GCSE

Physics

  1. Introduction to GCSE Physics (AQA) Coming soon
  2. 1. Energy

  3. 1.1 Energy Stores, Transfers and Power
  4. 1.2 Conservation and Dissipation of Energy Coming soon
  5. 1.3 National and Global Energy Resources Coming soon
  6. 2. Electricity
  7. 2.1 Current, Potential Difference and Resistance Coming soon
  8. 2.2 Series and Parallel Circuits Coming soon
  9. 2.3 Domestic Uses and Safety Coming soon
  10. 2.4 Energy Transfers Coming soon
  11. 2.5 Static Electricity Coming soon
  12. 3. Particle Model of Matter
  13. 3.1 Changes of State and the Particle Model Coming soon
  14. 3.2 Internal Energy and Energy Transfers Coming soon
  15. 3.3 Particle Model and Pressure Coming soon
  16. 4. Atomic Structure
  17. 4.1 Atoms and Isotopes Coming soon
  18. 4.2 Atoms and Nuclear Radiation Coming soon
  19. 4.3 Hazards and Uses of Radioactive Emissions and of Background Radiation Coming soon
  20. 4.4 Nuclear Fission and Fusion Coming soon
  21. 5. Forces
  22. 5.1 Forces and their Interactions Coming soon
  23. 5.2 Work Done and Energy Transfer Coming soon
  24. 5.3 Forces and Elasticity Coming soon
  25. 5.4 Moments, Levers and Gears Coming soon
  26. 5.5 Pressure and Pressure Differences in Fluids Coming soon
  27. 5.6 Forces and Motion Coming soon
  28. 5.7 Momentum [HT] Coming soon
  29. 6. Waves
  30. 6.1 Waves in Air, Fluids and Solids Coming soon
  31. 6.2 Electromagnetic Waves Coming soon
  32. 6.3 Black Body Radiation Coming soon
  33. 7. Magnetism and Electromagnetism
  34. 7.1 Permanent and Induced Magnetism, Magnetic Forces and Fields Coming soon
  35. 7.2 The Motor Effect Coming soon
  36. 7.3 Induced Potential, Transformers and the National Grid [HT] Coming soon
  37. 8. Space Physics
  38. 8.1 Solar System; Stability of Orbital Motions; Satellites Coming soon
  39. 8.2 Red-Shift Coming soon
  40. 9. Practical Activities
  41. 9.1 Required Practicals Coming soon
Module Progress
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Learning

In this lesson, we will explore the concept of conservation of momentum, describe examples of momentum in events like collisions, and learn how to perform calculations involving the collision of two objects.

Conservation of Momentum

A fundamental principle is the conservation of momentum, which states that in a closed system, the total momentum before an event is equal to the total momentum after the event. This principle allows us to analyse and predict the outcomes of various events, including collisions. 

A closed system refers to a scenario where no external forces act upon the objects involved, ensuring the conservation of momentum.

Momentum in Events

Collisions:

  • Elastic Collision: In an elastic collision, when two objects collide, they rebound or bounce off each other. The total kinetic energy of the system remains constant before and after the collision. This means that no energy is lost during the collision, and the objects conserve their initial kinetic energy.
  • Inelastic Collision: In an inelastic collision, when two objects collide, they stick together or deform upon impact. Unlike in an elastic collision, the total kinetic energy of the system is not conserved. Some kinetic energy is converted into other forms of energy, such as heat or sound. As a result, the objects lose some of their initial kinetic energy during the collision.

Explosion:

An explosion is a rapid and violent event in which an object or system breaks apart into multiple fragments, often releasing a significant amount of energy.

  • Conservation of Momentum: Despite the chaotic nature of an explosion, the principle of momentum conservation still applies. The total momentum of the system before the explosion is equal to the total momentum after the event. Even though the fragments may move in various directions, their combined momentum remains constant, demonstrating the conservation principle.

Calculations Involving Events

The conservation of momentum can be expressed mathematically using the equation:

Σm₁v₁ = Σm₂v₂

Variables:

  • Σm₁ = Sum of the masses of objects before the event in kilograms, kg
  • Σm₂ = Sum of the masses of objects after the event in kilograms, kg
  • v₁ = Velocity of objects before the event in metres per second, m/s
  • v₂ = Velocity of objects after the event in metres per second, m/s

In simpler terms, the total momentum of all objects involved in the system before the event is equal to the total momentum after the event, emphasising the concept that momentum is conserved during these interactions.

Conclusion

The conservation of momentum is a fundamental principle in physics that helps us understand the behaviour of objects in various events, particularly collisions. By recognising that the total momentum of a closed system remains constant, we can describe and predict the outcomes of such events.

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