Erbium (Er)
lanthanideSolid
Standard Atomic Weight
167.259 uElectron configuration
[Xe] 6s2 4f12Melting point
1528.85 °C (1802 K)Boiling point
2867.85 °C (3141 K)Density
9070 kg/m³Oxidation states
0, +1, +2, +3Electronegativity (Pauling)
1.24Ionization energy (1st)
Discovery year
1843Atomic radius
175 pmDetails
Erbium is a lanthanide metal and one of the heavier rare-earth elements. In compounds it is dominated by the +3 oxidation state, giving many salts a characteristic pale pink color. Its greatest technological importance comes from optical transitions of Er³⁺ ions, especially in silica glass, where they enable amplification near 1.55 micrometres for fiber-optic communications. It occurs in nature with other rare earths rather than as a native metal.
The pure metal is soft and malleable and has a bright, silvery, metallic luster. As with other rare-earth metals, its properties depend to a certain extent on the impurities present. The metal is fairly stable in air and does not oxidize as rapidly as some of the other rare-earth metals. Naturally occurring erbium is a mixture of six isotopes, all of which are stable. Nine radioactive isotopes of erbium are also recognized. Recent production techniques, using ion-exchange reactions, have resulted in much lower prices of the rare-earth metals and their compounds in recent years. Most of the rare-earth oxides have sharp absorption bands in the visible, ultraviolet, and near infrared. This property, associated with the electronic structure, gives beautiful pastel colors to many of the rare-earth salts.
The name derives from the Swedish town of Ytterby, where the ore gadolinite (in which it was found) was first mined. Erbium was discovered by the Swedish surgeon and chemist Carl-Gustav Mosander in 1843 in a yttrium sample. He separated the yttrium into yttrium, a rose-coloured salt he called terbium and a deep-yellow peroxide that he called erbium.
The mineral gadolinite ((Ce, La, Nd, Y)2FeBe2Si2O10), discovered in a quarry near the town of Ytterby, Sweden, has been the source of a great number of rare earth elements. In 1843, Carl Gustaf Mosander, a Swedish chemist, was able to separate gadolinite into three materials, which he named yttria, erbia and terbia. As might be expected considering the similarities between their names and properties, scientists soon confused erbia and terbia and, by 1877, had reversed their names. What Mosander called erbia is now called terbia and visa versa. From these two substances, Mosander discovered two new elements, terbium and erbium. Today, erbium is primarily obtained through an ion exchange process from the minerals xenotime (YPO4) and euxenite ((Y, Ca, Er, La, Ce, U, Th)(Nb, Ta, Ti)2O6).
Erbium, one of the so-called rare-earth elements on the lanthanide series, is found in the minerals mentioned under dysprosium. In 1842 Mosander separated "yttria" found in the mineral gadolinite, into three fractions which he called yttria, erbia, and terbia. The names erbia and terbia became confused in this early period. After 1860, Mosander's terbia was known as erbia, and after 1877, the earlier known erbia became terbia. The erbia of this period was later shown to consist of five oxides, now known as erbia, scandia, holmia, thulia and ytterbia. By 1905 Urbain and James independently succeeded in isolating fairly pure Er2O3. Klemm and Bommer first produced reasonably pure erbium metal in 1934 by reducing the anhydrous chloride with potassium vapor.
Images
Properties
Physical
Chemical
Thermodynamic
Nuclear
Abundance
Reactivity
N/A
Crystal Structure
Electronic Structure
Identifiers
Electron Configuration Measured
Er: 4f¹² 6s²[Xe] 4f¹² 6s²1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 5s² 5p⁶ 4f¹² 6s²Atomic model
Isotopes change neutron count, mass, and stability — not the electron configuration of a neutral atom.
Schematic atomic model, not to scale.
Atomic Fingerprint
Emission / Absorption Spectrum
Isotope Distribution
| Mass number | Atomic mass (u) | Natural abundance | Half-life |
|---|---|---|---|
| 164 Stable | 163.9292088 ± 0.000002 | 1.6010% | Stable |
| 166 Stable | 165.9302995 ± 0.0000022 | 33.5030% | Stable |
| 167 Stable | 166.9320546 ± 0.0000022 | 22.8690% | Stable |
| 168 Stable | 167.9323767 ± 0.0000022 | 26.9780% | Stable |
Phase / State
Reason: 1503.8 °C below melting point (1528.85 °C)
Schematic, not to scale
Phase transition points
Transition energies
Energy required to melt 1 mol at melting point
Energy required to vaporize 1 mol at boiling point
Energy required to sublime 1 mol at sublimation point
Density
At standard conditions
At standard conditions
Atomic Spectra
Showing 10 of 68 Atomic Spectra. Sorted by ion charge (ascending).
Lines Holdings ?
| Ion | Charge | Total lines | Transition probabilities | Level designations |
|---|---|---|---|---|
| Er I | 0 | 232 | 11 | 13 |
| Er II | +1 | 285 | 11 | 12 |
| Er III | +2 | 120 | 0 | 0 |
Levels Holdings ?
| Ion | Charge | Levels |
|---|---|---|
| Er I | 0 | 674 |
| Er II | +1 | 362 |
| Er III | +2 | 53 |
| Er IV | +3 | 10 |
| Er V | +4 | 2 |
| Er VI | +5 | 2 |
| Er VII | +6 | 2 |
| Er VIII | +7 | 2 |
| Er IX | +8 | 2 |
| Er X | +9 | 2 |
Ionic Radii
| Charge | Coordination | Spin | Radius |
|---|---|---|---|
| +3 | 6 | N/A | 89 pm |
| +3 | 7 | N/A | 94.5 pm |
| +3 | 8 | N/A | 100.4 pm |
| +3 | 9 | N/A | 106.2 pm |
Compounds
Isotopes (4)
| Mass number | Atomic mass (u) | Natural abundance | Half-life | Decay mode | |
|---|---|---|---|---|---|
| 164 Stable | 163.9292088 ± 0.000002 | 1.6010% ± 0.0030% | Stable | stable | |
| 166 Stable | 165.9302995 ± 0.0000022 | 33.5030% ± 0.0360% | Stable | stable | |
| 167 Stable | 166.9320546 ± 0.0000022 | 22.8690% ± 0.0090% | Stable | stable | |
| 168 Stable | 167.9323767 ± 0.0000022 | 26.9780% ± 0.0180% | Stable | stable |
Extended Properties
Covalent Radii (Extended)
Van der Waals Radii
Atomic & Metallic Radii
Numbering Scales
Electronegativity Scales
Polarizability & Dispersion
Miedema Parameters
Supply Risk & Economics
Phase Transitions & Allotropes
| Melting point | 1802.15 K |
| Boiling point | 3141.15 K |
Oxidation State Categories
Advanced Reference Data
Screening Constants (13)
| n | Orbital | σ |
|---|---|---|
| 1 | s | 1.3263 |
| 2 | p | 4.346 |
| 2 | s | 17.7984 |
| 3 | d | 13.6397 |
| 3 | p | 20.3891 |
| 3 | s | 20.9231 |
| 4 | d | 35.7288 |
| 4 | f | 40.0216 |
| 4 | p | 32.8908 |
| 4 | s | 31.768 |
Crystal Radii Detail (4)
| Charge | CN | Spin | rcrystal (pm) | Origin |
|---|---|---|---|---|
| 3 | VI | 103 | from r^3 vs V plots, | |
| 3 | VII | 108.5 | ||
| 3 | VIII | 114.4 | from r^3 vs V plots, | |
| 3 | IX | 120.2 | from r^3 vs V plots, |
Isotope Decay Modes (52)
| Isotope | Mode | Intensity |
|---|---|---|
| 142 | p | — |
| 143 | B+ | — |
| 143 | B+p | — |
| 144 | B+ | — |
| 145 | B+ | 100% |
| 145 | B+p | — |
| 146 | B+ | 100% |
| 146 | B+p | — |
| 147 | B+ | 100% |
| 147 | B+p | — |
X‑ray Scattering Factors (514)
| Energy (eV) | f₁ | f₂ |
|---|---|---|
| 10 | — | 0.18333 |
| 10.1617 | — | 0.18626 |
| 10.3261 | — | 0.18925 |
| 10.4931 | — | 0.19229 |
| 10.6628 | — | 0.19537 |
| 10.8353 | — | 0.1985 |
| 11.0106 | — | 0.20168 |
| 11.1886 | — | 0.20739 |
| 11.3696 | — | 0.21399 |
| 11.5535 | — | 0.2208 |
Additional Data
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
3.5 milligrams per kilogram
References (1)
Estimated Oceanic Abundance
The estimated element abundance in the earth's oceans.
8.7×10-7 milligrams per liter
References (1)
References
(9)
Data deposited in or computed by PubChem
The half-life and atomic mass data was provided by the Atomic Mass Data Center at the International Atomic Energy Agency.
Element data are cited from the Atomic weights of the elements (an IUPAC Technical Report). The IUPAC periodic table of elements can be found at https://iupac.org/what-we-do/periodic-table-of-elements/. Additional information can be found within IUPAC publication doi:10.1515/pac-2015-0703 Copyright © 2020 International Union of Pure and Applied Chemistry.
The information are cited from Pure Appl. Chem. 2018; 90(12): 1833-2092, https://doi.org/10.1515/pac-2015-0703.
Thomas Jefferson National Accelerator Facility (Jefferson Lab) is one of 17 national laboratories funded by the U.S. Department of Energy. The lab's primary mission is to conduct basic research of the atom's nucleus using the lab's unique particle accelerator, known as the Continuous Electron Beam Accelerator Facility (CEBAF). For more information visit https://www.jlab.org/
The periodic table at the LANL (Los Alamos National Laboratory) contains basic element information together with the history, source, properties, use, handling and more. The provenance data may be found from the link under the source name.
The periodic table contains NIST's critically-evaluated data on atomic properties of the elements. The provenance data that include data for atomic spectroscopy, X-ray and gamma ray, radiation dosimetry, nuclear physics, and condensed matter physics may be found from the link under the source name. Ref: https://www.nist.gov/pml/atomic-spectra-database
This section provides all form of data related to element Erbium.
The element property data was retrieved from publications.

