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HSCScience Physics · Y12 · M8
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Year 12 Physics Module 8 ⏱ ~45 min 5 MC · 2 Short Answer Lesson 9 of 17

The Nuclear Model of the Atom

In 1909, Hans Geiger and Ernest Marsden at Manchester University, under Ernest Rutherford's direction, fired 8 MeV alpha particles at gold foil 10⁻⁷ m thick. Most passed straight through, but 1 in 20,000 rebounded at angles greater than 90°. Rutherford calculated that such deflections required a nuclear radius of less than 10⁻¹⁴ m — meaning the nucleus occupies only 10⁻¹⁵ of the atom's volume and the atom is otherwise empty space. Rutherford published the nuclear model of the atom in 1911.

Today's hook: In 1909, Hans Geiger and Ernest Marsden at Manchester University fired a beam of 8 MeV alpha particles at a gold foil just 10⁻⁷ m thick. Of every 20,000 alpha particles fired, roughly 19,999 passed straight through. But 1 in 20,000 bounced back at angles greater than 90°. Ernest Rutherford said it was "as if you fired a 15-inch artillery shell at tissue paper and it came back and hit you." What does that 1-in-20,000 result tell you about the structure of the gold atoms inside that foil?
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Worksheets

Practise this lesson

Four printable worksheets that build from the foundations up to exam-style questions — start at whatever level suits you.

Before you read — predict

Imagine firing tiny positively charged particles at a thin gold foil. Most pass straight through, but a few bounce back at large angles.

Before reading on, answer:

  1. What does it mean that most particles pass straight through?
  2. What does it mean that some particles bounce back?
  3. What model of atomic structure would explain both observations?

Warm-up: In Thomson's "plum pudding" model, the positive charge in an atom is:

Learning Intentions
goals

Know — Rutherford's Model

  • Tiny dense nucleus (~$10^{-15}$ m)
  • Electrons orbit at large distance (~$10^{-10}$ m)
  • Mostly empty space

Understand — Scattering Evidence

  • Geiger-Marsden experiment
  • Most particles undeflected
  • Large-angle scattering explained

Can Do — Apply Nuclear Physics

  • Calculate closest approach ($r_{min}$)
  • Analyse scattering data
  • Evaluate atomic models critically
Scan these before reading
vocab
Alpha particle ($\alpha$)Helium nucleus ($^4_2\text{He}$); positively charged (+2e), mass ≈ 4 u. Used in Rutherford's scattering experiments.
NucleusTiny dense core of an atom containing protons and neutrons; diameter ~$10^{-15}$ m (femtometres).
Closest approach ($r_{min}$)Minimum distance of an alpha particle from the nucleus in a head-on collision; found by equating kinetic energy to electrical potential energy.
Atomic number ($Z$)Number of protons in the nucleus; defines the element and the nuclear charge.
Mass number ($A$)Total number of nucleons (protons + neutrons) in the nucleus. Nuclear radius scales as $R = R_0 A^{1/3}$.
Cross-lesson links: L10 showed supernovae create the heaviest elements. L11 begins examining atomic structure — the same nucleus that fusion builds in stars and that supernovae scatter across space. Rutherford's 1909 gold foil experiment is the most important physics experiment for this section of HSC; the quantitative result (1 in 20,000 backscattered) is regularly set as a calculation.
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The Geiger-Marsden Experiment
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How Rutherford discovered the nucleus

In 1909, Hans Geiger and Ernest Marsden, under Rutherford's direction, fired alpha particles (helium nuclei, $^4_2\text{He}$, charge $+2e$, mass $\approx 4$ u) at a very thin gold foil (~$10^{-7}$ m thick). They observed three key results:

  1. Most alpha particles passed straight through with little or no deflection. This indicated that atoms are mostly empty space.
  2. Some alpha particles were deflected through small angles ($< 10°$). This suggested the positive charge was concentrated, not spread evenly.
  3. A very few alpha particles (~1 in 8,000) were deflected by more than 90°, with some bouncing almost straight back. This required a very small, very dense, positively charged centre capable of exerting enormous repulsive Coulomb force.

Rutherford described this as "almost as incredible as if you fired a 15-inch shell at a piece of tissue paper and it came back and hit you." The results were completely incompatible with Thomson's "plum pudding" model, where positive charge was spread throughout the atom like a diffuse cloud.

Rutherford proposed the nuclear model:

  • Almost all the atom's mass is concentrated in a tiny nucleus (~$10^{-15}$ m).
  • The nucleus is positively charged.
  • Electrons orbit the nucleus at relatively large distances (~$10^{-10}$ m).
  • Most of the atom is empty space.
α source Gold foil Nucleus Most: straight through Some: small deflection Few: large angle Note: Nucleus greatly enlarged for visibility

Figure 1 — Alpha particle scattering showing mostly straight-through, some small deflection, and rare large-angle scattering. The fraction scattered by >90° was ~1 in 8,000.

Stop and check

Why would the plum pudding model predict only small-angle scattering? Why does large-angle scattering require a concentrated positive charge?

The Geiger-Marsden experiment (1909) fired alpha particles (+2e) at gold foil. Most passed straight through (atom is mostly empty space); ~1 in 8,000 scattered back (>90°), disproving Thomson's plum pudding model. Rutherford proposed a tiny dense positive nucleus (~10⁻¹⁵ m) with electrons orbiting at ~10⁻¹⁰ m.

Write this in your own words — exam questions often ask you to describe what the results implied about atomic structure.

In the Geiger-Marsden experiment, the fact that most alpha particles passed straight through the gold foil indicates that:

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Closest Approach and Nuclear Size
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Using energy conservation to probe the nucleus

We just saw that large-angle scattering in the Geiger-Marsden experiment proved atoms have a tiny dense positive nucleus. That raises a question: can we use the scattering data to actually measure how big the nucleus is? This card answers it → yes — by setting kinetic energy equal to Coulomb potential energy at closest approach, we get an upper limit on nuclear radius.

When an alpha particle approaches a nucleus head-on, its kinetic energy is converted to electrical potential energy. At the closest approach, all kinetic energy has become potential energy:

$$E_k = \dfrac{1}{4\pi\varepsilon_0} \dfrac{q_1 q_2}{r}$$

For an alpha particle ($q_1 = +2e$) approaching a nucleus with atomic number $Z$ ($q_2 = +Ze$):

$$r_{min} = \dfrac{1}{4\pi\varepsilon_0} \dfrac{2Ze^2}{E_k}$$

This gives an upper limit on the nuclear radius — the actual nucleus must be smaller than $r_{min}$ because the alpha particle turns around before reaching the nuclear surface. Rutherford's calculations gave nuclear radii on the order of $10^{-15}$ m (femtometres), about 100,000 times smaller than the atomic radius (~$10^{-10}$ m).

Later experiments confirmed that nuclear radius scales with mass number:

$$R = R_0 A^{1/3}$$

where $R_0 \approx 1.2$ fm and $A$ is the mass number (protons + neutrons). Since volume $\propto R^3 \propto A$ and mass $\propto A$, this implies nuclear density is approximately constant for all nuclei — nucleons are packed at roughly the same density throughout the periodic table.

Nuclear Physics Formulae

$r_{min} = \dfrac{1}{4\pi\varepsilon_0} \dfrac{2Ze^2}{E_k}$ — closest approach distance (head-on)

$R = R_0 A^{1/3}$ — nuclear radius ($R_0 \approx 1.2$ fm)

$F = \dfrac{1}{4\pi\varepsilon_0} \dfrac{q_1 q_2}{r^2}$ — Coulomb force

$E_p = \dfrac{1}{4\pi\varepsilon_0} \dfrac{q_1 q_2}{r}$ — electrical potential energy

$k = \dfrac{1}{4\pi\varepsilon_0} = 8.99\times10^9$ N·m²/C²; $e = 1.6\times10^{-19}$ C; 1 MeV $= 1.6\times10^{-13}$ J

+Ze α Ek = max Ep ≈ 0 α Ek = 0 Ep = max r_min Energy conservation: Ek(initial) = Ep(at r_min) = k·2Ze²/r_min

Figure 2 — At closest approach, all kinetic energy converts to electrical potential energy. The alpha particle momentarily stops before being repelled back.

Stop and check — worked problem

An alpha particle with kinetic energy 5.0 MeV approaches a gold nucleus ($Z = 79$) head-on. Calculate the distance of closest approach.

Given: $e = 1.6\times10^{-19}$ C, $k = 8.99\times10^9$ N·m²/C², 1 MeV $= 1.6\times10^{-13}$ J

Closest approach formula: r_min = k·2Ze²/E_k (set E_k = E_p at r_min). This is an upper limit on nuclear radius — the actual nucleus is smaller. R = R₀A^(1/3) with R₀ ≈ 1.2 fm shows constant nuclear density. Convert 1 MeV = 1.6×10⁻¹³ J before calculating. Nuclear radius ~10⁻¹⁵ m is 100,000× smaller than atomic radius ~10⁻¹⁰ m.

Note the key formula and the MeV conversion — both will appear in HSC calculations.

The distance of closest approach $r_{min}$ is an upper limit on the nuclear radius.

The nuclear radius formula $R = R_0 A^{1/3}$ implies that larger nuclei are less dense than smaller ones.

Increasing the kinetic energy of the alpha particle decreases the closest approach distance.

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Comparing Atomic Models
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What each model explains — and what it cannot

We just saw how Rutherford used closest approach calculations to pin down the nuclear radius at ~10⁻¹⁵ m. That raises a question: if Rutherford's nuclear model was such a success, why did physicists immediately need to replace it? This card answers it → classical electromagnetism predicts orbiting electrons would radiate energy and spiral into the nucleus — Rutherford's model cannot explain stable atoms.

Scientific models are judged by their ability to explain existing observations and predict new ones. The transition from Thomson's to Rutherford's model is a textbook example of how unexpected experimental evidence forces a paradigm shift.

Thomson's Model "Plum pudding" (1904) Diffuse positive cloud with embedded electrons Rutherford's Model Nuclear model (1911) +Ze Tiny dense positive nucleus electrons orbit at distance

Figure 3 — Thomson's plum pudding model (left) predicts only small-angle alpha scattering. Rutherford's nuclear model (right) explains large-angle scattering via strong Coulomb repulsion from the dense nucleus.

Rutherford's nuclear model explained the scattering data brilliantly, but it had a major unresolved problem: according to classical electromagnetism, an accelerating charge radiates energy. An orbiting electron would continuously radiate, lose energy, and spiral into the nucleus in a fraction of a second. This required a new theory — Bohr's quantum model — to explain why electrons remain in stable orbits.

HSC Tip — Rutherford Scattering

A common exam trap: confusing closest approach with nuclear radius. The closest approach is an upper limit — the alpha particle turns around before reaching the actual nuclear surface because Coulomb repulsion stops it. The actual nuclear radius is smaller. When calculating closest approach, convert MeV to joules: $1\text{ MeV} = 1.6\times10^{-13}$ J. Remember that $r_{min} \propto Z/E_k$ — higher energy alphas or lower-Z targets give smaller closest approach distances. Also note that Rutherford's model could not explain why electrons don't spiral into the nucleus (this required Bohr's quantum model).

Thomson's plum pudding model predicts only small-angle scattering — it is disproved by large-angle results. Rutherford's nuclear model (1911) explains large-angle scattering but fails classically: an orbiting electron radiates energy and should spiral into the nucleus in ~10⁻¹¹ s. This instability required Bohr's quantum model (1913) to resolve with quantised orbits.

Jot down both models' key features and the one fatal flaw in Rutherford's — this compare-and-contrast is a regular HSC question.

An alpha particle with $E_k = 7.7$ MeV approaches a gold nucleus ($Z = 79$) head-on. Using $r_{min} = k \cdot 2Ze^2/E_k$ with $k = 8.99\times10^9$ N·m²/C², $e = 1.6\times10^{-19}$ C, and 1 MeV $= 1.6\times10^{-13}$ J, the distance of closest approach in metres (to 2 sig figs) is approximately $2.96\times10^{-14}$ m. Enter the coefficient (the first two sig figs): _____×10⁻¹⁴ m.

Misconceptions — Final Check
Wrong: "The distance of closest approach equals the nuclear radius."
Right: The closest approach gives an upper limit on nuclear radius. The alpha particle stops at $r_{min}$ due to Coulomb repulsion — it never actually touches the nuclear surface. The real nuclear radius is smaller.
Wrong: "Rutherford's model is complete — it fully explains atomic structure."
Right: Rutherford's model cannot explain why electrons don't spiral into the nucleus (classical radiation), nor why atoms emit only specific wavelengths of light. These required Bohr's quantum model.

Three of these statements about Rutherford's nuclear model are correct. Pick the odd one out.

Activity 1 — Closest Approach Calculations
ApplyBand 4

Practice using $r_{min} = k \cdot 2Ze^2/E_k$

  1. An alpha particle with $E_k = 5.0$ MeV approaches a gold nucleus ($Z = 79$) head-on. Calculate the distance of closest approach in metres. ($k = 8.99\times10^9$ N·m²/C², $e = 1.6\times10^{-19}$ C, 1 MeV $= 1.6\times10^{-13}$ J)
  2. Repeat for a silver target ($Z = 47$). How does the closest approach compare to gold?
  3. If the alpha particle's kinetic energy is doubled, what happens to $r_{min}$? Explain using the formula.
  4. The nuclear radius formula gives $R = R_0 A^{1/3}$ with $R_0 = 1.2$ fm. Calculate the radius of a gold nucleus ($A = 197$) and compare it to your answer in Q1.
Activity 2 — Evaluating the Nuclear Model
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Compare models and explain experimental evidence

  1. Describe two observations from the Geiger-Marsden experiment and explain how each supports Rutherford's nuclear model over Thomson's plum pudding model.
  2. Explain why Rutherford's model was a significant advance over Thomson's model, even though it could not explain stable electron orbits.
  3. A student argues: "Because most alpha particles passed straight through, the nucleus must be large." Identify the flaw in this reasoning.
  4. The nuclear density of gold is approximately $2.3\times10^{17}$ kg/m³. Compare this to the density of water ($1000$ kg/m³). What does this tell us about how matter is distributed in an atom?
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