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Conservation of Momentum

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After the collision, the first block continues to. the right with a speed v1f = 1 m/s, and the ... After collision: px,f = m1v1 cos ?1 m2v2 cos ?2. py,f ... – PowerPoint PPT presentation

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Title: Conservation of Momentum


1
Conservation of Momentum
  • Chris Sedlack

2
Momentum Review
  • The momentum of a particle depends on its mass
    and its velocity
  • p mv
  • The force on a particle is the change in momentum
    over time
  • F dp/dt d(mv)/dt v dm/dt m dv/dt
  • ma (for constant m)

3
Conservation of Momentum
  • When there is no net external force on a system,
  • S pi S pf
  • Allows us to make predictions about systems even
    without knowledge regarding internal forces

4
1-D Example
  • A block of mass m1 10 kg slides along a
  • frictionless surface with velocity vi to the
    right
  • until it collides with a block of mass m2 5 kg.
  • After the collision, the first block continues to
  • the right with a speed v1f 1 m/s, and the
  • second block moves to the right with a speed
  • v2f 4 m/s. What was the initial speed of the
  • first block?

5
1-D Example Solution
  • Initial momentum
  • pi m1v1i m2v2i m1vi
  • Final momentum
  • pf m1v1f m2v2f
  • Conservation of momentum
  • pi pf
  • m1vi m1v1f m2v2f
  • vi v1f (m2/m1) v2f
  • Numerical result
  • vi 1 m/s (5 kg/10 kg)(4 m/s)
  • vi 3 m/s

6
Momentum Conservation in 2-D
  • Momentum is a vector
  • We must conserve each component individually

Before collision px,i m1vi
py,i 0 After collision
px,f m1v1 cos ?1 m2v2 cos ?2
py,f m1v1 sin ?1 - m2v2 sin ?2 Conservation of
momentum m1vi m1v1 cos ?1 m2v2
cos ?2 0 m1v1 sin ?1 - m2v2 sin
?2
7
Momentum Conservation and Newtons Third Law
  • For a two-particle system
  • ?p ?p1 ?p2
  • ?p1 ? F1 dt ?p2 ?
    F2 dt
  • ?p1 ? (F12 F1,ext) dt ?p2 ? (F21
    F2,ext) dt
  • ?p ? (F12 F21 F1,ext F2,ext) dt
  • No Net External Force F1,ext F2,ext 0
  • Newtons Third Law F12 -F21
  • ? ?p 0
  • Momentum is conserved!

8
Conservation of momentum Summary
  • Conservation of momentum is a consequence of
    Newtons Second and Third Laws
  • It applies when there is no net external force on
    a system
  • It allows us to calculate properties of a system
    even when the internal forces are unknown
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