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0. Physics 1710 Chapter 6—Circular Motion. Answer: a = ∆v/∆ t a = (112 m/s)/(2.5 sec) = 44.8 m/s 2 Thrust = force F = ma = (1800. kg)(44.8 m/s 2 ) ~ 81 kN. 0. Physics 1710 Chapter 6—Circular Motion. 1 ′ Lecture: - PowerPoint PPT Presentation
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Answer:Answer:
a = a = ∆v/∆∆v/∆t t a = (112 m/s)/(2.5 sec) = a = (112 m/s)/(2.5 sec) = 44.8 m/s44.8 m/s22
Thrust = forceThrust = forceF = ma = (1800. kg)(44.8 m/s F = ma = (1800. kg)(44.8 m/s 2 2 ) ~ 81 kN) ~ 81 kN
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
11′ Lecture:′ Lecture: • The net force on a body executing circular motion The net force on a body executing circular motion is equal to the mass times the centripetal is equal to the mass times the centripetal acceleration of the body. acceleration of the body. FFcentripetalcentripetal = = m m aaccentripetalentripetal
•aacentripetalcentripetal = = v v 22/ R/ R [toward the center]; [toward the center]; aa = - = -ωω22 rr
• In non-inertial frames of reference one may sense In non-inertial frames of reference one may sense fictitious forces.fictitious forces.
• At At terminal velocityterminal velocity the velocity-dependent the velocity-dependent resistive forces balance the accelerating forces so resistive forces balance the accelerating forces so that no further acceleration occurs.that no further acceleration occurs.
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
Centripetal Acceleration:Centripetal Acceleration:
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
x = r cos x = r cos θθyy = r sin = r sin θθ
vvxx = (dr/dt) cos = (dr/dt) cos θθ- r sin - r sin θθ(d (d θ/dt)θ/dt) vvyy = (dr/dt) sin = (dr/dt) sin θθ+r cos +r cos θθ(d (d θ/dt)θ/dt) Let (dr/dt) = 0Let (dr/dt) = 0 vvxx = - r = - r ω ω sin sin θθ
vvyy = +r = +r ω ω cos cos θθ
aaxx = dv= dvxx /dt= d(- r /dt= d(- r ω ω sin sin θ)/dt θ)/dt = = r r ωω22cos cos θ- θ- r r ω ω sin sin θ(d ω/dt)θ(d ω/dt)
aayy = dv= dvyy /dt= d(r /dt= d(r ω ω cos cos θ)/dt θ)/dt = -= -r r ωω22sin sin θ+ θ+ r r ω cosω cos θ(d ω/dt)θ(d ω/dt)
a a = = - ω- ω22 r + r + r r (d (d vvtangentialtangential /dt) /dt)
θθvvxx
vvyy
Centripetal Acceleration:Centripetal Acceleration:
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
a a centripetalcentripetal = = - v - v 22 / r / r
aa tangentialtangential = = r r (d v(d vtangentialtangential /dt)/dt)
F F = m = m a a
F F centripetalcentripetal = m a = m a centripetalcentripetal = = - mv - mv 22 / r / r
θθvvxx
vvyy
Demonstration: Ball on a StringDemonstration: Ball on a String
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
FFcentripetalcentripetal
rr
mm
vv
FFcentripetal centripetal = m v = m v 22/r /r
An athlete swings a 8 kg “hammer” around An athlete swings a 8 kg “hammer” around on a 1.2 m long cable at an angular on a 1.2 m long cable at an angular frequency of 1.0 revolution per second. How frequency of 1.0 revolution per second. How much force must he exert on the hammer much force must he exert on the hammer throw handle?throw handle?
Physics 1710 — Physics 1710 — e-Quize-Quiz
Answer Now !
1 2 3 4
7%
57%
22%
15%
1.1. About 12. NAbout 12. N
2.2. About 30. NAbout 30. N
3.3. About 78. NAbout 78. N
4.4. About 380. NAbout 380. N
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20
21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40
Demonstration: Ball on a StringDemonstration: Ball on a String
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
FFcentripetalcentripetal
rr
mm
vv
v = 2v = 2π r/T = 2(3.14) (1.2 m)/(1.0 sec) = 7.5 π r/T = 2(3.14) (1.2 m)/(1.0 sec) = 7.5 m/sm/s
FFcentripetal centripetal = m v = m v 22/r = (8.0 kg)(7.5 m/s)/r = (8.0 kg)(7.5 m/s)22/(1.2 /(1.2 m) m)
= 378 N ~ 380 N= 378 N ~ 380 N
Demonstration: Demonstration: Marble in a bottleMarble in a bottle
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
Why does the marble stay up on Why does the marble stay up on the side?the side?
No Talking!No Talking!Think!Think!
Confer!Confer!
Peer Instruction Peer Instruction TimeTime
Why does the marble stay up on the Why does the marble stay up on the side?side?
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
Satellites in OrbitSatellites in Orbit
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
Which orbit is most like that of the Space Which orbit is most like that of the Space Shuttle?Shuttle?
No Talking!No Talking!Think!Think! Confer!Confer!
Peer Instruction Peer Instruction TimeTime
Physics 1710Physics 1710 Unit 1—Review Unit 1—Review
11223344
Satellite Motion:Satellite Motion:• h ~ 100 km , h ~ 100 km , RR⊕ ⊕ ~ 6300 km~ 6300 km
•FFgg= G Mm/ r = G Mm/ r 22 GravitGravityy
• FFgg = F = Frr = mv = mv 22/r /r
• v = v = √[GM/r] = √[GM/(R√[GM/r] = √[GM/(R⊕ ⊕ + h)]~ √[GM/R+ h)]~ √[GM/R⊕ ⊕ ]]
= √[gR= √[gR⊕ ⊕ ]= √[(9.8 m/s]= √[(9.8 m/s22)(6.3 x10)(6.3 x1066m)m) ]= ]=
7.9x107.9x1033 m/s m/s
~17,600 mph~17,600 mph
• Why do the shuttle astronauts appear Why do the shuttle astronauts appear
“weightless?”“weightless?”
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
Satellites in OrbitSatellites in Orbit
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion
Orbiting satellites are in free fall but Orbiting satellites are in free fall but miss the earth because it curves.miss the earth because it curves.
Summary Summary • The net force on a body executing circular The net force on a body executing circular motion is equal to the mass times the centripetal motion is equal to the mass times the centripetal acceleration of the body.acceleration of the body.
•aacentripedalcentripedal = = v v 22/ R/ R [toward the center] [toward the center]
• The “centrifugal” force is a fictitious force due to The “centrifugal” force is a fictitious force due to a non-inertial frame of reference.a non-inertial frame of reference.
Physics 1710Physics 1710 Chapter 6—Circular Chapter 6—Circular Motion Motion