CCEA A-Level Physics 1210
Physical Quantities, Scalars and Vectors
Moments and Equilibrium
Linear Motion and Dynamics
Newton's Laws of Motion
Linear Momentum and Impulse
Work, Energy and Power
Current, Charge and Potential Difference
Resistance and Resistivity
Internal Resistance and Potential Dividers
Waves
Refraction
Lenses
Superposition, Interference and Diffraction
Quantum Physics
Wave-Particle Duality
Astronomy
Practical Skills and Data Analysis
Deformation of Solids
Thermal Physics
Uniform Circular Motion
Simple Harmonic Motion
The Nucleus and Radioactive Decay
Nuclear Energy, Fission and Fusion
Gravitational Fields
Electric Fields
Capacitors
Magnetic Fields
Charged Particles and Accelerators
Quantum Physics
Line spectra and the equation hf = ΔE
- 3 things to know
- Unit AS 2
Overview
Emission line spectrum and absorption line spectrum.
What you need to know
Answer each one before you reveal it.
An electron in hydrogen falls from the −3.4 eV level to the −13.6 eV level. Calculate the wavelength of the photon emitted.
An electron falls between two levels separated by 1.9 eV. Calculate the wavelength of the emitted photon and name the region of the spectrum.
Questions from this subtopic
Each one with the model answer underneath.
- 1
State the equation linking the frequency of an emitted photon to a change of energy level, defining each symbol.
Model answer
hf = ΔE, where h is the Planck constant in J s, f is the frequency of the emitted or absorbed photon in Hz and ΔE is the difference in energy between the two levels in joules.
- 2
Write the energy level transition equation in terms of the wavelength of the photon.
Model answer
hc/λ = ΔE, where h is the Planck constant, c is the speed of light in a vacuum, λ is the wavelength of the photon in metres and ΔE is the energy difference in joules.
- 3
What is an emission line spectrum?
Model answer
An emission line spectrum is a set of separate bright coloured lines on a dark background, each line corresponding to a photon emitted as an electron falls between two particular energy levels.
- 4
What is an absorption line spectrum?
Model answer
An absorption line spectrum is a continuous spectrum crossed by dark lines, formed when a cool gas absorbs from a continuous source exactly those photon energies that match its own energy level differences.
- 5
Why is the line spectrum of an element unique to that element?
Model answer
Every element has its own particular set of energy levels, so the set of possible differences between them, and therefore the set of photon energies emitted or absorbed, is different for each element.
- 6
An electron in hydrogen falls from the −3.4 eV level to the −13.6 eV level. Calculate the wavelength of the photon emitted.
Model answer
ΔE = 10.2 eV = 10.2 × 1.60 × 10⁻¹⁹ = 1.63 × 10⁻¹⁸ J, so λ = hc/ΔE = 1.989 × 10⁻²⁵ / 1.63 × 10⁻¹⁸ = 1.22 × 10⁻⁷ m, that is 122 nm, and hc ÷ 1.22 × 10⁻⁷ m returns 1.63 × 10⁻¹⁸ J.
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