Question 17N.3.SL.TZ0.12
Date | November 2017 | Marks available | [Maximum mark: 9] | Reference code | 17N.3.SL.TZ0.12 |
Level | SL | Paper | 3 | Time zone | TZ0 |
Command term | Determine, Draw, Identify, Show, Show that, Sketch, State | Question number | 12 | Adapted from | N/A |
Sirius is a binary star. It is composed of two stars, Sirius A and Sirius B. Sirius A is a main sequence star.
State what is meant by a binary star.
[1]
two stars orbiting a common centre «of mass»
Do not accept “stars which orbit each other”

The peak spectral line of Sirius B has a measured wavelength of 115 nm. Show that the surface temperature of Sirius B is about 25 000 K.
[1]
« x T = 2.9 x 10–3»
T = = 25217 «K»

The mass of Sirius B is about the same mass as the Sun. The luminosity of Sirius B is 2.5 % of the luminosity of the Sun. Show, with a calculation, that Sirius B is not a main sequence star.
[2]
use of the mass-luminosity relationship or = 1
if Sirius B is on the main sequence then = 1 «which it is not»
Conclusion is given, justification must be stated
Allow reverse argument beginning with luminosity

The Sun’s surface temperature is about 5800 K.
Determine the radius of Sirius B in terms of the radius of the Sun.
[2]
= 0.025
r Sirius = « =» 0.0085 r Sun

Identify the star type of Sirius B.
[1]
white dwarf

The image shows a Hertzsprung–Russell (HR) diagram.
The mass of Sirius A is twice the mass of the Sun. Using the Hertzsprung–Russell (HR) diagram,
draw the approximate positions of Sirius A, labelled A and Sirius B, labelled B.
[1]
Sirius A on the main sequence above and to the left of the Sun AND Sirius B on white dwarf area as shown
Both positions must be labelled
Allow the position anywhere within the limits shown.
sketch the expected evolutionary path for Sirius A.
[1]
arrow goes up and right and then loops to white dwarf area