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Q 1/225
Score 0
Meters per second, m/s
30
The units of speed are
Q 2/225
Score 0
The speed
30
On a distance - time graph, the gradient tells you...
225 questions
Q.
Meters per second, m/s
1
30 sec
Q.
The speed
2
30 sec
Q.
The object is not moving
3
30 sec
Q.
The object is moving at a constant speed
4
30 sec
Q.
The object is accelerating
5
30 sec
Q.
It must specify a direction.
6
30 sec
Q.
See image
7
30 sec
Q.
Meters per second, m/s (the same as speed)
8
30 sec
Q.
Meters per second squared, m/s^2
9
30 sec
Q.
The rate if acceleration
10
30 sec
Q.
The object is traveling at a steady speed.
11
30 sec
Q.
The object has a constant rate if acceleration or deceleration
12
30 sec
Q.
The rate if acceleration is increasing (or decreasing).
13
30 sec
Q.
The distance travelled
14
30 sec
Q.
Newtons
15
30 sec
Q.
Equal and opposite forces on each other.
16
30 sec
Q.
The table exerts an equal upwards force on the book.
17
30 sec
Q.
An object generally has lots of different forces acting on it at the same time.
18
30 sec
Q.
See image
19
30 sec
Q.
The object remains stationary
20
30 sec
Q.
The object will continue to move at the same steady speed in the same direction.
21
30 sec
Q.
The object will accelerate in the direction of the resultant force.
22
30 sec
Q.
If the force is in the same direction that the object is moving, the object will accelerate.
23
30 sec
Q.
See image
24
30 sec
Q.
The faster the car, the greater forwards force it has, meaning that a larger deceleration is required.
25
30 sec
Q.
Thinking distance and braking distance.
26
30 sec
Q.
The distance a car travels between the driver noticing the stimulus and applying the brakes.
27
30 sec
Q.
Driver being drunk, tired or under the influence of drugs.
28
30 sec
Q.
The distance a car travels between application of brakes and coming to a complete stop.
29
30 sec
Q.
Poorly maintained roads
30
30 sec
Q.
See image
31
30 sec
Q.
See image
32
30 sec
Q.
A resultant force must be acting on it.
33
30 sec
Q.
Gravity
34
30 sec
Q.
The amount a falling object accelerates due to the force of gravity.
35
30 sec
Q.
See image
36
30 sec
Q.
Newtons per kilogram, N/kg.
37
30 sec
Q.
An object falls through a fluid (liquid/gas).
38
30 sec
Q.
See image
39
30 sec
Q.
See image
40
30 sec
Q.
See image
41
30 sec
Q.
See image
42
30 sec
Q.
Make vehicle more streamlined > reduces air resistance > less fuel required to move it.
43
30 sec
Q.
See image
44
30 sec
Q.
The increase in an object's length from its original length when a stretching force is applied to it.
45
30 sec
Q.
Will return to its original shape after being deformed.
46
30 sec
Q.
Extension is directly proportional to the force applied, providing the limit of proportionality is not exceeded.
47
30 sec
Q.
The maximum force that can be applied to an elastic object before it will not return to its original shape after being deformed.
48
30 sec
Q.
When an object is stretched, work is done.
49
30 sec
Q.
See image
50
30 sec
Q.
See image
51
30 sec
Q.
A force must be being applied to it.
52
30 sec
Q.
See image
53
30 sec
Q.
The energy stored in an object because of its position in the Earth's gravitational field.
54
30 sec
Q.
See image
55
30 sec
Q.
The rate of energy transfer (in Joules per second).
56
30 sec
Q.
See image
57
30 sec
Q.
Watts, W
58
30 sec
Q.
Greater mass
59
30 sec
Q.
See image
60
30 sec
Q.
Kilogram-meters per second, kgm/s.
61
30 sec
Q.
See image
62
30 sec
Q.
When objects interact (collide), the total momentum before (as they move towards each other) is equal to the total momentum after (as they bounce apart/move off together).
63
30 sec
Q.
See image
64
30 sec
Q.
See image
65
30 sec
Q.
- shorter impact time
66
30 sec
Q.
See image
67
30 sec
Q.
See image
68
30 sec
Q.
Areas manufactured at the front and rear of cars, designed to fold up in a collision.
69
30 sec
Q.
See image
70
30 sec
Q.
A poor conductor of electricity
71
30 sec
Q.
Two insulators are rubbed together
72
30 sec
Q.
See image
73
30 sec
Q.
See image
74
30 sec
Q.
See image
75
30 sec
Q.
Required to push electrons around a complete circuit
76
30 sec
Q.
Two or more cells
77
30 sec
Q.
Enables the current to be broken
78
30 sec
Q.
Emits light as a sign that current is passing through/as a source of light.
79
30 sec
Q.
Only allows current through in one direction
80
30 sec
Q.
Only allows current through in one direction AND emits light when a current passes through
81
30 sec
Q.
Measures electrical current through a component
82
30 sec
Q.
See image
83
30 sec
Q.
Limits the current in the circuit
84
30 sec
Q.
Allows the current in the circuit ti be varied
85
30 sec
Q.
Contains a wire of specific thickness which melts if to great a current flows through, breaking the circuit. A safety feature, e.g. to prevent surges.
86
30 sec
Q.
Transfers electrical energy to thermal energy, heating the surroundings
87
30 sec
Q.
Measures potential difference across a component
88
30 sec
Q.
See image
89
30 sec
Q.
The rate of flow of charge (unit: Coulombs) past a point.
90
30 sec
Q.
See image
91
30 sec
Q.
The amount of energy transferred to a component (or work done on a component) per coulomb of charge flowing though it.
92
30 sec
Q.
See image
93
30 sec
Q.
The opposition to the flow of current.
94
30 sec
Q.
See image
95
30 sec
Q.
More energy is transferred to the component = greater resistance.
96
30 sec
Q.
Less energy transferred to the component = lower resistance.
97
30 sec
Q.
The current through a component/resistor is directly proportional to the potential difference across it (if the resistor is kept at a constant temperature).
98
30 sec
Q.
Increase current > temperature increases > resistance increases.
99
30 sec
Q.
Brighter light = lower resistance
100
30 sec
Q.
Higher temperature = lower resistance (opposite to all other resistors).
101
30 sec
Q.
All components are connected one after the other.
102
30 sec
Q.
See image
103
30 sec
Q.
Current is the same through all components (because there is no choice of route for charge).
104
30 sec
Q.
The potential differences of all components in the circuit add up to the potential difference of the supply.
105
30 sec
Q.
See image
106
30 sec
Q.
The resistances all components in the circuit add up to the total resistance of the circuit.
107
30 sec
Q.
Components are connected across the supply, creating separate loops.
108
30 sec
Q.
See image
109
30 sec
Q.
Different amounts of current can flow through different components (because there are junctions in the circuit).
110
30 sec
Q.
See image
111
30 sec
Q.
See image
112
30 sec
Q.
Every component's potential difference is the same (because they are all connected across the supply p.d.).
113
30 sec
Q.
Greater resistance = less current
114
30 sec
Q.
Supplied by cells and batteries.
115
30 sec
Q.
See image
116
30 sec
Q.
Supplied by the mains.
117
30 sec
Q.
See image
118
30 sec
Q.
How many full wavelengths pass a point in one second.
119
30 sec
Q.
See image
120
30 sec
Q.
50 Hz; changes direction 50 times per second.
121
30 sec
Q.
Between +325 and -325 volts
122
30 sec
Q.
230 Volts
123
30 sec
Q.
Brown, goes to the right
124
30 sec
Q.
Green and yellow stripy, in the middle
125
30 sec
Q.
Blue, goes to left
126
30 sec
Q.
If live wire touches the appliance's metal case, it could give you an
127
30 sec
Q.
See image
128
30 sec
Q.
See image
129
30 sec
Q.
The appliance is double-insulated
130
30 sec
Q.
An electromagnetic switch which cuts off the supply if the current exceeds a certain value
131
30 sec
Q.
A "residual current circuit breaker".
132
30 sec
Q.
See image
133
30 sec
Q.
Unstable
134
30 sec
Q.
Radioactive decay, where it emits radiation and turns into another elements.
135
30 sec
Q.
Unpredictable and random
136
30 sec
Q.
See image
137
30 sec
Q.
Is around us all the time
138
30 sec
Q.
See image
139
30 sec
Q.
When nuclear radiation passes through a material and collides with its atoms, knocking off electrons. This makes the atoms ions.
140
30 sec
Q.
See image
141
30 sec
Q.
The nucleus emits an alpha particle. Its mass number decreases by 4.
142
30 sec
Q.
See image
143
30 sec
Q.
2 protons and 2 neutrons
144
30 sec
Q.
See image
145
30 sec
Q.
See image
146
30 sec
Q.
They are relatively large, so have lots of collisions with the atoms of the material they pass through.
147
30 sec
Q.
See image
148
30 sec
Q.
See image
149
30 sec
Q.
See image
150
30 sec
Q.
- sheet of paper
151
30 sec
Q.
See image
152
30 sec
Q.
See image
153
30 sec
Q.
Smoke alarms
154
30 sec
Q.
See image
155
30 sec
Q.
See image
156
30 sec
Q.
A neutron in the nucleus changes into an electron and a proton. The electron is emitted from the nucleus.
157
30 sec
Q.
See image
158
30 sec
Q.
See image
159
30 sec
Q.
One high speed electron
160
30 sec
Q.
See image
161
30 sec
Q.
See image
162
30 sec
Q.
They are much smaller and faster than alpha particles, so have fewer collisions with the atoms of the material they pass through.
163
30 sec
Q.
See image
164
30 sec
Q.
See image
165
30 sec
Q.
See image
166
30 sec
Q.
- thin sheet of aluminium
167
30 sec
Q.
See image
168
30 sec
Q.
Monitoring thickness of paper/foil by measuring how much radiation passes through.
169
30 sec
Q.
See image
170
30 sec
Q.
The nucleus emits an electromagnetic wave
171
30 sec
Q.
Have no mass and no charge, so there is no change in mass number or atomic number.
172
30 sec
Q.
Rays can travel very deep into a material before hitting an atom.
173
30 sec
Q.
See image
174
30 sec
Q.
See image
175
30 sec
Q.
- several centimeters of lead
176
30 sec
Q.
See image
177
30 sec
Q.
Tracers in medicine. Swallowed and external detector tracks progress through body.
178
30 sec
Q.
See image
179
30 sec
Q.
Believed that the atom is a sphere of positive charge with negative electrons stuck in.
180
30 sec
Q.
They fired alpha particles at a thin sheet of gold foil.
181
30 sec
Q.
Most alpha particles passed straight through the foil.
182
30 sec
Q.
See image
183
30 sec
Q.
Some alpha particles were deflected through small angles.
184
30 sec
Q.
See image
185
30 sec
Q.
A few alpha particles rebounded through very large angles.
186
30 sec
Q.
See image
187
30 sec
Q.
The number of nuclei that decay per second.
188
30 sec
Q.
More reactive material.
189
30 sec
Q.
The time taken for the number of unstable nuclei in the sample to halve.
190
30 sec
Q.
See image
191
30 sec
Q.
Finds age of ancient objects
192
30 sec
Q.
Finds age of organic material e.g. Wood
193
30 sec
Q.
Finds age of igneous rocks
194
30 sec
Q.
Uranium-235 and Plutonium-239
195
30 sec
Q.
Neutron fired at nucleus > nucleus absorbs neutron > nucleus splits into 2 or 3 smaller nuclei > 2 or 3 neutrons are released > lots of energy released (much more than burning fossil fuels) > neutrons released can hit other nuclei and start a chain reaction!!! Has to be carefully controlled.
196
30 sec
Q.
Forcing two nuclei together by making them collide at very high speed so they form a single larger nucleus.
197
30 sec
Q.
See image
198
30 sec
Q.
Nuclei are positively charged > repel each other > requires huge amounts of energy to force them together > need to be heated to enormous temperatures > has to be contained in a magnetic field.
199
30 sec
Q.
See image
200
30 sec
Q.
- radon gas, seeping through ground from radioactive substances in rocks underground. Alpha particles, health hazard if inhaled.
201
30 sec
Q.
See image
202
30 sec
Q.
See image
203
30 sec
Q.
See image
204
30 sec
Q.
See image
205
30 sec
Q.
See image
206
30 sec
Q.
Re-used, but leftover radioactive waste has to be stored in secure conditions for many years to stop it contaminating the environment.
207
30 sec
Q.
- keep as far away from sources as possible
208
30 sec
Q.
See image
209
30 sec
Q.
See image
210
30 sec
Q.
Created by the Big Bang
211
30 sec
Q.
See image
212
30 sec
Q.
The Universe was a hot glowing ball of radiation. The nuclei of the lightest elements formed.
213
30 sec
Q.
The Universe expanded and cooled. Uncharged atoms were formed.
214
30 sec
Q.
A dark patchy cloud of hydrogen and helium. Dust and gas was pulled together by gravity to form stars.
215
30 sec
Q.
Intense heat. It was hot enough to start nuclear fusion. Stars began to emit visible light and other radiation.
216
30 sec
Q.
See image
217
30 sec
Q.
Cloud of dust and gas > pulled together by gravity > forms a PROTOSTAR > becomes denser > hydrogen and other light elements start nuclear fusion > energy released > star gets hotter and brighter > outward force of radiation is equal to inward force of gravity > star is stable. MAIN SEQUENCE STAR.
218
30 sec
Q.
Runs out of hydrogen nuclei > unbalanced forces pull star in so fast that temperature rockets > star expands and cools > RED GIANT > helium and other light elements fuse to form heavier elements > fusion stops > star contracts > WHITE DWARF > no more light emitted > star becomes denser > BLACK DWARF.
219
30 sec
Q.
Runs out of hydrogen nuclei > unbalanced forces pull star in so fast that temperature rockets > star expands and cools > RED SUPERGIANT > collapses > explodes > SUPERNOVA > outer layers thrown out into space > core remains > NEUTRON STAR (very very dense) > if neutron star is big enough it becomes a BLACK HOLE (gravity so strong not even light can escape).
220
30 sec
Q.
By fusion processes in stars.
221
30 sec
Q.
See image
222
30 sec
Q.
See image
223
30 sec
Q.
In the final stages of a massive star's life when there is enough energy. Then they are distributed through space by the supernova explosion.
224
30 sec
Q.
Heavier elements than iron are present in the sun and planets.