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
8.1.3 Orbital Motion, Natural and Artificial Satellites
In this lesson, we will explore the principles of orbital motion, focusing on natural satellites (moons) and artificial satellites. We will examine the similarities and distinctions between these celestial bodies and understand how gravity influences circular orbits and the relationship between velocity, speed, and radius.
Orbital Motion and Gravity
Gravity is the force that keeps celestial bodies (such as planets, moons, and satellites) in orbit around a central object, such as a planet or star. Planets, moons, and satellites are subjectThe person, place, thing, or idea the clause is about; performs or experiences the verb. to the gravitational attraction exerted by the central object they orbit.
Natural Satellites (Moons):
- Moons are natural satellites that orbit planets.
- They are typically much smaller in size compared to their parent planet and follow regular orbits determined by the gravitational pull of the planet.
Artificial Satellites:
- Artificial satellites are human-made objects intentionally placed into orbit around celestial bodies, such as the Earth.
- They serve various purposes, including communication, weather monitoring, navigation, and scientific research.
Circular Orbits and Changing Velocity (HT only)
In a circular orbit, the force of gravity acts as a centripetal force, continuously pulling the object toward the central body. As the object moves along its orbit, the direction of its velocity changes, but the magnitude of its speed remains constant.
Stable Orbits and Changing Radius (HT only)
For a stable orbit, the radius must change if the speed of the object changes. An increase in speed requires a larger radius to counterbalance the increased centripetal force of gravity, while a decrease in speed necessitates a smaller radius.
Conclusion
Orbital motion is governed by the force of gravity, enabling planets, moons, and artificial satellites to maintain their circular orbits. Natural satellites, or moons, orbit planets, while artificial satellites serve various purposes around celestial bodies.
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