Strontium
Strontium is a soft, silvery alkaline earth metal that reacts readily with air and water, much like calcium and barium nearby on the periodic table. It's best known outside chemistry for giving fireworks their vivid red color, and its name traces back to a small Scottish village.
- Group · Period
- 2 · 5
- At room temp
- solid
- Melts at
- 1050 K
- Density
- 2.64 g/cm³
- Discovered
- 1790
Uses
Strontium’s most visible role is in fireworks and signal flares, where its compounds produce the deep, brilliant red color familiar from countless displays. Strontium carbonate was also historically added to the glass in cathode-ray tube televisions and monitors to help block X-rays generated inside the tube from reaching the viewer. Strontium ferrite, a compound of strontium, iron and oxygen, is used to make durable, low-cost ceramic magnets found in everything from refrigerator magnets to small motors and speakers.
Because strontium behaves chemically much like calcium, some strontium compounds have also been studied and used in treatments aimed at supporting bone health, under close medical supervision given the element’s tendency to accumulate in bone tissue.
History
Strontium takes its name from Strontian, a small village in the Scottish Highlands, where an unusual mineral was found in a lead mine in the late 18th century. In 1790, physician and chemist Adair Crawford examined the mineral and concluded it contained a new “earth,” distinct from other known minerals of the time, though he wasn’t able to isolate the metal itself. That step came in 1808, when Humphry Davy used electrolysis — passing an electric current through a molten compound — to isolate pure strontium metal for the first time, adding it to the list of reactive metals he successfully isolated during that period.
Fun facts
- Strontium salts are what give fireworks and flares their brilliant red color.
- The element is named after Strontian, a small village in Scotland where the mineral it was first identified in was mined.
- The radioactive isotope strontium-90, a byproduct of nuclear fission, chemically mimics calcium closely enough that the body can mistake it for calcium and deposit it in bone.
Frequently asked questions
Why do strontium compounds turn fireworks red?
When strontium atoms are heated in a flame or explosion, their electrons absorb energy and then release it as light of a very specific wavelength, which for strontium falls in the red part of the visible spectrum. That's the same basic principle behind every colored firework and flare.
Was strontium discovered or isolated first, and by whom?
Scottish physician Adair Crawford recognized strontium ore as containing a previously unidentified 'earth' in 1790, but it took until 1808 for Humphry Davy to actually isolate the pure metal itself, using electrolysis — the same method he used to isolate several other reactive metals around that time.
Is all strontium radioactive and dangerous?
No — naturally occurring strontium is stable and not radioactive; it's found safely in rocks, minerals and even seawater. The radioactive isotope strontium-90 that raises health concerns is specifically a byproduct of nuclear fission, not something found naturally in significant amounts.
Compounds
5 notable compounds containing Sr
- SrCO3mineral
Strontium carbonate
A white, poorly water-soluble compound found naturally as the mineral strontianite, once the key ingredient in red phosphors and color television glass.
Used for: Ceramic ferrite magnets and pyrotechnic red colorant
- SrCl2salt
Strontium chloride
A white, water-soluble salt of strontium that colors flames a vivid red, a property put to use in fireworks and signal flares.
Used for: Toothpaste ingredient for sensitive teeth; red colorant in fireworks
- Sr(NO3)2salt
Strontium nitrate
A colorless, water-soluble oxidizing salt best known for producing the brilliant red flares seen in fireworks and road signal flares.
Used for: Red colorant and oxidizer in fireworks and signal flares
- SrOoxide
Strontium oxide
A caustic white solid, sometimes called strontia, that reacts vigorously with water to form strontium hydroxide.
Used for: Additive in specialty glass and ceramic glazes
- SrSO4mineral
Strontium sulfate
A sparingly soluble white mineral known as celestine, the principal natural ore from which strontium metal and its compounds are extracted.
Used for: Primary commercial ore of strontium
Isotopes
36 known isotopes
Swipe to see all columns →
| Isotope | Natural abundance | Half-life | Decay mode | Mass excess | Binding energy / nucleon | Decay width |
|---|---|---|---|---|---|---|
| Sr-84 stable | 0.56% | Stable | — | -80,649.58 keV | 8,677.51 keV | — |
| Sr-86 stable | 9.86% | Stable | — | -84,523.1 keV | 8,708.46 keV | — |
| Sr-87 stable | 7% | Stable | — | -84,880.08 keV | 8,705.24 keV | — |
| Sr-88 stable | 82.58% | Stable | — | -87,921.63 keV | 8,732.6 keV | — |
Show all 36 isotopes
| Sr-73 | — | 25 ms | Electron capture / beta-plus decay (100%), ECP | -31,950 keV | 8,102 keV | 1.82 × 10-14 eV |
| Sr-74 | — | 27 ms | Electron capture / beta-plus decay (100%), ECP | -40,827 keV | 8,221 keV | 1.69 × 10-14 eV |
| Sr-75 | — | 88 ms | Electron capture / beta-plus decay (100%), ECP (5.2%) | -46,618.7 keV | 8,296.51 keV | 5.18 × 10-15 eV |
| Sr-76 | — | 7.89 s | Electron capture / beta-plus decay (100%), ECP (0.000034%) | -54,247.65 keV | 8,393.93 keV | 5.78 × 10-17 eV |
| Sr-77 | — | 9.0 s | Electron capture / beta-plus decay (100%), ECP (0.08%) | -57,803.44 keV | 8,435.92 keV | 5.07 × 10-17 eV |
| Sr-78 | — | 160 s | Electron capture / beta-plus decay (100%) | -63,173.95 keV | 8,500.1 keV | 2.85 × 10-18 eV |
| Sr-79 | — | 2.25 m | Electron capture / beta-plus decay (100%) | -65,479.66 keV | 8,523.86 keV | 3.38 × 10-18 eV |
| Sr-80 | — | 106.3 m | Electron capture / beta-plus decay (100%) | -70,311.47 keV | 8,578.6 keV | 7.15 × 10-20 eV |
| Sr-81 | — | 22.3 m | Electron capture / beta-plus decay (100%) | -71,528.13 keV | 8,587.35 keV | 3.41 × 10-19 eV |
| Sr-82 | — | 25.35 d | Electron capture (100%) | -76,010.06 keV | 8,635.72 keV | 2.08 × 10-22 eV |
| Sr-83 | — | 32.41 h | Electron capture / beta-plus decay (100%) | -76,797.62 keV | 8,638.41 keV | 3.91 × 10-21 eV |
| Sr-85 | — | 64.849 d | Electron capture (100%) | -81,103.29 keV | 8,675.72 keV | 8.14 × 10-23 eV |
| Sr-89 | — | 50.563 d | Beta-minus decay (100%) | -86,209.03 keV | 8,705.92 keV | 1.04 × 10-22 eV |
| Sr-90 | — | 28.91 Y | Beta-minus decay (100%) | -85,950.95 keV | 8,696 keV | 5.00 × 10-25 eV |
| Sr-91 | — | 9.65 h | Beta-minus decay (100%) | -83,651.95 keV | 8,663.88 keV | 1.31 × 10-20 eV |
| Sr-92 | — | 2.611 h | Beta-minus decay (100%) | -82,867.37 keV | 8,648.91 keV | 4.85 × 10-20 eV |
| Sr-93 | — | 7.43 m | Beta-minus decay (100%) | -80,085.84 keV | 8,612.79 keV | 1.02 × 10-18 eV |
| Sr-94 | — | 75.3 s | Beta-minus decay (100%) | -78,845.72 keV | 8,593.83 keV | 6.06 × 10-18 eV |
| Sr-95 | — | 23.90 s | Beta-minus decay (100%) | -75,117.28 keV | 8,549.09 keV | 1.91 × 10-17 eV |
| Sr-96 | — | 1.07 s | Beta-minus decay (100%) | -72,918.25 keV | 8,521.2 keV | 4.26 × 10-16 eV |
| Sr-97 | — | 429 ms | Beta-minus decay (100%), Beta-minus, neutron emission (0.05%) | -68,580.67 keV | 8,471.85 keV | 1.06 × 10-15 eV |
| Sr-98 | — | 0.653 s | Beta-minus decay (100%), Beta-minus, neutron emission (0.23%) | -66,422.39 keV | 8,445.74 keV | 6.99 × 10-16 eV |
| Sr-99 | — | 0.269 s | Beta-minus decay (100%), Beta-minus, neutron emission (0.1%) | -62,518.53 keV | 8,402.52 keV | 1.70 × 10-15 eV |
| Sr-100 | — | 200 ms | Beta-minus decay (100%), Beta-minus, neutron emission (1.11%) | -59,817.51 keV | 8,372.2 keV | 2.28 × 10-15 eV |
| Sr-101 | — | 118 ms | Beta-minus decay (100%), Beta-minus, neutron emission (2.37%) | -55,324.91 keV | 8,324.74 keV | 3.87 × 10-15 eV |
| Sr-102 | — | 69 ms | Beta-minus decay (100%), Beta-minus, neutron emission (5.5%) | -52,159.31 keV | 8,291.22 keV | 6.61 × 10-15 eV |
| Sr-103 | — | 53 ms | Beta-minus decay (100%), B-2N, Beta-minus, neutron emission | -47,280 keV | 8,242 keV | 8.61 × 10-15 eV |
| Sr-104 | — | 53 ms | Beta-minus decay (100%), B-2N, Beta-minus, neutron emission | -43,760 keV | 8,206 keV | 8.61 × 10-15 eV |
| Sr-105 | — | 39 ms | Beta-minus decay (100%), Beta-minus, neutron emission, B-2N | -38,190 keV | 8,152 keV | 1.17 × 10-14 eV |
| Sr-106 | — | 20 ms | Beta-minus decay (100%), Beta-minus, neutron emission, B-2N | -34,300 keV | 8,114 keV | 2.28 × 10-14 eV |
| Sr-107 | — | 395 ns | Beta-minus decay, Beta-minus, neutron emission, B-2N | -28,250 keV | 8,057 keV | 1.16 × 10-9 eV |
| Sr-108 | — | — | Beta-minus decay (100%), Beta-minus, neutron emission, B-2N | — | — | — |