Four protons are fused together to four one helium nucleus The differential strong atomic force is released as energy and gamma radiation. Two of the protons are converted into neutrons, releasing positrons and electron neutrinos.
The core or the sun's photosphere.
In the sun, nuclear fusion occurs when hydrogen atoms combine to form helium. This process releases a large amount of energy in the form of light and heat. The immense pressure and temperature at the sun's core enable this fusion reaction to occur, sustaining the sun's energy output.
The majority of the Sun's radiation output comes from nuclear fusion reactions in its core, where hydrogen atoms are fused into helium. This process releases energy in the form of electromagnetic radiation, including visible light, ultraviolet light, and infrared radiation.
The temperature of the Sun's core is estimated to be around 15 million degrees Kelvin (27 million degrees Fahrenheit). This extreme heat is generated by nuclear fusion reactions that convert hydrogen into helium.
"The core is made of hot, dense gas in the plasmic state"
Helium
The nuclear reactions in the Suns core
nuclear fusion reactions at the core of sun
For nuclear fusion.
Helium is generated in the core of our sun by nuclear synthesis .During the nuclear fusion inside the sun , hydrogen is fused into helium .the main products generated in this reaction are - Gamma ray photon, positron, neutrino, isotopes of hydrogen and helium and large amount of energy .
The core or the sun's photosphere.
The primary source of the sun's energy is nuclear fusion. This process occurs in the sun's core, where hydrogen atoms combine to form helium, releasing vast amounts of energy in the form of light and heat.
The sun crushes hydrogen into helium with its immense gravity. This makes light and heat. This is a nuclear reaction.
The sun crushes hydrogen into helium with its immense gravity. This makes light and heat. This is a nuclear reaction.
Energy is produced in the sun's core through nuclear fusion, where hydrogen atoms combine to form helium, releasing a tremendous amount of energy in the process. The high temperatures and pressures in the core of the sun provide the conditions necessary for nuclear fusion to occur.
The nuclear reaction that combines hydrogen to form helium and produces most of the sun's energy is called nuclear fusion. In this reaction, hydrogen nuclei (protons) fuse together to form helium nuclei, releasing a large amount of energy in the form of light and heat.
The suns core is the innermost portion or the photosphere of the sun. It's the hottest layer and under the highest pressure, enabling nuclear fusion to take place, which produces the energy. The suns core temperature is estimated to be around 13.6 million degrees Kelvin.