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Lecture07 P2

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Homework: 51, 54, 59, 60 (pages 503, 504)

51. A sphere of radius 0.500 m, temperature 27.00C, and emissivity


0.850 is located in an environment of temperature 77.00C. At what
rate does the sphere (a) emit and (b) absorb thermal radiation? (c)
What is the sphere’s net rate of energy exchange?

(a) Prad  σεAT 4

A  4πR 2 ; T  273  27  300 (K)


Prad  1.23 10 (W) 3

(b) Pabs  σεAT 4


env
T env  273  77  350 (K)
Pabs  2.27 10 (W)
3

(c) Pnet  Pabs  Prad  2.27 10  1.23 10  1.04 10 (W)
3 3 3
54. If you were to walk briefly in space without a spacesuit while far
from the Sun (as an astronaut does in the movie 2001), you would feel
the cold of space – while you radiated energy, you would absorb almost
none from your environment. (a) At what rate would you lose energy?
(b) How much energy would you lose in 30 s? Assume that your
emissivity is 0.90, and estimate other data needed in the calculations.

(a) The heat transfer mechanism is radiation:

Prad  σεAT 4
8
Prad  5.67 10  0.9  2.0  310  9.4 10 (W)
4 2

(b) The energy lost in 30 s is:

E  Prad  t  9.4 10 2  30  2.8 10 4 (J)


59. In Figure a, two identical rectangular rods of metal are welded
end to end, with a temperature of T1=00C on the left side and a
temperature of T2=1000C on the right side. In 2.0 min, 10 J is
conducted at a constant rate from the right side to the left side. How
much time would be required to conduct 10 J if the rods were welded
side to side as in Figure b.

L
(a)

(b)
The heat transfer mechanism is conduction:
TH  TC
Pcond  kA
L

TH  TC
Pcond, a  kA a
La
TH  TC
Pcond, b  kA b
Lb
A b La
 Pcond, b  Pcond, a  2  2  Pcond, a  4Pcond, a
Aa Lb
so, the requested time is 2.0/4=0.5 min or 30 s.
60. The figure below shows the cross section of a wall made of three
layers. The thicknesses of the layers are L1, L2=0.750L1, and
L3=0.350L1. The thermal conductivities are k1, k2=0.900k1, and
k3=0.800k1. The temperatures at the left and right sides of the wall
Are 30.00C and -15.00C, respectively. Thermal conduction through
the wall has reached the steady state. (a) What is the temperature
difference T2 across layer 2 (between the left and right sides of the
layer)? If k2 were, instead, equal to 1.1k1, (b) would the rate at
which energy is conducted through the wall be greater than, less than,
or the same as previously, and (c) what would be the value of T2?

A(TH  TC ) AT2
(a) Pcond  
 (L/k) L 2 /k 2
(L 2 /k 2 )(TH  TC )
T2   16 .50 C
 (L/k)
(b) conductivity k increases  conduction
rate increases.
(c) Repeat the calculation in part (a):
T2  14 .50 C
Chapter 3 The Kinetic Theory of Gases

3.1. Ideal Gases


3.1.1. Experimental Laws and the Equation of State
3.1.2. Molecular Model of an Ideal Gas
3.2. Mean Free Path
3.3. The Boltzmann Distribution Law and The Distribution of
Molecular Speeds
3.4. The Molar Specific Heats of an Ideal Gas
3.5. The Equipartition of Energy Theorem
3.6. The Adiabatic Expansion of an Ideal Gas
Work Done by an Ideal Gas at Constant Temperature
A process at constant temperature is
called an isothermal expansion/compression.
The equation of state for n moles:
1 1
p  nRT  constant 
V V
The work done during an isothermal process:

dV  nRT lnV Vif


Vf Vf nRT
W   pdV  
V
Vi Vi V

Vf
W  nRT ln
Vi
Summary
The equations below allows us to calculate work done by the gas for
three special cases: Vf
W   pdV
Vi
1) If V  constant (isochoric ) : W0
2) If p  constant (isobaric) : W  p(Vf  Vi )  pV
3) If T  constant (isotherma l) : W  nRT ln f
V
Vi
Checkpoint 1: An ideal gas has an initial pressure of 3 pressure
units and an initial volume of 4 volume units. The table gives the
final pressure and volume of the gas (in those same units) in 5
processes. Which processes start and end on the same isotherm?

a b c d e
p 12 6 5 4 1
V 1 2 7 3 12
3.1.2. Molecular Model for an Ideal Gas

In this model:

1. The molecules obey Newton's laws of motion.

2. The molecules move in all direction with equal probability.

3. There is no interactions between molecules (no collisions


between molecules).

4. The molecules undergo elastic collisions with the walls.

Simulations:

http://www.phy.ntnu.edu.tw/ntnujava/index.php?topic=25

http://www2.biglobe.ne.jp/~norimari/science/JavaApp/Mole/e-gas.html
a. Pressure, Temperature, and RMS Speed
Problem: Let n moles of an ideal gas be confined in a cubical box of
volume V, (see the figure below). The walls of the box are held at
temperature T.
Key question: What is the connection between the pressure p exerted
by the gas and the speed of the molecules?

First, we consider a cubical box of edge length L, containing n moles


of an ideal gas. A molecule of mass m and velocity v is about to
collide with the shaded wall.
For an elastic collision, the
particle’s momentum (=m.v) along
the x axis is reserved and
change with an amount:

Δp x  (mv x )  (mv x )  2mv x


The average rate at which momentum is delivered to the shaded
wall by this molecule:
Δp x 2mv x mv 2x
 
Δt 2L/v x L
   
 dv d(mv) dp
Recall: F  ma  m  
dt dt dt
2
mv x
Fx,1 
L
The pressure exerted on the wall by this single molecule:
Fx,1
p1 
L2
For N molecules, the total pressure p:

Fx mv /L  mv /L  ...  mv
2 2 2
/L
p 2  x,1
2
x,2 x, N

L L
m 2
p   3 ( v x,1  v 2x,2  ...  v 2x, N )
L 
The average value of the square of the x components of all the
molecular speeds:
v v
2 2
 ...  v 2

v 
2
x
x,1 x,2 x, N

N
nmN A 2
p 3
vx
L
Since M  mN A : the molar mass of the gas
nM 2
VL : 3
p vx
V
For any molecule: v  vx  v y  vz
2 2 2 2

1 2
As all molecules move in random directions: v  v
2
x
3
nM 2
p v
3V
The square root of v 2 is called the root-mean-square speed:

v  v rms
2

2
nMv
p rms
3V

This relationship shows us how the pressure of the gas (a macroscopic


quantity) depends on the speed of the molecules (a microscopic quantity)

Combining with the equation of state: pV  nRT

3RT
v rms 
M
b. Translational Kinetic Energy
• Consider a single molecule of an ideal gas moving around in the box
(see Section a) .

1 2 1 2 1 2
K  mv  m v  mv rms
2 2 2
 1  3RT 1 3RT
K   m 
2  M 2 M/m
3RT
K
Recall:
2N A
R
The Boltzmann constant k: k 
NA
3
 K  kT  K does not depend on
2 the mass of the molecule
1 2 1 1 1 1
v  v  v  v  m v x  m v y  m v z  kT
2
x
2
y
2
z
2 2 2
3 2 2 2 2
Homework: 13, 14, 18, 20, 24 (p. 531-532)

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