When different isotopes of hydrogen fuse in the sun, they produce helium nuclei. Specifically, the fusion process in the sun involves the conversion of hydrogen isotopes, such as deuterium and tritium, into helium-4 nuclei, along with the release of energy in the form of gamma rays and solar radiation.
In the sun, hydrogen atoms fuse together to form helium through a process called nuclear fusion. This process releases energy in the form of light and heat, which is what sustains the sun's brightness and temperature.
All stars fuse hydrogen into helium - the slight difference in atomic weight between 4 hydrogen atoms and one helium atom, is given off as radiation.
No, the sun is made primarily of hydrogen and helium, not burning gas. The sun's energy comes from nuclear fusion in its core, where hydrogen atoms fuse to form helium, releasing energy in the process.
Hydrogen is the fuel used by the sun, helium is the waste produced by hydrogen use in the fusion process
Hydrogen atoms fuse into helium.
When hydrogen atoms fuse together in the sun's core, they create helium. This process releases energy in the form of light and heat, which provides the sun's power.
Yes, they do. Because of the enormous gravity of the sun Hydrogen atoms fuse to each other (only 2) to make Helium.
When different isotopes of hydrogen fuse in the sun, they produce helium nuclei. Specifically, the fusion process in the sun involves the conversion of hydrogen isotopes, such as deuterium and tritium, into helium-4 nuclei, along with the release of energy in the form of gamma rays and solar radiation.
When hydrogen nuclei fuse together, they can form helium. This fusion process is the energy source for stars, including our sun, where hydrogen nuclei combine to form helium through a series of nuclear reactions.
Hydrogen is in the sun, when the hydrogen atoms fuse (join together) they make helium in stars. this gives out lots of heat and light.
Hydrogen atoms fuse to become helium atoms during the process of nuclear fusion in stars. This process releases a large amount of energy and is the source of the sun's energy.
In the sun, hydrogen atoms fuse together to form helium through a process called nuclear fusion. This process releases energy in the form of light and heat, which is what sustains the sun's brightness and temperature.
Yes. Hydrogen atoms fuse together to form helium - releasing heat as a by-product. The helium atoms migrate from the centre of the sun to its surface - reverting back to hydrogen as they do so. The cycle repeats itself.
All stars fuse hydrogen into helium - the slight difference in atomic weight between 4 hydrogen atoms and one helium atom, is given off as radiation.
Hydrogen and helium are formed in Sun.
The sun "burns" hydrogen to make helium. At 10 million degrees Kelvin, hydrogen begins to fuse into helium. In other, larger stars all the hydrogen will fuse to become helium, then all the helium will fuse to become beryllium, all the beryllium will fuse to become carbon, and so on, until it reaches iron. Fusion no longer produces energy after iron, so the star either collapses or goes supernova. "Burning" is not the correct term, fusion is.