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Half-life · U-238

Uranium-238 half-life: 4.47 billion years

Watch 400 atoms of uranium-238 decay one by one, scrub through time and read the fraction left against the smooth decay curve.

Time-lapse · 1 half-life = 2 s ↔ Drag to scrub time · tap to pause
Time0.00half-lives

Every atom is still there

Elapsed0 y
Left (sample)400 of 400
Expected400 (100%)
Decayed0
Activity per g165 GBq
Dated age0 y

Activity is for 1 g of the pure isotope, from A = λN. Age is worked out from the fraction left in this sample.

The half-life of uranium-238 is 4.47 billion years. Every 4.47 billion years, half of the atoms that are left decay, so after 2 half-lives (8.94 bn y) a quarter is left, and after 10 (44.7 bn y) about 0.10%.

Written as a rate, the decay constant is λ = ln 2 ÷ T½ = 4.914 × 10⁻¹⁸ per second, and the average atom survives for the mean life τ = 6,448,846,833 years. One gram of the pure isotope contains 2.53 × 10²¹ atoms and has an activity of 12.4 kBq.

Half-life 4.47 billion years Mean life 6,448,846,833 years Left after 3 13% Left after 10 0.10% Activity per g 12.4 kBq Atoms per g 2.53 × 10²¹

Uranium-238 decay table

Each row is a number of half-lives, the time that takes for U-238, and what is left. The fraction is 2 raised to minus the number of half-lives, for any sample size.

Half-livesTimeFraction leftOdds an atom survives
14.47 bn y50%1 in 2
28.94 bn y25%1 in 4
313.4 bn y13%1 in 8
417.9 bn y6.3%1 in 16
522.3 bn y3.1%1 in 32
626.8 bn y1.6%1 in 64
835.8 bn y0.39%1 in 256
1044.7 bn y0.10%1 in 1,024

N = N₀ × 2^(−t ÷ 4.47 billion years). With only 400 atoms in the simulation the count scatters about the curve, because each atom decays at a random time.

How long until U-238 drops to a given level

Running the law backwards gives the time for the sample to fall to a chosen fraction, t = −T½ log₂(fraction). This is also how a measured fraction becomes an age.

Fraction leftTime neededHalf-lives
90%0.679 bn y0.152 half-lives
50%4.47 bn y1.00 half-lives
25%8.94 bn y2.00 half-lives
10%14.8 bn y3.32 half-lives
1.0%29.7 bn y6.64 half-lives
0.10%44.5 bn y9.97 half-lives

About uranium-238

Uranium-238 has a half-life of 4.47 billion years, within a few percent of the age of the Earth, about 4.54 billion years. Roughly half the uranium-238 that formed with the planet is still here, which is why it is a useful clock for the oldest rocks and zircon crystals, the oldest of which are about 4.4 billion years old.

It does not decay in one step. It passes through a chain of 14 steps, including radon-222 and polonium-214, before it ends as stable lead-206. Natural uranium is 99.3% uranium-238 and 0.7% uranium-235, the isotope used in reactors and weapons; see how Oppenheimer made the first nuke.

A worked example

A zircon crystal has kept 90% of its original uranium-238. How old is it?

t = −4.47 bn y × log₂(0.90) = 4.47 × 0.152 = 0.679 bn y. In practice geologists use the ratio of uranium to lead, which also tells how much has decayed.

Compare with other isotopes

The half-lives in the simulation span twenty orders of magnitude, from microseconds to billions of years. Each has its own page.

IsotopeHalf-lifeActivity per gram
Carbon-145,730 years165 GBq
Uranium-2384.47 billion years12.4 kBq
Iodine-1318.02 days4.6 PBq
Polonium-214164 microseconds11.9 YBq
Technetium-99m6.0 hours195 PBq

This page is one case from the full guide, Half-life and radioactive decay simulator, which covers every case, the assumptions behind the model and what it leaves out.

Other cases

Frequently asked questions

What is the half-life of uranium-238?

4.47 billion years. After that time half of any sample has decayed, and half remains.

How much U-238 is left after 3 half-lives?

One eighth, 13%, after 13.4 bn y.

Does the half-life depend on how much there is?

No. Each atom has the same chance of decaying in any moment, so the time for half of a sample to decay is the same for a gram or a ton. Heat, pressure and chemistry do not change it for ordinary decay.

When is U-238 gone?

It never reaches exactly zero, but after 10 half-lives (44.7 bn y) only 0.10% remains, which is the usual rule of thumb for “gone”.

Part of the learning path Stars and scale, from the Sun to a neutron star.

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