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Question 20N.3.SL.TZ0.17

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Date November 2020 Marks available [Maximum mark: 11] Reference code 20N.3.SL.TZ0.17
Level SL Paper 3 Time zone TZ0
Command term Estimate, Explain, Show, Suggest Question number 17 Adapted from N/A
17.
[Maximum mark: 11]
20N.3.SL.TZ0.17

The data for the star Eta Aquilae A are given in the table.

L is the luminosity of the Sun and M is the mass of the Sun.

(a)

Show by calculation that Eta Aquilae A is not on the main sequence.

[2]

Markscheme

«LL=M3.5M3.5=5.703.5=»442 

the luminosity of Eta (2630L) is very different «so it is not main sequence»

 

Allow calculation of L13.5 to give M=9.5M so not main sequence

OWTTE

(b(i))

Estimate, in pc, the distance to Eta Aquilae A using the parallax angle in the table.

[1]

Markscheme

d«=12.36×10-3»=424«pc» ✓

(b(ii))

Estimate, in pc, the distance to Eta Aquilae A using the luminosity in the table, given that L=3.83×1026W.

[3]

Markscheme

Use of d=L4πb ✓

=2630×3.83×10264π×7.20×10-10 ✓

«=1.055×10193.26×9.46×1015»=342«pc» ✓

 

Award [3] marks for a bald correct answer between 340 and 344«pc»

 

 

(c)

Suggest why your answers to (b)(i) and (b)(ii) are different.

[2]

Markscheme

parallax angle in milliarc seconds/very small/at the limits of measurement

uncertainties/error in measuring L οr b or θ

values same order of magnitude, so not significantly different

 

Accept answers where MP1 and MP2 both refer to parallax angle

OWTTE

(d)

Eta Aquilae A is a Cepheid variable. Explain why the brightness of Eta Aquilae A varies.

[3]

Markscheme

reference to change in size
reference to change in temperature
reference to periodicity of the process
reference to transparency / opaqueness