fisica1-youn-e-freedman-exercicios-resolvidos

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5.119: The analysis is the same as for Problem 5.95; in the case of the cone, the speed is related to the period by v = 2π R T = 2πh tan β T , or T = 2πh tan β v. The maximum and minimum speeds are the same as those found in Problem 5.95, cos β + µ s sin β vmax = gh tan β sin β − µ cos β v min = cos β − µ s sin β gh tan β . sin β + µ cos β The minimum and maximum values of the period T are then h tan β sin β − µ s cos β Tmin = 2π g cos β + µ sin β T max = 2π h tan β sin β + µ s cos β . g cos β − µ sin β s s s s
5.120: a) There are many ways to do these sorts of problems; the method presented is fairly straightforward in terms of application of Newton’s laws, but involves a good deal of algebra. For both parts, take the x-direction to be horizontal and positive to the right, and the y-direction to be vertical and positive upward. The normal force between the block and the wedge is n; the normal force between the wedge and the horizontal surface will not enter, as the wedge is presumed to have zero vertical acceleration. The horizontal acceleration of the wedge is A, and the components of acceleration of the block are a x and a y . The equations of motion are then MA = −n sin α ma ma x y = n sin α = n cosα − mg. Note that the normal force gives the wedge a negative acceleration; the wedge is expected to move to the left. These are three equations in four unknowns, A, a , a and n. Solution is possible with the imposition of the relation between A, a x and a y . An observer on the wedge is not in an inertial frame, and should not apply Newton’s laws, but the kinematic relation between the components of acceleration are not so restricted. To such an observer, the vertical acceleration of the block is a y, but the horizontal acceleration of the block is a x − A. To this observer, the block descends at an angle α , so the relation needed is ay = − tan α. ax − A At this point, algebra is unavoidable. Symbolic-manipulation programs may save some M solution time. A possible approach is to eliminate a x by noting that ax = − A (a result m that anticipates conservation of momentum), using this in the kinematic constraint to eliminate a y and then eliminating n. The results are: − gm A = ( M + m) tan α + ( M a x gM = ( M + m) tan α + ( M tan α) tan α) − g( M + m) tan α ay = ( M + m) tan α + ( M tan α) (b) When M >> m, A → 0, as expected (the large block won’t move). Also, g tanα ax → tanα + (1 tanα ) = g 2 = g sin α cosα, which is the acceleration of the block tan α + 1 ( g sin α in this case), with the factor of cos α giving the horizontal component. Similarly, a y → −g sin 2 α. (c) The trajectory is a spiral. x y
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Física I - Sears, Zemansky, Young
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5 1.1: 1mi × ( 5280ft mi) × ( 12
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1.15: a) If a meter stick can measu
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8 11 1.28: The moon is about 4× 10
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1.34: r o o 1.35: A ; A x = ( 12.0
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1.39: Using components as a check f
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1.43: a) The magnitude of A r + B r
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1.48: a) ˆ ˆ ˆ 2 2 2 i + j + k =
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1.53: Use of the right-hand rule to
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1.59: a) To three significant figur
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1.65: Let D r be the fourth force.
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1.68:a) R = A + B + C x R y = x x x
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1.70: The third leg must have taken
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−1 200−20 o 1.73: a) Angle of f
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1.75: Let +x be east and +y be nort
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1.78: (a) Take the beginning of the
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1.83: a) Parallelog ram area = 2 ×
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1.88: a) This is a statement of the
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1.91: A r and C r are perpendicular
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1.96: a) b) i) In AU, ii) In AU, ii
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Capítulo 2
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2.6: The s-waves travel slower, so
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2.14: (a) The displacement vector i
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2.18: a) The velocity at t = 0 is a
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2.20: a) The bumper’s velocity an
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2.26: a) x 0 < 0, v 0x < 0, a x < 0
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2.28: a) Interpolating from the gra
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2.31: a) At t = 3 s the graph is ho
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2.35: a) b) From the graph (Fig. (2
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2.37: a) The car and the motorcycle
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2.43: a) Using the method of Exampl
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2.45: a) v y = v0 y − gt = ( −6
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2.49: a) For a given initial upward
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2.51: a) From Eqs. (2.17) and (2.18
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2.53: a) The change in speed is the
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.0 m 2.56: a) 1.25m s. 25 = 20.0 s
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1 8 m ⎛ 365 d ⎞⎛ ⎞⎛ 2.62:
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2.66: a) The simplest way to do thi
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2 2.69: a) x = 1 2) a t , and with
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2.71: a) Travelling at 20 m s , Jua
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2.77: Let t 1 be the fall for the w
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2.82: a) 2.83: a) From Eq. (2.14),
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2 2.86: a) The helicopter accelerat
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2.90: a) Suppose that Superman fall
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2 2.93: The velocities are vA = α
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1 2.96: The time spent above y max
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2.98: a) Let the height be h and de
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3.1: a) v (5.3 m) − (1.1m) = 1.4
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3.7: a) b) r ˆ ˆ 2 v = αi − 2
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3.11: Take + y to be upward. Use Ch
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3.15: a) Solving Eq. (3.17) for v =
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v y . g 2 9.80 m s 0 16.0 m s 3.18:
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3.22: Substituting for t in terms o
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3.25: Take + y to be downward. a) U
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3.34: a) a 2 rad = ( 3 m/s) /(14 m)
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3.45: a) The a = 0 and a y = −2β
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3.48: a) The equations of motions a
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3.52: a) Setting y = −h in Eq. (3
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3.58: Equation 3.27 relates the ver
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3.60: a) This may be done by a dire
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3.64: Combining equations 3.25, 3.2
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3.66: (a) v x ( runner) = vx (ball)
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3.69: Take + y to be upward. a) The
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3.73: a) The acceleration is given
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3.76: a) dv dt = = d dt (1/ 2) vxax
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3.85: The three relative velocities
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3.90: As in the previous problem, t
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3.92: The x-position of the plane i
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4.1: a) For the magnitude of the su
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2 4.11: a) During the first 2.00 s,
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4.24: (a) Each crate can be conside
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4.27: a) b) For the chair, a y = 0
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4.33: a) The resultant must have no
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2 4.39: a) Both crates moves togeth
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4.43: a) The engine is pulling four
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Page 153 and 154: 4.51: a) L is the lift force b) ∑
Page 155 and 156: 2 4.54: The velocity as a function
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Page 159 and 160: 5.1: a) The tension in the rope mus
Page 161 and 162: 5.14: a) In level flight, the thrus
Page 163 and 164: 2L 5.20: Similar to Exercise 5.16,
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Page 177 and 178: 5.67: Consider the forces on the pe
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Page 183 and 184: 5.77: See Exercise 5.40. a) The max
Page 185 and 186: 5.82: We take the upward direction
Page 187 and 188: 5.85: Denote the magnitude of the a
Page 189 and 190: 5.92: (a) There is a contact force
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Page 195 and 196: mg mg 5.103: Without buoyancy, kv t
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Page 199 and 200: 5.109: a) For the same rotation rat
Page 201: 5.116: a) Differentiating twice, a
Page 205 and 206: 5.124: For convenience, take the po
Page 207 and 208: 5.126: In all cases, the tension in
Page 209 and 210: 6.1: a) ( 2.40 N) (1.5 m) = 3.60 J
Page 211 and 212: 6.10: a) From Eq. (6.6), 1 2 5 ⎛
Page 213 and 214: 6.18: As the example explains, the
Page 215 and 216: 6.27: a) The friction force is µ k
Page 217 and 218: 6.35: a) The static friction force
Page 219 and 220: 6.42: The initial and final kinetic
Page 221 and 222: 6.53: a) In terms of the accelerati
Page 223 and 224: 6.58: The work per unit mass is ( W
Page 225 and 226: 6.66: Let x be the distance past P.
Page 227 and 228: 6.71: The velocity and acceleration
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Page 231 and 232: 6.85: f = .25 mg soW f = W = −(0.
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Page 235 and 236: (8.00 hp)(746 W/hp) 6.99: a) = 358
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Page 239 and 240: 6.104: From F = m a, Fx = max, Fy =
Page 241 and 242: 7.1: From Eq. (7.2), mgy = (800 kg)
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Page 245 and 246: 2 7.16: U = 1 ky , where y is the v
Page 247 and 248: 1 2 1 2 7.24: From kx = mv , the re
Page 249 and 250: dU 3 3 7.34: From Eq. (7.15), F =
Page 251 and 252: 7.39: a) At constant speed, the upw
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1 2 7.46: a) U − U = mg( h − 2R
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7.49: a) K 1 + U1 + Wother = K2 + U
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7.54: To be at equilibrium at the b
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7.57: The two design conditions are
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7.62: a) The skier’s kinetic ener
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1 2 1 2 7.69: With U = 0 , K = 0 K
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7.74: a) From either energy or forc
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2 2 2 2 7.78: a) a = d x dt = −ω
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3 7.83: a) Along this line, x = y ,
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7.86: a) The slope of the U vs. x c
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Capítulo 8
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8.7: ∆p ∆t ( 0.0450 kg)( 25.0 m
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8.14: The impluse imparted to the p
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8.21: a) Taking v A and v B to be m
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8.25: m + m )(3.00 m s) = m (4.00 m
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8.31: Use conservation of the horiz
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8.37: Let +y be north and +x be sou
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8.43: a) In Eq. (8.24), let mA = m
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8.52: It turns out to be more conve
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8.63: The total momentum must be ze
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8.69: (This problem involves solvin
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8.72: a) The stuntman’s speed bef
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8.76: Just after the collision: ∑
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8.80: a) From the derivation in Sec
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8.83: a) In terms of the primed coo
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8.86: (a) For momentum to be conser
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8.90: a) For the x - and y - direct
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8.96: The trick here is to realize
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8.98: The two fragments are 3.00 kg
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8.101: a) If the objects stick toge
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8.107: a) For t < 0 the rocket is a
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8.111: a) The tension in the rope a
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9.1: a) 1.50 m = 0.60 rad = 34.4°
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2 9.10: a) ω = ω + α t = 1.50 ra
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9.18: The following table gives the
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9.24: From a rad = ω 2 r, 4 which
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vr 5.00 m s 9.33: The angular veloc
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9.40: a) In the expression of Eq. (
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2π 2 2 9.49: a) ω = T , so Eq. (9
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9.60: For this case, dm = γ dx. a)
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dθ 2 2 3 2 9.65: a) ω z = = 2γt
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9.70: a) The angular acceleration w
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9.75: I approximate my body as a ve
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9.81: a) Consider a small strip of
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9.84: Taking the zero of gravitatio
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9.90: a) In the case that no energy
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9.94: a) From the parallel-axis the
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9.99: a) Following the hint, the mo
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Capítulo 10
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10.6: (a) τ A = (50 N)(sin 60° )(
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1 2 2 = m 2 8.25 kg 0.0750 m = 0.02
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10.23: n = mg cos α mg sin θ −
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10.26: a) The angular speed of the
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10.32: I = mL 1 2 1 2 2 = ( 117 kg)
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10.40: The skater’s initial momen
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10.46: (a) Conservation of angular
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2 2π rad 10.51: a) Solving Eq. (10
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2 2θ 2θ 2θ I 10.57: t = = = . α
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10.63: The net torque on the pulley
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2 10.67: For the disk, K = (3 4) Mv
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10.72: (a) Στ = Iα and a = Rα T
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10.75: a) Use conservation of energ
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10.79: a) v = 10K 7m = ( 10)( 0.800
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10.84: (a) Στ = Iα 1 1 2 mg cos
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10.90: Angular momentum is conserve
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10.95: a) The initial angular momen
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10.100: a) The distance from the ce
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10.102: Denoting the upward forces
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11.1: Take the origin to be at the
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11.12: a) b) x = 6 .25 m when FA =
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11.18: a) Denote the length of the
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11.30: a) The volume would increase
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11.43: For the airplane to remain i
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11.49: The horizontal component of
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11.56: (a) and (b) Lower rod: Στ
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11.59: a) ∑τ = 0, axis at lower
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−4 −4 2 11.64: a) ∆w = −σ
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11.68: (a) ΣτElbow = 0 F (3.80 cm
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11.71: a) Consider the forces on th
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11.74: a) The center of gravity of
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11.79: a) Take torques about the po
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11.87: Use subscripts 1 to denote t
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11.93: a) Taking torques about the
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11.95: Assume that the center of gr
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