Syllabus
CIE 0625
Expand each topic and subtopic to browse syllabus points and deep-link directly to them.
Topics and syllabus points
1Motion, forces and energy74 total74 mapped
1.1Physical quantities and measurement techniques7 total7 mapped
Core
1.1.1
Describe the use of rulers and measuring cylinders to find a length or a volume
1 lessonMapped in:
1.1.2
Describe how to measure a variety of time intervals using clocks and digital timers
2 lesson s1.1.3
Determine an average value for a small distance and for a short interval of time by measuring multiples (including the period of oscillation of a pendulum)
2 lesson s
Supplement
1.1.4
Understand that a scalar quantity has magnitude (size) only and that a vector quantity has magnitude and direction
1 lesson
1.2Motion13 total13 mapped
Core
1.2.1
Define speed as distance travelled per unit time; recall and use the equation s v = t
1 lesson1.2.2
Define velocity as speed in a given direction
1 lesson1.2.3
Recall and use the equation total distance travelled average speed = total time taken
1 lesson1.2.4
Sketch, plot and interpret distance–time and speed–time graphs
1 lesson1.2.5
Determine, qualitatively, from given data or the shape of a distance–time graph or speed–time graph when an object is: (a) at rest (b) moving with constant speed (c) accelerating (d) decelerating
2 lesson s1.2.6
Calculate speed from the gradient of a straight-line section of a distance–time graph
1 lesson1.2.7
Calculate the area under a speed–time graph to determine the distance travelled for motion with constant speed or constant acceleration
1 lesson
Supplement
1.2.9
Define acceleration as change in velocity per unit time; recall and use the equation ∆v a = ∆t
1 lessonMapped in:
1.2.10
Determine from given data or the shape of a speed–time graph when an object is moving with: (a) constant acceleration (b) changing acceleration
1 lessonMapped in:
1.2.11
Calculate acceleration from the gradient of a speed–time graph
1 lessonMapped in:
1.2.12
Know that a deceleration is a negative acceleration and use this in calculations
1 lessonMapped in:
1.3Mass and weight5 total5 mapped
Core
1.3.1
State that mass is a measure of the quantity of matter in an object at rest relative to the observer
1 lessonMapped in:
1.3.2
State that weight is a gravitational force on an object that has mass
1 lessonMapped in:
1.3.3
Define gravitational field strength as force per unit mass; recall and use the equation W g = m and know that this is equivalent to the acceleration of free fall
2 lesson sMapped in:
1.3.4
Know that weights (and masses) may be compared using a balance
1 lessonMapped in:
Supplement
1.3.5
Describe, and use the concept of, weight as the effect of a gravitational field on a mass
1 lessonMapped in:
1.4Density4 total4 mapped
Core
1.4.1
Define density as mass per unit volume; recall and use the equation m ρ = V
1 lessonMapped in:
1.4.2
Describe how to determine the density of a liquid, of a regularly shaped solid and of an irregularly shaped solid which sinks in a liquid (volume by displacement), including appropriate calculations
1 lessonMapped in:
1.4.3
Determine whether an object floats based on density data
1 lessonMapped in:
Supplement
1.4.4
Determine whether one liquid will float on another liquid based on density data given that the liquids do not mix
1 lessonMapped in:
1.5Forces21 total21 mapped
1.5.1Effects of forces12 total12 mapped
Core
1.5.1.1
Know that forces may produce changes in the size and shape of an object
2 lesson sMapped in:
1.5.1.2
Sketch, plot and interpret load–extension graphs for an elastic solid and describe the associated experimental procedures
1 lessonMapped in:
1.5.1.3
Determine the resultant of two or more forces acting along the same straight line
1 lessonMapped in:
1.5.1.4
Know that an object either remains at rest or continues in a straight line at constant speed unless acted on by a resultant force
1 lessonMapped in:
1.5.1.5
State that a resultant force may change the velocity of an object by changing its direction of motion or its speed
1 lessonMapped in:
Supplement
1.5.1.9
Define the spring constant as force per unit extension; recall and use the equation F k = x
1 lessonMapped in:
1.5.1.10
Define and use the term ‘limit of proportionality’ for a load–extension graph and identify this point on the graph (an understanding of the elastic limit is not required)
1 lessonMapped in:
1.5.1.11
Recall and use the equation F = ma and know that the force and the acceleration are in the same direction
1 lessonMapped in:
1.5.1.12
Describe, qualitatively, motion in a circular path due to a force perpendicular to the motion as: (a) speed increases if force increases, with mass and radius constant (b) radius decreases if force increases, with mass and speed constant (c) an increased mass requires an increased force to keep speed and radius constant mv 2 (F = is not required) r
1 lessonMapped in:
1.5.2Turning effect of forces6 total6 mapped
Core
1.5.2.1
Describe the moment of a force as a measure of its turning effect and give everyday examples
1 lessonMapped in:
1.5.2.2
Define the moment of a force as moment = force × perpendicular distance from the pivot; recall and use this equation
1 lessonMapped in:
1.5.2.3
Apply the principle of moments to situations with one force each side of the pivot, including balancing of a beam
1 lessonMapped in:
1.5.2.4
State that, when there is no resultant force and no resultant moment, an object is in equilibrium
1 lessonMapped in:
Supplement
1.5.3Centre of gravity3 total3 mapped
Core
1.5.3.1
State what is meant by centre of gravity
1 lessonMapped in:
1.5.3.2
Describe an experiment to determine the position of the centre of gravity of an irregularly shaped plane lamina
1 lessonMapped in:
1.5.3.3
Describe, qualitatively, the effect of the position of the centre of gravity on the stability of simple objects
1 lessonMapped in:
1.6Momentum4 total4 mapped
Supplement
1.6.1
Define momentum as mass × velocity; recall and use the equation p = mv
1 lessonMapped in:
1.6.2
Define impulse as force × time for which force acts; recall and use the equation impulse = F∆t = ∆(mv)
1 lessonMapped in:
1.6.3
Apply the principle of the conservation of momentum to solve simple problems in one dimension
1 lessonMapped in:
1.6.4
Define resultant force as the change in momentum per unit time; recall and use the equation ∆p F = ∆t
1 lessonMapped in:
1.7Energy, work and power16 total16 mapped
1.7.1Energy6 total6 mapped
Core
1.7.1.1
State that energy may be stored as kinetic, gravitational potential, chemical, elastic (strain), nuclear, electrostatic and internal (thermal)
1 lessonMapped in:
1.7.1.2
Describe how energy is transferred between stores during events and processes, including examples of transfer by forces (mechanical work done), electrical currents (electrical work done), heating, and by electromagnetic, sound and other waves
1 lessonMapped in:
1.7.1.3
Know the principle of the conservation of energy and apply this principle to simple examples including the interpretation of simple flow diagrams
1 lessonMapped in:
Supplement
1.7.1.4
Recall and use the equation for kinetic energy 1 2 Ek = mv 2
1 lesson1.7.1.5
Recall and use the equation for the change in gravitational potential energy ∆Ep = mg∆h
1 lesson1.7.1.6
Know the principle of the conservation of energy and apply this principle to complex examples involving multiple stages, including the interpretation of Sankey diagrams
1 lessonMapped in:
1.7.2Work2 total2 mapped
1.7.3Energy resources7 total7 mapped
Core
1.7.3.1
Describe how useful energy may be obtained, or electrical power generated, from: (a) chemical energy stored in fossil fuels (b) chemical energy stored in biofuels (c) water, including the energy stored in waves, in tides and in water behind hydroelectric dams (d) geothermal resources (e) nuclear fuel (f) light from the Sun to generate electrical power (solar cells) (g) infrared and other electromagnetic waves from the Sun to heat water (solar panels) and be the source of wind energy including references to a boiler, turbine and generator where they are used
1 lessonMapped in:
1.7.3.2
Describe advantages and disadvantages of each method in terms of renewability, availability, reliability, scale and environmental impact
1 lessonMapped in:
1.7.3.3
Understand, qualitatively, the concept of efficiency of energy transfer
1 lessonMapped in:
Supplement
1.7.3.4
Know that radiation from the Sun is the main source of energy for all our energy resources except geothermal, nuclear and tidal
1 lessonMapped in:
1.7.3.5
Know that energy is released by nuclear fusion in the Sun
1 lessonMapped in:
1.7.3.6
Know that research is being carried out to investigate how energy released by nuclear fusion can be used to produce electrical energy on a large scale
1 lessonMapped in:
1.7.3.7
Define efficiency as: (a) (useful energy output) (%) efficiency = (× 100%) (total energy input) (b) (useful power output) (%) efficiency = (× 100%) (total power input) recall and use these equations
1 lessonMapped in:
1.7.4Power1 total1 mapped
Core
1.7.4.1
Define power as work done per unit time and also as energy transferred per unit time; recall and use the equations W (a) P = t ∆E (b) P = t
1 lessonMapped in:
1.8Pressure4 total4 mapped
Core
1.8.1
Define pressure as force per unit area; recall and use the equation F p = A
1 lessonMapped in:
1.8.2
Describe how pressure varies with force and area in the context of everyday examples
1 lessonMapped in:
1.8.3
Describe, qualitatively, how the pressure beneath the surface of a liquid changes with depth and density of the liquid
1 lessonMapped in:
Supplement
1.8.4
Recall and use the equation for the change in pressure beneath the surface of a liquid ∆p = ρg∆h
1 lessonMapped in:
2Thermal physics45 total45 mapped
2.1Kinetic particle model of matter13 total13 mapped
2.1.1States of matter2 total2 mapped
2.1.2Particle model8 total8 mapped
Core
2.1.2.1
Describe the particle structure of solids, liquids and gases in terms of the arrangement, separation and motion of the particles and represent these states using simple particle diagrams
1 lessonMapped in:
2.1.2.2
Describe the relationship between the motion of particles and temperature, including the idea that there is a lowest possible temperature (−273 °C), known as absolute zero, where the particles have least kinetic energy
1 lesson2.1.2.3
Describe the pressure and the changes in pressure of a gas in terms of the motion of its particles and their collisions with a surface
1 lesson2.1.2.4
Know that the random motion of microscopic particles in a suspension is evidence for the kinetic particle model of matter
1 lessonMapped in:
2.1.2.5
Describe and explain this motion (sometimes known as Brownian motion) in terms of random collisions between the microscopic particles in a suspension and the particles of the gas or liquid
1 lessonMapped in:
Supplement
2.1.2.6
Know that the forces and distances between particles (atoms, molecules, ions and electrons) and the motion of the particles affects the properties of solids, liquids and gases
1 lessonMapped in:
2.1.2.7
Describe the pressure and the changes in pressure of a gas in terms of the forces exerted by particles colliding with surfaces, creating a force per unit area
1 lesson2.1.2.8
Know that microscopic particles may be moved by collisions with light fast-moving molecules and correctly use the terms atoms or molecules as distinct from microscopic particles
1 lessonMapped in:
2.1.3Gases and the absolute scale of temperature3 total3 mapped
Core
2.1.3.1
Describe qualitatively, in terms of particles, the effect on the pressure of a fixed mass of gas of: (a) a change of temperature at constant volume (b) a change of volume at constant temperature
1 lesson2.1.3.2
Convert temperatures between kelvin and degrees Celsius; recall and use the equation T (in K) = θ (in °C) + 273
1 lesson
Supplement
2.1.3.3
Recall and use the equation pV = constant for a fixed mass of gas at constant temperature, including a graphical representation of this relationship
1 lesson
2.2Thermal properties and temperature15 total15 mapped
2.2.1Thermal expansion of solids, liquids and gases3 total3 mapped
Core
Supplement
2.2.1.3
Explain, in terms of the motion and arrangement of particles, the relative order of magnitudes of the expansion of solids, liquids and gases as their temperatures rise
1 lessonMapped in:
2.2.2Specific heat capacity4 total4 mapped
Core
2.2.2.1
Know that a rise in the temperature of an object increases its internal energy
1 lessonMapped in:
Supplement
2.2.2.2
Describe an increase in temperature of an object in terms of an increase in the average kinetic energies of all of the particles in the object
1 lessonMapped in:
2.2.2.3
Define specific heat capacity as the energy required per unit mass per unit temperature increase; recall and use the equation ∆E c = m∆θ
1 lessonMapped in:
2.2.2.4
Describe experiments to measure the specific heat capacity of a solid and a liquid
1 lessonMapped in:
2.2.3Melting, boiling and evaporation8 total8 mapped
Core
2.2.3.1
Describe melting and boiling in terms of energy input without a change in temperature
1 lessonMapped in:
2.2.3.2
Know the melting and boiling temperatures for water at standard atmospheric pressure
1 lessonMapped in:
2.2.3.3
Describe condensation and solidification in terms of particles
1 lessonMapped in:
2.2.3.4
Describe evaporation in terms of the escape of more-energetic particles from the surface of a liquid
1 lessonMapped in:
2.2.3.5
Know that evaporation causes cooling of a liquid
1 lessonMapped in:
Supplement
2.3Transfer of thermal energy17 total17 mapped
2.3.1Conduction4 total4 mapped
Core
2.3.1.1
Describe experiments to demonstrate the properties of good thermal conductors and bad thermal conductors (thermal insulators)
1 lesson
Supplement
2.3.1.2
Describe thermal conduction in all solids in terms of atomic or molecular lattice vibrations and also in terms of the movement of free (delocalised) electrons in metallic conductors
1 lesson2.3.1.3
Describe, in terms of particles, why thermal conduction is bad in gases and most liquids
1 lesson2.3.1.4
Know that there are many solids that conduct thermal energy better than thermal insulators but do so less well than good thermal conductors
1 lesson
2.3.2Convection2 total2 mapped
Core
2.3.3Radiation9 total9 mapped
Core
2.3.3.1
Know that thermal radiation is infrared radiation and that all objects emit this radiation
1 lesson2.3.3.2
Know that thermal energy transfer by thermal radiation does not require a medium
1 lesson2.3.3.3
Describe the effect of surface colour (black or white) and texture (dull or shiny) on the emission, absorption and reflection of infrared radiation
1 lesson
Supplement
2.3.3.4
Know that for an object to be at a constant temperature it needs to transfer energy away from the object at the same rate that it receives energy
1 lesson2.3.3.5
Know what happens to an object if the rate at which it receives energy is less or more than the rate at which it transfers energy away from the object
1 lesson2.3.3.6
Know how the temperature of the Earth is affected by factors controlling the balance between incoming radiation and radiation emitted from the Earth’s surface
1 lesson2.3.3.7
Describe experiments to distinguish between good and bad emitters of infrared radiation
1 lesson2.3.3.8
Describe experiments to distinguish between good and bad absorbers of infrared radiation
1 lesson2.3.3.9
Describe how the rate of emission of radiation depends on the surface temperature and surface area of an object
1 lesson
2.3.4Consequences of thermal energy transfer2 total2 mapped
Core
2.3.4.1
Explain some of the basic everyday applications and consequences of conduction, convection and radiation, including: (a) heating objects such as kitchen pans (b) heating a room by convection
1 lesson
Supplement
2.3.4.2
Explain some of the complex applications and consequences of conduction, convection and radiation where more than one type of thermal energy transfer is significant, including: (a) a fire burning wood or coal (b) a radiator in a car
1 lesson
3Waves56 total56 mapped
3.1General properties of waves10 total10 mapped
Core
3.1.1
Know that waves transfer energy without transferring matter
1 lessonMapped in:
3.1.2
Describe what is meant by wave motion as illustrated by vibrations in ropes and springs, and by experiments using water waves
1 lessonMapped in:
3.1.3
Describe the features of a wave in terms of wavefront, wavelength, frequency, crest (peak), trough, amplitude and wave speed
1 lessonMapped in:
3.1.4
Recall and use the equation for wave speed v = fλ
1 lessonMapped in:
3.1.5
Know that for a transverse wave, the direction of vibration is at right angles to the direction of propagation and understand that electromagnetic radiation, water waves and seismic S-waves (secondary) can be modelled as transverse
1 lessonMapped in:
3.1.6
Know that for a longitudinal wave, the direction of vibration is parallel to the direction of propagation and understand that sound waves and seismic P-waves (primary) can be modelled as longitudinal
1 lessonMapped in:
3.1.7
Describe how waves can undergo: (a) reflection at a plane surface (b) refraction due to a change of speed (c) diffraction through a narrow gap
1 lessonMapped in:
3.1.8
Describe the use of a ripple tank to show: (a) reflection at a plane surface (b) refraction due to a change in speed caused by a change in depth (c) diffraction due to a gap (d) diffraction due to an edge
1 lessonMapped in:
Supplement
3.2Light24 total24 mapped
3.2.1Reflection of light4 total4 mapped
Core
3.2.1.1
Define and use the terms normal, angle of incidence and angle of reflection
1 lessonMapped in:
3.2.1.2
Describe the formation of an optical image by a plane mirror and give its characteristics, i.e. same size, same distance from mirror, virtual
1 lessonMapped in:
3.2.1.3
State that for reflection, the angle of incidence is equal to the angle of reflection; recall and use this relationship
1 lessonMapped in:
Supplement
3.2.1.4
Use simple constructions, measurements and calculations for reflection by plane mirrors
1 lessonMapped in:
3.2.2Refraction of light9 total9 mapped
Core
3.2.2.1
Define and use the terms normal, angle of incidence and angle of refraction
1 lessonMapped in:
3.2.2.2
Describe an experiment to show refraction of light by transparent blocks of different shapes
1 lessonMapped in:
3.2.2.3
Describe the passage of light through a transparent material (limited to the boundaries between two mediums only)
1 lessonMapped in:
3.2.2.4
State the meaning of critical angle
1 lessonMapped in:
3.2.2.5
Describe internal reflection and total internal reflection using both experimental and everyday examples
1 lessonMapped in:
Supplement
3.2.2.6
Define refractive index, n, as the ratio of the speeds of a wave in two different regions
1 lessonMapped in:
3.2.2.7
Recall and use the equation sin i n = sin r
1 lessonMapped in:
3.2.2.8
Recall and use the equation 1 n = sin c
1 lessonMapped in:
3.2.2.9
Describe the use of optical fibres, particularly in telecommunications
1 lessonMapped in:
3.2.3Thin lenses8 total8 mapped
Core
Supplement
3.2.4Dispersion of light3 total3 mapped
Core
Supplement
3.2.4.3
Recall that visible light of a single frequency is described as monochromatic
1 lessonMapped in:
3.3Electromagnetic spectrum10 total10 mapped
Core
3.3.1
Know the main regions of the electromagnetic spectrum in order of frequency and in order of wavelength
1 lessonMapped in:
3.3.2
Know that all electromagnetic waves travel at the same high speed in a vacuum
1 lessonMapped in:
3.3.3
Describe typical uses of the different regions of the electromagnetic spectrum including: (a) radio waves; radio and television transmissions, astronomy, radio frequency identification (RFID) (b) microwaves; satellite television, mobile phones (cell phones), microwave ovens (c) infrared; electric grills, short range communications such as remote controllers for televisions, intruder alarms, thermal imaging, optical fibres (d) visible light; vision, photography, illumination (e) ultraviolet; security marking, detecting fake bank notes, sterilising water (f) X-rays; medical scanning, security scanners (g) gamma rays; sterilising food and medical equipment, detection of cancer and its treatment
1 lessonMapped in:
3.3.4
Describe the harmful effects on people of excessive exposure to electromagnetic radiation, including: (a) microwaves; internal heating of body cells (b) infrared; skin burns (c) ultraviolet; damage to surface cells and eyes, leading to skin cancer and eye conditions (d) X-rays and gamma rays; mutation or damage to cells in the body
1 lessonMapped in:
3.3.5
Know that communication with artificial satellites is mainly by microwaves: (a) some satellite phones use low orbit artificial satellites (b) some satellite phones and direct broadcast satellite television use geostationary satellites
1 lessonMapped in:
Supplement
3.3.6
Know that the speed of electromagnetic waves in a vacuum is 3.0 × 108 m / s and is approximately the same in air
1 lessonMapped in:
3.3.7
Know that many important systems of communications rely on electromagnetic radiation including: (a) mobile phones (cell phones) and wireless internet use microwaves because microwaves can penetrate some walls and only require a short aerial for transmission and reception (b) Bluetooth uses radio waves because radio waves pass through walls but the signal is weakened on doing so (c) optical fibres (visible light or infrared) are used for cable television and high-speed broadband because glass is transparent to visible light and some infrared; visible light and short wavelength infrared can carry high rates of data
1 lessonMapped in:
3.3.8
Know the difference between a digital and analogue signal
1 lessonMapped in:
3.3.9
Know that a sound can be transmitted as a digital or analogue signal
1 lessonMapped in:
3.3.10
Explain the benefits of digital signalling including increased rate of transmission of data and increased range due to accurate signal regeneration
1 lessonMapped in:
3.4Sound12 total12 mapped
Core
Supplement
3.4.11
Know that, in general, sound travels faster in solids than in liquids and faster in liquids than in gases
1 lessonMapped in:
3.4.12
Describe the uses of ultrasound in non- destructive testing of materials, medical scanning of soft tissue and sonar including calculation of depth or distance from time and wave speed
1 lessonMapped in:
4Electricity and magnetism88 total88 mapped
4.1Simple phenomena of magnetism11 total11 mapped
Core
4.1.1
Describe the forces between magnetic poles and between magnets and magnetic materials, including the use of the terms north pole (N pole), south pole (S pole), attraction and repulsion, magnetised and unmagnetised
1 lessonMapped in:
4.1.2
Describe induced magnetism
1 lessonMapped in:
4.1.3
State the differences between the properties of temporary magnets (made of soft iron) and the properties of permanent magnets (made of steel)
1 lessonMapped in:
4.1.4
State the difference between magnetic and non-magnetic materials
1 lessonMapped in:
4.1.5
Describe a magnetic field as a region in which a magnetic pole experiences a force
1 lessonMapped in:
4.1.6
Draw the pattern and direction of magnetic field lines around a bar magnet
1 lessonMapped in:
4.1.7
State that the direction of a magnetic field at a point is the direction of the force on the N pole of a magnet at that point
1 lessonMapped in:
4.1.8
Describe the plotting of magnetic field lines with a compass or iron filings and the use of a compass to determine the direction of the magnetic field
1 lessonMapped in:
4.1.9
Describe the uses of permanent magnets and electromagnets
1 lessonMapped in:
Supplement
4.2Electrical quantities32 total32 mapped
4.2.1Electric charge10 total10 mapped
Core
4.2.1.1
State that there are positive and negative charges
1 lessonMapped in:
4.2.1.2
State that positive charges repel other positive charges, negative charges repel other negative charges, but positive charges attract negative charges
1 lessonMapped in:
4.2.1.3
Describe simple experiments to show the production of electrostatic charges by friction and to show the detection of electrostatic charges
1 lessonMapped in:
4.2.1.4
Explain that charging of solids by friction involves only a transfer of negative charge (electrons)
1 lessonMapped in:
4.2.1.5
Describe an experiment to distinguish between electrical conductors and insulators
1 lessonMapped in:
4.2.1.6
Recall and use a simple electron model to explain the difference between electrical conductors and insulators and give typical examples
1 lessonMapped in:
Supplement
4.2.1.7
State that charge is measured in coulombs
1 lessonMapped in:
4.2.1.8
Describe an electric field as a region in which an electric charge experiences a force
1 lessonMapped in:
4.2.1.9
State that the direction of an electric field at a point is the direction of the force on a positive charge at that point
1 lessonMapped in:
4.2.1.10
Describe simple electric field patterns, including the direction of the field: (a) around a point charge (b) around a charged conducting sphere (c) between two oppositely charged parallel conducting plates (end effects will not be examined)
1 lessonMapped in:
4.2.2Electric current6 total6 mapped
Core
4.2.2.1
Know that electric current is related to the flow of charge
1 lesson4.2.2.2
Describe the use of ammeters (analogue and digital) with different ranges
1 lesson4.2.2.3
Describe electrical conduction in metals in terms of the movement of free electrons
1 lesson4.2.2.4
Know the difference between direct current (d.c.) and alternating current (a.c.)
1 lesson
Supplement
4.2.3Electromotive force and potential difference7 total7 mapped
Core
4.2.3.1
Define electromotive force (e.m.f.) as the electrical work done by a source in moving a unit charge around a complete circuit
1 lesson4.2.3.2
Know that e.m.f. is measured in volts (V)
1 lesson4.2.3.3
Define potential difference (p.d.) as the work done by a unit charge passing through a component
1 lesson4.2.3.4
Know that the p.d. between two points is measured in volts (V)
1 lesson4.2.3.5
Describe the use of voltmeters (analogue and digital) with different ranges
1 lesson
Supplement
4.2.4Resistance5 total5 mapped
Core
4.2.4.1
Recall and use the equation for resistance V R = I
1 lessonMapped in:
4.2.4.2
Describe an experiment to determine resistance using a voltmeter and an ammeter and do the appropriate calculations
1 lessonMapped in:
4.2.4.3
State, qualitatively, the relationship of the resistance of a metallic wire to its length and to its cross-sectional area
1 lessonMapped in:
Supplement
4.2.4.4
Sketch and explain the current–voltage graphs for a resistor of constant resistance, a filament lamp and a diode
1 lessonMapped in:
4.2.4.5
Recall and use the following relationship for a metallic electrical conductor: (a) resistance is directly proportional to length (b) resistance is inversely proportional to cross-sectional area
1 lessonMapped in:
4.2.5Electrical energy and electrical power4 total4 mapped
Core
4.2.5.1
Understand that electric circuits transfer energy from a source of electrical energy, such as an electrical cell or mains supply, to the circuit components and then into the surroundings
1 lessonMapped in:
4.2.5.2
Recall and use the equation for electrical power P = IV
1 lessonMapped in:
4.2.5.3
Recall and use the equation for electrical energy E = IVt
1 lessonMapped in:
4.2.5.4
Define the kilowatt-hour (kW h) and calculate the cost of using electrical appliances where the energy unit is the kW h
1 lessonMapped in:
4.3Electric circuits15 total15 mapped
4.3.1Circuit diagrams and circuit components2 total2 mapped
Core
4.3.1.1
Draw and interpret circuit diagrams containing cells, batteries, power supplies, generators, potential dividers, switches, resistors (fixed and variable), heaters, thermistors (NTC only), light- dependent resistors (LDRs), lamps, motors, bells, ammeters, voltmeters, magnetising coils, transformers, fuses and relays and know how these components behave in the circuit
3 lesson s
Supplement
4.3.1.2
Draw and interpret circuit diagrams containing diodes and light-emitting diodes (LEDs) and know how these components behave in the circuit
1 lessonMapped in:
4.3.2Series and parallel circuits10 total10 mapped
Core
4.3.2.1
Know that the current at every point in a series circuit is the same
1 lessonMapped in:
4.3.2.2
Know how to construct and use series and parallel circuits
1 lessonMapped in:
4.3.2.3
Calculate the combined e.m.f. of several sources in series
1 lessonMapped in:
4.3.2.4
Calculate the combined resistance of two or more resistors in series
1 lessonMapped in:
4.3.2.5
State that, for a parallel circuit, the current from the source is larger than the current in each branch
1 lessonMapped in:
4.3.2.6
State that the combined resistance of two resistors in parallel is less than that of either resistor by itself
1 lessonMapped in:
4.3.2.7
State the advantages of connecting lamps in parallel in a lighting circuit
1 lessonMapped in:
Supplement
4.3.2.8
Recall and use in calculations, the fact that: (a) the sum of the currents entering a junction in a parallel circuit is equal to the sum of the currents that leave the junction (b) the total p.d. across the components in a series circuit is equal to the sum of the individual p.d.s across each component (c) the p.d. across an arrangement of parallel resistances is the same as the p.d. across one branch in the arrangement of the parallel resistances
1 lessonMapped in:
4.3.2.9
Explain that the sum of the currents into a junction is the same as the sum of the currents out of the junction
1 lessonMapped in:
4.3.2.10
Calculate the combined resistance of two resistors in parallel
1 lessonMapped in:
4.3.3Action and use of circuit components3 total3 mapped
Core
4.3.3.1
Know that the p.d. across an electrical conductor increases as its resistance increases for a constant current
1 lessonMapped in:
Supplement
4.4Electrical safety5 total5 mapped
Core
4.4.1
State the hazards of: (a) damaged insulation (b) overheating cables (c) damp conditions (d) excess current from overloading of plugs, extension leads, single and multiple sockets when using a mains supply
1 lessonMapped in:
4.4.2
Know that a mains circuit consists of a live wire (line wire), a neutral wire and an earth wire and explain why a switch must be connected to the live wire for the circuit to be switched off safely
1 lessonMapped in:
4.4.3
Explain the use and operation of trip switches and fuses and choose appropriate fuse ratings and trip switch settings
1 lessonMapped in:
4.4.4
Explain why the outer casing of an electrical appliance must be either non-conducting (double-insulated) or earthed
1 lessonMapped in:
4.4.5
State that a fuse without an earth wire protects the circuit and the cabling for a double- insulated appliance
1 lessonMapped in:
4.5Electromagnetic effects25 total25 mapped
4.5.1Electromagnetic induction5 total5 mapped
Core
4.5.1.1
Know that a conductor moving across a magnetic field or a changing magnetic field linking with a conductor can induce an e.m.f. in the conductor
1 lessonMapped in:
4.5.1.2
Describe an experiment to demonstrate electromagnetic induction
1 lessonMapped in:
4.5.1.3
State the factors affecting the magnitude of an induced e.m.f.
1 lessonMapped in:
Supplement
4.5.2The a.c. generator2 total2 mapped
Supplement
4.5.2.1
Describe a simple form of a.c. generator (rotating coil or rotating magnet) and the use of slip rings and brushes where needed
1 lessonMapped in:
4.5.2.2
Sketch and interpret graphs of e.m.f. against time for simple a.c. generators and relate the position of the generator coil to the peaks, troughs and zeros of the e.m.f.
1 lessonMapped in:
4.5.3Magnetic effect of a current5 total5 mapped
Core
4.5.3.1
Describe the pattern and direction of the magnetic field due to currents in straight wires and in solenoids
1 lessonMapped in:
4.5.3.2
Describe an experiment to identify the pattern of the magnetic field (including direction) due to currents in straight wires and in solenoids
1 lessonMapped in:
4.5.3.3
Describe how the magnetic effect of a current is used in relays and loudspeakers and give examples of their application
1 lessonMapped in:
Supplement
4.5.4Force on a current-carrying conductor3 total3 mapped
Core
4.5.4.1
Describe an experiment to show that a force acts on a current-carrying conductor in a magnetic field, including the effect of reversing: (a) the current (b) the direction of the field
2 lesson s
Supplement
4.5.5The d.c. motor2 total2 mapped
Core
Supplement
4.5.6The transformer8 total8 mapped
Core
4.5.6.1
Describe the construction of a simple transformer with a soft-iron core, as used for voltage transformations
1 lessonMapped in:
4.5.6.2
Use the terms primary, secondary, step-up and step-down
1 lessonMapped in:
4.5.6.3
Recall and use the equation Vp Np Vs = Ns where p and s refer to primary and secondary
1 lessonMapped in:
4.5.6.4
Describe the use of transformers in high- voltage transmission of electricity
1 lessonMapped in:
4.5.6.5
State the advantages of high-voltage transmission
1 lessonMapped in:
Supplement
4.5.6.6
Explain the principle of operation of a simple iron-cored transformer
1 lessonMapped in:
4.5.6.7
Recall and use the equation for 100% efficiency in a transformer IpVp = IsVs where p and s refer to primary and secondary
1 lessonMapped in:
4.5.6.8
Recall and use the equation P = I2R to explain why power losses in cables are smaller when the voltage is greater
1 lessonMapped in:
5Nuclear physics31 total31 mapped
5.1The nuclear model of the atom11 total11 mapped
5.1.1The atom3 total3 mapped
Core
Supplement
5.1.1.3
Describe how the scattering of alpha (α) particles by a sheet of thin metal supports the nuclear model of the atom, by providing evidence for: (a) a very small nucleus surrounded by mostly empty space (b) a nucleus containing most of the mass of the atom (c) a nucleus that is positively charged
1 lessonMapped in:
5.1.2The nucleus8 total8 mapped
Core
5.1.2.1
Describe the composition of the nucleus in terms of protons and neutrons
1 lessonMapped in:
5.1.2.2
State the relative charges of protons, neutrons and electrons as +1, 0 and –1 respectively
1 lessonMapped in:
5.1.2.3
Define the terms proton number (atomic number) Z and nucleon number (mass number) A and be able to calculate the number of neutrons in a nucleus A
1 lessonMapped in:
5.1.2.4
Use the nuclide notation Z X
1 lessonMapped in:
5.1.2.5
Explain what is meant by an isotope and state that an element may have more than one isotope
1 lessonMapped in:
Supplement
5.1.2.6
Describe the processes of nuclear fission and nuclear fusion as the splitting or joining of nuclei, to include the nuclide equation and qualitative description of mass and energy changes without values
1 lessonMapped in:
5.1.2.7
Know the relationship between the proton number and the relative charge on a nucleus
1 lessonMapped in:
5.1.2.8
Know the relationship between the nucleon number and the relative mass of a nucleus
1 lessonMapped in:
5.2Radioactivity20 total20 mapped
5.2.1Detection of radioactivity5 total5 mapped
Core
5.2.1.1
Know what is meant by background radiation
1 lessonMapped in:
5.2.1.2
Know the sources that make a significant contribution to background radiation including: (a) radon gas (in the air) (b) rocks and buildings (c) food and drink (d) cosmic rays
1 lessonMapped in:
5.2.1.3
Know that ionising nuclear radiation can be measured using a detector connected to a counter
1 lessonMapped in:
5.2.1.4
Use count rate measured in counts / s or counts / minute
1 lessonMapped in:
Supplement
5.2.1.5
Use measurements of background radiation to determine a corrected count rate
1 lessonMapped in:
5.2.2The three types of nuclear emission4 total4 mapped
Core
5.2.2.1
Describe the emission of radiation from a nucleus as spontaneous and random in direction
1 lessonMapped in:
5.2.2.2
Identify alpha (α), beta (β) and gamma (γ) emissions from the nucleus by recalling: (a) their nature (b) their relative ionising effects (c) their relative penetrating abilities (β+ are not included, β-particles will be taken to refer to β –)
1 lessonMapped in:
Supplement
5.2.3Radioactive decay5 total5 mapped
Core
5.2.3.1
Know that radioactive decay is a change in an unstable nucleus that can result in the emission of α-particles or β-particles and/or γ-radiation and know that these changes are spontaneous and random
1 lessonMapped in:
5.2.3.2
State that during α-decay or β-decay, the nucleus changes to that of a different element
1 lessonMapped in:
Supplement
5.2.3.3
Know that isotopes of an element may be radioactive due to an excess of neutrons in the nucleus and/or the nucleus being too heavy
1 lessonMapped in:
5.2.3.4
Describe the effect of α-decay, β-decay and γ-emissions on the nucleus, including an increase in stability and a reduction in the number of excess neutrons; the following change in the nucleus occurs during β-emission neutron → proton + electron
1 lessonMapped in:
5.2.3.5
Use decay equations, using nuclide notation, to show the emission of α-particles, β-particles and γ-radiation
1 lessonMapped in:
5.2.4Half-life3 total3 mapped
Core
5.2.4.1
Define the half-life of a particular isotope as the time taken for half the nuclei of that isotope in any sample to decay; recall and use this definition in simple calculations, which might involve information in tables or decay curves (calculations will not include background radiation)
1 lessonMapped in:
Supplement
5.2.4.2
Calculate half-life from data or decay curves from which background radiation has not been subtracted
1 lessonMapped in:
5.2.4.3
Explain how the type of radiation emitted and the half-life of an isotope determine which isotope is used for applications including: (a) household fire (smoke) alarms (b) irradiating food to kill bacteria (c) sterilisation of equipment using gamma rays (d) measuring and controlling thicknesses of materials with the choice of radiations used linked to penetration and absorption (e) diagnosis and treatment of cancer using gamma rays
1 lessonMapped in:
5.2.5Safety precautions3 total3 mapped
Core
Supplement
5.2.5.3
Explain safety precautions for all ionising radiation in terms of reducing exposure time, increasing distance between source and living tissue and using shielding to absorb radiation
1 lessonMapped in:
6Space physics30 total30 mapped
6.1The Earth and the Solar System14 total14 mapped
6.1.1The Earth4 total4 mapped
Core
6.1.1.1
Know that the Earth is a planet that rotates on its axis, which is tilted, once in approximately 24 hours, and use this to explain observations of the apparent daily motion of the Sun and the periodic cycle of day and night
1 lessonMapped in:
6.1.1.2
Know that the Earth orbits the Sun once in approximately 365 days and use this to explain the periodic nature of the seasons
1 lessonMapped in:
6.1.1.3
Know that it takes approximately one month for the Moon to orbit the Earth and use this to explain the periodic nature of the Moon’s cycle of phases
1 lessonMapped in:
Supplement
6.1.1.4
Define average orbital speed from the equation
1 lessonMapped in:
6.1.2The Solar System10 total10 mapped
Core
6.1.2.1
Describe the Solar System as containing: (a) one star, the Sun (b) the eight named planets and know their order from the Sun (c) minor planets that orbit the Sun, including dwarf planets such as Pluto and asteroids in the asteroid belt (d) moons, that orbit the planets (e) smaller Solar System bodies, including comets and natural satellites
1 lessonMapped in:
6.1.2.2
Know that, in comparison to each other, the four planets nearest the Sun are rocky and small and the four planets furthest from the Sun are gaseous and large, and explain this difference by referring to an accretion model for Solar System formation, to include: (a) the model’s dependence on gravity (b) the presence of many elements in interstellar clouds of gas and dust (c) the rotation of material in the cloud and the formation of an accretion disc
1 lessonMapped in:
6.1.2.3
Know that the strength of the gravitational field (a) at the surface of a planet depends on the mass of the planet (b) around a planet decreases as the distance from the planet increases
1 lessonMapped in:
6.1.2.4
Calculate the time it takes light to travel a significant distance such as between objects in the Solar System
1 lessonMapped in:
6.1.2.5
Know that the Sun contains most of the mass of the Solar System and this explains why the planets orbit the Sun
1 lessonMapped in:
6.1.2.6
Know that the force that keeps an object in orbit around the Sun is the gravitational attraction of the Sun
1 lessonMapped in:
Supplement
6.1.2.7
Know that planets, minor planets and comets have elliptical orbits, and recall that the Sun is not at the centre of the elliptical orbit, except when the orbit is approximately circular
1 lessonMapped in:
6.1.2.8
Analyse and interpret planetary data about orbital distance, orbital duration, density, surface temperature and uniform gravitational field strength at the planet’s surface
1 lessonMapped in:
6.1.2.9
Know that the strength of the Sun’s gravitational field decreases and that the orbital speeds of the planets decrease as the distance from the Sun increases
1 lessonMapped in:
6.1.2.10
Know that an object in an elliptical orbit travels faster when closer to the Sun and explain this using the conservation of energy
1 lessonMapped in:
6.2Stars and the Universe16 total16 mapped
6.2.1The Sun as a star2 total2 mapped
Core
6.2.1.1
Know that the Sun is a star of medium size, consisting mostly of hydrogen and helium, and that it radiates most of its energy in the infrared, visible light and ultraviolet regions of the electromagnetic spectrum
1 lessonMapped in:
Supplement
6.2.1.2
Know that stars are powered by nuclear reactions that release energy and that in stable stars the nuclear reactions involve the fusion of hydrogen into helium
1 lessonMapped in:
6.2.2Stars3 total3 mapped
Core
6.2.2.1
State that: (a) galaxies are each made up of many billions of stars (b) the Sun is a star in the galaxy known as the Milky Way (c) other stars that make up the Milky Way are much further away from the Earth than the Sun is from the Earth (d) astronomical distances can be measured in light-years, where one light-year is the distance travelled in (the vacuum of) space by light in one year
1 lessonMapped in:
Supplement
6.2.2.2
Know that one light-year is equal to 9.5 × 1015 m
1 lessonMapped in:
6.2.2.3
Describe the life cycle of a star: (a) a star is formed from interstellar clouds of gas and dust that contain hydrogen (b) a protostar is an interstellar cloud collapsing and increasing in temperature as a result of its internal gravitational attraction (c) a protostar becomes a stable star when the inward force of gravitational attraction is balanced by an outward force due to the high temperature in the centre of the star (d) all stars eventually run out of hydrogen as fuel for the nuclear reaction (e) most stars expand to form red giants and more massive stars expand to form red supergiants when most of the hydrogen in the centre of the star has been converted to helium (f) a red giant from a less massive star forms a planetary nebula with a white dwarf star at its centre (g) a red supergiant explodes as a supernova, forming a nebula containing hydrogen and new heavier elements, leaving behind a neutron star or a black hole at its centre (h) the nebula from a supernova may form new stars with orbiting planets
1 lessonMapped in:
6.2.3The Universe11 total11 mapped
Core
6.2.3.1
Know that the Milky Way is one of many billions of galaxies making up the Universe and that the diameter of the Milky Way is approximately 100 000 light-years
1 lessonMapped in:
6.2.3.2
Describe redshift as an increase in the observed wavelength of electromagnetic radiation emitted from receding stars and galaxies
1 lessonMapped in:
6.2.3.3
Know that the light emitted from distant galaxies appears redshifted in comparison with light emitted on the Earth
1 lessonMapped in:
6.2.3.4
Know that redshift in the light from distant galaxies is evidence that the Universe is expanding and supports the Big Bang Theory
1 lessonMapped in:
Supplement
6.2.3.5
Know that microwave radiation of a specific frequency is observed at all points in space around us and is known as cosmic microwave background radiation (CMBR)
1 lessonMapped in:
6.2.3.6
Explain that the CMBR was produced shortly after the Universe was formed and that this radiation has been expanded into the microwave region of the electromagnetic spectrum as the Universe expanded
1 lessonMapped in:
6.2.3.7
Know that the speed v at which a galaxy is moving away from the Earth can be found from the change in wavelength of the galaxy’s starlight due to redshift
1 lessonMapped in:
6.2.3.8
Know that the distance d of a far galaxy can be determined using the brightness of a supernova in that galaxy
1 lessonMapped in:
6.2.3.9
Define the Hubble constant H0 as the ratio of the speed at which the galaxy is moving away from the Earth to its distance from the Earth; recall and use the equation v H0 = d
1 lessonMapped in:
6.2.3.10
Know that the current estimate for H0 is 2.2 × 10 –18 per second
1 lessonMapped in:
6.2.3.11
Know that the equation d 1 = v H0 represents an estimate for the age of the Universe and that this is evidence for the idea that all the matter in the Universe was present at a single point
1 lessonMapped in: