Aluminio
Aluminio
Aluminium is remarkable for its low density and its ability to resist corrosion
through the phenomenon of passivation. Aluminium and its alloys are vital to the
aerospace industry[8] and important in transportation and building industries, such
as building facades and window frames.[9] The oxides and sulfates are the most
useful compounds of aluminium.[8]
Despite its prevalence in the environment, no known form of life uses aluminium
salts metabolically, but aluminium is well tolerated by plants and animals.[10]
Because of these salts' abundance, the potential for a biological role for them is
of continuing interest, and studies continue.
Contents
1 Physical characteristics
1.1 Nuclei and isotopes
1.2 Electron shell
1.3 Bulk
2 Chemistry
2.1 Inorganic compounds
2.1.1 Rarer oxidation states
2.1.1.1 Aluminium(I)
2.1.1.2 Aluminium(II)
2.2 Organoaluminium compounds and related hydrides
3 Natural occurrence
3.1 In space
3.2 On Earth
4 History
5 Etymology
5.1 Spelling
6 Production and refinement
6.1 Bayer process
6.2 Hall�H�roult process
6.3 Recycling
7 Applications
7.1 Metal
7.2 Compounds
8 Biology
8.1 Toxicity
8.2 Effects
8.3 Exposure routes
8.4 Treatment
9 Environmental effects
10 See also
11 Notes
12 References
13 Bibliography
14 Further reading
15 External links
Physical characteristics
Nuclei and isotopes
Main article: Isotopes of aluminium
Of aluminium isotopes, only 27
Al
is stable. This is consistent with aluminium having an odd atomic number.[b] It is
the only aluminium isotope that has existed on Earth in its current form since the
creation of the planet. Very nearly all the element on Earth is present as this
isotope, which makes aluminium a mononuclidic element and means that its standard
atomic weight practically equates to that of the isotope. The standard atomic
weight of aluminium is low in comparison with many other metals,[c] which has
consequences for the element's properties (see below). This makes aluminium very
useful in nuclear magnetic resonance (NMR), as its single stable isotope has a high
NMR sensitivity.[12]
All other isotopes of aluminium are radioactive. The most stable of these is 26Al
(half-life 720,000 years) and therefore could not have survived since the formation
of the planet. However, minute traces of 26Al are produced from argon in the
atmosphere by spallation caused by cosmic ray protons. The ratio of 26Al to 10Be
has been used for radiodating of geological processes over 105 to 106 year time
scales, in particular transport, deposition, sediment storage, burial times, and
erosion.[13] Most meteorite scientists believe that the energy released by the
decay of 26Al was responsible for the melting and differentiation of some asteroids
after their formation 4.55 billion years ago.[14]
The remaining isotopes of aluminium, with mass numbers ranging from 22 to 43, all
have half-lives well under an hour. Three metastable states are known, all with
half-lives under a minute.[11]
Electron shell
An aluminium atom has 13 electrons, arranged in an electron configuration of
[Ne]3s23p1,[15] with three electrons beyond a stable noble gas configuration.
Accordingly, the combined first three ionization energies of aluminium are far
lower than the fourth ionization energy alone.[16] Such an electron configuration
is shared with the other well-characterized members of its group, boron, gallium,
indium, and thallium; it is also expected for nihonium. Aluminium can relatively
easily surrender its three outermost electrons in many chemical reactions (see
below). The electronegativity of aluminium is 1.61 (Pauling scale).[17]
Bulk
Aluminium metal has an appearance ranging from silvery white to dull gray,
depending on the surface roughness. A fresh film of aluminium serves as a good
reflector (approximately 92%) of visible light and an excellent reflector (as much
as 98%) of medium and far infrared radiation.
The density of aluminium is 2.70 g/cm3, about 1/3 that of steel, much lower than
other commonly encountered metals, making aluminium parts easily identifiable
through their lightness.[21] Aluminium's low density compared to most other metals
arises from the fact that its nuclei are much lighter, while difference in the unit
cell size does not compensate for this difference. The only lighter metals are the
metals of groups 1 and 2, which apart from beryllium and magnesium are too reactive
for structural use (and beryllium is very toxic).[22] Aluminium is not as strong or
stiff as steel, but the low density makes up for this in the aerospace industry and
for many other applications where light weight is crucial.
Pure aluminium is quite soft and lacking in strength. In most applications various
aluminium alloys are used instead because of their higher strength and hardness.
The yield strength of pure aluminium is 7�11 MPa, while aluminium alloys have yield
strengths ranging from 200 MPa to 600 MPa.[23] Aluminium is ductile, and malleable
allowing it to be easily drawn and extruded. It is also easily machined, and the
low melting temperature of 660 �C allows for easy casting.
Etched surface from a high purity (99.9998%) aluminium bar, size 55�37 mm
Chemistry
Main article: Compounds of aluminium
Aluminium combines characteristics of pre- and post-transition metals. Since it has
few available electrons for metallic bonding, like its heavier group 13 congeners,
it has the characteristic physical properties of a post-transition metal, with
longer-than-expected interatomic distances.[20] Furthermore, as Al3+ is a small and
highly charged cation, it is strongly polarizing and aluminium compounds tend
towards covalency;[25] this behaviour is similar to that of beryllium (Be2+), an
example of a diagonal relationship.[26] However, unlike all other post-transition
metals, the underlying core under aluminium's valence shell is that of the
preceding noble gas, whereas for gallium and indium it is that of the preceding
noble gas plus a filled d-subshell, and for thallium and nihonium it is that of the
preceding noble gas plus filled d- and f-subshells. Hence, aluminium does not
suffer the effects of incomplete shielding of valence electrons by inner electrons
from the nucleus that its heavier congeners do. Aluminium's electropositive
behavior, high affinity for oxygen, and highly negative standard electrode
potential are all more similar to those of scandium, yttrium, lanthanum, and
actinium, which have ds2 configurations of three valence electrons outside a noble
gas core: aluminium is the most electropositive metal in its group.[20] Aluminium
also bears minor similarities to the metalloid boron in the same group; AlX3
compounds are valence isoelectronic to BX3 compounds (they have the same valence
electronic structure), and both behave as Lewis acids and readily from adducts.[27]
Additionally, one of the main motifs of boron chemistry is regular icosahedral
structures, and aluminium forms an important part of many icosahedral quasicrystal
alloys, including the Al�Zn�Mg class.[28]
Aluminium reacts with most nonmetals upon heating, forming compounds such as
aluminium nitride (AlN), aluminium sulfide (Al2S3), and the aluminium halides
(AlX3). It also forms a wide range of intermetallic compounds involving metals from
every group on the periodic table. Aluminium has a high chemical affinity to
oxygen, which renders it suitable for use as a reducing agent in the thermite
reaction. A fine powder of aluminium metal reacts explosively on contact with
liquid oxygen; under normal conditions, however, aluminium forms a thin oxide layer
that protects the metal from further corrosion by oxygen, water, or dilute acid, a
process termed passivation.[25][29] This layer is destroyed by contact with mercury
due to amalgamation or with salts of some electropositive metals.[25] As such, the
strongest aluminium alloys are less corrosion-resistant due to galvanic reactions
with alloyed copper,[23] and aluminium's corrosion resistance is greatly reduced by
aqueous salts, particularly in the presence of dissimilar metals.[20] In addition,
although the reaction of aluminium with water at temperatures below 280 �C is of
interest for the production of hydrogen, commercial application of this fact has
challenges in circumventing the passivating oxide layer, which inhibits the
reaction, and in storing the energy required to regenerate the aluminium metal.[30]
In hot concentrated hydrochloric acid, aluminium reacts with water with evolution
of hydrogen, and in aqueous sodium hydroxide or potassium hydroxide at room
temperature to form aluminates�protective passivation under these conditions is
negligible.[31] The reaction with aqueous alkali is often written:[25]
Inorganic compounds
The vast majority of compounds, including all aluminium-containing minerals and all
commercially significant aluminium compounds, feature aluminium in the oxidation
state 3+. The coordination number of such compounds varies, but generally Al3+ is
either six- or four-coordinate. Almost all compounds of aluminium(III) are
colorless.[25]
Al2O3 + 3 SiO2
fuse
?
Al2(SiO3)3
Al2O3 + CaO
fuse
?
Ca(AlO2)2
This behaviour of Al(OH)3 is termed amphoterism, and is characteristic of weakly
basic cations that form insoluble hydroxides and whose hydrated species can also
donate their protons. Further examples include Be2+, Zn2+, Ga3+, Sn2+, and Pb2+;
indeed, gallium in the same group is slightly more acidic than aluminium. One
effect of this is that aluminium salts with weak acids are hydrolysed in water to
the aquated hydroxide and the corresponding nonmetal hydride: aluminium sulfide
yields hydrogen sulfide, aluminium nitride yields ammonia, and aluminium carbide
yields methane. Aluminium cyanide, acetate, and carbonate exist in aqueous solution
but are unstable as such; only incomplete hydrolysis takes place for salts with
strong acids, such as the halides, nitrate, and sulfate. For similar reasons,
anhydrous aluminium salts cannot be made by heating their "hydrates": hydrated
aluminium chloride is in fact not AlCl3�6H2O but [Al(H2O)6]Cl3, and the Al�O bonds
are so strong that heating is not sufficient to break them and form Al�Cl bonds
instead:[25]
2[Al(H2O)6]Cl3
heat
?
Al2O3 + 6 HCl + 9 H2O
All four trihalides are well known. Unlike the structures of the three heavier
trihalides, aluminium fluoride (AlF3) features six-coordinate aluminium, which
explains its involatility and insolubility as well as high heat of formation. Each
aluminium atom is surrounded by six fluorine atoms in a distorted octahedral
arrangement, with each fluorine atom being shared between the corners of two
octahedra in a structure related to but distorted from that of ReO3. Such {AlF6}
units also exist in complex fluorides such as cryolite, Na3AlF6, but should not be
considered as [AlF6]3- complex anions as the Al�F bonds are not significantly
different in type from the other M�F bonds.[34] Such differences in coordination
between the fluorides and heavier halides are not unusual, occurring in SnIV and
BiIII as well for example; even bigger differences occur between CO2 and SiO2.[34]
AlF3 melts at 1,290 �C (2,354 �F) and is made by reaction of aluminium oxide with
hydrogen fluoride gas at 700 �C (1,292 �F).[34]
The only stable chalcogenides under normal conditions are aluminium sulfide
(Al2S3), selenide (Al2Se3), and telluride (Al2Te3). All three are prepared by
direct reaction of their elements at about 1,000 �C (1,832 �F) and quickly
hydrolyse completely in water to yield aluminium hydroxide and the respective
hydrogen chalcogenide. As aluminium is a small atom relative to these chalcogens,
these have four-coordinate tetrahedral aluminium with various polymorphs having
structures related to wurtzite, with two-thirds of the possible metal sites
occupied either in an orderly (a) or random (�) fashion; the sulfide also has a ?
form related to ?-alumina, and an unusual high-temperature hexagonal form where
half the aluminium atoms have tetrahedral four-coordination and the other half have
trigonal bipyramidal five-coordination.[37] Four pnictides, aluminium nitride
(AlN), aluminium phosphide (AlP), aluminium arsenide (AlAs), and aluminium
antimonide (AlSb), are known. They are all III-V semiconductors isoelectronic to
silicon and germanium, all of which but AlN have the zinc blende structure. All
four can be made by high-temperature (and possibly high-pressure) direct reaction
of their component elements.[37]
Aluminium(I)
Main article: Aluminium(I)
AlF, AlCl, AlBr, and AlI exist in the gaseous phase when the respective trihalide
is heated with aluminium, and at cryogenic temperatures. Their instability in the
condensed phase is due to their ready disproportionation to aluminium and the
respective trihalide: the reverse reaction is favored at high temperature (although
even then they are still short-lived), explaining why AlF3 is more volatile when
heated in the presence of aluminium metal, as is aluminium metal when heated in the
presence of AlCl3.[34]
Aluminium(II)
Very simple Al(II) compounds are invoked or observed in the reactions of Al metal
with oxidants. For example, aluminium monoxide, AlO, has been detected in the gas
phase after explosion[39] and in stellar absorption spectra.[40] More thoroughly
investigated are compounds of the formula R4Al2 which contain an Al�Al bond and
where R is a large organic ligand.[41]
Natural occurrence
See also: List of countries by bauxite production
In space
Aluminium's per-particle abundance in the Solar System is 3.15 ppm (parts per
million).[46][d] It is the twelfth most abundant of all elements and third most
abundant among the elements that have odd atomic numbers, after hydrogen and
nitrogen.[46] The only stable isotope of aluminium, 27Al, is the eighteenth most
abundant nucleus in the Universe. It is created almost entirely after fusion of
carbon in massive stars that will later become Type II supernovae: this fusion
creates 26Mg, which, upon capturing free protons and neutrons becomes aluminium.
Some smaller quantities of 27Al are created in hydrogen burning shells of evolved
stars, where 26Mg can capture free protons.[47] Essentially all aluminium now in
existence is 27Al; 26Al was present in the early Solar System but is currently
extinct. However, the trace quantities of 26Al that do exist are the most common
gamma ray emitter in the interstellar gas.[47]
On Earth
Bauxite, a major aluminium ore. The red-brown color is due to the presence of iron
oxide minerals.
Overall, the Earth is about 1.59% aluminium by mass (seventh in abundance by mass).
[48] Aluminium occurs in greater proportion in the Earth than in the Universe
because aluminium easily forms the oxide and becomes bound into rocks and aluminium
stays in the Earth's crust while less reactive metals sink to the core.[47] In the
Earth's crust, aluminium is the most abundant (8.3% by mass) metallic element and
the third most abundant of all elements (after oxygen and silicon).[49] A large
number of silicates in the Earth's crust contain aluminium.[50] In contrast, the
Earth's mantle is only 2.38% aluminium by mass.[51]
Because of its strong affinity for oxygen, aluminium is almost never found in the
elemental state; instead it is found in oxides or silicates. Feldspars, the most
common group of minerals in the Earth's crust, are aluminosilicates. Aluminium also
occurs in the minerals beryl, cryolite, garnet, spinel, and turquoise.[52]
Impurities in Al2O3, such as chromium and iron, yield the gemstones ruby and
sapphire, respectively.[53] Native aluminium metal can only be found as a minor
phase in low oxygen fugacity environments, such as the interiors of certain
volcanoes.[54] Native aluminium has been reported in cold seeps in the northeastern
continental slope of the South China Sea. It is possible that these deposits
resulted from bacterial reduction of tetrahydroxoaluminate Al(OH)4-.[55]
Although aluminium is a common and widespread element, not all aluminium minerals
are economically viable sources of the metal. Almost all metallic aluminium is
produced from the ore bauxite (AlOx(OH)3�2x). Bauxite occurs as a weathering
product of low iron and silica bedrock in tropical climatic conditions.[56] In
2017, most bauxite was mined in Australia, China, Guinea, and India.[57]
History
Main article: History of aluminium
Friedrich W�hler, the chemist who first thoroughly described metallic elemental
aluminium
The history of aluminium has been shaped by usage of alum. The first written record
of alum, made by Greek historian Herodotus, dates back to the 5th century BCE.[58]
The ancients are known to have used alum as a dyeing mordant and for city defense.
[58] After the Crusades, alum, an indispensable good in the European fabric
industry,[59] was a subject of international commerce;[60] it was imported to
Europe from the eastern Mediterranean until the mid-15th century.[61]
The nature of alum remained unknown. Around 1530, Swiss physician Paracelsus
suggested alum was a salt of an earth of alum.[62] In 1595, German doctor and
chemist Andreas Libavius experimentally confirmed this.[63] In 1722, German chemist
Friedrich Hoffmann announced his belief that the base of alum was a distinct earth.
[64] In 1754, German chemist Andreas Sigismund Marggraf synthesized alumina by
boiling clay in sulfuric acid and subsequently adding potash.[64]
Attempts to produce aluminium metal date back to 1760.[65] The first successful
attempt, however, was completed in 1824 by Danish physicist and chemist Hans
Christian �rsted. He reacted anhydrous aluminium chloride with potassium amalgam,
yielding a lump of metal looking similar to tin.[66][67] He presented his results
and demonstrated a sample of the new metal in 1825.[68][69] In 1827, German chemist
Friedrich W�hler repeated �rsted's experiments but did not identify any aluminium.
[70] (The reason for this inconsistency was only discovered in 1921.)[71] He
conducted a similar experiment in the same year by mixing anhydrous aluminium
chloride with potassium and produced a powder of aluminium.[67] In 1845, he was
able to produce small pieces of the metal and described some physical properties of
this metal.[71] For many years thereafter, W�hler was credited as the discoverer of
aluminium.[72]
The statue of Anteros in Piccadilly Circus, London, was made in 1893 and is one of
the first statues cast in aluminium.
As W�hler's method could not yield great quantities of aluminium, the metal
remained rare; its cost exceeded that of gold.[70] The first industrial production
of aluminium was established in 1856 by French chemist Henri Etienne Sainte-Claire
Deville and companions.[73] Deville had discovered that aluminium trichloride could
be reduced by sodium, which was more convenient and less expensive than potassium,
which W�hler had used.[74] Even then, aluminium was still not of great purity and
produced aluminium differed in properties by sample.[75]
Prices of aluminium dropped and aluminium became widely used in jewelry, everyday
items, eyeglass frames, optical instruments, tableware, and foil in the 1890s and
early 20th century. Aluminium's ability to form hard yet light alloys with other
metals provided the metal many uses at the time.[79] During World War I, major
governments demanded large shipments of aluminium for light strong airframes.[80]
By the mid-20th century, aluminium had become a part of everyday life and an
essential component of housewares.[81] During the mid-20th century, aluminium
emerged as a civil engineering material, with building applications in both basic
construction and interior finish work,[82] and increasingly being used in military
engineering, for both airplanes and land armor vehicle engines.[83] Earth's first
artificial satellite, launched in 1957, consisted of two separate aluminium semi-
spheres joined together and all subsequent space vehicles have used aluminium to
some extent.[78] The aluminium can was invented in 1956 and employed as a storage
for drinks in 1958.[84]
The real price for aluminium declined from $14,000 per metric ton in 1900 to $2,340
in 1948 (in 1998 United States dollars).[85] Extraction and processing costs were
lowered over technological progress and the scale of the economies. However, the
need to exploit lower-grade poorer quality deposits and the use of fast increasing
input costs (above all, energy) increased the net cost of aluminium;[86] the real
price began to grow in the 1970s with the rise of energy cost.[87] Production moved
from the industrialized countries to countries where production was cheaper.[88]
Production costs in the late 20th century changed because of advances in
technology, lower energy prices, exchange rates of the United States dollar, and
alumina prices.[89] The BRIC countries' combined share in primary production and
primary consumption grew substantially in the first decade of the 21st century.[90]
China is accumulating an especially large share of world's production thanks to
abundance of resources, cheap energy, and governmental stimuli;[91] it also
increased its consumption share from 2% in 1972 to 40% in 2010.[92] In the United
States, Western Europe, and Japan, most aluminium was consumed in transportation,
engineering, construction, and packaging.[93]
Etymology
Aluminium is named after alumina, or aluminium oxide in modern nomenclature. The
word "alumina" comes from "alum", the mineral from which it was collected. The word
"alum" comes from alumen, a Latin word meaning "bitter salt".[94] The word alumen
stems from the Proto-Indo-European root *alu- meaning "bitter" or "beer".[95]
Spelling
The -ium suffix followed the precedent set in other newly discovered elements of
the time: potassium, sodium, magnesium, calcium, and strontium (all of which Davy
isolated himself). Nevertheless, element names ending in -um were known at the
time; for example, platinum (known to Europeans since the 16th century), molybdenum
(discovered in 1778), and tantalum (discovered in 1802). The -um suffix is
consistent with the universal spelling alumina for the oxide (as opposed to
aluminia); compare to lanthana, the oxide of lanthanum, and magnesia, ceria, and
thoria, the oxides of magnesium, cerium, and thorium, respectively.
In 1812, British scientist Thomas Young[100] wrote an anonymous review of Davy's
book, in which he objected to aluminum and proposed the name aluminium: "for so we
shall take the liberty of writing the word, in preference to aluminum, which has a
less classical sound."[101] This name did catch on: while the -um spelling was
occasionally used in Britain, the American scientific language used -ium from the
start.[102] Most scientists used -ium throughout the world in the 19th century;
[103] it still remains the standard in most other languages.[99] In 1828, American
lexicographer Noah Webster used exclusively the aluminum spelling in his American
Dictionary of the English Language.[104] In the 1830s, the -um spelling started to
gain usage in the United States; by the 1860s, it had become the more common
spelling there outside science.[102] In 1892, Hall used the -um spelling in his
advertising handbill for his new electrolytic method of producing the metal,
despite his constant use of the -ium spelling in all the patents he filed between
1886 and 1903. It was subsequently suggested this was a typo rather than intended.
[99] By 1890, both spellings had been common in the U.S. overall, the -ium spelling
being slightly more common; by 1895, the situation had reversed; by 1900, aluminum
had become twice as common as aluminium; during the following decade, the -um
spelling dominated American usage.[105] In 1925, the American Chemical Society
adopted this spelling.[105]
The International Union of Pure and Applied Chemistry (IUPAC) adopted aluminium as
the standard international name for the element in 1990.[106] In 1993, they
recognized aluminum as an acceptable variant;[106] the most recent 2005 edition of
the IUPAC nomenclature of inorganic chemistry acknowledges this spelling as well.
[107] IUPAC official publications use the -ium spelling as primary but lists both
where appropriate.[e]