Nuclear Fusion
Produces is the verb.
Stars like our sun and hydrogen bombs produce energy through nuclear fusion.
The sun produces energy through nuclear fusion, a process where hydrogen atoms combine to form helium, releasing vast amounts of energy. This same process serves as the basis for nuclear energy on Earth, where nuclear power plants use controlled nuclear fission reactions to generate electricity.
Stars do not require an atmosphere like Earth's to burn. The nuclear fusion process at their core generates energy, with the high temperatures and pressures sustaining the reaction. Oxygen is not a necessary component for this process to occur.
Nickel and iron accumulate in the interior of large stars and do not release energy by any kind of nuclear reaction.
Nuclear fusion is the process that produces energy in the stars, including our sun
Nuclear fusion is the type of nuclear reaction that takes place in stars. This reaction involves the fusion of hydrogen atoms to form helium, releasing a large amount of energy in the process.
The equation representing the fusion reaction in stars like the Sun is: 4 hydrogen nuclei (protons) -> helium nucleus + energy This fusion process, known as nuclear fusion, occurs in the core of stars and is responsible for the energy that sustains the star's life.
Nuclear fusion is the process that powers stars, including our sun. The intense heat and pressure in the core of a star creates the conditions necessary for nuclear fusion to occur, releasing vast amounts of energy. Scientists are working on harnessing this same process for practical energy production on Earth through nuclear fusion reactors.
Nuclear Fusion
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.
Produces is the verb.
That is called "nuclear fusion".
Stars produce huge amounts of energy through nuclear fusion in their cores. This process involves the fusion of hydrogen atoms to form helium, releasing immense amounts of energy in the form of light and heat. The intense pressure and temperature at the core of a star are necessary for nuclear fusion to occur.
nuclear fusion
One example of a nuclear reaction involving beryllium is the reaction of beryllium-9 with an alpha particle (helium-4 nucleus) to produce carbon-12 and a neutron. This reaction is important in stellar nucleosynthesis and occurs in high-energy environments such as inside stars.