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DP IB Physics: SL

Topic Questions

Home / IB / Physics: SL / DP / Topic Questions / 6. Circular Motion & Gravitation / 6.2 Newton’s Law of Gravitation / Structured Questions


6.2 Newton’s Law of Gravitation

Question 1a

Marks: 2

The distance from the Earth to the Sun is 1.5 × 1011 m. The mass of the Earth is 6 × 1024 kg and the mass of the Sun is 3.3 × 105  times the mass of the Earth.

(a)
Estimate the gravitational force between the Sun and the Earth.
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    Question 1b

    Marks: 3

    Mars is 1.5 times further away from the Sun than the Earth and is 10 times lighter than Earth.

    (b)
    Predict the gravitational force between Mars and the Sun.
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      Question 1c

      Marks: 2
      (c)
      Determine the acceleration of free fall on a planet 20 times as massive as the Earth and with a radius 10 times larger.
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        Question 1d

        Marks: 3
        (d)
        Calculate the orbital speed of the Earth around the Sun.
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          Key Concepts
          Circular Orbits

          Question 2a

          Marks: 4

          A satellite orbits the Earth with mass M above the equator with a period, T equal to 48 hours. The mass of the Earth is 5.972 × 1024 kg. 

          (a)
          Derive an equation for the radius, r of the satellite’s orbit.
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            Key Concepts
            Circular Orbits

            Question 2b

            Marks: 3

            The mean radius of Earth is 6.37 × 106 m.

            (b)
            Calculate the height of the satellite above the Earth’s surface.
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              Key Concepts
              Circular Orbits

              Question 2c

              Marks: 3

              The Hubble Space Telescope is in orbit around the Earth at a height of 490 km above the Earth’s surface.

              (c)
              Calculate Hubble’s speed.
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                Key Concepts
                Circular Orbits

                Question 2d

                Marks: 2
                (d)
                Calculate the magnitude of the gravitational field on the Hubble Space Telescope at this height above the Earth’s surface.
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                  Question 3a

                  Marks: 3

                  Europa, a moon of Jupiter, has an orbital period of 85 hours and an orbital radius of  670 900 km.

                  (a)
                  Outline why Europa moves with uniform circular motion.
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                    Key Concepts
                    Circular Orbits

                    Question 3b

                    Marks: 3
                    (b)
                    Show that the orbital speed of Europa is 14 km s–1.
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                      Question 3c

                      Marks: 3
                      (c)
                      Deduce the mass of Jupiter.
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                        Question 3d

                        Marks: 3

                        Ganymede is the largest of Jupiter’s Moons. It has an orbital period of 7.15 days and an orbital speed of 10.880 km s–1.

                        (d)
                        Calculate the orbital radius of Ganymede in terms of billions of km.
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                          Key Concepts
                          Circular Orbits

                          Question 4a

                          Marks: 2
                          (a)
                          Define Newton’s universal law of gravitation.
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                            Question 4b

                            Marks: 2

                            The diagram shows a satellite orbiting the Earth. The satellite is part of the network of global–positioning satellites (GPS) that transmit radio signals used to locate the position of receivers that are located on the Earth. 

                                                                        q4b_newtons-law-of-gravitation_ib-sl-physics-sq-medium

                            When the satellite is directly overhead the microwave signal reaches the receiver 62 ms after leaving the satellite. 

                            (b)
                            Calculate the height of the satellite above the surface of the Earth.
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                              Key Concepts
                              Circular Orbits

                              Question 4c

                              Marks: 2
                              (c)
                              Explain why the satellite is accelerating towards the centre of the Earth even though its orbital speed is constant.
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                                Key Concepts
                                Circular Orbits

                                Question 4d

                                Marks: 2

                                The radius of Earth is 6.4 × 106 m.

                                (d)
                                Calculate the gravitational field strength of the Earth at the position of the satellite.

                                                      Mass of Earth = 6.0 × 1024 kg

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                                  Question 5a

                                  Marks: 2

                                  A satellite is in a circular orbit around a planet of mass M.

                                                                      q5a_newtons-law-of-gravitation_ib-sl-physics-sq-medium

                                  (a)
                                  Sketch arrows to represent the velocity and acceleration of the satellite.
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                                    Key Concepts
                                    Circular Orbits

                                    Question 5b

                                    Marks: 2
                                    (b)
                                    Show that the angular speed, ω is related to the orbital radius r by 

                                                                                     

                                             r =cube root of fraction numerator G M over denominator omega squared end fraction end root

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                                      Question 5c

                                      Marks: 2

                                      Because of friction with the upper atmosphere, the satellite slowly moves into another circular orbit with a smaller radius before.

                                      (c)
                                      Suggest the effect of this on the satellites angular speed. 
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                                        Key Concepts
                                        Circular Orbits

                                        Question 5d

                                        Marks: 3

                                        Titus and Enceladus are two of Saturn’s moons. Data about these moons are given in the table.

                                        Moon Orbit radius / m Angular speed / rad s-1
                                        Titan 1.22 cross times109  
                                        Enceladus 2.38 cross times 108 5.31 cross times10-5

                                        (d)
                                        Determine the mass of Saturn.
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                                          Key Concepts
                                          Circular Orbits