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Subjects

IGCSE Physics

  • 1 Motion, forces and energy
    1.1

    Measurement 测量

    Syllabus
    Core Supplement
    1 Describe the use of rulers and measuring cylinders to find a length or a volume
    2 Describe how to measure a variety of time intervals using clocks and digital timers
    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)
    4 Understand that a scalar quantity has magnitude (size) only and that a vector quantity has magnitude and direction
    5 Know that the following quantities are scalars: distance, speed, time, mass, energy and temperature
    6 Know that the following quantities are vectors: force, weight, velocity, acceleration, momentum, electric field strength and gravitational field strength
    7 Determine, by calculation or graphically, the resultant of two vectors at right angles, limited to forces or velocities only

    Source: Cambridge International syllabus

    Resolving a vector into components

    Length and volume

    Use a ruler 直尺 to measure length. Read the scale with your eye straight in front of the mark to avoid a reading error.

    Lowering an irregular solid into a measuring cylinder; the rise in water level is its volume
    The water an irregular solid pushes up gives its volume
    Reading a measuring cylinder at the bottom of the meniscus, eye level with the mark
    Read a measuring cylinder at the bottom of the meniscus, with your eye level

    Use a measuring cylinder 量筒 to measure the volume of a liquid. Read the scale at the bottom of the curved surface (the meniscus 弯月面), with your eye level with it.

    Measuring small amounts

    A single small length or a short time is hard to measure well. The trick is to measure many and divide 测多个再相除:

    • To find the thickness of one page, measure 100 pages and divide by 100.
    • To find the time for one swing of a pendulum, measure the time for 20 swings and divide by 20. One full swing is called the period 周期.

    This makes the uncertainty 不确定度 (the size of the error) much smaller.

    Scalars and vectors

    A scalar 标量 has size (magnitude 大小) only. A vector 矢量 has size and direction.

    • Scalars: distance, speed, time, mass 质量, energy 能量, temperature 温度.
    • Vectors: force, weight 重力, velocity 速度, acceleration 加速度, momentum 动量.

    To add two vectors at right angles (90°), draw them as two sides of a rectangle. The resultant 合矢量 is the diagonal. Find its size with Pythagoras and its direction with trigonometry.

    $$R = \sqrt{a^2 + b^2}$$
    Two perpendicular vectors drawn as the sides of a rectangle, with the resultant as the diagonal
    Two vectors at right angles add to a resultant $R$, the diagonal of the rectangle
    Explore

    Scalars & vectors

    resultant = a + b

    Add two vectors tip-to-tail to find the resultant.

    Vocabulary Train
    English Chinese Pinyin
    ruler 直尺 zhí chǐ
    measuring cylinder 量筒 liáng tǒng
    meniscus 弯月面 wān yuè miàn
    measure many and divide 测多个再相除 cè duō gè zài xiāng chú
    pendulum bǎi
    period 周期 zhōu qī
    uncertainty 不确定度 bù què dìng dù
    scalar 标量 biāo liàng
    magnitude 大小 dà xiǎo
    vector 矢量 shǐ liàng
    resultant 合矢量 hé shǐ liàng
    mass 质量 zhì liàng
    energy 能量 néng liàng
    temperature 温度 wēn dù
    force
    weight 重力 zhòng lì
    velocity 速度 sù dù
    acceleration 加速度 jiā sù dù
    momentum 动量 dòng liàng
    1.2

    Motion 运动

    Syllabus
    Core Supplement
    1 Define speed as distance travelled per unit time; recall and use the equation
    $$v = \frac{s}{t}$$
    2 Define velocity as speed in a given direction
    3 Recall and use the equation
    $$\text{average speed} = \frac{\text{total distance travelled}}{\text{total time taken}}$$
    9 Define acceleration as change in velocity per unit time; recall and use the equation
    $$a = \frac{\Delta v}{\Delta t}$$
    4 Sketch, plot and interpret distance–time and speed–time graphs
    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 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
    6 Calculate speed from the gradient of a straight-line section of a distance–time graph 11 Calculate acceleration from the gradient of a speed–time graph
    7 Calculate the area under a speed–time graph to determine the distance travelled for motion with constant speed or constant acceleration
    12 Know that a deceleration is a negative acceleration and use this in calculations
    8 State that the acceleration of free fall $g$ for an object near to the surface of the Earth is approximately constant and is approximately $9.8\text{ m/s}^2$ 13 Describe the motion of objects falling in a uniform gravitational field with and without air/ liquid resistance, including reference to terminal velocity

    Source: Cambridge International syllabus

    Speed and velocity

    Speed 速率 is the distance travelled per unit time.

    $$v = \frac{s}{t}$$

    Velocity is speed in a stated direction. So velocity is a vector but speed is a scalar.

    $$\text{average speed} = \frac{\text{total distance}}{\text{total time}}$$

    Acceleration

    Acceleration is the change in velocity per unit time.

    $$a = \frac{\Delta v}{\Delta t}$$

    Here $\Delta v$ means "the change in velocity". A deceleration 减速 (slowing down) is a negative acceleration.

    Worked example. A car speeds up from $8\ \text{m/s}$ to $20\ \text{m/s}$ in $4.0\ \text{s}$. Find its acceleration.

    $$a = \frac{\Delta v}{\Delta t} = \frac{20 - 8}{4.0} = 3.0\ \text{m/s}^2$$

    Motion graphs

    A distance–time graph 距离-时间图 shows how far an object has gone:

    • A flat (horizontal) line means the object is at rest 静止.
    • A straight slope means constant speed. The gradient 斜率 (steepness) is the speed.
    • A curve that gets steeper means the object is speeding up.
    Three distance–time lines: a flat line, a straight slope, and a curve that gets steeper
    The shape of a distance–time line: flat is at rest, a straight slope is constant speed, a rising curve is speeding up

    A speed–time graph 速度-时间图 shows how fast an object is going:

    • A flat line means constant speed.
    • A straight slope means constant acceleration. The gradient is the acceleration.
    • The area under the line 线下面积 is the distance travelled.
    A velocity–time graph with a sloping line whose gradient is the acceleration and whose shaded area is the distance
    On a velocity–time graph the gradient is the acceleration and the area under the line is the distance travelled

    Falling objects

    Near the Earth, all objects speed up as they fall at the same rate. This is the acceleration of free fall 自由落体加速度, $g \approx 9.8\ \text{m/s}^2$.

    When an object falls through air, air resistance 空气阻力 (a drag force) acts upward. As it speeds up, air resistance grows. When air resistance equals the weight, the resultant force is zero and the object stops speeding up. It then falls at a steady terminal velocity 收尾速度.

    A falling object with weight and air resistance arrows, shown just after release and at terminal velocity
    At first the weight is bigger than the air resistance, so the object speeds up; at terminal velocity the two are equal and the speed is steady
    Explore

    Velocity–time graph

    Change u and a. The gradient is the acceleration; the area under the line is the distance travelled.

    Vocabulary Train
    English Chinese Pinyin
    Speed 速率 sù lǜ
    deceleration 减速 jiǎn sù
    distance–time graph 距离-时间图 jù lí - shí jiān tú
    at rest 静止 jìng zhǐ
    gradient 斜率 xié lǜ
    speed–time graph 速度-时间图 sù dù - shí jiān tú
    area under the line 线下面积 xiàn xià miàn jī
    acceleration of free fall 自由落体加速度 zì yóu luò tǐ jiā sù dù
    air resistance 空气阻力 kōng qì zǔ lì
    terminal velocity 收尾速度 shōu wěi sù dù
    motion 运动 yùn dòng
    1.3

    Mass and weight

    Syllabus
    Core Supplement
    1 State that mass is a measure of the quantity of matter in an object at rest relative to the observer
    2 State that weight is a gravitational force on an object that has mass 5 Describe, and use the concept of, weight as the effect of a gravitational field on a mass
    3 Define gravitational field strength as force per unit mass; recall and use the equation
    $$g = \frac{W}{m}$$
    and know that this is equivalent to the acceleration of free fall
    4 Know that weights (and masses) may be compared using a balance

    Source: Cambridge International syllabus

    Mass is the amount of matter 物质 in an object. It is measured in kilograms (kg) and does not change when you move the object.

    Weight is the force of gravity on a mass. It is measured in newtons (N). Weight can change: it is smaller on the Moon because the Moon's gravity is weaker.

    Gravitational field strength 重力场强度 is the force per unit mass:

    $$g = \frac{W}{m}$$

    This $g$ has the same value as the acceleration of free fall ($\approx 9.8\ \text{N/kg}$). You can compare masses with a balance 天平.

    A laboratory balance measures mass; weight is the gravitational force on that mass
    A laboratory balance measures mass; weight is the gravitational force on that mass
    Explore

    Weight and mass

    W = mg

    Weight is proportional to mass — the gradient is the gravitational field strength g (about 10 N/kg on Earth).

    Vocabulary Train
    English Chinese Pinyin
    matter 物质 wù zhì
    Gravitational field strength 重力场强度 zhòng lì chǎng qiáng dù
    balance 天平 tiān píng
    1.4

    Density 密度

    Syllabus
    Core Supplement
    1 Define density as mass per unit volume; recall and use the equation
    $$\rho = \frac{m}{V}$$
    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
    3 Determine whether an object floats based on density data 4 Determine whether one liquid will float on another liquid based on density data given that the liquids do not mix

    Source: Cambridge International syllabus

    Density is the mass per unit volume.

    $$\rho = \frac{m}{V}$$

    The symbol $\rho$ is the Greek letter "rho". The unit is $\text{kg/m}^3$ or $\text{g/cm}^3$.

    To find density: measure the mass with a balance, find the volume, then divide.

    • Regular solid 规则固体 (like a box): measure the sides and calculate the volume.
    • Irregular solid 不规则固体 (a strange shape): lower it into water in a measuring cylinder. The rise in water level is its volume. This is the displacement method 排水法.

    An object floats 漂浮 if its density is less than the density of the liquid. It sinks if its density is greater.

    Worked example. A stone of mass $54\ \text{g}$ is lowered into a measuring cylinder. The water level rises from $20\ \text{cm}^3$ to $40\ \text{cm}^3$. Find the density of the stone.

    The volume of the stone is the rise in water level, $40 - 20 = 20\ \text{cm}^3$, so

    $$\rho = \frac{m}{V} = \frac{54}{20} = 2.7\ \text{g/cm}^3$$
    An iceberg floats with most of its volume hidden: ice is slightly less dense than water
    An iceberg floats with most of its volume hidden: ice is slightly less dense than water
    Explore

    Floating and density

    Change the object's density and the liquid: it floats if it's less dense, and the denser it is the more sits underwater. Iron sinks in water but floats on mercury.

    Vocabulary Train
    English Chinese Pinyin
    Regular solid 规则固体 guī zé gù tǐ
    Irregular solid 不规则固体 bù guī zé gù tǐ
    displacement method 排水法 pái shuǐ fǎ
    floats 漂浮 piāo fú
    density 密度 mì dù
    1.5

    Forces

    Syllabus

    1.5.1 Effects of forces

    Core Supplement
    1 Know that forces may produce changes in the size and shape of an object 9 Define the spring constant as force per unit extension; recall and use the equation
    $$k = \frac{F}{x}$$
    2 Sketch, plot and interpret load–extension graphs for an elastic solid and describe the associated experimental procedures 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)
    3 Determine the resultant of two or more forces acting along the same straight line 11 Recall and use the equation $F = ma$ and know that the force and the acceleration are in the same direction
    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
    5 State that a resultant force may change the velocity of an object by changing its direction of motion or its speed 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 ($F = \frac{mv^2}{r}$ is not required)
    6 Describe solid friction as the force between two surfaces that may impede motion and produce heating
    7 Know that friction (drag) acts on an object moving through a liquid
    8 Know that friction (drag) acts on an object moving through a gas (e.g. air resistance)

    1.5.2 Turning effect of forces

    Core Supplement
    1 Describe the moment of a force as a measure of its turning effect and give everyday examples
    2 Define the moment of a force as $\text{moment} = \text{force} \times \text{perpendicular distance from the pivot}$; recall and use this equation
    3 Apply the principle of moments to situations with one force each side of the pivot, including balancing of a beam 5 Apply the principle of moments to other situations, including those with more than one force each side of the pivot
    4 State that, when there is no resultant force and no resultant moment, an object is in equilibrium 6 Describe an experiment to demonstrate that there is no resultant moment on an object in equilibrium

    1.5.3 Centre of gravity

    Core Supplement
    1 State what is meant by centre of gravity
    2 Describe an experiment to determine the position of the centre of gravity of an irregularly shaped plane lamina
    3 Describe, qualitatively, the effect of the position of the centre of gravity on the stability of simple objects

    Source: Cambridge International syllabus

    The principle of moments
    Hooke's law & the elastic limit

    A force is a push or a pull. A force can change the shape 形状, the speed, or the direction of an object.

    Stretching (Hooke's law)

    When you hang a load on a spring, it stretches. The stretch is called the extension 伸长量.

    On a load–extension graph 载荷-伸长图 the line is straight at first: extension is proportional to load. The point where the line stops being straight is the limit of proportionality 比例极限.

    A load–extension graph: a straight line through the origin that curves away past a marked point
    Load is proportional to extension until the limit of proportionality, then the line curves

    The spring constant 弹簧常数 is the force per unit extension:

    $$k = \frac{F}{x}$$

    A large $k$ means a stiff spring.

    Resultant force and Newton's laws

    Add forces on a straight line to get the resultant force 合力 (forces one way are positive, the other way negative).

    • If the resultant force is zero, the object stays at rest or keeps moving in a straight line at constant speed. (Newton's first law.)
    • If the resultant force is not zero, the object accelerates in the direction of the force:
    $$F = ma$$
    A box on the ground with four labelled force arrows: normal force up, weight down, push right, friction left
    A free-body diagram shows every force on the box as a labelled arrow

    Worked example. A $1200\ \text{kg}$ car has a $3000\ \text{N}$ driving force and $600\ \text{N}$ of friction. Find its acceleration.

    First find the resultant force: $3000 - 600 = 2400\ \text{N}$. Then

    $$a = \frac{F}{m} = \frac{2400}{1200} = 2.0\ \text{m/s}^2$$

    Friction

    Friction 摩擦力 is the force between two surfaces that touch. It tries to stop motion and makes things heat up. Drag (friction in a liquid or gas, like air resistance) also slows objects down.

    Moments — the turning effect

    The moment 力矩 of a force is its turning effect about a pivot 支点.

    $$\text{moment} = \text{force} \times \text{perpendicular distance from the pivot}$$

    The unit is the newton metre (N m).

    Principle of moments 力矩原理: when an object is balanced (in equilibrium 平衡),

    $$\text{total clockwise moment} = \text{total anticlockwise moment}$$

    An object is in equilibrium when there is no resultant force and no resultant moment.

    A beam balanced on a central pivot with a force and distance on each side
    The beam balances when the clockwise moment equals the anticlockwise moment

    Worked example. A $30\ \text{N}$ weight sits $0.20\ \text{m}$ to the left of a pivot. How far to the right must a $20\ \text{N}$ weight sit to balance the beam?

    Balanced, so anticlockwise moment $=$ clockwise moment:

    $$30 \times 0.20 = 20 \times d \quad\Rightarrow\quad d = \frac{6.0}{20} = 0.30\ \text{m}$$

    Centre of gravity

    The centre of gravity 重心 is the single point where all the weight of an object seems to act.

    For a flat shape (lamina 薄片), hang it from a pin and let it settle; draw a vertical line down from the pin using a plumb line. Repeat from another point. The centre of gravity is where the lines cross.

    An object is more stable 稳定 when its centre of gravity is low and its base is wide. It tips over when the centre of gravity passes outside the base.

    Explore

    Forces & Newton's laws

    F = ma (resultant)

    The resultant force sets the acceleration; balanced forces ⇒ none.

    Vocabulary Train
    English Chinese Pinyin
    shape 形状 xíng zhuàng
    extension 伸长量 shēn cháng liàng
    load–extension graph 载荷-伸长图 zài hè - shēn cháng tú
    limit of proportionality 比例极限 bǐ lì jí xiàn
    spring constant 弹簧常数 tán huáng cháng shù
    resultant force 合力 hé lì
    Friction 摩擦力 mó cā lì
    moment 力矩 lì jǔ
    pivot 支点 zhī diǎn
    Principle of moments 力矩原理 lì jǔ yuán lǐ
    equilibrium 平衡 píng héng
    centre of gravity 重心 zhòng xīn
    lamina 薄片 báo piàn
    stable 稳定 wěn dìng
    Exercise sheet
    1.6

    Momentum

    Syllabus
    Core Supplement
    1 Define momentum as mass $\times$ velocity; recall and use the equation $p = mv$
    2 Define impulse as force $\times$ time for which force acts; recall and use the equation $\text{impulse} = F\Delta t = \Delta(mv)$
    3 Apply the principle of the conservation of momentum to solve simple problems in one dimension
    4 Define resultant force as the change in momentum per unit time; recall and use the equation $F = \frac{\Delta p}{\Delta t}$

    Source: Cambridge International syllabus

    Conservation of momentum in a collision

    Momentum is mass times velocity. It is a vector.

    $$p = mv$$

    Impulse 冲量 is the force times the time it acts, and it equals the change in momentum:

    $$\text{impulse} = F\,\Delta t = \Delta(mv)$$

    So the resultant force is the change in momentum per unit time:

    $$F = \frac{\Delta p}{\Delta t}$$

    Conservation of momentum 动量守恒: when objects collide and no outside force acts, the total momentum before equals the total momentum after.

    $$m_1 u_1 + m_2 u_2 = m_1 v_1 + m_2 v_2$$

    (Here $u$ is a velocity before and $v$ is a velocity after.)

    Worked example. A $2.0\ \text{kg}$ trolley moving at $3.0\ \text{m/s}$ hits a stationary $1.0\ \text{kg}$ trolley and they stick together. Find their common velocity afterwards.

    Total momentum is conserved, so

    $$(2.0 \times 3.0) + (1.0 \times 0) = (2.0 + 1.0)\,v \quad\Rightarrow\quad v = \frac{6.0}{3.0} = 2.0\ \text{m/s}$$
    Explore

    Momentum in a collision

    Set the masses and speeds and collide them. Total momentum is conserved.

    Vocabulary Train
    English Chinese Pinyin
    Impulse 冲量 chōng liàng
    Conservation of momentum 动量守恒 dòng liàng shǒu héng
    Exercise sheet
    1.7

    Energy, work and power

    Syllabus

    1.7.1 Energy

    Core Supplement
    1 State that energy may be stored as kinetic, gravitational potential, chemical, elastic (strain), nuclear, electrostatic and internal (thermal)
    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
    4 Recall and use the equation for kinetic energy $E_k = \frac{1}{2}mv^2$
    5 Recall and use the equation for the change in gravitational potential energy $\Delta E_p = mg\Delta h$
    3 Know the principle of the conservation of energy and apply this principle to simple examples including the interpretation of simple flow diagrams 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

    1.7.2 Work

    Core Supplement
    1 Understand that mechanical or electrical work done is equal to the energy transferred
    2 Recall and use the equation for mechanical working $W = Fd = \Delta E$

    1.7.3 Energy resources

    Core Supplement
    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 4 Know that radiation from the Sun is the main source of energy for all our energy resources except geothermal, nuclear and tidal
    2 Describe advantages and disadvantages of each method in terms of renewability, availability, reliability, scale and environmental impact 5 Know that energy is released by nuclear fusion in the Sun
    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
    3 Understand, qualitatively, the concept of efficiency of energy transfer 7 Define efficiency as: (a) $(\%) \text{ efficiency} = \frac{\text{(useful energy output)}}{\text{(total energy input)}} (\times 100\%)$ (b) $(\%) \text{ efficiency} = \frac{\text{(useful power output)}}{\text{(total power input)}} (\times 100\%)$ recall and use these equations

    1.7.4 Power

    Core Supplement
    1 Define power as work done per unit time and also as energy transferred per unit time; recall and use the equations (a) $P = \frac{W}{t}$ (b) $P = \frac{\Delta E}{t}$

    Source: Cambridge International syllabus

    Energy stores

    Energy can be stored 储存 in different ways: kinetic 动能, gravitational potential 重力势能, chemical 化学能, elastic (strain) 弹性势能, nuclear 核能, electrostatic 静电能, and internal (thermal) 内能.

    Energy is transferred 转移 between stores by forces (mechanical work), by electric currents, by heating, and by waves (such as light and sound).

    A row of tall white wind turbines standing in the sea under a blue sky
    Wind turbines transfer energy from the kinetic store of the moving air to electricity

    Kinetic and potential energy

    Kinetic energy is the energy of a moving object:

    $$E_k = \frac{1}{2}mv^2$$

    The change in gravitational potential energy when an object goes up or down by a height $\Delta h$:

    $$\Delta E_p = mg\,\Delta h$$

    Conservation of energy

    The principle of conservation of energy 能量守恒定律 says energy is never made or destroyed; it only moves between stores. A falling object turns gravitational potential energy into kinetic energy. A Sankey diagram 桑基图 shows how the input energy splits into useful energy and wasted 浪费 energy.

    A pendulum shown at its two highest points and its lowest point, with the swing height marked
    Energy moves between gravitational potential energy (at the highest points) and kinetic energy (at the lowest point)
    Roller-coaster cars running down a curved track, with a tall hill behind
    On a roller-coaster, gravitational potential energy stored at the top of the hill becomes kinetic energy as the cars speed down

    Worked example. A $0.50\ \text{kg}$ ball is dropped from a height of $1.8\ \text{m}$. Ignoring air resistance, find its speed just before it lands. (Take $g = 10\ \text{m/s}^2$.)

    All the gravitational potential energy becomes kinetic energy, so $\tfrac{1}{2}mv^2 = mg\,\Delta h$. The mass cancels, leaving $v^2 = 2g\,\Delta h$:

    $$v = \sqrt{2 \times 10 \times 1.8} = \sqrt{36} = 6.0\ \text{m/s}$$

    Because the mass cancels, every object dropped from this height would land at the same speed.

    Work

    Work done 做功 equals the energy transferred. When a force moves an object:

    $$W = Fd = \Delta E$$

    The unit of work and energy is the joule 焦耳 (J).

    Power

    Power 功率 is the work done (or energy transferred) per unit time.

    $$P = \frac{W}{t} = \frac{\Delta E}{t}$$

    The unit is the watt 瓦特 (W). $1\ \text{W} = 1\ \text{J/s}$.

    Efficiency

    Efficiency 效率 tells you how much of the input energy becomes useful energy.

    $$\text{efficiency} = \frac{\text{useful energy output}}{\text{total energy input}} \times 100\%$$

    Efficiency is always less than 100% because some energy is always wasted (usually as heat).

    Worked example. A motor is supplied with $200\ \text{J}$ of electrical energy and lifts a load, giving it $150\ \text{J}$ of gravitational potential energy. Find its efficiency.

    $$\text{efficiency} = \frac{150}{200} \times 100\% = 75\%$$
    A Sankey diagram with a wide input band splitting into a useful band and a wasted band
    A Sankey diagram for this motor: the band widths are proportional to the energy, so the 200 J input splits into 150 J useful and 50 J wasted as heat

    Energy resources

    We generate electricity from many energy resources. Most spin a turbine that drives a generator – often by boiling water to make steam (fossil fuels, nuclear fuel, geothermal, biofuels), or directly by moving water or air (hydroelectric, waves, tides, wind). Solar cells make electricity from sunlight directly; solar panels heat water.

    Resource Renewable? Notes
    fossil fuels (coal, oil, gas) no reliable, high output, but CO₂ and pollution
    nuclear fuel no huge output, no CO₂, but radioactive waste
    biofuels yes roughly carbon-neutral if replanted
    hydroelectric yes reliable, but a dam floods land
    wind yes clean, but intermittent
    solar yes clean, but only in daylight
    geothermal / tidal yes reliable but limited to certain places

    Most of these trace back to the Sun (fossil fuels are ancient stored sunlight; wind and waves come from solar heating) – the exceptions are geothermal, nuclear, and tidal energy. The Sun itself is powered by nuclear fusion 核聚变, joining hydrogen nuclei into helium.

    Explore

    Energy flow & efficiency

    Input energy splits into useful output and wasted energy; efficiency is the useful fraction, and the total is always conserved.

    Explore

    Conservation of energy

    Drop the object: GPE turns into KE, and the total stays the same when there's no friction.

    Vocabulary Train
    English Chinese Pinyin
    stored 储存 chǔ cún
    transferred 转移 zhuǎn yí
    principle of conservation of energy 能量守恒定律 néng liàng shǒu héng dìng lǜ
    Sankey diagram 桑基图 sāng jī tú
    wasted 浪费 làng fèi
    Work done 做功 zuò gōng
    joule 焦耳 jiāo ěr
    Power 功率 gōng lǜ
    watt 瓦特 wǎ tè
    Efficiency 效率 xiào lǜ
    nuclear fusion 核聚变 hé jù biàn
    kinetic 动能 dòng néng
    gravitational potential 重力势能 zhòng lì shì néng
    chemical 化学能 huà xué néng
    elastic (strain) 弹性势能 tán xìng shì néng
    nuclear 核能 hé néng
    electrostatic 静电能 jìng diàn néng
    internal (thermal) 内能 nèi néng
    Exercise sheet
    1.8

    Pressure 压强

    Syllabus
    Core Supplement
    1 Define pressure as force per unit area; recall and use the equation $p = \frac{F}{A}$
    2 Describe how pressure varies with force and area in the context of everyday examples
    3 Describe, qualitatively, how the pressure beneath the surface of a liquid changes with depth and density of the liquid 4 Recall and use the equation for the change in pressure beneath the surface of a liquid $\Delta p = \rho g \Delta h$

    Source: Cambridge International syllabus

    Pressure is the force per unit area.

    $$p = \frac{F}{A}$$

    The unit is the pascal 帕斯卡 (Pa). $1\ \text{Pa} = 1\ \text{N/m}^2$.

    A small area gives a large pressure (a sharp knife cuts well). A large area gives a small pressure (snowshoes stop you sinking).

    Pressure in a liquid

    In a liquid, pressure increases with depth 深度 and with the liquid's density:

    $$\Delta p = \rho g \,\Delta h$$

    This is why a dam is built thicker at the bottom, where the water pressure is greatest. Pressure in a liquid acts in all directions.

    A tank of liquid with arrows pushing outward on the side wall, longer the deeper they are
    The deeper the liquid, the greater the pressure, so the outward push on the wall grows with depth
    The huge curved concrete wall of the Hoover Dam holding back a reservoir
    A real dam is built much thicker at the bottom, because the water pushes hardest where it is deepest

    Worked example. Find the extra pressure at a depth of $2.0\ \text{m}$ in water (density $1000\ \text{kg/m}^3$, $g = 10\ \text{N/kg}$).

    $$\Delta p = \rho g\,\Delta h = 1000 \times 10 \times 2.0 = 20\,000\ \text{Pa}$$
    Explore

    Pressure

    p = ρg·h

    Pressure in a liquid is proportional to depth.

    Vocabulary Train
    English Chinese Pinyin
    pascal 帕斯卡 pà sī kǎ
    depth 深度 shēn dù
    measurement 测量 cè liáng
    pressure 压强 yā qiáng
    Exercise sheet
    1.8

    Exam tips

    • On a distance–time graph the gradient is the speed; on a speed–time graph the gradient is the acceleration and the area under the line is the distance travelled. Never read one graph as if it were the other.
    • Mass (kg) is the amount of matter and is the same everywhere; weight (N) is the force of gravity, $W = mg$. On the Moon your mass is unchanged but your weight is smaller.
    • Speed is a scalar; velocity is a vector. Something moving at steady speed around a curve is still accelerating, because its direction keeps changing.
    • In Hooke's law, load is proportional to extension only up to the limit of proportionality. Use the extension (stretched length − original length), never the whole length.
    • Momentum $p = mv$ is conserved in a collision. Give each velocity a $+$ or $-$ sign for its direction before you add them.
    • Convert units first (cm → m, g → kg). Use $p = F/A$ for a solid pressing on a surface, but $p = \rho g h$ for the pressure inside a liquid — they are different formulas.
  • 2 Thermal physics
    2.1

    States of matter 物态

    Syllabus

    2.1.1 States of matter

    Core Supplement
    1 Know the distinguishing properties of solids, liquids and gases
    2 Know the terms for the changes in state between solids, liquids and gases (gas to solid and solid to gas transfers are not required)

    2.1.2 Particle model

    Core Supplement
    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 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
    2 Describe the relationship between the motion of particles and temperature, including the idea that there is a lowest possible temperature ($-273\,{}^{\circ}\text{C}$), known as absolute zero, where the particles have least kinetic energy
    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 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
    4 Know that the random motion of microscopic particles in a suspension is evidence for the kinetic particle model of matter 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
    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

    2.1.3 Gases and the absolute scale of temperature

    Core Supplement
    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 3 Recall and use the equation $pV = \text{constant}$ for a fixed mass of gas at constant temperature, including a graphical representation of this relationship
    2 Convert temperatures between kelvin and degrees Celsius; recall and use the equation $T\text{ (in K)} = \theta\text{ (in }^{\circ}\text{C)} + 273$

    Source: Cambridge International syllabus

    Kinetic theory: gas pressure

    Matter exists in three states: solid 固体, liquid 液体 and gas 气体.

    State Shape Volume Particles
    Solid fixed fixed close together, in a regular pattern, vibrating
    Liquid takes the shape of the container fixed close together, no pattern, can move past each other
    Gas fills the container changes far apart, fast, random motion

    The changes of state are: melting (solid → liquid), boiling/evaporating (liquid → gas), condensation 凝结 (gas → liquid) and solidification 凝固 (liquid → solid).

    Vocabulary Train
    English Chinese Pinyin
    states of matter 物态 wù tài
    solid 固体 gù tǐ
    liquid 液体 yè tǐ
    gas 气体 qì tǐ
    condensation 凝结 níng jié
    solidification 凝固 níng gù
    Exercise sheet
    2.1

    The kinetic particle model 分子动理论

    All matter is made of tiny particles 粒子 that are always moving. This is the kinetic particle model.

    • In a solid the particles only vibrate 振动 about fixed positions.
    • In a liquid they are still close but can slide past each other.
    • In a gas they are far apart and move quickly in random directions.
    Three boxes of particles: an ordered grid for a solid, a close jumble for a liquid, and a few fast-moving particles for a gas
    The same particles in three states: fixed and ordered in a solid, close but disordered in a liquid, far apart and fast in a gas

    Temperature and particle energy

    When you heat a substance, its particles move faster, so they have more kinetic energy 动能. Temperature 温度 is a measure of the average kinetic energy of the particles.

    The lowest possible temperature is absolute zero 绝对零度, $-273\,{}^{\circ}\text{C}$. At this point the particles have the least possible energy.

    A white digital thermometer with a long metal probe and a small screen, beside its storage case
    A digital thermometer measures temperature by sensing the kinetic energy of the particles it touches

    Gas pressure

    Gas particles hit the walls of their container. Each hit is a tiny push. The pressure 压强 of the gas is the total force of these hits per unit area.

    Gas particles moving in all directions inside a box, striking the walls
    The gas pressure is the total force of countless particle hits on each unit area of the wall
    • Heating a gas (at constant volume) makes particles move faster and hit harder and more often, so the pressure rises.
    • Squeezing a gas into a smaller volume (at constant temperature) means more hits per second on each unit of area, so the pressure rises.

    For a fixed mass of gas at constant temperature:

    $$pV = \text{constant}$$

    So if the volume halves, the pressure doubles.

    A curve of pressure against volume that falls steeply then levels off, with points showing that halving the volume doubles the pressure
    At constant temperature the pressure–volume graph is a curve: halve the volume and the pressure doubles, so $pV$ stays constant

    Worked example. A gas has a volume of $200\ \text{cm}^3$ at a pressure of $100\ \text{kPa}$. It is squeezed to $50\ \text{cm}^3$ at constant temperature. Find the new pressure.

    Since $pV$ stays constant, $p_1 V_1 = p_2 V_2$:

    $$100 \times 200 = p_2 \times 50 \quad\Rightarrow\quad p_2 = \frac{20\,000}{50} = 400\ \text{kPa}$$

    Brownian motion

    If you look at smoke in air under a microscope, you see tiny specks moving in a jerky, random way. This is Brownian motion 布朗运动. The specks are pushed by fast, invisible air particles hitting them. It is strong evidence for the kinetic particle model.

    A large smoke grain on a zig-zag path, surrounded by small fast air particles hitting it
    Random hits from fast air particles push a smoke grain along a jerky, random path

    The kelvin scale

    Scientists often use the kelvin 开尔文 (K) temperature scale, which starts at absolute zero. To convert:

    $$T\text{ (in K)} = \theta\text{ (in }^{\circ}\text{C}) + 273$$

    So $0\,{}^{\circ}\text{C} = 273\ \text{K}$.

    Worked example. Convert $25\,{}^{\circ}\text{C}$ to kelvin, and $200\ \text{K}$ to degrees Celsius.

    $$25 + 273 = 298\ \text{K}, \qquad 200 - 273 = -73\,{}^{\circ}\text{C}$$
    Explore

    Squeeze a gas (Boyle's law)

    Slide the piston in to shrink the volume. The same particles get crammed into less space, so they hit the walls more often and the pressure climbs — while pressure × volume stays constant.

    Vocabulary Train
    English Chinese Pinyin
    kinetic particle model 分子动理论 fèn zǐ dòng lǐ lùn
    particle 粒子 lì zi
    vibrate 振动 zhèn dòng
    kinetic energy 动能 dòng néng
    temperature 温度 wēn dù
    absolute zero 绝对零度 jué duì líng dù
    pressure 压强 yā qiáng
    Brownian motion 布朗运动 bù lǎng yùn dòng
    kelvin 开尔文 kāi ěr wén
    2.2

    Thermal expansion 热膨胀

    Syllabus

    2.2.1 Thermal expansion of solids, liquids and gases

    Core Supplement
    1 Describe, qualitatively, the thermal expansion of solids, liquids and gases at constant pressure 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
    2 Describe some of the everyday applications and consequences of thermal expansion

    2.2.2 Specific heat capacity

    Core Supplement
    1 Know that a rise in the temperature of an object increases its internal energy 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
    3 Define specific heat capacity as the energy required per unit mass per unit temperature increase; recall and use the equation
    $$c = \frac{\Delta E}{m\Delta\theta}$$
    4 Describe experiments to measure the specific heat capacity of a solid and a liquid

    2.2.3 Melting, boiling and evaporation

    Core Supplement
    1 Describe melting and boiling in terms of energy input without a change in temperature 6 Describe the differences between boiling and evaporation
    2 Know the melting and boiling temperatures for water at standard atmospheric pressure
    3 Describe condensation and solidification in terms of particles
    4 Describe evaporation in terms of the escape of more-energetic particles from the surface of a liquid 7 Describe how temperature, surface area and air movement over a surface affect evaporation
    5 Know that evaporation causes cooling of a liquid 8 Explain the cooling of an object in contact with an evaporating liquid

    Source: Cambridge International syllabus

    When matter is heated, its particles move more and take up more space, so the material expands. Gases expand the most, then liquids, then solids.

    Everyday examples: gaps are left between railway lines; bridges sit on rollers; a tight metal lid loosens when heated.

    Two railway rails with a small gap when cool, then expanded and touching when hot
    A small gap is left between rails when cool, so when they expand in the heat the gap closes instead of buckling the track
    Explore

    Heating and specific heat capacity

    Q = mcΔT

    The heat energy needed is proportional to the temperature rise for a given mass of material.

    Vocabulary Train
    English Chinese Pinyin
    thermal expansion 热膨胀 rè péng zhàng
    Exercise sheet
    2.2

    Internal energy and specific heat capacity

    The internal energy 内能 of an object is the total energy of all its particles. Heating an object raises its internal energy and usually its temperature.

    The specific heat capacity 比热容 is the energy needed to raise the temperature of 1 kg of a material by 1 °C.

    $$c = \frac{\Delta E}{m\,\Delta\theta}$$

    A material with a high specific heat capacity (like water) needs a lot of energy to warm up and cools down slowly.

    Worked example. How much energy is needed to heat $2.0\ \text{kg}$ of water from $20\,{}^{\circ}\text{C}$ to $70\,{}^{\circ}\text{C}$? The specific heat capacity of water is $4200\ \text{J/(kg}\,{}^{\circ}\text{C)}$.

    Rearranging $c = \frac{\Delta E}{m\,\Delta\theta}$ gives $\Delta E = mc\,\Delta\theta$, with $\Delta\theta = 70 - 20 = 50\,{}^{\circ}\text{C}$:

    $$\Delta E = 2.0 \times 4200 \times 50 = 420\,000\ \text{J} = 420\ \text{kJ}$$
    Boiling water: internal energy rises with temperature; specific heat capacity is energy per kg per °C
    Boiling water: internal energy rises with temperature; specific heat capacity is energy per kg per °C
    Vocabulary Train
    English Chinese Pinyin
    internal energy 内能 nèi néng
    specific heat capacity 比热容 bǐ rè róng
    2.2

    Melting, boiling and evaporation

    Melting 熔化 and boiling 沸腾 need energy, but the temperature stays the same while the state changes. This energy breaks the forces between particles. For water at normal air pressure, melting is at $0\,{}^{\circ}\text{C}$ and boiling at $100\,{}^{\circ}\text{C}$.

    A heating curve of temperature against time, with flat plateaus during melting and during boiling
    While the substance melts and while it boils the temperature stays flat, even though energy is still being added

    Evaporation 蒸发 is when a liquid changes to a gas at its surface, below the boiling point. The fastest particles escape from the surface. Because the fastest (most energetic) particles leave, the average energy of those left behind falls, so the liquid cools down 冷却.

    Evaporation is faster when the temperature is higher, the surface area is larger, and there is more air movement over the surface.

    Explore

    The heating curve — watch the temperature pause

    While the substance is melting or boiling the temperature stays flat, even though heat is still going in — the energy breaks bonds instead of warming it.

    Vocabulary Train
    English Chinese Pinyin
    melting 熔化 róng huà
    boiling 沸腾 fèi téng
    evaporation 蒸发 zhēng fā
    cools down 冷却 lěng què
    2.3

    Transfer of thermal energy 热能传递

    Syllabus

    2.3.1 Conduction

    Core Supplement
    1 Describe experiments to demonstrate the properties of good thermal conductors and bad thermal conductors (thermal insulators) 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
    3 Describe, in terms of particles, why thermal conduction is bad in gases and most liquids
    4 Know that there are many solids that conduct thermal energy better than thermal insulators but do so less well than good thermal conductors

    2.3.2 Convection

    Core Supplement
    1 Know that convection is an important method of thermal energy transfer in liquids and gases
    2 Explain convection in liquids and gases in terms of density changes and describe experiments to illustrate convection

    2.3.3 Radiation

    Core Supplement
    1 Know that thermal radiation is infrared radiation and that all objects emit this radiation
    2 Know that thermal energy transfer by thermal radiation does not require a medium 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
    3 Describe the effect of surface colour (black or white) and texture (dull or shiny) on the emission, absorption and reflection of infrared radiation 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
    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
    7 Describe experiments to distinguish between good and bad emitters of infrared radiation
    8 Describe experiments to distinguish between good and bad absorbers of infrared radiation
    9 Describe how the rate of emission of radiation depends on the surface temperature and surface area of an object

    2.3.4 Consequences of thermal energy transfer

    Core Supplement
    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 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

    Source: Cambridge International syllabus

    Thermal energy moves from hotter places to colder places in three ways.

    Conduction

    Conduction 热传导 is the transfer of thermal energy through a material without the material moving. Heated particles vibrate more and pass the energy to their neighbours. In metals, free (delocalised) electrons 自由电子 carry energy quickly, so metals are good thermal conductors 热导体.

    Materials that conduct badly (like air, wood and plastic) are thermal insulators 热绝缘体.

    A metal bar heated at one end, its particles vibrating and passing energy toward the cool end
    In conduction the vibrating particles pass energy to their neighbours, so energy flows from the hot end to the cool end

    Convection

    Convection 对流 happens in liquids and gases. When a fluid is heated it expands, becomes less dense, and rises. Cooler, denser fluid sinks to take its place. This circle of moving fluid is a convection current.

    A beaker of water heated from below, with a loop arrow showing hot water rising and cool water sinking
    Heated fluid rises and cooler fluid sinks, setting up a convection current

    Convection cannot happen in a solid because the particles cannot move from place to place.

    Radiation

    Thermal radiation 热辐射 is energy carried by infrared 红外线 waves. All objects emit it, and it needs no material to travel through — it can cross empty space (this is how energy reaches us from the Sun).

    A surface that is dull 暗淡 and black is a good emitter 发射体 and a good absorber 吸收体 of infrared. A surface that is shiny and white is a poor emitter and a good reflector 反射体.

    A dull black surface giving off many infrared waves next to a shiny surface giving off few
    A dull black surface emits (and absorbs) infrared much better than a shiny, white one
    Three pictures of one hand: in ordinary light, then warm and glowing yellow in a thermal camera, then cooler and darker
    A thermal (infrared) camera turns the infrared given off by a warm hand into a picture; brighter means hotter

    An object stays at a constant temperature when it emits energy at the same rate as it absorbs energy. The rate of emission is greater when the surface is hotter and larger.

    Explore

    Heat transfer lab

    Compare the routes by which thermal energy moves.

    Vocabulary Train
    English Chinese Pinyin
    transfer of thermal energy 热能传递 rè néng chuán dì
    conduction 热传导 rè chuán dǎo
    delocalised electrons 自由电子 zì yóu diàn zi
    thermal conductor 热导体 rè dǎo tǐ
    thermal insulator 热绝缘体 rè jué yuán tǐ
    convection 对流 duì liú
    thermal radiation 热辐射 rè fú shè
    infrared 红外线 hóng wài xiàn
    dull 暗淡 àn dàn
    emitter 发射体 fā shè tǐ
    absorber 吸收体 xī shōu tǐ
    reflector 反射体 fǎn shè tǐ
    2.3

    Exam tips

    • In the kinetic particle model, heating a gas makes its particles move faster and hit the walls harder and more often, so the pressure rises. The particles themselves do not get bigger.
    • Evaporation happens only at the surface and at any temperature; boiling happens throughout the liquid at one fixed temperature. Evaporation cools the liquid left behind, because the fastest particles escape.
    • During melting and boiling the temperature stays constant even though energy is still being supplied — that energy breaks the forces between particles.
    • For specific heat capacity use $\Delta E = mc\,\Delta\theta$, where $\Delta\theta$ is the change in temperature, not the final temperature.
    • Dull black surfaces are the best emitters and absorbers of infrared; shiny, light surfaces are the best reflectors. Convection needs a fluid to flow, so it cannot happen in a solid.
  • 3 Waves
    3.1

    General properties of waves

    Syllabus
    Core Supplement
    1 Know that waves transfer energy without transferring matter
    2 Describe what is meant by wave motion as illustrated by vibrations in ropes and springs, and by experiments using water waves
    3 Describe the features of a wave in terms of wavefront, wavelength, frequency, crest (peak), trough, amplitude and wave speed
    4 Recall and use the equation for wave speed $v = f \lambda$
    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
    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
    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 9 Describe how wavelength and gap size affects diffraction through a gap
    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 10 Describe how wavelength affects diffraction at an edge

    Source: Cambridge International syllabus

    Transverse vs longitudinal waves

    A wave carries energy 能量 from place to place without carrying matter. For example, a water wave makes a floating cork bob up and down, but the cork does not travel along with the wave.

    Describing a wave

    • wavefront 波前: a line joining points on a wave that move together (for example, the top of one ripple)
    • wavelength 波长 ($\lambda$): the distance between two neighbouring wavefronts (one full wave)
    • frequency 频率 ($f$): the number of waves passing a point each second, measured in hertz (Hz)
    • crest 波峰 (top) and trough 波谷 (bottom)
    • amplitude 振幅: the largest distance a point moves from its rest position
    • wave speed 波速 ($v$): how fast a wavefront travels
    A wave with the wavelength, amplitude, crest and trough labelled
    The parts of a wave: wavelength, amplitude, crest and trough

    These are linked by the wave equation:

    $$v = f\lambda$$
    A transverse wave with the wavelength, amplitude, crest, trough and direction of travel labelled
    The wavelength is the distance between two crests; the amplitude is the height from the rest position to a crest

    Worked example. A sound wave travels at $340\ \text{m/s}$ and has a frequency of $170\ \text{Hz}$. Find its wavelength.

    Rearranging $v = f\lambda$ gives $\lambda = \dfrac{v}{f}$:

    $$\lambda = \frac{340}{170} = 2.0\ \text{m}$$

    Two types of wave

    • In a transverse wave 横波 the particles vibrate at right angles (90°) to the direction the wave travels (its propagation 传播). Light and water waves are transverse.
    • In a longitudinal wave 纵波 the particles vibrate along the same direction as the wave travels. Sound is longitudinal.
    A transverse wave above a longitudinal wave, showing how the particles move in each
    In a transverse wave the particles vibrate across the travel direction; in a longitudinal wave they vibrate along it, making compressions and rarefactions

    Wave behaviour

    All waves can show three behaviours, which you can see in a ripple tank 波纹水槽:

    • reflection 反射: the wave bounces off a surface.
    • refraction 折射: the wave changes speed (and usually direction) when it enters a different material or depth.
    • diffraction 衍射: the wave spreads out after passing through a gap or around an edge. The spreading is greatest when the gap is about the same size as the wavelength.
    Straight wavefronts reaching a barrier with a narrow gap and spreading into curved wavefronts beyond it
    Plane waves passing through a narrow gap spread out into curved waves — diffraction is strongest when the gap is about one wavelength wide
    Two sets of circular ripples in a water tank overlapping to make a pattern of light and dark lines
    Two dippers in a ripple tank make circular water waves that overlap — a quick way to study how waves behave
    Explore

    Properties of waves

    y = a sin(bx + c)

    A wave: a is amplitude, b sets the wavelength.

    Explore

    Transverse & longitudinal waves

    Flip between a transverse wave (particles bob up and down, like water and light) and a longitudinal one (particles slide back and forth, bunching into compressions, like sound). The wave moves; the particles stay put.

    Explore

    Two waves overlapping

    Change the second wave. Where waves meet they add — sometimes reinforcing, sometimes cancelling.

    Vocabulary Train
    English Chinese Pinyin
    wave
    energy 能量 néng liàng
    wavefront 波前 bō qián
    wavelength 波长 bō cháng
    frequency 频率 pín lǜ
    crest 波峰 bō fēng
    trough 波谷 bō gǔ
    amplitude 振幅 zhèn fú
    wave speed 波速 bō sù
    transverse wave 横波 héng bō
    propagation 传播 chuán bō
    longitudinal wave 纵波 zòng bō
    ripple tank 波纹水槽 bō wén shuǐ cáo
    reflection 反射 fǎn shè
    refraction 折射 zhé shè
    diffraction 衍射 yǎn shè
    Light guāng
    Sound 声音 shēng yīn
    Exercise sheet
    3.2

    Light

    Syllabus

    3.2.1 Reflection of light

    Core Supplement
    1 Define and use the terms normal, angle of incidence and angle of reflection
    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
    3 State that for reflection, the angle of incidence is equal to the angle of reflection; recall and use this relationship 4 Use simple constructions, measurements and calculations for reflection by plane mirrors

    3.2.2 Refraction of light

    Core Supplement
    1 Define and use the terms normal, angle of incidence and angle of refraction
    2 Describe an experiment to show refraction of light by transparent blocks of different shapes 6 Define refractive index, $n$, as the ratio of the speeds of a wave in two different regions
    3 Describe the passage of light through a transparent material (limited to the boundaries between two mediums only) 7 Recall and use the equation
    $$n = \frac{\sin i}{\sin r}$$
    4 State the meaning of critical angle 8 Recall and use the equation
    $$n = \frac{1}{\sin c}$$
    5 Describe internal reflection and total internal reflection using both experimental and everyday examples 9 Describe the use of optical fibres, particularly in telecommunications

    3.2.3 Thin lenses

    Core Supplement
    1 Describe the action of thin converging and thin diverging lenses on a parallel beam of light
    2 Define and use the terms focal length, principal axis and principal focus (focal point)
    3 Draw and use ray diagrams for the formation of a real image by a converging lens 6 Draw and use ray diagrams for the formation of a virtual image by a converging lens
    4 Describe the characteristics of an image using the terms enlarged/same size/diminished, upright/inverted and real/virtual 7 Describe the use of a single lens as a magnifying glass
    5 Know that a virtual image is formed when diverging rays are extrapolated backwards and does not form a visible projection on a screen
    8 Describe the use of converging and diverging lenses to correct long-sightedness and short-sightedness

    3.2.4 Dispersion of light

    Core Supplement
    1 Describe the dispersion of light as illustrated by the refraction of white light by a glass prism
    2 Know the traditional seven colours of the visible spectrum in order of frequency and in order of wavelength 3 Recall that visible light of a single frequency is described as monochromatic

    Source: Cambridge International syllabus

    A converging lens forms an image
    Total internal reflection

    Reflection

    When light hits a mirror, it reflects. We measure angles from the normal 法线 (a line at 90° to the surface).

    The law of reflection: the angle of incidence 入射角 equals the angle of reflection 反射角.

    A plane mirror 平面镜 forms an image that is the same size as the object, the same distance behind the mirror, and virtual (it cannot be caught on a screen).

    An incident ray and a reflected ray meeting at a mirror, with equal angles either side of the normal
    At a plane mirror the angle of incidence $i$ equals the angle of reflection $r$, both measured from the normal

    Refraction

    When light passes from one material into another, it changes speed and bends. The angle in the second material is the angle of refraction 折射角.

    A ray passing from air into glass, bending towards the normal
    Going from air into glass the light slows down and bends towards the normal, so $i > r$

    The refractive index 折射率 $n$ compares the speed of light in the two materials:

    $$n = \frac{\sin i}{\sin r}$$

    Worked example. A ray of light passes from air into glass. The angle of incidence is 60° and the angle of refraction is 35°. Find the refractive index of the glass. (Take $\sin i = 0.87$ and $\sin r = 0.57$.)

    $$n = \frac{\sin i}{\sin r} = \frac{0.87}{0.57} = 1.5$$

    When light tries to leave glass or water and the angle is too large, it cannot get out and instead reflects completely. This is total internal reflection 全反射. It happens when the angle inside is bigger than the critical angle 临界角 $c$:

    $$n = \frac{1}{\sin c}$$
    Two glass blocks: in one the ray refracts out, in the other it is totally internally reflected
    Below the critical angle the light refracts out; above it the light is totally internally reflected

    This effect is used in optical fibres 光纤, thin glass threads that carry light signals for telephones and the internet.

    A bunch of thin fibres held in a hand, each one glowing brightly at its tip in a dark room
    Total internal reflection keeps light bouncing along each fibre until it shines out at the tip

    Lenses

    A converging lens 凸透镜 (fat in the middle) bends parallel rays inwards to a point called the principal focus 焦点. The distance from the lens to this point is the focal length 焦距. A diverging lens 凹透镜 (thin in the middle) spreads rays out.

    Parallel rays passing through a converging lens and meeting at the principal focus
    A converging lens bends parallel rays to meet at the principal focus; the focal length $f$ is the lens-to-focus distance

    A converging lens can form a real image 实像 (rays really meet; can be shown on a screen) or, when the object is very close, a virtual image 虚像 (rays only seem to come from it). Used close to the eye, a converging lens is a magnifying glass 放大镜.

    A hand holding a round convex lens, through which the houses behind appear upside down
    Held away from the eye, a converging lens forms a real image – here the houses behind it appear upside down

    Dispersion

    A glass prism 棱镜 splits white light into the colours of the spectrum 光谱. This splitting is called dispersion 色散.

    A prism splitting a beam of white light into a fan of colours from red to violet
    A prism refracts violet light most and red light least, so white light spreads into a spectrum

    The order of colours is red, orange, yellow, green, blue, indigo, violet. Red light has the longest wavelength and the lowest frequency; violet is the opposite. Light of a single frequency (one pure colour) is monochromatic 单色.

    A narrow beam of white light entering a glass prism and fanning out into a bright band of rainbow colours on a black background
    White light entering a real glass prism spreads into the full spectrum of colours
    Explore

    Bend a light ray

    Shine light into water, glass or diamond and change the angle. The ray slows and bends toward the normal — the denser the material (higher n), the more it bends. That bending is why a straw looks broken in a glass, and why diamonds sparkle.

    Explore

    Image formation by a converging lens

    Trace the three special rays from the object — where they meet is the image. Move the object closer than the focal point to flip it into a magnifying glass.

    Vocabulary Train
    English Chinese Pinyin
    normal 法线 fǎ xiàn
    angle of incidence 入射角 rù shè jiǎo
    angle of reflection 反射角 fǎn shè jiǎo
    plane mirror 平面镜 píng miàn jìng
    angle of refraction 折射角 zhé shè jiǎo
    refractive index 折射率 zhé shè lǜ
    total internal reflection 全反射 quán fǎn shè
    critical angle 临界角 lín jiè jiǎo
    optical fibres 光纤 guāng xiān
    converging lens 凸透镜 tū tòu jìng
    principal focus 焦点 jiāo diǎn
    focal length 焦距 jiāo jù
    diverging lens 凹透镜 āo tòu jìng
    real image 实像 shí xiàng
    virtual image 虚像 xū xiàng
    magnifying glass 放大镜 fàng dà jìng
    prism 棱镜 léng jìng
    spectrum 光谱 guāng pǔ
    dispersion 色散 sè sàn
    monochromatic 单色 dān sè
    Exercise sheet
    3.3

    The electromagnetic spectrum 电磁波谱

    Syllabus
    Core Supplement
    1 Know the main regions of the electromagnetic spectrum in order of frequency and in order of wavelength
    2 Know that all electromagnetic waves travel at the same high speed in a vacuum 6 Know that the speed of electromagnetic waves in a vacuum is $3.0 \times 10^8\text{ m/s}$ and is approximately the same in air
    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
    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
    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 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
    8 Know the difference between a digital and analogue signal
    9 Know that a sound can be transmitted as a digital or analogue signal
    10 Explain the benefits of digital signalling including increased rate of transmission of data and increased range due to accurate signal regeneration

    Source: Cambridge International syllabus

    The electromagnetic spectrum is a family of waves that all travel at the same high speed in a vacuum 真空, $3.0 \times 10^8\ \text{m/s}$. In order from longest wavelength (lowest frequency) to shortest:

    Region A typical use Danger from too much
    radio waves 无线电波 radio and TV signals
    microwaves 微波 mobile phones, satellite TV, cooking heating of body cells
    infrared 红外线 remote controls, thermal imaging, grills skin burns
    visible light seeing, photography
    ultraviolet 紫外线 sterilising water, checking bank notes skin cancer, eye damage
    X-rays X射线 medical and security scans damage to cells
    gamma rays 伽马射线 sterilising equipment, treating cancer mutation of cells

    As you go from radio waves to gamma rays, the frequency rises, the wavelength falls, and the energy (and danger) rises.

    A coloured band of the electromagnetic spectrum from radio waves to gamma rays
    From radio waves to gamma rays the wavelength falls while the frequency and energy rise

    Digital and analogue signals

    Radio waves and microwaves carry information as signals, and a signal is either analogue 模拟 or digital 数字. An analogue signal varies continuously and can take any value; a digital signal is a stream of just two values, on or off (1 or 0).

    Modern communication prefers digital signalling for two reasons the exam asks for:

    • a higher rate of data transmission;
    • a greater range: a weak digital signal can be regenerated back to a clean 1/0 exactly, because only two levels have to be told apart, so noise picked up along the way is removed. An analogue signal cannot be cleaned up this way, so its noise builds up.
    Explore

    Slide across the spectrum

    Radio waves, visible light and gamma rays are all the same wave — only the wavelength changes, and with it the frequency, photon energy and everyday use.

    Vocabulary Train
    English Chinese Pinyin
    vacuum 真空 zhēn kōng
    radio waves 无线电波 wú xiàn diàn bō
    microwaves 微波 wēi bō
    infrared 红外线 hóng wài xiàn
    ultraviolet 紫外线 zǐ wài xiàn
    X-rays X射线 X shè xiàn
    gamma rays 伽马射线 gā mǎ shè xiàn
    analogue 模拟 mó nǐ
    digital 数字 shù zì
    The electromagnetic spectrum 电磁波谱 diàn cí bō pǔ
    3.4

    Sound 声音

    Syllabus
    Core Supplement
    1 Describe the production of sound by vibrating sources
    2 Describe the longitudinal nature of sound waves 10 Describe compression and rarefaction
    3 State the approximate range of frequencies audible to humans as 20Hz to 20000Hz
    4 Know that a medium is needed to transmit sound waves
    5 Know that the speed of sound in air is approximately 330–350m/s 11 Know that, in general, sound travels faster in solids than in liquids and faster in liquids than in gases
    6 Describe a method involving a measurement of distance and time for determining the speed of sound in air
    7 Describe how changes in amplitude and frequency affect the loudness and pitch of sound waves
    8 Describe an echo as the reflection of sound waves
    9 Define ultrasound as sound with a frequency higher than 20kHz 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

    Source: Cambridge International syllabus

    Sound is made by a vibrating object. It is a longitudinal wave: the air is squeezed into a compression 压缩 (particles close together) and stretched into a rarefaction 稀疏 (particles far apart).

    • Sound needs a medium 介质 (a material) to travel through, so it cannot travel through a vacuum.
    • Humans can hear frequencies from about $20\ \text{Hz}$ to $20\,000\ \text{Hz}$.
    • Sound travels much slower than light (about $340\ \text{m/s}$ in air), and faster in liquids and solids than in gases.
    • A larger amplitude makes a louder sound (greater loudness 响度); a higher frequency makes a higher pitch 音调. So a dolphin's rapid clicks are high-pitched, and a hard drum-hit (big vibration) is loud.

    A reflected sound is an echo 回声. You can find the speed of sound by timing an echo over a known distance.

    Worked example. A student stands 85 m from a large wall and claps once. The echo returns 0.50 s later. Find the speed of sound.

    The sound travels to the wall and back, a distance of $2 \times 85 = 170\ \text{m}$, in $0.50\ \text{s}$:

    $$v = \frac{s}{t} = \frac{170}{0.50} = 340\ \text{m/s}$$

    Ultrasound 超声波 is sound above $20\,000\ \text{Hz}$ – too high for humans to hear. Its uses rely on reflection: sonar measures water depth, medical scanning images a baby or soft tissue, and non-destructive testing finds cracks inside metal without cutting it open. Like an echo, an ultrasound pulse travels there and back, so halve the total distance to reach the object.

    Worked example. A sonar pulse returns from the seabed $0.10\ \text{s}$ after it is sent; sound travels at $1500\ \text{m/s}$ in water. The pulse covers $s = v\times t = 1500\times0.10 = 150\ \text{m}$ there and back, so the sea is $150/2 = 75\ \text{m}$ deep.

    A microphone converts sound vibrations in air into an electrical signal
    A microphone converts sound vibrations in air into an electrical signal
    Explore

    Sound

    y = a sin(bt + c)

    Louder = bigger amplitude; higher pitch = higher frequency.

    Vocabulary Train
    English Chinese Pinyin
    compression 压缩 yā suō
    rarefaction 稀疏 xī shū
    medium 介质 jiè zhì
    loudness 响度 xiǎng dù
    pitch 音调 yīn diào
    echo 回声 huí shēng
    Ultrasound 超声波 chāo shēng bō
    3.4

    Exam tips

    • Learn $v = f\lambda$ and be ready to rearrange it. Measure all angles of incidence, reflection and refraction from the normal (the line at 90° to the surface), never from the surface itself.
    • Transverse waves vibrate across the direction of travel (light, water); longitudinal waves vibrate along it (sound). Sound needs a medium, so it cannot cross a vacuum; light can.
    • Total internal reflection happens only when light travels from a denser material to a less dense one and the angle inside is bigger than the critical angle.
    • Know the electromagnetic spectrum in order — radio, microwave, infrared, visible, ultraviolet, X-ray, gamma. All travel at the same speed in a vacuum; frequency and energy rise from radio to gamma.
    • Going into a denser material (air → glass) light slows down and bends towards the normal; leaving it (glass → air) light speeds up and bends away.
  • 4 Electricity and magnetism
    4.1

    Magnetism

    Syllabus
    Core Supplement
    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 10 Explain that magnetic forces are due to interactions between magnetic fields
    2 Describe induced magnetism
    3 State the differences between the properties of temporary magnets (made of soft iron) and the properties of permanent magnets (made of steel
    4 State the difference between magnetic and non-magnetic materials
    5 Describe a magnetic field as a region in which a magnetic pole experiences a force
    6 Draw the pattern and direction of magnetic field lines around a bar magnet 11 Know that the relative strength of a magnetic field is represented by the spacing of the magnetic field lines
    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
    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
    9 Describe the uses of permanent magnets and electromagnets

    Source: Cambridge International syllabus

    A magnet 磁体 can attract some metals. Every magnet has two ends, called poles 磁极: a north pole 北极 (N pole) and a south pole 南极 (S pole).

    Two magnets: N facing S attract; N facing N repel
    Like poles repel; unlike poles attract

    The rule for two poles is like the rule for charges:

    • Poles that are the same (N and N, or S and S) repel 排斥 (push apart).
    • Poles that are different (N and S) attract 吸引 (pull together).

    A magnet attracts a magnetic material 磁性材料, such as iron, steel, cobalt and nickel. Other materials (copper, plastic, wood) are non-magnetic and feel no force.

    Induced magnetism

    Put a piece of iron near or touching a magnet, and the iron becomes a magnet itself. This is induced magnetism 感应磁性. The end of the iron nearest the magnet gains the opposite pole, so the two then attract.

    Temporary and permanent magnets

    • Soft iron 软铁 is easy to magnetise 磁化 but loses its magnetism quickly. It is used for a temporary magnet 临时磁体.
    • Steel is harder to magnetise but keeps its magnetism. It is used for a permanent magnet 永磁体.

    So an unmagnetised 未磁化 piece of soft iron is the best core for an electromagnet, while steel is best for a bar magnet.

    Magnetic fields

    A magnetic field 磁场 is a region 区域 where a magnetic pole feels a force. We draw it with magnetic field lines 磁场线:

    • The lines come out of the N pole and go into the S pole.
    • The field direction at a point is the direction of the force on the N pole of a small test magnet placed there.
    • Where the lines are close together the field is strong; where they are far apart the field is weak.
    A bar magnet with field lines looping from the north pole to the south pole
    The field lines of a bar magnet come out of the N pole and go into the S pole

    You can show the pattern by sprinkling iron filings 铁屑 on paper over a magnet, or by moving a small plotting compass 指南针 around it (the needle points along the field).

    Tiny iron filings on white paper lining up into curved lines around a red and blue bar magnet
    Iron filings line up along the field lines, showing the field pattern of a bar magnet

    Uses of magnets

    • Permanent magnets: fridge door catches, compass needles, loudspeakers.
    • Electromagnets 电磁铁 (magnetic only while a current flows): cranes that lift scrap iron, electric bells, relays. An electromagnet can be switched on and off and made stronger, which a permanent magnet cannot.

    Magnetic forces happen because the fields of the two magnets push and pull on each other.

    Explore

    Make the magnetic field visible

    Compass needles trace the field from N to S; switch between attract and repel and watch the whole pattern reorganise, with a neutral point appearing for like poles.

    Vocabulary Train
    English Chinese Pinyin
    magnet 磁体 cí tǐ
    magnetic pole 磁极 cí jí
    north pole 北极 běi jí
    south pole 南极 nán jí
    repel 排斥 pái chì
    attract 吸引 xī yǐn
    magnetic material 磁性材料 cí xìng cái liào
    induced magnetism 感应磁性 gǎn yìng cí xìng
    soft iron 软铁 ruǎn tiě
    magnetise 磁化 cí huà
    temporary magnet 临时磁体 lín shí cí tǐ
    steel gāng
    permanent magnet 永磁体 yǒng cí tǐ
    unmagnetised 未磁化 wèi cí huà
    magnetic field 磁场 cí chǎng
    region 区域 qū yù
    magnetic field lines 磁场线 cí chǎng xiàn
    iron filings 铁屑 tiě xiè
    compass 指南针 zhǐ nán zhēn
    electromagnet 电磁铁 diàn cí tiě
    4.2

    Static electricity

    Syllabus

    4.2.1 Electric charge

    Core Supplement
    1 State that there are positive and negative charges 7 State that charge is measured in coulombs
    2 State that positive charges repel other positive charges, negative charges repel other negative charges, but positive charges attract negative charges 8 Describe an electric field as a region in which an electric charge experiences a force
    3 Describe simple experiments to show the production of electrostatic charges by friction and to show the detection of electrostatic charges 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
    4 Explain that charging of solids by friction involves only a transfer of negative charge (electrons) 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)
    5 Describe an experiment to distinguish between electrical conductors and insulators
    6 Recall and use a simple electron model to explain the difference between electrical conductors and insulators and give typical examples

    4.2.2 Electric current

    Core Supplement
    1 Know that electric current is related to the flow of charge 5 Define electric current as the charge passing a point per unit time; recall and use the equation $I = \frac{Q}{t}$
    2 Describe the use of ammeters (analogue and digital) with different ranges
    3 Describe electrical conduction in metals in terms of the movement of free electrons 6 State that conventional current is from positive to negative and that the flow of free electrons is from negative to positive
    4 Know the difference between direct current (d.c.) and alternating current (a.c.)

    4.2.3 Electromotive force and potential difference

    Core Supplement
    1 Define electromotive force (e.m.f.) as the electrical work done by a source in moving a unit charge around a complete circuit 6 Recall and use the equation for e.m.f. $E = \frac{W}{Q}$
    2 Know that e.m.f. is measured in volts (V)
    3 Define potential difference (p.d.) as the work done by a unit charge passing through a component 7 Recall and use the equation for p.d. $V = \frac{W}{Q}$
    4 Know that the p.d. between two points is measured in volts (V)
    5 Describe the use of voltmeters (analogue and digital) with different ranges

    4.2.4 Resistance

    Core Supplement
    1 Recall and use the equation for resistance $R = \frac{V}{I}$ 4 Sketch and explain the current–voltage graphs for a resistor of constant resistance, a filament lamp and a diode
    2 Describe an experiment to determine resistance using a voltmeter and an ammeter and do the appropriate calculations
    3 State, qualitatively, the relationship of the resistance of a metallic wire to its length and to its cross-sectional area 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

    4.2.5 Electrical energy and electrical power

    Core Supplement
    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
    2 Recall and use the equation for electrical power $P = IV$
    3 Recall and use the equation for electrical energy $E = IVt$
    4 Define the kilowatt-hour (kWh) and calculate the cost of using electrical appliances where the energy unit is the kWh

    Source: Cambridge International syllabus

    There are two kinds of electric charge 电荷: positive charge 正电荷 and negative charge 负电荷. The rule is like the rule for poles — same charges repel, different charges attract.

    A girl touching a Van de Graaff generator dome with her hair standing straight up and pushing apart
    Every hair picks up the same charge from the dome, and like charges repel — so the hairs push apart

    Charging by friction

    When you rub two different materials together, electrons 电子 (tiny negative particles) move from one to the other. This is charging by friction 摩擦起电.

    • The material that gains electrons becomes negative.
    • The material that loses electrons becomes positive.

    Only the negative electrons move; the positive charge stays in place. For example, a plastic rod rubbed with a cloth becomes negative because electrons move from the cloth onto the rod, leaving the cloth positive.

    Conductors and insulators

    • A conductor 导体 (copper and other metals) lets charge flow through it easily, because it has free electrons that can move.
    • An insulator 绝缘体 (plastic, rubber, glass) does not let charge flow, because its electrons cannot move freely.

    To test a material, join it in a circuit with a lamp and a battery: the lamp lights only for a conductor.

    Electric fields and ions

    Charge is measured in coulombs 库仑 (C). An electric field 电场 is a region where an electric charge feels a force. Its direction at a point is the direction of the force on a positive charge. Simple field patterns (the arrows show the direction):

    • around a point charge 点电荷: straight lines, pointing away from a positive charge and towards a negative charge;
    • around a charged ball (sphere): the same, spreading out evenly all around;
    • between two parallel plates with opposite charges: straight, evenly spaced lines from the positive plate to the negative plate.
    Field lines pointing out of a positive charge, into a negative charge, and straight down between two charged plates
    Electric field lines point away from a positive charge and towards a negative one; between parallel plates the field is uniform

    An atom is normally neutral. If it loses electrons it becomes a positive ion 离子; if it gains electrons it becomes a negative ion.

    Explore

    Rub a balloon and watch it charge

    Rubbing moves electrons onto the balloon, making it negative — then it attracts a neutral wall or your hair, but repels another negative balloon.

    Vocabulary Train
    English Chinese Pinyin
    electric charge 电荷 diàn hè
    positive charge 正电荷 zhèng diàn hè
    negative charge 负电荷 fù diàn hè
    electron 电子 diàn zi
    charging by friction 摩擦起电 mó cā qǐ diàn
    conductor 导体 dǎo tǐ
    insulator 绝缘体 jué yuán tǐ
    coulomb 库仑 kù lún
    electric field 电场 diàn chǎng
    point charge 点电荷 diǎn diàn hè
    ion 离子 lí zi
    Exercise sheet
    4.2

    Electric current

    An electric current 电流 is a flow of electric charge. It is measured in amperes 安培 (A) with an ammeter 电流表, joined in series in the circuit.

    Current is the charge that passes a point each second:

    $$I = \frac{Q}{t}$$

    Here $I$ is current (A), $Q$ is charge (C) and $t$ is time (s). Rearranged, $Q = It$.

    Worked example. A current of $3.0\ \text{A}$ flows through a lamp for $20\ \text{s}$. How much charge passes through it?

    $$Q = It = 3.0 \times 20 = 60\ \text{C}$$

    In a metal the current is a flow of free electrons 自由电子. There are two "directions" to know:

    • Conventional current 常规电流 is taken to flow from + to − round the outside of the cell.
    • The free electrons really drift the other way, from − to +.

    A direct current 直流电 (d.c.) always flows one way, as from a battery. An alternating current 交流电 (a.c.) keeps swapping direction many times each second, as from the mains supply 市电.

    A steady horizontal line for direct current beside a wave crossing zero for alternating current
    Direct current is steady in one direction; alternating current keeps swapping direction, crossing zero many times each second
    Vocabulary Train
    English Chinese Pinyin
    electric current 电流 diàn liú
    ampere 安培 ān péi
    ammeter 电流表 diàn liú biǎo
    free electrons 自由电子 zì yóu diàn zi
    conventional current 常规电流 cháng guī diàn liú
    direct current 直流电 zhí liú diàn
    alternating current 交流电 jiāo liú diàn
    mains supply 市电 shì diàn
    4.2

    E.m.f. and potential difference

    A cell gives energy 能量 to the charges that move through it. Two quantities describe this, and both are measured in volts 伏特 (V).

    • The electromotive force 电动势 (e.m.f.) of a source is the electrical work it does to drive unit charge all the way round a complete circuit 电路.
    • The potential difference 电势差 (p.d.) across a component is the work done by unit charge as it passes through that component.

    A voltmeter 电压表 measures e.m.f. or p.d. It is joined in parallel (across the component).

    A circuit with a voltmeter across the cell reading the e.m.f. and a voltmeter across the lamp reading the potential difference
    A voltmeter across the cell reads the e.m.f. (energy each coulomb is given); a voltmeter across the lamp reads the p.d. (energy each coulomb spends there).

    Both are work done per unit charge:

    $$E = \frac{W}{Q}, \qquad V = \frac{W}{Q}$$

    where $W$ is the energy transferred (J) and $Q$ is the charge (C). For example, if a cell does $120\ \text{J}$ of work moving $60\ \text{C}$ of charge round a circuit, its e.m.f. is $120 / 60 = 2\ \text{V}$.

    Vocabulary Train
    English Chinese Pinyin
    energy 能量 néng liàng
    volt 伏特 fú tè
    electromotive force 电动势 diàn dòng shì
    circuit 电路 diàn lù
    potential difference 电势差 diàn shì chà
    voltmeter 电压表 diàn yā biǎo
    4.2

    Resistance

    Resistance 电阻 measures how hard it is for current to flow. A bigger resistance gives a smaller current. It is measured in ohms 欧姆 (Ω).

    $$R = \frac{V}{I}$$

    To find the resistance of a component, join an ammeter in series (to read $I$) and a voltmeter across it (to read $V$), then divide.

    Worked example. A $12\ \text{V}$ battery drives a current of $0.50\ \text{A}$ through a lamp. Find the lamp's resistance.

    $$R = \frac{V}{I} = \frac{12}{0.50} = 24\ \Omega$$

    For a metal wire at constant temperature:

    • a longer wire has a bigger resistance — resistance is directly proportional 成正比 to length, $R \propto l$;
    • a thicker wire has a smaller resistance — resistance is inversely proportional 成反比 to cross-sectional area 横截面积, $R \propto \dfrac{1}{A}$.

    So doubling the length doubles the resistance; doubling the area halves it. (Area depends on the diameter squared, so a small change in diameter changes the resistance a lot.)

    Current–voltage graphs show how three components behave:

    Component Shape of the I–V graph What it tells you
    resistor 电阻器 (fixed) straight line through the origin resistance is constant, so $I \propto V$
    filament lamp 灯丝灯泡 S-shaped, getting flatter as $V$ rises the wire heats up, so its resistance rises
    diode 二极管 current one way only very high resistance the "wrong" way
    Three current-voltage graphs: a straight line for a resistor, an S-shaped curve for a filament lamp, and a one-way curve for a diode
    A resistor gives a straight line; a filament lamp curves as it heats up; a diode lets current pass only one way
    Explore

    Ohm's law

    V = IR

    For an ohmic conductor the current is proportional to the voltage — the gradient is 1/resistance.

    Explore

    I–V characteristics

    A resistor gives a straight line; a filament lamp and a diode do not. Pick a component and read I and R off the curve.

    Explore

    Resistance

    V = R·I

    Ohm's law: voltage is proportional to current — the gradient is the resistance R.

    Vocabulary Train
    English Chinese Pinyin
    resistance 电阻 diàn zǔ
    ohm 欧姆 ōu mǔ
    directly proportional 成正比 chéng zhèng bǐ
    inversely proportional 成反比 chéng fǎn bǐ
    cross-sectional area 横截面积 héng jié miàn jī
    resistor 电阻器 diàn zǔ qì
    filament lamp 灯丝灯泡 dēng sī dēng pào
    diode 二极管 èr jí guǎn
    4.2

    Electrical energy and power

    A circuit transfers energy from a source (a cell or the mains) to the components, and then into the surroundings (often as heat, light or sound).

    Electrical power 电功率 is the energy transferred each second, measured in watts 瓦特 (W):

    $$P = IV$$

    The electrical energy 电能 transferred in a time $t$, measured in joules 焦耳 (J), is:

    $$E = IVt$$

    Worked example. A $12\ \text{V}$ motor draws a current of $2.0\ \text{A}$. Find its power, and the energy it transfers in $30\ \text{s}$.

    $$P = IV = 2.0 \times 12 = 24\ \text{W}$$
    $$E = Pt = 24 \times 30 = 720\ \text{J}$$

    The kilowatt-hour

    Home electricity bills use a bigger energy unit, the kilowatt-hour 千瓦时 (kWh). One kilowatt-hour is the energy used by a $1\ \text{kW}$ appliance 电器 in $1$ hour.

    $$\text{energy (kWh)} = \text{power (kW)} \times \text{time (h)}$$
    $$\text{cost} = \text{energy (kWh)} \times \text{price per kWh}$$

    For example, a $2\ \text{kW}$ heater 加热器 used for $3$ hours uses $2 \times 3 = 6\ \text{kWh}$. If one kWh costs $20$ cents, the cost is $6 \times 20 = 120$ cents.

    A modern household electricity meter with a digital display reading zero kilowatt-hours
    A household electricity meter counts the energy used, in kilowatt-hours (kWh) — the number it shows is what you pay for
    Vocabulary Train
    English Chinese Pinyin
    electrical power 电功率 diàn gōng lǜ
    watt 瓦特 wǎ tè
    electrical energy 电能 diàn néng
    joule 焦耳 jiāo ěr
    kilowatt-hour 千瓦时 qiān wǎ shí
    appliance 电器 diàn qì
    heater 加热器 jiā rè qì
    4.3

    Circuits

    Syllabus

    4.3.1 Circuit diagrams and circuit components

    Core Supplement
    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 2 Draw and interpret circuit diagrams containing diodes and light-emitting diodes (LEDs) and know how these components behave in the circuit

    4.3.2 Series and parallel circuits

    Core Supplement
    1 Know that the current at every point in a series circuit is the same 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
    2 Know how to construct and use series and parallel circuits
    3 Calculate the combined e.m.f. of several sources in series
    4 Calculate the combined resistance of two or more resistors in series
    5 State that, for a parallel circuit, the current from the source is larger than the current in each branch 9 Explain that the sum of the currents into a junction is the same as the sum of the currents out of the junction
    6 State that the combined resistance of two resistors in parallel is less than that of either resistor by itself 10 Calculate the combined resistance of two resistors in parallel
    7 State the advantages of connecting lamps in parallel in a lighting circuit

    4.3.3 Action and use of circuit components

    Core Supplement
    1 Know that the p.d. across an electrical conductor increases as its resistance increases for a constant current 2 Describe the action of a variable potential divider
    3 Recall and use the equation for two resistors used as a potential divider
    $$\frac{R_1}{R_2} = \frac{V_1}{V_2}$$

    Source: Cambridge International syllabus

    Circuit components

    You should know these components and how they behave:

    Component What it does
    cell 电池 / battery 电池组 drives current round the circuit (a battery is two or more cells)
    power supply 电源 a source of d.c. or a.c.
    switch 开关 breaks or completes the circuit
    resistor (fixed) gives a fixed resistance
    variable resistor 可变电阻器 a resistance you can change, to control the current
    fuse 保险丝 melts and breaks the circuit if the current is too big
    lamp / heater turns electrical energy into light / into heat
    thermistor 热敏电阻 its resistance falls as it gets hotter
    light-dependent resistor 光敏电阻 (LDR) its resistance falls as the light gets brighter
    diode / light-emitting diode 发光二极管 (LED) lets current one way only; an LED also gives out light
    relay 继电器 a switch worked by an electromagnet (small current controls a big one)
    motor 电动机 turns electrical energy into movement
    bell 电铃 makes a sound
    transformer 变压器 changes the size of an a.c. voltage
    A chart of standard circuit symbols: cell, battery, switch, lamp, resistor, variable resistor, fuse, ammeter, voltmeter, diode, thermistor and LDR
    The standard symbols used to draw circuit diagrams
    Rows of small resistors held in paper tape, each with coloured bands and two wire legs
    Real resistors: the coloured bands give each one's resistance in ohms

    Series and parallel

    In a series 串联 circuit the parts form one single loop:

    • the current is the same at every point;
    • the supply p.d. is shared between the components;
    • cells in series add their e.m.f.s (when they point the same way);
    • resistors in series add up: $R_{\text{total}} = R_1 + R_2 + \dots$

    In a parallel 并联 circuit the parts are on separate branches:

    • each branch gets the full supply p.d.;
    • the current splits, so the current from the source is bigger than the current in any one branch;
    • the total resistance 总电阻 is less than the smallest single resistance.

    Lamps in a home are wired in parallel: each gets the full voltage, and if one fails the others stay on.

    A series circuit with two lamps in one loop next to a parallel circuit with two lamps on separate branches
    In a series circuit the components share one loop; in a parallel circuit each lamp has its own branch

    For calculations (with the rules above):

    • at a junction 节点, the total current flowing in equals the total current flowing out;
    • in series, the supply p.d. equals the sum of the p.d.s across the components;
    • in parallel, the p.d. across each branch is the same;
    • two resistors in parallel combine as
    $$\frac{1}{R_{\text{total}}} = \frac{1}{R_1} + \frac{1}{R_2}$$

    Worked example. A $6\ \Omega$ resistor and a $3\ \Omega$ resistor are connected in parallel. Find their combined resistance.

    $$\frac{1}{R_{\text{total}}} = \frac{1}{6} + \frac{1}{3} = \frac{1}{6} + \frac{2}{6} = \frac{3}{6} = \frac{1}{2} \quad\Rightarrow\quad R_{\text{total}} = 2\ \Omega$$

    Notice the combined resistance ($2\ \Omega$) is smaller than the smaller of the two resistors.

    Potential dividers

    Two resistors in series share the supply voltage. This is a potential divider 分压器. For the same current, a bigger resistance has a bigger p.d. across it, so the bigger resistor takes the bigger share:

    $$\frac{R_1}{R_2} = \frac{V_1}{V_2}$$

    A variable potential divider (or a variable resistor) lets you change the output voltage smoothly, for example from $0\ \text{V}$ up to the full supply. If you use a thermistor or an LDR as one of the resistors, the output voltage changes with temperature or light — handy for switching a heater or a lamp on and off automatically.

    Explore

    Build the current with Ohm's law

    Turn up the voltage and the electrons speed up and the bulb glows brighter; add resistance and the current drops. I = V/R, brightness = power.

    Vocabulary Train
    English Chinese Pinyin
    cell 电池 diàn chí
    battery 电池组 diàn chí zǔ
    power supply 电源 diàn yuán
    switch 开关 kāi guān
    variable resistor 可变电阻器 kě biàn diàn zǔ qì
    fuse 保险丝 bǎo xiǎn sī
    thermistor 热敏电阻 rè mǐn diàn zǔ
    light-dependent resistor 光敏电阻 guāng mǐn diàn zǔ
    light-emitting diode 发光二极管 fā guāng èr jí guǎn
    relay 继电器 jì diàn qì
    motor 电动机 diàn dòng jī
    bell 电铃 diàn líng
    transformer 变压器 biàn yā qì
    series 串联 chuàn lián
    parallel 并联 bìng lián
    total resistance 总电阻 zǒng diàn zǔ
    junction 节点 jié diǎn
    potential divider 分压器 fēn yā qì
    Exercise sheet
    4.4

    Electrical safety

    Syllabus
    Core Supplement
    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
    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
    3 Explain the use and operation of trip switches and fuses and choose appropriate fuse ratings and trip switch settings
    4 Explain why the outer casing of an electrical appliance must be either non-conducting (double-insulated) or earthed
    5 State that a fuse without an earth wire protects the circuit and the cabling for a double-insulated appliance

    Source: Cambridge International syllabus

    A home is fed by the mains. The mains is dangerous if it is used wrongly.

    Hazards

    These are hazards 危险 (dangers) with mains electricity:

    • damaged insulation 绝缘层 — bare wires can give a shock or start a fire;
    • overheating 过热 cables — too much current makes a cable hot, which can start a fire;
    • damp 潮湿 conditions — water lets current pass into a person, raising the risk of a shock;
    • overloading 过载 — plugging too many appliances into one socket 插座 draws too much current.

    Live, neutral and earth

    A mains cable has three wires:

    • the live wire 火线 carries the high voltage;
    • the neutral wire 零线 completes the circuit at about zero voltage;
    • the earth wire 地线 is a safety wire joined to the ground.

    A switch (and a fuse) must be fitted in the live wire. Then, when the switch is off, the appliance is cut off from the high voltage and is safe to touch.

    A wired three-pin plug with the earth wire green/yellow at the top, the neutral wire blue on the left, and the live wire brown on the right with the fuse fitted in it
    In a three-pin plug the live (brown) and neutral (blue) carry the current, the earth (green/yellow) is the safety wire, and the fuse always sits in the live wire.

    Fuses, trip switches and earthing

    A fuse is a thin wire that melts if the current gets too big, breaking the circuit before the cable overheats. Choose a fuse rating 额定值 just above the normal working current — for example a $13\ \text{A}$ fuse for an appliance that normally uses about $10\ \text{A}$.

    A trip switch 跳闸开关 (circuit breaker) does the same job but acts faster and can be reset instead of replaced.

    The metal casing 外壳 of an appliance must be made safe in one of two ways:

    • earthed 接地: the casing is joined to the earth wire. If a live wire touches the casing, a large current flows to earth and blows the fuse.
    • double-insulated 双重绝缘: the casing is plastic, so it can never become live. Such an appliance needs no earth wire; its fuse still protects the cable.
    The inside of a home consumer unit showing a row of miniature circuit breakers and two RCD trip switches
    A home consumer unit: each MCB is a trip switch that cuts off its circuit when the current gets too big; the RCD (80 A, 30 mA) cuts off even faster if it detects a fault to earth
    Explore

    Electrical safety route

    Follow fault current and see how safety devices protect people.

    Vocabulary Train
    English Chinese Pinyin
    hazard 危险 wēi xiǎn
    insulation 绝缘层 jué yuán céng
    overheating 过热 guò rè
    damp 潮湿 cháo shī
    overloading 过载 guò zài
    socket 插座 chā zuò
    live wire 火线 huǒ xiàn
    neutral wire 零线 líng xiàn
    earth wire 地线 dì xiàn
    fuse rating 额定值 é dìng zhí
    trip switch 跳闸开关 tiào zhá kāi guān
    casing 外壳 wài ké
    earthed 接地 jiē dì
    double-insulated 双重绝缘 shuāng chóng jué yuán
    4.5

    Electromagnetic effects

    Syllabus

    4.5.1 Electromagnetic induction

    Core Supplement
    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 4 Know that the direction of an induced e.m.f. opposes the change causing it
    2 Describe an experiment to demonstrate electromagnetic induction 5 State and use the relative directions of force, field and induced current
    3 State the factors affecting the magnitude of an induced e.m.f.

    4.5.2 The a.c. generator

    Core Supplement
    1 Describe a simple form of a.c. generator (rotating coil or rotating magnet) and the use of slip rings and brushes where needed
    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.

    4.5.3 Magnetic effect of a current

    Core Supplement
    1 Describe the pattern and direction of the magnetic field due to currents in straight wires and in solenoids 4 State the qualitative variation of the strength of the magnetic field around straight wires and solenoids
    2 Describe an experiment to identify the pattern of the magnetic field (including direction) due to currents in straight wires and in solenoids
    3 Describe how the magnetic effect of a current is used in relays and loudspeakers and give examples of their application 5 Describe the effect on the magnetic field around straight wires and solenoids of changing the magnitude and direction of the current

    4.5.4 Force on a current-carrying conductor

    Core Supplement
    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 Recall and use the relative directions of force, magnetic field and current
    3 Determine the direction of the force on beams of charged particles in a magnetic field

    4.5.5 The d.c. motor

    Core Supplement
    1 Know that a current-carrying coil in a magnetic field may experience a turning effect and that the turning effect is increased by increasing: (a) the number of turns on the coil (b) the current (c) the strength of the magnetic field 2 Describe the operation of an electric motor, including the action of a split-ring commutator and brushes

    4.5.6 The transformer

    Core Supplement
    1 Describe the construction of a simple transformer with a soft-iron core, as used for voltage transformations 6 Explain the principle of operation of a simple iron-cored transformer
    2 Use the terms primary, secondary, step-up and step-down
    3 Recall and use the equation
    $$\frac{V_p}{V_s} = \frac{N_p}{N_s}$$
    where p and s refer to primary and secondary
    7 Recall and use the equation for 100% efficiency in a transformer
    $$I_p V_p = I_s V_s$$
    where p and s refer to primary and secondary
    4 Describe the use of transformers in high-voltage transmission of electricity
    5 State the advantages of high-voltage transmission 8 Recall and use the equation
    $$P = I^2 R$$
    to explain why power losses in cables are smaller when the voltage is greater

    Source: Cambridge International syllabus

    The transformer: turns ratio
    Electromagnetic induction

    The magnetic effect of a current

    A current in a wire makes a magnetic field around it.

    • Around a straight wire the field lines are circles around the wire; the field is stronger close to the wire. Reverse the current and the field reverses.
    • A solenoid 螺线管 (a long coil 线圈 of wire) makes a field just like a bar magnet, with a N pole at one end and a S pole at the other. The field inside is strong and even.

    You can show both patterns with iron filings or a plotting compass. The field gets stronger if you increase the current, add more turns, or place a soft-iron core inside.

    A straight wire with circular field lines around it, beside a solenoid with a bar-magnet-like field
    A current makes circular field lines around a straight wire, and a bar-magnet-like field for a solenoid

    The magnetic effect is used in a relay and in a loudspeaker: in a loudspeaker 扬声器 a changing current in a coil makes the coil push and pull a paper cone, which moves the air and makes sound.

    Electromagnetic induction

    When a wire moves across a magnetic field, or the field through a coil changes, an e.m.f. is induced in the wire. If the wire is part of a complete circuit, this e.m.f. drives a current. This is electromagnetic induction 电磁感应.

    To show it: move a magnet in and out of a coil joined to a sensitive meter, and watch the needle flick. The induced e.m.f. is bigger when you use a stronger magnet, move faster, or use more turns on the coil. The induced e.m.f. always acts to oppose the change that causes it.

    The a.c. generator

    An a.c. generator 交流发电机 turns movement into electricity. A coil is spun in a magnetic field (or a magnet is spun near a coil). As it turns, the field through the coil keeps changing, so an alternating e.m.f. is induced.

    • Slip rings 滑环 and carbon brushes 电刷 carry the current out to the circuit while the coil keeps turning.
    • The e.m.f. is largest when the coil is flat (moving fastest across the field) and zero when the coil is upright (moving along the field). So the e.m.f.–time graph is a wave: peak, zero, opposite peak, zero, for each turn.
    A coil turning between magnet poles, connected through slip rings and brushes, with a sine-wave a.c. output
    Turning the coil induces an alternating e.m.f.; the slip rings carry the a.c. out to the circuit

    Force on a current-carrying conductor

    When a current-carrying wire lies in a magnetic field, the field of the wire and the field of the magnet push on each other, so the wire feels a force. This is the motor effect.

    • Reverse the current, or reverse the field, and the force reverses.
    • Make the current bigger or the field stronger, and the force is bigger.

    The force, the field and the current are at right angles to one another. You can find the force direction with the left-hand rule: thumb = force (motion), first finger = field (N to S), second finger = current.

    A current-carrying wire between two magnet poles, with the force at right angles to the field and current
    A current-carrying wire in a magnetic field feels a force at right angles to both the field and the current

    A moving stream of charged particles is a current, so a magnetic field pushes it sideways too — it deflects 偏转 the beam. (Remember electrons flow opposite to the conventional current.)

    The d.c. motor

    A coil carrying a current in a magnetic field feels a turning effect 转动效应, because the forces on its two sides act in opposite directions. This is a d.c. motor 直流电动机. The turning effect is bigger with more turns on the coil, a bigger current, or a stronger field.

    A split-ring commutator 换向器 swaps the current direction in the coil every half-turn. This keeps the coil turning the same way instead of stopping after half a turn.

    A coil between magnet poles with opposite forces on its two sides, a split-ring commutator, brushes and a battery
    The forces on the two sides of the coil form a couple; the split-ring commutator keeps it turning one way
    Close-up of carbon brushes on springs pressing against the copper bars of a d.c. machine commutator
    In a real d.c. machine, carbon brushes press on the copper commutator bars to feed current to the spinning coil

    The transformer

    A transformer changes the size of an a.c. voltage. It has two coils wound on a soft-iron core 软铁芯:

    • the primary coil 原线圈 takes in the a.c. voltage;
    • the secondary coil 副线圈 gives out the changed voltage.

    The a.c. in the primary makes a changing magnetic field in the core. The core carries this field to the secondary, where it induces an a.c. e.m.f. The voltages and the numbers of turns are linked by:

    $$\frac{V_p}{V_s} = \frac{N_p}{N_s}$$

    Worked example. A transformer has $1200$ turns on the primary coil and $100$ turns on the secondary coil. The primary is connected to a $240\ \text{V}$ a.c. supply. Find the secondary voltage.

    $$\frac{240}{V_s} = \frac{1200}{100} = 12 \quad\Rightarrow\quad V_s = \frac{240}{12} = 20\ \text{V}$$

    Fewer turns on the secondary, so this is a step-down transformer.

    A transformer: a primary and a secondary coil wound on a soft-iron core, with an a.c. supply on the primary
    The changing field in the core links the two coils; the voltage ratio equals the turns ratio
    A grey metal transformer fixed to a wooden electricity pole, with thick insulated cables running to it
    A real transformer on a power pole steps the high voltage in the cables down to a safer voltage for homes

    If the secondary has more turns it is a step-up 升压 transformer (voltage rises); fewer turns make a step-down 降压 transformer (voltage falls). For example, a transformer changing $240\ \text{V}$ to $12\ \text{V}$ is a step-down type, and the primary has $20$ times as many turns as the secondary.

    If a transformer is 100% efficient, the power in equals the power out:

    $$I_p V_p = I_s V_s$$

    So a step-up transformer raises the voltage but lowers the current.

    Why we use high voltage to send power

    Electricity is sent across the country by high-voltage transmission 高压输电. The power lost as heat in the cables is

    $$P = I^2 R$$

    where $R$ is the resistance of the cables. A step-up transformer raises the voltage and so lowers the current for the same power ($P = IV$). A smaller current means much less power wasted in the cables. A step-down transformer then lowers the voltage again to a safe value before it reaches homes.

    A tall steel lattice pylon carrying many cables across the countryside against an evening sky
    Pylons hold the cables that carry electricity at very high voltage, which keeps the current — and the wasted power — low
    Explore

    The force that spins a motor

    A current in a magnetic field is pushed at right angles to both — reverse the current or flip the magnet and it pushes the other way. That is what turns a motor.

    Explore

    The generator

    V = a sin(bt)

    A spinning coil induces a sinusoidal voltage — the AC output.

    Explore

    Transformer

    Add turns to the secondary to step the voltage up, fewer to step it down — Vs/Vp = Ns/Np, exactly how the grid moves power efficiently.

    Vocabulary Train
    English Chinese Pinyin
    solenoid 螺线管 luó xiàn guǎn
    coil 线圈 xiàn quān
    loudspeaker 扬声器 yáng shēng qì
    electromagnetic induction 电磁感应 diàn cí gǎn yìng
    a.c. generator 交流发电机 jiāo liú fā diàn jī
    slip rings 滑环 huá huán
    brushes 电刷 diàn shuā
    deflect 偏转 piān zhuǎn
    turning effect 转动效应 zhuǎn dòng xiào yìng
    d.c. motor 直流电动机 zhí liú diàn dòng jī
    split-ring commutator 换向器 huàn xiàng qì
    soft-iron core 软铁芯 ruǎn tiě xīn
    primary coil 原线圈 yuán xiàn quān
    secondary coil 副线圈 fù xiàn quān
    step-up 升压 shēng yā
    step-down 降压 jiàng yā
    high-voltage transmission 高压输电 gāo yā shū diàn
    Exercise sheet
    4.5

    Exam tips

    • Current is the same everywhere in a series circuit; in a parallel circuit it splits between the branches. Voltage (p.d.) is shared out in series, but is the same across every parallel branch.
    • Adding resistors in series increases the total resistance ($R_1 + R_2$); adding them in parallel makes the total less than the smallest single resistor.
    • An ammeter goes in series and has very low resistance; a voltmeter goes in parallel across a component and has very high resistance.
    • In a transformer $\dfrac{V_p}{V_s} = \dfrac{N_p}{N_s}$: more turns on the secondary steps the voltage up, fewer steps it down. Transformers only work on a.c.
    • Power is sent across country at high voltage so the current — and the heat wasted in the cables, $P = I^2R$ — is small.
    • Fit the switch and the fuse in the live wire, and choose a fuse rating just above the appliance's normal working current.
  • 5 Nuclear physics
    5.1

    The atom

    Syllabus

    5.1.1 The atom

    Core Supplement
    1 Describe the structure of an atom in terms of a positively charged nucleus and negatively charged electrons in orbit around the nucleus 3 Describe how the scattering of alpha ($\alpha$) 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
    2 Know how atoms may form positive ions by losing electrons or form negative ions by gaining electrons

    5.1.2 The nucleus

    Core Supplement
    1 Describe the composition of the nucleus in terms of protons and neutrons
    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
    2 State the relative charges of protons, neutrons and electrons as +1, 0 and –1 respectively
    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 7 Know the relationship between the proton number and the relative charge on a nucleus
    8 Know the relationship between the nucleon number and the relative mass of a nucleus
    4 Use the nuclide notation $^{A}_{Z}\text{X}$
    5 Explain what is meant by an isotope and state that an element may have more than one isotope

    Source: Cambridge International syllabus

    An atom 原子 is made of a tiny central nucleus 原子核 with electrons 电子 moving around it (in orbit 轨道, like planets around the Sun).

    • The nucleus has a positive charge 电荷.
    • The electrons have a negative charge.
    • The atom as a whole is neutral, because the positive and negative charges are equal.

    Almost all the mass 质量 is in the nucleus, but the nucleus is very small compared with the whole atom. So an atom is mostly empty space.

    A central nucleus of protons and neutrons with electrons moving in circular orbits around it
    The nuclear atom: a tiny dense nucleus of protons and neutrons, with electrons in orbits around it

    Ions

    An atom is neutral, but it can gain or lose electrons to become an ion 离子.

    • Lose one or more electrons → a positive ion (now there are more protons than electrons).
    • Gain one or more electrons → a negative ion.

    The alpha-scattering experiment

    This experiment gave the evidence for the nuclear model. Alpha particles α粒子 (small, fast, positive) were fired at a very thin gold foil 金箔, and the scattering 散射 (the way they bounced off) was watched.

    The results and what they tell us:

    • Almost all the alpha particles went straight through. → The atom is mostly empty space.
    • A few were deflected 偏转 (bent) through small angles. → The nucleus has a positive charge, which pushes the positive alpha particles away.
    • A very few bounced almost straight back. → The nucleus is very small and very heavy, and holds most of the mass of the atom.
    Alpha particles fired at a gold foil: most pass straight through, a few deflect, a very few bounce back
    Most alpha particles pass straight through; a few are deflected and a very few bounce back off the tiny dense nucleus
    Explore

    Inside the atom

    A tiny dense nucleus sits at the centre with electrons in shells around it — drag the proton number and watch the shells fill outward.

    Vocabulary Train
    English Chinese Pinyin
    atom 原子 yuán zi
    nucleus 原子核 yuán zǐ hé
    electron 电子 diàn zi
    orbit 轨道 guǐ dào
    charge 电荷 diàn hè
    mass 质量 zhì liàng
    ion 离子 lí zi
    alpha particle α粒子 α lì zi
    gold foil 金箔 jīn bó
    scattering 散射 sǎn shè
    deflect 偏转 piān zhuǎn
    5.1

    Inside the nucleus

    The nucleus is made of two kinds of particle, together called nucleons 核子:

    • protons 质子, which have a relative 相对 charge of $+1$;
    • neutrons 中子, which have a relative charge of $0$ (they are neutral).

    An electron has a relative charge of $-1$. A proton and a neutron each have a relative mass of about $1$; an electron is almost massless in comparison.

    Two numbers describe a nucleus:

    • the proton number 质子数 $Z$ (also called the atomic number) — the number of protons;
    • the nucleon number 核子数 $A$ (also called the mass number) — the number of protons plus neutrons.

    So the number of neutrons is $A - Z$.

    We write a nucleus in nuclide 核素 notation:

    $$^{A}_{Z}\text{X}$$

    where X is the chemical symbol. For example, $^{197}_{\ 79}\text{Au}$ has $79$ protons and $197 - 79 = 118$ neutrons. The relative charge of the whole nucleus is just $+Z$ (here $+79$), and its relative mass is about $A$.

    Isotopes

    Isotopes 同位素 are atoms of the same element (the same $Z$) but with different numbers of neutrons (different $A$). They behave the same in chemistry but differently in the nucleus. For example, $^{12}_{\ 6}\text{C}$ and $^{14}_{\ 6}\text{C}$ are both carbon.

    Two carbon nuclei: carbon-12 with six protons and six neutrons, carbon-14 with six protons and eight neutrons
    Isotopes of carbon have the same six protons but different numbers of neutrons, so they are the same element with a different mass

    Nuclear fission and fusion

    In nuclear fission 核裂变, a heavy nucleus absorbs a neutron and then splits into two smaller nuclei, giving out two or three neutrons and a lot of energy 能量:

    $$^{235}_{\ 92}\text{U} + ^{1}_{0}\text{n} \rightarrow\ ^{141}_{\ 56}\text{Ba} + ^{92}_{36}\text{Kr} + 3\,{}^{1}_{0}\text{n}$$
    A neutron hitting a U-235 nucleus, which splits into Ba and Kr plus more neutrons and energy
    A neutron splits a U-235 nucleus into two smaller nuclei, releasing more neutrons and energy

    The top numbers (nucleon numbers) balance on both sides, and so do the bottom numbers (proton numbers). You can use this to find a missing number — for example, how many neutrons are released.

    In nuclear fusion 核聚变, two light nuclei join to make a heavier one, also giving out energy. This is how the Sun makes its energy, joining hydrogen nuclei to make helium. The reaction below — two heavy forms of hydrogen (deuterium and tritium) joining into helium — is the one used in fusion reactors on Earth:

    $$^{2}_{1}\text{H} + ^{3}_{1}\text{H} \rightarrow\ ^{4}_{2}\text{He} + ^{1}_{0}\text{n}$$
    Two small hydrogen nuclei joining to form a helium nucleus plus a neutron and energy
    In fusion two light nuclei join into a heavier one, releasing a neutron and energy — the deuterium–tritium reaction used in fusion reactors

    In both fission and fusion, a small amount of mass is lost and turned into energy.

    Two large cooling towers of a nuclear power station beside a river, giving off white clouds of steam
    A nuclear power station uses the energy from fission to make electricity; the towers release waste heat as steam
    Explore

    The fission chain reaction

    A neutron splits a uranium nucleus, which releases energy AND more neutrons — those split more nuclei, and so on.

    Vocabulary Train
    English Chinese Pinyin
    nucleon 核子 hé zǐ
    proton 质子 zhì zi
    relative 相对 xiāng duì
    neutron 中子 zhōng zi
    proton number 质子数 zhì zi shù
    nucleon number 核子数 hé zǐ shù
    nuclide 核素 hé sù
    isotope 同位素 tóng wèi sù
    nuclear fission 核裂变 hé liè biàn
    energy 能量 néng liàng
    nuclear fusion 核聚变 hé jù biàn
    hydrogen qīng
    helium hài
    5.2

    Radioactivity

    Syllabus

    5.2.1 Detection of radioactivity

    Core Supplement
    1 Know what is meant by background radiation
    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
    3 Know that ionising nuclear radiation can be measured using a detector connected to a counter
    4 Use count rate measured in counts / s or counts / minute 5 Use measurements of background radiation to determine a corrected count rate

    5.2.2 The three types of nuclear emission

    Core Supplement
    1 Describe the emission of radiation from a nucleus as spontaneous and random in direction
    2 Identify alpha ($\alpha$), beta ($\beta$) and gamma ($\gamma$) emissions from the nucleus by recalling: (a) their nature (b) their relative ionising effects (c) their relative penetrating abilities ($\beta^+$ are not included, $\beta$-particles will be taken to refer to $\beta^-$) 3 Describe the deflection of $\alpha$-particles, $\beta$-particles and $\gamma$-radiation in electric fields and magnetic fields
    4 Explain their relative ionising effects with reference to: (a) kinetic energy (b) electric charge

    5.2.3 Radioactive decay

    Core Supplement
    1 Know that radioactive decay is a change in an unstable nucleus that can result in the emission of $\alpha$-particles or $\beta$-particles and/or $\gamma$-radiation and know that these changes are spontaneous and random 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
    2 State that during $\alpha$-decay or $\beta$-decay, the nucleus changes to that of a different element 4 Describe the effect of $\alpha$-decay, $\beta$-decay and $\gamma$-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 $\beta$-emission neutron $\rightarrow$ proton + electron
    5 Use decay equations, using nuclide notation, to show the emission of $\alpha$-particles, $\beta$-particles and $\gamma$-radiation

    5.2.4 Half-life

    Core Supplement
    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) 2 Calculate half-life from data or decay curves from which background radiation has not been subtracted
    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

    5.2.5 Safety precautions

    Core Supplement
    1 State the effects of ionising nuclear radiations on living things, including cell death, mutations and cancer
    2 Describe how radioactive materials are moved, used and stored in a safe way 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

    Source: Cambridge International syllabus

    Radioactive decay & half-life

    A nucleus that is unstable 不稳定 will sooner or later break down and give out radiation 辐射. This is radioactive 放射性 decay 衰变. A nucleus may be unstable because it has too many neutrons, or because it is too heavy.

    Decay is spontaneous 自发 (it happens on its own, and you cannot speed it up or slow it down) and random 随机 (you cannot say which nucleus will decay next, or exactly when).

    Background radiation

    Some radiation is around us all the time. This is background radiation 背景辐射. Its main sources are:

    • radon gas in the air (usually the biggest source);
    • rocks and buildings;
    • food and drink;
    • cosmic rays 宇宙射线 from space.

    Measuring radiation

    Radiation can be measured with a detector 探测器 joined to a counter 计数器. The count rate 计数率 is the number of counts each second (or each minute).

    To find the true count rate from a source, first measure the background count rate on its own, then subtract it. The answer is the corrected 修正 count rate:

    $$\text{corrected count rate} = \text{measured count rate} - \text{background count rate}$$

    Worked example. A detector placed next to a source reads $250$ counts/min. With the source taken away, the background count rate is $30$ counts/min. Find the corrected count rate.

    $$250 - 30 = 220\ \text{counts/min}$$
    A small white handheld Geiger counter with a screen showing "200 CPM" (counts per minute)
    A Geiger counter detects radiation and shows the count rate, here in counts per minute (CPM)
    Explore

    Radioactive decay

    N = N₀·b

    The number of unstable nuclei decays exponentially.

    Vocabulary Train
    English Chinese Pinyin
    unstable 不稳定 bù wěn dìng
    radiation 辐射 fú shè
    radioactive 放射性 fàng shè xìng
    decay 衰变 shuāi biàn
    spontaneous 自发 zì fā
    random 随机 suí jī
    background radiation 背景辐射 bèi jǐng fú shè
    radon dōng
    cosmic rays 宇宙射线 yǔ zhòu shè xiàn
    detector 探测器 tàn cè qì
    counter 计数器 jì shù qì
    count rate 计数率 jì shù lǜ
    corrected 修正 xiū zhèng
    Exercise sheet
    5.2

    The three types of radiation

    The radiation can be one of three types. Each type is ionising 电离, which means it can knock electrons off atoms in its path.

    Type What it is Ionising effect Stopped by
    alpha (α) a helium nucleus: 2 protons + 2 neutrons, charge $+2$ strongest a sheet of paper, or a few cm of air
    beta (β) a fast-moving electron, charge $-1$ medium a few mm of aluminium
    gamma (γ) a high-energy electromagnetic wave 电磁波, no charge weakest thick lead or concrete (only reduced, never fully stopped)

    So an alpha particle is the most ionising but the least penetrating 穿透 (it is easily absorbed 吸收). A beta particle β粒子 is in the middle. Gamma radiation γ射线 is the least ionising but the most penetrating.

    Alpha stopped by paper, beta stopped by aluminium, gamma only reduced by lead
    Paper stops alpha, a few millimetres of aluminium stops beta, and thick lead only reduces gamma

    We can explain the ionising effects from charge and kinetic energy 动能: an alpha particle has a large charge ($+2$) and is slow and heavy, so it pulls strongly on the electrons it passes and ionises a lot. A beta particle has a smaller charge and moves faster, so it ionises less.

    Deflection in fields

    Because alpha and beta particles are charged, they are deflected by an electric field 电场 and by a magnetic field 磁场. They bend in opposite directions, because their charges have opposite signs, and the lighter beta particle bends more. Gamma rays have no charge, so they are not deflected at all.

    Alpha bending one way, beta bending the other way and more, gamma going straight between two charged plates
    Alpha and beta bend in opposite directions; the lighter beta bends more, and uncharged gamma is not deflected
    Vocabulary Train
    English Chinese Pinyin
    ionising 电离 diàn lí
    aluminium
    electromagnetic wave 电磁波 diàn cí bō
    lead qiān
    penetrating 穿透 chuān tòu
    absorb 吸收 xī shōu
    beta particle β粒子 β lì zi
    gamma radiation γ射线 γ shè xiàn
    kinetic energy 动能 dòng néng
    electric field 电场 diàn chǎng
    magnetic field 磁场 cí chǎng
    5.2

    Decay equations

    When a nucleus decays, the nucleon and proton numbers must balance on both sides.

    Alpha decay — the nucleus loses 2 protons and 2 neutrons, so $A$ falls by $4$ and $Z$ falls by $2$. It becomes a different element:

    $$^{A}_{Z}\text{X} \rightarrow\ ^{A-4}_{Z-2}\text{Y} + ^{4}_{2}\alpha$$

    Worked example. A radium nucleus $^{226}_{\ 88}\text{Ra}$ emits an alpha particle. Find the nucleon number and proton number of the new nucleus.

    Alpha decay lowers $A$ by $4$ and $Z$ by $2$:

    $$^{226}_{\ 88}\text{Ra} \rightarrow\ ^{222}_{\ 86}\text{Rn} + ^{4}_{2}\alpha$$

    So the new nucleus (radon) has nucleon number $222$ and proton number $86$.

    Beta decay — inside the nucleus a neutron changes into a proton plus an electron:

    $$\text{neutron} \rightarrow \text{proton} + \text{electron}$$

    The fast electron leaves as the beta particle. So $A$ stays the same but $Z$ rises by $1$, giving a different element:

    $$^{24}_{11}\text{Na} \rightarrow\ ^{24}_{12}\text{Mg} + ^{\ \ 0}_{-1}\beta$$

    Gamma emission — the nucleus loses only energy, so $A$ and $Z$ do not change. Alpha and beta decay leave the nucleus more stable 稳定; gamma is often given out at the same time to carry away spare energy.

    Vocabulary Train
    English Chinese Pinyin
    stable 稳定 wěn dìng
    5.2

    Half-life

    Because decay is random, we cannot follow one nucleus. Instead we describe a large sample 样品 using its half-life.

    The half-life 半衰期 of an isotope is the time taken for half the unstable nuclei in a sample to decay. After each half-life, the count rate (or the number of unstable nuclei left) falls to half.

    For example, if a source has a count rate of $800$ counts/min and a half-life of $3$ hours:

    Time / hours 0 3 6 9
    Count rate / (counts/min) 800 400 200 100

    After $6$ hours (two half-lives) the count rate has halved twice: $800 \to 400 \to 200$. You can read a half-life off a decay graph by finding the time for the count rate to drop from any value to half of it.

    Worked example. The activity of a source falls from $800$ counts/min to $100$ counts/min. Its half-life is $5$ days. How long did this take?

    Count the halvings: $800 \to 400 \to 200 \to 100$ is three half-lives, so the time is $3 \times 5 = 15\ \text{days}$.

    A decay curve of count rate against time, halving at each half-life
    Each half-life $T$ the count rate halves: $N_0 \to N_0/2 \to N_0/4 \to N_0/8$
    Explore

    Half-life — watch the nuclei decay

    Each nucleus has a fixed chance of decaying, at random. Move time forward: about half the remaining nuclei decay every half-life — so the count halves, then halves again.

    Vocabulary Train
    English Chinese Pinyin
    sample 样品 yàng pǐn
    half-life 半衰期 bàn shuāi qī
    5.2

    Uses of radioactivity

    The isotope chosen for a job depends on its type of radiation and its half-life:

    • smoke alarms 烟雾报警器 use an alpha source (alpha is easily blocked, so it is safe outside the alarm, and a long half-life means it lasts for years);
    • using radiation on food, or on equipment, kills bacteria 细菌 and germs — this needs penetrating gamma rays to sterilise 消毒 the sealed item;
    • measuring and controlling the thickness of paper or metal sheets uses a beta source (the amount that passes through changes with the thickness);
    • gamma rays are used to find and to treat cancer 癌症 inside the body, because they can pass out of (or into) the body.
    A patient held still by a mesh mask under a radiotherapy machine, with green alignment lasers crossing the mask
    Radiotherapy: a mesh mask holds the patient still while alignment lasers aim gamma rays precisely at a tumour to treat cancer
    Vocabulary Train
    English Chinese Pinyin
    smoke alarm 烟雾报警器 yān wù bào jǐng qì
    bacteria 细菌 xì jūn
    sterilise 消毒 xiāo dú
    cancer 癌症 ái zhèng
    5.2

    Safety

    Ionising radiation harms living cells 细胞. It can cause cell death, mutations 突变 (changes to the genes) and cancer.

    When working with radioactive sources, keep the dose 剂量 (the amount of radiation received) low by:

    • reducing the exposure 照射 time — spend as little time near the source as possible;
    • increasing the distance between you and the source;
    • using shielding 屏蔽, such as lead, between the source and your body.

    Radioactive sources should be handled with tongs (not bare hands), kept pointing away from people, and stored in a lead-lined box.

    Vocabulary Train
    English Chinese Pinyin
    living cells 细胞 xì bāo
    mutation 突变 tū biàn
    dose 剂量 jì liàng
    exposure 照射 zhào shè
    shielding 屏蔽 píng bì
    5.2

    Exam tips

    • The nucleon number (top) is protons + neutrons; the proton number (bottom) is protons only. Number of neutrons = nucleon number − proton number.
    • Isotopes have the same proton number but different nucleon numbers — the same element with a different number of neutrons.
    • Rank the radiations two ways: alpha is the most ionising but least penetrating (stopped by paper); gamma is the least ionising but most penetrating (needs thick lead). Beta is in between (stopped by a few mm of aluminium).
    • In every decay equation the top numbers must balance and the bottom numbers must balance. Alpha decay: $A-4$, $Z-2$. Beta decay: $A$ unchanged, $Z+1$.
    • Always subtract the background count rate before using a source's readings. After $n$ half-lives the count rate has halved $n$ times — count the halvings rather than guessing from the total time.
  • 6 Space physics
    6.1

    The Earth, the Sun and the Moon

    Syllabus

    6.1.1 The Earth

    Core Supplement
    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
    2 Know that the Earth orbits the Sun once in approximately 365 days and use this to explain the periodic nature of the seasons 4 Define average orbital speed from the equation $v = \frac{2\pi r}{T}$ where $r$ is the average radius of the orbit and $T$ is the orbital period; recall and use this equation
    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

    6.1.2 The Solar System

    Core Supplement
    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 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
    8 Analyse and interpret planetary data about orbital distance, orbital duration, density, surface temperature and uniform gravitational field strength at the planet’s surface
    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
    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
    4 Calculate the time it takes light to travel a significant distance such as between objects in the Solar System
    5 Know that the Sun contains most of the mass of the Solar System and this explains why the planets orbit the Sun
    6 Know that the force that keeps an object in orbit around the Sun is the gravitational attraction of the Sun 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
    10 Know that an object in an elliptical orbit travels faster when closer to the Sun and explain this using the conservation of energy

    Source: Cambridge International syllabus

    The Earth spins (rotates 自转) on its axis once in about $24$ hours. The axis is tilted 倾斜 (not straight up). This spin gives us day and night, and makes the Sun 太阳 appear to move across the sky each day.

    The Earth also moves around the Sun in an orbit 轨道, once in about $365$ days (one year). Because the axis is tilted, different parts of the Earth lean towards the Sun at different times of the year. This gives the seasons 季节: it is summer in the half of the Earth that leans towards the Sun.

    The tilted Earth at two points in its orbit: the north leaning toward the Sun, and half a year later leaning away
    The axis keeps the same tilt all year, so each hemisphere leans toward the Sun for one half of the orbit and away for the other

    The Moon 月球 orbits the Earth once in about one month. As it goes round, we see different amounts of its lit side, which gives the phases 月相 of the Moon (new moon, half moon, full moon).

    The Moon at four points around its orbit of the Earth, each with the half facing the Sun lit
    The Moon's lit half always faces the Sun, so as it orbits we see different amounts of it: a new moon between us and the Sun, a full moon opposite the Sun, and half moons in between

    So, from shortest to longest: one day (Earth's spin) < one month (Moon's orbit) < one year (Earth's orbit).

    The full grey disc of the Moon, covered in dark patches and bright craters, against black space
    The full Moon, Earth's natural satellite
    Explore

    Why the Moon changes shape

    The Sun always lights half the Moon; the phase is simply how much of that lit half faces us as the Moon orbits — it is not Earth's shadow.

    Vocabulary Train
    English Chinese Pinyin
    rotate 自转 zì zhuàn
    axis zhóu
    tilted 倾斜 qīng xié
    Sun 太阳 tài yáng
    orbit 轨道 guǐ dào
    seasons 季节 jì jié
    Moon 月球 yuè qiú
    phases 月相 yuè xiàng
    6.1

    Orbital speed

    For an object going round a circle, the distance for one full orbit is the circumference 周长 $2\pi r$, where $r$ is the radius of the orbit. The orbital speed 轨道速率 is this distance divided by the period 周期 $T$ (the time for one orbit):

    $$v = \frac{2\pi r}{T}$$

    The same equation works for planets, moons and satellites.

    Worked example. A space station orbits the Earth at a radius of $r = 7000\ \text{km}$ and takes $T = 5800\ \text{s}$ for one orbit. Find its orbital speed.

    First convert the radius to metres: $7000\ \text{km} = 7.0 \times 10^6\ \text{m}$. Then

    $$v = \frac{2\pi r}{T} = \frac{2\pi \times 7.0 \times 10^6}{5800} \approx 7600\ \text{m/s}$$
    The ISS in orbit: orbital speed is the speed that keeps a satellite in free-fall circular motion
    The ISS in orbit: orbital speed is the speed that keeps a satellite in free-fall circular motion
    Vocabulary Train
    English Chinese Pinyin
    circumference 周长 zhōu cháng
    orbital speed 轨道速率 guǐ dào sù lǜ
    period 周期 zhōu qī
    6.1

    The Solar System

    The Solar System 太阳系 has one star, the Sun, at its centre. Around it move the eight planets 行星. In order from the Sun they are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune.

    • The four planets nearest the Sun are small and rocky 岩石.
    • The four planets furthest from the Sun are large and gaseous 气态 — they are made mostly of gas 气体, with no solid surface to stand on.
    • The two nearer giants, Jupiter and Saturn, are gas giants 气态巨行星. The two outer giants, Uranus and Neptune, are ice giants 冰巨行星: they hold much more ice, so they are not true gas giants.
    The Sun with Mercury, Venus, Earth and Mars, then the asteroid belt, then Jupiter, Saturn, Uranus and Neptune
    The Sun and its eight planets in order: four small rocky planets, then the asteroid belt, then four large gaseous planets — the gas giants Jupiter and Saturn and the ice giants Uranus and Neptune (not to scale)
    The full red disc of Mars against black space, with darker surface markings and a thin polar haze
    Mars, the red planet, one of the rocky inner planets
    The full disc of Jupiter showing brown and white cloud bands and the orange Great Red Spot
    Jupiter, the largest planet, with its swirling bands of gas
    Saturn with its wide, flat system of rings, photographed from the side by the Cassini spacecraft
    Saturn and its rings, photographed by the Cassini spacecraft

    The Solar System also contains:

    • minor planets, such as dwarf planets 矮行星 like Pluto, and asteroids 小行星 (most lie in the asteroid belt between Mars and Jupiter);
    • moons (natural satellites 卫星) that orbit the planets;
    • comets 彗星 and other small bodies.

    Orbits and gravity

    The Sun holds most of the mass of the Solar System. Its gravity 引力 (gravitational pull) reaches out and keeps the planets in their orbits. This force is the gravitational attraction of the Sun.

    The gravitational field strength 重力场强度 tells you how strong gravity is:

    • at the surface of a planet it is bigger for a planet with more mass;
    • around a planet it gets weaker as you move further away.

    In the same way, the Sun's gravity gets weaker further out, so the outer planets move more slowly (smaller orbital speed) than the inner ones.

    Most orbits are not perfect circles but ellipses 椭圆 (a stretched circle), and the Sun is not at the centre of the ellipse. A comet has a very stretched orbit. An object in an elliptical orbit moves faster when it is closer to the Sun. We explain this with the conservation of energy 能量守恒 — the total energy 能量 stays the same, so as the object's gravitational potential energy 重力势能 falls (coming closer), its kinetic energy 动能 rises (it speeds up).

    An elliptical orbit with the Sun at one focus, the planet moving fast when close and slow when far
    The Sun sits at one focus of the ellipse; the planet speeds up as it comes closer and slows down as it moves away

    Light travel time

    Distances in space are huge, so we often work out how long light takes to cross them. Light travels at $3.0 \times 10^8\ \text{m/s}$. Using $\text{time} = \dfrac{\text{distance}}{\text{speed}}$, light from the Sun (about $1.5 \times 10^{11}\ \text{m}$ away) takes about $500\ \text{s}$, which is roughly $8$ minutes, to reach the Earth.

    Explore

    Watch the planets race

    The closer a planet is to the Sun, the faster it orbits — Mercury in 88 days, Jupiter in 12 years — because the Sun's gravity is stronger close in.

    Vocabulary Train
    English Chinese Pinyin
    Solar System 太阳系 tài yáng xì
    planet 行星 xíng xīng
    rocky 岩石 yán shí
    gaseous 气态 qì tài
    gas 气体 qì tǐ
    gas giant 气态巨行星 qì tài jù xíng xīng
    ice giant 冰巨行星 bīng jù xíng xīng
    dwarf planet 矮行星 ǎi xíng xīng
    asteroid 小行星 xiǎo xíng xīng
    satellite 卫星 wèi xīng
    comet 彗星 huì xīng
    gravity 引力 yǐn lì
    gravitational field strength 重力场强度 zhòng lì chǎng qiáng dù
    ellipse 椭圆 tuǒ yuán
    conservation of energy 能量守恒 néng liàng shǒu héng
    energy 能量 néng liàng
    gravitational potential energy 重力势能 zhòng lì shì néng
    kinetic energy 动能 dòng néng
    6.1

    How the Solar System formed

    The planets formed from a giant cloud of gas and dust 尘埃 in space, which contained many chemical elements 元素. This is the accretion 吸积 model:

    • gravity pulled the cloud together;
    • the cloud was spinning, so it flattened into a spinning accretion disc 吸积盘;
    • most of the matter fell to the centre and became the Sun, while the planets grew from the leftover material in the disc.

    Near the hot young Sun, only rock and metal could stay solid, so the inner planets are rocky. Far out, where it was cold, gases could also collect, so the outer planets grew large and gaseous.

    A glowing orange disc of dust around a young star, crossed by dark rings where planets are sweeping up material
    A real accretion disc around the young star HL Tauri: the dark gaps are where new planets are gathering up the dust — our Solar System began the same way
    Vocabulary Train
    English Chinese Pinyin
    dust 尘埃 chén āi
    element 元素 yuán sù
    accretion 吸积 xī jī
    accretion disc 吸积盘 xī jī pán
    6.2

    The Sun as a star

    Syllabus

    6.2.1 The Sun as a star

    Core Supplement
    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 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

    6.2.2 Stars

    Core Supplement
    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
    2 Know that one light-year is equal to $9.5 \times 10^{15}$ m
    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

    6.2.3 The Universe

    Core Supplement
    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
    2 Describe redshift as an increase in the observed wavelength of electromagnetic radiation emitted from receding stars and galaxies
    3 Know that the light emitted from distant galaxies appears redshifted in comparison with light emitted on the Earth
    4 Know that redshift in the light from distant galaxies is evidence that the Universe is expanding and supports the Big Bang Theory
    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)
    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
    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
    8 Know that the distance $d$ of a far galaxy can be determined using the brightness of a supernova in that galaxy
    9 Define the Hubble constant $H_0$ 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
    $$H_0 = \frac{v}{d}$$
    10 Know that the current estimate for $H_0$ is $2.2 \times 10^{-18}$ per second
    11 Know that the equation
    $$\frac{d}{v} = \frac{1}{H_0}$$
    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

    Source: Cambridge International syllabus

    The Sun is a star 恒星 of medium size, made mostly of hydrogen and helium. It radiates most of its energy in the infrared, visible light and ultraviolet 紫外线 parts of the electromagnetic spectrum 电磁波谱.

    A star is powered by nuclear reactions 核反应 in its core. In a stable star, the reaction is nuclear fusion 核聚变: hydrogen nuclei join to make helium, releasing huge amounts of energy.

    The Sun shown as a glowing orange disc with a bright prominence at the edge, imaged in ultraviolet light by NASA's Solar Dynamics Observatory
    The Sun, our nearest star, seen in ultraviolet light
    Vocabulary Train
    English Chinese Pinyin
    star 恒星 héng xīng
    hydrogen qīng
    helium hài
    ultraviolet 紫外线 zǐ wài xiàn
    electromagnetic spectrum 电磁波谱 diàn cí bō pǔ
    nuclear reaction 核反应 hé fǎn yìng
    nuclear fusion 核聚变 hé jù biàn
    6.2

    Stars, galaxies and the Universe

    A galaxy 星系 is a group of many billions of stars held together by gravity. Our Sun is one star in the galaxy called the Milky Way 银河系. All the other stars in the Milky Way are very much further from the Earth than the Sun is.

    A spiral galaxy seen face-on, with curved arms of stars winding out from a bright centre and a smaller companion galaxy at the edge
    A spiral galaxy: billions of stars held together by gravity

    Distances between stars are so big that we measure them in light-years 光年. One light-year is the distance light travels in one year (in the vacuum of space), which is about $9.5 \times 10^{15}\ \text{m}$.

    The Milky Way is about $100\,000$ light-years across (its diameter 直径). It is just one of many billions of galaxies. All of these galaxies together make up the Universe 宇宙.

    A large telescope on a mountain at night fires a thin yellow laser straight up towards the glowing band of the Milky Way
    A giant telescope studies the night sky; the laser helps it make sharp images of distant stars
    Vocabulary Train
    English Chinese Pinyin
    galaxy 星系 xīng xì
    Milky Way 银河系 yín hé xì
    light-year 光年 guāng nián
    diameter 直径 zhí jìng
    Universe 宇宙 yǔ zhòu
    6.2

    The life cycle of a star

    A star is born, lives and dies over a very long time:

    1. A star forms from an interstellar cloud 星际云 of gas and dust that contains hydrogen.
    2. Gravity pulls the cloud inwards, and it heats up. This collapsing, heating cloud is a protostar 原恒星.
    3. The protostar becomes a stable 稳定 star when the inward pull of gravity is balanced by an outward push caused by the very high temperature in its centre.
    4. In time, every star runs out of hydrogen fuel 燃料 for fusion.

    What happens next depends on the mass of the star:

    • A medium star (like the Sun) swells into a red giant 红巨星. It then throws off its outer layers as a glowing cloud called a planetary nebula 星云, leaving a small, hot white dwarf 白矮星 at the centre.
    • A much heavier star swells into a red supergiant 红超巨星 and then explodes as a supernova 超新星. This blast spreads out a nebula containing hydrogen and new, heavier elements, and leaves behind a neutron star 中子星 or a black hole 黑洞.
    A flow chart of a star's life, branching by mass into the red-giant and red-supergiant paths
    Every star begins in a nebula; how it ends depends on its mass

    The nebula from a supernova can later form new stars, with planets orbiting them — so our own Solar System came from earlier stars.

    Explore

    The life cycle of a star

    Gravity pulls a gas cloud together; fusion lights the star; when its fuel runs low it swells and finally fades.

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    The life cycle of a Sun-like star

    Step through how a star like our Sun is born, lives and dies.

    Vocabulary Train
    English Chinese Pinyin
    interstellar cloud 星际云 xīng jì yún
    protostar 原恒星 yuán héng xīng
    stable 稳定 wěn dìng
    fuel 燃料 rán liào
    red giant 红巨星 hóng jù xīng
    nebula 星云 xīng yún
    white dwarf 白矮星 bái ǎi xīng
    red supergiant 红超巨星 hóng chāo jù xīng
    supernova 超新星 chāo xīn xīng
    neutron star 中子星 zhōng zi xīng
    black hole 黑洞 hēi dòng
    6.2

    The expanding Universe

    When a star or galaxy moves away from us (it is receding 退行), the light we receive from it has a longer wavelength 波长 than normal — it is shifted towards the red end of the spectrum. This is redshift 红移.

    Two spectra: the lines of a distant galaxy shifted toward the red end compared with a nearby one
    The dark lines in a distant galaxy's spectrum are shifted toward the red end — this is redshift

    The light from distant galaxies is redshifted, and the further away a galaxy is, the bigger its redshift. This tells us that the galaxies are moving apart: the Universe is expanding 膨胀. Running this backwards, everything was once together at a single point — this is the evidence for the Big Bang 大爆炸 theory.

    Galaxies around us each with an arrow pointing away, longer arrows for the more distant galaxies
    Every galaxy is moving away from us, and the farther ones move away faster — the Universe is expanding

    More evidence and the age of the Universe

    Faint microwave 微波 radiation 辐射 is found coming from every direction in space. This is the cosmic microwave background radiation 宇宙微波背景辐射 (CMBR). It was made as high-energy radiation soon after the Big Bang, and has been stretched out into the microwave part of the spectrum as the Universe expanded.

    An oval all-sky map speckled blue and red, showing tiny temperature differences in the microwave background
    The whole sky mapped in microwaves: this faint glow reaches us from every direction as the leftover heat of the young Universe — strong evidence for the Big Bang

    For a distant galaxy:

    • its speed $v$ of moving away can be found from the redshift of its starlight;
    • its distance $d$ can be found from the brightness of a supernova seen in it.

    The Hubble constant 哈勃常数 $H_0$ links these two:

    $$H_0 = \frac{v}{d}$$

    Its value today is about $2.2 \times 10^{-18}$ per second. Turning this around gives an estimate for the age of the Universe:

    $$\frac{d}{v} = \frac{1}{H_0}$$

    Worked example. The Hubble constant is about $H_0 = 2.2 \times 10^{-18}$ per second. Estimate the age of the Universe.

    $$\frac{1}{H_0} = \frac{1}{2.2 \times 10^{-18}} \approx 4.5 \times 10^{17}\ \text{s}$$

    That is roughly $14$ billion years.

    This works because every galaxy seems to have started from the same single point at the same time — more support for the Big Bang.

    Explore

    The expanding Universe

    v = H₀·d

    Galaxies recede faster the farther they are — speed is proportional to distance.

    Vocabulary Train
    English Chinese Pinyin
    receding 退行 tuì xíng
    wavelength 波长 bō cháng
    redshift 红移 hóng yí
    expanding 膨胀 péng zhàng
    Big Bang 大爆炸 dà bào zhà
    microwave 微波 wēi bō
    radiation 辐射 fú shè
    cosmic microwave background radiation 宇宙微波背景辐射 yǔ zhòu wēi bō bèi jǐng fú shè
    Hubble constant 哈勃常数 hā bó cháng shù
    6.2

    Exam tips

    • In $v = \dfrac{2\pi r}{T}$, $r$ is the orbit radius and $T$ is the time for one full orbit in seconds — convert km to m and hours to seconds first.
    • Planets closer to the Sun feel stronger gravity, so they orbit faster and take less time. In an elliptical orbit a body speeds up as it nears the Sun (gravitational potential energy turns into kinetic energy).
    • A light-year is a distance, not a time — how far light travels in one year.
    • A star is stable when the inward pull of gravity is balanced by the outward push from the energy released by fusion in its core. What it becomes when its fuel runs out depends on its mass.
    • Redshift — light from distant galaxies shifted to longer (redder) wavelengths, with a bigger shift the further away — is the evidence that the Universe is expanding, which supports the Big Bang.

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