Binding energy
The binding energy of atomic nuclei plotted against the atomic number of the nuclei.
BINDING ENERGY1 - Amount of energy released at the creation of a particular isotope. Protons and neutron are held together by the "strong force".
Binding Energy
The energy needed to pull an electron away from its atom.
Bipolar Flow ...
Binding energy is the mechanical energy required to disassemble a whole into separate parts. A bound system has a lower potential energy than its constituent parts; this is what keeps the system together....
of specific isotope
Isotope ...
Binding energy of an atomic nucleus. The energy holding a nucleus together, balancing the attraction of the strong nuclear (attractive) force and the electrical repulsion of a large number of positive protons, confined together in a small space.
Binding Energy
(a) The energy required to break up a system. In particular, the binding energy of an atomic nucleus is the energy released in the formation of the nucleus.
binding energy - (n.)
Energy derived from the conversion of mass to energy when neutrons and protons are combined to form nuclei.
blackbody - (n.) ...
binding energy (Plasma Physics and Fusion Energy Glossary) Energy required to separate two objects; conversely, energy released when two objects are allow to bind together. Equivalent to the mass defect via E=mc^2.
thermionic emission Direct ejection of electrons as the result of heating and material, which raises electron energy beyond the binding energy that holds the electron in the material.
*Gravitational binding energy
*Gravitational collapse
*Gravitational constant
*Gravitational field
*Gravitational force
*Gravitational instability
*Gravitational lens
*Gravitational lensing
*Gravitational microlensing ...
These processes are able to create elements up to iron and nickel, the region of the isotopes having the highest binding energy per nucleon.
In particular, the binding energy of an atomic nucleus is the energy released in the formation of the nucleus. The most strongly bound nuclei are those with atomic weights between about 50 and 65 (the iron group).
The energy released in most nuclear reactions is much larger than that in chemical reactions, because the binding energy that holds a nucleus together is far greater than the energy that holds electrons to a nucleus.
The laws of motion do not require that bodies move in circles (or even ellipses for that matter), but if they have some binding energy, they must move in ellipses (not counting perturbations by other bodies), ...
The binding energy of a neutron star is much less than that of a non-collapsed stellar core. The tremendous amount of energy generated by the neutron star formation drives the supernova.
Iron is said to have the greatest nuclear binding energy of any element. Any nucleus with more or fewer protons or neutrons has less nuclear binding energy and is not quite so stable as the iron-56 nucleus.
The planet's internal heat was originally released during its accretion (see gravitational binding energy), and since then additional heat has continued to be generated by the decay of radioactive elements such as uranium, thorium, and potassium.
Many of these appear to be fairly uniform, so by the virial theorem the total kinetic energy should be half the total gravitational binding energy of the galaxies.
In the AGB phase, the outer layers of the star will be greatly extended and will not be strongly bound. Mass loss, pulsations, and a low binding energy of the outer layers can cause them to be released from the star, ...
Prominences, flares, coronal mass ejections
Helioseismology : observations and internal structure
The sun's energy source
Inadequacy of chemical or gravitational energy sources
Binding energy curve for all elements : ...
 See also: Energy, Time, Element, Temperature, Mass
  
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