Radioactive Decay (alpha, beta, gamma)

    OCR
    GCSE
    Physics

    This comprehensive study guide for OCR GCSE Physics (7.3) demystifies radioactive decay. It provides a detailed breakdown of alpha, beta, and gamma radiation, focusing on the core knowledge required to secure top marks in your exam, complete with worked examples and multimedia assets.

    7
    Min Read
    3
    Examples
    5
    Questions
    6
    Key Terms
    🎙 Podcast Episode
    Radioactive Decay (alpha, beta, gamma)
    14:06
    0:00-14:06

    Study Notes

    An overview of Alpha, Beta, and Gamma radiation emitted from an unstable nucleus.

    Overview

    Radioactive decay is a fundamental concept in nuclear physics, describing how unstable atomic nuclei release energy to become more stable. For your OCR GCSE Physics exam, a thorough understanding of the three main types of decay—alpha (α), beta (β), and gamma (γ)—is essential. This topic is not just about memorising properties; it's about applying that knowledge to balance nuclear equations, understand safety precautions, and explain real-world applications. Examiners will test your ability to compare the ionising and penetrating power of each radiation type and link these properties to their uses, such as in smoke detectors and medical treatments. This guide will walk you through the core principles, provide examiner insights, and equip you with the skills to tackle any question on radioactive decay with confidence. Expect to see a mix of short-answer definition questions (AO1), application questions (AO2), and longer evaluation questions (AO3).

    Listen to the GCSE Physics revision podcast on Radioactive Decay.

    Key Concepts

    Concept 1: The Unstable Nucleus and Random Decay

    At the heart of radioactivity is the unstable nucleus. An atomic nucleus can be unstable if it has an imbalance of protons and neutrons, or simply too much energy. To achieve stability, it spontaneously emits radiation. A crucial point that candidates must remember is that this process is entirely random and spontaneous. You cannot predict which nucleus will decay next, nor can you influence the rate of decay by changing physical conditions like temperature, pressure, or by chemical reactions. This is a common misconception tested by examiners.

    Examiner's Note: Credit is often given for explicitly stating that decay is a nuclear process, unaffected by external factors. A typical 1-mark question might be: "State two factors that do not affect the rate of radioactive decay."

    Concept 2: Alpha (α) Decay

    An alpha particle is a helium nucleus, composed of 2 protons and 2 neutrons. It has a relative mass of 4 and a charge of +2. When a nucleus undergoes alpha decay, it ejects an alpha particle.

    • Effect on Nucleus: The mass number (top number) decreases by 4. The atomic number (bottom number) decreases by 2. This means the element itself changes, a process called transmutation.
    • Properties: Due to their size and +2 charge, alpha particles are highly ionising. They readily knock electrons off atoms they collide with. However, this causes them to lose energy quickly, giving them very low penetrating power. They are stopped by just a few centimetres of air or a single sheet of paper.

    Example: Uranium-238 decays into Thorium-234.

    Concept 3: Beta (β) Decay

    A beta particle is a high-energy electron ejected from the nucleus. This is a critical point: it originates from the nucleus, not the electron shells. Beta decay occurs when a neutron in the nucleus turns into a proton.

    • Effect on Nucleus: The mass number remains unchanged (as one neutron is lost but one proton is gained). The atomic number increases by 1 (due to the new proton).
    • Properties: Beta particles are much smaller and faster than alpha particles. They have a charge of -1. They are moderately ionising and have moderate penetrating power. They can travel several metres in air and are stopped by about 5mm of aluminium.

    Example: Carbon-14 decays into Nitrogen-14.

    Concept 4: Gamma (γ) Emission

    Gamma radiation is not a particle; it is a high-energy electromagnetic wave. It has no mass and no charge. Gamma emission often occurs after an alpha or beta decay event, as it is a way for the newly formed nucleus to release excess energy and settle into a more stable state.

    • Effect on Nucleus: There is no change to the mass number or the atomic number of the nucleus.
    • Properties: Because they have no charge or mass, gamma rays are weakly ionising. They do not interact strongly with atoms. This same property gives them very high penetrating power. They can only be significantly reduced by several centimetres of lead or metres of concrete.

    Comparison of the penetrating and ionising power of the three main types of radiation.

    Mathematical/Scientific Relationships

    Balancing nuclear equations is a core mathematical skill for this topic. The fundamental rule is the conservation of mass number and atomic number.

    The Golden Rule: The sum of the mass numbers (top) on the left side of the equation must equal the sum on the right. The sum of the atomic numbers (bottom) on the left must also equal the sum on the right.

    A quick-reference guide to balancing nuclear decay equations.

    Formulas (Must Memorise)

    1. Alpha Decay General Form:

      • A/Z X → (A-4)/(Z-2) Y + 4/2 α
      • Where X is the parent nucleus and Y is the daughter nucleus.
    2. Beta Decay General Form:

      • A/Z X → A/(Z+1) Y + 0/-1 β (or 0/-1 e)
      • Where X is the parent nucleus and Y is the daughter nucleus.
    3. Gamma Emission General Form:

      • A/Z X* → A/Z X + γ
      • The asterisk (*) denotes an excited nucleus.

    Practical Applications

    Examiners expect you to link the properties of each radiation type to its uses. Marks are awarded for justifying the choice of radiation.

    ApplicationRadiation UsedProperty JustificationTier
    Smoke DetectorsAlpha (α)High ionising power creates a current in the air. Low penetrating power means it is safely contained and won't escape the detector casing.Both
    Paper Thickness GaugeBeta (β)Moderate penetrating power allows it to pass through paper but be affected by thickness changes. Alpha would be stopped; gamma would pass through unaffected.Both
    Sterilising EquipmentGamma (γ)High penetrating power allows it to penetrate packaging to kill all bacteria. As it is not a particle, it does not make the equipment radioactive.Both
    Medical TracersGamma (γ)High penetrating power allows it to be detected outside the body. Low ionising power minimises tissue damage. A short half-life is also crucial.Higher
    Cancer TreatmentGamma (γ)High penetrating power allows it to reach deep-seated tumours. The beam can be focused to kill cancer cells while minimising damage to healthy tissue.Higher

    Safety: Irradiation vs. Contamination

    A common source of confusion is the difference between irradiation and contamination.

    • Irradiation: This is when an object or person is exposed to radiation from an external source. The exposure stops when the source is removed. Shielding (e.g., lead apron) and distance are the main protective measures.
    • Contamination: This is when radioactive atoms get onto or into an object or person. The person is now a source of radiation. This is far more dangerous, especially with alpha emitters, as the internal organs are directly exposed to highly ionising radiation. Protective clothing (gloves, lab coat) and careful handling are required to prevent contamination.

    Visual Resources

    2 diagrams and illustrations

    Comparison of the penetrating and ionising power of the three main types of radiation.
    Comparison of the penetrating and ionising power of the three main types of radiation.
    A quick-reference guide to balancing nuclear decay equations.
    A quick-reference guide to balancing nuclear decay equations.

    Interactive Diagrams

    2 interactive diagrams to visualise key concepts

    YesNoYesNoIs the radiation stopped by paper?It is Alpha radiationIs it stopped by 5mm of Aluminium?It is Beta radiationIt is Gamma radiation

    A simple flowchart to identify a type of radiation based on its penetrating power. This is a useful decision-making tool for exam questions.

    Gamma PropertiesBeta PropertiesAlpha PropertiesRadioactive DecayEmits RadiationUnstable NucleusTypesAlpha αBeta βGamma γHelium NucleusHigh IonisingLow PenetrationElectron from NucleusMedium IonisingMedium PenetrationEM WaveLow IonisingHigh Penetration

    A concept map summarising the three types of radioactive decay and their key properties.

    Worked Examples

    3 detailed examples with solutions and examiner commentary

    Practice Questions

    Test your understanding — click to reveal model answers

    Q1

    State two ways in which a beta particle differs from an alpha particle.

    2 marks
    foundation

    Hint: Think about their charge and what they are made of.

    Q2

    A sample of radioactive material is placed in a lead box. A detector outside the box records a high count rate. A sheet of 5mm thick aluminium is placed between the box and the detector, and the count rate drops to almost zero. What type of radiation is the sample emitting? Explain your answer.

    3 marks
    standard

    Hint: Consider what each material is known to stop.

    Q3

    The nucleus of a nitrogen atom, ¹⁴₇N, can be changed into an oxygen atom, ¹⁷₈O, by bombarding it with a particle. Write a balanced nuclear equation for this reaction and identify the bombarding particle.

    4 marks
    challenging

    Hint: Set up the equation with an unknown particle X and balance the top and bottom numbers.

    Q4

    Describe the difference between being irradiated and being contaminated with a radioactive substance.

    2 marks
    standard

    Hint: Think about where the radioactive source is in relation to the person.

    Q5

    Explain why gamma radiation is used for sterilising medical instruments.

    3 marks
    standard

    Hint: Link two key properties of gamma to this application.

    Explore this topic further

    View Topic PageAll Physics Topics

    Key Terms

    Essential vocabulary to know

    More Physics Study Guides

    View all

    Refraction

    OCR
    GCSE

    This guide explains light refraction for OCR GCSE Physics (4.6), covering why light bends, how to draw ray diagrams, and the secrets to exam success. Master the concepts of optical density and total internal reflection to secure top marks.

    Isotopes

    OCR
    GCSE

    This guide provides a comprehensive overview of isotopes for OCR GCSE Physics (7.2), focusing on core definitions, calculations, and exam technique. It's designed to help you secure maximum marks by mastering the difference between isotopes and ions, understanding nuclear notation, and avoiding common pitfalls.

    Galaxies

    OCR
    GCSE

    Unlock top marks in your OCR GCSE Physics exam by mastering Galaxies (Topic 8.7). This guide breaks down the vastness of space into bite-sized, exam-focused chunks, from the structure of our Milky Way to the mind-bending evidence for the Big Bang.

    Planets

    OCR
    GCSE

    This topic covers the structure of our Solar System, the role of gravitational forces in maintaining planetary orbits, and the historical shift from geocentric to heliocentric models. Understanding these concepts is essential for securing marks in both Foundation and Higher Tier questions, particularly those testing orbital mechanics and the nature of scientific progress.

    Stars

    OCR
    GCSE

    Explore the dramatic life and death of stars, from stable main sequence suns to explosive supernovae. This guide for OCR GCSE Physics (8.6) provides everything candidates need to master stellar evolution, secure top marks, and understand our cosmic origins."

    The Solar System

    OCR
    GCSE

    This guide covers OCR GCSE Physics Topic 8.1, The Solar System. It explores the shift from geocentric to heliocentric models, the physics of orbital motion, and the complete life cycles of stars. Mastering this topic is crucial for tackling high-mark questions on stellar evolution and gravitational forces.