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Half-Life Calculator

Solve for Nₜ, N₀, time, or half-life · Decay chart · Step-by-step solution

Quick-Load Isotopes

☢️ Enter any three values - remaining quantity, initial quantity, time, and half-life - to solve for the fourth. Or use a Quick-Load isotope.

Half-Life · Mean Lifetime · Decay Constant Converter

Enter any one value to convert to the other two. The three constants describe the same decay process from different perspectives.

The Half-Life Formula

Half-life describes how a quantity undergoing exponential decay decreases over time. After each half-life period, the remaining quantity is halved. The three equivalent forms of the decay equation connect the four key variables:

Nₜ = N₀ × (1/2)^(t / t½) Primary form using half-life directly Nₜ = N₀ × e^(-λt) Exponential form using decay constant λ Nₜ = N₀ × e^(-t/τ) Exponential form using mean lifetime τ

Rearranging for each unknown:

Solve for t: t = t½ × log(Nₜ/N₀) / log(0.5) Solve for t½: t½ = t × log(0.5) / log(Nₜ/N₀) Solve for N₀: N₀ = Nₜ / (0.5)^(t/t½) Solve for Nₜ: Nₜ = N₀ × (0.5)^(t/t½)

All four forms are algebraically equivalent. The relationships between the three decay constants are:

t½ = ln(2) / λ ≈ 0.693147 / λ τ = 1 / λ = t½ / ln(2) ≈ 1.4427 × t½ λ = ln(2) / t½ = 1 / τ

Percent Remaining After N Half-Lives

The fraction remaining after N half-lives is (1/2)ᴺ. The table below shows how rapidly the quantity decreases:

Half-LivesFractionPercent RemainingPercent Decayed
01/1100%0%
11/250.000%50.000%
21/425.000%75.000%
31/812.500%87.500%
41/166.250%93.750%
51/323.125%96.875%
71/1280.781%99.219%
101/10240.0977%99.902%
201/1,048,5760.0001%~100%
ℹ️
After 10 half-lives, less than 0.1% of the original quantity remains. This rule is commonly applied in nuclear medicine to determine when a patient is safe to leave isolation after radioactive treatment, and in radiological safety to determine when a spill site is safe to re-enter.

Common Isotopes and Their Half-Lives

IsotopeHalf-LifeDecay TypePrimary Use / Context
Carbon-14 (¹⁴C)5,730 yearsBeta (β⁻)Archaeological and geological dating up to ~50,000 years
Tritium (³H)12.32 yearsBeta (β⁻)Luminescent watch dials, nuclear weapons triggers
Iodine-131 (¹³¹I)8.02 daysBeta + gammaThyroid cancer treatment, thyroid function imaging
Fluorine-18 (¹⁸F)109.8 minutesPositron (β⁺)PET scan tracer (FDG glucose analog)
Cesium-137 (¹³⁷Cs)30.17 yearsBeta + gammaIndustrial gauging, Chernobyl/Fukushima contamination marker
Strontium-90 (⁹⁰Sr)28.8 yearsBeta (β⁻)Nuclear fallout, bone-seeking like calcium
Radium-226 (²²⁶Ra)1,600 yearsAlphaHistorical use in luminous paints, sealed source radiotherapy
Radon-222 (²²²Rn)3.82 daysAlphaBuilding air quality concern, lung cancer risk from accumulation
Plutonium-239 (²³⁹Pu)24,100 yearsAlphaNuclear weapons, MOX fuel, long-term waste disposal concern
Uranium-238 (²³⁸U)4.47 billion yearsAlphaUranium-lead geological dating, nuclear fuel
Potassium-40 (⁴⁰K)1.25 billion yearsBeta + electron capturePotassium-argon geological dating, natural radiation source in body
Uranium-235 (²³⁵U)703.8 million yearsAlphaFissile material in nuclear reactors and weapons

Carbon-14 Dating

Radiocarbon dating uses the known half-life of carbon-14 (5,730 years) to determine the age of organic materials. The method relies on the fact that cosmic rays continuously produce carbon-14 in the upper atmosphere by bombarding nitrogen-14 atoms. This carbon-14 is incorporated into carbon dioxide, absorbed by plants through photosynthesis, and then passes up the food chain to animals.

The ratio of carbon-14 to carbon-12 in a living organism remains approximately constant because the organism continuously exchanges carbon with the environment. Once the organism dies, it stops absorbing new carbon, and the carbon-14 that was present begins to decay at the known rate of t½ = 5,730 years.

Carbon-14 dating example: A sample contains 25% of the carbon-14 expected in a living organism. Nₜ/N₀ = 0.25 → t = 5730 × log(0.25)/log(0.5) t = 5730 × (-1.386)/(-0.693) = 5730 × 2 = 11,460 years

The practical upper limit for carbon-14 dating is about 50,000 years, at which point the remaining carbon-14 concentration is too small to measure accurately. For older materials (millions to billions of years), geologists use isotopes with much longer half-lives, such as potassium-40 to argon-40 (1.25 billion years) and uranium-238 to lead-206 (4.47 billion years).

Frequently Asked Questions

Does half-life change with temperature or pressure?
For radioactive nuclear decay, the half-life is independent of temperature, pressure, chemical state, and physical form. The decay originates in the nucleus and is unaffected by the electron shell configuration or external conditions. This is a key property that makes radioactive dating reliable - the rate has not changed over billions of years. This is in contrast to chemical reactions, which are strongly affected by temperature (Arrhenius equation), and biological processes, where half-life of a drug in the body depends strongly on metabolism and health.
What is the difference between half-life and mean lifetime?
Half-life (t½) is the time for exactly 50% of atoms to decay. Mean lifetime (τ) is the average time a single atom survives before decaying, which equals the half-life divided by ln(2): τ = t½/0.693 ≈ 1.443 × t½. The mean lifetime is always about 44% longer than the half-life. After one mean lifetime, about 36.8% (= 1/e) of the original atoms remain - more than the 50% at one half-life, because the mean is pulled by long-surviving atoms.
How is half-life used in medicine?
In nuclear medicine, short-lived isotopes are preferred for imaging so patients are not exposed to radiation longer than necessary. Fluorine-18 (half-life 110 minutes) is used in PET scans - it decays away within hours after the scan. Iodine-131 (half-life 8 days) is used to treat thyroid cancer, delivering a localised radiation dose. Pharmacological half-life (how quickly the body eliminates a drug) is a separate concept from nuclear half-life and is used to determine dosing intervals.
What does it mean for a substance to never fully decay?
In theory, exponential decay never reaches exactly zero - there is always a (1/2)^N fraction remaining, no matter how large N is. In practice, radioactive materials do reach zero once the last atom decays, because atoms are discrete. The practical threshold is usually defined as after 10 half-lives (0.1% remaining) for most safety and engineering purposes. For isotopes with very long half-lives like uranium-238 (4.47 billion years), a kilogram of uranium takes far longer than the current age of the universe to decay by half.