Question bank

A-Level CAIE Physics 22 4 Energy Levels In Atoms And Line Spectra Question Bank

Practice A-Level CAIE Physics 22 4 Energy Levels In Atoms And Line Spectra questions by syllabus topic with past-paper context, marks, difficulty and question previews on Eduninja.

8 matching questions · Open interactive library

Question 7

7

9 marks

Question 7(a)

7(a)

The emission spectrum of atomic hydrogen consists of a number of discrete wavelengths. Explain how this observation leads to an understanding that there are discrete electron energy levels in atoms.

Mediumstructured2 marks

Answer

each wavelength is associated with a discrete change in energy M1 discrete energy change / difference implies discrete levels A1 [2]

Question 7(b)

7(b)

Some electron energy levels in atomic hydrogen are illustrated in Fig. 7.1. The longest wavelength produced as a result of electron transitions between two of the energy levels shown in Fig. 7.1 is \(4.0 \times 10^{-6} \mathrm{~m}\).

structured5 marks

Question 7(b)(i)

7(b)(i)

On Fig. 7.1, 1. draw, and mark with the letter L , the transition giving rise to the wavelength of \(4.0 \times 10^{-6} \mathrm{~m}\), 2. draw, and mark with the letter S , the transition giving rise to the shortest wavelength.

Mediumstructured2 marks

Answer

1. arrow from -0.54 eV to -0.85 eV , labelled \(\mathrm{L} \quad\) B1 [1] 2. arrow from -0.54 eV to -3.4 eV , labelled S B1 [1] (two correct arrows, but only one label - allow 2 marks) (two correct arrows, but no labels - allow 1 mark)

Question 7(b)(ii)

7(b)(ii)

Calculate the wavelength for the transition you have shown in (i) part 2. m

Mediumstructured3 marks

Answer

\(E=h c / \lambda\) C1 \((3.4-0.54) \times 1.6 \times 10^{-19}=\left(6.63 \times 10^{-34} \times 3.0 \times 10^{8}\right) / \lambda \quad\) C1 \(\lambda=4.35 \times 10^{-7} \mathrm{~m} \quad\) A1

Question 7(c)

7(c)

Photon energies in the visible spectrum vary between approximately 3.66 eV and 1.83 eV . Determine the energies, in eV, of photons in the visible spectrum that are produced by transitions between the energy levels shown in Fig. 7.1. photon energies eV

Mediumstructured2 marks

Answer

\(-1.50 \rightarrow-3.4=1.9 \mathrm{eV}\) \(-0.85 \rightarrow-3.4=2.55 \mathrm{eV}\) (allow 2.6 eV ) \(-0.54 \rightarrow-3.4=2.86 \mathrm{eV}\) (allow 2.9 eV ) 3 correct, 2 marks with -1 mark for each additional energy 2 correct, 1 mark but no marks if any additional energy differences B2

Question 8

8

White light is incident on a cloud of cool hydrogen gas, as illustrated in Fig. 8.1. The spectrum of the light emerging from the gas cloud is found to contain a number of dark lines.

structured4 marks

Question 8(a)

8(a)

Explain why these dark lines occur.

Mediumstructured3 marks

Answer

photon 'absorbed' by electron B1 photon has energy equal to difference in energy of two energy levels B1 electron de-excites emitting photon (of same energy) in any direction B1 [3]

Question 8(b)

8(b)

Some electron energy levels in a hydrogen atom are illustrated in Fig. 8.2. One dark line is observed at a wavelength of 435 nm .

structured1 marks

Question 8(b)(ii)

8(b)(ii)

On Fig. 8.2, draw an arrow to indicate the energy change that gives rise to this dark line.

Mediumstructured1 marks

Answer

arrow pointing in either direction between -3.41 eV and \(-0.55 \mathrm{eV} \quad\) B1 [1]

Question 8

8

2 marks

Question 8(b)

8(b)

An emission spectrum is seen as a series of differently coloured lines on a black background. Suggest how this observation provides evidence for discrete electron energy levels in atoms.

Mediumstructured2 marks

Answer

each (coloured) line corresponds to one wavelength/frequency energy = Planck constant × frequency implies specific energy change between energy levels B1 so discrete levels A0

Question 7

7

11 marks

Question 7(a)

7(a)

Explain how the line spectrum of hydrogen provides evidence for the existence of discrete electron energy levels in atoms.

Mediumstructured3 marks

Answer

each line represents photon of specific energy

Question 7(b)

7(b)

Some electron energy levels in atomic hydrogen are illustrated in Fig. 7.1. Two possible electron transitions A and B giving rise to an emission spectrum are shown. These electron transitions cause light of wavelengths 654 nm and 488 nm to be emitted.

structured4 marks

Question 7(b)(i)

7(b)(i)

On Fig. 7.1, draw an arrow to show a third possible transition.

Mediumstructured1 marks

Answer

arrow from -0.85 eV level to -1.5 eV level

Question 7(b)(ii)

7(b)(ii)

Calculate the wavelength of the emitted light for the transition in (i). wavelength = m

Mediumstructured3 marks

Answer

\(\Delta E=h c / \lambda\) photon emitted as a result of energy change of electron specific energy changes so discrete levels

Question 7(c)

7(c)

The light in a beam has a continuous spectrum of wavelengths from 400 nm to 700 nm . The light is incident on some cool hydrogen gas, as illustrated in Fig. 7.2. Using the values of wavelength in (b), state and explain the appearance of the spectrum of the emergent light.

Mediumstructured4 marks

Question 7

7

7 marks

Question 7(a)

7(a)

A beam of white light passes through a cloud of cool gas. The spectrum of the transmitted light is viewed and contains a number of dark lines. Explain why these dark lines occur.

Mediumstructured4 marks

Answer

photon absorbed (by electron) and electron excited B1 photon energy equal to difference in (energy of two) energy levels B1 photon energy relates to a single wavelength / single frequency B1 electron de-excites and emits photon in any direction B1

Question 7(b)

7(b)

Some energy levels for the electron in an isolated hydrogen atom are illustrated in Fig. 7.1. Table 7.1 shows the wavelengths of photons that are emitted in the transitions to n=2 from the other energy levels shown in Fig. 7.1. The energy associated with the energy level n=2 is -3.40 eV . Calculate the energy, in J , of energy level n=3. energy = ..... J

Mediumstructured3 marks

Answer

\(\frac{h c}{\lambda}=\Delta E\) C1 uses 658 nm C1 \[ \begin{aligned} \frac{6.63 \times 10^{-34} \times 3.00 \times 10^{8}}{658 \times 10^{-9}}=-\mathrm{E}_{1}-\left(-3.40 \times 1.60 \times 10^{-19}\right) E_{1}=-2.42 \times 10^{-19} \mathrm{~J} \end{aligned} \] A1

Question 8

8

Fig. 8.1 shows part of the emission spectrum of visible radiation emitted by hydrogen gas in a star in a distant galaxy. The galaxy is moving away from the Earth at a speed of \(6.2 \times 10^{6} \mathrm{~ms}^{-1}\) .

structured2 marks

Question 8(b)

8(b)

2 marks

Question 8(b)(ii)

8(b)(ii)

(ii)Determine the energy,in eV ,of the energy level from which the electron transition originates to cause the emission of this radiation. energy level= eV[2]

Mediumstructured2 marks

Answer

photon energy \(=\left(4.08 \times 10^{-19}\right) /\left(1.60 \times 10^{-19}\right)\) \[ =2.55 \mathrm{eV} \] C1 energy level =-3.40+2.55 \[ =-0.85 \mathrm{eV} \] A1

Question 8

8

Fig. 8.1 shows the lowest four energy levels of an electron in an isolated atom. Fig. 8.2 shows the lines in the emission spectrum of the atom that correspond to the transitions of the electron from n=3 to n=1 and from n=4 to n=1.

structured6 marks

Question 8(a)

8(a)

Explain, with reference to photons, why there is a single frequency of electromagnetic radiation that corresponds to each of these transitions.

Mediumstructured2 marks

Answer

transition (emits) (one) photon with energy equal to the difference in energy between the two levels B1 frequency of radiation corresponds to energy of photon B1

Question 8(b)

8(b)

4 marks

Question 8(b)(i)

8(b)(i)

On Fig. 8.2, draw a line that corresponds to the transition of the electron from n=2 to n=1. Label this line A.

Easystructured2 marks

Answer

line to the left of the pair in Fig. 8.2, labelled A B1 larger gap between line A and the nearest of the pair in Fig. 8.2 than between the lines in the pair B1

Question 8(b)(ii)

8(b)(ii)

On Fig. 8.2, draw a line that corresponds to the transition of the electron from n=3 to n=2. Label this line B.

Easystructured2 marks

Answer

line to the left of both the pair in Fig. 8.2 and line A, labelled B B1 larger gap between line B and line A than between line A and the nearest one of the pair in Fig. 8.2 B1

Question 8(c)

8(c)

The frequency of radiation represented by line A is \(f_{\mathrm{A}}\). The frequency of radiation represented by line B is \(f_{\mathrm{B}}\). The energy of the ground state (n=1) is \(E_{1}\). Determine an expression, in terms of \(f_{\mathrm{A}}, f_{\mathrm{B}}, E_{1}\) and the Planck constant h, for the energy \(E_{3}\) of the energy level n=3.

Hardstructured0 marks

Answer

E=h f C1 \(E_{3}=E_{1}+h\left(f_{\mathrm{A}}+f_{\mathrm{B}}\right)\) A1

Question 9

9

6 marks

Question 9(a)

9(a)

Fig. 9.1 shows the visible part of the emission spectrum from hydrogen gas in a laboratory on the Earth. The numbers indicate the wavelength, in nm , represented by each line.

structured6 marks

Question 9(a)(i)

9(a)(i)

Explain how the emission spectrum provides evidence for the existence of discrete energy levels for the electron in a hydrogen atom.

Mediumstructured3 marks

Answer

energy of photon has a corresponding frequency - change in electron energy level emits a single photon - photon energy = difference in energy levels - discrete frequencies must have come from discrete energy gaps - discrete energy changes imply discrete energy levels Any three points, 1 mark each B3

Question 9(a)(ii)

9(a)(ii)

Fig. 9.2 shows five of the energy levels in the hydrogen atom. The wavelengths of radiation shown in Fig. 9.1 relate to transitions to the -3.400 eV level in Fig. 9.2. Show that the energy level X is -1.51 eV .

Mediumstructured3 marks

Answer

transition (to -3.400 eV ) from X corresponds to 658 nm line C1 \(E_{1}-E_{2}=h c / \lambda\) C1 \[ E_{1}-(-3.400)=\left(6.63 \times 10^{-34} \times 3.00 \times 10^{8}\right) /\left(658 \times 10^{-9} \times 1.60 \times 10^{-19}\right) \] and so \(E_{1}=-1.51 \mathrm{eV}\) (full substitution and answer needed) A1