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-Gravitational Field -Gravitational Potential Energy AP Physics C Mrs. Coyle.

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Presentation on theme: "-Gravitational Field -Gravitational Potential Energy AP Physics C Mrs. Coyle."— Presentation transcript:

1 -Gravitational Field -Gravitational Potential Energy AP Physics C Mrs. Coyle

2 Remember: Remember: Newton’s Law of Universal Gravitation -Universal Gravitation Constant G=6.67x 10 - 11 Nm 2 /kg 2 -The gravitational force is a field force.

3 Review Question Review Question: Which exerts a greater force, the earth on the moon or the moon on the earth?

4 Gravitational Field: t Gravitational Field: the space around a mass. Here a test mass would feel a gravitational force. Gravitational Field Vector: Gravitational Field Vector:

5 Gravitational Field Vector, g at the surface of the Earth

6 g above the Earth’s surface r = R E + hNote: g decreases with increasing altitude As r , the weight of the object approaches zero

7 Variation of g with Height from the surface of the Earth

8 Remember The gravitational force is conservative The gravitational force is a central force (A central force has a direction towards the center and its magnitude depends only on r) A central force can be represented by

9 Work done by the Gravitational Force A particle moves from A to B while acted on by a central force F We approximate the path along A to B with radial and arc zigzags The work done by F along the arcs is zero The work done by F along the radial direction is

10 Work done by the Gravitational Force The work done is independent of the path and depends only on r f and r i This proves that the gravitational force is conservative.

11 Gravitational Potential Energy As a particle moves from A to B, its gravitational potential energy changes by:

12 Gravitational Potential Energy of the Earth-particle system The reference point is chosen at infinity where the force on a particle would approach zero. U i = 0 for r i = ∞ This is valid only for r > = R E and not valid for r < R E U is negative because of the choice of U i

13 Gravitational Potential Energy of the Earth- particle system

14 Gravitational Potential Energy of any two particles

15 Gravitational Potential Energy of a system of any two particles U = -Gm 1 m 2 r The reference point U=0 is at infinity.

16 Gravitational Potential Energy

17 An outside force must do positive work to increase the separation between two objects This work gives the objects a greater potential energy (less negative).

18 Binding Energy The absolute value of the potential energy is the binding energy An outside force must supply energy gretaer or equal to the binding energy to separate the particles to an infinite distance of separation. The excess energy will be in the form of kinetic energy of the particles when they are at infinite separation.

19 Systems with Three or More Particles (Configuration of Masses) The total gravitational potential energy of the system is the sum over all pairs of particles Gravitational potential energy obeys the superposition principle

20 Systems with Three Particles The absolute value of U total represents the work needed to separate the particles by an infinite distance. Remember energy is a scalar quantity.

21 Configurations of Masses Gravitational Forces are added using the vector component method. To find the Gravitational Potential Energy of the configuration of masses, the individual energies are added as scalars. A force would have to supply an amount of energy equal to the individual energy in order to separate the masses by an infinite distance.

22 Ex #31 A system consists of three particles, each of mass 5.00g, located at the corners of an equilateral triangle with sides of 30.0cm. a)Calculate the potential energy of the system. b)If the particles are released simultaneously, where will they collide? Ans: a) -1.67x10 -14 J


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