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Heat Transfer

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Chapter 22 Heat Transfer Consequences of the Greenhouse Effect Continued The near unanimous view of climate scientists is that human activity is a main driver of ... – PowerPoint PPT presentation

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Title: Heat Transfer


1
Chapter 22
  • Heat Transfer

2
The Big Idea
  • Heat can be transferred by conduction, by
    convection, and by radiation
  • Heat transfer from warmer to cooler objects
  • Will reach same temperature
  • Thermal equilibrium
  • Three ways to equalize temperatures
  • Conduction
  • Convection
  • Radiation

3
22.1 Conduction
  • Conduction transfer of energy with in materials
    and between different materials that are in
    direct contact
  • Conductors materials that conduct heat well
  • Metals are the best conductors
  • Silver is the most conductive
  • In conduction, collisions between particles
    transfer thermal energy, without any over
    transfer of matter

4
Conductors
  • Materials that have loose outer electrons are
    good conductors of heat
  • Metals best conductors of heat and electricity
  • If materials are in the same vicinity, they will
    have the same temperature (room temperature)

5
Insulators
  • Liquids and gases make good insulators
  • Insulator any material that is a poor conductor
    of heat and that delays the transfer of heat
  • Heat is energy and is tangible

6
22.2 Convection
  • Conduction involves transfer of energy from
    molecule to molecule
  • Energy moves but molecules do not
  • Convection heat transfer by movement of the
    heated substance itself
  • In convection, heat is transferred by movement of
    the hotter substance from one place to another

7
Convection Continued
  • Convection occurs in all fluids
  • Convection works
  • Fluid is heated
  • Expands of fluid
  • Fluid becomes less dense and rises
  • Application of Archimedes's principle
  • Convection currents have influence on air

8
Moving Air
  • Convection currents stirring produce winds
  • Uneven absorption of heat causes uneven heating
    near the surface and creates convection currents
  • During the day, land is warmer than the air and
    produces a breeze. At night, the land is cooler
    than the water so air flows in the opposite
    direction

9
Cooling Air
  • Rising warm air expands
  • Less atmospheric pressure squeezes on higher
    altitudes
  • When air expands it cools
  • Molecules get speed from other molecules
  • With expanding air the average speed of molecules
    decreases and the air cools

10
22.3 Radiation
  • Suns heat is transmitted by radiation
  • Radiation energy transmitted by electromagnetic
    waves
  • Radiant energy any energy transmitted by
    radiation

11
Radiation Continued
  • In radiation, heat is transmitted in the form of
    radiant energy or electromagnetic waves
  • Radiant energy
  • Radio waves - Visible light
  • Micro waves - X-rays
  • Radiant energy is listed in wavelengths
  • Longest to shortest

12
22.4 Emission of Radiant Energy
  • All substances continuously emit radiant energy
    in a mixture of wavelengths
  • Low temperature objects emit long waves
  • High temperature objects emit short waves
  • An infrared thermometer measure the infrared
    radiant energy emitted by a body and converts it
    to temperature

13
Emission of Radiant Energy Continued
  • People emit low frequency of infrared
  • Types of light
  • Hot enough, visible light
  • 500 oC, red light
  • Higher then 500 oC, yellow light
  • Stellar radiation radiant energy emitted by
    stars
  • White hot, blue hot, red hot

14
Emission of Radiant Energy Continued
  • Suns temperature (5500 oC) emits radiant energy,
    visible on electromagnetic spectrum
  • Terrestrial radiation radiant energy that is
    emitted by the Earth
  • Infrared waves, not visible to us
  • Radiant energy encounters objects, some absorbed
    some reflected
  • Absorbed increases internal energy

15
22.5 Absorption of Radiant Energy
  • Everything emits energy
  • Everything absorbs energy from the environment

16
Absorption and Emission
  • Objects absorb and radiate energy at the same
    rate
  • Goes to thermal equilibrium with its environment
  • When an object radiates more energy it has a new
    thermal equilibrium
  • Good emitters of radiant energy are also good
    absorbers poor emitters are poor absorbers

17
Absorption and Emission Continued
  • Dark objects remain hotter than their
    surroundings on a hot day and cool faster at
    night
  • All objects in thermal contact reach thermal
    equilibrium

18
Absorption and Reflection
  • Absorption and reflection are opposite processes
  • Good absorber reflects little radiant energy
  • Appear dark
  • Radiant energy that enters an opening has little
    chance of leaving before it is completely absorbed

19
Absorption and Reflection Continued
  • Good reflectors are poor absorbers
  • Light colored objects reflect more light and heat
    and dark colored objects absorb more light and
    energy
  • Sun during the day is a net absorber, at night it
    is a net emitter

20
22.6 Newtons Law of Cooling
  • An object hotter then its surroundings eventually
    cools to match the surrounding temperature
  • Rate of cooling how many degrees change per unit
    of time
  • The rate of cooling of an object depends on how
    much hotter the object is than the surroundings

21
Newtons Law of Cooling Continued
  • The colder the objects surroundings, the faster
    the object will be cool
  • The temperature difference is small, the rate of
    cooling is low and vice versa
  • Newtons law of cooling states the rate of
    cooling is approximately proportional to the
    temperature difference between the object and its
    surroundings

22
22.7 Global Warming and the Greenhouse Effect
  • Greenhouse effect warming of the planets
    surface due to the trapping of radiation by the
    planets atmosphere

23
Causes of Greenhouse Effect
  • Two concepts
  • All things radiate heat and wavelength depends on
    temperature
  • High temperatures have short waves
  • Low temperatures have long waves
  • Transparency of things depends on the wavelength
    of radiation

24
Causes of the Greenhouse Effect Continued
  • Same effect in Earths atmosphere
  • Surface of Earth absorbs energy
  • Reradiates part of the energy in longer
    wavelengths
  • Long wavelengths cannot escape the Earths
    atmosphere, warms Earth
  • Earths temperature depends on the energy
    balanced between incoming solar radiation and
    outgoing terrestrial radiation

25
Consequences of the Greenhouse Effect
  • Over years, solar radiation that comes to Earth
    equals terrestrial radiation Earth emits
  • Materials such as fossil fuels changes absorption
    and reflection of solar radiation
  • Not if energy is solar, wind, water
  • Can change Earths temperature

26
Consequences of the Greenhouse Effect Continued
  • The near unanimous view of climate scientists is
    that human activity is a main driver of global
    warming and climate change
  • Water vapor is the main greenhouse gas
  • CO2 is the most rapidly increasing

27
THE END! ?
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