GCSE Physics Full Spec Points (double only)

1.01 use the following units: kilogram (kg), metre (m), metre/second (m/s), metre/second^2(m/s^2), newton (N), second (s) and newton/kilogram(N/kg)

1.19 know that the stopping distance of a vehicle is made up of the sum of the thinking distance and the breaking distance

1.20 describe the factors affecting vehicle stopping distance, including speed, mass, road condition and reaction time

1.21 describe the forces acting on falling objects (explain why falling objects reach a terminal velocity)

1.22 practical investigate how extension varies with applied force for helical springs, metal wires and rubber bands

1.23 know the the initial linear region of a force-extension graph is associated with Hooke’s law

1.24 describe elastic behaviour as the ability of a material to recover its original shape after the forces causing the deformation have been removed

2.01 use the following units: ampere (A), coulomb (C), joule (J), ohm (Ω), second (s), volt (V) and watt (W)

2.02 understand how the use of insulation, double insulation, earthing, fuses and circuit breakers protects the device or user in a range of domestic appliances

2.03 understand why a current in a resistor results in the electral transfer of energy and an increase in temperature, and how this can be used in a variety of domestic contexts

2.04 know and use the relationship between power, current and voltage: and apply the relationship to the selection of appropriate fuses

2.05 use the relationship between energy transferred, current, voltage and time: E= I × V × T

2.06 know the difference between mains electricity being alternating current (a.c.) and direct current (d.c.) being supplied by a cell or battery

2.07 explain why a series or parallel circuit is more appropriate for particular applications, including domestic lighting

2.08 understand how the current in a series circuit depends on the applied voltage and the number and nature of other components

2.09 describe how current varies with voltage in wires, resistors, metal filament lamps and diodes, and how to investigate this experimentally

2.10 describe the qualitative effect of changing resistance on the current in a circuit

2.11 describe the qualitative variation of resistance of light-dependent resistors (LDRs) with illumination and thermistors with temperature

2.12 know that lamps and LEDs can be used to indicate the presence of a current in a circuit

2.13 know and use the relationship between voltage, current and resistance: V = I × R

2.14 know that current is the rate of flow of charge

2.15 know and use the relationship between charge, current and time: Q = I × t

2.16 know that electric current in solid metallic conductors is a flow of negatively charged electrons

2.17 understand why current is conserved at a junction in a circuit

2.18 know that the voltage across two components connected in parallel is the same

2.19 calculate the currents, voltages and resistances of two resistive components connected in a series circuit

2.20 know that: voltage is the energy transferred per unit charge passed and the volt is a joule per coulomb

2.21 know and use the relationship between energy transferred, charge and voltage: E = Q × V

2.22 identify common materials which are electrical conductors or insulators, including metals and plastics

2.23 practical: investigate how insulating materials can be charged by friction

2.24 explain how positive and negative electrostatic charges are produced on materials by the loss and gain of electrons

2.25 know that there are forces of attraction between unlike charges and forces of repulsion between like charges

2.26 explain electrostatic phenomena in terms of the movement of electrons

2.27 explain the potential dangers of electrostatic charges, e.g. when fuelling aircraft and tankers

2.28 explain some uses of electrostatic charges, e.g. in photocopiers and inkjet printers

3.01 use the following units: degree (°), hertz (Hz), metre (m), metre/second (m/s) and second (s)

3.02 explain the difference between longitudinal and transverse waves

3.03 know the definitions of amplitude, wavefront, frequency, wavelength and period of a wave

3.04 know that waves transfer energy and information without transferring matter

3.05 know and use the relationship between the speed, frequency and wavelength of a wave: v = f × λ

3.06 use the relationship between frequency and time period: time period x frequency = 1 or f = 1/T

3.07 use the above relationships in different contexts including sound waves and electromagnetic waves

3.08 explain why there is a change in the observed frequency and wavelength of a wave when its source is moving relative to an observer, and that this is known as the Doppler effect

3.09 explain that all waves can be reflected and refracted

3.10 know that light is part of a continuous electromagnetic spectrum that includes radio, microwave, infrared, visible, ultraviolet, x-ray and gamma ray radiations and that all these waves travel at the same speed in free space

3.11 know the order of the electromagnetic spectrum in terms of decreasing wavelength and increasing frequency, including the colours of the visible spectrum

3.12 Explain some of the uses of electromagnetic radiations, including: radio waves: broadcasting and communications, microwaves: cooking and satellite transmissions, infrared: heaters and night vision equipment, visible light: optical fibres and photography, ultraviolet: fluorescent lamps, x-rays: observing the internal structure of objects and materials, including for medical applications, gamma rays: sterilising food and medical equipment.

3.13 explain the detrimental effects of excessive exposure of the human body to electromagnetic waves, including: microwaves: internal heating of body tissue, infrared: skin burns, ultraviolet: damage to surface cells and blindness, gamma rays: cancer, mutation and describe simple protective measures against the risks

3.14 know that light waves are transverse waves and that they can be reflected and refracted

3.15 use the law of reflection (the angle of incidence equals the angle of reflection)

3.16 draw ray diagrams to illustrate reflection and refraction

3.17 practical: investigate the refraction of light, using rectangular blocks, semi-circular blocks and triangular prisms

3.18 know and use the relationship between refractive index, angle of incidence and angle of refraction

3.19 practical: investigate the refractive index of glass, using a glass block

3.20 describe the role of total internal reflection in transmitting information along optical fibres and in prisms

3.21 explain the meaning of critical angle c

3.22 know and use the relationship between critical angle and refractive index:

3.23 know that sound waves are longitudinal waves which can be reflected and refracted

3.24 know that the frequency range for human hearing is 20–20 000 Hz

3.25 practical: investigate the speed of sound in air

3.26 understand how an oscilloscope and microphone can be used to display a sound wave

3.27 practical: investigate the frequency of a sound wave using an oscilloscope

3.28 understand how the pitch of a sound relates to the frequency of vibration of the source

3.29 understand how the loudness of a sound relates to the amplitude of vibration of the source

4.01 use the following units: kilogram (kg), joule (J), metre (m), metre/second (m/s), metre/second2 (m/s2), newton (N), second (s) and watt (W)

4.02 describe energy transfers involving energy stores: energy stores: chemical, kinetic, gravitational, elastic, thermal, magnetic, electrostatic, nuclear and energy transfers: mechanically, electrically, by heating, by radiation (light and sound)

4.03 use the principle of conservation of energy

4.04 know and use the relationship between efficiency, useful energy output and total energy output:

4.05 describe a variety of everyday and scientific devices and situations, explaining the transfer of the input energy in terms of the above relationship, including their representation by Sankey diagrams

4.06 describe how thermal energy transfer may take place by conduction, convection and radiation

4.07 explain the role of convection in everyday phenomena

4.08 explain how emission and absorption of radiation are related to surface and temperature

4.09 practical: investigate thermal energy transfer by conduction, convection and radiation

4.10 explain ways of reducing unwanted energy transfer, such as insulation

4.11 know and use the relationship between work done, force and distance moved in the direction of the force: W = F × d

4.12 know that work done is equal to energy transferred

4.13 know and use the relationship between gravitational potential energy, mass, gravitational field strength and height: GPE = m × g × h

4.14 know and use the relationship: kinetic energy = 1/2×m×v^2

4.15 understand how conservation of energy produces a link between gravitational potential energy, kinetic energy and work

4.16 describe power as the rate of transfer of energy or the rate of doing work

4.17 use the relationship between power, work done (energy transferred) and time taken:

4.18 describe the energy transfers involved in generating electricity using: wind, water, geothermal resources, solar heating systems, solar cells, fossil fuels, nuclear power

4.19 describe the advantages and disadvantages of methods of large-scale electricity production from various renewable and non-renewable resources

5.01 use the following units: degree Celsius (°C), Kelvin (K), joule (J), kilogram (kg), kilogram/metre3 (kg/m3), metre (m), metre2 (m2), metre3 (m3), metre/second (m/s), metre/second2 (m/s2), newton (N) and pascal (Pa)

5.02 use the following unit: joules/kilogram degree Celsius (J/kg °C)

5.03 know and use the relationship between density, mass and volume:

5.04 practical: investigate density using direct measurements of mass and volume

5.05 know and use the relationship between pressure, force and area:

5.06 understand how the pressure at a point in a gas or liquid at rest acts equally in all directions

5.07 know and use the relationship for pressure difference: p = h × ρ × g

5.15 explain how molecules in a gas have random motion and that they exert a force and hence a pressure on the walls of a container

5.16 understand why there is an absolute zero of temperature which is –273 °C

5.17 describe the Kelvin scale of temperature and be able to convert between the Kelvin and Celsius scales

5.18 understand why an increase in temperature results in an increase in the average speed of gas molecules

5.19 know that the Kelvin temperature of a gas is proportional to the average kinetic energy of its molecules

5.20 Explain, for a fixed amount of gas, the qualitative relationship between: pressure and volume at constant temperature, pressure and Kelvin temperature at constant volume.

5.21 use the relationship between the pressure and Kelvin temperature of a fixed mass of gas at constant volume:

5.22 use the relationship between the pressure and volume of a fixed mass of gas at constant temperature:

6.01 use the following units: ampere (A), volt (V) and watt (W)

6.02 know that magnets repel and attract other magnets and attract magnetic substances

6.03 describe the properties of magnetically hard and soft materials

6.04 understand the term magnetic field line

6.05 know that magnetism is induced in some materials when they are placed in a magnetic field

6.06 practical: investigate the magnetic field pattern for a permanent bar magnet and between two bar magnets

6.07 describe how to use two permanent magnets to produce a uniform magnetic field pattern

6.08 know that an electric current in a conductor produces a magnetic field around it

6.12 understand why a force is exerted on a current-carrying wire in a magnetic field, and how this effect is applied in simple d.c. electric motors and loudspeakers

6.13 use the left-hand rule to predict the direction of the resulting force when a wire carries a current perpendicular to a magnetic field

6.14 describe how the force on a current-carrying conductor in a magnetic field changes with the magnitude and direction of the field and current

6.15 know that a voltage is induced in a conductor or a coil when it moves through a magnetic field or when a magnetic field changes through it and describe the factors that affect the size of the induced voltage

6.16 describe the generation of electricity by the rotation of a magnet within a coil of wire and of a coil of wire within a magnetic field, and describe the factors that affect the size of the induced voltage

7.01 use the following units: becquerel (Bq), centimetre (cm), hour (h), minute (min) and second (s)

7.02 describe the structure of an atom in terms of protons, neutrons and electrons and use symbols such as 146C to describe particular nuclei

7.03 know the terms atomic (proton) number, mass (nucleon) number and isotope

7.04 know that alpha (α) particles, beta (β−) particles, and gamma (γ) rays are ionising radiations emitted from unstable nuclei in a random process

7.05 describe the nature of alpha (α) particles, beta (β−) particles, and gamma (γ) rays, and recall that they may be distinguished in terms of penetrating power and ability to ionise

7.06 practical: investigate the penetration powers of different types of radiation using either radioactive sources or simulations

7.07 describe the effects on the atomic and mass numbers of a nucleus of the emission of each of the four main types of radiation (alpha, beta, gamma and neutron radiation)

7.08 understand how to balance nuclear equations in terms of mass and charge

7.09 know that photographic film or a Geiger−Müller detector can detect ionising radiations

7.10 explain the sources of background (ionising) radiation from Earth and space

7.11 know that the activity of a radioactive source decreases over a period of time and is measured in becquerels

7.12 know the definition of the term half-life and understand that it is different for different radioactive isotopes

7.13 use the concept of the half-life to carry out simple calculations on activity, including graphical methods

7.14 describe uses of radioactivity in industry and medicine

7.15 describe the difference between contamination and irradiation

7.16 describe the dangers of ionising radiations, including: that radiation can cause mutations in living organisms, that radiation can damage cells and tissue, the problems arising from the disposal of radioactive waste and how the associated risks can be reduced.

7.17 know that nuclear reactions, including fission, fusion and radioactive decay, can be a source of energy

7.18 understand how a nucleus of U-235 can be split (the process of fission) by collision with a neutron, and that this process releases energy as kinetic energy of the fission products

7.19 know that the fission of U-235 produces two radioactive daughter nuclei and a small number of neutrons

7.20 describe how a chain reaction can be set up if the neutrons produced by one fission strike other U-235 nuclei

7.21 describe the role played by the control rods and moderator in the fission process

7.22 understand the role of shielding around a nuclear reactor

7.23 explain the difference between nuclear fusion and nuclear fission

7.24 describe nuclear fusion as the creation of larger nuclei resulting in a loss of mass from smaller nuclei, accompanied by a release of energy

7.25 know that fusion is the energy source for stars

7.26 explain why nuclear fusion does not happen at low temperatures and pressures, due to electrostatic repulsion of protons

8.01 use the following units: kilogram (kg), metre (m), metre/second (m/s), metre/second2 (m/s2), newton (N), second (s), newton/kilogram (N/kg)

8.02 know that: the universe is a large collection of billions of galaxies, a galaxy is a large collection of billions of stars, our solar system is in the Milky Way galaxy

8.03 understand why gravitational field strength, g, varies and know that it is different on other planets and the Moon from that on the Earth

8.04 explain that gravitational force: causes moons to orbit planets, causes the planets to orbit the Sun, causes artificial satellites to orbit the Earth, causes comets to orbit the Sun

8.05 describe the differences in the orbits of comets, moons and planets

8.06 use the relationship between orbital speed, orbital radius and time period:

8.07 understand how stars can be classified according to their colour

8.08 know that a star’s colour is related to its surface temperature

8.09 describe the evolution of stars of similar mass to the Sun through the following stages: nebula, star (main sequence) , red giant, white dwarf

8.10 describe the evolution of stars with a mass larger than the Sun

8.11 understand how the brightness of a star at a standard distance can be represented using absolute magnitude

8.12 draw the main components of the Hertzsprung–Russell diagram (HR diagram)

8.13 describe the past evolution of the universe and the main arguments in favour of the Big Bang

8.14 describe evidence that supports the Big Bang theory (red-shift and cosmic microwave background (CMB) radiation)

8.15 describe that if a wave source is moving relative to an observer there will be a change in the observed frequency and wavelength

8.16 use the equation relating change in wavelength, wavelength, velocity of a galaxy and the speed of light:

8.17 describe the red-shift in light received from galaxies at different distances away from the Earth

8.18 explain why the red-shift of galaxies provides evidence for the expansion of the universe