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Understanding Collisions and Momentum Conservation
Dec 3, 2024
Lecture Notes: Collisions with Professor Dave
Introduction to Collisions
Definition:
A collision occurs whenever an object in motion comes into contact with another object.
Applications:
This concept applies to pool balls, molecules, asteroids, planets, etc.
Conservation of Linear Momentum
Principle:
In any collision, there must be a conservation of linear momentum.
Types of Collisions:
Different collisions manifest momentum conservation in various ways.
Types of Collisions
Elastic Collisions
Characteristics:
Objects remain separate after collision.
Total kinetic energy and momentum of the system are conserved.
No energy lost as a result of the collision.
Examples:
Pool table balls.
Atomic/molecular collisions in an ideal gas.
Nearly elastic examples: Soccer ball kicked by a player (minimal energy lost to heat and sound).
Perfectly Inelastic Collisions
Characteristics:
Objects collide and move together as a single mass.
Easy momentum analysis: Treat as a single object after collision.
Expression: (m_1v_1 + m_2v_2 = (m_1 + m_2) \times V_{final})
Examples:
Celestial bodies (e.g., asteroids) fusing together.
Car collisions.
Energy Considerations:
Total momentum conserved, but total kinetic energy is not.
Energy conversion into sound, heat, and internal energy._
Inelastic Collisions
Characteristics:
Somewhere between elastic and perfectly inelastic.
Some kinetic energy is lost to collision.
Simplifies mathematical predictions.
Conclusion
Linear Motion Review:
Covered kinematics, dynamics, harmonic motion, and momentum.
Next Topic:
Next session will explore circular motion.
Additional Notes
Contact Information:
For more tutorials, subscribe to the channel or email Professor Dave at
[email protected]
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Support:
Consider supporting on Patreon for continuous content creation.
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Full transcript