Question 20N.3.SL.TZ0.17
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 |
The data for the star Eta Aquilae A are given in the table.
is the luminosity of the Sun and is the mass of the Sun.
Show by calculation that Eta Aquilae A is not on the main sequence.
[2]
✓
the luminosity of Eta (2630) is very different «so it is not main sequence» ✓
Allow calculation of to give so not main sequence
OWTTE

Estimate, in , the distance to Eta Aquilae A using the parallax angle in the table.
[1]
✓

Estimate, in , the distance to Eta Aquilae A using the luminosity in the table, given that .
[3]
Use of ✓
✓
✓
Award [3] marks for a bald correct answer between and

Suggest why your answers to (b)(i) and (b)(ii) are different.
[2]
parallax angle in milliarc seconds/very small/at the limits of measurement ✓
uncertainties/error in measuring οr or ✓
values same order of magnitude, so not significantly different ✓
Accept answers where MP1 and MP2 both refer to parallax angle
OWTTE

Eta Aquilae A is a Cepheid variable. Explain why the brightness of Eta Aquilae A varies.
[3]
reference to change in size ✓
reference to change in temperature ✓
reference to periodicity of the process ✓
reference to transparency / opaqueness ✓
