Year 8 Physics: Forces, Motion, Light, Magnetism, and the Universe

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Comprehensive vocabulary flashcards covering Year 8 Physics topics: Speed, Forces, Turning Moments, Pressure, Diffusion, Light, Reflection, Refraction, Magnetism, Electromagnets, Galaxies, and Exoplanetary Systems.

52 Terms

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Speed

A measure of how fast an object is moving, calculated using the formula speed=distancetime\text{speed} = \frac{\text{distance}}{\text{time}}, with the standard SI unit of metres per second (m/s\text{m/s}).

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Light Gate

An electronic instrument consisting of a light beam shining onto a light-sensitive switch that automatically starts and stops an electronic timer when an object breaks the beam to measure speed accurately.

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Radar Speed-Trap Gun

A device that emits a beam of radio waves towards a moving vehicle and calculates its speed by measuring the time difference and Doppler shift of the reflected waves.

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Distance-Time Graph

A graph that plots distance on the vertical axis against time on the horizontal axis, where a horizontal section represents a stationary object and the gradient represents speed.

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Velocity

A description of both the speed and the direction of a moving object, such as an aeroplane flying at 900 km/h900\,\text{km/h} due north.

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Balanced Forces

Forces acting on an object that cancel each other out to produce a net resultant force of zero, causing the object to remain at rest or continue moving at a constant speed in a straight line.

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Unbalanced Forces

Forces acting on an object that do not cancel out, producing a non-zero resultant force that causes the object to accelerate, decelerate, or change direction.

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Normal Force

The perpendicular supporting force exerted upward by a surface against an object resting on it, balancing the object's downward weight.

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Upthrust

The upward force exerted by a fluid (such as water) on an object submerged or floating in it, opposing the object's downward weight.

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Plimsoll Line

A legal reference mark on a ship's hull introduced by Samuel Plimsoll in 1876 that indicates the maximum safe water level to prevent overloading in waters of varying density and temperature.

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Bathyscaphe

A deep-ocean exploration craft that floods its air tanks with water to sink and slowly releases iron pellets to reduce weight and rise back to the surface.

<p>A deep-ocean exploration craft that floods its air tanks with water to sink and slowly releases iron pellets to reduce weight and rise back to the surface.</p>
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Lever

A simple machine composed of two arms and a fulcrum that acts as a force multiplier, allowing a small effort applied over a long distance to overcome a large load over a short distance.

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Fulcrum

The fixed support or pivot point about which a lever turns.

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Moment of a Force

The turning effect produced by a force around a fulcrum, calculated by moment=force×distance from the fulcrum\text{moment} = \text{force} \times \text{distance from the fulcrum} and measured in newton metres (Nm\text{Nm}).

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Principle of Moments

The law formulated by Archimedes stating that when an object is in equilibrium, the sum of clockwise moments about any point equals the sum of anti-clockwise moments about that point.

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Pressure

The amount of force exerted per unit area, calculated using the equation P=FAP = \frac{F}{A}.

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Pascal (Pa)

The standard SI unit for pressure, equivalent to one newton per square metre (1 N/m21\,\text{N/m}^2).

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Hydraulic System

A mechanism that utilizes an incompressible liquid to transmit pressure equally in all directions, functioning as a force multiplier in car brakes and hydraulic jacks.

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Atmospheric Pressure

The downward pressure exerted in all directions by the layer of gases surrounding the Earth, measuring approximately 100 000 N/m2100\,000\,\text{N/m}^2 at the surface.

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Eustachian Tube

A tube connecting the throat to the middle ear that opens during swallowing to equalize the air pressure inside the middle ear with the pressure outside.

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Hovercraft

A vehicle that uses fans to force air beneath a flexible skirt, creating a trapped cushion of high-pressure air that lifts it above land or water to reduce friction.

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Diffusion

The process by which particles spread out and intermix from an area of high concentration to an area of low concentration due to their constant random motion.

<p>The process by which particles spread out and intermix from an area of high concentration to an area of low concentration due to their constant random motion.</p>
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Luminous Object

An object that produces and gives out its own light, such as the Sun or a lamp.

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Incident Ray

A beam or ray of light that strikes a reflective or refractive surface.

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Reflected Ray

A ray of light that bounces off a surface after striking it.

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Normal (Optics)

An imaginary line drawn perpendicular (90∘90^\circ) to a surface at the point where a light ray strikes it.

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Law of Reflection

The scientific principle stating that the angle of incidence is equal to the angle of reflection (i=ri = r), with both angles measured from the normal.

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Specular Reflection

Orderly, mirror-like reflection occurring when parallel light rays strike a flat, smooth surface and reflect at identical angles, producing a clear image.

<p>Orderly, mirror-like reflection occurring when parallel light rays strike a flat, smooth surface and reflect at identical angles, producing a clear image.</p>
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Diffuse Reflection

Scattered, irregular reflection occurring when light strikes a rough surface, dispersing the rays in different directions so no clear image is formed.

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Refraction

The bending of a light ray as it passes at an angle from one transparent medium into another, caused by a change in the speed of light.

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Dispersion

The splitting of white light into its constituent spectrum of colours when passing through a prism due to different colours refracting by slightly different amounts.

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Spectrum

The continuous range of constituent colours produced when white light is dispersed, consisting of red, orange, yellow, green, blue, indigo, and violet.

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Ole Rømer

The Danish astronomer (1644–1710) who demonstrated that light has a finite speed by calculating that eclipses of Jupiter's moons occurred earlier when Earth was closer in orbit.

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Armand Fizeau

The French physicist (1819–1896) who measured the speed of light over a distance of 9 km9\,\text{km} using a candle and timed apparatus, calculating a value of 314 262 944 m/s314\,262\,944\,\text{m/s}.

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Primary Colours of Light

The three fundamental colours of light—red, green, and blue—which can be added together in equal intensity to produce white light.

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Colour Subtraction

The process by which a transparent colour filter absorbs all colours of white light except its own colour, which it transmits.

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Magnetic Field

The region around a magnet in which its magnetic force acts on magnetic materials or other magnets.

<p>The region around a magnet in which its magnetic force acts on magnetic materials or other magnets.</p>
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Magnetic Materials

Metals that are attracted to magnets, the primary examples being iron, steel, nickel, and cobalt.

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Lines of Force

Lines that visually represent a magnetic field, pointing from North to South outside a magnet, where closer spacing denotes a stronger magnetic field.

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Electromagnet

A temporary magnet constructed from a coil of wire wrapped around an iron core, which gains magnetism when an electric current flows and loses it when switched off.

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William Gilbert

The English physician and scientist (1544–1603) who experimented with a spherical lodestone model of Earth, demonstrating that Earth acts like a giant magnet.

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Hans Christian Ørsted

The Danish physicist (1777–1851) who discovered electromagnetism in 1820 after observing that an electric current passing along a wire deflected a nearby compass needle.

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Galaxy

A massive gravitational system containing millions or billions of stars, stellar dust, gas, and planetary systems.

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Milky Way

The spiral galaxy containing our Solar System, measuring approximately 100 000 light-years100\,000\,\text{light-years} across and rotating once every 225225 to 250 million years250\,\text{million years}.

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Intergalactic Space

The vast, near-total vacuum situated between galaxies, characterized by an estimated density of only 1 atom1\,\text{atom} of hydrogen per cubic metre (m3\text{m}^3).

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Spiral Galaxy

A pinwheel-shaped galaxy featuring a central bulge and winding outer arms, containing young and old stars, gas, and stellar dust clouds where stars form.

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Elliptical Galaxy

A spherical or elongated football-shaped galaxy lacking spiral arms, composed predominantly of older stars with very little gas and dust.

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Irregular Galaxy

A galaxy with no distinct symmetric shape, rich in dust and gas, often formed by gravitational interactions or collisions between galaxies.

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Exoplanet

A planet that orbits a star located outside of our Solar System.

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Transit Method (The Wink)

An indirect detection technique that identifies exoplanets by measuring the periodic dip in a star's brightness as a planet passes between the star and an observer.

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Habitable Zone (Goldilocks Zone)

The orbital region around a star where the levels of heat and light are suitable for liquid water to exist on a planetary surface.

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Asteroid

A small rocky remnant left over from the formation of the solar system that possesses its own gravity and orbits a star.