University Physics: Comprehensive Notes on Momentum, Collisions, and Impulse
Course Logistics and Upcoming Schedule
Homework Assignments
- The current homework is due on the 3rd (this Sunday) at 5:00 PM.
- If a student feels comfortable with the dynamics questions on the homework, they should feel prepared for the upcoming quiz.
- Submission process: Students should submit the homework by Sunday. The instructor will then send back the solutions, which can be used to study for the quiz on Monday.
- Homework for the new topic, Momentum, will be posted this evening.
Quiz Details
- Quiz 4 is scheduled for the 4th (next Monday).
- The format is very similar to the kinematics quiz: it will consist of four multiple-choice questions with multiple parts.
- It will be graded and returned shortly after.
Midterm Examination
- The midterm is scheduled for the 11th (the Monday after next).
- Unlike the quizzes, the midterm will be free response rather than multiple choice.
- It covers two main topics: Kinematics and Dynamics.
- There will be four questions total, with two questions dedicated to each topic.
- Difficulty: It will be slightly harder and longer than the quizzes, but students will have the entire class time to complete it.
Practice Midterm
- A practice midterm session will be held on the 6th.
- This session replaces the scheduled lab time.
- Attendance is optional/not mandatory.
- The practice exam will be sent out on the 4th for review, and the solutions will be discussed in person on the 6th. Eventually, these solutions will be posted online.
Conservation of Momentum in One Dimension
Conceptual Overview
- Momentum is conserved because, according to Newton's Third Law, if mass 1 (m1) pushes on mass 2 (m2) with a force (F12), mass 2 must push back on mass 1 with an equal and opposite force (F21).
- These internal forces cancel each other out, resulting in a total net force of zero for the system.
- When the net force (Fnet) is zero, total momentum is conserved: Pinitial, total=Pfinal, total.
The Astronaut Scenario
- Two astronauts are initially at rest in space (v1=0, v2=0).
- Given data:
- Mass 1 (m1): 55kg
- Mass 2 (m2): 85kg
- Final velocity of mass 1 (v3): −5m/s (the negative sign indicates movement to the left).
- Conservation Equation:
- m1v1+m2v2=m1v3+m2v4
- Since initial velocities are zero: 0=m1v3+m2v4
- Solving for the final velocity of mass 2 (v4):
- v4=m2−(m1v3)
- v4=85kg−(55kg×−5m/s)
- v4≈3.234m/s
Sanity Check
- It makes sense that m2 has a smaller velocity than m1 because m2 is more massive. Applying the same force to a larger mass results in smaller acceleration/velocity (F=ma).
- In space, when two objects push off each other, the smaller object moves faster and the heavier object moves slower.
Distance Calculation
- To find the total distance between them after 10s:
- Displacement of Mass 1 (ΔdA): −5m/s×10s=−50m
- Displacement of Mass 2 (ΔdB): 3.24m/s×10s=32.4m
- Total distance is the sum of the absolute values: ∣−50∣+∣32.4∣=82.4m.
Types of Collisions
Definition of a Collision
- A collision occurs when two or more objects apply force to each other for a very short period of time (an instant).
Elastic Collisions
- Objects collide and bounce off each other, remaining separated afterward.
- Momentum is conserved: m1v1+m2v2=m1v3+m2v4.
- Example: Bullet passing through a block
- Bullet mass (m1): 22g=22×10−3kg
- Bullet initial velocity (v1): 240m/s
- Block mass (m2): 212kg
- Block initial velocity (v2): 0m/s
- Bullet final velocity (v3): 150m/s
- Solve for final block velocity (v4): v4=m2m1v1−m1v3.
Inelastic Collisions
- Objects collide and stick together, becoming one single mass.
- Momentum is conserved: m1v1+m2v2=(m1+m2)v3.
- Example: Bullet embedded in a block
- Bullet mass (m1): 25g=25×10−3kg
- Bullet initial velocity (v1): 230m/s
- Block (m2) is stationary (v2=0).
- Calculation of system velocity (v3): v3=m1+m2m1v1≈4.04m/s.
- Height Calculation (Post-collision Kinematics)
- Once the bullet-block system has its shared velocity (v3), it may rise to a certain height (Δdy).
- This becomes a kinematics problem using the equation: (vfy)2=(viy)2+2ayΔdy.
- At the maximum height, final velocity in the y-direction is zero (vfy=0).
Conservation of Momentum in Two Dimensions
Principle of Independence
- If the net force in the x and y directions is zero, conservation of momentum occurs in both axes independently.
- During a 2D collision between mass A and mass B, the forces exerted (FAB and FBA) are equal and opposite in magnitude and direction.
- This implies the components are also equal and opposite: FAB,x=−FBA,x and FAB,y=−FBA,y.
Equations for 2D Problem Solving
- X-axis: m1v1x+m2v2x=m1v3x+m2v4x
- Y-axis: m1v1y+m2v2y=m1v3y+m2v4y
Vector Decomposition Example (Pool Balls)
- Ball A (3kg): 5m/s at 30∘ north of east.
- v1x=5cos(30∘)≈4.33m/s
- v1y=5sin(30∘)=2.5m/s
- Ball B (3kg): 4m/s at 140∘ north of east.
- v2x=4cos(140∘)≈−3.06m/s
- v2y=4sin(140∘)≈2.57m/s
- Ball B Final (v4): 3m/s at 80∘.
- v4x=3cos(80∘)≈0.52m/s
- v4y=3sin(80∘)≈2.95m/s
- Solving for Ball A's final velocity (v3):
- Solve the x-momentum equation to find v3x.
- Solve the y-momentum equation to find v3y.
- Combine components using the Pythagorean theorem: v3=(v3x)2+(v3y)2.
- Find direction: θ=tan−1(v3xv3y).
2D Inelastic Collisions
- Objects stick and move with a shared velocity v3 in a specific 2D direction.
- X-momentum: m1v1x+m2v2x=(m1+m2)v3x
- Y-momentum: m1v1y+m2v2y=(m1+m2)v3y
Impulse and Change in Momentum
Definition of Impulse (I)
- Impulse is the change in momentum (ΔP) experienced by a single object.
Formulas for Impulse
- Momentum method: I=ΔP=mvf−mvi
- Force method: Since Fnet=ΔtΔP, then I=Fnet×Δt.
- Here, Δt is the "contact time" describing how long the net force acts on the object.
One-Dimensional Impulse Examples
- Horizontal: A 5kg ball traveling east at 5m/s hits a wall and bounces back at −2m/s.
- I=5(−2)−5(5)=−35kg⋅m/s.
- Vertical (Falling Vase): A 4kg vase is dropped from 15m and stops when hitting the ground.
- Scene 1 (The Fall): Find velocity just before impact (vf1).
- (vf1)2=0+2(−9.8)(−15)
- vf1≈−17.15m/s
- Scene 2 (The Impact): Initial velocity (vi2) = −17.15m/s. Final velocity (vf2) = 0.
- I=m(vf2−vi2)=4(0−(−17.15))=68.6kg⋅m/s.
Force Analysis During Impact
- Net Force Calculation: Using contact time Δt=10ms=10×10−3s.
- Fnet=ΔtI=0.0168.6=6,860N.
- Normal Force Calculation: Fnet is the vector sum of the normal force (Fn) and gravity (Fg).
- Fnet=Fn−Fg⇒Fn=Fnet+mg
- Fn=6860+(4×9.8)=6,899.2N.
- Vase Integrity: If the max force the vase can take is 100N, it will certainly break under 6,899.2N.
Effect of a Cushion
- A cushion increases the contact time (Δt).
- If Δt increases, Fnet decreases even if the total impulse (I) remains the same.
- Example: With a cushion, Fnet≈27.44N and Fn≈67N. In this case, the vase survives because 67\,N < 100\,N.
Impulse in Two Dimensions
Conceptual Model
- Finding impulse in 2D involves calculating the change in momentum for both the x and y components.
- X-impulse: Ix=mvfx−mvix=Fnet,xΔt
- Y-impulse: Iy=mvfy−mviy=Fnet,yΔt
Example: Diagonal Bounce
- A 2kg ball strikes a surface at 3m/s at a 45∘ angle and bounces back at the same speed and angle toward the left.
- Components:
- vix=3cos(45∘)≈2.12m/s
- viy=3sin(45∘)≈2.12m/s
- vfx=−3cos(45∘)≈−2.12m/s
- vfy=3sin(45∘)≈2.12m/s
- Calculated Impulses:
- Ix=2(−2.12−2.12)=−8.48kg⋅m/s
- Iy=2(2.12−2.12)=0kg⋅m/s (the vertical component of velocity remained unchanged).
Questions & Discussion
Student Question: "Where'd you get the four from for the equation?"
Instructor Response: That's the mass (m). The mass of the vase is 4kg.