released is directly proportional to the mass, as in Einstein's equation E=MC2. All stars in theory begin with Hydrogen, two H atoms are fused to form Helium, this continues until Iron, when it takes more energy to fuse the nuclei than is released, thus ending the life of the star
A nuclear reaction - either fusion or fission - is required to turn matter into energy.
Nuclear fusion, of lighter elements onto heavier elements.
Energy in a star's core is generated through nuclear fusion, where hydrogen atoms combine to form helium releasing a massive amount of energy in the process. The extreme temperature and pressure in the core of a star make this fusion process possible, sustaining the star's energy output.
A process called nuclear fusion.
energy released during the process of nuclear fusion in the star's core
nucleur fusion
A star gets its energy from nuclear fusion reactions that occur in its core. These reactions fuse lighter elements, such as hydrogen, into heavier elements, releasing energy in the process. This energy is what fuels a star's brightness and heat.