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Last update: December 1, 2025

Aluminium (Al, Z = 13): From Precious Metal to Everyday Material

Model of the aluminium atom

Simplified atomic model of the aluminium atom. The most abundant isotope is \(\,^{27}\mathrm{Al}\,\) with its 13 protons and 14 neutrons.
Image source: astronoo.com (new window) — AI-generated image, public domain.

Role in astrophysics and cosmochemistry

Aluminium is produced in massive stars through nuclear fusion during the advanced stages of their evolution. The radioactive isotope aluminium-26 (\(\,^{26}\mathrm{Al}\)), with a half-life of 717,000 years, is particularly important in astrophysics. Its decay produces characteristic gamma radiation that allows mapping of active star-forming regions in our galaxy. The presence of aluminium-26 in primitive meteorites indicates that the solar system formed in an environment rich in recent supernovae. This isotope also contributed to the internal heating of the early bodies of the solar system, playing a role in their geochemical differentiation.

History of the discovery of aluminium

Although aluminium is the third most abundant element in the Earth's crust, its extraction has long been a major challenge. In 1807, Humphry Davy (1778-1829) identified the existence of a metal in alumina (aluminium oxide) and proposed the name aluminum. In 1825, Hans Christian Ørsted (1777-1851) produced a small amount of impure aluminium by reducing aluminium chloride with a potassium amalgam. In 1827, Friedrich Wöhler (1800-1882) improved the process and obtained aluminium powder. It was Henri Sainte-Claire Deville (1818-1881) who, in 1854, developed the first industrial process using sodium as a reducing agent. Finally, in 1886, Paul Héroult (1863-1914) in France and Charles Martin Hall (1863-1914) in the United States simultaneously discovered the electrolytic process that revolutionized aluminium production and made it accessible to the general public.

N.B.:
Aluminium was once more precious than gold. In the mid-19th century, before the invention of the Hall-Héroult process, aluminium was more expensive than gold and was reserved for luxury items. Napoleon III owned an aluminium table service that he reserved for his most prestigious guests, while others had to make do with gold tableware. The top of the Washington Monument, inaugurated in 1884, was crowned with a 2.8 kg aluminium pyramid, then the largest piece of cast aluminium in the world, a symbol of modernity and technical progress.

Structure and fundamental properties of aluminium

Aluminium (symbol Al, atomic number 13) is a metal from the group 13 elements (formerly group IIIA). Its atom has 13 protons, 13 electrons, and usually 14 neutrons in its only stable isotope (\(\,^{27}\mathrm{Al}\)).
At room temperature, aluminium is a solid, silvery-white, remarkably light metal (density ≈ 2.70 g/cm³), malleable, ductile, and an excellent conductor of electricity and heat. The melting point of aluminium: 933.47 K (660.32 °C). The boiling point: 2,792 K (2,519 °C). Aluminium spontaneously forms a thin layer of aluminium oxide (Al₂O₃) on its surface, which remarkably protects it from corrosion.

Table of aluminium isotopes

Aluminium isotopes (key physical properties)
Isotope / NotationProtons (Z)Neutrons (N)Atomic mass (u)Natural abundanceHalf-life / StabilityDecay / Remarks
Aluminium-27 — \(\,^{27}\mathrm{Al}\,\)131426.981539 u100%StableOnly stable isotope of aluminium; basis for all its applications.
Aluminium-26 — \(\,^{26}\mathrm{Al}\)131325.986892 uCosmic trace717,000 yearsRadioactive β\(^+\) and electron capture giving \(\,^{26}\mathrm{Mg}\). Produced in stars and by cosmic rays; used to date meteorites.
Aluminium-28 — \(\,^{28}\mathrm{Al}\)131527.981910 uNot natural2.245 minutesRadioactive β\(^-\) decaying into silicon-28. Produced in the laboratory.
Aluminium-29 — \(\,^{29}\mathrm{Al}\)131628.980445 uNot natural6.56 minutesRadioactive β\(^-\) giving silicon-29. Used in nuclear research.
Other isotopes — \(\,^{21}\mathrm{Al}\) to \(\,^{43}\mathrm{Al}\)138 — 30— (variable)Not naturalMilliseconds to secondsVery unstable isotopes produced artificially; research in nuclear physics.

Electronic configuration and electron shells of aluminium

N.B.:
Electron shells: How electrons are organized around the nucleus (new window).

Aluminium has 13 electrons distributed over three electron shells. Its full electronic configuration is: 1s² 2s² 2p⁶ 3s² 3p¹, or simplified: [Ne] 3s² 3p¹. This configuration can also be written as: K(2) L(8) M(3).

Detailed structure of aluminium shells

K shell (n=1): contains 2 electrons in the 1s subshell. This inner shell is complete and very stable.
L shell (n=2): contains 8 electrons distributed as 2s² 2p⁶. This shell is also complete, forming a noble gas configuration (neon).
M shell (n=3): contains 3 electrons distributed as 3s² 3p¹. The 3s orbitals are complete, while the 3p orbitals contain only one electron out of 6 possible. This outer shell is therefore very incomplete.

Valence electrons and oxidation states of aluminium

Aluminium has 3 valence electrons (configuration 3s² 3p¹) in group 13 of the periodic table. It exhibits only one stable oxidation state: +3 (Al³⁺ ion).

Stability of the Al³⁺ ion

By losing its 3 electrons, aluminium forms the Al³⁺ ion, which adopts the electronic configuration of neon [Ne], giving it great stability. Unlike other metals, aluminium does not exhibit intermediate oxidation states.

Chemical properties and bonds

This electronic structure allows it to form various bonds: ionic with non-metals, metallic in its pure state, and sometimes covalent. It has a strong affinity for oxygen.

Passivation and corrosion resistance

In air, aluminium spontaneously forms a thin layer of Al₂O₃ (alumina) oxide that protects it from corrosion. This natural passivation explains its durability despite its intrinsic reactivity.

Industrial importance

Aluminium is the most used metal after iron, appreciated for its lightness (2.7 g/cm³), good electrical and thermal conductivity, malleability, and strength. It is essential in aeronautics, packaging, construction, and the electrical industry. It is the 3rd most abundant element in the Earth's crust.

Chemical reactivity of aluminium

Despite its high thermodynamic reactivity, aluminium appears chemically inert due to the protective oxide layer that forms instantly on its surface. This passivation can be artificially enhanced by anodization. Aluminium reacts with acids (releasing hydrogen) and strong bases (forming aluminates). At high temperatures, it can reduce many metal oxides in highly exothermic reactions (thermite reaction). Aluminium mainly forms compounds in the +III oxidation state, notably aluminium oxide (Al₂O₃), aluminium chloride (AlCl₃), and aluminium sulphate (Al₂(SO₄)₃).

Industrial and technological applications of aluminium

Economic and environmental importance of aluminium

Aluminium is the most produced non-ferrous metal in the world, with annual production exceeding 65 million tonnes. Its primary production by electrolysis is very energy-intensive, consuming about 15,000 kWh per tonne of aluminium produced. However, aluminium recycling has a remarkable energy balance: remelting recycled aluminium requires only 5% of the energy needed for primary production. About 75% of all aluminium ever produced is still in use today thanks to recycling. This infinite recyclability without loss of quality makes aluminium a key material for the circular economy and ecological transition.

Extraction and production of aluminium

Aluminium is mainly extracted from bauxite, an ore rich in hydrated aluminium oxide. The Bayer process purifies bauxite into alumina (Al₂O₃). Alumina is then reduced to metallic aluminium by the Hall-Héroult process: electrolysis in a bath of molten cryolite at about 960 °C. The main bauxite-producing countries are Australia, Guinea, Brazil, and China. Aluminium production requires a lot of electricity, so it is concentrated in countries with abundant and cheap hydroelectric energy.

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To explore in this category

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The Atom in All Its Forms: From Ancient Intuition to Quantum Mechanics

How Are Electrons Distributed in an Atom?

Half-Life of Nuclides: Implications for Radioactivity and Chronology

Periodic Table of Chemical Elements - History and Organization

Why does life depend so much on oxygen?

Hydrogen (H, Z = 1): The Key to Cosmic Creation

Helium (He, Z = 2): A Relic of the Big Bang and Stellar Actor

Lithium (Li, Z = 3): The Key Element of Modern Batteries

Beryllium (Be, Z = 4): A Rare Metal with Exceptional Properties

Boron (B, Z = 5): A Key Element in Materials Science

Carbon (C, Z = 6): The Element of Life

Nitrogen (N, Z = 7): The Abundant and Inert Element in the Atmosphere

Oxygen (O, Z = 8): The Element at the Heart of Life

Fluorine (F, Z = 9): The Reactive and Essential Chemical Element

Neon (Ne, Z = 10): The Noble Element of Rare Gases

Sodium (Na, Z = 11): The Reactive and Versatile Element

Magnesium (Mg, Z = 12): The Essential Element for Biology and Industry

Aluminum (Al, Z = 13): The Light and Versatile Element

Silicon (Si, Z = 14): The Key Element of Earth and Modern Technologies

Phosphorus (P, Z = 15): A Fundamental Element for Life

Sulfur (S, Z = 16): The Essential Element for Life and Industry

Chlorine (Cl, Z = 17): The Key Element in the Chemical Industry and Disinfection

Argon (Ar, Z = 18): The Noble Element of the Atmosphere

Potassium (K, Z = 19): From Fire on Water to the Beating of the Heart

Calcium (Ca, Z = 20): Architect of Bones and Sculptor of Mountains

Scandium (Sc, Z = 21): The Triumph of Scientific Prediction

Titanium (Ti, Z = 22): A Light Metal with Extraordinary Properties

Vanadium (V, Z = 23): A Strategic Metal with Multiple Facets

Chromium (Cr, Z = 24): A Brilliant Metal with Remarkable Properties

Manganese (Mn, Z = 25): A Transition Metal with Multiple Facets

Iron (Fe, Z = 26): The Metallic Pillar of Our Civilization

Cobalt (Co, Z = 27): A Magnetic Metal with Strategic Properties

Nickel (Ni, Z = 28): A Resistant Metal with Magnetic Properties

Copper (Z=29): A Conductive Metal with Remarkable Properties

Zinc (Zn, Z = 30): A Protective Metal with Essential Properties

Gallium (Ga, Z = 31): The Metal with Extraordinary Physical Properties

Germanium (Ge, Z = 32): The Metalloid That Pioneered the Electronic Age

Arsenic (As, Z = 33): The Metalloid with Two Faces

Selenium (Se, Z = 34): The Essential Photoelectric Element

Bromine (Br, Z = 35): The Liquid Halogen with Toxic Vapors

Krypton (Kr, Z = 36): The Noble Gas with Spectral Lights

Rubidium (Rb, Z = 37): The Alkali Metal of Atomic Clocks

Strontium (Sr, Z = 38): The Metal of Red Fireworks

Yttrium (Y, Z = 39): A Rare Earth with Revolutionary Technological Applications

Zirconium (Zr, Z = 40): The Ultra-Resistant Metal of Nuclear Reactors

Niobium (Nb, Z = 41): The Superconductor of CERN and Modern Steels

Molybdenum (Mo, Z = 42): The Essential Metal for High-Performance Steels

Technetium (Tc, Z = 43): The First Entirely Artificial Element

Ruthenium (Ru, Z = 44): The Precious Metal of Advanced Technologies

Rhodium (Rh, Z = 45): The Most Precious Metal in the World

Palladium (Pd, Z = 46): The Hydrogen Sponge of Green Technologies

Silver (Ag, Z = 47): The Millennial Metal with Record Conductivity

Cadmium (Cd, Z = 48): The Controversial Metal of Ni-Cd Batteries

Indium (In, Z = 49): The Invisible Element of Modern Screens

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Tellurium (Te, Z = 52): The Rare Metalloid of Renewable Energies

Iodine (I, Z = 53): The Violet Halogen Essential for Life

Xenon (Xe, Z = 54): The Rare Noble Gas with Exceptional Properties

Cesium (Cs, Z = 55): The Most Reactive Metal and Keeper of Time

Barium (Ba, Z = 56): The Heavy Metal of Medical Imaging

Lanthanum (La, Z = 57): The Standard-Bearer of Rare Earths

Cerium (Ce, Z = 58): The Paradoxically Abundant Rare Earth

Praseodymium (Pr, Z = 59): The Green Rare Earth

Neodymium (Nd, Z = 60): The King of Permanent Magnets

Promethium (Pm, Z = 61): The Phantom Rare Earth

Samarium (Sm, Z = 62): A Terrestrial Magnet with Stellar Origins

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Holmium (Ho, Z = 67): The Magnetic Atom of Medical Lasers

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Thulium (Tm, Z = 69): The Atom of Laser Light and X-Rays

Ytterbium (Yb, Z = 70): The Atom of Time and Laser Light

Lutetium (Lu, Z = 71): The Ultimate Rare Earth Gem

Hafnium (Hf, Z = 72): The Atom of Nuclear Reactors and Microprocessors

Tantalum (Ta, Z = 73): The Metal of Life and High Technology

Tungsten (W, Z = 74): The Metal that Defies Fire

Rhenium (Re, Z = 75): The Metal of Records and High Technology

Osmium (Os, Z = 76): The Metal of Extreme Density and Hardness

Iridium (Ir, Z = 77): Witness to Celestial Cataclysms

Platinum (Pt, Z = 78): The Unalterable King of Precious Metals

Gold (Au, Z = 79): The Metal of Eternity and Wealth

Mercury (Hg, Z = 80): The Liquid and Toxic Metal

Thallium (Tl, Z = 81): The Perfect Poison and the Element of Shadows

Lead (Pb, Z = 82): The Heavy Metal of Civilization and Toxicity

Bismuth (Bi, Z = 83): The Heavy and Colorful Metal for Medical Applications

Polonium (Po, Z = 84): The Element of Radioactivity and Danger

Astatine (At, Z = 85): The Phantom of the Periodic Table

Radon (Rn, Z = 86): The Domestic Radioactive Gas

Francium (Fr, Z = 87): The Elusive Alkali

Radium (Ra, Z = 88): The Element That Glowed in the Dark

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Thorium (Th, Z = 90): An Abundant Nuclear Energy Source

Protactinium (Pa, Z = 91): The Intermediate and Fleeting Element

Uranium (U, Z = 92): The Element with Contained Energy