Year 9 Physics End of Term 3 Assessment Revision

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Practice flashcards covering vocabulary and core concepts for Year 9 Physics Revision, including motion, energy transfers, thermal physics, and states of matter.

Last updated 7:40 PM on 6/2/26
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30 Terms

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Speed

The distance travelled per unit time.

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Velocity

The speed of an object in a given direction.

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Acceleration

The change in velocity per unit time, calculated using the formula a=vuta = \frac{v-u}{t}.

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Acceleration of free fall

A constant acceleration experienced by objects near to the Earth.

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Distance-time graph gradient

The gradient of the line represents the velocity.

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Velocity-time graph gradient

The gradient of the line represents the acceleration.

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Velocity-time graph area

The area under the line represents the distance travelled.

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Kinetic energy store

The energy store associated with moving objects.

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Gravitational potential store

The energy store gained by objects when they are lifted through a gravitational field.

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Elastic potential store

The energy store in objects that are stretched, squashed, or bent.

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Magnetic store

The energy store involving magnetic materials interacting with each other.

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Electrostatic store

The energy store involving objects with charge, such as electrons and protons, interacting with one another.

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Chemical store

The energy store where chemical reactions transfer energy into or away from a substance.

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Nuclear store

The energy store from which atomic nuclei release energy during nuclear reactions.

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Thermal store

The energy store all objects have; the hotter the object, the more energy it has in this store.

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Efficiency

The ratio of the useful energy output to the total energy supplied, often expressed as a percentage: efficiency=useful energy outputtotal energy input×100%\text{efficiency} = \frac{\text{useful energy output}}{\text{total energy input}} \times 100\%.

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Sankey diagrams

Visual representations of energy transfers where the width of arrows shows the proportions of energy transfers taking place.

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Conduction

The transfer of thermal energy in solids and liquids by the vibration of particles.

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Thermal insulators

Poor conductors, usually non-metals, that transfer heat slowly and are used to reduce unwanted energy transfer.

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Convection

The transfer of thermal energy in fluids (liquids and gases) occurring when molecules move from an area of high to low thermal energy.

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Radiation (Thermal)

The transfer of thermal energy by infrared radiation, which is part of the electromagnetic spectrum and does not require a medium.

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Density

The mass per unit volume of a substance, measured in kg/m3kg/m^3, calculated as ρ=mV\rho = \frac{m}{V}.

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Pressure

The force per unit area, measured in Pascals (PaPa), calculated as P=FAP = \frac{F}{A}.

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Pressure in a liquid

The pressure beneath a liquid surface that increases with depth, density, and gravitational field strength, given by p=h×ρ×gp = h \times \rho \times g.

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Specific heat capacity

The amount of energy required to raise the temperature of 1kg1\,kg of a substance by 1C1^{\circ}C, measured in J/kgCJ/kg^{\circ}C.

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Absolute zero

The temperature at which the pressure of a gas is zero, equivalent to 273C-273^{\circ}C or 0K0\,K.

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Kelvin scale

A temperature scale where an increment of one Kelvin is equal to an increment of one degree Celsius, calculated as temperature in Kelvin=temperature in degrees Celsius+273\text{temperature in Kelvin} = \text{temperature in degrees Celsius} + 273.

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Boyle's Law

For a gas at fixed mass and temperature, the pressure multiplied by the volume is constant: P1×V1=P2×V2P_1 \times V_1 = P_2 \times V_2.

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Evaporation

The escape of higher-energy molecules from the surface of a liquid, which lowers the average kinetic energy and temperature of the remaining liquid.

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Boiling

A change of state occurring throughout a liquid only at its boiling point, where molecules gain enough energy to break bonds and become a gas.