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20 April 2017
Heat
transfer
Evaporation
Formulae
Checking
answers
Generating
Electricity
Efficiency
Interpreting
graphs
How science
works
Red-shift
Infrared
Radiation
Particles
Heating/
Insulation
Electrical
Energy
Waves
EM
Spectrum
Big Bang
20 April 2017
Energy transfer by heating
• 3 methods – conduction, convection, radiation
• The bigger the temperature difference
between an object and its surroundings, the
faster the rate at which energy is
transferred by heating.
• Rate of transfer of energy depends on
surface area and volume, object materials,
surfaces.
Back
20 April 2017
Infrared Radiation
• All objects emit and absorb infrared
• The hotter an object is, the more IR it emits
in a given time (time is important!)
• Dark, matt surfaces – good absorbers, good
emitters (this means that a dark, matt object will heat
up faster or cool down faster than a light, shiny one)
• Light, shiny surfaces – poor absorbers, poor
emitters, good reflectors.
Back
20 April 2017
Particles
Back
Conduction, convection,
evaporation and
condensation all
transfer energy, and all
involve particles in
their theories.
In an object, the
more kinetic energy
the particles have,
the hotter the
object is.
Conduction
All to do with particles
banging into each other
and passing on KE.
Metals have free
electrons which can also
pass on KE, making
metals excellent
conductors. The
arrangement of
particles in a substance
determine how good a
conductor it is.
Convection Takes place in liquids and gases.
When a liquid or gas gets hotter, the
particles have more KE  they move around
more, making the liquid or gas less dense.
Therefore, hot liquids or gases will rise above
cooler liquids or gases. (HEAT DOES NOT RISE, HOT
LIQUIDS AND GASES DO!!)
Particle arrangements:
Solid – fixed in place, least amount of KE but still some movement
Liquid – some fixed arrangement, free to slide over each other, more KE
than solid
Gas – free to move about randomly, no fixed arrangement, lots of KE
20 April 2017
Evaporation
Back
Particles in a
liquid are held
together by
forces
The particles
need lots of
kinetic energy
to overcome
these forces
Particles can gain
kinetic energy through
heating but that
energy has to come
from somewhere
Liquids on your skin get the
energy they need for
evaporation from your skin.
So your skin is losing
energy through heating
the particles and it will
feel colder.
If particles are leaving
the liquid on your skin
through evaporation,
they are taking kinetic
energy with them.
The average kinetic
energy of the liquid on
your skin has dropped.
20 April 2017
Heating and Insulation
Back
Insulation materials
aim to reduce energy
transfer by heating –
they may reduce
conduction,
convection, and
radiation.
New heating systems or insulation for a
house cost money. The payback time of an
investment tells you how long it will take to
get your money back based on how much the
investment saves you.
Payback time = initial investment
saving per year
Liquids on your skin get the
energy they need for
evaporation from your skin.Insulation materials for homes
(including double glazing) are
often given a U-value. This is a
measure of how effective the
insulator is. The lower the U-
value, the better the material
is as an insulator.
Solar panels sometimes contain
water that is heated by the
Sun. The pipes in a solar panel
are often black. The hot water
can be used for heating.
20 April 2017
Efficiency
• Two formulae (you’ll be given both)
• Efficiency = useful energy out (x 100%)
total energy in
• Efficiency = useful power out (x 100%)
total power in
• You might need to rearrange these and put
in the numbers.
• Answers can be given either as a
percentage (e.g. 30%) or as a decimal (0.3)
 DO NOT combine these (e.g. 0.3%)
20 April 2017
Efficiency
• Sankey diagrams are often used to show
efficiency
• Efficient:
• Not efficient:
Back
Most energy is
transferred to
a useful form.
Most energy is
transferred to a non-
useful form – it is wasted.
The ratio of useful energy
transferred to total energy in gives
you the efficiency of the machine
represented by the Sankey diagram.
20 April 2017
Generating Electricity
BackBack
Power stations heat
water to make
steam  steam
turns a turbine 
the turbine spins a
generator
Heat can be
generated by:
burning fossil fuels
nuclear fission
burning biofuels
Heat can be
generated by:
burning fossil fuels
nuclear fission
burning biofuels
Water and wind can
drive a turbine directly
(no need for heating)
Small-scale
generation is useful
in remote areas.
The Sun’s energy can
be used to generate
electricity (either by
heating water or
directly)
Different methods
of generating have
different effects on
the atmosphere
Different methods
of generating have
different effects on
the atmosphere
National grid – a grid of
cables and transformers
transferring electrical
energy around the country
National grid – a grid of
cables and transformers
transferring electrical
energy around the country
Step-up transformer  voltage up,
current down  lower current means
less heating in cables  less energy
wasted in the cables
Step-up transformer  voltage up,
current down  lower current means
less heating in cables  less energy
wasted in the cables
Step-down transformer  voltage down, current
up  voltage is stepped down to a level which is
safe to use in homes, factories, etc.
At night, power stations still
generate electricity. Fewer people
use electricity at night (they’re
asleep…) so the supply of electricity
is much greater than the demand.
Electricity companies can therefore
sell electricity for less during the
night.
20 April 2017
Electrical Energy
Back
There are a few formulae you should be familiar with (some will be given
to you in the exam).
There are a few formulae you should be familiar with (some will be given
to you in the exam).
Energy transferred = power x time
E (Joules) = P (watts) x t (seconds)
Energy transferred in kWh = power x time
E (kWh) = P (kW) x t (hours)
Cost of using electricity = number of kWh x cost per kWh
Electrical appliances are machines, they transfer energy
from one form to another. For example, a light bulb takes in
electrical energy and gives out light and heat; a hair dryer
takes in electrical energy and gives out heat, sound, and
kinetic energy.
Back
20 April 2017
Waves
Waves transfer energyWaves transfer energy
Wave speed (m/s) = frequency (Hertz) x wavelength (metres)
v = f x λ
Waves can be reflected, refracted
(light changing direction), and
diffracted (spread out – much greater
diffraction when the obstruction or
gap is a similar size to the wavelength)
Back
Transverse
Vibrations are
perpendicular to the
direction of energy
transfer
Transverse
Vibrations are
perpendicular to the
direction of energy
transfer
Longitudinal
Vibrations are parallel
to the direction of
energy transfer.
Compressions – where
the lines are close
together.
Rarefaction – where the
lines are spread out.
Longitudinal
Vibrations are parallel
to the direction of
energy transfer.
Compressions – where
the lines are close
together.
Rarefaction – where the
lines are spread out.
 Electromagnetic
waves are
transverse.
 Sound waves are
longitudinal.
 Mechanical waves
can be either.
 Electromagnetic
waves are
transverse.
 Sound waves are
longitudinal.
 Mechanical waves
can be either.
angle of incidence = angle
of reflection
20 April 2017
Electromagnetic Spectrum
Electromagnetic waves form a continuous spectrum – the EM spectrumElectromagnetic waves form a continuous spectrum – the EM spectrum
Decreasing wavelength, increasing frequency, waves transfer more energy
All EM
waves
travel at
the same
speed in a
vacuum.
All EM
waves
travel at
the same
speed in a
vacuum.
Some of these EM waves can be used for communications:
Radio waves – TV and radio (these can be diffracted by mountains)
Microwaves – mobile phones and satellite TV
Infrared – remote controls and optical fibres
Visible light - photography
Some of these EM waves can be used for communications:
Radio waves – TV and radio (these can be diffracted by mountains)
Microwaves – mobile phones and satellite TV
Infrared – remote controls and optical fibres
Visible light - photography
Back
20 April 2017
Big Bang Theory
BackBack
The Big Bang theory
states that…
Everything in the
known Universe was
contained at a very
hot, very dense
initial point. A rapid
expansion took place
around 13.7 billion
years ago in which
space, time and all
matter were
created. There are
2 key pieces of
evidence for this
theory – CMBR and
Red-shift.
Red-shift is another piece of evidence that the
Universe is expanding because it shows us that
galaxies are moving away from each other.
Red-shift is another piece of evidence that the
Universe is expanding because it shows us that
galaxies are moving away from each other.
Other theories:
There are other theories for the origins of the
Universe. The Steady State theory suggests
that the Universe has always been huge and is
expanding because matter is entering the
Universe through white holes. However, there is
very little evidence for this theory.
Cosmic Microwave Background Radiation (evidence
for Big Bang theory)
If you look into space with your eyes, you will
see a lot of emptiness. But if you use microwave
detectors you will see a lot of cosmic microwave
background radiation (CMBR). The existence of
this radiation can only be explained by the Big
Bang theory.
Cosmic Microwave Background Radiation (evidence
for Big Bang theory)
If you look into space with your eyes, you will
see a lot of emptiness. But if you use microwave
detectors you will see a lot of cosmic microwave
background radiation (CMBR). The existence of
this radiation can only be explained by the Big
Bang theory.
20 April 2017
Red-shift
BackBack
Doppler  an object
making a sound is
moving away from
you, the sound waves
stretch out 
wavelength
increases, frequency
decreases
Doppler can also be
applied to light, but
the object emitting
the light needs to be
moving very fast and
huge distances  this
is called Red-shift
Doppler can also be
applied to light, but
the object emitting
the light needs to be
moving very fast and
huge distances  this
is called Red-shift
Absorption spectra:
These show which
colours of light are
absorbed by, for
example, the
atmosphere of a
planet or the
contents of a galaxy.
The absorbed light is
shown by dark lines
on a colour spectrum.
For a galaxy moving
away from us, these
lines are shifted
towards the red end
of the spectrum.
Red-shift is one piece of evidence for the
theory that the universe started through a
very rapid expansion (the Big Bang) and is
continuing to expand (CMBR is another piece of
evidence).
Red-shift is one piece of evidence for the
theory that the universe started through a
very rapid expansion (the Big Bang) and is
continuing to expand (CMBR is another piece of
evidence).
The faster a star or galaxy is moving away
from us, the bigger the red-shift will be.
The faster a star or galaxy is moving away
from us, the bigger the red-shift will be.
Blue-shift is the opposite to red-shift. If a galaxy is moving
towards us the wavelength of light reduces and the spectrum
of light is shifted towards the blue part of the spectrum.
Blue-shift is the opposite to red-shift. If a galaxy is moving
towards us the wavelength of light reduces and the spectrum
of light is shifted towards the blue part of the spectrum.
20 April 2017
Formulae
• The formulae you need to use will
(probably) be given to you
• You should be able to rearrange the
formulae when asked
• After that, all you need to do is put in
the numbers
Back
If X = Y x Z
Y = X
Z
Z = X
Y
20 April 2017
How science works
• Bias – if research is funded by a company (e.g. a
mobile phone company) there is the possibility
that the results could be biased, or even not
published if they do not favour the sponsoring
company.
• Reliability – Results are reliable if they are
repeatable by others. Results can be compared
with others to check reliability. Reliability of
data can be improved through collecting lots of
data and calculating an average.
• Sample size – experiments should use as large a
sample of people as possible to get a good
representation of a population.
20 April 2017
How science works
• Control groups – Used in investigations to allow a
comparison to be made.
• Issues:
Ethical – using people (particularly children)
or animals in scientific research
Economic – research being funded by
companies, governments, etc.
Social – how the results of scientific
research affect people
Environmental – research projects can have a
negative impact on an environment even
if there is some benefit (e.g. wind
farms)
Back
20 April 2017
Interpreting graphs
• Use numbers from the graph to back up
any conclusions
• Use terms and units given to you in the
graph
• Use numbers from the graph as well
• If there is more than one plot on the
graph, compare the plots in your answer
• The graph might show a relationship
between X and Y – i.e. directly/indirectly
proportional
20 April 2017
Interpreting graphsTemperature(o
C)
Time (s)
What does this
graph tell you?
• Red starts at a higher temperature than blue.
• The temperature of red decreases more rapidly
than blue.
• Blue maintains a constant temperature for
longer. Back
20 April 2017
Checking your answers
• After you’ve calculated an answer, have a
good look at it and compare it to the
question  does it look right?
• E.g. A student is asked to calculate the
mass of some water being heated in a
beaker. She gets a result of 2.3 x 1012
kg…
• Make sure you use a calculator if you’re not
confident doing it by hand!
Back

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Aqa p1 revision ppt

  • 1. 20 April 2017 Heat transfer Evaporation Formulae Checking answers Generating Electricity Efficiency Interpreting graphs How science works Red-shift Infrared Radiation Particles Heating/ Insulation Electrical Energy Waves EM Spectrum Big Bang
  • 2. 20 April 2017 Energy transfer by heating • 3 methods – conduction, convection, radiation • The bigger the temperature difference between an object and its surroundings, the faster the rate at which energy is transferred by heating. • Rate of transfer of energy depends on surface area and volume, object materials, surfaces. Back
  • 3. 20 April 2017 Infrared Radiation • All objects emit and absorb infrared • The hotter an object is, the more IR it emits in a given time (time is important!) • Dark, matt surfaces – good absorbers, good emitters (this means that a dark, matt object will heat up faster or cool down faster than a light, shiny one) • Light, shiny surfaces – poor absorbers, poor emitters, good reflectors. Back
  • 4. 20 April 2017 Particles Back Conduction, convection, evaporation and condensation all transfer energy, and all involve particles in their theories. In an object, the more kinetic energy the particles have, the hotter the object is. Conduction All to do with particles banging into each other and passing on KE. Metals have free electrons which can also pass on KE, making metals excellent conductors. The arrangement of particles in a substance determine how good a conductor it is. Convection Takes place in liquids and gases. When a liquid or gas gets hotter, the particles have more KE  they move around more, making the liquid or gas less dense. Therefore, hot liquids or gases will rise above cooler liquids or gases. (HEAT DOES NOT RISE, HOT LIQUIDS AND GASES DO!!) Particle arrangements: Solid – fixed in place, least amount of KE but still some movement Liquid – some fixed arrangement, free to slide over each other, more KE than solid Gas – free to move about randomly, no fixed arrangement, lots of KE
  • 5. 20 April 2017 Evaporation Back Particles in a liquid are held together by forces The particles need lots of kinetic energy to overcome these forces Particles can gain kinetic energy through heating but that energy has to come from somewhere Liquids on your skin get the energy they need for evaporation from your skin. So your skin is losing energy through heating the particles and it will feel colder. If particles are leaving the liquid on your skin through evaporation, they are taking kinetic energy with them. The average kinetic energy of the liquid on your skin has dropped.
  • 6. 20 April 2017 Heating and Insulation Back Insulation materials aim to reduce energy transfer by heating – they may reduce conduction, convection, and radiation. New heating systems or insulation for a house cost money. The payback time of an investment tells you how long it will take to get your money back based on how much the investment saves you. Payback time = initial investment saving per year Liquids on your skin get the energy they need for evaporation from your skin.Insulation materials for homes (including double glazing) are often given a U-value. This is a measure of how effective the insulator is. The lower the U- value, the better the material is as an insulator. Solar panels sometimes contain water that is heated by the Sun. The pipes in a solar panel are often black. The hot water can be used for heating.
  • 7. 20 April 2017 Efficiency • Two formulae (you’ll be given both) • Efficiency = useful energy out (x 100%) total energy in • Efficiency = useful power out (x 100%) total power in • You might need to rearrange these and put in the numbers. • Answers can be given either as a percentage (e.g. 30%) or as a decimal (0.3)  DO NOT combine these (e.g. 0.3%)
  • 8. 20 April 2017 Efficiency • Sankey diagrams are often used to show efficiency • Efficient: • Not efficient: Back Most energy is transferred to a useful form. Most energy is transferred to a non- useful form – it is wasted. The ratio of useful energy transferred to total energy in gives you the efficiency of the machine represented by the Sankey diagram.
  • 9. 20 April 2017 Generating Electricity BackBack Power stations heat water to make steam  steam turns a turbine  the turbine spins a generator Heat can be generated by: burning fossil fuels nuclear fission burning biofuels Heat can be generated by: burning fossil fuels nuclear fission burning biofuels Water and wind can drive a turbine directly (no need for heating) Small-scale generation is useful in remote areas. The Sun’s energy can be used to generate electricity (either by heating water or directly) Different methods of generating have different effects on the atmosphere Different methods of generating have different effects on the atmosphere National grid – a grid of cables and transformers transferring electrical energy around the country National grid – a grid of cables and transformers transferring electrical energy around the country Step-up transformer  voltage up, current down  lower current means less heating in cables  less energy wasted in the cables Step-up transformer  voltage up, current down  lower current means less heating in cables  less energy wasted in the cables Step-down transformer  voltage down, current up  voltage is stepped down to a level which is safe to use in homes, factories, etc. At night, power stations still generate electricity. Fewer people use electricity at night (they’re asleep…) so the supply of electricity is much greater than the demand. Electricity companies can therefore sell electricity for less during the night.
  • 10. 20 April 2017 Electrical Energy Back There are a few formulae you should be familiar with (some will be given to you in the exam). There are a few formulae you should be familiar with (some will be given to you in the exam). Energy transferred = power x time E (Joules) = P (watts) x t (seconds) Energy transferred in kWh = power x time E (kWh) = P (kW) x t (hours) Cost of using electricity = number of kWh x cost per kWh Electrical appliances are machines, they transfer energy from one form to another. For example, a light bulb takes in electrical energy and gives out light and heat; a hair dryer takes in electrical energy and gives out heat, sound, and kinetic energy. Back
  • 11. 20 April 2017 Waves Waves transfer energyWaves transfer energy Wave speed (m/s) = frequency (Hertz) x wavelength (metres) v = f x λ Waves can be reflected, refracted (light changing direction), and diffracted (spread out – much greater diffraction when the obstruction or gap is a similar size to the wavelength) Back Transverse Vibrations are perpendicular to the direction of energy transfer Transverse Vibrations are perpendicular to the direction of energy transfer Longitudinal Vibrations are parallel to the direction of energy transfer. Compressions – where the lines are close together. Rarefaction – where the lines are spread out. Longitudinal Vibrations are parallel to the direction of energy transfer. Compressions – where the lines are close together. Rarefaction – where the lines are spread out.  Electromagnetic waves are transverse.  Sound waves are longitudinal.  Mechanical waves can be either.  Electromagnetic waves are transverse.  Sound waves are longitudinal.  Mechanical waves can be either. angle of incidence = angle of reflection
  • 12. 20 April 2017 Electromagnetic Spectrum Electromagnetic waves form a continuous spectrum – the EM spectrumElectromagnetic waves form a continuous spectrum – the EM spectrum Decreasing wavelength, increasing frequency, waves transfer more energy All EM waves travel at the same speed in a vacuum. All EM waves travel at the same speed in a vacuum. Some of these EM waves can be used for communications: Radio waves – TV and radio (these can be diffracted by mountains) Microwaves – mobile phones and satellite TV Infrared – remote controls and optical fibres Visible light - photography Some of these EM waves can be used for communications: Radio waves – TV and radio (these can be diffracted by mountains) Microwaves – mobile phones and satellite TV Infrared – remote controls and optical fibres Visible light - photography Back
  • 13. 20 April 2017 Big Bang Theory BackBack The Big Bang theory states that… Everything in the known Universe was contained at a very hot, very dense initial point. A rapid expansion took place around 13.7 billion years ago in which space, time and all matter were created. There are 2 key pieces of evidence for this theory – CMBR and Red-shift. Red-shift is another piece of evidence that the Universe is expanding because it shows us that galaxies are moving away from each other. Red-shift is another piece of evidence that the Universe is expanding because it shows us that galaxies are moving away from each other. Other theories: There are other theories for the origins of the Universe. The Steady State theory suggests that the Universe has always been huge and is expanding because matter is entering the Universe through white holes. However, there is very little evidence for this theory. Cosmic Microwave Background Radiation (evidence for Big Bang theory) If you look into space with your eyes, you will see a lot of emptiness. But if you use microwave detectors you will see a lot of cosmic microwave background radiation (CMBR). The existence of this radiation can only be explained by the Big Bang theory. Cosmic Microwave Background Radiation (evidence for Big Bang theory) If you look into space with your eyes, you will see a lot of emptiness. But if you use microwave detectors you will see a lot of cosmic microwave background radiation (CMBR). The existence of this radiation can only be explained by the Big Bang theory.
  • 14. 20 April 2017 Red-shift BackBack Doppler  an object making a sound is moving away from you, the sound waves stretch out  wavelength increases, frequency decreases Doppler can also be applied to light, but the object emitting the light needs to be moving very fast and huge distances  this is called Red-shift Doppler can also be applied to light, but the object emitting the light needs to be moving very fast and huge distances  this is called Red-shift Absorption spectra: These show which colours of light are absorbed by, for example, the atmosphere of a planet or the contents of a galaxy. The absorbed light is shown by dark lines on a colour spectrum. For a galaxy moving away from us, these lines are shifted towards the red end of the spectrum. Red-shift is one piece of evidence for the theory that the universe started through a very rapid expansion (the Big Bang) and is continuing to expand (CMBR is another piece of evidence). Red-shift is one piece of evidence for the theory that the universe started through a very rapid expansion (the Big Bang) and is continuing to expand (CMBR is another piece of evidence). The faster a star or galaxy is moving away from us, the bigger the red-shift will be. The faster a star or galaxy is moving away from us, the bigger the red-shift will be. Blue-shift is the opposite to red-shift. If a galaxy is moving towards us the wavelength of light reduces and the spectrum of light is shifted towards the blue part of the spectrum. Blue-shift is the opposite to red-shift. If a galaxy is moving towards us the wavelength of light reduces and the spectrum of light is shifted towards the blue part of the spectrum.
  • 15. 20 April 2017 Formulae • The formulae you need to use will (probably) be given to you • You should be able to rearrange the formulae when asked • After that, all you need to do is put in the numbers Back If X = Y x Z Y = X Z Z = X Y
  • 16. 20 April 2017 How science works • Bias – if research is funded by a company (e.g. a mobile phone company) there is the possibility that the results could be biased, or even not published if they do not favour the sponsoring company. • Reliability – Results are reliable if they are repeatable by others. Results can be compared with others to check reliability. Reliability of data can be improved through collecting lots of data and calculating an average. • Sample size – experiments should use as large a sample of people as possible to get a good representation of a population.
  • 17. 20 April 2017 How science works • Control groups – Used in investigations to allow a comparison to be made. • Issues: Ethical – using people (particularly children) or animals in scientific research Economic – research being funded by companies, governments, etc. Social – how the results of scientific research affect people Environmental – research projects can have a negative impact on an environment even if there is some benefit (e.g. wind farms) Back
  • 18. 20 April 2017 Interpreting graphs • Use numbers from the graph to back up any conclusions • Use terms and units given to you in the graph • Use numbers from the graph as well • If there is more than one plot on the graph, compare the plots in your answer • The graph might show a relationship between X and Y – i.e. directly/indirectly proportional
  • 19. 20 April 2017 Interpreting graphsTemperature(o C) Time (s) What does this graph tell you? • Red starts at a higher temperature than blue. • The temperature of red decreases more rapidly than blue. • Blue maintains a constant temperature for longer. Back
  • 20. 20 April 2017 Checking your answers • After you’ve calculated an answer, have a good look at it and compare it to the question  does it look right? • E.g. A student is asked to calculate the mass of some water being heated in a beaker. She gets a result of 2.3 x 1012 kg… • Make sure you use a calculator if you’re not confident doing it by hand! Back