Lecture07 P2
Lecture07 P2
Lecture07 P2
(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.
Prad σεAT 4
8
Prad 5.67 10 0.9 2.0 310 9.4 10 (W)
4 2
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 ) AT2
(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
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 ) : W0
2) If p constant (isobaric) : W p(Vf Vi ) pV
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:
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?
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
VL : 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
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)