GCSE Physics (Triple) Edexcel

This subject is broken down into 69 topics in 7 modules:

  1. Motion, Forces and Conservation of Energy 12 topics
  2. Waves and the Electromagnetic Spectrum 12 topics
  3. Radioactivity and Astronomy 14 topics
  4. Forces and Energy 4 topics
  5. Electricity and Circuits 8 topics
  6. Electric and Magnetic Fields 9 topics
  7. Matter 10 topics
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This page was last modified on 28 September 2024.

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Physics (Triple)

Motion, Forces and Conservation of Energy

Motion and Forces: Distance, Displacement, Speed and Velocity

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Motion and Forces: Distance, Displacement, Speed and Velocity

Distance and Displacement

  • Distance is a scalar quantity that refers to "how much ground an object has covered" during its motion.
  • Displacement, in contrast, is a vector quantity that refers to "how far out of place an object is"; it is the object's overall change in position.
  • Whilst distance refers to the total route travelled, displacement represents the straight line distance in a specific direction from the starting point to the endpoint of a journey.

Calculating Distance and Displacement

  • Distance is calculated by the actual path taken, whereas displacement involves the shortest distance in a specific direction.
  • To calculate displacement you subtract the initial position from the final position.

Speed

  • Speed is a scalar quantity that refers to "how fast an object is moving" or the rate at which an object covers distance.
  • It is usually measured in metres per second (m/s) or kilometres per hour (km/h).
  • Average speed can be calculated using the formula: speed = distance travelled / time taken.

Velocity

  • Velocity is the speed of something in a given direction. It's a vector quantity, meaning it has both magnitude (speed) and direction.
  • Just as with speed, velocity is usually measured in metres per second (m/s) or kilometres per hour (km/h).
  • You can calculate average velocity with the following formula: velocity = displacement / time taken.

Differences between Speed and Velocity

  • Although speed and velocity are often used interchangeably in everyday language, they mean different things scientifically.
  • Speed refers to how fast something is going, but velocity also tells you the direction of the movement.
  • An object's speed can remain constant while its velocity changes (for example if it changes direction), and vice versa.

Graphical Representation of Motion

  • Graphs can be used to represent both speed and velocity; A distance-time graph shows how far an object has travelled at any given moment, whilst a velocity-time graph shows both speed and direction.
  • On a distance-time graph, a horizontal line represents an object not moving. A diagonal line represents a constant speed, and a curved line indicates changing speed.
  • In a velocity-time graph, the gradient of the slope is equal to the acceleration, whilst the area under the graph represents the displacement. The steeper the gradient, the greater the acceleration. A falling gradient signifies deceleration.

Course material for Physics (Triple), module Motion, Forces and Conservation of Energy, topic Motion and Forces: Distance, Displacement, Speed and Velocity

Physics (Triple)

Radioactivity and Astronomy

Astronomy: Red-Shift

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Astronomy: Red-Shift

The Concept of Red-Shift

  • Red-shift is an important concept in astronomy, referring to the increase in wavelength, and subsequent decrease in frequency, of light from distant objects as perceived from an observer's point of view.
  • This phenomenon is a direct application of the Doppler effect, which states that the observed frequency of a wave depends on the relative motion of the source and the observer.
  • When an object moves away from the observer, the light waves from the object get stretched, which means they move towards the red end of the spectrum, hence the name 'Red-shift'.

Interpreting the Red-Shift

  • High-redshift objects in the universe are typically further away. The greater the red-shift, the faster the object is moving away from us. This measurement gives astronomers a way to gauge the speed and direction of distant galaxies.
  • Study of red-shift patterns provide strong evidence for the expansion of the universe, known as Hubble's Law. The law states that the recessional velocity of a galaxy increases with its distance from us, meaning the further away a galaxy is, the faster it is moving away from us.
  • By observing how much the light from an object is red-shifted, astronomers can also estimate the distance of far-flung objects such as galaxies and quasars.

Red-Shift in the Context of the Big Bang Theory

  • The observation of red-shifts in light from distant galaxies is significant evidence in support of the Big Bang theory, which proposes that the universe began from a very high density and high temperature state and has been expanding ever since.
  • The cosmic microwave background radiation - the afterglow of the Big Bang detected in all directions of the universe - also exhibits a red-shift, which corresponds to very high temperatures, as expected from the theory.
  • However, the causes and implications of red-shift along with the age and size of the Universe are continually being researched, as our understanding of the universe continues to refine.

Dangers of Misinterpreting Red-Shift

  • Astronomers must be careful not to mistake red-shift for other forms of light stretching, such as gravitational red-shift, which occurs when light has to 'fight against' gravity to escape an object.
  • An object's motion within a galaxy can also lead to red-shift or blue-shift. This intrinsic shift, as it is known, must be accounted for before the cosmic red-shift can be correctly determined.
  • Red-shift measurements can contain errors, such as those arising from equipment limitations or incorrect assumptions. Validation of red-shift interpretations therefore generally requires other supportive astronomical observations.

Course material for Physics (Triple), module Radioactivity and Astronomy, topic Astronomy: Red-Shift

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