Plasma : The Fourth State of Matter
Plasma (from Ancient Greek πλάσμα, meaning "moldable substance"
is one of the four fundamental states of matter, and was first described by
chemist Irving Langmuir in the 1920s. Unlike the other three states, solid,
liquid, and gas, plasma does not exist
freely on the Earth's surface under
normal conditions. Plasma can only be artificially generated by heating or
subjecting a neutral gas to a strong electromagnetic field to the point an
ionised gaseous substance becomes increasingly electrically conductive, and
long-range electromagnetic fields dominate the behavior of the matter.
Plasma and ionised gases have unique properties and display behaviors
unlike those of the other states, and the transition between them is mostly a
matter of nomenclature and subject to interpretation. Based on the surrounding
environmental temperature and density, partially ionised or fully ionised forms
of plasma may be produced. Neon signs or lightning storms are examples of
partially ionised plasma, while the interior of the Sun is an example of fully
ionised plasma,along with the solar corona and stars.
Positive charges in ions is achieved by stripping away electrons orbiting
the atomic nuclei, where the total number of electrons removed is only related
to either increasing temperature or the local density of other ionised matter.
This also can be accompanied by the dissociation of molecular bonds, though
this process is distinctly different from chemical processes of ion interactions
in liquids or the behavior of shared ions in metals. The response of plasma to
electromagnetic fields can be usefully employed in many modern technological
devices, such as plasma televisions or plasma etching.
Plasma may be the most abundant form of ordinary matter in the universe, although
this hypothesis is currently tentative based on the existence and unknown
properties of dark matter. Plasma is mostly associated with stars, extending to
the rarefied intracluster medium and possibly the intergalactic regions.
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