Dysprosium
Dysprosium is a soft, silvery lanthanide first isolated in 1886 after a notoriously difficult separation from holmium — a struggle reflected in its name, Greek for "hard to get." Today it's a critical ingredient in the powerful magnets that keep electric motors running at high temperatures.
- Group · Period
- — · 6
- At room temp
- solid
- Melts at
- 1685 K
- Density
- 8.55 g/cm³
- Discovered
- 1886
Uses
Dysprosium’s most important modern role is as an additive to neodymium-iron-boron magnets — the strong permanent magnets found in electric vehicle motors, wind turbine generators, and hard disk drives. On its own, neodymium magnet material starts to lose its magnetism as it heats up, but blending in a small percentage of dysprosium makes it far more resistant to that high-temperature demagnetization, which matters a great deal inside a motor running hot under load. Dysprosium also absorbs neutrons effectively, so it’s used in some nuclear reactor control rod materials, and it contributes to Terfenol-D, the shape-changing alloy it shares with terbium.
Because of how central it is to high-performance magnets, dysprosium is closely watched as a “critical” rare earth — demand from electric vehicles and renewable energy has made reliable access to it a genuine strategic concern for manufacturers.
History
Dysprosium was isolated in 1886 by French chemist Paul-Émile Lecoq de Boisbaudran, who extracted it from holmium oxide after a long and painstaking series of chemical separations. Boisbaudran chose a name that reflected the ordeal: dysprosium comes from the Greek word for “hard to get at.” As with several other lanthanides discovered in this period, it took additional years of work by other chemists to confirm dysprosium as a genuinely distinct element and produce it in a reasonably pure form.
Fun facts
- Dysprosium's name comes from the Greek word for 'hard to get,' a nod to how difficult it was to separate from the other rare earths it was mixed with.
- Adding even a small amount of dysprosium to neodymium magnets lets them keep working at the high temperatures found inside electric vehicle motors and wind turbine generators.
- Dysprosium is strongly attracted to magnetic fields and is studied at extremely low temperatures for its unusual magnetic behavior.
Frequently asked questions
What is dysprosium actually used for?
Its main modern use is as an additive in neodymium-iron-boron magnets, the strong permanent magnets used in electric motors, generators, and wind turbines. A small amount of dysprosium mixed in makes these magnets far more resistant to losing their magnetism at the high operating temperatures those motors reach. It's also used in some nuclear reactor control rods because it absorbs neutrons well.
Why is dysprosium called a 'hard to get' element?
When it was isolated in 1886, dysprosium was tangled up with holmium and other closely related lanthanides in the same mineral, and separating it required dozens of repeated chemical procedures. French chemist Paul-Émile Lecoq de Boisbaudran named it dysprosium from the Greek "dysprositos," meaning hard to get at, to capture just how stubborn that separation was.
Is dysprosium considered a critical mineral?
Yes — because it's essential for high-performance magnets used in electric vehicles and wind turbines, and because its supply is concentrated in relatively few places, dysprosium is often listed among the rare-earth elements governments and manufacturers consider critical to secure reliable supplies of.
Compounds
2 notable compounds containing Dy
- DyCl3halide
Dysprosium(III) chloride
A pale yellow-green, hygroscopic dysprosium salt normally handled as its hexahydrate, serving as the common entry point into dysprosium chemistry.
Used for: Laboratory precursor for dysprosium metal and other dysprosium compounds
- Dy2O3oxide
Dysprosium(III) oxide
A white, highly magnetic rare-earth oxide and the standard commercial form of dysprosium, valued for its strong response to magnetic fields even among the lanthanides.
Used for: Precursor for dysprosium additives in high-strength neodymium magnets
Isotopes
38 known isotopes
Swipe to see all columns →
| Isotope | Natural abundance | Half-life | Decay mode | Mass excess | Binding energy / nucleon | Decay width |
|---|---|---|---|---|---|---|
| Dy-156 stable | 0.056% | Stable | — | -70,529.39 keV | 8,192.44 keV | — |
| Dy-158 stable | 0.095% | Stable | — | -70,407.15 keV | 8,190.13 keV | — |
| Dy-160 stable | 2.329% | Stable | — | -69,672.43 keV | 8,184.05 keV | — |
| Dy-161 stable | 18.889% | Stable | — | -68,055.49 keV | 8,173.31 keV | — |
| Dy-162 stable | 25.475% | Stable | — | -68,181.17 keV | 8,173.46 keV | — |
| Dy-163 stable | 24.896% | Stable | — | -66,380.86 keV | 8,161.78 keV | — |
| Dy-164 stable | 28.26% | Stable | — | -65,967.65 keV | 8,158.71 keV | — |
Show all 38 isotopes
| Dy-139 | — | 0.6 s | Electron capture / beta-plus decay (100%), ECP (11%) | -37,700 keV | 7,971 keV | 7.60 × 10-16 eV |
| Dy-140 | — | — | Electron capture / beta-plus decay | -42,830 keV | 8,008 keV | — |
| Dy-141 | — | 0.9 s | Electron capture / beta-plus decay (100%), Beta-plus, proton emission | -45,382 keV | 8,027 keV | 5.07 × 10-16 eV |
| Dy-142 | — | 2.3 s | Electron capture / beta-plus decay (100%), ECP (0.06%) | -50,120 keV | 8,061 keV | 1.98 × 10-16 eV |
| Dy-143 | — | 5.6 s | Electron capture / beta-plus decay (100%), ECP | -52,168.95 keV | 8,075.05 keV | 8.15 × 10-17 eV |
| Dy-144 | — | 9.1 s | Electron capture / beta-plus decay (100%), ECP | -56,570.09 keV | 8,105.59 keV | 5.01 × 10-17 eV |
| Dy-145 | — | 6 s | Electron capture / beta-plus decay (100%), ECP (50%) | -58,242.61 keV | 8,116.89 keV | 7.60 × 10-17 eV |
| Dy-146 | — | 33.2 s | Electron capture / beta-plus decay (100%) | -62,554.93 keV | 8,146.11 keV | 1.37 × 10-17 eV |
| Dy-147 | — | 67 s | Electron capture / beta-plus decay (100%), Beta-plus, proton emission (0.05%) | -64,196.05 keV | 8,156.77 keV | 6.81 × 10-18 eV |
| Dy-148 | — | 3.3 m | Electron capture / beta-plus decay (100%) | -67,859.4 keV | 8,180.94 keV | 2.30 × 10-18 eV |
| Dy-149 | — | 4.2 m | Electron capture / beta-plus decay (100%) | -67,693.99 keV | 8,179.1 keV | 1.81 × 10-18 eV |
| Dy-150 | — | 7.17 m | Electron capture / beta-plus decay (64%), Alpha decay (36%) | -69,309.62 keV | 8,189.15 keV | 1.06 × 10-18 eV |
| Dy-151 | — | 17.9 m | Electron capture / beta-plus decay (94.4%), Alpha decay (5.6%) | -68,752.39 keV | 8,184.68 keV | 4.25 × 10-19 eV |
| Dy-152 | — | 2.38 h | Electron capture / beta-plus decay (99.9%), Alpha decay (0.1%) | -70,117.96 keV | 8,192.92 keV | 5.32 × 10-20 eV |
| Dy-153 | — | 6.4 h | Electron capture / beta-plus decay (99.9906%), Alpha decay (0.0094%) | -69,143.2 keV | 8,185.75 keV | 1.98 × 10-20 eV |
| Dy-154 | — | 3.0E+6 Y | Alpha decay (100%) | -70,394.02 keV | 8,193.13 keV | 4.82 × 10-30 eV |
| Dy-155 | — | 9.9 h | Electron capture / beta-plus decay (100%) | -69,155.94 keV | 8,184.36 keV | 1.28 × 10-20 eV |
| Dy-157 | — | 8.14 h | Electron capture / beta-plus decay (100%) | -69,424.67 keV | 8,184.63 keV | 1.56 × 10-20 eV |
| Dy-159 | — | 144.4 d | Electron capture (100%) | -69,167.22 keV | 8,181.58 keV | 3.66 × 10-23 eV |
| Dy-165 | — | 2.332 h | Beta-minus decay (100%) | -63,612.29 keV | 8,143.91 keV | 5.43 × 10-20 eV |
| Dy-166 | — | 81.6 h | Beta-minus decay (100%) | -62,584.47 keV | 8,137.28 keV | 1.55 × 10-21 eV |
| Dy-167 | — | 6.20 m | Beta-minus decay (100%) | -59,911.45 keV | 8,120.88 keV | 1.23 × 10-18 eV |
| Dy-168 | — | 8.7 m | Beta-minus decay (100%) | -58,558.4 keV | 8,112.53 keV | 8.74 × 10-19 eV |
| Dy-169 | — | 39 s | Beta-minus decay (100%) | -55,596.01 keV | 8,094.76 keV | 1.17 × 10-17 eV |
| Dy-170 | — | 55 s | Beta-minus decay (100%) | -53,710 keV | 8,084 keV | 8.30 × 10-18 eV |
| Dy-171 | — | 4.1 s | Beta-minus decay (100%) | -50,010 keV | 8,062 keV | 1.11 × 10-16 eV |
| Dy-172 | — | 160 ns | Beta-minus decay | -47,760 keV | 8,049 keV | 2.85 × 10-9 eV |
| Dy-173 | — | 1.43 s | Beta-minus decay (100%) | -43,740 keV | 8,026 keV | 3.19 × 10-16 eV |
| Dy-174 | — | 160 ns | Beta-minus decay | -41,130 keV | 8,011 keV | 2.85 × 10-9 eV |
| Dy-175 | — | — | Beta-minus decay (100%), Beta-minus, neutron emission | -36,730 keV | 7,986 keV | — |
| Dy-176 | — | — | Beta-minus decay (100%), Beta-minus, neutron emission | -33,610 keV | 7,969 keV | — |