Nuclear Energy

 

Nuclear Energy is energy due to the splitting (fission) of the nuclei of atom(s). The conversion of nuclear mass to energy is consistent with the mass-energy equivalence formula ΔE = Δm.c², in which ΔE = energy release, Δm = mass defect, and c = the speed of light in a vacuum (a physical constant).

Nuclear energy is released by three exoenergetic (or exothermic) processes:

    * Radioactive decay, where a neutron or proton in the radioactive nucleus decays spontaneously by emitting either particles, electromagnetic radiation (gamma rays), neutrinos (or all of them)
    * Fusion, two atomic nuclei fuse together to form a heavier nucleus
    * Fission, the breaking of a heavy nucleus into two (more rarely three) lighter nuclei

Nuclear energy was first discovered by French physicist Henri Becquerel in 1896, when he found that photographic plates stored in the dark near uranium were blackened like X-ray plates, which had been just recently discovered at the time 1895.

Nuclear chemistry can be used as a form of alchemy to turn lead into gold or change any atom to any other atom (albeit through many steps). Radionuclide (radioisotope) production often involves irradiation of another isotope (or more precisely a nuclide), with alpha particles, beta particles, or gamma rays.

Iron has the highest binding energy per nucleon of any atom. If an atom of lower average binding energy is changed into an atom of higher average binding energy, energy is given off. The chart shows that fusion of hydrogen, the combination to form heavier atoms, releases energy, as does fission of uranium, the breaking up of a larger nucleus into smaller parts. Stability varies between isotopes: the isotope U-235 is much less stable than the more common U-238.

 

 

Related Topics:

Energy

Elastic Energy

Springs

Hooke's Law

Energy

Conservation of Energy

Potential Energy

Chemical Energy

Heat Energy

Kinetic Energy

 

Related Flash Simulations:

Work and Energy