Question 21N.2.SL.TZ0.6
Date | November 2021 | Marks available | [Maximum mark: 9] | Reference code | 21N.2.SL.TZ0.6 |
Level | SL | Paper | 2 | Time zone | TZ0 |
Command term | Estimate, Explain, Show that | Question number | 6 | Adapted from | N/A |
Titan is a moon of Saturn. The Titan-Sun distance is 9.3 times greater than the Earth-Sun distance.
Show that the intensity of the solar radiation at the location of Titan is 16 W m−2
[1]
incident intensity OR «W m−2» ✓
Allow the use of 1400 for the solar constant.

Titan has an atmosphere of nitrogen. The albedo of the atmosphere is 0.22. The surface of Titan may be assumed to be a black body. Explain why the average intensity of solar radiation absorbed by the whole surface of Titan is 3.1 W m−2
[3]
exposed surface is ¼ of the total surface ✓
absorbed intensity = (1−0.22) × incident intensity ✓
0.78 × 0.25 × 15.7 OR 3.07 «W m−2» ✓
Allow 3.06 from rounding and 3.12 if they use 16 W m−2.

Show that the equilibrium surface temperature of Titan is about 90 K.
[1]
σT 4 = 3.07
OR
T = 86 «K» ✓

The orbital radius of Titan around Saturn is and the period of revolution is .
Show that where is the mass of Saturn.
[2]
correct equating of gravitational force / acceleration to centripetal force / acceleration ✓
correct rearrangement to reach the expression given ✓
Allow use of for MP1.

The orbital radius of Titan around Saturn is 1.2 × 109 m and the orbital period is 15.9 days. Estimate the mass of Saturn.
[2]
«s» ✓
«kg» ✓
Award [2] marks for a bald correct answer.
Allow ECF from MP1.
