Cosmology (AQA A Level Physics)

Exam Questions

32 mins6 questions
1
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3 marks

A star is orbiting the black hole in M87. The star is observed in the plane of its orbit.

The wavelength of a spectral line observed in the light emitted from the star varies between a maximum and a minimum value.

  • maximum value observed = 374.96 nm

  • minimum value observed = 373.53 nm

Calculate the orbital speed of the star.

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2
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2 marks

Astronomers recently used the radial velocity method to discover an exoplanet orbiting HD 66141.

Describe the main features of the radial velocity method in the detection of planets.

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3a
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3 marks

Figure 2 shows, for some galaxies, how their recession speed v varies with distance d from the Earth.

Figure 2

A scatter plot showing velocity in km/s on the vertical axis and distance in Mpc on the horizontal axis, with data points clustered upward.

Estimate, using Figure 2, the age in seconds of the Universe.

3b
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2 marks

The estimate in part (a) assumes that the Universe has expanded at a constant rate.

Measurements involving type 1a supernovae that are at large distances from Earth caused astronomers to make a modification to this assumption.

State:

  • the modification

  • the explanation that was proposed to account for this modification.

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4a
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2 marks

U Cephei is an eclipsing binary system consisting of two stars that orbit their common centre of mass.

The primary star is class B; the secondary star is class G.

Figure 1 shows the variation of apparent magnitude of U Cephei with time as observed from Earth.

Figure 1

Graph showing apparent magnitude over 6 days on a grid. It features three periodic drops from magnitude 7 to 9, suggesting an eclipsing binary star.

Explain the shape of the graph in Figure 1.

4b
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1 mark

A particular spectral line has a wavelength of 486.136 nm when measured from a source in the laboratory.

This line is also present in the absorption spectrum of the primary star of U Cephei.

When observed from Earth, the wavelength of the primary star’s absorption line varies as shown in Table 1.

Table 1

Wavelength / nm

maximum value

486.498

minimum value

485.672

State why the average of the values in Table 1 is different from the laboratory value.

4c
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3 marks

Show that the orbital speed of the primary star is about 250 km s−1.

4d
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2 marks

Calculate the orbital radius of the primary star.

4e
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1 mark

Which absorption lines would be most prominent in the spectrum of the primary star?

  • hydrogen

  • hydrogen and helium

  • ionised metals

  • neutral metals

4f
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2 marks

A different eclipsing binary star system is thought to consist of a white dwarf star and a neutron star.

Discuss how astronomers could confirm this.

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5a
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2 marks

IC2497 is a galaxy that contained a quasar. It is believed that the quasar stopped emitting radiation several thousand years ago.

Suggest why the quasar stopped emitting radiation.

5b
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4 marks

IC2497 has a red shift of 0.0516

Determine the distance from the Earth to IC2497.

Give an appropriate unit for your answer.

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6a
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3 marks

Table 3 contains information about two galaxies.

Table 3

Galaxy

Red shift, z

Distance from Earth / ly

NGC 936

4.8 × 10–3

6.8 × 107

NGC 3379

3.0 × 10–3

3.2 × 107

Discuss whether these data are consistent with Hubble’s Law.

6b
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2 marks

Quasars are the most distant measurable objects.

Discuss one problem associated with the determination of the distance from the Earth to a quasar.

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