Nuclear Decay Calculator

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Nuclear Decay Calculator

Find out how much of a radioactive sample remains after a given time. Enter a starting quantity, half-life, and elapsed time to see the full exponential decay breakdown.

⚛️ Half-Life Formula
📉 Exponential Decay
🧮 Decay Constant
🔬 Any Isotope

Calculate Radioactive Decay

Enter your starting quantity, the isotope’s half-life, and the time elapsed. The calculator will show the remaining amount, the decay constant, and how many half-lives have passed.

Decay Solver

Project remaining quantity using the half-life decay formula

💡 Pro Tip: You can enter the half-life and elapsed time in different units (say, half-life in years and elapsed time in days); the calculator converts both to seconds internally before doing the maths.
Half-Life: The time for half of a radioactive sample to decay. It never changes, regardless of how much material you start with.
Decay Constant (λ): Equal to ln(2) divided by the half-life, this describes the probability of decay per unit time for any single atom.
Exponential, Not Linear: Quantity never technically reaches zero; it approaches it asymptotically, halving again and again.
Quantity vs Activity: This tool tracks the amount of material remaining, not its radioactivity (activity), which is usually measured in becquerels or curies.
⚠️ Educational Use Only: This calculator is for learning and general estimation. It is not a substitute for radiological safety assessments, dosimetry, or professional nuclear physics calculations.

Understanding Radioactive Decay

Radioactive decay follows a simple, predictable pattern at the level of a large sample, even though it’s random for any single atom. Here’s the logic behind the calculation.

1

Start With the Half-Life

Every radioactive isotope has a fixed half-life, the time it takes for half of any sample of it to decay. This value is unique to each isotope.

2

Convert to a Decay Constant

The decay constant λ = ln(2) / half-life gives the fraction of atoms decaying per unit time, which is what actually drives the exponential formula.

3

Apply the Exponential Formula

The remaining quantity is N = N₀ × (1/2)^(t / half-life). Each time t reaches another full half-life, the quantity halves again.

4

Read Off the Result

The output tells you how much of the original material is left, how much has decayed, and how many half-lives have elapsed in total.

Common Isotope Half-Lives

Approximate half-lives for some widely referenced isotopes, useful as starting points for the calculator above.

Isotope Approximate Half-Life Common Use / Context
Carbon-14≈ 5,730 yearsRadiocarbon dating of organic material
Iodine-131≈ 8.02 daysMedical imaging and thyroid treatment
Cobalt-60≈ 5.27 yearsIndustrial radiography, radiotherapy
Radon-222≈ 3.82 daysNaturally occurring indoor air contaminant
Caesium-137≈ 30.17 yearsEnvironmental contamination studies
Uranium-235≈ 703.8 million yearsNuclear fuel and geological dating
Uranium-238≈ 4.47 billion yearsGeological dating of rock formations
Potassium-40≈ 1.25 billion yearsPotassium-argon geological dating
Plutonium-239≈ 24,100 yearsNuclear fuel and weapons material tracking

Nuclear Decay FAQ

Answers to the most frequently asked questions about radioactive decay and half-life calculations.

Half-life is the time it takes for half of the radioactive atoms in a sample to decay into a different, more stable form. It’s a fixed, characteristic property of each isotope, so a sample of a given isotope always takes the same amount of time to fall to half its original quantity, regardless of how much you start with.

The remaining quantity after time t is N = N0 × (1/2)^(t / half-life), where N0 is the starting quantity. This can also be written using the decay constant as N = N0 × e^(−λt), where the decay constant λ equals ln(2) divided by the half-life.

No. Radioactive decay is a random process at the level of an individual atom, so there is no way to predict exactly when any one atom will decay. Half-life only describes the statistical average behaviour of a very large number of atoms, which is why decay calculations work reliably for real samples containing trillions of atoms.

For almost all practical purposes, no. Radioactive decay rates come from the nucleus of the atom, which is essentially unaffected by the surrounding chemical or physical environment, including temperature, pressure, and the chemical compound the atom is part of. This is different from ordinary chemical reactions, which do speed up or slow down with these conditions.

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