The energy in stars is created when hydrogren plasma, under extreme pressure and temperature, fuses to make helium plasma. The difference in mass between hydrogren and helium is also a difference in binding energy, which is released during the ongoing fusion reaction.
Nuclear fusion.
The energy source of stars
The process that supplies the energy for the stars is nuclear fusion. Nuclear fusion is a process in which atomic nuclei combine to form a heavier nucleus, releasing a large amount of energy in the process. In stars, the fusion of hydrogen atoms into helium is the primary source of energy. Under the intense heat and pressure of a star's core, hydrogen atoms are fused together to form helium, releasing a tremendous amount of energy in the form of light and heat. This process is what allows stars to shine and provides the energy necessary to sustain life on Earth.
Nuclear Fusion
gravitational pull
create energy
The energy comes from "nuclear fusion". Stars like the Sun create helium from hydrogen by this method, and that gives out energy. That's how the Sun creates energy.
The energy comes from "nuclear fusion". Stars like the Sun create helium from hydrogen by this method, and that gives out energy. That's how the Sun creates energy.
The energy source of stars
Nuclear fusion.
create energy
Create energy
This process is called photosynthesis.
Nuclear fusion is the process that produces energy in the stars, including our sun
Nuclear fusion
We know that that process is what goes on inside stars and generates the energy they radiate into space, and we cause the same process to occur and to generate energy in nuclear power plants and weapons.
The process that supplies the energy for the stars is nuclear fusion. Nuclear fusion is a process in which atomic nuclei combine to form a heavier nucleus, releasing a large amount of energy in the process. In stars, the fusion of hydrogen atoms into helium is the primary source of energy. Under the intense heat and pressure of a star's core, hydrogen atoms are fused together to form helium, releasing a tremendous amount of energy in the form of light and heat. This process is what allows stars to shine and provides the energy necessary to sustain life on Earth.