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Cosmology (A-level only)

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Question 3

The Triangulum Galaxy (M33) and the Andromeda Galaxy (M31) are members of the Local Group. The Triangulum Galaxy is currently moving towards Andromeda at a speed of 24 km s−124\text{ km s}^{-1}24 km s−1, and the distance between them is approximately 230 kpc230\text{ kpc}230 kpc.

a.

Discuss whether these data can be used to estimate an age for the Universe.

[2]
b.

There is a supermassive black hole at the centre of a nearby active galaxy. The mass of this black hole is 2.40×1092.40 \times 10^92.40×109 solar masses.

Calculate the radius of the event horizon of this black hole. State an appropriate unit for your answer. (Take 1 solar mass=1.99×1030 kg1\text{ solar mass} = 1.99 \times 10^{30}\text{ kg}1 solar mass=1.99×1030 kg, G=6.67×10−11 N m2 kg−2G = 6.67 \times 10^{-11}\text{ N m}^2\text{ kg}^{-2}G=6.67×10−11 N m2 kg−2, and c=3.00×108 m s−1c = 3.00 \times 10^8\text{ m s}^{-1}c=3.00×108 m s−1.)

[3]
c.

Over cosmic timescales, galactic collisions are predicted to trigger quasar activity. Explain what is meant by a quasar, and suggest how a galactic merger can produce a quasar. In your answer you should:

  • describe the typical properties of a quasar
  • explain how observations of quasars provide evidence for these properties
  • suggest the process of quasar formation/activation that is likely when two galaxies merge.
[6]

Cosmology (A-level only) Questions

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