In nuclear physics, the half‑life of an isotope is the time required for half of the nuclei in a sample to decay. If you start with \$N0\$ atoms, after one half‑life you will have \$N0/2\$ atoms remaining.
The number of atoms remaining after a time \$t\$ is given by:
\$N(t)=N0\left(\frac{1}{2}\right)^{\frac{t}{T{1/2}}}\$
Where \$T_{1/2}\$ is the half‑life of the isotope.
Let’s walk through a few examples. 📊
| Half‑life (t) | Atoms remaining |
|---|---|
| 0 | 100 |
| 1 T1/2 | 50 |
| 2 T1/2 | 25 |
| 3 T1/2 | 12.5 |
Step 1: Identify \$N_0\$ (any number, say 1000 atoms). Step 2: Plug into the formula:
\$N(11460)=1000\left(\frac{1}{2}\right)^{\frac{11460}{5730}}=1000\left(\frac{1}{2}\right)^2=250\$
So 250 atoms remain. 🎉
Since 18 hours = 3 half‑lives, the activity reduces by a factor of 2³ = 8.
\$200\;\mu\text{Ci} \times \frac{1}{8} = 25\;\mu\text{Ci}\$
| Isotope | Half‑life |
|---|---|
| C‑14 (Carbon‑14) | 5730 years |
| I‑131 (Iodine‑131) | 8.02 days |
| Cs‑137 (Cesium‑137) | 30.17 years |
| U‑238 (Uranium‑238) | 4.468 × 10⁹ years |
Remember: Half‑life is a powerful tool for dating fossils, medical imaging, and nuclear power. Keep practicing the calculations, and the numbers will start to feel natural! 🚀