Module 03: Motion and Gravitation Flashcards

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1
Q

Lesson 3.1: Uniform Circular Motion

What is uniform circular motion?

A

An object that moves in a circle at a constant speed (v)

  1. Magnitude of the velocity remains constant
  2. Direction of the velocity continuously changes as it goes around a circle
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2
Q

Lesson 3.1: Uniform Circular Motion

Describe acceleration in a uniform circular motion:

A

Constantly accelerating:

  • Defined as the rate of change of velocity, a change in direction of velocity is an acceleration, just like a change in magnitude.
  • Constantly accelerating even when speed is constant
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3
Q

Lesson 3.1: Uniform Circular Motion

How do you calculate acceleration in Uniform Circular Motion (when t != 0)?

A
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4
Q

Lesson 3.1: Uniform Circular Motion

What is Centripetal (Radial) Acceleration?

A

🔬 Centripetal (Radial) Acceleration: (aR)Directed along the radius, towards the centre of the circle

When ∆t is very small (approaching zero):

  1. ∆l and ∆Θ are also very small
  2. v2 will be almost parallel to v1 & ∆v will be essentially perpendicular to them (towards the centre of the circle)
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5
Q

Lesson 3.1: Uniform Circular Motion

How do you calculate the magnitude of radial acceleration?

A
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6
Q

Lesson 3.1: Uniform Circular Motion

What is the formula to determine radial acceleration?

A
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7
Q

Lesson 3.1: Uniform Circular Motion

How does velocity change depending on speed and radius?

A

(1) Greater the speed (v) - the faster the velocity changes direction
(2) Larger the radius - the less rapidly the velocity changes direction

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8
Q

Lesson 3.1: Uniform Circular Motion

Describe the acceleration and velocity vectors of uniform circular motion:

A
  1. Acceleration vector points towards the center of the circle (v is constant)
  2. Velocity vector points in the direction of motion (Tangential to the circle)

Perpendicular to each other

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9
Q

Lesson 3.1: Uniform Circular Motion

What are frequencies and periods in a circular motion and how does it relate to speed?

A

Circular motion described in terms of …

  1. Frequency (f): number of revolutions per second
  2. Period (T): time required to complete one revolution

Relationship: T = 1/f

Speed travels a distance 2πr in one revolution:

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10
Q

Lesson 3.1: Uniform Circular Motion

What is centripetal force and how is it calculated?

A

(According to Newton’s Second Law [ΣF = ma]) a net force is necessary to give it centripetal acceleration

Calculate the magnitude needed where ΣFR = maR and where aR = v2/r:

ΣFR=maR=m(v2/r)

Net force directed towards the centre of the circle - called centripetal force

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11
Q

Lesson 3.1: Uniform Circular Motion

What are the problem-solving steps to solve uniform circular motion questions?

A

1. Draw a FBD: show all forces (tension in a cord, gravity from Earth, normal force, friction) but not something that doesn’t belong (like centrifugal force)

  1. Determine which forces act to provide the centripetal acceleration. The component that acts radially, towards or away from the centre of the circular path.
    Sum of these forces provides the centripetal acceleration: aR = v2/r
  2. Choose a convenient coordinate system
  3. Apply Newton’s second law to the radial component: ΣFR=maR=m(v2/r)
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12
Q

Lesson 3.1: Uniform Circular Motion

Describe what happens when a car traveled around a curve?

A
  • Feels like you are thrust outwards towards the right side door
  • You move in a straight line, whereas the car moves in a curved path
  • To make you go in the curved path, the seat (friction) and door of the car (direct contact) exert force on you
  • The car also has a force exerted on it towards the centre of the curve if it is to move that curve
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13
Q

Lesson 3.1: Uniform Circular Motion

What friction applies when a car is breaking?

A
  • Wheels travel without slipping or sliding, the bottom of the tires rest against the road The friction force the road exerts is static
  • If static friction is less than mv2/r and the car skid out of control = friction force becomes kinetic friction (smaller than static friction)
  • Worse when the wheels lock: (when rolling, static friction exists) tires slide and friction force (kinetic) is less
  • The direction also changes:
    Static friction can point perpendicular to the velocity
    The force no longer points towards the centre of the circle, and car continues in a curved path
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14
Q

Lesson 3.1: Uniform Circular Motion

How do banked curves help reduce the chance of skidding?

A
  • Normal force exerted by a banked road (perpendicular to the road) will have a component towards the centre of the circle - reducing friction
  • Given banking angle Θ, one speed for which no friction at all is required
  • When the horizontal component of the normal force towards the centre of the curve, FNsinΘ = to the force required to give the vehicle its centripetal acceleration:

FNsinΘ = mv2/r

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15
Q

Lesson 3.2: Law of Universal Gravitation

Describe the centripetal acceleration of the moon due to the Earth’s gravity:

A
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16
Q

Lesson 3.2: Law of Universal Gravitation

How is the gravitational force related to the distance from Earth’s centre?

A
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17
Q

Lesson 3.2: Law of Universal Gravitation

How does gravity relate to distance and the mass of an object?

A
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18
Q

Lesson 3.2: Law of Universal Gravitation

What is the Law of Universal Gravitation?

A

🔬 Law of Universal Gravitation: Every particle in the universe attracts every other particle with a force that is proportional to the product of their masses and inversely proportional to the square of the distance between them.

Magnitude of Gravitational Force:

  • m1 and m2 are masses, r is the distance, and G is the universal constant (measured experimentally)
  • G = 6.67 * 10-11 N*m2/kg2
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19
Q

Lesson 3.2: Law of Universal Gravitation

How can you determine the Force of Gravity on an Object on the Earth’s Surface?

A
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20
Q

How are satellites put into orbit?

A
  • Put into orbit by accelerating it to a sufficiently high tangential speed
    • If its too high, it will escape
    • If its too low, it will return to earth
  • Put into circular motion - because it requires the least takeoff speed
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21
Q

How are satellites kept in space by their high speed?

A

Satellite in orbit is falling (accelerating) towards Earth, but its high tangential speed keeps it from hitting Earth

Needed acceleration = v2/r

Newton’s law of universal gravitation: (Apply Newton’s second law ΣFR = maR in the radial direction)

  • Height: r = rE + h
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22
Q

How does apparent weightlessness occur in an elevator?

A

If the elevator is in freefall

then a = -g and w=mg-mg=0

The bag appears to be weightless

Called = APPARENT WEIGHTLESSNESS

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23
Q

What is Kepler’s First Law?

A

The path of each planet around the Sun is an ellipse with the Sun at one focus

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24
Q

What is Kepler’s Second Law?

A

Each planet moves so that an imaginary line drawn from the Sun to the planet sweeps out equal areas in equal periods of time

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25
Q

What is Kepler’s Third Law?

A

The ratio of squares of the period T of any two planets revolving around the Sun

  • The mean distance equals the semimajor axis s]
  • T1 and T2 are the periods, and s1 and s2 represent their mean distances from the Sun:
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26
Q

Lesson 3.1 Questions

1. (I) A child sitting 1.20 m from the center of a merry-go-round moves with a speed of 1.10 m/s. Calculate (a) the centripetal acceleration of the child and (b) the net horizontal force exerted on the child (mass = 22.5 kg).

A
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27
Q

Lesson 3.1 Questions

3. (I) A horizontal force of 310 N is exerted on a 2.0-kg ball as it rotates (at arm’s length) uniformly in a horizontal circle of radius 0.90 m. Calculate the speed of the ball.

A
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28
Q

Lesson 3.1 Questions

5. (II) A 0.55-kg ball, attached to the end of a horizontal cord, is revolved in a circle of radius 1.3 m on a frictionless horizontal surface. If the cord will break when the tension in it exceeds 75 N, what is the maximum speed the ball can have?

A
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29
Q

Lesson 3.1 Questions

7. (II) A car drives straight down toward the bottom of a valley and up the other side on a road whose bottom has a radius of curvature of 115 m. At the very bottom, the normal force on the driver is twice his weight. At what speed was the car traveling?

A
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30
Q

Lesson 3.1 Questions

11. (II) How many revolutions per minute would a 25-m-diameter Ferris wheel need to make for the passengers to feel “weightless” at the topmost point?

A
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31
Q

Lesson 3.1 Questions

13. (II) A proposed space station consists of a circular tube that will rotate about its center (like a tubular bicycle tire), Fig. 5–39. The circle formed by the tube has a diameter of 1.1 km. What must be the rotation speed (revolutions per day) if an effect nearly equal to gravity at the surface of the Earth (say, 0.90 g) is to be felt?

A
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32
Q

Lesson 3.1 Questions

17. (II) Two blocks, with masses mA and mB, are connected to each other and to a central post by thin rods as shown in Fig. 5–41. The blocks revolve about the post at the same frequency f (revolutions per second) on a frictionless horizontal surface at distances rA and rB from the post. Derive an algebraic expression for the tension in each rod.

A
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33
Q

Lesson 3.2 Questions

29. (I) At the surface of a certain planet, the gravitational acceleration g has a magnitude of 12.0 m/s2. A 24.0-kg brass ball is transported to this planet. What is (a) the mass of the brass ball on the Earth and on the planet, and (b) the weight of the brass ball on the Earth and on the planet?

A
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34
Q

Lesson 3.2 Questions

33. (II) Calculate the acceleration due to gravity on the Moon, which has radius 1.74 × 106 m and mass 7.35 × 1022 kg.

A
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35
Q

Lesson 3.2 Questions

35. (II) Given that the acceleration of gravity at the surface of Mars is 0.38 of what it is on Earth, and that Mars’ radius is 3400 km, determine the mass of Mars.

A
36
Q

Lesson 3.2 Questions

37. (II) A hypothetical planet has a mass 2.80 times that of Earth, but has the same radius. What is g near its surface?

A
37
Q

Lesson 3.2 Questions

39. (II) Calculate the effective value of g, the acceleration of gravity, at (a) 6400 m, and (b) 6400 km, above the Earth’s surface.

A
38
Q

Lesson 3.3 Questions

45. (I) A space shuttle releases a satellite into a circular orbit 780 km above the Earth. How fast must the shuttle be moving (relative to Earth’s center) when the release occurs?

A
39
Q

Lesson 3.3 Questions

47. (II) You know your mass is 62 kg, but when you stand on a bathroom scale in an elevator, it says your mass is 77 kg. What is the acceleration of the elevator, and in which direction?

A
40
Q

Lesson 3.3 Questions

49. (II) Calculate the period of a satellite orbiting the Moon, 95 km above the Moon’s surface. Ignore effects of the Earth. The radius of the Moon is 1740 km.

A
41
Q

Lesson 3.3 Questions

51. (II) What will a spring scale read for the weight of a 58.0-kg woman in an elevator that moves (a) upward with constant speed 5.0 m/s, (b) downward with constant speed 5.0 m/s, (c) with an upward acceleration 0.23 g, (d) with a downward acceleration 0.23 g, and (e) in free fall?

A
42
Q

Lesson 3.3 Questions

57. (I) Neptune is an average distance of 4.5 × 109 km from the Sun. Estimate the length of the Neptunian year using the fact that the Earth is 1.50 × 108 km from the Sun on average.

A
43
Q

Lesson 3.3 Questions

59. (I) Use Kepler’s laws and the period of the Moon (27.4 d) to determine the period of an artificial satellite orbiting very near the Earth’s surface.

A
44
Q

Lesson 3.3 Questions

61. (II) Our Sun revolves about the center of our Galaxy (mG » 4 × 1041 kg) at a distance of about 3 × 104 light-years [1 ly = (3.00 × 108 m/s) • (3.16 × 107 s/yr) • (1.00 yr)]. What is the period of the Sun’s orbital motion about the center of the Galaxy?

A
45
Q

Lesson 3.3 Questions

65. (II) Halley’s comet orbits the Sun roughly once every 76 years. It comes very close to the surface of the Sun on its closest approach (Fig. 5–45). Estimate the greatest distance of the comet from the Sun. Is it still “in” the solar system? What planet’s orbit is nearest when it is out there?

A
46
Q

Lab Experiment: Centripetal Acceleration

Define uniform circular motion:

A

Uniform Circular Motion: Object travels in a circular path at a constant speed, while their direction of velocity changes

47
Q

Lab Experiment: Centripetal Acceleration

What is centripetal acceleration?

A

Centripetal Acceleration: change in velocity - always points towards the center of the circular path traveled by the object.

48
Q

Lab Experiment: Centripetal Acceleration

What is the rotational axis?

A

Rotational Axis: Center point of the circular path, perpendicular to the plane of rotation

49
Q

Lab Experiment: Centripetal Acceleration

What is tangential velocity?

A
50
Q

Lab Experiment: Centripetal Acceleration

What is centripetal force?

A

Experienced by an object in uniform circular motion:

Fc = mac = mv2 / r

51
Q

Lab Experiment: Centripetal Acceleration

How do you determine the speed for centripetal force?

A
  • Angular Displacement: Angle, Θ, measured in radians, related to the degrees by the following conversion:

1 rev = 2π radians

  • Arc Length (s): distance traced out in a circular path after creating a subtended angle, Θ.

s = Θr

  • Circumference: (C) C = Θ1 revr = 2πr
  • Speed determined using the circumference and the period:

v= displacement / time= 2πr / T = C / T

52
Q

Lab Experiment: Centripetal Acceleration

What is tension?

A

Tension: is a force transmitted through a string that allows a force to act over a distance

Tension = Fg = mg = Fc

53
Q

Determine the force providing the centripetal force for: a car making a turn

A

static friction between the car tire and the road

54
Q

Determine the force providing the centripetal force for child swinging around a pole.

A

the pulling force of the child’s arms

55
Q

Determine the force providing the centripetal force for a person sitting on a bench facing the center of a carousel

A

the normal force of the bench and the person’s back and/or the friction force of the bench seat and the person’s bottom

56
Q

Determine the force providing the centripetal force for a rock swinging on a string

A

d. the tension of the string

57
Q

Determine the force providing the centripetal force for the Earth Orbiting the Sun:

A

the gravitational force of the Sun on the Earth

58
Q

A car goes around a circular curve on a horizontal road at constant speed. What is the direction of the friction force on the car due to the road?

  1. tangent to the curve opposite to the direction of the car’s motion
  2. perpendicular to the curve inward
  3. perpendicular to the curve outward
  4. tangent to the curve in the forward direction
  5. There is no friction on the car because its speed is constant.
A
  1. perpendicular to the curve inward
59
Q

Module 03 Exam

When an object moves in uniform circular motion, the direction of its acceleration is

  1. in the same direction as its velocity vector.
  2. in the opposite direction of its velocity vector.
  3. is directed away from the center of its circular path.
  4. depends on the speed of the object.
  5. is directed toward the center of its circular path.
A
  1. is directed toward the center of its circular path
60
Q

Module 03 Exam

Two small objects, with masses m and M, are originally a distance r apart, and the magnitude of the gravitational force on each one is F. The masses are changed to 2m and 2M, and the distance is changed to 4r. What is the magnitude of the new gravitational force?

A

F/4

61
Q

Module 03 Exam

A spaceship is traveling to the Moon. At what point is it beyond the pull of Earth’s gravity?

  1. when it is half-way there
  2. when it gets above the atmosphere
  3. It is never beyond the pull of Earth’s gravity.
  4. when it is closer to the Moon than it is to Earth
A
  1. It is never beyond the pull of Earth’s gravity
62
Q

Module 03 Exam

Planet A has twice the mass of Planet B. From this information, what can we conclude about the acceleration due to gravity at the surface of Planet A compared to that at the surface of Planet B?

  1. The acceleration due to gravity on Planet A must be twice as great as the acceleration due to gravity on Planet B.
  2. The acceleration due to gravity on Planet A is the same as the acceleration due to gravity on Planet B.
  3. The acceleration due to gravity on Planet A must be four times as great as the acceleration due to gravity on Planet B.
  4. The acceleration due to gravity on Planet A is greater than the acceleration due to gravity on Planet B, but we cannot say how much greater.
  5. We cannot conclude anything about the acceleration due to gravity on Planet A without knowing the radii of the two planets.
A
  1. We cannot conclude anything about the acceleration due to gravity on Planet A without knowing the radii of the two planets
63
Q

Module 03 Exam

Halley’s Comet is in a highly elliptical orbit around the sun. Therefore the orbital speed of Halley’s Comet, while traveling around the sun,

  1. is constant.
  2. decreases as it nears the Sun.
  3. increases as it nears the Sun.
  4. is zero at two points in the orbit.
A
  1. increases as it nears the Sun
64
Q

Module 03 Exam

The curved section of a horizontal highway is a circular unbanked arc of radius 740 m. If the coefficient of static friction between this roadway and typical tires is 0.40, what would be the maximum safe driving speed for this horizontal curved section of highway?

A

54 m/s

65
Q

Module 03 Exam

A jet plane flying 600 m/s experiences an acceleration of 4.0 g when pulling out of a circular dive. What is the radius of curvature of the circular part of the path in which the plane is flying?

A

9200 m

66
Q

Module 03 Exam

One way that future space stations may create artificial gravity is by rotating the station. Consider a cylindrical space station 380 m in diameter that is rotating about its longitudinal axis. Astronauts walk on the inside surface of the space station. How long will it take for each rotation of the cylinder if it is to provide “normal” gravity for the astronauts?

A

28 s

67
Q

Module 03 Exam

A 2.0-kg ball is moving with a constant speed of 5.0 m/s in a horizontal circle whose diameter is 1.0 m. What is the magnitude of the net force on the ball?

A

100 N

68
Q

Module 03 Exam

A small 175-g ball on the end of a light string is revolving uniformly on a frictionless surface in a horizontal circle of diameter 1.0 m. The ball makes 2.0 revolutions every 1.0 s.

  • *(a)** What are the magnitude and direction of the acceleration of the ball?
  • *(b)** Find the tension in the string.
A
69
Q

Module 03 Exam

A future use of space stations may be to provide hospitals for severely burned persons. It is very painful for a badly burned person on Earth to lie in bed. In a space station, the effect of gravity can be reduced or even eliminated. How long should each rotation take for a doughnut-shaped hospital of 200-m radius so that persons on the outer perimeter would experience 1/10 the normal gravity of Earth?

A

1.5 min

70
Q

Module 03 Exam

A curved portion of highway has a radius of curvature of 65 m. As a highway engineer, you want to bank this curve at the proper angle for a steady speed of 22 m/s.

(a) What banking angle should you specify for this curve?
(b) At the proper banking angle, what normal force and what friction force does the highway exert on a 750-kg car going around the curve at the proper speed?

A

Since the curved portion of the highway is at the proper banking angle, there will be no force of friction if the car goes around the path.

71
Q

Module 03 Exam

What is the magnitude of the gravitational force that two small 7.00-kg balls exert on each other when they are 35.0 cm apart? (G = 6.67 × 10-11 N ∙ m2/kg2)

A
72
Q

Module 03 Exam

Two identical tiny balls of highly compressed matter are 1.50 m apart. When released in an orbiting space station, they accelerate toward each other at 2.00 cm/s2. What is the mass of each of them? (G = 6.67 × 10-11 N ∙ m2/kg2)

A
73
Q

Module 03 Exam

As a 70-kg person stands at the seashore gazing at the tides (which are caused by the Moon), how large is the gravitational force on that person due to the Moon? The mass of the Moon is 7.35 × 1022 kg, the distance to the Moon is 3.82 × 108 m, and G = 6.67 × 10-11 N ∙ m2/kg2.

A

0.0024 N

74
Q

Module 03 Exam

A very dense 1500-kg point mass (A) and a dense 1200-kg point mass (B) are held in place 1.00 m apart on a frictionless table. A third point mass is placed between the other two at a point that is 20.0 cm from B along the line connecting A and B. When the third mass is suddenly released, find the magnitude and direction (toward A or toward B) of its initial acceleration. (G = 6.67 × 10-11 N ∙ m2/kg2)

A
75
Q

Module 03 Exam

The mass of the Moon is 7.4 × 1022 kg, its radius is 1.74 × 103 km, and it has no atmosphere. What is the acceleration due to gravity at the surface of the Moon? (G = 6.67 × 10-11 N ∙ m2/kg2)

A

1.6 m/s2

76
Q

Module 03 Exam

The mass of Pluto is 1.31 × 1022 kg and its radius is 1.15 × 106 m. What is the acceleration of a freely-falling object at the surface of Pluto if it has no atmosphere? (G = 6.67 × 10-11 N ∙ m2/kg2)

A

0.661 m/s2

77
Q

Module 03 Exam

The earth has radius R. A satellite of mass 100 kg is in orbit at an altitude of 3R above the earth’s surface. What is the satellite’s weight at the altitude of its orbit?

A

61 N

78
Q

Module 03 Exam

A spherically symmetric planet has four times the earth’s mass and twice its radius. If a jar of peanut butter weighs 12 N on the surface of the Earth, how much would it weigh on the surface of this planet?

A

12 N

79
Q

Module 03 Exam

A 2.10-kg hammer is transported to the Moon. The radius of the Moon is 1.74 × 106 m, its mass is 7.35 × 1022 kg, and G = 6.67 × 10-11 N ∙ m2/kg2. How much does the hammer weigh on Earth and on the Moon?

A
80
Q

Module 03 Exam

The captain of a spaceship orbiting planet X discovers that to remain in orbit at from the planet’s center, she needs to maintain a speed of 68m/s What is the mass of planet X? (G = 6.67 × 10-11 N ∙ m2/kg2)

A

2.8 × 1019 kg

81
Q

Module 03 Exam

You are the science officer on a visit to a distant solar system. Prior to landing on a planet you measure its diameter to be 1.8 × 107 m. You have previously determined that the planet orbits 2.9 × 1011 m from its star with a period of 402 earth days. Once on the surface you find that the acceleration due to gravity is 19.5 m/s2. What are the masses of (a) the planet and (b) the star? (G = 6.67 × 10-11 N ∙ m2/kg2)

A

(a) 2.4 kg × 1025 kg,
(b) 1.2 kg × 1031 kg

82
Q

Module 03 Exam

In another solar system, a planet has a moon that is 4.0 × 105 m in diameter. Measurements reveal that this moon takes 3.0 x 105 s to make each orbit of diameter 1.8 × 108 m. What is the mass of the planet? (G = 6.67 × 10-11 N ∙ m2/kg2)

A

4.8 × 1024 kg

83
Q

Module 03 Exam

The International Space Station is orbiting at an altitude of about 370 km above the earth’s surface. The mass of the earth is 5.97 × 1024 kg, the radius of the earth is 6.38 × 106 m, and G = 6.67 × 10-11 N ∙ m2/kg2. Assume a circular orbit.

(a) What is the period of the International Space Station’s orbit?
(b) What is the speed of the International Space Station in its orbit?

A
84
Q

Module 03 Exam

A satellite of mass 500 kg orbits the earth with a period of 6,000 s. The earth has a mass of 5.97 × 1024 kg, a radius of 6.38 × 106 m, and G = 6.67 × 10-11 N ∙ m2/kg2.

(a) Calculate the magnitude of the earth’s gravitational force on the satellite.
(b) Determine the altitude of the satellite above the earth’s surface.

A
85
Q

Module 03 Exam

A large telescope of mass 8410 kg is in a circular orbit around the earth, making one revolution every 927 minutes. What is the magnitude of the gravitational force exerted on the satellite by the earth? (G = 6.67 × 10-11 N ∙ m2/kg2, Mearth = 6.0 × 1024 kg)

A
86
Q

Module 03 Exam

The innermost satellite of Jupiter orbits the planet with a radius of 422 × 103 km and a period of 1.77 days. What is the mass of Jupiter? (G = 6.67 × 10-11 N ∙ m2/kg2)

A

1.89 × 1027 kg

87
Q

Module 03 Exam

It takes the planet Jupiter 12 years to orbit the sun once in a nearly circular orbit. Assuming that Jupiter’s orbit is truly circular, what is the distance from Jupiter to the sun, given that the distance from the earth to the sun is 1.5 × 1011 m?

A

7.9 × 1011 m