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Worked Solutions

Module 8: From the Universe to the Atom — Worked Solutions (HSC Physics)

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Worked examples for HSC Physics Module 8: From the Universe to the Atom. Each shows where the marks are awarded, the key idea, and the full solution explained by your choice of tutor — Stella, Ella or Cassie.

How to use these

Try each question first, then check your working. Use the tutor tabs to read the full solution in the style that suits you: Stella is direct and challenging, Ella is warm and explains the why, and Cassie is concise and analytical.

Useful constants: Planck's constant $h = 6.63 \times 10^{-34}\ \text{J s}$, speed of light $c = 3.0 \times 10^8\ \text{m s}^{-1}$, and $1\ \text{eV} = 1.6 \times 10^{-19}\ \text{J}$.

Example 1 — Atomic energy levels

Standard 3 marks

Question

A hydrogen atom emits a photon when an electron transitions from an energy level of $-1.51\ \text{eV}$ to a level of $-3.40\ \text{eV}$. Using $h = 6.63 \times 10^{-34}\ \text{J s}$, $c = 3.0 \times 10^8\ \text{m s}^{-1}$ and $1\ \text{eV} = 1.6 \times 10^{-19}\ \text{J}$, calculate the wavelength of the emitted photon.

Solution

The photon energy equals the drop in level energy: $\Delta E = E_{high} - E_{low}$.

$$\Delta E = (-1.51) - (-3.40) = 1.89\ \text{eV}$$

Convert to joules: $\Delta E = 1.89 \times 1.6\times10^{-19} = 3.024\times10^{-19}\ \text{J}$.

Now use $E = \dfrac{hc}{\lambda}$, rearranged for wavelength:

$$\lambda = \frac{hc}{\Delta E} = \frac{(6.63\times10^{-34})(3.0\times10^8)}{3.024\times10^{-19}} = 6.58\times10^{-7}\ \text{m}$$

So $\lambda \approx 6.58\times10^{-7}\ \text{m}$ — red light, as expected for this Balmer transition. Take the difference of the levels first, then convert; don't convert each level separately.

Where the marks go

  • 1 mark: Correct energy difference $\Delta E = 1.89\ \text{eV}$ converted to $3.024\times10^{-19}\ \text{J}$
  • 1 mark: Uses $\lambda = \dfrac{hc}{\Delta E}$ with correct substitution
  • 1 mark: Correct wavelength $\lambda = 6.58\times10^{-7}\ \text{m}$ with units

Key idea

A photon carries the energy gap between levels: $\Delta E = \dfrac{hc}{\lambda}$, so $\lambda = \dfrac{hc}{\Delta E}$ — quantised levels give a discrete emission spectrum.

Example 2 — Nuclear mass defect and binding energy

Challenging 4 marks

Question

A helium-4 nucleus is made of 2 protons and 2 neutrons. The mass of a proton is $1.6726 \times 10^{-27}\ \text{kg}$, the mass of a neutron is $1.6749 \times 10^{-27}\ \text{kg}$, and the measured mass of the helium-4 nucleus is $6.6447 \times 10^{-27}\ \text{kg}$. Using $c = 3.0 \times 10^8\ \text{m s}^{-1}$, calculate the mass defect and the binding energy of the nucleus.

Solution

First add up the masses of the separate nucleons:

$$2(1.6726\times10^{-27}) + 2(1.6749\times10^{-27}) = 6.6950\times10^{-27}\ \text{kg}$$

The mass defect is the difference between this and the measured nuclear mass:

$$\Delta m = 6.6950\times10^{-27} - 6.6447\times10^{-27} = 5.03\times10^{-29}\ \text{kg}$$

Convert that "missing" mass to energy with $E = \Delta m c^2$:

$$E = (5.03\times10^{-29})(3.0\times10^8)^2 = 4.53\times10^{-12}\ \text{J}$$

Mass defect $5.03\times10^{-29}\ \text{kg}$, binding energy $4.53\times10^{-12}\ \text{J}$. The defect is tiny — keep all your significant figures until the final step.

Where the marks go

  • 1 mark: Correct total nucleon mass $6.6950\times10^{-27}\ \text{kg}$
  • 1 mark: Correct mass defect $\Delta m = 5.03\times10^{-29}\ \text{kg}$
  • 1 mark: Applies $E = \Delta m c^2$ with correct substitution
  • 1 mark: Correct binding energy $E = 4.53\times10^{-12}\ \text{J}$ with units

Key idea

The mass defect $\Delta m$ is the difference between the sum of nucleon masses and the measured nuclear mass; the binding energy is $E = \Delta m c^2$ — the energy equivalent of the missing mass.