HSC Resources Β· Physics Homework Notes
Lecture slides and notes for Ch06 Gravitation and Gravity from the Physics Homework Notes module in HSC Resources by Md Ahbab. 14 pages.

PHYSICS 1ST PAPER CHAPTER 6 Gravitation and Gravity Question 1 Look at the stimulus below. planet π π= 1.52 Γ 1025 kg satellite π= 7.5 Γ 1022 kg spaceship 4.5 Γ 108 m (a) State Newtonβs law of gravitation. (b) Will the velocities of two satellites of different masses in the same orbit be the same or different? Explain. (c) Determine the velocity of the satellite. (d) Give a mathematical judgement whether the resultant force on the spaceship would be zero or not at any place while it travels from the planet to the satellite. Solution (a) Every particle of the universe attracts every other particle. The force is proportional to the product of their masses. It is inversely proportional to the square of their distance. (b) The velocities will be the same. Let a satellite of mass πmove round a planet of mass π. The radius of its orbit is π. The gravitational force supplies the centripetal force. ππ£2 π = πΊππ π2 β π£= βοΈ πΊπ π The mass πof the satellite cancels. The velocity depends only on πand π. Hence two satellites in the same orbit have the same velocity. ahbab.dev 1
(c) Here, Mass of the planet π= 1.52 Γ 1025 kg Radius of the orbit π= 4.5 Γ 108 m Gravitational constant πΊ= 6.673 Γ 10β11 N m2 kgβ2 The velocity of the satellite in its orbit is π£= βοΈ πΊπ π = βοΈ 6.673 Γ 10β11 Γ 1.52 Γ 1025 4.5 Γ 108 m sβ1 = βοΈ 2.254 Γ 106 m sβ1 = 1501 m sβ1 π£= 1.5 km sβ1 (d) Let the spaceship have the mass π0 and the satellite the mass π. The planet and the satellite pull the spaceship in opposite directions. π π π0 πΉ1 πΉ2 π₯ πβπ₯ Let the resultant force be zero at a distance π₯from the planet. The two pulls are then equal. πΊππ0 π₯2 = πΊππ0 (πβπ₯)2 πβπ₯ π₯ = βοΈ π π= βοΈ 7.5 Γ 1022 1.52 Γ 1025 = 0.0702 π= 1.0702 π₯ π₯= 4.5 Γ 108 1.0702 m = 4.20 Γ 108 m The value of π₯is positive and less than π. Hence this point lies on the path of the spaceship. π₯= 4.2 Γ 108 m from the planet The resultant force on the spaceship is zero at this point only. Before this point the pull of the planet is greater. After it the pull of the satellite is greater. ahbab.dev 2
Question 2 The graph shows the variation of the gravitational force πΉof the moon on a body of mass 1000 kg with the distance πfrom the centre of the moon. 1.75 2.2 3.1 4.3 0.25 0.5 1.0 1.6 radius of the moon π(Γ106 m) πΉ(Γ103 N) Given, radius of the earth, π = 6.4 Γ 106 m, acceleration due to gravity of the earth, π= 9.8 m sβ2 and πΊ= 6.67 Γ 10β11 N m2 kgβ2. (a) What is called centre of gravity? (b) The acceleration due to gravity of an object falling from different heights does not remain uniform. Explain. (c) Determine the mass of the moon using the data of the stimulus. (d) Using the data of the stimulus compare the gravitational forces on the body at heights 2.55Γ106 m from the earthβs and the moonβs surfaces. Solution (a) The point where the whole weight of a body acts is called centre of gravity. (b) The acceleration due to gravity at a height βabove the earth is πβ= πΊπ (π + β)2 Here πand π are the mass and radius of the earth. The value of πβdepends on the height β. A falling body comes nearer to the earth, so βdecreases. The value of πβtherefore increases during the fall. Hence the acceleration does not remain uniform. (c) From the graph, the force at the surface of the moon is
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