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14 Heat

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14 Heat Homework: Problems: 3, 5, 13, 21, 33, 47, 49. Internal Energy Heat Capacity & Specific Heat Phase Transitions Thermal Conduction ... – PowerPoint PPT presentation

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Title: 14 Heat


1
14 Heat
  • Homework
  • Problems 3, 5, 13, 21, 33, 47, 49.
  • Internal Energy
  • Heat Capacity Specific Heat
  • Phase Transitions
  • Thermal Conduction

2
Heat
  • Heat is energy transferred due to temperature
    difference.
  • Symbol, Q J
  • Ex. 4186J heat needed to raise 1kg of water one
    degree C.

3
example cs
  • in J/(kgC)
  • aluminum 920
  • copper 390
  • ice 2100
  • water 4186

4
specific heat
  • c Q/mDT J/(kgK)
  • heat to raise 1kg by 1 degree C or K.
  • slope warming curve DT/Q 1/(mc)
  • Q mcDT

5
Calorimetry
  • Measure heat lost/gained

6
Example Calorimetry
  • 2kg of substance-A heated to 100C. Placed in
    5kg of water at 20C. After five minutes the water
    temp. is 25C.
  • heat lost by substance heat gained water.

7
continued
8
Phase Transitions Latent Heat
  • L Q/m J/(kg)
  • heat needed to melt (f) or vaporize (v) 1kg

9
example Ls
  • in J/kg
  • melting (f) vaporization (v)
  • alcohol 100,000 850,000
  • water 333,000 2,226,000

10
Example
  • How much heat must be added to 0.5kg of ice at 0C
    to melt it?
  • Q mL (0.5kg)(333,000J/kg)
  • 167,000J
  • same amount of heat must be removed from 0.5kg
    water at 0C to freeze it.

11
Heat Transfer
  • Conduction
  • Convection
  • Radiation

12
Conduction
  • Heat conduction is the transmission of heat
    through matter.
  • dense substances are usually better conductors
  • most metals are excellent conductors

13
conduction equation
  • heat current energy/time watts
  • heat current kADT/L
  • k thermal conductivity
  • DT temperature difference, L below

14
conduction example
  • some conductivities in J/(m-s-C)
  • silver 429 copper 401 aluminum 240
  • Ex Water in aluminum pot. bottom 101C, inside
    100C, thickness 3mm, area 280sq.cm.
  • Q/t kA(Th-Tc)/L
  • (240)(0.028)(101-100)/(0.003)
  • 2,240 watts heat current

15
Heat transfer
  • 2m x 1m window, 4mm thick, single pane glass.
  • Assume temp. difference 5C
  • Q/t kA(DT)/L (0.84)(2)(5)/0.004
  • About 2,000 watts

16
R-Factors and Thermal Resistance
17
Convection
  • Convection transfer through bulk motion of a
    fluid.
  • Natural, e.g. warm air rises, cool falls
  • Forced, e.g. water-cooled engine

18
Radiation
  • Heat transfer by electromagnetic radiation, e.g.
    infrared.
  • Examples
  • space heaters with the shiny reflector use
    radiation to heat.
  • If they add a fan, they use both radiation and
    convection

19
Summary
  • Definition of Internal Energy
  • Heat Capacity
  • Specific Heat
  • Phase Transitions
  • Latent Heat
  • Phase Diagrams
  • Energy Transport by Conduction, Convection, and
    Radiation

20
Example
  • A student wants to check c for an unknown
    substance. She adds 230J of heat to 0.50kg of the
    substance. The temperature rises 4.0K.

21
Greenhouse Effect
  • dirtier air must be at higher temperature to
    radiate out as much as Earth receives
  • higher temperature air is associated with higher
    surface temperatures, thus the term global
    warming
  • very complicated model!

22
Phase Change
  • freeze (liquid to solid)
  • melt (solid to liquid)
  • evaporate (liquid to gas)
  • sublime (solid to gas)
  • phase changes occur at constant temperature

23
Temperature vs. Heat (ice, water, water vapor)
24
Heat and Phase Change
  • Latent Heat of Fusion heat supplied to melt or
    the heat removed to freeze
  • Latent Heat of Vaporization heat supplied to
    vaporize or heat removed to liquify.

25
Newtons Law of Cooling
  • For a body cooling in a draft (i.e., by forced
    convection), the rate of heat loss is
    proportional to the difference in temperatures
    between the body and its surroundings
  • rate of heat-loss DT

26
Real Greenhouse
  • covering allows sunlight to enter, which warms
    the ground and air inside the greenhouse.
  • the house is mostly enclosed so the warm air
    cannot leave, thus keeping the greenhouse warm (a
    car in the sun does this very effectively!)

27
Solar Power
  • Solar Constant
  • Describes the Solar Radiation that falls on an
    area above the atmosphere 1.37 kW / m².In
    space, solar radiation is practically constant
    on earth it varies with the time of day and year
    as well as with the latitude and weather. The
    maximum value on earth is between 0.8 and 1.0 kW
    / m².
  • see solarserver.de
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