Find the moments of inertia about the x & y axes:

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Presentation transcript:

Find the moments of inertia about the x & y axes: Problem 31 Find the moments of inertia about the x & y axes: m = 1.8 kg, M = 3.1 kg

Problem 40 m each blade = 160 kg. Moment of inertia I? Starts from rest, torque τ to get ω = 5 rev/s (10π rad/s) in t = 8 s?

Example 8-11 M = 4 kg, FT = 15 N Frictional torque: τfr = 1.1 m N t = 0, ω0 = 0; t = 3 s, ω = 30 rad/s I = ? Calculate the angular acceleration: ω = ω0+ αt, α = (ω - ω0)/t = 10 rad/s2 N’s 2nd Law: ∑τ = Iα FTR - τfr = Iα  I = [(15)(0.33) -1.1]/10 I = 0.385 kg m2

a  Example 8-12 a) α = ? (pulley) b) t = 0, at rest. The same pulley, connected to a bucket of weight mg = 15 N (m = 1.53 kg). M = 4 kg I = 0.385 kg m2; τfr = 1.1 m N a) α = ? (pulley) a = ? (bucket) b) t = 0, at rest. t = 3 s, ω = ? (pulley) v = ? (bucket) a 

Translation-Rotation Analogues & Connections Displacement x θ Velocity v ω Acceleration a α Force (Torque) F τ Mass (moment of inertia) m I Newton’s 2nd Law: ∑F = ma ∑τ = Iα Kinetic Energy (KE) (½)mv2 ? CONNECTIONS v = rω, atan= rα, aR = (v2/r) = ω2 r τ = rF, I = ∑(mr2)

Section 8-7: Rotational Kinetic Energy Translational motion (Ch. 6): (KE)trans = (½)mv2 Rigid body rotation, angular velocity ω. Rigid  Every point has the same ω. Body is made of particles, masses m. For each m at a distance r from the rotation axis: v = rω. The Rotational KE is: (KE)rot = ∑[(½)mv2] = (½)∑(mr2ω2) = (½)∑(mr2)ω2 ω2 goes outside the sum, since it’s the same everywhere in the body As we just saw, the moment of inertia, I  ∑(mr2)  (KE)rot = (½)Iω2 (Analogous to (½)mv2)

Translation-Rotation Analogues & Connections Displacement x θ Velocity v ω Acceleration a α Force (Torque) F τ Mass (moment of inertia) m I Newton’s 2nd Law ∑F = ma ∑τ = Iα Kinetic Energy (KE) (½)mv2 (½)Iω2 CONNECTIONS v = rω, atan= rα, aR = (v2/r) = ω2 r τ = rF, I = ∑(mr2)

Sect. 8-7: Rotational + Translational KE Rigid body rotation: (KE)rot = (½)Iω2 Now, consider a rigid body, mass M, rotating (angular velocity ω) about an axis through the CM. At the same time, the CM is translating with velocity vCM Example, a wheel rolling without friction. For this, we saw earlier that vCM = rω. The KE now has 2 parts: (KE)trans & (KE)rot  Total KE = translational KE + rotational KE KE = (KE)trans + (KE)rot or KE = (½)M(vCM)2 + (½)ICMω2 where: ICM = Moment of inertia about an axis through the CM

Example 8-13  y = 0 KE+PE conservation: where KE has 2 parts!! A sphere rolls down an incline (no slipping or sliding). KE+PE conservation: (½)Mv2 + (½)Iω2 + MgH = constant, or (KE)1 +(PE)1 = (KE)2 + (PE)2 where KE has 2 parts!! (KE)trans = (½)Mv2 (KE)rot = (½)Iω2  v = 0, ω = 0 v = ?   y = 0

Conceptual Example 8-14: Who Wins the Race? v increases as I decreases! Demonstration! MgH = (½)Mv2 + (½)ICMω2 Gravitational PE is Converted to Translational + Rotational KE! Hoop: ICM = MR2 Cylinder: ICM = (½)MR2 Sphere: ICM = (2/5)MR2 (also, v = ωR)

 Ffr does no work! Friction: Necessary for objects to roll without slipping. Example: work done by friction hasn’t been included (used KE +PE =const). WHY? Because Ffr  Motion  Ffr does no work!