92U238.0289
Actinide

Uranium

Uranium is a dense, silvery-white metal and the heaviest element found on Earth in more than trace amounts. It's mildly radioactive in its natural form, decaying extremely slowly, but it owes its fame to a rarer isotope, uranium-235, which can sustain a nuclear chain reaction — the basis of both nuclear power and the first atomic weapons.

Group · Period
— · 7
At room temp
solid
Melts at
1408 K
Density
18.95 g/cm³
Discovered
1789

Uses

Uranium’s defining modern use is as nuclear fuel: uranium-235, enriched to usable concentrations, sustains the chain reactions that power nuclear plants generating electricity for hundreds of millions of people, and in far more concentrated form formed the core of the first atomic weapons. Depleted uranium — what’s left after enrichment, mostly uranium-238 — is dense enough to be used in armor-piercing ammunition and as counterweights in aircraft, applications that rely on its weight rather than its radioactivity.

Long before any of that was possible, uranium had a much quieter role: its compounds were prized for coloring glass and ceramic glazes a distinctive yellow-green, an industry that predates any understanding of radioactivity and largely ended once the risks became clear.

History

Uranium was identified in 1789 by German chemist Martin Heinrich Klaproth, who found a new element in the mineral pitchblende and named it after the planet Uranus. The pure metal wasn’t isolated until 1841, by French chemist Eugène-Melchior Péligot. Uranium’s most consequential chapter began in 1896, when Henri Becquerel noticed that uranium salts fogged photographic plates without any light source — the discovery of radioactivity. Decades later, the 1938 discovery that uranium nuclei could be split, and the realization that this fission could release enormous energy, set in motion the research that led to both nuclear power and nuclear weapons.

Fun facts

  • Uranium was the very substance in which radioactivity was first detected, by Henri Becquerel in 1896, years before the phenomenon even had a name.
  • Natural uranium is over 99% uranium-238, with less than 1% of the fissile uranium-235 that reactors and weapons need — which is why it must be enriched.
  • Uranium glass, popular in the early 20th century, contains trace uranium that makes it glow bright green under ultraviolet light.

Frequently asked questions

Is all uranium radioactive?

Yes, every isotope of uranium is radioactive, though most decay extremely slowly. Natural uranium's dominant isotope, uranium-238, has a half-life of about 4.5 billion years — roughly the age of the Earth — so a lump of it is only mildly radioactive to handle.

Why does nuclear fuel need to be 'enriched'?

Reactors and weapons rely on uranium-235, the isotope that splits easily when struck by a neutron, but natural uranium contains less than 1% of it. Enrichment concentrates the uranium-235 fraction — typically to a few percent for power reactors, far higher for weapons — through processes like gas centrifuges.

Why is uranium named after a planet?

German chemist Martin Klaproth named it after Uranus, which had been discovered just eight years earlier, in 1781. It followed a chemistry tradition of the time of naming new discoveries after new astronomical ones.

Compounds

4 notable compounds containing U

  • U3O8oxide

    Triuranium octoxide

    A dark green-black mixed-valence oxide containing uranium in both the +5 and +6 states, and the thermodynamically most stable uranium oxide in air across a wide temperature range. It's the form uranium ore concentrate settles into after milling.

    Used for: Standard storage and shipping form of milled uranium ore ("yellowcake")

  • UO2oxide

    Uranium dioxide

    A black, ceramic solid with a fluorite crystal structure in which each uranium atom sits surrounded by eight oxygen atoms. It's the most thermally and chemically stable uranium oxide, holding its solid form up to temperatures near 2865°C.

    Used for: Fuel pellets in nuclear power reactors

  • UF6halide

    Uranium hexafluoride

    A volatile, colorless solid that sublimes readily and turns into a dense, corrosive gas just above room temperature. Its six fluorine atoms make it the only uranium compound volatile enough to be processed by gas centrifuge or diffusion.

    Used for: Feedstock gas for uranium enrichment

  • UF4halide

    Uranium tetrafluoride

    A green, non-volatile crystalline solid nicknamed "green salt," made by reacting uranium oxide with hydrofluoric acid. It's the intermediate step between uranium oxide and the volatile hexafluoride used for enrichment.

    Used for: Intermediate in uranium enrichment and uranium metal production

Isotopes

40 known isotopes

Swipe to see all columns →

IsotopeNatural abundanceHalf-lifeDecay modeMass excessBinding energy / nucleonDecay width
U-234 0.0054% 2.455E+5 Y Alpha decay (100%), Spontaneous fission (1.64e-9%), Mg (1.4e-11%) 38,144.96 keV 7,600.72 keV 5.89 × 10-29 eV
U-235 0.7204% 7.04E+8 Y Alpha decay (100%), Spontaneous fission (7e-9%), {+25}Ne (8e-10%) 40,918.78 keV 7,590.92 keV 2.05 × 10-32 eV
U-238 99.2742% 4.468E9 Y Alpha decay (100%), Spontaneous fission (0.0000545%) 47,307.73 keV 7,570.13 keV 3.24 × 10-33 eV
Show all 40 isotopes
U-214 0.52 ms Alpha decay (100%) 8.77 × 10-13 eV
U-215 0.7 ms Alpha decay (0%), Electron capture / beta-plus decay 24,889.31 keV 7,620.78 keV 6.52 × 10-13 eV
U-216 4.5 ms Alpha decay (100%) 23,066.43 keV 7,631.31 keV 1.01 × 10-13 eV
U-217 16 ms Alpha decay (100%), Electron capture / beta-plus decay 22,971 keV 7,634 keV 2.85 × 10-14 eV
U-218 0.65 ms Alpha decay (100%) 21,894.66 keV 7,640.72 keV 7.02 × 10-13 eV
U-219 60 us Alpha decay (100%) 23,295.95 keV 7,636.29 keV 7.60 × 10-12 eV
U-221 0.66 us Alpha decay (100%) 24,520 keV 7,634.68 keV 6.91 × 10-10 eV
U-222 4.7 us Alpha decay (100%) 24,272.83 keV 7,637.77 keV 9.71 × 10-11 eV
U-223 18 us Alpha decay (100%), Electron capture / beta-plus decay (0.2%) 26,045.28 keV 7,631.76 keV 2.53 × 10-11 eV
U-224 396 us Alpha decay (100%) 25,742.69 keV 7,635.07 keV 1.15 × 10-12 eV
U-225 69 ms Alpha decay (100%) 27,372 keV 7,629.77 keV 6.61 × 10-15 eV
U-226 268 ms Alpha decay (100%) 27,328.8 keV 7,631.92 keV 1.70 × 10-15 eV
U-227 1.1 m Alpha decay (100%) 29,045.03 keV 7,626.29 keV 6.91 × 10-18 eV
U-228 9.1 m Alpha decay (95%), Electron capture (5%) 29,220 keV 7,627.48 keV 8.36 × 10-19 eV
U-229 58 m Electron capture (80%), Alpha decay (20%) 31,210.62 keV 7,620.72 keV 1.31 × 10-19 eV
U-230 20.23 d Alpha decay (100%), {+22}Ne (4.8e-12%) 31,615.02 keV 7,620.92 keV 2.61 × 10-22 eV
U-231 4.2 d Electron capture (100%), Alpha decay (0.004%) 33,805.95 keV 7,613.39 keV 1.26 × 10-21 eV
U-232 68.9 Y Alpha decay (100%), {+24}Ne (8.9e-10%), Spontaneous fission (2.7e-12%) 34,609.45 keV 7,611.9 keV 2.10 × 10-25 eV
U-233 1.5919E5 Y Alpha decay (100%), 24NE (7.2e-11%), Spontaneous fission (6e-11%) 36,919.11 keV 7,603.96 keV 9.08 × 10-29 eV
U-236 2.342E7 Y Alpha decay (100%), Spontaneous fission (9.4e-8%) 42,444.58 keV 7,586.49 keV 6.17 × 10-31 eV
U-237 6.752 d Beta-minus decay (100%) 45,390.13 keV 7,576.1 keV 7.82 × 10-22 eV
U-239 23.45 m Beta-minus decay (100%) 50,572.67 keV 7,558.56 keV 3.24 × 10-19 eV
U-240 14.1 h Beta-minus decay (100%) 52,715.5 keV 7,551.77 keV 8.99 × 10-21 eV
U-241 Beta-minus decay 56,197 keV 7,539 keV
U-242 16.8 m Beta-minus decay (100%) 58,620 keV 7,532 keV 4.53 × 10-19 eV
U-243 Beta-minus decay 62,480 keV 7,518 keV
U-244 Beta-minus decay
U-245 Beta-minus decay
U-246 Beta-minus decay
U-247 Beta-minus decay
U-248 Beta-minus decay
U-249 Beta-minus decay
U-250 Beta-minus decay
U-251 Beta-minus decay
U-253 Beta-minus decay, Beta-minus, neutron emission
U-254 Beta-minus decay (100%), Beta-minus, neutron emission
U-255 Beta-minus decay, Beta-minus, neutron emission