Binding Energy (AQA A Level Physics): Revision Note

Exam code: 7408

Katie M

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Binding energy per nucleon graph

  • In order to compare nuclear stability, it is useful to look at the binding energy per nucleon

  • The binding energy per nucleon is defined as:

The binding energy of a nucleus divided by the number of nucleons in the nucleus

  • A higher binding energy per nucleon indicates a higher stability

  • In other words, more energy is required to separate the nucleons contained within a nucleus

Graph of average binding energy per nucleon against number of nucleons, rising to a peak at iron-56 near 8.8 MeV then gradually falling towards uranium-235 and uranium-238. Fusion and fission arrows point towards the peak.
By plotting a graph of binding energy per nucleon against nucleon number, the stability of elements can be inferred

Key features of the graph

  • At low values of A:

    • Nuclei have lower binding energies per nucleon than at large values of A, but they tend to be stable when N = Z

    • This means light nuclei have weaker electrostatic forces and will undergo fusion

    • The gradient is much steeper compared to the gradient at large values of A

    • This means that fusion reactions release a greater binding energy than fission reactions

  • At high values of A:

    • Nuclei have generally higher binding energies per nucleon, but this gradually decreases with A

    • This means the heaviest elements are the most unstable and will undergo fission

    • The gradient is less steep compared to the gradient at low values of A

    • This means that fission reactions release less binding energy than fusion reactions

  • Iron (A = 56) has the highest binding energy per nucleon, which makes it the most stable of all the elements

  • Helium (4He), carbon (12C) and oxygen (16O) do not fit the trend

    • Helium-4 is a particularly stable nucleus hence it has a high binding energy per nucleon

    • Carbon-12 and oxygen-16 can be considered to be three and four helium nuclei, respectively, bound together

Comparing fusion and fission

Similarities

  • In both fusion and fission, the total mass of the products is slightly less than the total mass of the reactants

  • The mass defect is equivalent to the binding energy that is released

  • As a result, both fusion and fission reactions release energy

Differences

  • In fusion, two smaller nuclei combine into a larger nucleus

  • In fission, an unstable nucleus splits into two smaller nuclei

  • Fusion occurs between light nuclei (A < 56)

  • Fission occurs in heavy nuclei (A > 56)

  • In light nuclei, attractive nuclear forces dominate over repulsive electrostatic forces between protons, and this contributes to nuclear stability 

  • In heavy nuclei, repulsive electrostatic forces between protons begin to dominate over attractive nuclear forces, and this contributes to nuclear instability

  • Fusion releases much more energy per kg than fission

  • Fusion requires a greater initial input of energy than fission

Worked Example

The equation below represents one possible decay of the induced fission of a nucleus of uranium-235.

U92235 + n01 → Sr3891 + Xe54142 + 3n01

The graph shows the binding energy per nucleon plotted against nucleon number A.

Graph of binding energy per nucleon against nucleon number A, rising to a peak near A = 56 then declining. Readings are U-235: 7.5 MeV, Sr-91: 8.7 MeV and Xe-142: 8.2 MeV

Calculate the energy released:

(a) By the fission process represented by the equation [3]

(b) When 1.0 kg of uranium, containing 3% by mass of U-235, undergoes fission [3]

Answer:

Part (a)

Step 1: Use the graph to identify each isotope’s binding energy per nucleon

Annotated graph of binding energy per nucleon against nucleon number A, rising to a peak near A = 56 then declining. Readings are U-235: 7.5 MeV, Sr-91: 8.7 MeV and Xe-142: 8.2 MeV
  • Binding energy per nucleon (U-235) = 7.5 MeV

  • Binding energy per nucleon (Sr-91) = 8.2 MeV

  • Binding energy per nucleon (Xe-142) = 8.7 MeV [1 mark]

Step 2: Determine the binding energy of each isotope

Binding energy = Binding Energy per Nucleon × Mass Number

  • Binding energy of U-235 nucleus = (235 × 7.5) = 1762.5 MeV

  • Binding energy of Sr-91 = (91 × 8.2) = 746.2 MeV

  • Binding energy of Xe-142 = (142 × 8.7) = 1235.4 MeV [1 mark]

Step 3: Calculate the energy released

Energy released = Binding energy after (Sr + Xe) – Binding energy before (U)

Energy released = (1235.4 + 746.2) − 1762.5 = 219.1 MeV [1 mark]

Part (b)

Step 1: Calculate the energy released by 1 mol of uranium-235

  • There are NA (Avogadro’s number) atoms in 1 mol of U-235, which is equal to a mass of 235 g

  • Energy released by 235 g of U-235 = (6.02 × 1023) × 219.1 MeV

Step 2: Convert the energy released from MeV to J

  • 1 MeV = 1.6 × 10−13 J

Energy released = (6.02 × 1023) × 219.1 × (1.6 × 10−13) = 2.1104 × 1013 J [1 mark]

Step 3: Work out the proportion of uranium-235 in the sample

  • 1 kg of uranium which is 3% U-235 contains 0.03 kg or 30 g of U-235 [1 mark]

Step 4: Calculate the energy released by the sample

Energy released from 1 kg of Uranium = (2.1104 × 1013) × 30235

Energy released from 1 kg of Uranium = 2.69 × 1012 J [1 mark]

Examiner Tips and Tricks

Checklist on what to include (and what not to include) in an exam question asking you to draw a graph of binding energy per nucleon against nucleon number:

  • You will be expected to draw the best fit curve AND a cross to show the anomaly that is helium

  • Do not begin your curve at A = 0A = 0, this is not a nucleus

  • Make sure to correctly label both axes AND units for binding energy per nucleon

  • You will be expected to include numbers on the axes, mainly at the peak to show the position of iron (56Fe)

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Katie M

Author: Katie M

Expertise: Curriculum Expert

Katie has always been passionate about the sciences, and completed a degree in Astrophysics at Sheffield University. She decided that she wanted to inspire other young people, so moved to Bristol to complete a PGCE in Secondary Science. She particularly loves creating fun and absorbing materials to help students achieve their exam potential.

Timothy Sit

Reviewer: Timothy Sit

Expertise: Content Creator

Timothy graduated with a first class degree in Mathematics and Physics from the University of Warwick. After working as a postgraduate researcher, Timothy has worked as a content creator for various online revision platforms, creating physics resources for a range of levels and exam boards.