How to Calculate Half-Life — Formula and Worked Examples (2026)
Modern Physics · 9 min read

Half-life — how radioactive decay is calculated, step by step

Half-life is the time it takes for exactly half of a radioactive sample to decay. This guide breaks down the half-life formula, walks through worked examples, and explains why radioactive decay is random for individual atoms but perfectly predictable for large samples.

N = N₀(½)^(t/T)the formula
5,730 yrsCarbon-14 half-life
Randomat the atomic level
50%

What is half-life?

Half-life is the time it takes for half of the radioactive atoms in a sample to decay into a different, more stable form. Every radioactive isotope has its own fixed, unchanging half-life — from fractions of a second to billions of years — regardless of the sample’s size, temperature, or chemical state.

Radioactive decay happens randomly for any individual atom — there’s no way to predict exactly when one specific nucleus will decay. But with enormous numbers of atoms in a real sample (billions upon billions), that randomness averages out into a completely predictable pattern described by half-life.

This predictability is what makes half-life so useful — from dating ancient artifacts with carbon-14 to calculating safe storage times for nuclear waste.

The half-life formula and related quantities

These formulas let you calculate remaining quantity, elapsed time, or decay constant for any radioactive sample.

Half-life and radioactive decay formulas
ConceptFormulaWhat it meansReal-world example
Remaining quantityN = N₀(½)^(t/T)Amount remaining after time t, given starting amount N₀ and half-life THow much Carbon-14 remains in a 10,000-year-old fossil
Decay constantλ = ln(2) / TConverts half-life into the exponential decay rate constantUsed in the continuous decay formula N = N₀e^(−λt)
ActivityA = λNRate of decay events per second, measured in becquerelsRadiation output of a medical isotope sample
Number of half-lives elapsedn = t / THow many half-life periods have passedDetermining decay stage without a calculator, using simple halving

A worked half-life example, step by step

Carbon-14 dating is the classic real-world application — here’s exactly how it works.

01 Start with a known half-life

Carbon-14 has a half-life of 5,730 years. If a fossil originally had 100% of its expected Carbon-14, and now has 25% remaining, that tells you exactly how many half-lives have passed.

100%

02 Halve it repeatedly

25% is one-quarter of the original — that’s two halvings (100% → 50% → 25%), so two half-lives have passed: 2 × 5,730 = 11,460 years.

03 Confirm with the formula

Using N = N₀(½)^(t/T): 0.25 = (½)^(t/5730) solves to t = 11,460 years — matching the step-by-step halving exactly, which is a useful way to sanity-check your algebra.

t = 11,460 yrs

Where half-life matters in real life

  • Carbon-14 dating: Archaeologists date organic remains up to about 50,000 years old by measuring how much Carbon-14 (half-life 5,730 years) remains compared to living organisms.
  • Nuclear medicine: Medical isotopes like Technetium-99m (half-life ~6 hours) are chosen specifically so they decay away quickly after a scan, minimizing patient radiation exposure.
  • Nuclear power and waste storage: Engineers calculate storage requirements for spent fuel using the half-lives of various radioactive byproducts, some of which persist for thousands of years.
  • Smoke detectors: Many household smoke detectors contain a tiny amount of Americium-241 (half-life ~432 years), which ionizes air to detect smoke particles.
  • Geological dating: Uranium-lead dating, using a half-life of about 4.5 billion years, lets geologists determine the age of rocks and even the Earth itself.
  • Food irradiation and sterilization: Cobalt-60 sources, with a half-life of about 5.27 years, are used in controlled doses to sterilize medical equipment and some foods.

Common half-life mistakes

  • Assuming half-life means ‘half the atoms decay, then decay stops’: Decay continues indefinitely — after one half-life, half remains; after two half-lives, a quarter remains; it never reaches exactly zero in a finite time.
  • Thinking you can predict when a specific atom will decay: Radioactive decay is fundamentally random for individual atoms — half-life only describes probability across huge numbers of atoms, not any single one.
  • Confusing half-life with total decay time: A sample isn’t ‘gone’ after one half-life — it’s halved. Common estimates suggest a sample is negligible after about 5-10 half-lives, not just one.
  • Forgetting that half-life is constant regardless of conditions: Unlike chemical reaction rates, radioactive half-life doesn’t change with temperature, pressure, or chemical bonding — it’s a nuclear property, not a chemical one.
  • Mixing up decay constant (λ) and half-life (T) in formulas: They’re related by λ = ln(2)/T but are not the same number — plugging one into a formula meant for the other gives a badly wrong answer.

Key takeaways

  • Half-life is the time for exactly half of a radioactive sample to decay.
  • The formula is N = N₀(½)^(t/T), where T is the half-life and t is elapsed time.
  • Decay is random for individual atoms but statistically predictable for large samples.
  • Half-life is a fixed nuclear property, unaffected by temperature, pressure, or chemistry.
  • Real-world uses include carbon dating, nuclear medicine, and geological dating.
  • A sample never reaches exactly zero — it approaches zero asymptotically over many half-lives.

Frequently asked questions about half-life

What is half-life?

Half-life is the time it takes for half of the radioactive atoms in a sample to decay into a different form. Every isotope has its own fixed half-life.

What is the formula for half-life calculations?

N = N₀(½)^(t/T), where N is the remaining quantity, N₀ is the starting quantity, t is elapsed time, and T is the half-life.

Can you predict when a single atom will decay?

No. Decay is fundamentally random for any individual atom. Half-life only describes the predictable statistical behavior of a very large number of atoms.

Does temperature or pressure affect half-life?

No. Radioactive half-life is a nuclear property that stays constant regardless of temperature, pressure, or the chemical compound the atom is part of.

How does carbon-14 dating use half-life?

By comparing the ratio of remaining Carbon-14 (half-life 5,730 years) to stable carbon in a sample against the ratio in living organisms, scientists calculate how many half-lives — and therefore how many years — have passed.

PF

Written and reviewed by the Physics Fundamentals Editorial Team

Our content is written by physics educators and reviewed against standard references, including NIST’s physical constants database and university-level open courseware, so every formula and example on this page reflects widely accepted physics standards.

Ready to run your own half-life calculations?

Try the interactive half-life calculator, or continue to nuclear decay equations to see the atomic-level changes half-life is describing.