In chemistry, a 'metal' (
Greek: ''Metallon'') is an
element that readily loses electrons to form positive
ions (cations) and has
metallic bonds between metal atoms. Metals form
ionic bonds with non-metals. They are sometimes described as a
lattice of positive ions surrounded by a cloud of delocalized
electrons. The metals are one of the three groups of elements as distinguished by their ionization and bonding properties, along with the
metalloids and
nonmetals. On the
periodic table, a diagonal line drawn from
boron (B) to
polonium (Po) separates the metals from the nonmetals. Most elements on this line are metalloids, sometimes called
semi-metals; elements to the lower left are metals; elements to the upper right are nonmetals.
An alternative definition of metals is that they have overlapping
conduction bands and
valence bands in their electronic structure. This definition opens up the category for metallic polymers and other organic metals, which have been made by researchers and employed in high-tech devices. These synthetic materials often have the characteristic silvery-grey reflectiveness (luster) of elemental metals.
The traditional definition focuses on the bulk properties of metals. They tend to be lustrous, ductile, malleable, and good
conductors of electricity, while nonmetals are generally brittle (if
solid), lack luster, and are
insulators.
Chemical properties
Most metals are chemically reactive, reacting with oxygen in the air to form oxides over changing timescales (for example iron
rusts over years and
potassium burns in seconds). The
alkali metals react quickest followed by the
alkaline earth metals, found in the leftmost two groups of the
periodic table. The
transition metals take much longer to oxidize (such as
iron,
copper,
zinc,
nickel). Others, like
palladium,
platinum and
gold, do not react with the atmosphere at all. Some metals form a barrier layer of
oxide on their surface which cannot be penetrated by further oxygen molecules and thus retain their shiny appearance and good conductivity for many decades (like
aluminium, some
steels, and
titanium). The
oxides of metals are
basic (as opposed to those of nonmetals, which are
acidic), although this may be considered a rule of thumb, rather than a fact.
Painting or
anodising metals are good ways to prevent their
corrosion. However, a more reactive metal in the
electrochemical series must be chosen for coating, especially when chipping of the coating is expected. Water and the two metals form an
electrochemical cell, and if the coating is less reactive than the coatee, the coating actually ''promotes'' corrosion.
Physical properties
Traditionally, metals have certain characteristic physical properties: they are usually shiny (they have ''metallic
luster''), have a high
density, are
ductile and
malleable, usually have a high
melting point, are usually hard, are usually a solid at room temperature and conduct
electricity,
heat and
sound well. However, this is mainly because the low density, soft, low melting point metals (the
alkali and
alkaline earth metals) happen to be reactive, and we rarely encounter them in their elemental, metallic form.
The electrical and thermal conductivity of metals originate from the fact that in the
metallic bond the outer electrons of the metal
atoms form a gas of nearly free electrons, moving as an electron gas in a background of positive charge formed by the
ion cores. Good mathematical predictions for electrical conductivity, as well as the electrons' contribution to the heat capacity and heat conductivity of metals can be calculated from the
free electron model, which does not take the detailed structure of the ion lattice into account.
When considering the exact band structure and binding energy of a metal, it is necessary to take into account the positive potential caused by the specific arrangement of the ion cores - which is periodic in
crystals. The most important consequence of the periodic potential is the formation of a small
band gap at the boundary of the
brillouin zone. Mathematically, the potential of the ion cores is treated in the
nearly-free electron model.
Alloys
An alloy is a mixture of two or more
elements in
solid solution in which the major component is a metal. Most pure metals are either too soft, brittle or chemically reactive for practical use. Combining different ratios of metals as alloys modify the properties of pure metals to produce desirable characteristics. The aim of making alloys is generally to make them less brittle, harder, resistant to corrosion, or have a more desirable color and luster. Examples of alloys are
steel (
iron and
carbon),
brass (
copper and
zinc),
bronze (
copper and
tin), and
duralumin (
aluminium and
copper). Alloys specially designed for highly demanding applications, such as
jet engines, may contain more than ten elements.
Categories
Base metal
Main articles: Base metal
In
chemistry, the term ''base metal'' is used informally to refer to a metal that
oxidizes or
corrodes relatively easily, and reacts variably with dilute
hydrochloric acid (HCl) to form
hydrogen. Examples include
iron,
nickel,
lead and
zinc.
Copper is considered a base metal as it oxidizes relatively easily, although it does not react with HCl. It is commonly used in opposition to
noble metal.
In
alchemy, a 'base metal' was a common and inexpensive metal, as opposed to
precious metals, mainly
gold and
silver. A longtime goal of the alchemists was the transmutation of base metals into precious metals.
In
numismatics, coins used to derive their value primarily from the
precious metal content. Most modern currencies are
fiat currency, allowing the coins to be made of 'base metal'.
Ferrous metal
Main articles: Ferrous and non-ferrous metals
The term "ferrous" is derived from the
latin word meaning "containing iron". This can include pure iron, such as
wrought iron, or an alloy such as
steel. Ferrous metals are often
magnetic, but not exclusively.
Noble metal
Main articles: Noble metal
'Noble metals' are metals that are resistant to
corrosion or
oxidation, unlike most
base metals. They tend to be precious metals, often due to perceived rarity. Examples include
tantalum,
platinum, and
rhodium.
Precious metal
Main articles: Precious metal
A 'precious metal' is a rare metallic
chemical element of high
economic value.
Chemically, the precious metals are less
reactive than most elements, have high
luster and high electrical conductivity. Historically, precious metals were important as
currency, but are now regarded mainly as investment and industrial
commodities.
Gold,
silver,
platinum and
palladium each have an
ISO 4217 currency code. The best-known precious metals are gold and silver. While both have industrial uses, they are better known for their uses in
art,
jewelry, and
coinage. Other precious metals include the
Platinum group metals:
ruthenium,
rhodium,
palladium,
osmium,
iridium, and
platinum, of which platinum is the most widely traded.
Plutonium and
uranium could also be considered precious metals.
The demand for precious metals is driven not only by their practical use, but also by their role as investments and a
store of value. Palladium was, as of summer 2006, valued at a little under half the price of gold, and platinum at around twice that of gold. Silver is substantially less expensive than these metals, but is often traditionally considered a precious metal for its role in coinage and jewelry.
Extraction
Main articles: Ore,
Mining
Metals are often extracted from the Earth by means of mining, resulting in ores that are relatively rich sources of the requisite elements. Ore is located by
prospecting techniques, followed by the exploration and examination of deposits. Mineral sources are generally divided into
surface mines, which are mined by excavation using heavy equipment, and
subsurface mines.
Once the ore is mined, the metals must be
extracted, usually by chemical or electrolytic reduction.
Pyrometallurgy uses high temperatures to convert ore into raw metals, while
hydrometallurgy employs
aqueous chemistry for the same purpose. The methods used depend on the metal and their contaminants.
Metallurgy
Main articles: Metallurgy
Metallurgy is a domain of materials science that studies the physical and chemical behavior of metallic elements, their intermetallic compounds, and their mixtures, which are called alloys.
Applications
Some metals and metal alloys possess high structural strength per unit mass, making them useful materials for carrying large loads or resisting impact damage. Metal alloys can be engineered to have high resistance to shear, torque and deformation. However the same metal can also be vulnerable to fatigue damage through repeated use, or from sudden stress failure when a load capacity is exceeded. The strength and resilience of metals has led to their frequent use in high-rise building and bridge construction, as well as most vehicles, many appliances, tools, pipes, non-illuminated signs and railroad tracks.
Metals are good conductors, making them valuable in electrical appliances and for carrying an electric current over a distance with little energy lost. Electrical power grids rely on metal cables to distribute electricity. Home electrical systems, for the most part, are wired with copper wire for its good conducting properties.
The thermal conductivity of metal is useful for containers to heat materials over a flame. Metal is also used for
heat sinks to protect sensitive equipment from overheating.
The high reflectivity of some metals is important in the construction of mirrors, including precision astronomical instruments. This last property can also make metallic jewelry aesthetically appealing.
Some metals have specialized uses; Radioactive metals such as
Uranium and
Plutonium are used in
nuclear power plants to produce energy via
nuclear fission. Mercury is a liquid at room temperature and is used in switches to complete a circuit when it flows over the switch contacts.
Shape memory alloy is used for applications such as pipes, fasteners and vascular
stents.
Trade

Metal and
ore imports in 2005
The
World Bank reports that China was the top importer of ores and metals in 2005 followed by the USA and Japan.
Astronomy
Main articles: Metallicity
In the specialised usage of
astronomy and
astrophysics, the term "metal" is often used to refer to any element other than
hydrogen or
helium, and includes substances as chemically non-metallic as
neon,
fluorine, and
oxygen. Because the temperatures of stellar bodies allow practically no solid or liquid matter, and little normal chemistry can exist at temperatures that break down almost all chemical bonds, the term "metal" refers to materials that result from the triple-helium process which are much scarcer than hydrogen and helium in stars in the
main sequence.
See also
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Amorphous metal
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Electric field screening
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Metalworking
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Metallic bond
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Metallurgy
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Steel
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Structural steel
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Transition metal
External links
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