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
8.1.1 Our Solar System
In this lesson, we will delve into the components of our solar system, understand its place within the Milky Way galaxy, and explore the formation and life cycle of the Sun.
Components of Our Solar System
Our solar system is a fascinating part of the universe, comprising the Sun, eight planets, numerous moons, and other celestial bodies.
The Sun:
- The Sun is the only star of our solar system, providing light, heat, and energy to the planets and other celestial bodies.
- It accounts for the majority of the mass in the solar system.
Planets:
- There are eight planets in our solar system, including Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.
- These planets orbit the Sun and have distinctive characteristics, such as size, composition, and atmosphere.
Dwarf Planets and Moons:
- In addition to the eight planets, our solar system is home to dwarf planets, such as Pluto, Ceres, and Eris.
- Moons, natural satellites that orbit planets, are also integral parts of our solar system. Examples include Earth's Moon and Jupiter's moon, Europa.
Our Solar System in the Milky Way Galaxy
The Milky Way galaxy is a vast collection of stars, gas, and dust, of which our solar system is a tiny part. Our solar system resides within one of the galaxy's spiral arms, known as the Orion Arm or Local Spur.
Formation of the Sun
- The Sun and other stars are formed from vast clouds of dust and gas called nebulae.
- The force of gravity causes the dust and gas to collapse and come together, forming a dense core known as a protostar.
- As the protostar continues to accumulate mass, the pressure and temperature at its core become sufficient for nuclear fusionNuclear fusion is a reaction in which two or more atomic nuclei, combine to form one or more atomic nuclei and neutrons. to occur.
Life Cycle of a Star
- Fusion reactions within the core of a star, like the Sun, generate immense amounts of energy.
- This energy creates an equilibrium between the gravitational collapse of the star and the outward pressure from the fusion reactions.
- Throughout its life cycle, a star undergoes various stages, such as the main sequence, red giant, and eventually, either a white dwarf, neutron star, or supernova, depending on its mass.
Conclusion
Our solar system, consisting of the Sun, planets, moons, and other celestial bodies, is a mesmerising part of the Milky Way galaxy. The formation of the Sun from a cloud of dust and gas, and its ongoing fusion reactions, sustain the balance between gravitational collapse and fusion energy.
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