Your SlideShare is downloading. ×
Lecture13
Upcoming SlideShare
Loading in...5
×

Thanks for flagging this SlideShare!

Oops! An error has occurred.

×
Saving this for later? Get the SlideShare app to save on your phone or tablet. Read anywhere, anytime – even offline.
Text the download link to your phone
Standard text messaging rates apply

Lecture13

283
views

Published on

Published in: Technology, Economy & Finance

0 Comments
0 Likes
Statistics
Notes
  • Be the first to comment

  • Be the first to like this

No Downloads
Views
Total Views
283
On Slideshare
0
From Embeds
0
Number of Embeds
0
Actions
Shares
0
Downloads
2
Comments
0
Likes
0
Embeds 0
No embeds

Report content
Flagged as inappropriate Flag as inappropriate
Flag as inappropriate

Select your reason for flagging this presentation as inappropriate.

Cancel
No notes for slide
  • W = K + U
    v = sqrt ( 2 m_2 g h / ( m1+m2))
  • Transparency
  • Transcript

    • 1. Physics 101: Lecture 13, Pg 1 Physics 101:Physics 101: Lecture 13Lecture 13 RotationalRotational Kinetic EnergyKinetic Energy andand RotationalRotational InertiaInertia Exam II
    • 2. Physics 101: Lecture 13, Pg 2 Overview of SemesterOverview of Semester Newton’s Laws Σ F = m a Work-Energy Σ F = m a multiply both sides by d Σ W = ∆KE Energy is “conserved” Useful when know Work done by forces Impulse-Momentum Σ F = m a multiply both sides by ∆t Σ I = ∆p Momentum is “conserved” Useful when know about EXTERNAL forces Works in each direction independently
    • 3. Physics 101: Lecture 13, Pg 3 Linear and Angular MotionLinear and Angular Motion Linear Angular Displacement x θ Velocity v ω Acceleration a α Inertia m I KE ½ m v2 N2L F=ma Momentum p = mv Today!
    • 4. Physics 101: Lecture 13, Pg 4 Comment on axes and signComment on axes and sign (i.e. what is positive and negative)(i.e. what is positive and negative) Whenever we talk about rotation, it is implied that there is a rotation “axis”. This is usually called the “z” axis (we usually omit the z subscript for simplicity). Counter-clockwise (increasing θ) is usually called positive. Clockwise (decreasing θ) is usually called negative. [demo] z +ω
    • 5. Physics 101: Lecture 13, Pg 5 Energy ACT/demoEnergy ACT/demo When the bucket reaches the bottom, it’s potential energy has decreased by an amount mgh. Where has this energy gone? A) Kinetic Energy of bucket B) Kinetic Energy of flywheel C) Both 1 and 2. At bottom, bucket has zero velocity, energy must be in flywheel!
    • 6. Physics 101: Lecture 13, Pg 6 Rotational Kinetic EnergyRotational Kinetic Energy Consider a mass M on the end of a string being spun around in a circle with radius r and angular frequency ω [demo] Mass has speed v = ω r Mass has kinetic energy » K = ½ M v2 » = ½ M ω2 r2 Rotational Kinetic Energy is energy due to circular motion of object. M
    • 7. Physics 101: Lecture 13, Pg 7 Rotational InertiaRotational Inertia II Tells how much “work” is required to get object spinning. Just like mass tells you how much “work” is required to get object moving. Ktran = ½ m v2 Linear Motion Krot = ½ I ω2 Rotational Motion I = Σ miri 2 (units kg m2 ) Note! Rotational Inertia (or “Moment of Inertia”) depends on what you are spinning about (basically the ri in the equation).
    • 8. Physics 101: Lecture 13, Pg 8 Rotational Inertia TableRotational Inertia Table For objects with finite number of masses, use I = Σ m r2 . For “continuous” objects, use table below (p. 263 of book).
    • 9. Physics 101: Lecture 13, Pg 9 Merry Go RoundMerry Go Round KE = 4 x ½ m v2 = 4 x ½ m ω r2 = ½ I ω2 Where I = 4 m r2 Further mass is from axis of rotation, greater KE it has. [strength contest] BA Four kids (mass m) are riding on a (light) merry-go-round rotating with angular velocity ω=3 rad/s. In case A the kids are near the center (r=1.5 m), in case B they are near the edge (r=3 m). Compare the kinetic energy of the kids on the two rides. A) KA > KB B) KA = KB C) KA < KB
    • 10. Physics 101: Lecture 13, Pg 10 Inertia RodsInertia Rods Two batons have equal mass and length. Which will be “easier” to spin A) Mass on ends B) Same C) Mass in center I = Σ m r2 Further mass is from axis of rotation, greater moment of inertia (harder to spin)
    • 11. Physics 101: Lecture 13, Pg 11 Preflight: Rolling RacePreflight: Rolling Race (Hoop vs Cylinder)(Hoop vs Cylinder) A solid and hollow cylinder of equal mass roll down a ramp with height h. Which has greatest KE at bottom? A) Solid B) Hollow C) Same 25% 20% 54% “Both start with same PE so they both end with same KE.”
    • 12. Physics 101: Lecture 13, Pg 12 Preflight: Rolling RacePreflight: Rolling Race (Hoop vs Cylinder)(Hoop vs Cylinder) A solid and hollow cylinder of equal mass roll down a ramp with height h. Which has greatest speed at the bottom of the ramp? A) Solid B) Hollow C) Same 50% 17% 33% “Well, I don't see how rolling things down a ramp would make me a dare-devil, thrill seeker...” “Evel Knievel must be ‘rolling’ in his grave at such a travesty” I = MR2 I = ½ MR2
    • 13. Physics 101: Lecture 13, Pg 13 Main IdeasMain Ideas Rotating objects have kinetic energy KE = ½ I ω2 Moment of Inertia I = Σ mr2 Depends on Mass Depends on axis of rotation Energy is conserved but need to include rotational energy too: Krot = ½ I ω2
    • 14. Physics 101: Lecture 13, Pg 14 Massless Pulley ExampleMassless Pulley Example Consider the two masses connected by a pulley as shown. Use conservation of energy to calculate the speed of the blocks after m2 has dropped a distance h. Assume the pulley is massless. finalfinalinitialinitial KUKU +=+ 2 2 2 12 2 1 2 1 00 vmvmghm ++−=+ 21 22 mm ghm v + = 2 2 2 122 vmvmghm += UKWNC ∆+∆=∑ Note: Tension does positive work on 1 and negative work on 2. Net work (on 1 and 2) by tension is ZERO.
    • 15. Physics 101: Lecture 13, Pg 15 Massive Pulley ActMassive Pulley ActConsider the two masses connected by a pulley as shown. If the pulley is massive, after m2 drops a distance h, the blocks will be moving A) faster than B) the same speed as C) slower than if it was a massless pulley finalfinalinitialinitial KUKU +=+ 22 2 2 12 2 1 2 1 2 1 0 ωIvmvmghm +++−= 2 22 2 2 12 2 1 2 1 2 1 2 1            +++= R v MRvmvmghm 22 2 2 12 4 1 2 1 2 1 Mvvmvmghm +++= 2/ 2 21 2 Mmm ghm v ++ = Slower because some energy goes into spinning pulley!
    • 16. Physics 101: Lecture 13, Pg 16 SummarySummary Rotational Kinetic Energy Krot = ½ I ω2 Rotational Inertia I = Σ miri 2 Energy Still Conserved!

    ×