Revision notes
Read the core explanations from Understanding Nuclear Equations before testing yourself from memory.
1. What Are Nuclear Equations?
When radioactive atoms decay, they don't just disappear - they transform into different atoms. Nuclear equations are the scientific way of showing exactly what happens during this transformation.
Think of a nuclear equation like a recipe. On the left side, you have your starting ingredient (the radioactive nucleus). On the right side, you have what you end up with (the new nucleus plus whatever particle was emitted). The equation must balance - you can't create or destroy protons and neutrons, only rearrange them.
Every nucleus in a nuclear equation is written with two numbers: the mass number (top) shows the total protons plus neutrons, and the atomic number (bottom) shows just the protons. This notation tells us exactly which element we're dealing with and which isotope.
2. The Language of Decay - Alpha and Beta Symbols
Nuclear decay involves specific particles being emitted, and each has its own symbol. You need to recognise these symbols instantly in exams because they appear in every nuclear equation.
The alpha particle symbol makes sense when you think about it - it's literally a helium nucleus, so it has mass number 4 (2 protons + 2 neutrons) and atomic number 2 (2 protons). The beta particle is trickier - it's an electron, so it has virtually no mass (mass number 0) but carries negative charge (atomic number -1).
**Trap**: Many students think beta particles are positrons or that they come from electron shells. Actually, beta particles are electrons created inside the nucleus when a neutron transforms into a proton plus an electron.
3. How Decay Changes the Nucleus
Here's where nuclear equations become powerful - they show you exactly how the nucleus changes during decay. Different types of decay affect mass and charge in predictable ways.
When an alpha particle shoots out, it takes 4 units of mass (2 protons + 2 neutrons) and 2 units of positive charge with it. This means the remaining nucleus becomes lighter and less positively charged. The element actually changes because it now has fewer protons.
Beta decay works differently. When a neutron in the nucleus converts to a proton plus an electron, the electron (beta particle) gets ejected. The mass stays the same because you still have the same total number of particles, but the charge increases by 1 because you now have one more proton.
4. Gamma Rays - The Exception
Gamma rays are different from alpha and beta particles. They're electromagnetic radiation - pure energy with no mass and no charge. When a nucleus emits a gamma ray, it's getting rid of excess energy but not changing its composition.
This means gamma emission doesn't change the mass number or atomic number of the nucleus. The element stays the same, but the nucleus moves from an excited state to a lower energy state. Think of it like a light bulb giving off light - the bulb doesn't change, it just releases energy.
In nuclear equations, gamma rays are often written as $\gamma$ or sometimes omitted entirely because they don't affect the mass or charge balance. The key point for exams is knowing that gamma emission leaves the nucleus chemically unchanged.
5. Balancing Nuclear Equations - The Conservation Rules
Nuclear equations follow strict conservation laws - the total mass number and total atomic number must be the same on both sides. This is your key to solving any nuclear equation problem, even when you don't know all the details.
The conservation approach works for any type of decay. For beta decay, remember that the beta particle contributes 0 to mass but -1 to charge. For gamma decay, the gamma ray contributes nothing to either mass or charge totals.
6. Exam Success with Nuclear Equations
Nuclear equation questions are mark-winners if you know the method. Examiners love testing whether you can balance equations and identify the changes that occur during decay.
**Common exam mistakes**: Writing beta particles as $^0_1e$ instead of $^0_{-1}e$ (wrong charge), forgetting to balance both mass and atomic numbers, and confusing which number represents what in nuclear notation.
The key to success is systematic checking. After writing any nuclear equation, verify that the mass numbers add up correctly on both sides, then check the atomic numbers. This two-step verification catches most errors before you submit your answer.