The mass of the star and the related temperature of the stellar core determine the thermonuclear process type of the star. The stars of the solar mass produce energy from Hydrogen in the proton-proton cycle (two and three proton nuclei appear in intermediate stages of the fusion, end product is Helium); stars twice (or more) as heavy run the HNC cycle (Although Helium is here still the end product, Nitrogen and Carbon appear in intermediate fusion stages, too). Once the Hydrogen is used up, gravity collapse makes the temperatures rise until the next , heavier element fusion cycle is activated.
As the temperature rises, other numerous fusion cycles can produce all existing elements. The heaviest ones are created in the extraordinary high temperatures of the supernovae-explosions
In nuclear fusion of hydrogen, the transformation of mass into energy occurs. This is in accordance with Einstein's equation E=mc^2, where a small amount of mass is converted into a large amount of energy.
The nuclear reaction that occurs in the sun is fusion. This process involves the fusing of hydrogen atoms to form helium, releasing a large amount of energy in the form of light and heat. Fusion is the main source of energy for the sun and other stars.
No, normally it occurs at temperatures of millions of degrees. It does occur at room temperature, but not in significant amount; any possible practical use of "cold fusion" is, so far, speculation.
Nuclear fusion occurs in the solar core.
The main thermonuclear reaction in the sun is the fusion of hydrogen nuclei (protons) into helium nuclei. This process, known as nuclear fusion, releases a tremendous amount of heat energy and is responsible for powering the sun and providing light and warmth to the Earth.
In nuclear fusion of hydrogen, the transformation of mass into energy occurs. This is in accordance with Einstein's equation E=mc^2, where a small amount of mass is converted into a large amount of energy.
The nuclear reaction that occurs in the sun is fusion. This process involves the fusing of hydrogen atoms to form helium, releasing a large amount of energy in the form of light and heat. Fusion is the main source of energy for the sun and other stars.
Fusion occurs in the sun.
Fusion occurs in the sun.
Central part of the Sun where nuclear fusion occurs is called core.
Fusion occurs in the core of the Sun
iron
Hydrogen fusion occurs in the core of the sun, where hydrogen atoms combine to form helium through a series of nuclear reactions. This process releases a huge amount of energy in the form of light and heat.
Fusion is a nuclear reaction in which two light atomic nuclei combine to form a heavier nucleus, releasing a large amount of energy in the process. It occurs naturally in the core of stars, including our sun, where high temperatures and pressures allow hydrogen atoms to fuse into helium. Scientists are also working on developing fusion as a potential clean and abundant energy source here on Earth.
fusion
Nuclear fusion occurs in the solar core.
No, normally it occurs at temperatures of millions of degrees. It does occur at room temperature, but not in significant amount; any possible practical use of "cold fusion" is, so far, speculation.