1. © 2012 Pearson Education, Inc. Conceptual Physical Science 5 th Edition Chapter 4: GRAVITY, PROJECTILES, AND SATELLITES © 2012 Pearson Education, Inc.

2. This lecture will help you understand: The Universal Law of Gravity The Inverse-Square Law: Gravity and Distance Weight and Weightlessness Universal Gravitation Projectile Motion Fast-Moving Projectiles—Satellites Circular Satellite Orbits Elliptical Orbits Escape Speed

3. © 2012 Pearson Education, Inc. The Legend of the Falling Apple Newton was not the first to discover gravity. Newton discovered that gravity is universal. Legend—Newton, sitting under an apple tree, realized that the force between Earth and the apple is the same as that between moons and planets and everything else.

4. © 2012 Pearson Education, Inc. The Fact of the Falling Moon In ancient times, it was believed that stars, planets, and the Moon moved in divine circles, free from forces of Earth. Newton recognized that some force must be acting on the planets, otherwise their paths would be straight lines. Newton also realized that any force on a planet would be directed toward a fixed, central point – the sun. Newtonian Synthesis – the union of terrestrial and cosmic laws.

5. © 2012 Pearson Education, Inc. The Fact of the Falling Moon We now know that the Moon falls around Earth in the sense that it falls beneath the straight line it would follow if no force acted on it. The Moon maintains a tangential velocity, which ensures a nearly circular motion around and around Earth rather than into it. This path is similar to the paths of planets around the Sun.

6. © 2012 Pearson Education, Inc. Newton’s most celebrated synthesis is of A.earthly and heavenly laws. B.weight on Earth and weightlessness in outer space. C.masses and distances. D.the paths of tossed rocks and the paths of satellites. The Universal Law of Gravity CHECK YOUR NEIGHBOR

7. © 2012 Pearson Education, Inc. A.earthly and heavenly laws. B.weight on Earth and weightlessness in outer space. C.masses and distances. D.the paths of tossed rocks and the paths of satellites. Comment: This synthesis provided hope that other natural phenomena followed universal laws, and ushered in the Age of Enlightenment. Newton’s most celebrated synthesis is of The Universal Law of Gravity CHECK YOUR ANSWER

8. © 2012 Pearson Education, Inc. The Universal Law of Gravity Newton’s Law of Universal Gravitation Every body in the universe attracts every other body with a mutually attracting force. For two bodies, this force is directly proportional to the product of their masses and inversely proportional to the square of the distance separating them, F = G m 1  m 2 d 2d 2

9. © 2012 Pearson Education, Inc. Newton’s Law of Universal Gravity The greater m 1 and m 2  the greater the force of attraction between them. The greater the distance of separation d, the weaker is the force of attraction—weaker as the inverse square of the distance between their centers. F = G m 1  m 2 d 2d 2

10. © 2012 Pearson Education, Inc. Inverse-square law: relates the intensity of an effect to the inverse square of the distance from the cause The greater the distance from Earth, the less the gravitational force on an object. No matter how great the distance, gravity approaches, but never reaches, zero. The Inverse-Square Law : Gravity and Distance

11. © 2012 Pearson Education, Inc. The Inverse-Square Law: Gravity and Distance The inverse square law holds for gravity and for all phenomena in which the effect from a localized source spreads uniformly throughout the surrounding space We only sense gravitation when large masses are involved. The force of attraction between you and the earth is your weight. Your weight depends on both your mass and your distance from the center of the earth. A child that weighs 300N at sea level, weighs only 299N on Mount Everest – and much less the further away from earth he gets - but he will never weigh zero. Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison Wesley

12. © 2012 Pearson Education, Inc. Inverse-Square Law

13. © 2012 Pearson Education, Inc. Inverse-Square Law

14. © 2012 Pearson Education, Inc. The force of gravity between two planets depends on their The Inverse-Square Law: Gravity and Distance CHECK YOUR NEIGHBOR A.masses and distance apart. B.planetary atmospheres. C.rotational motions. D.All of the above.

15. © 2012 Pearson Education, Inc. The force of gravity between two planets depends on their A.masses and distance apart. B.planetary atmospheres. C.rotational motions. D.All of the above. Explanation: The equation for gravitational force, cites only masses and distances as variables. Rotation and atmospheres are irrelevant. The Inverse-Square Law: Gravity and Distance CHECK YOUR ANSWER F = G m 1  m 2 d 2d 2

16. © 2012 Pearson Education, Inc. A.doubles. B.quadruples. C.reduces by half. D.reduces by one quarter. If the masses of two planets are each somehow doubled, the force of gravity between them The Inverse-Square Law: Gravity and Distance CHECK YOUR NEIGHBOR

17. © 2012 Pearson Education, Inc. A.doubles. B.quadruples. C.reduces by half. D.reduces by one quarter. Explanation: Note that both masses double, so double  double = quadruple. If the masses of two planets are each somehow doubled, the force of gravity between them The Inverse-Square Law: Gravity and Distance CHECK YOUR ANSWER

18. © 2012 Pearson Education, Inc. A.double. B.quadruple C.reduce by half. D.reduce by one quarter. If the mass of one planet is somehow doubled, the force of gravity between it and a neighboring planet would The Universal Law of Gravity CHECK YOUR NEIGHBOR

19. © 2012 Pearson Education, Inc. A.double. B.quadruple. C.reduce by half. D.reduce by one quarter. Explanation: Let the equation guide your thinking: Note that if one mass doubles, the force between them doubles. If the mass of one planet is somehow doubled, the force of gravity between it and a neighboring planet would The Universal Law of Gravity CHECK YOUR ANSWER F = G m 1  m 2 d 2d 2

20. © 2012 Pearson Education, Inc. The Universal Gravitational Constant, G G is the proportionality constant in Newton’s law of gravitation. G has the same magnitude as the gravitational force between two 1-kg masses that are 1 meter apart: 6.67  10 –11 N. So G = 6.67  10 –11 N  m 2 /kg 2. F = 6.67  10 –11 N  m 2 /kg 2 (m 1  m 2 )/d 2

21. © 2012 Pearson Education, Inc. The Universal Gravitational Constant, G Once the value of G was known, the mass of earth could be calculated: F = G (m 1 x m 2 / d 2 ) M1 (the mass of the earth) was determined to be: 6 x 10 24 kg

22. © 2012 Pearson Education, Inc. A. . B.g. C.acceleration due to gravity. D.speed of uniform motion. The universal gravitational constant, G, which links force to mass and distance, is similar to the familiar constant The Universal Gravitational Constant, G CHECK YOUR NEIGHBOR

23. © 2012 Pearson Education, Inc. A. . B.g. C.acceleration due to gravity. D.speed of uniform motion. Explanation: Just as  relates the circumference of a circle to its diameter, G relates force to mass and distance. The universal gravitational constant, G, which links force to mass and distance, is similar to the familiar constant The Universal Gravitational Constant, G CHECK YOUR ANSWER

24. © 2012 Pearson Education, Inc. Weight is the force exerted against a supporting floor or weighing scale. Weightlessness is a condition wherein a support force is lacking—free fall, for example. Weight and Weightlessness

25. © 2012 Pearson Education, Inc. Weight and Weightlessness Example of weightlessness: No support force. An astronaut is weightless because he or she is not supported by anything. The body responds as if gravity forces were absent, and this gives the sensation of weightlessness.

26. © 2012 Pearson Education, Inc. Weight and Weightlessness When you step on a scale, you are compressing a spring inside the scale Once the elastic force of the deformed spring balances the gravitational attraction between the earth and you, the pointer stops at your weight If you stand on a scale in an accelerating elevator you will find variations in your weight: –Elevator accelerates upward – springs in scale are more compressed – you weigh more –Elevator accelerates downward – springs in scale are less compressed – you weigh less –If elevator cable breaks and elevator falls freely – you would be weightless!

27. © 2012 Pearson Education, Inc. Weight and Weightlessness

28. © 2012 Pearson Education, Inc. A.greater. B.less. C.zero. D.the normal weight. When an elevator accelerates upward, your weight reading on a scale is Weight and Weightlessness CHECK YOUR NEIGHBOR

29. © 2012 Pearson Education, Inc. A.greater. B.less. C.zero. D.the normal weight. Explanation: The support force pressing on you is greater, so you weigh more. When an elevator accelerates upward, your weight reading on a scale is Weight and Weightlessness CHECK YOUR ANSWER

30. © 2012 Pearson Education, Inc. A.greater. B.less. C.zero. D.the normal weight. When an elevator accelerates downward, your weight reading is Weight and Weightlessness CHECK YOUR NEIGHBOR

31. © 2012 Pearson Education, Inc. A.greater. B.less. C.zero. D.the normal weight. Explanation: The support force pressing on you is less, so you weigh less. Question: Would you weigh less in an elevator that moves downward at constant velocity? When an elevator accelerates downward, your weight reading is Weight and Weightlessness CHECK YOUR ANSWER

32. © 2012 Pearson Education, Inc. A.greater. B.less. C.zero. D.the normal weight. When the elevator cable breaks, the elevator falls freely so your weight reading is Weight and Weightlessness CHECK YOUR NEIGHBOR

33. © 2012 Pearson Education, Inc. A.greater. B.less. C.zero. D.the normal weight. Explanation: There is still a downward gravitational force acting on you, but gravity is not felt as weight because there is no support force. So your weight is zero. When the elevator cable breaks, the elevator falls freely so your weight reading is Weight and Weightlessness CHECK YOUR ANSWER

34. © 2012 Pearson Education, Inc. A.moves upward. B.moves downward. C.accelerates upward. D.All of the above. If you weigh yourself in an elevator, you’ll weigh more when the elevator Weight and Weightlessness CHECK YOUR NEIGHBOR

35. © 2012 Pearson Education, Inc. A.moves upward. B.moves downward. C.accelerates upward. D.All of the above. Explanation: The support provided by the floor of an elevator is the same whether the elevator is at rest or moving at constant velocity. Only accelerated motion affects weight. If you weigh yourself in an elevator, you’ll weigh more when the elevator Weight and Weightlessness CHECK YOUR ANSWER

36. © 2012 Pearson Education, Inc. Projectile Motion Projectile is any object that moves through the air or through space under the influence of gravity. Curved path of projectile (parabola) Example: A stone thrown horizontally curves downward due to gravity.

37. © 2012 Pearson Education, Inc. Projectile Motion Projectile curves as a result of these 2 components: 1. constant motion horizontally – it rolls of its own inertia and covers equal distances in equal amounts of time 2. accelerated motion vertically – just like free fall – the faster an object falls, the greater the distance covered in each second

38. © 2012 Pearson Education, Inc. Projectile Motion Projectile motion is a combination of a horizontal component and a vertical component

39. © 2012 Pearson Education, Inc. Projectile Motion Parabola Note that only the vertical velocity component changes with time. The horizontal component remains constant.

40. © 2012 Pearson Education, Inc. Projectile Motion Curved path – combination of horizontal and vertical motion If air resistance is small, the horizontal and vertical components of a projectile’s velocity are completely independent of each other Their combined effect produces the trajectories of projectiles

41. © 2012 Pearson Education, Inc. A.increases. B.decreases. C.remains the same. D.Not enough information. The velocity of a typical projectile can be represented by horizontal and vertical components. Assuming negligible air resistance, the horizontal component along the path of the projectile Projectile Motion CHECK YOUR NEIGHBOR

42. © 2012 Pearson Education, Inc. A.increases. B.decreases. C.remains the same. D.Not enough information. Explanation: Because there is no force horizontally, no horizontal acceleration occurs. The velocity of a typical projectile can be represented by horizontal and vertical components. Assuming negligible air resistance, the horizontal component along the path of the projectile Projectile Motion CHECK YOUR ANSWER

43. © 2012 Pearson Education, Inc. A.downward, g. B.due to a combination of constant horizontal motion and accelerated downward motion. C.opposite to the force of gravity. D.centripetal. When no air resistance acts on a fast-moving baseball, its acceleration is Projectile Motion CHECK YOUR NEIGHBOR

44. © 2012 Pearson Education, Inc. A.downward, g. B.due to a combination of constant horizontal motion and accelerated downward motion. C.opposite to the force of gravity. D.centripetal. When no air resistance acts on a fast-moving baseball, its acceleration is Projectile Motion CHECK YOUR ANSWER

45. © 2012 Pearson Education, Inc. Horizontal Projectiles Two Things to Know: –The ball’s horizontal component of velocity doesn’t change as the falling ball moves forward (no force is acting horizontally) –The ball’s vertical component of velocity does change due to gravity. The vertical distances become further apart with time Parabola – the trajectory of a projectile that accelerates only in the vertical direction while moving at a constant horizontal velocity

46. © 2012 Pearson Education, Inc. Projectiles Launched at an Angle If a cannonball is shot at an upward angle, it should follow a straight line path (no gravity) But with gravity, the cannonball falls until it finally reaches the ground So, where does the cannonball end up? D = ½ g t 2

47. © 2012 Pearson Education, Inc. Projectile Altitude and Range For equal launching speeds, the same range is obtained from two different projection angles—a pair that add up to 90 . Example: Same range occurs for a 75  launch and a 15  launch of the same initial

48. © 2012 Pearson Education, Inc. A.45 . B.60 . C.75 . D.None of the above. A ball tossed at an angle of 30  with the horizontal will go as far downrange as one tossed at the same speed at an angle of Projectile Altitude and Range CHECK YOUR NEIGHBOR

49. © 2012 Pearson Education, Inc. A ball tossed at an angle of 30  with the horizontal will go as far downrange as one tossed at the same speed at an angle of A.45 . B.60 . C.75 . D.None of the above. Explanation: Same initial-speed projectiles have the same range when their launching angles add up to 90 . Why this is true involves a bit of trigonometry—which in the interest of time, we’ll not pursue here. Projectile Altitude and Range CHECK YOUR ANSWER

50. © 2012 Pearson Education, Inc. The Effect of Air Resistance on Projectiles With air resistance, both range and altitude are decreased Without air resistance, the speed lost going up is the same as the speed gained while coming down.

51. © 2012 Pearson Education, Inc. Fast-Moving Projectiles—Satellites Satellite - any projectile moving fast enough to fall continually around the Earth (without falling into it). To become an Earth satellite, the projectile’s horizontal velocity must be great enough for its trajectory to match Earth’s curvature.

52. © 2012 Pearson Education, Inc. Fast-Moving Projectiles—Satellites The Earth’s curvature drops a vertical distance of 5 meters for each 8000 m tangent to the surface. So to orbit Earth, a projectile must travel 8000 m in the time it takes to fall 5 m (18,000 miles/hour).

53. © 2012 Pearson Education, Inc. A.10 meters. B.5 meters below the dashed line. C.less than 5 meters below the straight-line path. D.None of the above. As the ball leaves the girl’s hand, one second later it will have fallen Fast-Moving Projectiles—Satellites CHECK YOUR NEIGHBOR

54. © 2012 Pearson Education, Inc. A.10 meters. B.5 meters below the dashed line. C.less than 5 meters below the straight-line path. D.None of the above. Comment: Whatever the speed, the ball will fall a vertical distance of 5 meters below the dashed line. As the ball leaves the girl’s hand, one second later it will have fallen Fast-Moving Projectiles—Satellites CHECK YOUR ANSWER

55. © 2012 Pearson Education, Inc. A.matches the curved surface of Earth. B.results in a straight line. C.spirals out indefinitely. D.None of the above. When you toss a projectile sideways, it curves as it falls. It will be an Earth satellite if the curve it makes Fast-Moving Projectiles—Satellites CHECK YOUR NEIGHBOR

56. © 2012 Pearson Education, Inc. A.matches the curved surface Earth. B.results in a straight line. C.spirals out indefinitely. D.None of the above. Explanation: For an 8-km tangent, Earth curves downward 5 m. So, a projectile traveling horizontally at 8 km/s will fall 5 m in that time and follow the curve of the Earth. When you toss a projectile sideways, it curves as it falls. It will be an Earth satellite if the curve it makes Fast-Moving Projectiles—Satellites CHECK YOUR ANSWER

57. © 2012 Pearson Education, Inc. Circular Satellite Orbits If a cannonball could be launched at 8 km/s, it would follow earth’s curvature and glide in a circular path around earth If it were fired at a slower speed, it would crash back into earth If it were fired at a faster speed, it would overshoot a circular orbit – out to space In a circular orbit, the speed of a satellite is not changed by gravity, only direction changes

58. © 2012 Pearson Education, Inc. Circular Satellite Orbits For a satellite close to earth, the period (time to make a complete orbit around the earth) is 90 minutes The further a satellite is from earth, the slower its speed, the longer its path, and the longer its period The moon has a period of 27.3 days! Copyright © 2008 Pearson Education, Inc., publishing as Pearson Addison Wesley

59. © 2012 Pearson Education, Inc. Circular Satellite Orbits A payload into orbit requires control over direction of rocket –initially, rocket is fired vertically, then tipped –once above the atmosphere, the rocket is aimed horizontally speed of rocket –payload is given a final thrust to orbital speed of 8 km/s to fall around Earth and become an Earth satellite

60. © 2012 Pearson Education, Inc. Circular Satellite Orbits Positioning beyond Earth’s atmosphere, where air resistance is almost totally absent Example: Space shuttles are launched to altitudes of 150 km or more, to be above air drag. (Are they above Earth’s gravitational field? NO!)

61. © 2012 Pearson Education, Inc. A.a circle. B.an ellipse. C.an oval that is almost elliptical. D.a circle with a square corner, as seen throughout your book. When a satellite travels at constant speed, the shape of its path is Satellite Motion CHECK YOUR NEIGHBOR

62. © 2012 Pearson Education, Inc. A.a circle. B.an ellipse. C.an oval that is almost elliptical. D.a circle with a square corner, as seen throughout your book. When a satellite travels at constant speed, the shape of its path is Satellite Motion CHECK YOUR ANSWER

63. © 2012 Pearson Education, Inc. Elliptical Orbits Ellipse The oval path followed by a satellite. The closed path taken by a point that moves in such a way that the sum of its distances from two fixed points (called foci) is constant. The closer the foci to each other, the more circular it gets.

64. © 2012 Pearson Education, Inc. Elliptical Orbits Elliptical orbit speed of satellite varies –initially, if speed is greater than needed for circular orbit, satellite overshoots a circular path and moves away from Earth –satellite loses speed and then regains it as it falls back toward Earth –it rejoins its original path with the same speed it had initially –procedure is repeated

65. © 2012 Pearson Education, Inc. A.varies. B.remains constant. C.acts at right angles to its motion. D.All of the above. The speed of a satellite in an elliptical orbit Elliptical Orbits CHECK YOUR NEIGHBOR

66. © 2012 Pearson Education, Inc. A.varies. B.remains constant. C.acts at right angles to its motion. D.All of the above. The speed of a satellite in an elliptical orbit Elliptical Orbits CHECK YOUR ANSWER

67. © 2012 Pearson Education, Inc. Escape Speed Escape speed the initial speed that an object must reach to escape gravitational influence of Earth 11.2 kilometers per second from Earth’s surface Escape velocity is escape speed when direction is involved

68. © 2012 Pearson Education, Inc. Escape Speed Superman tosses a ball 8 km/s horizontally from the top of a mountain (just above air resistance): –90 minutes later – he can turn around and catch it –Tossed slightly faster – it takes an elliptical orbit and takes slightly longer to return –Tossed at more than 11.2 km/s – it escapes earth –Tossed at more than 42.5 km/s – it escapes the solar system

69. © 2012 Pearson Education, Inc. Escape Speed First probe to escape the solar system is Pioneer 10, launched from Earth in 1972. accomplished by directing the probe into the path of oncoming Jupiter

70. © 2012 Pearson Education, Inc. A.forever leaves Earth’s gravitational field. B.outruns the influence of Earth’s gravity but is never beyond it. C.comes to an eventual stop, eventually returning to Earth at some future time. D.All of the above. When a projectile achieves escape speed from Earth, it Escape Speed CHECK YOUR NEIGHBOR

71. © 2012 Pearson Education, Inc. A.forever leaves Earth’s gravitational field. B.outruns the influence of Earth’s gravity but is never beyond it. C.comes to an eventual stop, eventually returning to Earth at some future time. D.All of the above. When a projectile achieves escape speed from Earth, it Escape Speed CHECK YOUR ANSWER