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fusion point - перевод на немецкий
![Melting points (in blue) and boiling points (in pink) of the first eight [[carboxylic acids]] (°C)](https://commons.wikimedia.org/wiki/Special:FilePath/Carboxylic.Acids.Melting.&.Boiling.Points.jpg?width=200 "Melting points (in blue) and boiling points (in pink) of the first eight [[carboxylic acids]] (°C)")
![The [[nuclear binding energy]] curve. The formation of nuclei with masses up to [[iron-56]] releases energy, as illustrated above.](https://commons.wikimedia.org/wiki/Special:FilePath/Binding energy curve - common isotopes.svg?width=200 "The [[nuclear binding energy]] curve. The formation of nuclei with masses up to [[iron-56]] releases energy, as illustrated above.")
![The [[CNO cycle]] dominates in stars heavier than the Sun.](https://commons.wikimedia.org/wiki/Special:FilePath/CNO Cycle.svg?width=200 "The [[CNO cycle]] dominates in stars heavier than the Sun.")
![The [[proton–proton chain]] reaction, branch I, dominates in stars the size of the Sun or smaller.](https://commons.wikimedia.org/wiki/Special:FilePath/Fusion in the Sun.svg?width=200 "The [[proton–proton chain]] reaction, branch I, dominates in stars the size of the Sun or smaller.")
![The [[electrostatic force]] between the positively charged nuclei is repulsive, but when the separation is small enough, the quantum effect will tunnel through the wall. Therefore, the prerequisite for fusion is that the two nuclei be brought close enough together for a long enough time for quantum tunneling to act.](https://commons.wikimedia.org/wiki/Special:FilePath/Nuclear fusion forces diagram.svg?width=200 "The [[electrostatic force]] between the positively charged nuclei is repulsive, but when the separation is small enough, the quantum effect will tunnel through the wall. Therefore, the prerequisite for fusion is that the two nuclei be brought close enough together for a long enough time for quantum tunneling to act.")
![The ''[[Tokamak à configuration variable]]'', research fusion reactor, at the [[École Polytechnique Fédérale de Lausanne]] (Switzerland).](https://commons.wikimedia.org/wiki/Special:FilePath/TCV vue gen.jpg?width=200 "The ''[[Tokamak à configuration variable]]'', research fusion reactor, at the [[École Polytechnique Fédérale de Lausanne]] (Switzerland).")
Определение
Википедия
The melting point (or, rarely, liquefaction point) of a substance is the temperature at which it changes state from solid to liquid. At the melting point the solid and liquid phase exist in equilibrium. The melting point of a substance depends on pressure and is usually specified at a standard pressure such as 1 atmosphere or 100 kPa.
When considered as the temperature of the reverse change from liquid to solid, it is referred to as the freezing point or crystallization point. Because of the ability of substances to supercool, the freezing point can easily appear to be below its actual value. When the "characteristic freezing point" of a substance is determined, in fact, the actual methodology is almost always "the principle of observing the disappearance rather than the formation of ice, that is, the melting point."
