iGCSE Physics (Triple) CAIE

This subject is broken down into 70 topics in 7 modules:

  1. Astrophysics 15 topics
  2. General Physics 14 topics
  3. Space Physics 12 topics
  4. Thermal Physics 8 topics
  5. Properties of Waves, Including Light and Sound 6 topics
  6. Electricity and Magnetism 10 topics
  7. Atomic Physics 5 topics
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  • 7
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  • 70
    topics
  • 27,586
    words of revision content
  • 3+
    hours of audio lessons

This page was last modified on 28 September 2024.

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Physics (Triple)

Space Physics

Introduction to Astronomy

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Introduction to Astronomy

The Solar System

  • The solar system consists of our sun, eight planets with their moons, dwarfs planets, asteroids, comets, and other celestial bodies.
  • The planets are orbiting around the sun in paths known as elliptical orbits.
  • The four inner planets (Mercury, Venus, Earth, Mars) also referred to as terrestrial planets, are made primarily of rock and metal.
  • The four outer planets (Jupiter, Saturn, Uranus, Neptune), called gas giants and ice giants, are composed largely of gases and hold numerous moons.

Stars and Galaxies

  • A star, like the Sun, is a hot sphere of gas that emits light and energy generated through nuclear reactions.
  • Stars of different sizes, ages and temperatures have different colours. The hottest stars are white or blue, while the cooler stars are red.
  • All the stars we see at night are located in our own galaxy, the Milky Way.
  • There are billions of galaxies in the Universe, some of which are spiral-shaped like the Milky Way, while others are elliptical or irregular in shape.

The Universe

  • The universe is the entirety of space and time, and all matter and energy in it.
  • The universe is believed to have originated around 13.8 billion years ago in the Big Bang.
  • The universe has been expanding since its formation, a concept known as the expanding universe theory.
  • Dark matter is hypothesised to make up about 85% of the matter in the universe.
  • Dark energy, a mysterious form of energy, is thought to be responsible for the acceleration in the expansion of the universe.

Observational Astronomy

  • Telescopes are used to observe distant objects in space, with some collecting visible light and others collecting different types of electromagnetic radiation.
  • Radio astronomy uses large antennas to detect radio waves from space.
  • Space probes are robotic spacecraft sent away from Earth to explore other planets and celestial bodies up close.

Key Astronomers

  • Nicolaus Copernicus first proposed that the Earth revolves around the sun, contradicting the long-held belief that Earth was the centre of the Universe.
  • Galileo Galilei is known for improvements to the telescope that enabled detailed observations of the planets, leading him to support Copernicus's model.
  • Edwin Hubble discovered that there are many galaxies outside the Milky Way and provided substantial evidence of the expanding universe.

Course material for Physics (Triple), module Space Physics, topic Introduction to Astronomy

Physics (Triple)

General Physics

Work Done

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Work Done

Understanding Work Done

  • The concept of work done is used to explain the transfer of energy when a force acts on an object and moves it.
  • Work done, or work, is calculated using the formula: work done = force x distance.
  • Therefore, work is only done when an object moves.
  • The unit of work done is the Joule (J).

Work Done on an Object

  • When a force is applied to an object and it moves, work is done on the object.
  • If the object does not move, even if force is applied, no work is done.
  • The direction of force and the movement of the object matters. Force and displacement must be in the same direction for work to be done.
  • Work done against the gravitational force is referred to as gravitational work done.

Work Done and Energy Transfers

  • Work done leads to the transfer of energy.
  • Energy can either be transferred from one form to another or transferred to another object.
  • The energy transferred is equivalent to the work done on the object.

Work Done in Lifting Objects

  • Work done in lifting an object is equal to the weight of the object lifted times the distance it's moved vertically. The formula is work done = mgh, where 'm' is mass, 'g' is acceleration due to gravity and 'h' is the height lifted.
  • The work done against gravity is transferred into gravitational potential energy of the object.

Power and Work Done

  • Power is the rate at which work is done or energy is transferred.
  • Work done per unit of time defines power. Thus, power = work done / time.
  • The unit for power is the watt (W), which is defined as one joule per second.

A deep understanding of the concept of work done will help you to analyse how forces and objects interact with each other. Refer back to this content regularly and ensure you understand the implications of these points on practical scenarios. This will help you feel better prepared for your Physics exam.

Course material for Physics (Triple), module General Physics, topic Work Done

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