Top Banner
Circular Motion and Gravitation Section 1 Preview Section 1 Circular Motion Section 2 Newton’s Law of Universal Gravitation Section 3 Motion in Space Section 4 Torque and Simple Machines
69

Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Dec 27, 2015

Download

Documents

Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

Preview

Section 1 Circular Motion

Section 2 Newton’s Law of Universal Gravitation

Section 3 Motion in Space

Section 4 Torque and Simple Machines

Page 2: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

What do you think?

• Consider the following objects moving in circles:• A car traveling around a circular ramp on the highway• A ball tied to a string being swung in a circle • The moon as it travels around Earth• A child riding rapidly on a playground merry-go-round

• For each example above, answer the following:• Is the circular motion caused by a force?• If so, in what direction is that force acting? • What is the source of the force acting on each object?

Page 3: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Section 1Circular Motion and Gravitation

Tangential Speed (vt)

• Speed in a direction tangent to the circle

• Uniform circular motion: vt has a constant value– Only the direction changes– Example shown to the right

• How would the tangential speed of a horse near the center of a carousel compare to one near the edge? Why?

Page 4: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

Centripetal Acceleration (ac)

• Acceleration is a change in velocity (size or direction).

• Direction of velocity changes continuously for uniform circular motion.

• What direction is the acceleration?– the same direction as v– toward the center of the circle

• Centripetal means “center seeking”

Page 5: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

Centripetal Acceleration (magnitude)

• How do you think the magnitude of the acceleration depends on the speed?

• How do you think the magnitude of the acceleration depends on the radius of the circle?

Page 6: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

Tangential Acceleration

• Occurs if the speed increases• Directed tangent to the circle• Example: a car traveling in a circle

– Centripetal acceleration maintains the circular motion.• directed toward center of circle

– Tangential acceleration produces an increase or decrease in the speed of the car.

• directed tangent to the circle

Page 7: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

Click below to watch the Visual Concept.

Visual Concept

Centripetal Acceleration

Page 8: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Section 1Circular Motion and Gravitation

Centripetal Force (Fc)

c cF ma2

and tc

va

r

2

so tc

mvF

r

Page 9: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

Centripetal Force

• Maintains motion in a circle• Can be produced in different

ways, such as– Gravity– A string– Friction

• Which way will an object move if the centripetal force is removed?– In a straight line, as shown on

the right

Page 10: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

Describing a Rotating System

• Imagine yourself as a passenger in a car turning quickly to the left, and assume you are free to move without the constraint of a seat belt.– How does it “feel” to you during the turn? – How would you describe the forces acting on you during this

turn?

• There is not a force “away from the center” or “throwing you toward the door.”– Sometimes called “centrifugal force”

• Instead, your inertia causes you to continue in a straight line until the door, which is turning left, hits you.

Page 11: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

Classroom Practice Problems

• A 35.0 kg child travels in a circular path with a radius of 2.50 m as she spins around on a playground merry-go-round. She makes one complete revolution every 2.25 s.– What is her speed or tangential velocity? (Hint: Find

the circumference to get the distance traveled.)– What is her centripetal acceleration?– What centripetal force is required?

• Answers: 6.98 m/s, 19.5 m/s2, 682 N

Page 12: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 1

Now what do you think?

• Consider the following objects moving in circles:• A car traveling around a circular ramp on the highway• A ball tied to a string being swung in a circle • The moon as it travels around Earth• A child riding rapidly on a playground merry-go-round

• For each example above, answer the following:• Is the circular motion caused by a force?• If so, in what direction is that force acting? • What is the source of the force acting on each object?

Page 13: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

What do you think?

Imagine an object hanging from a spring scale. The scale measures the force acting on the object. • What is the source of this force? What is pulling or

pushing the object downward?• Could this force be diminished? If so, how?• Would the force change in any way if the object was

placed in a vacuum?• Would the force change in any way if Earth stopped

rotating?

Page 14: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Newton’s Thought Experiment• What happens if you fire a

cannonball horizontally at greater and greater speeds?

• Conclusion: If the speed is just right, the cannonball will go into orbit like the moon, because it falls at the same rate as Earth’s surface curves.

• Therefore, Earth’s gravitational pull extends to the moon.

Page 15: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Law of Universal Gravitation

• Fg is proportional to the product of the masses (m1m2).

• Fg is inversely proportional to the distance squared (r2).– Distance is measured center to center.

• G converts units on the right (kg2/m2) into force units (N).– G = 6.673 x 10-11 N•m2/kg2

Page 16: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Law of Universal Gravitation

Page 17: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Gravitational Force

• If gravity is universal and exists between all masses, why isn’t this force easily observed in everyday life? For example, why don’t we feel a force pulling us toward large buildings?– The value for G is so small that, unless at least one of

the masses is very large, the force of gravity is negligible.

Page 18: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Ocean Tides

• What causes the tides?• How often do they occur? • Why do they occur at certain times? • Are they at the same time each day?

Page 19: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Ocean Tides

• Newton’s law of universal gravitation is used to explain the tides. – Since the water directly below the moon is closer than

Earth as a whole, it accelerates more rapidly toward the moon than Earth, and the water rises.

– Similarly, Earth accelerates more rapidly toward the moon than the water on the far side. Earth moves away from the water, leaving a bulge there as well.

– As Earth rotates, each location on Earth passes through the two bulges each day.

– Link to web

Page 20: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Gravity is a Field Force

• Earth, or any other mass, creates a force field.

• Forces are caused by an interaction between the field and the mass of the object in the field.

• The gravitational field (g) points in the direction of the force, as shown.

Page 21: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Calculating the value of g

• Since g is the force acting on a 1 kg object, it has a value of 9.81 N/m (on Earth).– The same value as ag (9.81 m/s2)

• The value for g (on Earth) can be calculated as shown below.

2 2

g E EF Gmm Gm

gm mr r

Page 22: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Classroom Practice Problems

• Find the gravitational force that Earth

(mE = 5.97 1024 kg) exerts on the moon

(mm= 7.35 1022 kg) when the distance between them is 3.84 x 108 m.– Answer: 1.99 x 1020 N

• Find the strength of the gravitational field at a point 3.84 x 108 m from the center of Earth.– Answer: 0.00270 N/m or 0.00270 m/s2

Page 23: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 2

Now what do you think?

Imagine an object hanging from a spring scale. The scale measures the force acting on the object. – What is the source of this force? What is pulling or

pushing the object downward?– Could this force be diminished? If so, how?– Would the force change in any way if the object was

placed in a vacuum?– Would the force change in any way if Earth stopped

rotating?

Page 24: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 3

What do you think?

• Make a sketch showing the path of Earth as it orbits the sun.

• Describe the motion of Earth as it follows this path.

• Describe the similarities and differences between the path and motion of Earth and that of other planets.

Page 25: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 3

What do you think?

• What does the term weightless mean to you?• Have you ever observed someone in a

weightless environment? If so, when?• How did their weightless environment differ from a

normal environment?

Page 26: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 3

Weight and Weightlessness

• Bathroom scale– A scale measures the downward force exerted on it.– Readings change if someone pushes down or lifts up

on you.• Your scale reads the normal force acting on you.

Page 27: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 3

Apparent Weightlessness

• Elevator at rest: the scale reads the weight (600 N).• Elevator accelerates downward: the scale reads less.• Elevator in free fall: the scale reads zero because it no

longer needs to support the weight.

Page 28: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 3

Apparent Weightlessness

• You are falling at the same rate as your surroundings.– No support force from the floor is needed.

• Astronauts are in orbit, so they fall at the same rate as their capsule.

• True weightlessness only occurs at great distances from any masses.– Even then, there is a weak gravitational force.

Page 29: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 3

Now what do you think?

• Make a sketch showing the path of Earth as it orbits the sun.

• Describe the motion of Earth as it follows this path.

• Describe the similarities and differences between the path and motion of Earth and that of other planets.

Page 30: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 3

Now what do you think?

• What does the term weightless mean to you?• Have you ever observed someone in a

weightless environment? If so, when?• How did their weightless environment differ from a

normal environment?

Page 31: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Simple Machines

• Change the size or direction of the input force• Mechanical advantage (MA) compares the input

force to the output force.– When Fout > Fin then MA > 1

• MA can also be determined from the distances the input and output forces move.

MA FoutFin

dindout

Page 32: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Click below to watch the Visual Concept.

Visual Concept

Overview of Simple Machines

Page 33: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Simple Machines• Simple machines alter the force

and the distance moved.• For the inclined plane shown:

– F2 < F1 so MA >1 and d2 > d1

• If the ramp is frictionless, the work is the same in both cases.– F1d1 = F2d2

• With friction, F2d2 > F1d1.– The force is reduced but the work

done is greater.

Page 34: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Efficiency of Simple Machines

• Efficiency measures work output compared to work input.– In the absence of friction, they are equal.

• Real machines always have efficiencies less than 1, but they make work easier by changing the force required to do the work.

eff Wout

Win

Page 35: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Preview

• Multiple Choice

• Short Response

• Extended Response

Page 36: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice1. An object moves in a circle at a constant speed.

Which of the following is not true of the object?

A. Its acceleration is constant.

B. Its tangential speed is constant.

C. Its velocity is constant.

D. A centripetal force acts on the object.

Page 37: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice1. An object moves in a circle at a constant speed.

Which of the following is not true of the object?

A. Its acceleration is constant.

B. Its tangential speed is constant.

C. Its velocity is constant.

D. A centripetal force acts on the object.

Page 38: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Use the passage below to answer questions 2–3.

A car traveling at 15 m/s on a flat surface turns in a circle with a radius of 25 m.

2. What is the centripetal acceleration of the car?

F. 2.4 10-2 m/s2

G. 0.60 m/s2

H. 9.0 m/s2

J. zero

Multiple Choice, continued

Page 39: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continuedUse the passage below to answer questions 2–3.

A car traveling at 15 m/s on a flat surface turns in a circle with a radius of 25 m.

2. What is the centripetal acceleration of the car?

F. 2.4 10-2 m/s2

G. 0.60 m/s2

H. 9.0 m/s2

J. zero

Page 40: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continuedUse the passage below to answer questions 2–3.

A car traveling at 15 m/s on a flat surface turns in a circle with a radius of 25 m.

3. What is the most direct cause of the car’s centripetal acceleration?

A. the torque on the steering wheel

B. the torque on the tires of the car

C. the force of friction between the tires and the road

D. the normal force between the tires and the road

Page 41: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continuedUse the passage below to answer questions 2–3.

A car traveling at 15 m/s on a flat surface turns in a circle with a radius of 25 m.

3. What is the most direct cause of the car’s centripetal acceleration?

A. the torque on the steering wheel

B. the torque on the tires of the car

C. the force of friction between the tires and the road

D. the normal force between the tires and the road

Page 42: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued4. Earth (m = 5.97 1024 kg) orbits the sun (m =

1.99 1030 kg) at a mean distance of 1.50 1011 m. What is the gravitational force of the sun on Earth? (G = 6.673 10-11 N•m2/kg2)

F. 5.29 1032 N

G. 3.52 1022 N

H. 5.90 10–2 N

J. 1.77 10–8 N

Page 43: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued4. Earth (m = 5.97 1024 kg) orbits the sun (m =

1.99 1030 kg) at a mean distance of 1.50 1011 m. What is the gravitational force of the sun on Earth? (G = 6.673 10-11 N•m2/kg2)

F. 5.29 1032 N

G. 3.52 1022 N

H. 5.90 10–2 N

J. 1.77 10–8 N

Page 44: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued

5. Which of the following is a correct interpretation of

the expression ?

A. Gravitational field strength changes with an object’s distance from Earth.

B. Free-fall acceleration changes with an object’s distance from Earth.

C. Free-fall acceleration is independent of the falling object’s mass.

D. All of the above are correct interpretations.

ag g GmEr2

Page 45: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued

5. Which of the following is a correct interpretation of

the expression ?

A. Gravitational field strength changes with an object’s distance from Earth.

B. Free-fall acceleration changes with an object’s distance from Earth.

C. Free-fall acceleration is independent of the falling object’s mass.

D. All of the above are correct interpretations.

ag g GmEr2

Page 46: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued6. What data do you need to calculate the orbital

speed of a satellite?

F. mass of satellite, mass of planet, radius of orbit

G. mass of satellite, radius of planet, area of orbit

H. mass of satellite and radius of orbit only

J. mass of planet and radius of orbit only

Page 47: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued6. What data do you need to calculate the orbital

speed of a satellite?

F. mass of satellite, mass of planet, radius of orbit

G. mass of satellite, radius of planet, area of orbit

H. mass of satellite and radius of orbit only

J. mass of planet and radius of orbit only

Page 48: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued7. Which of the following choices correctly describes

the orbital relationship between Earth and the sun?

A. The sun orbits Earth in a perfect circle.

B. Earth orbits the sun in a perfect circle.

C. The sun orbits Earth in an ellipse, with Earth

at one focus.

D. Earth orbits the sun in an ellipse, with the sun

at one focus.

Page 49: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued7. Which of the following choices correctly describes

the orbital relationship between Earth and the sun?

A. The sun orbits Earth in a perfect circle.

B. Earth orbits the sun in a perfect circle.

C. The sun orbits Earth in an ellipse, with Earth

at one focus.

D. Earth orbits the sun in an ellipse, with the sun

at one focus.

Page 50: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued

Use the diagram to answer

questions 8–9.8. The three forces acting onthe wheel have equal magnitudes. Which force willproduce the greatest torque on the wheel?

F. F1

G. F2

H. F3

J. Each force will produce the same torque.

Page 51: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued

Use the diagram to answer

questions 8–9.8. The three forces acting onthe wheel have equal magnitudes. Which force willproduce the greatest torque on the wheel?

F. F1

G. F2

H. F3

J. Each force will produce the same torque.

Page 52: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued

Use the diagram to answer

questions 8–9.9. If each force is 6.0 N, the angle between F1 and F2 is 60.0°, and the radius of the wheel is 1.0 m, what is theresultant torque on the wheel?

A. –18 N•m C. 9.0 N•m

B. –9.0 N•m D. 18 N•m

Page 53: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued

Use the diagram to answer

questions 8–9.9. If each force is 6.0 N, the angle between F1 and F2 is 60.0°, and the radius of the wheel is 1.0 m, what is theresultant torque on the wheel?

A. –18 N•m C. 9.0 N•m

B. –9.0 N•m D. 18 N•m

Page 54: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued10. A force of 75 N is applied to a lever. This force

lifts a load weighing 225 N. What is the mechanical advantage of the lever?

F. 1/3

G. 3

H. 150

J. 300

Page 55: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued10. A force of 75 N is applied to a lever. This force

lifts a load weighing 225 N. What is the mechanical advantage of the lever?

F. 1/3

G. 3

H. 150

J. 300

Page 56: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued11. A pulley system has an efficiency of 87.5

percent. How much work must you do to lift a desk weighing 1320 N to a height of 1.50 m?

A. 1510 J

B. 1730 J

C. 1980 J

D. 2260 J

Page 57: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued11. A pulley system has an efficiency of 87.5

percent. How much work must you do to lift a desk weighing 1320 N to a height of 1.50 m?

A. 1510 J

B. 1730 J

C. 1980 J

D. 2260 J

Page 58: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued12. Which of the following statements is correct?

F. Mass and weight both vary with location.

G. Mass varies with location, but weight does not.

H. Weight varies with location, but mass does

not.

J. Neither mass nor weight varies with location.

Page 59: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued12. Which of the following statements is correct?

F. Mass and weight both vary with location.

G. Mass varies with location, but weight does not.

H. Weight varies with location, but mass does

not.

J. Neither mass nor weight varies with location.

Page 60: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued13. Which astronomer discovered that planets

travel in elliptical rather than circular orbits?

A. Johannes Kepler

B. Nicolaus Copernicus

C. Tycho Brahe

D. Claudius Ptolemy

Page 61: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Multiple Choice, continued13. Which astronomer discovered that planets

travel in elliptical rather than circular orbits?

A. Johannes Kepler

B. Nicolaus Copernicus

C. Tycho Brahe

D. Claudius Ptolemy

Page 62: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Short Response14. Explain how it is possible for all the water to

remain in a pail that is whirled in a vertical path, as shown below.

Page 63: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Short Response14. Explain how it is possible for all the water to

remain in a pail that is whirled in a vertical path, as shown below.

Answer: The water remains in the pail even when the pail is upside down because the water tends to move in a straight path due to inertia.

Page 64: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Short Response, continued15. Explain why approximately two high tides take

place every day at a given location on Earth.

Page 65: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Short Response, continued15. Explain why approximately two high tides take

place every day at a given location on Earth.

Answer: The moon’s tidal forces create two bulges on Earth. As Earth rotates on its axis once per day, any given point on Earth passes through both bulges.

Page 66: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Short Response, continued16. If you used a machine to increase the output

force, what factor would have to be sacrificed? Give an example.

Page 67: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Short Response, continued16. If you used a machine to increase the output

force, what factor would have to be sacrificed? Give an example.

Answer: You would have to apply the input force over a greater distance. Examples may include any machines that increase output force at the expense of input distance.

Page 68: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Extended Response

17. Mars orbits the sun (m = 1.99 1030 kg) at a mean distance of 2.28 1011 m. Calculate the length of

the Martian year in Earth days. Show all of your work. (G = 6.673 10–11 N•m2/kg2)

Page 69: Circular Motion and GravitationSection 1 Preview Section 1 Circular MotionCircular Motion Section 2 Newton’s Law of Universal GravitationNewton’s Law of.

Circular Motion and Gravitation Section 4

Extended Response

17. Mars orbits the sun (m = 1.99 1030 kg) at a mean distance of 2.28 1011 m. Calculate the length of

the Martian year in Earth days. Show all of your work. (G = 6.673 10–11 N•m2/kg2)

Answer: 687 days