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Date November 2016 Marks available 2 Reference code 16N.3.HL.TZ0.25
Level Higher level Paper Paper 3 Time zone Time zone 0
Command term Calculate Question number 25 Adapted from N/A

Question

The graph shows the observed orbital velocities of stars in a galaxy against their distance from the centre of the galaxy. The core of the galaxy has a radius of 4.0 kpc.

Calculate the rotation velocity of stars 4.0 kpc from the centre of the galaxy. The average density of the galaxy is 5.0 × 10–21 kg m–3.

[2]
a.

Explain why the rotation curves are evidence for the existence of dark matter.

[2]
b.

Markscheme

v = «\(\sqrt {\frac{{4\pi G\rho }}{3}} r\)» \( = \sqrt {\frac{4}{3} \times \pi  \times 6.67 \times {{10}^{ - 11}} \times 5.0 \times {{10}^{ - 21}}}  \times \left( {4000 \times 3.1 \times {{10}^{16}}} \right)\)

v is about 146000 «m s–1» or 146 «km s–1»
Accept answer in the range of 140000 to 160000 «m s–1».

a.

rotation curves/velocity of stars were expected to decrease outside core of galaxy

flat curve suggests existence of matter/mass that cannot be seen – now called dark matter

b.

Examiners report

[N/A]
a.
[N/A]
b.

Syllabus sections

Option D: Astrophysics » Option D: Astrophysics (Additional higher level option topics) » D.5 – Further cosmology (HL only)
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