Boron compounds, particularly borax, have been known since antiquity and were used in glassmaking and as cleaning agents. In 1808, elemental boron was isolated almost simultaneously by two teams of chemists: Joseph Louis Gay-Lussac (1778-1850) and Louis-Jacques Thénard (1777-1857) in France, and Humphry Davy (1778-1829) in England. The French chemists heated boric acid with metallic potassium, while Davy used electrolysis. The name boron derives from the Persian bûrah via the Arabic buraq, which referred to borax. It was not until 1909 that Ezekiel Weintraub (1880-1965) produced boron with over 99% purity by reducing boron halides with hydrogen on a heated tantalum filament.
Boron (symbol B, atomic number 5) is a metalloid located between metals and non-metals in the periodic table, consisting of five protons, usually six neutrons (for the most common isotope), and five electrons. The two stable isotopes are boron-11 \(\,^{11}\mathrm{B}\) (≈ 80.1%) and boron-10 \(\,^{10}\mathrm{B}\) (≈ 19.9%).
At room temperature, elemental boron exists in several allotropic forms. The most stable crystalline form is β-rhombohedral boron, an extremely hard (close to diamond on the Mohs scale), brittle, black solid, and semiconductor. Boron has a moderate density (≈ 2.34 g/cm³) and exceptional resistance to high temperatures. The temperature at which the liquid and solid states can coexist (melting point): 2349 K (2076 °C). The temperature at which it transitions from liquid to gas (boiling point): 4200 K (3927 °C).
| Isotope / Notation | Protons (Z) | Neutrons (N) | Atomic mass (u) | Natural abundance | Half-life / Stability | Decay / Remarks |
|---|---|---|---|---|---|---|
| Boron-8 — \(\,^{8}\mathrm{B}\,\) | 5 | 3 | 8.024607 u | Unnatural | 0.770 s | Radioactive β\(^+\) and alpha particle emission; produced in the Sun via the pp chain. |
| Boron-10 — \(\,^{10}\mathrm{B}\,\) | 5 | 5 | 10.012937 u | ≈ 19.9 % | Stable | High neutron capture cross-section; used as a neutron absorber and in neutron capture therapy. |
| Boron-11 — \(\,^{11}\mathrm{B}\,\) | 5 | 6 | 11.009305 u | ≈ 80.1 % | Stable | Major isotope; used in NMR spectroscopy and the chemical industry. |
| Boron-12 — \(\,^{12}\mathrm{B}\,\) | 5 | 7 | 12.014352 u | Unnatural | 0.0202 s | Radioactive β\(^-\) decay to \(\,^{12}\mathrm{C}\); artificially produced in accelerators. |
| Boron-13 — \(\,^{13}\mathrm{B}\,\) | 5 | 8 | 13.017780 u | Unnatural | 0.0174 s | Radioactive β\(^-\); rapidly decays by emitting electrons. |
| Other isotopes — \(\,^{7}\mathrm{B},\,^{9}\mathrm{B},\,^{14}\mathrm{B}-\,^{19}\mathrm{B}\) | 5 | 2, 4, 9-14 | — (resonances) | Unnatural | \(10^{-21}\) — 0.013 s | Very unstable states observed in nuclear physics; decay by neutron emission or β radioactivity. |
N.B. :
Electron shells: How electrons organize around the nucleus.
Boron has 5 electrons distributed across two electron shells. Its full electronic configuration is: 1s² 2s² 2p¹, or simplified as: [He] 2s² 2p¹. This configuration can also be written as: K(2) L(3).
K Shell (n=1): Contains 2 electrons in the 1s sub-shell. This inner shell is complete and highly stable.
L Shell (n=2): Contains 3 electrons distributed as 2s² 2p¹. The 2s orbitals are complete, while the 2p orbitals contain only one electron out of 6 possible. Thus, 5 electrons are missing to reach the stable neon configuration with 8 electrons (octet).
The 3 electrons in the outer shell (2s² 2p¹) are the valence electrons of boron. This configuration explains its chemical properties:
By losing its 3 valence electrons, boron forms the B³⁺ ion (oxidation state +3), its most common and virtually exclusive oxidation state in its ionic compounds.
Boron can also exhibit oxidation states of 0 (elemental boron) and sometimes +1 or +2 in specific compounds, but these states are rare.
Due to its high charge and small size, the B³⁺ ion is highly polarizing, and boron mainly forms covalent bonds rather than ionic ones.
The electronic configuration of boron, with 3 electrons in its valence shell, places it in group 13 of the periodic table and marks the transition between metals and non-metals. This structure gives it characteristic properties: boron is a metalloid (semi-metal) with intermediate properties between metals and non-metals; it typically forms three covalent bonds by sharing its three valence electrons; and often exhibits electron deficiency in its compounds (fewer than 8 electrons around boron). Boron has a notable particularity: its compounds generally do not obey the octet rule. In BF₃, for example, boron has only 6 valence electrons, making it a Lewis acid (electron acceptor). This electron deficiency makes boron highly reactive toward compounds with free electron pairs. Elemental boron exists in several allotropic forms, all characterized by complex three-dimensional structures.
The importance of boron, although less universal than that of carbon or nitrogen, is significant in several fields: in metallurgy, it is used as a hardening agent in steels and to produce special alloys; boron-10 is used in nuclear reactors as a neutron absorber due to its high neutron capture cross-section; boron compounds such as boric acid H₃BO₃ are used as antiseptics and insecticides; borax (sodium tetraborate) is an important industrial compound used in detergents, glassmaking, and ceramics; boron fibers and boron carbide (B₄C) are extremely hard materials used in armor and high-performance applications; boron is also an essential micronutrient for plants.
Boron has three valence electrons and exhibits unique and complex chemistry. Due to its small atomic size and high electronegativity (for a group 13 element), boron primarily forms covalent bonds rather than ionic bonds. A remarkable feature of boron is its tendency to form molecular structures with multicenter bonds, where an insufficient number of valence electrons are shared among several atoms (three-center, two-electron bonds).
Elemental boron is relatively inert at room temperature due to a protective oxide layer. At high temperatures, it reacts with oxygen to form boron oxide (B₂O₃), with nitrogen to give boron nitride (BN), and with halogens to form trihalides (BF₃, BCl₃). Boranes (boron hydrides) constitute a fascinating class of compounds with varied and unusual geometric structures. Boron also forms borides with many metals, some of which have exceptional hardness.
In its compounds, boron is mainly found in the +3 oxidation state, although lower oxidation states exist in some complex structures. Boron is essential for plants and plays an important role in plant biochemistry, although its exact role in animals remains debated.
Like beryllium and lithium, boron was not produced in significant quantities during the primordial nucleosynthesis of the Big Bang. The primordial universe jumped directly from helium to heavier elements without creating much boron. The boron present in the current universe mainly comes from cosmic spallation: the fragmentation of heavier atoms (carbon, nitrogen, oxygen) by collision with high-energy cosmic rays in the interstellar medium.
The abundance of boron in ancient stars and cosmic rays provides crucial information about the history and intensity of galactic cosmic rays during the evolution of our galaxy. The observed boron/carbon ratio in different regions of the galaxy helps constrain models of cosmic ray propagation and better understand the energetic processes that accelerate them.
In stars, boron is rapidly destroyed at temperatures above about 5 million kelvin by proton capture, making it a sensitive indicator of convective mixing processes in stellar interiors. Astronomers use boron observations in stellar atmospheres to test models of stellar rotation and matter transport in young stars.
Boron also plays a role in explosive nucleosynthesis during supernovae. Nuclear reactions involving boron can occur in the ejected outer layers during the explosion, contributing to the chemical enrichment of the interstellar medium. Boron-8, an unstable radioactive isotope, is produced in the Sun via the proton-proton chain and contributes to the solar neutrino flux detected on Earth, allowing physicists to test models of the solar interior.
The study of the boron-10/boron-11 isotope ratio in primitive meteorites reveals information about the conditions of the early protoplanetary disk and the processes of solar system formation. Isotopic variations of boron in these ancient objects testify to the chemical and physical processes that shaped our planetary system 4.6 billion years ago.
N.B.:
Boranes constitute a fascinating family of hydrogen and boron compounds with unusual molecular structures. The simplest, diborane (B₂H₆), has a structure where hydrogen atoms form "bridges" between two boron atoms via three-center, two-electron bonds. This unique chemistry of boron has revolutionized our understanding of chemical bonding and earned William Lipscomb the Nobel Prize in Chemistry in 1976 for his work on boranes. Complex boranes can form spectacular polyhedral cages like dodecaborate (B₁₂H₁₂²⁻), an icosahedral structure of great stability. These compounds have played an important historical role in the development of modern theoretical chemistry and continue to inspire research in materials chemistry and nanotechnology.
