How do fission and fusion release energy, and how is the energy found from the mass difference?
Nuclear fission and fusion, the conservation of mass-energy, and the calculation of the energy released using the mass difference and .
An SQA Higher Physics answer on nuclear reactions, covering nuclear fission and fusion, the conservation of mass-energy, and how to calculate the energy released from the mass difference using E equals mc squared.
Reviewed by: AI editorial process; not yet individually human-reviewed
Have a quick question? Jump to the Q&A page
Jump to a section
What this key area is asking
The SQA wants you to describe nuclear fission and fusion, state that mass and energy together are conserved, and calculate the energy released in a nuclear reaction from the mass difference using .
Fission and fusion
In fission, a nucleus such as uranium-235 absorbs a slow neutron, becomes unstable and splits. The released neutrons can trigger further fissions, giving a chain reaction that, when controlled, powers a nuclear reactor. In fusion, light nuclei such as deuterium and tritium are forced together at extremely high temperatures and pressures; this is the process that powers the Sun and the stars.
Conservation of mass-energy and E = mc^2
In a nuclear reaction the total mass before is slightly greater than the total mass after. The difference is the mass defect, and it does not vanish: it is converted into energy. Mass and energy are two forms of the same thing, linked by Einstein's relationship.
The key to every calculation is to find the difference between the total mass of the reactants and the total mass of the products, then multiply by . Because , even a mass defect of a few releases picojoules of energy per reaction, which is vast on the nuclear scale.
Examples in context
Nuclear power stations use a controlled fission chain reaction in uranium or plutonium to boil water and drive turbines; control rods absorb neutrons to keep the chain reaction steady. The Sun shines by fusing hydrogen into helium in its core, converting about four million tonnes of mass into energy every second. Experimental reactors such as ITER aim to harness fusion on Earth, which would give a near-limitless, low-waste energy source if the engineering of confining a hot plasma can be solved. Nuclear weapons release the same mass-energy uncontrolled. In every case the energy comes from a small loss of mass multiplied by the huge factor .
Try this
Q1. State the difference between nuclear fission and nuclear fusion. [2 marks]
- Cue. Fission splits a heavy nucleus into smaller nuclei; fusion joins light nuclei into a heavier one.
Q2. A reaction loses of mass. Calculate the energy released. Take . [3 marks]
- Cue. .
Q3. Explain why nuclear reactions release so much more energy than chemical reactions for the same mass of fuel. [1 mark]
- Cue. A measurable mass is converted to energy through , and the factor is enormous, whereas chemical reactions only rearrange electrons.
Exam-style practice questions
Practice questions written in the style of SQA exam questions on this dot point, with worked answer explainers. The year tag is the paper they imitate, not the source.
SQA Higher 20194 marksIn a fusion reaction the total mass of the particles decreases by 4.0 times ten to the power minus twenty-nine kg. Calculate the energy released. Take c as 3.0 times ten to the power eight metres per second.Show worked answer →
The lost mass is converted to energy.
Relationship: .
Substitution: .
Answer: J.
Markers reward squaring the speed of light, using the mass difference (not a total mass), and the answer with unit. A frequent slip is forgetting to square c.
SQA Higher 20214 marksState the difference between nuclear fission and nuclear fusion, and explain why both processes release energy in terms of the masses of the particles before and after the reaction.Show worked answer →
Fission is the splitting of a large, heavy nucleus into two smaller nuclei (plus neutrons), usually triggered by absorbing a neutron. Fusion is the joining of two small, light nuclei into a larger nucleus.
Both release energy because the total mass of the products is slightly less than the total mass of the reactants. This mass difference (the mass defect) is converted into energy according to . Because is very large, even a tiny mass loss releases a great deal of energy.
Markers reward correct definitions of fission (splitting heavy nuclei) and fusion (joining light nuclei), and linking the released energy to a loss of mass through .
Related dot points
- The standard model of fermions (quarks and leptons) and force-mediating bosons, the classification of hadrons into baryons and mesons, and antimatter.
An SQA Higher Physics answer on the standard model, covering the fermions (quarks and leptons), the force-mediating bosons, the classification of hadrons into baryons and mesons, and antimatter.
- The work done accelerating a charge through a potential difference, the force on a charge moving in a magnetic field, and the operation of particle accelerators.
An SQA Higher Physics answer on forces on charged particles, covering the work done accelerating a charge through a potential difference, the force on a charge moving in a magnetic field, and how particle accelerators work.
- The photon model of light, the photoelectric effect, the work function and threshold frequency, and the photoelectric equation for the kinetic energy of emitted electrons.
An SQA Higher Physics answer on wave-particle duality and the photoelectric effect, covering the photon model of light, the work function and threshold frequency, and the photoelectric equation for the kinetic energy of emitted electrons.
- Coherence and path difference, constructive and destructive interference, and the diffraction grating equation relating wavelength, slit spacing and the angle to a maximum.
An SQA Higher Physics answer on interference and diffraction, covering coherence and path difference, constructive and destructive interference, and the diffraction grating equation relating wavelength, slit spacing and the angle to a maximum.
- Refraction and the refractive index, critical angle and total internal reflection, and the emission and absorption line spectra produced by electron energy-level transitions.
An SQA Higher Physics answer on refraction and spectra, covering refraction and the refractive index, the critical angle and total internal reflection, and the emission and absorption line spectra produced by electron energy-level transitions.
Sources & how we know this
- SQA Higher Physics Course Specification — SQA (2018)