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Laabri

Double Science (Physics) Retrospective Revision guide

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Last updated over 1 year ago
146 Nsɛmmisa
Hyɛ no nsow a efi ɔkyerɛwfo no hɔ:

A document for students to use to identify areas of the syllabus to work on.

1 Forces and motion

(a) Units

2

(b) Movement and position

2
2
2
2
2
2
2
2

(c) Forces, movement, shape and momentum

2
2
2
2
2
2
2
2
2
2
2
2
2
2
2 Electricity

(a) Units

2

(b) Mains electricity

2
2
2
2
2

(c) Energy and voltage in circuits

2
2
2
2
2
2
2
2
2
2
2
2
2
2
2
3 Waves

(a) Units

2

(b) Properties of waves

2
2
2
2
2
2
2
2

(c) The electromagnetic spectrum

2
2
2
2

(d) Light and Sound

2
2
2
2
2
2
2
2
2
2
4 Energy resources and energy transfers

(a) Units

2

(b) Energy transfers

2
2
2
2
2
2
2
2
2

(c) Work and power

2
2
2
2
2
2
2
5 Solids, liquids and gases

(a) Units

2

(b) Density and pressure

2
2
2
2
2

(c) Ideal gas molecules

2
2
2
2
2
2
2
2
6 Magnetism and electromagnetism

(a) Units

2

(b) Magnetism

2
2
2
2
2
2

(c) Electromagnetism

2
2
2
2

(d) Electromagnetic induction

2
2
7 Radioactivity and particles

(a) Units

2

(b) Radioactivity

2
2
2
2
2
2
2
2
2
2
2
2
2
2
2

(c) Fission and fusion

2
2
2
2
2
2
2
2
2
2
8 Astrophysics

(a) Units

2

(b) Motion in the universe

2
2
2
2

(c) Stellar evolution

2
2
2
2
Asemmisa {{asɛmmisaAhyɛnsode}}
1.

1.1

use the following units: kilogram (kg), metre (m), metre/second (m/s),

metre/second2 (m/s2), newton (N), second (s) and newton/kilogram (N/kg)

Asemmisa {{asɛmmisaAhyɛnsode}}
2.

1.3

plot and explain distance−time graphs

Asemmisa {{asɛmmisaAhyɛnsode}}
3.

1.4

know and use the relationship between average speed, distance moved and time

taken:

Asemmisa {{asɛmmisaAhyɛnsode}}
4.

1.5

practical: investigate the motion of everyday objects such as toy cars or tennis balls

Asemmisa {{asɛmmisaAhyɛnsode}}
5.

1.6

know and use the relationship between acceleration, change in velocity and time

taken:

Asemmisa {{asɛmmisaAhyɛnsode}}
6.

1.7

plot and explain velocity-time graphs

Asemmisa {{asɛmmisaAhyɛnsode}}
7.

1.8

determine acceleration from the gradient of a velocity−time graph

Asemmisa {{asɛmmisaAhyɛnsode}}
8.

1.9

determine the distance travelled from the area between a velocity−time graph and

the time axis

Asemmisa {{asɛmmisaAhyɛnsode}}
9.

1.10

use the relationship between final speed, initial speed, acceleration and distance

moved:

Asemmisa {{asɛmmisaAhyɛnsode}}
10.

1.11

describe the effects of forces between bodies such as changes in speed, shape or

direction

Asemmisa {{asɛmmisaAhyɛnsode}}
11.

1.12

identify different types of force such as gravitational or electrostatic

Asemmisa {{asɛmmisaAhyɛnsode}}
12.

1.13

understand how vector quantities differ from scalar quantities

Asemmisa {{asɛmmisaAhyɛnsode}}
13.

1.14

understand that force is a vector quantity

Asemmisa {{asɛmmisaAhyɛnsode}}
14.

1.15

calculate the resultant force of forces that act along a line

Asemmisa {{asɛmmisaAhyɛnsode}}
15.

1.16

know that friction is a force that opposes motion

Asemmisa {{asɛmmisaAhyɛnsode}}
16.

1.17

know and use the relationship between unbalanced force, mass and acceleration:

force = mass × acceleration

F = m × a

Asemmisa {{asɛmmisaAhyɛnsode}}
17.

1.18

know and use the relationship between weight, mass and gravitational field strength:

weight = mass × gravitational field strength

W = m × g

Asemmisa {{asɛmmisaAhyɛnsode}}
18.

1.19

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

distance and the braking distance

Asemmisa {{asɛmmisaAhyɛnsode}}
19.

1.20

describe the factors affecting vehicle stopping distance, including speed, mass, road

condition and reaction time

Asemmisa {{asɛmmisaAhyɛnsode}}
20.

1.21

describe the forces acting on falling objects (and explain why falling objects reach a

terminal velocity)

Asemmisa {{asɛmmisaAhyɛnsode}}
21.

1.22

practical: investigate how extension varies with applied force for helical springs, metal

wires and rubber bands

Asemmisa {{asɛmmisaAhyɛnsode}}
22.

1.23

know that the initial linear region of a force-extension graph is associated with

Hooke’s law

Asemmisa {{asɛmmisaAhyɛnsode}}
23.

1.24

describe elastic behaviour as the ability of a material to recover its original shape

after the forces causing deformation have been removed

Asemmisa {{asɛmmisaAhyɛnsode}}
24.

2.1

use the following units: ampere (A), coulomb (C), joule (J), ohm (Ω), second (s),

volt (V) and watt (W)

Asemmisa {{asɛmmisaAhyɛnsode}}
25.

2.2

understand how the use of insulation, double insulation, earthing, fuses and circuit

breakers protects the device or user in a range of domestic appliances

Asemmisa {{asɛmmisaAhyɛnsode}}
26.

2.3

understand why a current in a resistor results in the electrical transfer of energy and

an increase in temperature, and how this can be used in a variety of domestic

contexts

Asemmisa {{asɛmmisaAhyɛnsode}}
27.

2.4

know and use the relationship between power, current and voltage:

power = current × voltage

P = I × V

and apply the relationship to the selection of appropriate fuses

Asemmisa {{asɛmmisaAhyɛnsode}}
28.

2.5

use the relationship between energy transferred, current, voltage and time:

energy transferred = current × voltage × time

E = I × V x t

Asemmisa {{asɛmmisaAhyɛnsode}}
29.

2.6

know the difference between mains electricity being alternating current (a.c.) and

direct current (d.c.) being supplied by a cell or battery

Asemmisa {{asɛmmisaAhyɛnsode}}
30.

2.7

explain why a series or parallel circuit is more appropriate for particular applications,

including domestic lighting

Asemmisa {{asɛmmisaAhyɛnsode}}
31.

2.8

understand how the current in a series circuit depends on the applied voltage and the

number and nature of other components

Asemmisa {{asɛmmisaAhyɛnsode}}
32.

2.9

describe how current varies with voltage in wires, resistors, metal filament lamps and

diodes, and how to investigate this experimentally

Asemmisa {{asɛmmisaAhyɛnsode}}
33.

2.10

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

Asemmisa {{asɛmmisaAhyɛnsode}}
34.

2.11

describe the qualitative variation of resistance of light-dependent resistors (LDRs)

with illumination and of thermistors with temperature

Asemmisa {{asɛmmisaAhyɛnsode}}
35.

2.12

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

circuit

Asemmisa {{asɛmmisaAhyɛnsode}}
36.

2.13

know and use the relationship between voltage, current and resistance:

voltage = current × resistance

V = I × R

Asemmisa {{asɛmmisaAhyɛnsode}}
37.

2.14

know that current is the rate of flow of charge

Asemmisa {{asɛmmisaAhyɛnsode}}
38.

2.15

know and use the relationship between charge, current and time:

charge = current × time

Q = I × t

Asemmisa {{asɛmmisaAhyɛnsode}}
39.

2.16

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

electrons

Asemmisa {{asɛmmisaAhyɛnsode}}
40.

2.17

understand why current is conserved at a junction in a circuit

Asemmisa {{asɛmmisaAhyɛnsode}}
41.

2.18

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

Asemmisa {{asɛmmisaAhyɛnsode}}
42.

2.19

calculate the currents, voltages and resistances of two resistive components

connected in a series circuit

Asemmisa {{asɛmmisaAhyɛnsode}}
43.

2.20

know that:

• voltage is the energy transferred per unit charge passed

• the volt is a joule per coulomb.

Asemmisa {{asɛmmisaAhyɛnsode}}
44.

2.21

know and use the relationship between energy transferred, charge and voltage:

energy transferred = charge × voltage

E = Q × V

Asemmisa {{asɛmmisaAhyɛnsode}}
45.

3.1

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

second (s)

Asemmisa {{asɛmmisaAhyɛnsode}}
46.

3.2

explain the difference between longitudinal and transverse waves

Asemmisa {{asɛmmisaAhyɛnsode}}
47.

3.3

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

wave

Asemmisa {{asɛmmisaAhyɛnsode}}
48.

3.4

know that waves transfer energy and information without transferring matter

Asemmisa {{asɛmmisaAhyɛnsode}}
49.

3.5

know and use the relationship between the speed, frequency and wavelength of a

wave:

wave speed = frequency × wavelength

v = f × λ

Asemmisa {{asɛmmisaAhyɛnsode}}
50.

3.6

use the relationship between frequency and time period:

Asemmisa {{asɛmmisaAhyɛnsode}}
51.

3.7

use the above relationships in different contexts including sound waves and

electromagnetic waves

Asemmisa {{asɛmmisaAhyɛnsode}}
52.

3.8

explain why there is a change in the observed frequency and wavelength of a wave

when its source is moving relative to an observer, and that this is known as the

Doppler effect

Asemmisa {{asɛmmisaAhyɛnsode}}
53.

3.9

explain that all waves can be reflected and refracted

Asemmisa {{asɛmmisaAhyɛnsode}}
54.

3.10

know that light is part of a continuous electromagnetic spectrum that includes radio,

microwave, infrared, visible, ultraviolet, x-ray and gamma ray radiations and that all

these waves travel at the same speed in free space

Asemmisa {{asɛmmisaAhyɛnsode}}
55.

3.11

know the order of the electromagnetic spectrum in terms of decreasing wavelength

and increasing frequency, including the colours of the visible spectrum

Asemmisa {{asɛmmisaAhyɛnsode}}
56.

3.12

explain some of the uses of electromagnetic radiations, including:

• radio waves: broadcasting and communications

• microwaves: cooking and satellite transmissions

• infrared: heaters and night vision equipment

• visible light: optical fibres and photography

• ultraviolet: fluorescent lamps

• x-rays: observing the internal structure of objects and materials, including for

medical applications

• gamma rays: sterilising food and medical equipment.

Asemmisa {{asɛmmisaAhyɛnsode}}
57.

3.13

explain the detrimental effects of excessive exposure of the human body to

electromagnetic waves, including:

• microwaves: internal heating of body tissue

• infrared: skin burns

• ultraviolet: damage to surface cells and blindness

• gamma rays: cancer, mutation and describe simple protective measures against the risks

Asemmisa {{asɛmmisaAhyɛnsode}}
58.

3.14

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

refracted

Asemmisa {{asɛmmisaAhyɛnsode}}
59.

3.15

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

Asemmisa {{asɛmmisaAhyɛnsode}}
60.

3.16

draw ray diagrams to illustrate reflection and refraction

Asemmisa {{asɛmmisaAhyɛnsode}}
61.

3.17

practical: investigate the refraction of light, using rectangular blocks, semi-circular

blocks and triangular prisms

Asemmisa {{asɛmmisaAhyɛnsode}}
62.

3.18

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

of refraction:

Asemmisa {{asɛmmisaAhyɛnsode}}
63.

3.19

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

Asemmisa {{asɛmmisaAhyɛnsode}}
64.

3.20

describe the role of total internal reflection in transmitting information along optical

fibres and in prisms

Asemmisa {{asɛmmisaAhyɛnsode}}
65.

3.21

explain the meaning of critical angle c

Asemmisa {{asɛmmisaAhyɛnsode}}
66.

3.22

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

Asemmisa {{asɛmmisaAhyɛnsode}}
67.

3.23

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

Asemmisa {{asɛmmisaAhyɛnsode}}
68.

4.1

use the following units: kilogram (kg), joule (J), metre (m), metre/second (m/s),

metre/second2 (m/s2), newton (N), second (s) and watt (W)

Asemmisa {{asɛmmisaAhyɛnsode}}
69.

4.2

describe energy transfers involving energy stores:

• energy stores: chemical, kinetic, gravitational, elastic, thermal, magnetic, electrostatic, nuclear

• energy transfers: mechanically, electrically, by heating, by radiation (light and sound)

Asemmisa {{asɛmmisaAhyɛnsode}}
70.

4.3

use the principle of conservation of energy

Asemmisa {{asɛmmisaAhyɛnsode}}
71.

4.4

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

energy output:

Asemmisa {{asɛmmisaAhyɛnsode}}
72.

4.5

describe a variety of everyday and scientific devices and situations, explaining the

transfer of the input energy in terms of the above relationship, including their

representation by Sankey diagrams

Asemmisa {{asɛmmisaAhyɛnsode}}
73.

4.6

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

radiation

Asemmisa {{asɛmmisaAhyɛnsode}}
74.

4.7

explain the role of convection in everyday phenomena

Asemmisa {{asɛmmisaAhyɛnsode}}
75.

4.8

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

temperature

Asemmisa {{asɛmmisaAhyɛnsode}}
76.

4.9

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

Asemmisa {{asɛmmisaAhyɛnsode}}
77.

4.10

explain ways of reducing unwanted energy transfer, such as insulation

Asemmisa {{asɛmmisaAhyɛnsode}}
78.

4.11

know and use the relationship between work done, force and distance moved in the

direction of the force:

work done = force × distance moved

W = F × d

Asemmisa {{asɛmmisaAhyɛnsode}}
79.

4.12

know that work done is equal to energy transferred

Asemmisa {{asɛmmisaAhyɛnsode}}
80.

4.13

know and use the relationship between gravitational potential energy, mass,

gravitational field strength and height:

gravitational potential energy = mass × gravitational field strength × height

GPE = m × g × h

Asemmisa {{asɛmmisaAhyɛnsode}}
81.

4.14

know and use the relationship:

Asemmisa {{asɛmmisaAhyɛnsode}}
82.

4.15

understand how conservation of energy produces a link between gravitational

potential energy, kinetic energy and work

Asemmisa {{asɛmmisaAhyɛnsode}}
83.

4.16

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

Asemmisa {{asɛmmisaAhyɛnsode}}
84.

4.17

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

Asemmisa {{asɛmmisaAhyɛnsode}}
85.

5.1

use the following units: degree Celsius (°C), Kelvin (K), joule (J), kilogram (kg),

kilogram/metre3 (kg/m3), metre (m), metre2 (m2), metre3 (m3), metre/second (m/s),

metre/second2 (m/s2), newton (N) and pascal (Pa)

Asemmisa {{asɛmmisaAhyɛnsode}}
86.

5.3

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

Asemmisa {{asɛmmisaAhyɛnsode}}
87.

5.4

practical: investigate density using direct measurements of mass and volume

Asemmisa {{asɛmmisaAhyɛnsode}}
88.

5.5

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

Asemmisa {{asɛmmisaAhyɛnsode}}
89.

5.6

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

directions

Asemmisa {{asɛmmisaAhyɛnsode}}
90.

5.7

know and use the relationship for pressure difference:

pressure difference = height × density × gravitational field strength

p = h × ρ × g

Asemmisa {{asɛmmisaAhyɛnsode}}
91.

5.15

explain how molecules in a gas have random motion and that they exert a force and

hence a pressure on the walls of a container

Asemmisa {{asɛmmisaAhyɛnsode}}
92.

5.16

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

Asemmisa {{asɛmmisaAhyɛnsode}}
93.

5.17

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

and Celsius scales

Asemmisa {{asɛmmisaAhyɛnsode}}
94.

5.18

understand why an increase in temperature results in an increase in the average

speed of gas molecules

Asemmisa {{asɛmmisaAhyɛnsode}}
95.

5.19

know that the Kelvin temperature of a gas is proportional to the average kinetic

energy of its molecules

Asemmisa {{asɛmmisaAhyɛnsode}}
96.

5.20

explain, for a fixed amount of gas, the qualitative relationship between:

• pressure and volume at constant temperature

• pressure and Kelvin temperature at constant volume.

Asemmisa {{asɛmmisaAhyɛnsode}}
97.

5.21

use the relationship between the pressure and Kelvin temperature of a fixed mass of

gas at constant volume:

Asemmisa {{asɛmmisaAhyɛnsode}}
98.

5.22

use the relationship between the pressure and volume of a fixed mass of gas at

constant temperature:

p1V1 = p2V2

Asemmisa {{asɛmmisaAhyɛnsode}}
99.

6.1

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

Asemmisa {{asɛmmisaAhyɛnsode}}
100.

6.2

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

Asemmisa {{asɛmmisaAhyɛnsode}}
101.

6.3

describe the properties of magnetically hard and soft materials

Asemmisa {{asɛmmisaAhyɛnsode}}
102.

6.4

understand the term magnetic field line

Asemmisa {{asɛmmisaAhyɛnsode}}
103.

6.5

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

magnetic field

Asemmisa {{asɛmmisaAhyɛnsode}}
104.

6.6

practical: investigate the magnetic field pattern for a permanent bar magnet and

between two bar magnets

Asemmisa {{asɛmmisaAhyɛnsode}}
105.

6.7

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

pattern

Asemmisa {{asɛmmisaAhyɛnsode}}
106.

6.8

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

Asemmisa {{asɛmmisaAhyɛnsode}}
107.

6.12

understand why a force is exerted on a current-carrying wire in a magnetic field, and

how this effect is applied in simple d.c. electric motors and loudspeakers

Asemmisa {{asɛmmisaAhyɛnsode}}
108.

6.13

use the left-hand rule to predict the direction of the resulting force when a wire

carries a current perpendicular to a magnetic field

Asemmisa {{asɛmmisaAhyɛnsode}}
109.

6.14

describe how the force on a current-carrying conductor in a magnetic field changes

with the magnitude and direction of the field and current

Asemmisa {{asɛmmisaAhyɛnsode}}
110.

6.15

know that a voltage is induced in a conductor or a coil when it moves through a

magnetic field or when a magnetic field changes through it and describe the factors

that affect the size of the induced voltage

Asemmisa {{asɛmmisaAhyɛnsode}}
111.

6.16

describe the generation of electricity by the rotation of a magnet within a coil of wire

and of a coil of wire within a magnetic field and describe the factors that affect the

size of the induced voltage

Asemmisa {{asɛmmisaAhyɛnsode}}
112.

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

second (s)

Asemmisa {{asɛmmisaAhyɛnsode}}
113.

7.2

describe the structure of an atom in terms of protons, neutrons and electrons and use

symbols such as

to describe particular nuclei

Asemmisa {{asɛmmisaAhyɛnsode}}
114.

7.3

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

Asemmisa {{asɛmmisaAhyɛnsode}}
115.

7.4

know that alpha (α) particles, beta (β−) particles, and gamma (γ) rays are ionising

radiations emitted from unstable nuclei in a random process

Asemmisa {{asɛmmisaAhyɛnsode}}
116.

7.5

describe the nature of alpha (α) particles, beta (β−) particles, and gamma (γ) rays,

and recall that they may be distinguished in terms of penetrating power and ability to

ionise

Asemmisa {{asɛmmisaAhyɛnsode}}
117.

7.6

practical: investigate the penetration powers of different types of radiation using

either radioactive sources or simulations

Asemmisa {{asɛmmisaAhyɛnsode}}
118.

7.7

describe the effects on the atomic and mass numbers of a nucleus of the emission of

each of the four main types of radiation (alpha, beta, gamma and neutron radiation)

Asemmisa {{asɛmmisaAhyɛnsode}}
119.

7.8

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

Asemmisa {{asɛmmisaAhyɛnsode}}
120.

7.9

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

Asemmisa {{asɛmmisaAhyɛnsode}}
121.

7.10

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

Asemmisa {{asɛmmisaAhyɛnsode}}
122.

7.11

know that the activity of a radioactive source decreases over a period of time and is

measured in becquerels

Asemmisa {{asɛmmisaAhyɛnsode}}
123.

7.12

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

radioactive isotopes

Asemmisa {{asɛmmisaAhyɛnsode}}
124.

7.13

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

graphical methods

Asemmisa {{asɛmmisaAhyɛnsode}}
125.

7.14

describe uses of radioactivity in industry and medicine

Asemmisa {{asɛmmisaAhyɛnsode}}
126.

7.15

describe the difference between contamination and irradiation

Asemmisa {{asɛmmisaAhyɛnsode}}
127.

7.16

describe the dangers of ionising radiations, including:

• that radiation can cause mutations in living organisms

• that radiation can damage cells and tissue

• the problems arising from the disposal of radioactive waste and how the

associated risks can be reduced.

Asemmisa {{asɛmmisaAhyɛnsode}}
128.

7.17

know that nuclear reactions, including fission, fusion and radioactive decay, can be a

source of energy

Asemmisa {{asɛmmisaAhyɛnsode}}
129.

7.18

understand how a nucleus of U-235 can be split (the process of fission) by collision

with a neutron, and that this process releases energy as kinetic energy of the fission

products

Asemmisa {{asɛmmisaAhyɛnsode}}
130.

7.19

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

number of neutrons

Asemmisa {{asɛmmisaAhyɛnsode}}
131.

7.20

describe how a chain reaction can be set up if the neutrons produced by one fission

strike other U-235 nuclei

Asemmisa {{asɛmmisaAhyɛnsode}}
132.

7.21

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

Asemmisa {{asɛmmisaAhyɛnsode}}
133.

7.22

understand the role of shielding around a nuclear reactor

Asemmisa {{asɛmmisaAhyɛnsode}}
134.

7.23

explain the difference between nuclear fusion and nuclear fission

Asemmisa {{asɛmmisaAhyɛnsode}}
135.

7.24

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

Asemmisa {{asɛmmisaAhyɛnsode}}
136.

7.25

know that fusion is the energy source for stars

Asemmisa {{asɛmmisaAhyɛnsode}}
137.

7.26

explain why nuclear fusion does not happen at low temperatures and pressures, due

to electrostatic repulsion of protons

Asemmisa {{asɛmmisaAhyɛnsode}}
138.

8.1

use the following units: kilogram (kg), metre (m), metre/second (m/s),

metre/second2 (m/s2), newton (N), second (s), newton/kilogram (N/kg)

Asemmisa {{asɛmmisaAhyɛnsode}}
139.

8.2

know that:

• the universe is a large collection of billions of galaxies

• a galaxy is a large collection of billions of stars

• our solar system is in the Milky Way galaxy.

Asemmisa {{asɛmmisaAhyɛnsode}}
140.

8.3

understand why gravitational field strength, g, varies and know that it is different on

other planets and the Moon from that on the Earth.

Asemmisa {{asɛmmisaAhyɛnsode}}
141.

8.4

explain that gravitational force:

• causes moons to orbit planets

• causes the planets to orbit the Sun

• causes artificial satellites to orbit the Earth

• causes comets to orbit the Sun.

Asemmisa {{asɛmmisaAhyɛnsode}}
142.

8.6

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

Asemmisa {{asɛmmisaAhyɛnsode}}
143.

8.7

understand how stars can be classified according to their colour

Asemmisa {{asɛmmisaAhyɛnsode}}
144.

8.8

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

Asemmisa {{asɛmmisaAhyɛnsode}}
145.

8.9

describe the evolution of stars of similar mass to the Sun through the following

stages:

• nebula

• star (main sequence)

• red giant

• white dwarf

Asemmisa {{asɛmmisaAhyɛnsode}}
146.

8.10

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