43
PHY115 – Sault College – Bazlur slide 1 Heat Transfer

PHY115 – Sault College – Bazlurslide 1 Heat Transfer

Embed Size (px)

Citation preview

Page 1: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 1

Heat Transfer

Page 2: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 2

Heat TransferHeat transfers from warmer to cooler things.

If several objects with different temperatures are in contact, those that are warm become cooler and those that are cool become warmer.

They tend to reach a common temperature.

This equalizing of temperature occurs in three ways: by

– conduction, – convection, and – radiation.

Page 3: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 3

ConductionHold one end of an iron nail in a flame. It will quickly become too

hot to hold. The heat enters the metal nail at the end that is kept in the flame and the heat is transmitted along the nail's whole length.

The transmission of heat in this manner is called conduction.

The fire causes the atoms at the heated end of the nail to move more rapidly.

Because of their increased motion, these atoms and free electrons collide with their neighbors, and so on. This bumping process continues until the increased motion has been transmitted to all the atoms and the entire body has become hot.

Heat conduction occurs by electron and atomic collisions.

Page 4: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 4

ConductorsHow well a solid object conducts heat depends on the

bonding within its atomic or molecular structure.

Solids built of atoms that have one or more “loose” outer electrons conduct heat (and electricity) well.

Metals have the “loosest” outer electrons, which are free to carry energy by collisions throughout the metal.

They are excellent conductors of heat and electricity for this reason.

Silver is the best, copper is next, and, among the common metals, aluminum and then iron are next in order.

Page 5: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 5

InsulatorsWool, wood, straw, paper, cork, and Styrofoam, on the

other hand, are poor conductors of heat.

The outer electrons in the atoms of these materials are firmly attached.

Poor conductors are called insulators.

Page 6: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 6

Low conductivity of wood Wood is a good insulator even when it's red hot, which is

why firewalking professor John Suchocki can walk barefoot on red-hot wooden coals without burning his feet

Page 7: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 7

Tile is a better conductor The tile floor feels colder than the wooden floor, even

though both floor materials are the same temperature.

This is because tile is a better conductor of heat than wood, and so heat is more readily conducted out of the foot touching the tile.

Page 8: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 8

Air is a very poor conductorMost liquids and gases are poor heat conductors.

Air is a very poor conductor, which, as previously mentioned, is why your hand isn't harmed if put briefly in a hot pizza oven.

The good insulating properties of such things as wool, fur, and feathers are largely due to the air spaces they contain.

Other porous substances are likewise good insulators because of their many small air spaces.

Be glad that air is a poor conductor; if it weren't, you'd feel quite chilly on a 20°C (68°F) day!

Page 9: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 9

Which house is better insulated?

Page 10: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 10

ConvectionLiquids and gases transmit heat mainly by convection,

which is heat transfer due to the actual motion of the fluid itself.

Unlike conduction (in which heat is transferred by successive collisions of electrons and atoms), convection involves the motion of mass - the overall motion of a fluid.

Convection can occur in all fluids, whether liquids or gases.

Page 11: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 11

ConvectionWhether we heat water in a pan or heat

air in a room, the process is the same.

As the fluid is heated from below, the molecules at the bottom begin moving faster, spreading apart more, becoming less dense, so they are buoyed upward.

Denser cooler fluid moves in to take the place of the now-warmed fluid at the bottom.

In this way, convection currents keep the fluid stirred up as it heats - warmer fluid moving away from the heat source and cooler fluid moving toward the heat source.

Page 12: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 12

Convection currents

Convection currents occur in the atmosphere, affecting the weather.

When air is warmed, it expands. In doing so it becomes less dense than the surrounding air. Like a balloon, it is buoyed upward.

When the rising air reaches an altitude at which its density matches that of the surrounding air, it no longer rises.

This is evident when we see smoke from a fire rise and then settle off as it cools and its density matches that of the surrounding air.

Page 13: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 13

As the air expands, it coolsRising warm air expands because

less atmospheric pressure squeezes on it as it rises to higher altitudes.

As the air expands, it cools.

Do the following experiment right now. – With your mouth open, blow on your

hand. Your breath is warm. – Now repeat but this time pucker your

lips to make a small hole so your breath expands as it leaves your mouth. Note that your breath is appreciably cooler! Expanding air cools.

Page 14: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 14

ConvectionThe hot steam expands from the pressure cooker and is

cool to Millie's touch.

Page 15: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 15

ConvectionConvection currents stirring the atmosphere

result in winds.

Page 16: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 16

ConvectionConvection currents flow upwards.

Page 17: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 17

RadiationEnergy from the sun passes through space and then through the

Earth's atmosphere and warms the Earth's surface.

This energy does not pass through the atmosphere by conduction, for air is a poor conductor.

Nor does it pass through by convection, for convection begins only after the Earth is warmed.

We also know that neither convection nor conduction is possible in the empty space between our atmosphere and the sun.

We can see that energy must be transmitted some other way - by

electromagnetic radiation.

The energy so radiated is called radiant energy.

Page 18: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 18

RadiationRadiant energy is in the form of electromagnetic waves.

It includes radio waves, microwaves, infrared radiation, visible light, ultraviolet radiation, X rays, and gamma rays.

These types of radiant energy are listed in order of wavelength, from longest to shortest.

Infrared (below-the-red) radiation has longer wavelengths than visible light.

The longest visible wavelengths are for red light, and the shortest are for violet light.

Ultraviolet (beyond-the-violet) radiation has shorter wavelengths.

Page 19: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 19

Electromagnetic Waves

Page 20: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 20

Light Spectrum• Light 700nm – 400nm, 1015Hz

• Optical fiber uses 850, 1310, 1550nm

Page 21: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 21

WavesThe wavelength of radiation is related to the frequency of

radiation.

Frequency is the rate of vibration of a wave.

The girl in Figure shakes a rope at a low frequency (left), and a higher frequency (right).

Note that the low-frequency shake produces a long lazy wave, and the higher-frequency one produces shorter waves.

Likewise with electromagnetic waves.

High-frequency vibrations produce short waves and low-frequency vibrations produce longer waves.

Which one needs more energy to produce?

Page 22: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 22

Electromagnetic WavesTypes of radiant energy (electromagnetic waves).

Page 23: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 23

Emission of Radiant EnergyAll substances at any temperature above

absolute zero emit radiant energy.

The peak frequency of the radiant energy is directly proportional to the absolute temperature T of the emitter.

Page 24: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 24

Emission of Radiant EnergyThe surface of the sun has a high temperature and

therefore emits radiant energy at a high frequency - much of it in the visible portion of the electromagnetic spectrum.

The surface of the Earth, by comparison, is relatively cool, and so radiant energy it emits has a frequency lower than that of visible light.

The radiation emitted by the Earth is in the form of infrared waves - below our threshold of sight.

Radiant energy emitted by the Earth is called terrestrial radiation.

Page 25: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 25

Absorption of Radiant EnergyIf everything is emitting energy, why doesn't

everything finally run out of it?

The answer is, everything is also absorbing energy.

Good emitters of radiant energy are also good absorbers; poor emitters are poor absorbers.

For example, a radio antenna constructed to be a good emitter of radio waves is also, by its very design, a good receiver (absorber) of them.

A poorly designed transmitting antenna is also a poor receiver.

Page 26: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 26

Absorption and EmissionWhen the containers are filled with hot (or cold)

water, the blackened one cools (or warms) faster.

Page 27: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 27

Absorption of Radiant EnergyAbsorption and reflection are opposite processes.

A good absorber of radiant energy reflects very little radiant energy, including visible light.

Hence, a surface that reflects very little or no radiant energy looks dark.

So a good absorber appears dark and a perfect absorber reflects no radiant energy and appears completely black.

The pupil of the eye, for example, allows light to enter with no reflection, which is why it appears black.

An exception occurs in flash photography when pupils appear pink, which occurs when very bright light is reflected off the eye's inner pink surface and back through the pupil.

Page 28: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 28

ReflectorsGood reflectors, on the other hand, are poor

absorbers.

Clean snow is a good reflector and therefore does not melt rapidly in sunlight.

If the snow is dirty, it absorbs radiant energy from the sun and melts faster.

Dropping black soot from an aircraft onto snow-covered mountains is a technique sometimes used in flood control.

Page 29: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 29

Absorber and ReflectorPaint your house a _____________ color.

Page 30: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 30

Reflector and EmittersLight-colored buildings stay cooler in summer

because they reflect much of the incoming radiant energy.

Light-colored buildings are also poor emitters, and so they retain more of their internal energy than darker buildings and stay warmer in winter.

Paint your house a light color.

Page 31: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 31

Newton's Law of Cooling An object at a different temperature from its

surroundings will ultimately come to a common temperature with its surroundings.

A relatively hot object cools as it warms its surroundings; a cool object warms as it cools its surroundings.

Page 32: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 32

Newton's law of coolingThe rate of cooling of an object - whether by

conduction, convection, or radiation - is approximately proportional to the temperature difference ΔT between the object and its surroundings.

This is known as Newton's law of cooling.

Page 33: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 33

Wind ChillThe rate of cooling we experience on a cold day

can be increased by the added convection of wind.

We speak of this in terms of wind chill.

For example, a wind chill of −20°C means we are losing heat at the same rate as if the temperature were −20°C without wind.

Page 34: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 34

The Greenhouse Effect The Earth and its atmosphere gain energy when they

absorb radiant energy from the sun.

This warms the Earth.

The Earth, in turn, emits terrestrial radiation, much of which escapes to outer space.

Absorption and emission go on at equal rates to produce an average equilibrium temperature.

Over the last 500,000 years the average temperature of the Earth has fluctuated between 19°C and 27°C and is presently at the high point, 27°C.

The Earth's temperature increases when either the radiant energy coming in increases, or there is a decrease in the escape of terrestrial radiation.

Page 35: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 35

The Greenhouse EffectGlass is transparent to short-wavelength radiation

but opaque to long-wavelength radiation.

Reradiated energy from the plant is long wavelength because the plant has a relatively low temperature.

Page 36: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 36

Solar PowerStep from the shade into the sunshine and you're

noticeably warmed.

The warmth you feel isn't so much because the sun is hot, for its surface temperature of 6000°C is no hotter than the flames of some welding torches.

We are warmed principally because the sun is so big.

Page 37: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 37

Solar PowerAs a result, it emits enormous amounts of energy,

less than one part in a billion of which reaches the Earth.

Nonetheless, the amount of radiant energy received each second over each square meter at right angles to the sun's rays at the top of the atmosphere is 1400 joules (1.4 kJ).

This input of energy is called the solar constant.

This is equivalent in power units to 1.4 kJ/s or kilowatts per square meter (1.4 kW/m2).

Page 38: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 38

Solar EnergyOver each square meter of area perpendicular to

the sun's rays at the top of the atmosphere, the sun pours 1400 J of radiant energy each second.

Hence the solar constant is 1.4 kJ/s/m2, or 1.4 kW/m2.

Page 39: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 39

Energy per unit areaIs it the distance from the sun or the angle of the

sun's rays on Earth that accounts for frigid polar regions and tropical equatorial regions?

Where is the energy per unit area less?

Page 40: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 40

Controlling Heat Transfer A nice way to review the methods of heat transfer is by

considering a device that inhibits all three methods: the vacuum bottle.

A vacuum bottle (which you may know by the trademarked name Thermos) consists of a double-walled glass container with a vacuum between the walls.

(There is usually an outer covering as well.)

The glass surfaces that face each other are silvered.

A close-fitting stopper made of cork or plastic seals the bottle. Any liquid in a vacuum bottle - hot or cold - will remain close to its original temperature for many hours.

Page 41: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 41

Controlling Heat Transfer• Heat transfer by conduction through

the vacuum is impossible. Some heat escapes by conduction through the glass and stopper, but this is a slow process as glass and plastic or cork are poor conductors.

• The vacuum also prevents heat loss through the walls by convection.

• Heat loss by radiation is reduced by the silvered surfaces of the walls, which reflect heat waves back into the bottle.

Page 42: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 42

Summary• Conduction • Convection• Radiation• Newton's law of cooling • Greenhouse effect • Solar constant• Solar power

Page 43: PHY115 – Sault College – Bazlurslide 1 Heat Transfer

PHY115 – Sault College – Bazlur slide 43

SummaryConduction The transfer of heat energy by molecular and electron

collisions within a substance (especially a solid).

Convection The transfer of heat energy in a gas or liquid by means of currents in the heated fluid. The fluid moves, carrying energy with it.

Radiation The transfer of energy by means of electromagnetic waves.

Newton's law of cooling The rate of loss of heat from an object is proportional to the temperature difference between the object and its surroundings.

Greenhouse effect Warming of the lower atmosphere by short-wavelength radiation from the sun that penetrates the atmosphere, is absorbed by the Earth, and is re-radiated at longer wavelengths that cannot easily escape the Earth's atmosphere.

Solar constant 1400 J/m2 received from the sun each second at the top of the Earth's atmosphere on an area perpendicular to the sun's rays; expressed in terms of power, 1.4 kW/m2.

Solar power Energy per unit time derived from the sun.