Astronoo - Back to homepage
X (new window) Bluesky (new window) Pinterest (new window)
English Français Español Português 日本語 Deutsch 中文
Last update: December 18, 2025

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

Model of the yttrium atom

Image description: Simplified atomic model of the yttrium atom. The most abundant (and only stable) isotope is \(\,^{89}\mathrm{Y}\,\) with its 39 protons, 39 electrons, and 50 neutrons.
Image source: astronoo.com (new window) — AI-generated image, public domain.

History of the Discovery of Yttrium

Yttrium has a fascinating history linked to a small Swedish village that gave its name to four chemical elements. In 1787, Swedish lieutenant and amateur chemist Carl Axel Arrhenius (1757-1824) discovered near the village of Ytterby (located on the island of Resarö in the Stockholm archipelago) an unusual black mineral that he named ytterbite (now called gadolinite).

In 1794, Finnish chemist Johan Gadolin (1760-1852) analyzed this mineral and isolated what he believed to be a new earth oxide, which he named yttria (yttrium oxide, Y₂O₃). However, this oxide actually contained several mixed rare earth elements, and it took over a century to separate them all.

Pure yttrium metal was not isolated until 1828 by German chemist Friedrich Wöhler (1800-1882), who managed to reduce yttrium chloride (YCl₃) with potassium. However, the metal obtained still contained impurities. It was not until the early 20th century, with the development of more sophisticated separation techniques, that truly pure yttrium was obtained.

The name yttrium comes from the village of Ytterby, which also gave its name to three other elements discovered in the same ore: ytterbium (Yb), terbium (Tb), and erbium (Er). No other place in the world has given its name to as many chemical elements.

Structure and Fundamental Properties

Yttrium (symbol Y, atomic number 39) is a transition metal in group 3 of the periodic table. Although chemically very similar to the lanthanides (rare earths), it is not strictly part of them because it has no electrons in the 4f orbitals. Its atom has 39 protons, 50 neutrons (for the stable isotope \(\,^{89}\mathrm{Y}\)) and 39 electrons with the electronic configuration [Kr] 4d¹ 5s².

At room temperature, yttrium is a bright silvery-white solid metal, relatively light for a transition metal (density ≈ 4.47 g/cm³). It has a hexagonal close-packed crystal structure at room temperature, which transforms into a body-centered cubic structure above 1,478 °C.

Yttrium is a relatively soft and ductile metal that can be easily machined, rolled, and drawn. It has good electrical and thermal conductivity, typical of transition metals. Like most rare earths, yttrium is paramagnetic at room temperature.

A remarkable property of yttrium is its strong affinity for oxygen. At room temperature, it quickly forms a thin oxide layer (Y₂O₃) that partially protects it from further oxidation. However, in the presence of moisture or at high temperatures, oxidation becomes faster. Finely divided yttrium can even be pyrophoric (spontaneously ignite in air).

Melting point of yttrium (liquid state): 1,799 K (1,526 °C).
Boiling point of yttrium (gaseous state): 3,609 K (3,336 °C).

Table of Yttrium Isotopes

Yttrium isotopes (key physical properties)
Isotope / NotationProtons (Z)Neutrons (N)Atomic mass (u)Natural abundanceHalf-life / StabilityDecay / Remarks
Yttrium-89 — \(\,^{89}\mathrm{Y}\,\)395088.905848 u100 %StableOnly stable and natural isotope of yttrium. Mononuclidic element.
Yttrium-90 — \(\,^{90}\mathrm{Y}\,\)395189.907152 uSynthetic≈ 64.0 hoursRadioactive (β⁻). Pure beta emitter used in radiotherapy and nuclear medicine to treat certain cancers (radioactive microspheres).
Yttrium-88 — \(\,^{88}\mathrm{Y}\,\)394987.909501 uSynthetic≈ 106.6 daysRadioactive (electron capture, β⁺). Positron emitter used in PET imaging (positron emission tomography).
Yttrium-91 — \(\,^{91}\mathrm{Y}\,\)395290.907305 uSynthetic≈ 58.5 daysRadioactive (β⁻). Fission product in nuclear reactors. Contributor to radioactive fallout.
Yttrium-87 — \(\,^{87}\mathrm{Y}\,\)394886.910876 uSynthetic≈ 79.8 hoursRadioactive (electron capture, β⁺). Used in medical research.

Electronic Configuration and Electron Shells of Yttrium

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

Yttrium has 39 electrons distributed over five electron shells. Its full electronic configuration is: 1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹ 5s², or simplified: [Kr] 4d¹ 5s². This configuration can also be written as: K(2) L(8) M(18) N(8) O(3).

Detailed Structure of the 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 18 electrons distributed as 3s² 3p⁶ 3d¹⁰. This shell is complete with the 3d subshell fully filled.
N shell (n=4): contains 8 electrons distributed as 4s² 4p⁶. This shell has a noble gas configuration (krypton), which is why the simplified electronic configuration starts with [Kr].
O shell (n=5): contains 3 electrons distributed as 4d¹ 5s². These three electrons are the valence electrons of yttrium.

Valence Electrons and Oxidation States

The 3 electrons in the outer shell (4d¹ 5s²) are the valence electrons of yttrium. This configuration explains its chemical properties:

The almost exclusive oxidation state of yttrium is +3, where it loses its three valence electrons to form the Y³⁺ ion with the stable configuration [Kr] (isoelectronic with krypton). This noble gas configuration with complete subshells is extremely stable, which is why yttrium almost exclusively forms compounds with an oxidation state of +3.

Oxidation states of +2 and +1 have been observed in very rare organometallic compounds or under extreme experimental conditions, but they are very unstable and quickly re-oxidize. The +3 state completely dominates the chemistry of yttrium.

Chemical Reactivity

Yttrium is a relatively reactive metal, particularly with oxygen and water. At room temperature, it quickly forms a thin oxide layer (Y₂O₃) that partially protects it from further oxidation. However, this protection is imperfect, especially in the presence of moisture.

Yttrium reacts slowly with oxygen at room temperature but vigorously at high temperatures (>400 °C), forming yttrium(III) oxide: 4Y + 3O₂ → 2Y₂O₃. Finely divided yttrium can spontaneously ignite in air (pyrophoric), emitting intense light.

With water, yttrium reacts slowly at room temperature but rapidly when heated, forming yttrium hydroxide and releasing hydrogen gas: 2Y + 6H₂O → 2Y(OH)₃ + 3H₂. This reaction accelerates considerably with increasing temperature.

Yttrium reacts with all acids, even diluted ones, to form yttrium(III) salts and release hydrogen: 2Y + 6HCl → 2YCl₃ + 3H₂. It also dissolves in concentrated strong bases, forming complex hydroxides.

With halogens, yttrium reacts vigorously to form trihalides: 2Y + 3X₂ → 2YX₃ (where X = F, Cl, Br, I). It also reacts with sulfur, selenium, tellurium, nitrogen (forming nitride Y₃N₅ at high temperature), carbon (forming carbides YC₂ and Y₂C₃), and many other non-metals.

Yttrium oxide (Y₂O₃), also called yttria, is a particularly important compound. It is a very thermally stable (melting point: 2,425 °C) and chemically inert white powder. It has a cubic bixbyite-type crystal structure and is used in many technological applications.

Industrial and Technological Applications of Yttrium

Role in Astrophysics and Cosmology

Yttrium is synthesized in stars through several nucleosynthesis processes. It is mainly formed during the explosive burning of silicon during type II supernova explosions, which produces nuclei in the mass region A ≈ 90. the s-process (slow neutron capture) in AGB stars (asymptotic giant branch) also contributes to the production of yttrium.

The stable isotope \(\,^{89}\mathrm{Y}\) is the only natural isotope of yttrium (mononuclidic element), which simplifies the study of its cosmic abundance. This isotopic uniqueness reflects the particular stability of the nucleus with 39 protons and 50 neutrons, close to the magic neutron number N = 50.

The abundance of yttrium in the universe is relatively high for a rare earth element, about 5 × 10⁻¹⁰ times that of hydrogen in number of atoms. This abundance places it at the level of neodymium or samarium among the lanthanides, although it is not itself a lanthanide.

The yttrium/iron ([Y/Fe]) ratio measured in old metal-poor stars provides important information on primordial nucleosynthesis. Very old stars in the galactic halo show a relatively constant [Y/Fe] ratio, suggesting that both yttrium and iron are mainly produced by type II supernovae, although by different processes.

The spectral lines of ionized yttrium (Y II) are easily observable in stellar spectra and are important indicators of the chemical composition of stars. The Y II line at 3982.6 Å is particularly used in stellar spectroscopy. The study of these lines in stars of different populations (young, old, metal-poor) allows tracing the history of the chemical enrichment of the Galaxy.

In primitive meteorites, the analysis of yttrium abundances and other refractory elements helps to understand the processes of condensation and chemical fractionation in the primitive solar nebula. Yttrium, being a refractory element (condensing at high temperature), is preferentially concentrated in certain types of minerals in the oldest meteorites.

The radioactive isotopes of yttrium, notably ⁸⁸Y and ⁹⁰Y, are produced during supernova explosions and briefly contribute (from a few months to a few years) to the residual luminosity of these events. The study of these isotopes helps to understand the detailed mechanisms of stellar explosions.

N.B.:
Yttrium is present in the Earth's crust at a concentration of about 0.0033% by mass (33 ppm), making it more abundant than lead, tin, or molybdenum. Contrary to its name "rare earth," yttrium is not particularly rare; this historical name refers to the difficulty of its extraction and purification rather than its absolute rarity.

Yttrium does not form its own ores but is always associated with lanthanides in rare earth minerals. The main minerals containing yttrium are xenotime (YPO₄, yttrium phosphate rich in heavy rare earths, containing up to 60% Y₂O₃), bastnäsite ((Ce,La,Y)CO₃F, fluorocarbonate of light rare earths with 0.1 to 10% Y₂O₃), monazite ((Ce,La,Nd,Th)PO₄, rare earth phosphate containing 2 to 3% Y₂O₃), and the ion adsorption clays of southern China (rich in medium and heavy rare earths including yttrium).

The extraction of yttrium is complex and costly. The ores are first attacked by concentrated acids to dissolve the rare earths. Then, sophisticated separation techniques are employed: solvent extraction (using organic chelating agents), ion exchange on specific resins, or fractional precipitation. These processes must be repeated many times because the chemical properties of rare earths are extremely similar. The final reduction of Y₂O₃ oxide to yttrium metal is done by metallothermic reduction (with calcium) under vacuum or inert atmosphere, followed by distillation to remove excess calcium.

Global production of rare earth oxides containing yttrium is dominated by China (≈ 60% of world production), followed by the United States, Australia, Myanmar, and India. Major deposits include Bayan Obo in Inner Mongolia (China), Mountain Pass in California (United States), Mount Weld in Australia, and the ionic clays of Jiangxi (China). Annual yttrium production is about 8,900 tons (expressed as Y₂O₃ equivalent).

The recycling of yttrium is becoming strategically important with the rapid growth in demand (≈ 8% per year), particularly for permanent magnets, phosphors from used screens, and catalysts. However, the current recycling rate remains low (<1%) due to technical complexity and the high cost of recovery processes. The European Union and the United States classify yttrium as a critical strategic material due to its importance for advanced technologies (renewable energies, defense, electronics) and the geographical concentration of its production.

🏠

To explore in this category

The energies required for nuclear fusion and why uranium is a limit
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

Tin (Sn, Z = 50): The Ancestral Metal of the Bronze Age

Antimony (Sb, Z = 51): The Overlooked Strategic Metalloid

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

Europium (Eu, Z = 63): The Red Luminescent Phosphor

Gadolinium (Gd, Z = 64): The Magnetic Atom of Medical Imaging

Terbium (Tb, Z = 65): The Green Luminescent and Magnetic Atom

Dysprosium (Dy, Z = 66): The Magnetic Atom of Green Energy

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

Erbium (Er, Z = 68): The Fundamental Dopant of Fiber Optic Networks

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

Actinium (Ac, Z = 89): A Key Element of the Actinide Series

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