In nuclear fusion, you take 4 atoms of hydrogen, and fuse them into helium. The resulting atom has less mass then the 4 atoms combined. That loss of mass is what we gets as energy.
How much energy you may ask? E = mc2.
The sun's energy comes from a process called nuclear fusion. In the sun's core, hydrogen atoms fuse together to form helium, releasing vast amounts of energy in the process. This is what powers the sun and provides energy to sustain life on Earth.
The energy in the sun is released through nuclear fusion. This process involves the fusion of hydrogen atoms to form helium, releasing large amounts of energy in the form of heat and light.
Nuclear fusion. Stellar fusion in volves a number of different fusion reactions throughout the star's life, but the primary and (usually) the longest burning is the fusion of hydrogen into helium. This consumes most of the nuclear energy in the sun, and it usually accounts for the type of fusion that goes on for most of the life of the star. A link is provided to the Wikipedia article on the proton-proton chain, which is the "technical term" for hydrogen fusion into helium.
The fusion of hydrogen nuclei in the sun produces helium, along with energy in the form of light and heat. This process is known as nuclear fusion and is the source of the sun's energy.
The sun creates energy through nuclear fusion, where hydrogen atoms combine to form helium, releasing immense amounts of energy in the process. This process occurs in the sun's core, where temperatures and pressures are high enough to initiate fusion reactions.
The sun's energy comes from a process called nuclear fusion. In the sun's core, hydrogen atoms fuse together to form helium, releasing vast amounts of energy in the process. This is what powers the sun and provides energy to sustain life on Earth.
Hydrogen is turned into helium in the fusion process that releases the Sun's energy.
Nuclear fusion, hydrogen burns and the energy gets turned into mass
The process responsible for the enormous energy in the Sun is nuclear fusion. In the core of the Sun, hydrogen atoms combine to form helium, releasing a tremendous amount of energy in the process. This energy is what powers the Sun and sustains life on Earth.
Fusion is the process by which the sun produces energy. In the sun's core, hydrogen atoms fuse together to form helium, releasing large amounts of energy in the form of heat and light in the process. This continuous fusion reaction is what powers the sun and allows it to shine.
Nuclear fusion
nuclear fusion
No, nuclear fusion in the sun is not wind energy. Wind energy is generated from the kinetic energy of moving air masses, while nuclear fusion in the sun is the process by which the sun produces energy through the fusion of hydrogen atoms into helium.
The energy in the sun is released through nuclear fusion. This process involves the fusion of hydrogen atoms to form helium, releasing large amounts of energy in the form of heat and light.
Nuclear fusion. Stellar fusion in volves a number of different fusion reactions throughout the star's life, but the primary and (usually) the longest burning is the fusion of hydrogen into helium. This consumes most of the nuclear energy in the sun, and it usually accounts for the type of fusion that goes on for most of the life of the star. A link is provided to the Wikipedia article on the proton-proton chain, which is the "technical term" for hydrogen fusion into helium.
They are the same.
nuclear fusion.