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Table 1 shows telemetry data for four newly deployed artificial satellites orbiting Mars.

SatelliteMean distance from Mars' centre (km\text{km}km)Time taken for one orbit (hours\text{hours}hours)
Satellite Alpha6 0006\,00060004.54.54.5
Satellite Beta12 00012\,0001200012.712.712.7
Satellite Gamma18 00018\,0001800023.423.423.4
Satellite Delta24 00024\,0002400036.036.036.0
a.

Describe the relationship between the satellite's mean distance from Mars' centre and the time taken for one orbit.

[1]
b.

Calculate the orbital speed of Satellite Beta in km/h\text{km/h}km/h. Use the equation: orbital speed=2π×mean distancetime taken for one orbit\text{orbital speed} = \frac{2\pi \times \text{mean distance}}{\text{time taken for one orbit}}orbital speed=time taken for one orbit2π×mean distance​ Give your answer to 3 significant figures.

[3]

Solar system; stability of orbital motions; satellites (physics only) Questions

Practise AQA GCSE Physics Solar system; stability of orbital motions; satellites (physics only) with exam-style questions for Foundation and Higher tier. 27 questions covering Our solar system, The life cycle of a star, and Orbital motion, natural and artificial satellites, matched to the AQA GCSE Physics (8463) specification and written in Paper 1 and Paper 2 style. Every question includes a full worked solution and mark scheme, so you can see where marks are awarded rather than just whether you got the answer right.

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Solar system; stability of orbital motions; satellites (physics only) Questions

  1. GCSE
  2. /Physics
  3. /Solar system; stability of orbital motions; satellites (physics only)