It is thermo-nuclear fusion.
That is two atoms of hydrogen aredraw to each other by gravity. They become so close they fuse together and release energy in the process.
This happens billions of times over in a given locality in space, and as such a star forms.
In stars, the primary nuclear reaction is nuclear fusion, where lighter atomic nuclei combine to form heavier nuclei, releasing vast amounts of energy. The most common fusion process in stars like the Sun is the conversion of hydrogen into helium through a series of reactions known as the proton-proton chain. This reaction releases energy in the form of light and heat, which powers the star and contributes to the processes that sustain life on Earth. In more massive stars, other fusion processes can occur, including the fusion of helium into heavier elements.
In dwarf stars, the fusion of hydrogen into helium primarily occurs through the proton-proton chain reaction. In this process, four hydrogen nuclei (protons) are ultimately converted into one helium-4 nucleus, releasing energy in the form of gamma rays, positrons, and neutrinos. This energy production is what powers dwarf stars, allowing them to maintain stability against gravitational collapse. As hydrogen is consumed, the star evolves, leading to changes in its structure and lifecycle.
The most abundant type of stars is red dwarves.
Correct. M-type stars on the main sequence are called red dwarfs.
stars there called stars
Chemical
It doesn't. The nuclear/chemical reaction that powers the other stars is entirely independent of what our sun is doing.
fermentation
Nuclear fusion is the type of nuclear reaction that occurs in stars. Older stars with a collapsing center can exceed a temperature of one hundred million Kelvin.
a nuclear recation is formed
The most common nuclear reaction is nuclear fusion, where atoms combine to form a heavier nucleus. This reaction is what powers the sun and other stars, as well as hydrogen bombs.
An example of a nuclear reaction is nuclear fusion, where two light atomic nuclei combine to form a heavier nucleus, releasing a large amount of energy in the process. This reaction is the process that powers the sun and other stars.
Stars are powered by nuclear fusion
Helium and a neutron: D + T --> He + n + 17.59 MeV
This involves "nuclear fusion" reactions.
The fusion of hydrogen to helium is a reaction that commonly occurs in the core of stars, including our sun. This process, called nuclear fusion, releases tremendous amounts of energy in the form of light and heat. It is the main source of energy that powers stars and sustains their brightness and heat.
there is light from the sun which over powers the stars