Overview of Radioactivity
Radioactivity refers to the process by which unstable atomic nuclei spontaneously emit radiation to become more stable. This phenomenon was first discovered by Henri Becquerel and later studied in detail by Marie and Pierre Curie. The section introduces three main types of radioactive emissions:
- Alpha Particles: Positively charged helium nuclei with high ionizing power but low penetration ability.
- Beta Particles: Negatively charged electrons with moderate penetration and ionizing powers.
- Gamma Rays: High-energy electromagnetic waves with no charge, capable of passing through substantial barriers like lead, but exhibiting low ionizing power.
The concept of radioactive decay is explored, indicating how unstable nuclei transition to more stable daughter nuclei through different types of decay processes, including alpha decay, beta decay, and gamma emission.
Nuclear reactions, such as fission (the splitting of heavy nuclei) and fusion (the combining of light nuclei), are different processes that release energy. The section emphasizes the notion of half-life, describing the time it takes for half of a radioactive sample to decay.
Applications in fields such as medicine (e.g., cancer treatment and medical imaging), industry (e.g., thickness control), agriculture (e.g., pest control), and archaeology (e.g., carbon-14 dating) illustrate the versatility of radioactive materials. Lastly, safety measures for handling radioactive substances are crucial to minimize exposure.