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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 / Multiple Choice


6.2 Newton’s Law of Gravitation

Question 1

Marks: 1

The weight of a body on the surface of a planet orbiting a star is 80 N. The star has twice the density of the planet and its diameter is 500 times greater. 

What is the weight of the body on the surface of the star?  

  • 40 kN

  • 80 kN

  • 120 kN

  • 160 kN

Choose your answer
  

Question 2

Marks: 1

Let r0 represent the radius of Earth.

Which of the following shows the variation of the magnitude of the Earth's gravitational field strength g with radial distance r from its centre of mass, r = 0?

You may assume that mass is uniformly distributed beneath the Earth's surface. 

6-2-sl-mcq-hard-q2-phy

    Choose your answer
      

    Question 3

    Marks: 1

    At a point above a moon's surface and a distance xfrom its centre, the gravitational field strength is 5 N kg–1. At the moon's surface itself, the field strength is 9 N kg–1

    Which of the following gives the value for the radius of the planet? 

    • 5 x

    • 5 over 3 x

    • fraction numerator square root of 5 over denominator 3 end fraction x

    • square root of 5 over 3 end root x

    Choose your answer
      

    Question 4

    Marks: 1

    A binary system consisting of a star of mass M and 5M orbit each other at a distance r between their centre of mass. The resultant gravitational field strength is zero along the line between their centres at a distance x from the centre of the star of mass M. What is the value of the ratio r over x

    You may wish to use the quadratic formula: 

    p equals fraction numerator negative b plus-or-minus square root of b squared minus 4 a c end root over denominator 2 a end fraction

    For solutions to the equation:

    a p squared plus b p plus c equals 0

    • fraction numerator square root of 5 over denominator 5 end fraction

    • square root of 1 fifth end root

    • 1 minus square root of 5

    • 1 plus square root of 5

    Choose your answer
      

    Question 5

    Marks: 1

    Which single condition enables Newton's universal law of gravitation to be used to predict the force between two masses m1 and m2

    • m1 and m2 both have large radii

    • The radial distance between m1 and m2 is constant

    • m1 and m2 are very massive

    • m1 and m2 behave as point masses

    Choose your answer
      

    Question 6

    Marks: 1

    A planet of mass m and radius r rotates so rapidly that material at its equator only just remains on its surface. What is the period of its rotation? 

    • 2 pi square root of r over G end root

    • 2 pi square root of G over r end root

    • 2 pi square root of fraction numerator r over denominator G m end fraction end root

    • 2 pi square root of fraction numerator r cubed over denominator G m end fraction end root

    Choose your answer
      

    Question 7

    Marks: 1

    Two planetary systems, very far apart from each other, have suns with masses S1 and S2. They each have exoplanets P1 and P2 of mass m1 and m2 respectively, which are observed to have circular orbits of equal radii. If P1 completes an orbit in 1 thirdthe time taken by P2, which of the following may be deduced? 

    • S1S2 and m1 = 3m2

    • S1 = 3S2

    • S1 = 3S2 and m1 = m2

    • S1 = 9S2 only

    Choose your answer
      

    Question 8

    Marks: 1

    Two spherical bodies have the same radius, but one has thrice the mass of the other. At which point, A-D on the diagram below, could the resultant gravitational field of the two masses have the greatest magnitude? 

    6-2-sl-mcq-hard-q8-phy

      Choose your answer
        

      Question 9

      Marks: 1

      A mass m is placed at the centre of a thin, hollow, spherical shell of mass M and radius r

      6-2-sl-mcq-hard-q9-phy

      What is the magnitude of the resultant gravitational force on m and M

        Magnitude of resultant gravitational force on m Magnitude of resultant gravitational force on M
      A. 0 fraction numerator G M m over denominator r squared end fraction
      B. fraction numerator G M m over denominator r squared end fraction fraction numerator G M m over denominator r squared end fraction
      C. 0 0
      D. fraction numerator G M m over denominator r squared end fraction 0
        Choose your answer
          

        Question 10

        Marks: 1

        Two stationary bodies of mass m1 and m2 are a distance d apart. A third body, situated on the line joining m1 and m2, experiences no resultant gravitational force. Which of the following is a possible distance between the third body and m1

        • x equals fraction numerator square root of m subscript 1 end root over denominator square root of m subscript 1 end root minus square root of m subscript 2 end root end fraction

        • x equals d open parentheses fraction numerator square root of m subscript 1 end root over denominator square root of m subscript 1 end root minus square root of m subscript 2 end root end fraction close parentheses

        • x equals fraction numerator square root of m subscript 2 end root over denominator square root of m subscript 1 end root minus square root of m subscript 2 end root end fraction

        • x equals d open parentheses fraction numerator square root of m subscript 2 end root over denominator square root of m subscript 1 end root minus square root of m subscript 2 end root end fraction close parentheses

        Choose your answer