DP Physics (first assessment 2025)

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Question SPM.2.HL.TZ0.4

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Date May Specimen-2023 Marks available [Maximum mark: 7] Reference code SPM.2.HL.TZ0.4
Level HL Paper 2 Time zone TZ0
Command term Determine, Draw, Outline, Show that Question number 4 Adapted from N/A
4.
[Maximum mark: 7]
SPM.2.HL.TZ0.4

A satellite moves around Earth in a circular orbit.

 

(a)

Draw an arrow on the diagram to represent the direction of the acceleration of the satellite.

[1]

Markscheme

arrow normal to the orbit towards the Earth ✓

(b)

The following data are given:

                                Mass of Earth, M = 5.97 × 1024 kg
                              Radius of Earth, R = 6.37 × 106 m
           Orbital period of the satellite, T = 5.62 × 103 s

(b.i)

Kepler’s Third Law of orbital motion states that T2=kr3 where k is a constant and r is the orbital radius of the satellite.

Show that k=4π2GM.

[1]

Markscheme

use of vorbital=2πrT AND either vorbital=GMr or mvorbital2r=GMmr2 correctly manipulated ✓

«to yield T2=4π2GMr3»

Allow use of ω.

(b.ii)

Determine the height of the satellite above the Earth’s surface.

[2]

Markscheme

r=GMT24π23=6.67×10-11×5.97×1024×562024π23 ✓

=6.83×106 «m»

height = «6.83×106-6.37×106=» 4.6×105 «m» ✓

(c)

The atmosphere exerts a small viscous drag force on the satellite.

Outline how the total energy, kinetic energy, and gravitational potential energy change for the satellite during one orbit around Earth.

[3]

Markscheme

Total energy is reduced ✓

hence decrease in orbital radius leads to increase in kinetic energy ✓

decrease in potential energy must be larger than increase in kinetic energy for total energy to decrease ✓

Allow ECF from b ii.