GCSE
Physics
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Introduction to GCSE Physics (AQA) Coming soon
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1.1 Energy Stores, Transfers and Power
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1.2 Conservation and Dissipation of Energy Coming soon
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1.3 National and Global Energy Resources Coming soon
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2.1 Current, Potential Difference and Resistance Coming soon
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2.2 Series and Parallel Circuits Coming soon
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2.3 Domestic Uses and Safety Coming soon
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2.4 Energy Transfers Coming soon
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2.5 Static Electricity Coming soon
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3.1 Changes of State and the Particle Model Coming soon
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3.2 Internal Energy and Energy Transfers Coming soon
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3.3 Particle Model and Pressure Coming soon
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4.1 Atoms and Isotopes Coming soon
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4.2 Atoms and Nuclear Radiation Coming soon
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4.3 Hazards and Uses of Radioactive Emissions and of Background Radiation Coming soon
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4.4 Nuclear Fission and Fusion Coming soon
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5.1 Forces and their Interactions Coming soon
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5.2 Work Done and Energy Transfer Coming soon
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5.3 Forces and Elasticity Coming soon
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5.4 Moments, Levers and Gears Coming soon
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5.5 Pressure and Pressure Differences in Fluids Coming soon
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5.6 Forces and Motion Coming soon
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5.6.1 Describing Motion Along a Line
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5.6.2 Distance and Displacement
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5.6.3 Speed
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5.6.4 Velocity
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5.6.5 The Distance–Time Relationship
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5.6.6 Acceleration
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5.6.7 Forces, Accelerations and Newton's Laws of Motion
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5.6.8 Newton's First Law
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5.6.9 Newton's Second Law
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5.6.10 Newton's Third Law
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5.6.11 Forces and Braking
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5.6.12 Stopping Distance
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5.6.13 Reaction Time
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5.6.14 Factors Affecting Braking Distance
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5.6.1 Describing Motion Along a Line
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5.7 Momentum [HT] Coming soon
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6.1 Waves in Air, Fluids and Solids Coming soon
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6.2 Electromagnetic Waves Coming soon
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6.3 Black Body Radiation Coming soon
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7.1 Permanent and Induced Magnetism, Magnetic Forces and Fields Coming soon
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7.2 The Motor Effect Coming soon
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7.3 Induced Potential, Transformers and the National Grid [HT] Coming soon
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8.1 Solar System; Stability of Orbital Motions; Satellites Coming soon
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8.2 Red-Shift Coming soon
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9.1 Required Practicals Coming soon
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9.1.1 Required Practical Activity 1
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9.1.2 Required Practical Activity 2
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9.1.3 Required Practical Activity 3
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9.1.4 Required Practical Activity 4
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9.1.5 Required Practical Activity 5
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9.1.6 Required Practical Activity 6
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9.1.7 Required Practical Activity 7
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9.1.8 Required Practical Activity 8
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9.1.9 Required Practical Activity 9
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9.1.10 Required Practical Activity 10
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9.1.1 Required Practical Activity 1
1. Energy
5.7.2 Conservation of Momentum HT
In this lesson, we will explore the concept of conservationThe professional care, preservation, and restoration of archaeological materials and sites, often requiring scientific expertise. 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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