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Bellringer 11/12 A worker does 25 J of work lifting a bucket, then sets the bucket back down in the same place. What is the total net work done on the bucket?

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Bellringer 11/12. A worker does 25 J of work lifting a bucket, then sets the bucket back down in the same place. What is the total net work done on the bucket?. Chapter 7: Circular Motion and Gravitation. Object is moving tangent to the circle - PowerPoint PPT Presentation

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Page 1: Bellringer  11/12

Bellringer 11/12

• A worker does 25 J of work lifting a bucket, then sets the bucket back down in the same place. What is the total net work done on the bucket?

Page 2: Bellringer  11/12

Chapter 7: Circular Motion and Gravitation

Page 3: Bellringer  11/12

• Circular Motion – motion of an object about a single axis at a constant speed

Object is moving tangent to the circle

- Direction of the velocity vector is the same direction of the object’s motion – the velocity vector is directed tangent to the circle

Object moving in a circle is accelerating

Page 4: Bellringer  11/12

• Tangential speed (vt) – speed of an object in circular motion When vt is constant = uniform circular motion Depends on distance

Page 5: Bellringer  11/12

Centripetal Acceleration

• Centripetal Acceleration – acceleration directed toward the center of a circular path (center-seeking)

Centripetal Accelerationac = vt

2/rCentripetal Acceleration = (tangential speed)2 /radius of

circular path

Page 6: Bellringer  11/12

Example

• A test car moves at a constant speed around a circular track. If the car is 48.2 m from the track’s center and has a centripetal acceleration of 8.05m/s2, what is the car’s tangential speed?

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• Tangential acceleration – acceleration due to the change in speed

Page 8: Bellringer  11/12

• Centripetal Force – net force directed toward the center of an object’s circular path

Centripetal ForceFc = mvt

2/rCentripetal Force= mass x (tangential speed)2 /radius of

circular path

Example: Gravitational Force – keeps moon in its orbit

Page 9: Bellringer  11/12

Example

• A pilot is flying a small plane at 56.6m/s in a circular path with a radius of 188.5m. The centripetal force needed to maintain the plane’s circular motion is 1.89x104 N. What is the plane’s mass?

Page 10: Bellringer  11/12

Example

• A car is negotiating a flat curve of radius 50. m with a speed of 20. m/s. If the centripetal force provided by friction is 1.2 x 104 N.

• A. What is the mass of the car?• B. What is the coefficient of friction?

Page 11: Bellringer  11/12

Centripetal vs Centrifugal

• Centrifugal – center fleeing – away from the center/outward DOES NOT EXIST!!!! Fake force!

Page 12: Bellringer  11/12

Bellringer 11/14

• A building superintendent twirls a set of keys in a circle at the end of a cord. If the keys have a centripetal acceleration of 145 m/s2 and the cord has a length of 0.34m, what is the tangential speed of the keys?

Page 13: Bellringer  11/12

• Gravitational Force – mutual force of attraction between particles of matter

Newton’s Law of Universal GravitationFg = G m1m2

r2

Gravitational Force= constant x mass1 x mass2(distance between masses) 2

G = 6.673x10 -11 N•m 2 kg 2

Page 14: Bellringer  11/12

Example

• Find the distance between a 0.300kg billiard ball and a 0.400kg billiard ball if the magnitude of the gravitational force between them is 8.92x10 -11 N.

Page 15: Bellringer  11/12

Gravity’s Influence

• Tides – periodic rise and fall of water

Page 16: Bellringer  11/12

Field Force

• Gravitational force is an interaction between a mass and the gravitational field created by other masses

Gravitational Field Strengthg = Fg /m

g = 9.81m/s2 on Earth’s surface

Page 17: Bellringer  11/12

Weight changes with location

• Weight = mass x free-fall acceleration or

● Weight = mass x gravitational field strength

Fg = Gmme / r2

g = Fg /m = Gmme /m r2 = Gme / r2

Page 18: Bellringer  11/12

Weight

• Gravitational field strength depends only on mass and distance – your distance increases, g decreases…your weight decreases

Page 19: Bellringer  11/12

Bellringer 11/15

• A 7.55x1013 kg comet orbits the sun with a speed of 0.173km/s. If the centripetal force on the comet is 505N, how far is it from the sun?

Page 20: Bellringer  11/12

Example

• Suppose the value of G has just been discovered. Use the value of G and an approximate value for Earth’s radius to find an approximation for Earth’s mass.

Page 21: Bellringer  11/12

Example• Earth has a mass of 5.97x1024kg and a

radius of 6.38x106 m, while Saturn has a mass of 5.68x1026 kg and a radius of 6.03x107 m. Find the weight of a 65.0kg person at the following locations

a. On the surface of Earthb. 1000km above the surface of Earthc. On the surface of Saturnd. 1000 km above the surface of Saturn

Page 22: Bellringer  11/12

Example

• A scam artist hopes to make a profit by buying and selling gold at different altitudes for the same price per weight. Should the scam artist buy or sell at the higher altitude? Explain.

Page 23: Bellringer  11/12

Bellringer 11/18

• What is the force of gravity between two 74.0kg physics students that are sitting 85.0cm apart?

Page 24: Bellringer  11/12

Motion in Space

• Claudius Ptolemy Thought Earth was the center of the universe

• Nicolaus Copernicus Thought Earth orbits the sun in perfect circles

Page 25: Bellringer  11/12

Johannes Kepler

Kepler’s Laws of Planetary Motion

- First Law: Each planets travels in an elliptical orbit around the sun, the sun is at one of the focal points

Page 26: Bellringer  11/12

Kepler’s Laws of Planetary Motion

- Second Law: An imaginary line drawn from the sun to any planet sweeps out equal areas in equal time

intervals

Page 27: Bellringer  11/12

Kepler’s Laws of Planetary Motion

- Third Law: The square of a planet’s orbital period (T2 ) is proportional to the cube of the average distance (r3 )

between the planet and the sun

Planet Period(s)

AverageDist. (m)

T2/R3

(s2/m3)

Earth 3.156 x 107 s

1.4957 x 1011 2.977 x 10-19

Mars 5.93 x 107 s 2.278 x 1011 2.975 x 10-19

Page 28: Bellringer  11/12

Example• The moons orbiting Jupiter follow the same

laws of motion as the planets orbiting the sun. One of the moons is called Io - its distance from Jupiter's center is 4.2 units and it orbits Jupiter in 1.8 Earth-days. Another moon is called Ganymede; it is 10.7 units from Jupiter's center. Make a prediction of the period of Ganymede using Kepler's law of harmonies.

Answer: 7.32 days

Page 29: Bellringer  11/12

Period and Speed of an object in circular motion

T = 2π r3 vt = G m Gm r

T = Orbital period r = mean radiusm = mass of central object vt = orbital speed

√ √

m is the mass of the central object. Mass of the planet/satellite that is in orbit does not affect the period or speed

Page 30: Bellringer  11/12

Example

• During a spacecraft’s fifth orbit around Venus, it traveling at a mean altitude of 361km. If the orbit had been circular, what would the spacecraft’s period and speed have been?

Page 31: Bellringer  11/12

Example

• At what distance above Earth would a satellite have a period of 125 minutes?

Page 32: Bellringer  11/12

Bellringer 11/19

• At the surface of a red giant star, the gravitational force on 1.00kg is only 2.19x10-3 N. If its mass equals 3.98x1031 kg, what is the star’s radius?

Page 33: Bellringer  11/12

What is the correct answer?• Astronauts on the orbiting space station are

weightless because…a. There is no gravity in space and they do not

weight anythingb. Space is a vacuum and they is no gravity in a

vacuumc. Space is a vacuum and there is no air

resistance in a vacuumd. The astronauts are far from Earth’s surface at a

location where gravitation has a minimal affect

Page 34: Bellringer  11/12

Weight and Weightlessness

• Weightlessness – sensation when all contact forces are removed

Page 36: Bellringer  11/12

Example

• Otis’ mass is 80kg. a. What is the scale reading when Otis

accelerates upward at 0.40m/s2 b. What is the scale reading when Otis is

traveling upward at a constant velocity at 2.0m/s

c. Otis stops at the top floor and then accelerates downward at a rate of 0.40m/s2