Chapter 11Chapter 11
Energy in Thermal ProcessesEnergy in Thermal Processes
Vocabulary, 3 Kinds of EnergyVocabulary, 3 Kinds of Energy
Internal Energy U = Energy of microscopic motion and inter-molucular forces
WorkW = -Fx = -PV is work done by expansion (next chapter)
HeatQ = Energy transfer from microscopic contact
VPQU next chapter
Temperature and Specific HeatTemperature and Specific Heat
Add energy -> T rises
TmcQ
•cH20 = 1.0 cal/(gºC)•1 calorie = 4.186 J
Mass
Property of material
Example 11.1Example 11.1
Bobby Joe drinks a 130 “calorie” can of soda. If the efficiency for turning energy into work is 20%, how many 4 meter floors must Bobby Joe ascend in order to work off the soda and maintain her 55 kg mass?
Nfloors = 50.4
Example 11.2Example 11.2
Aluminum has a specific heat of .0924 cal/gºC. If 110 g of hot water at 90 ºC is added to an aluminum cup of mass 50 g which is originally at a temperature of 23 ºC, what is the final temperature of the equilibrated water/cup combo?
T = 87.3 ºC
Phase Changes and Latent HeatPhase Changes and Latent Heat T does not rise when phases change (at constant P) Examples: solid -> liquid (fusion), liquid -> vapor
(vaporization) Latent heat = energy required to change phases
mLQ Property of substance /transition
Example 11.3Example 11.3
1.0 liters of water is heated from 12 ºC to 100 ºC, then boiled away.a) How much energy is required to bring the water to boiling?b) How much extra energy is required to vaporize the water?c) If electricity costs $75 per MW-hrs, what was the cost of boiling the water?
a) Q = 8.8x104 cal = 3.68x105 J
b) Q = 5.4x105 cal = 2.26x106 J
c) 5.5 ¢
Example 11.4Example 11.4
Consider Bobby Joe from the previous example. If the 80% of the 130 kcals from her soda went into heat which was taken from her body from radiation, how much water was perspired to maintain her normal body temperature? (Assume a latent heat of vaporization of 540 cal/g even though T = 37 ºC)
= 193 g
A can of soda has ~ 325 g of H20Some fluid drips away
Three Kinds of Heat TranserThree Kinds of Heat Transer
Conduction Shake your neighbor - pass it down Examples: Heating a skillet, losing heat
through the walls Convection
Move hot region to a different location Examples: Hot-water heating for
buildings Circulating air Unstable atmospheres
Radiation Light is emitted from hot object Examples: Stars, Incandescent bulbs
ConductionConduction
Power depends on area A, thickness x, temperature difference t and conductivity of material
x
TkAP
Conductivity is propertyof material
Example 11.5Example 11.5A copper pot of radius 12 cm and thickness 5 mm sits on a burner and boils water. The temperature of the burner is 115 ºC while the temperature of the inside of the pot is 100 ºC. What mass of water is boiled away every minute?DATA: kCu = 397 W/mºC
m=1.43 kg
Conductivities and R-valuesConductivities and R-values Conductivity (k)
Property of Material SI units are W/(m ºC)
kxR
R
TA
x
TkAP
/
R-Valueo Property of material and thickness x.o Measures resistance to heato Useful for comparing insulation productso Quoted values are in AWFUL units
Conducitivities Conducitivities and R-valuesand R-values
ARGH!
What makes a good heat conductor?What makes a good heat conductor?
•“Free” electrons (metals)•Easy transport of sound (lattice vibrations)
•Stiff is good•Low Density is good•Pure crystal structure
Diamond is perfect!
R-values for layersR-values for layers
Consider a layered system, e.g. glass-air-glass
...)(
...
...
321
321
321
RRRA
PA
PR
A
PR
A
PR
TTTT
R
TAP
...321 RRRR
Example 11.6Example 11.6
Consider three panes of glass, each of thickness 5 mm.The panes trap two 2.5 cm layers of air in a large glass door. How much power leaks through a 2.0 m2 glass door if the temperature outside is -40 ºC and the temperature inside is 20 ºC?DATA: kglass= 0.84 WmºC, kair= 0.0234 Wm ºC
P = 55.7 W
ConvectionConvection
If warm air blows across the room, it is convection If there is no wind, it is conduction Can be instigated by turbulence or instabilities
Why are windows triple paned?Why are windows triple paned?
To stop convection!
Transfer of heat by radiationTransfer of heat by radiation
All objects emit light if T > 0 Colder objects emit longer wavelengths
(red or infra-red) Hotter objects emit shorter wavelengths
(blue or ultraviolet) Stefan’s Law give power of emitted radiation
4AeTP = 5.6696x10-8 W/(m2ºK4)is the Stefan-Boltzmann constant
Emissivity, 0 < e < 1, usually near 1
Example 11.7Example 11.7
If the temperature of the Sun fell 5%, and the radius shrank 10%, what would be the percentage change of the Sun’s power output?
- 34%
Example 11.8Example 11.8
DATA: The sun radiates 3.74x1026 W Distance from Sun to Earth = 1.5x1011 m Radius of Earth = 6.36x106 m
a) What is the intensity (power/m2) of sunlight when it reaches Earth?
b) How much power is absorbed by Earth in sunlight? (assume that none of the sunlight is reflected)
c) What average temperature would allow Earth to radiate an amount of power equal to the amount of sun power absorbed?
a) 1323 W/m2
b) 1.68x1017 W
c) T = 276 ºK = 3 ºC = 37 ºF
What is neglected in estimate?What is neglected in estimate?
•Earth is not at one single temperature•Some of Sun’s energy is reflected•Emissivity lower at Earth’s thermal wavelengths than at Sun’s wavelengths•Radioactive decays inside Earth
•Hot underground (less so in Canada)•Most of Jupiter’s radiation
NOTE: Venus has a surface T of 900 C
Greenhouse GasesGreenhouse GasesSun is much hotter than Earth so sunlight has much shorter wavelengths than light radiated by Earth (infrared)Emissivity of Earth depends on wavelengthCO2 in Earth’s atmosphere reflects in the infrared
oBarely affects incoming sunlight oReduces emissivity, e, of re-radiated heat
Global Global warmingwarming
Tearth has risen ~ 1 ºF ~ consistent with greenhouse effectOther gases, e.g. S02, could cool Earth