5,728.489096
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5,728.489096
time
8,264.46281
time
0.000121
1/time
2.0005
0.249909
75.0091
%
The Half-Life Calculator determines the half-life of a radioactive substance from either its decay constant or experimental measurements. Half-life ($$t_{1/2}$$) is one of the most fundamental properties of any radioactive isotope, representing the time required for exactly half of the atoms in a sample to undergo decay. This value is intrinsic to each nuclide and remains constant regardless of the amount of material, environmental conditions, or chemical form.
From carbon dating to nuclear medicine dosimetry, from reactor engineering to environmental contamination assessment, the half-life governs how quickly radioactive materials transform and how long their effects persist. This calculator supports both direct computation from the decay constant and inverse calculation from measured sample data.
The half-life relates to the decay constant $$\lambda$$ through the fundamental relationship:
$$t_{1/2} = \frac{\ln(2)}{\lambda} = \frac{0.693147}{\lambda}$$
When experimental measurements are available (initial quantity $$N_0$$, final quantity $$N$$, and elapsed time $$t$$), the half-life can be determined by rearranging the decay equation:
$$N = N_0 \cdot e^{-\lambda t}$$
Solving for $$\lambda$$ and then $$t_{1/2}$$:
$$\lambda = \frac{\ln(N_0/N)}{t}$$
$$t_{1/2} = \frac{t \cdot \ln(2)}{\ln(N_0/N)}$$
The mean life (average lifetime) of an atom before decay is:
$$\tau = \frac{1}{\lambda} = \frac{t_{1/2}}{\ln(2)} \approx 1.4427 \times t_{1/2}$$
The mean life is always longer than the half-life by a factor of $$1/\ln(2)$$, reflecting the asymmetric exponential distribution of individual atom lifetimes.
The Half-Life tells you how long it takes for half of any given sample to decay — it is a fixed property of the isotope independent of sample size. The Mean Life is the average time an individual atom survives before decaying, always about 44.3% longer than the half-life. The Decay Constant gives the instantaneous probability of decay per unit time. When using measurement mode, Half-Lives in Given Period shows how many half-lives fit in your observation window, helping validate the measurement accuracy.
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With λ = 1.2097×10⁻⁴ yr⁻¹, the calculated half-life is approximately 5,730 years, matching the known C-14 half-life used in radiocarbon dating.
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Starting with 1000 atoms and finding 250 remaining after 11,460 years gives a half-life of ~5,730 years. Exactly 2 half-lives elapsed (1000→500→250).
A half-life is the time required for exactly half of the radioactive atoms in a sample to decay. After one half-life, 50% remains; after two, 25%; after three, 12.5%; and so on. It is a statistical measure that applies to large populations of atoms and is constant for each specific isotope.
Under normal conditions, no. Half-life is determined by nuclear structure and fundamental forces. However, extreme conditions such as very high pressures, intense electromagnetic fields, or electron capture in highly ionized atoms can slightly alter half-lives. These changes are typically negligible for practical purposes.
Some nuclear resonance states have half-lives as short as 10⁻²² seconds. Among ground-state isotopes, hydrogen-7 has one of the shortest at about 2.3 × 10⁻²³ seconds. These extremely unstable nuclei decay almost instantaneously after formation.
Tellurium-128 holds the record with a half-life of approximately 2.2 × 10²⁴ years, over a trillion times the age of the universe. Bismuth-209, once considered stable, was found to have a half-life of about 1.9 × 10¹⁹ years.
For short half-lives, scientists measure the decrease in activity over time using radiation detectors. For very long half-lives, they measure the specific activity of a known mass of material. The decay constant is derived from the measured activity and known number of atoms, then converted to half-life.
Mean life ($$\tau = t_{1/2}/\ln 2$$) is the average time an atom exists before decaying. It is longer than the half-life because the exponential distribution is right-skewed — while half the atoms decay before $$t_{1/2}$$, some survive much longer, pulling the average above the median. The ratio is always $$\tau/t_{1/2} = 1/\ln 2 \approx 1.443$$.
Generally, longer half-lives indicate greater nuclear stability. Stable isotopes can be thought of as having infinite half-lives. The half-life depends on the type of decay, the nuclear binding energy, quantum tunneling probabilities, and the energy difference between parent and daughter states.
The mathematical formula is identical for any first-order exponential process, including biological elimination of drugs and chemicals. However, biological half-life refers to clearance from the body through metabolism and excretion, not radioactive decay. The effective half-life combines both: $$1/t_{eff} = 1/t_{phys} + 1/t_{bio}$$.
Theoretically, you need at least two measurements (initial and final quantity at known times). In practice, multiple measurements at different times are taken to reduce statistical uncertainty and confirm exponential behavior. The calculator uses the two-point method for simplicity.
For alpha decay, the Geiger-Nuttall law shows an inverse relationship: higher decay energies generally correspond to shorter half-lives. This is because higher-energy alpha particles have a greater probability of quantum tunneling through the nuclear potential barrier. For beta decay, the relationship is more complex and depends on the transition type.
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