The process of fusion, where hydrogen is fused into heavier elements, releasing energy in the process.
That would be nuclear fusion, like what happens in stars, when two hydrogen nuclei combine to form a helium nucleus.
This description fits the definition of a star, specifically the sun. Stars are massive celestial bodies primarily composed of hydrogen atoms that undergo nuclear fusion to produce heat and light.
Hydrogen and helium are primarily formed inside stars through nuclear fusion processes. As stars age and go through various stages of stellar evolution, they can also produce heavier elements such as carbon, oxygen, and iron through fusion reactions in their cores.
Hydrogen atoms have one proton in their nuclei. When two hydrogen atoms fuse together they make one helium atom that contains two protons in its nucleus. This is called nuclear fusion, which powers the stars in the universe.
Stars that are currently forming in the vicinity of the Sun have a high hydrogen content, typically around 70-75% of their mass. Hydrogen is the main fuel source for nuclear fusion in these young stars, as they convert hydrogen into helium in their cores.
Stars like our sun and hydrogen bombs produce energy through nuclear fusion.
Both hydrogen bombs and stars produce energy through nuclear fusion reactions that convert hydrogen atoms into helium. This process releases a tremendous amount of energy in the form of light and heat.
The cores of stars and hydrogen bombs.
In the cores of stars and hydrogen bombs.
This is produced by nuclear fusion
fusion reactions, where lighter elements combine to release tremendous amounts of energy. In stars, the fusion of hydrogen into helium powers their luminosity and heat. Hydrogen bombs use isotopes of hydrogen to trigger a controlled fusion reaction, releasing a massive amount of explosive energy.
Nuclear fusion. Stars like the sun are basically hydrogen bombs at their core. Hydrogen bombs are fusion bombs, building heavier elements up from hydrogen in their high pressure and temperature cores. All the chemical elements in your body apart from hydrogen were built up in stars that exploded long, long ago,
Stars obtain energy through the majority of their lives by the process of thermonuclear fusion of the nuclei of light elements to produce nuclei of heavier elements. Initially the processes fuses hydrogen nuclei, producing helium nuclei (similar to what hydrogen bombs do), but the process ceases when it produces nickel and iron nuclei at which point the star begins dying as it has run out of nuclear fuel.
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.
Stars produce light by "burning" hydrogen in a nuclear fusion, whereas some animals produce light when chemical compounds mix together to produce a glow
In nuclear physics and nuclear chemistry, nuclear fusionis the process by which multiple like-charged atomic nuclei join together to form a heavier nucleus. It is accompanied by the release or absorption of energy.
Stars are huge balls of glowing gas, primarily hydrogen and helium, that produce light and energy through nuclear fusion in their cores.