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    Unit 8, Chapter 26

    CPO Science

    Foundations of Physics

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    Unit 8: Matter and Energy

    26.1 Heat Conduction

    26.2 Convection

    26.3 Radiation

    Chapter 26 Heat Transfer

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    Chapter 26 Objectives1. Explain the relationship between temperature and thermal

    equilibrium.

    2. Explain how heat flows in physical systems in terms ofconduction, convection, and radiation.

    3. Apply the concepts of thermal insulators and conductors topractical systems.

    4. Describe free and forced convection and recognize theseprocesses in real-life applications.

    5. Identify the relationship between wavelength, color, infraredlight, and thermal radiation.

    6. Calculate the heat transfer in watts for conduction, convection,

    and radiation in simple systems.

    7. Explain how the three heat-transfer processes are applied toevaluating the energy efficiency of a house or building.

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    Chapter 26 Vocabulary Terms infrared

    windchill factor

    thermal insulator thermal equilibrium

    forced convection

    R-value

    convection

    blackbody spectrum

    thermal conductivity

    thermal conductor

    blackbody heat transfer

    thermal radiation

    free convection

    heat transfer coefficient

    conduction

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    26.1 Heat Conduction

    Key Question:

    How does heat passthrough differentmaterials?

    *Students read Section 26.1AFTER Investigation 26.1

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    26.1 Heat Transfer The science of how heat flows is called heat

    transfer.

    There are three ways heat transfer works:conduction, convection, and radiation.

    Heat flow depends on the temperature difference.

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    26.1 Thermal Equilibrium Two bodies are in thermal

    equilibrium with each

    other when they have thesame temperature.

    In nature, heat always

    flows from hot to cold untilthermal equilibrium isreached.

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    26.1 Heat Conduction Conduction is the transfer of heat through

    materials by the direct contact of matter.

    Dense metals like copper and aluminum are verygood thermal conductors.

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    26.1 Heat Conduction A thermal insulator is a material that conducts

    heat poorly.

    Heat flows very slowly through the plastic so thatthe temperature of your hand does not rise verymuch.

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    26.1 Heat Conduction Styrofoam gets its

    insulating ability by

    trapping spaces of airin bubbles.

    Solids usually arebetter heat conductors

    than liquids, andliquids are betterconductors thangases.

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    26.1 Heat Conduction The ability to conduct

    heat often depends moreon the structure of amaterial than on thematerial itself.

    Solid glass is a thermal

    conductor when it isformed into a beaker orcup.

    When glass is spun intofine fibers, the trapped airmakes a thermal insulator.

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    26.1 Thermal Conductivity

    The thermal conductivity of a material describeshow well the material conducts heat.

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    26.1 ThermalConductivity

    Heat conduction insolids and liquidsworks by transferringenergy through

    bonds betweenatoms or molecules.

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    26.1 Heat Conduction Equation

    PH = k A (T2 -T1)L

    Area of cross section (m2)

    Length (m)

    Thermal conductivity

    (watts/m

    o

    C)

    Heat flow(watts)

    Temperaturedifference (oC)

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    26.1 Variables for conduction

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    26.1 Calculate Heat Transfer

    A copper bar connects two beakers of water at differenttemperatures.

    One beaker is at 100C and the other is at 0C.

    The bar has a cross section area of 0.0004 m2 and is one-halfmeter (0.5 m) long.

    How many watts of heat are conducted through the bar fromthe hot beaker to the cold beaker?

    The thermal conductivity of copper is 401 W/mC.

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    26.2 Convection

    Key Question:

    Can moving matter carrythermal energy?

    *Students read Section 26.2AFTER Investigation 26.2

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    26.2 Convection Convection is the transfer of

    heat by the motion of liquids

    and gases. Convection in a gas occursbecause gas expands whenheated.

    Convection occurs becausecurrents flow when hot gasrises and cool gas sink.

    Convection in liquids alsooccurs because of differences

    in density.

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    26.2 Convection When the flow of gas or

    liquid comes from

    differences in density andtemperature, it is calledfree convection.

    When the flow of gas orliquid is circulated bypumps or fans it is calledforced convection.

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    26.2 Convection

    Convection depends onspeed.

    Motion increases heattransfer by convection inall fluids.

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    26.2 Convection Convection depends on

    surface area.

    If the surface contactingthe fluid is increased, therate of heat transfer alsoincreases.

    Almost all devices madefor convection have finsfor this purpose.

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    26.2 Forced Convection

    Both free and forced convection help toheat houses and cool car engines.

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    26.2 Convection and Sea Breezes

    On a smaller scale nearcoastlines, convection is

    responsible for sea breezes. During the daytime, land is much

    hotter than the ocean.

    A sea breeze is created when hot

    air over the land rises due toconvection and is replaced bycooler air from the ocean.

    At night the temperature reverses

    so a land breeze occurs.

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    26.2 Convection Currents Much of the Earths climate is regulated by giant

    convection currents in the ocean.

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    26.2 Heat Convection Equation

    PH = h A (T2 -T1)

    Area contacting fluids (m2)Heat transfer coefficient(watts/m2oC)

    Heat flow(watts)

    Temperaturedifference (oC)

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    26.2 Calculating convection The surface of a window is a

    temperature of 18C (64oF).

    A wind at 5C (41o

    F) is blowingon the window fast enough tomake the heat transfercoefficient 100 W/m2C.

    How much heat is transferredbetween the window and the airif the area of the window is 0.5square meters?

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    26.3 Radiation

    Key Question:

    How does heat from thesun get to Earth?

    *Students read Section 26.3AFTER Investigation 26.3

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    26.3 Radiation Radiation is heat transfer by

    electromagnetic waves.

    Thermal radiation iselectromagnetic waves(including light) produced byobjects because of their

    temperature. The higher the temperature

    of an object, the morethermal radiation it gives off.

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    26.3 Radiant Heat

    We do not see thethermal radiation

    because it occurs atinfrared wavelengthsinvisible to the humaneye.

    Objects glow differentcolors at differenttemperatures.

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    26.3 Radiant Heat A rock at room

    temperature does notglow.

    The curve for 20Cdoes not extend intovisible wavelengths.

    As objects heat up they

    start to give off visiblelight, or glow.

    At 600C objects glowdull red, like the burner

    on an electric stove.

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    26.3 Radiant Heat As the temperature rises, thermal

    radiation produces shorter-wavelength, higher energy light.

    At 1,000C the color is yellow-orange, turning to white at 1,500C.

    If you carefully watch a bulb on adimmer switch, you see its color

    change as the filament gets hotter.

    The bright white light from a bulb isthermal radiation from an extremelyhot filament, near 2,600C.

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    26.3 Radiant Heat

    The graph of powerversus wavelengthfor a perfectblackbody is calledthe blackbody

    spectrum.

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    26.3 Radiant Heat A perfect blackbody is a surface that reflects

    nothing and emits pure thermal radiation.

    The white-hot filament of a bulb is agood blackbody because all light fromthe filament is thermal radiation andalmost none of it is reflected from other

    sources.

    The curve for 2,600C shows thatradiation is emitted over the whole

    range of visible light.

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    26.3 Radiant Heat A star is a near-perfect

    blackbody.

    The distribution of energybetween different wavelengths(colors) depends strongly on thetemperature.

    Sirius is a hot, young star about

    twice as big as the sun and 22times as bright.

    Because its temperature ishotter, Sirius appears bluer than

    the sun.

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    26.3 Radiant Heat The total power emitted as thermal radiation by a

    blackbody depends on temperature (T) and

    surface area (A

    ).

    Real surfaces usually emit less than the blackbodypower, typically between 10 and 90 percent.

    The Kelvin temperature scale is used in theStefan-Boltzmann formula because thermalradiation depends on the temperature above

    absolute zero.

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    26.3 Stefan-Boltzmann formula

    P = s AT4

    Surface area (m2)

    Stefan-Boltzmannconstant5.67 x 10-8 watts/m2K4)

    Power(watts)

    Absolute temperature(K)

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    26.3 Calculate Radiant Power The filament in a light bulb has a

    diameter of 0.5 millimeters anda length of 50 millimeters.

    The surface area of the filamentis 4 10-8 m2.

    If the temperature is 3,000 K,how much power does thefilament radiate?

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    26.3 Radiant Heat When comparing heat

    transfer for a pot 10 cm

    above a heating elementon a stove, radiant heataccounts for 74%

    How is heat transferredwhen the pot sits on theelement?

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    Application: Energy-efficient Buildings