thermo_lecturenote sep2013.pdf
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Universiti Kuala Lumpur
An Engineering Approach
!introduction to principles and applications of
macroscopic thermodynamics!
!"#$%&'()*%+,-
to accompany
Thermodynamics: An Engineering Approach, 6th editionby Yunus A. engel and Michael A. Boles
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General Overview
the ultimate goal is toDESIGNproductsthat meet society needs
Mechanical Engineering! Mechanics! Energy! Systems! Design
Thermodynamics!A part of the Energycomponentsof mechanical engineering.
! Governs ALL energyconsuming and transforming
devices and systems.
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Course OverviewBasic Concept
TerminologyPure Substance
Energy, Energy
Transfer and Analysis
Closed & Open System 2ndLaw
Thermodynamics
Thermodynamics ApplicationPower Generation Refrigeration
! Gas Power Cycle! Vapor Power Cycle! Combined Gas Power Cycle
! Refrigeration Cycle
!Thermodynamic& Energy
!Dimension!Unit!System &Control Volumes
!Process!Cycle!Temperature!Zeroth Law!Pressure
!Phase & PhaseChange
!Property Diagram!Property Table!Equation of State!Ideal Gas!Real Gas!CompressibilityFactor!ThermodynamicsProperties
!Forms of Energy!Energy Transfer
by Heat
!Energy Transferby work
!Mechanical Works!The 1stLaw!EnergyConversion!Energy &Environment
!Energy Balance!Specific Heats!Internal Energy!Enthalpy!Mass Balance!Flow Work andEnergy of Flowing
Fluid!Steady Flow!Unsteady Flow
!Energy Reservoir!Heat Engine!Refrigeration!Heat Pump!Reversible andIrreversible Process
!Carnot Cycle!Carnot Principle!Carnot Devices
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Course ObjectiveThe objective of this course are.
! to cover the basic principlesofthermodynamics
! to present a wealth of real-worldengineering applications forengineering practices
! to develop an intuitiveunderstanding of the subject matter
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Universiti Kuala Lumpur
Introduction and Basic Concepts
Chapter 1!"#$%&'()*%+,-
to accompany
Thermodynamics: An Engineering Approach, 6th editionby Yunus A. engel and Michael A. Boles
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Outline
! Thermodynamicsand Energy! Application AreasofThermodynamics
! Dimensionsand Units! Systemand Control Volume! Propertiesof a System! Density andSpecific Gravity! Stateand Equilibrium! Processesand Cycles! Temperature andZeroth Law!
Pressure
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THERMODYNAMICS and ENERGY
! thermodynamics is the science ofenergy it about understanding the
patterns of energy changeand how
these changes relate to the state of
matter
! thermodynamics is a branch ofphysics that is built upon the
fundamental laws that heatand workobey
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Conservation of Energy! During an interaction, energycan change from one form toanotherbut the total amount of
energy remains constant.
! Energy cannot be created ordestroyed.
Energy cannot be created ordestroyed; it can only change
forms (the first law).
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The 1stLaw of Thermodynamics
! An expression of theconservation of energy principle.! The first law asserts thatenergy is a thermodynamic
property.
Conservation of energyprinciple for the human
body.
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The 2ndLaw of Thermodynamics
! It asserts that energy hasqualityas well as quantity, andactual processes occur in the
direction of decreasing quality of
energy.
Heat flows in the directionof decreasing temperature.
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Classical vs Statistical
Classical thermodynamics!A macroscopic approachto the study ofthermodynamics that does not require a knowledge ofthe behavior of individual particles.
! It provides a direct and easy way to the solution ofengineering problems and it is used in this text.
Statistical thermodynamics!
A microscopic approach, based on the averagebehavior of large groups of individual particles.
! It is used in this text only in the supporting role.
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Application Areas
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DIMENSIONSrefer to physical nature of quantity
Primary/FundamentalMass m
Length LTime s
Temperature TPressure P
!"#$%'($)
Secondary/DerivedVelocity v
Energy EVolume V
Area A
+),-.)% 0,(1 2,-1#,3
! !
amF =
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UNITSdefining how measurements are made
English SystemUnited States Customary System (USCS)
12 in. in1 ft, 16 oz in1 lb
!no numerical base
! units are related arbitrarilyMetric System SIInternational System
meter (m), kilogram (kg)
! simple and logical based on a decimalrelationship between the various units
! mostly used for scientific andengineering work
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Dimensional HomogeneityAll equation MUSTbe dimensionally
homogeneous
( )
kJkJkJ
kgXkgkJkJkJ
+=
+!
( ) ( )
kgkJkJkJ
kg
kJkJkJE
+!
""#
$%%&
'+= 25
correction
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SYSTEM, SURROUNDINGS, BOUNDARY
Thermodynamics
System
System! a quantity of matter or a region
in space! may be considered as CLOSEDorOPEN
! system depending on whether a fixedMASS or fixed VOLUMEis chosen
Boundary!.control surface! real or imaginary surface thatseparates the system from its
surroundings! contact surface shared by the systemand its surroundings! zero thickness without mass andvolume
! can either be fixed or movable
Energy
Flow
Surroundings! mass or region outside thesystem
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SYSTEM
0=dtdm
ClosedSystem
OpenSystem
Mass Flow
Mass Flow
Energy
Flow
Energy
Flow
IsolatedSystem
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Closed SYSTEMAlso known as CONTROL MASS, when a
particular quantity of matter in a systemunder study contains the same matter with
fixed amount of mass.
no mass may enter or leave the system
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Open SYSTEMAlso known as CONTROL VOLUME,
has mass as well as energy crossingthe boundary or CONTROL
SURFACE.
mass FLOW across their control surface
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Open SYSTEM
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Isolated SYSTEM! Energy in the form of work or heat can cross theboundary. In the event that energy is not allowedto cross in a closed system, the system is known
as ISOLATED SYSTEM.
! Normally a collection of a a main system and itssurroundings that are exchanging mass andenergy among themselves and no other system.
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Properties of a SYSTEM! Every system has certain characteristics bywhich its physical condition is described. Such
characteristic of a system is called a PROPERTY,it is used to describe a system and predict its
behavior.
! Property is INDEPENDENT OF THE PATHused toarrive at the system condition! Some familiar properties are Pressure,Temperature, Volume and Mass. Other may include
viscosity, thermal conductivity, modulus of
elasticity, thermal expansion coefficient, electric
resistivity, and even velocity and elevation.
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Properties of a SYSTEM! Properties are considered to be either intensiveor extensive.
! Intensive properties are those that areindependent of the mass of the system. (not
additive to the
! Extensive properties are those whose valuesdepend on the size of the system.
EXTENSIVE
mass
volume
energy
velocity
additive over the
system
INTENSIVE
temperature
pressure
density
specific volume
not additive over the
system
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Properties of a SYSTEM
! Properties are considered to beeither intensive or extensive.! Intensive properties are thosethat are independent of the mass
of the system. (not additive over
the system)! Extensive properties are thosewhose values depend on the size
of the system. (additive over the
system)
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extensive properties per unit mass areintensive properties
SPECIFIC VOLUME DENSITY
Properties of a SYSTEM
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Density is defined as a mass per unit volume
Density
Specific volume is the reciprocal of density
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Continuum! Matter is made up of atoms that are widely spaced in
the gas phase. Yet it is very convenient to disregard theatomic nature of a substance and view it as acontinuous, homogeneous matter with no holes, that is,a continuum.! The continuum idealization allows us to
treat properties as point functions and toassume the properties vary continually inspace with no jump discontinuities.! This idealization is valid as long as the
size of the system we deal with is largerelative to the space between themolecules.! This is the case in practically all
problems.
! In this text we will limit our considerationto substances that can be modeled as acontinuum.
Despite the large gapsbetween molecules, asubstance can be treatedas a continuum because ofthe very large number ofmolecules even in an
extremely small volume.
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When the density of a substance is given relative to the
density of a well-know substance, then it is called SpecificGravity or Relative Density.
Specific Gravity
OH
SG
2
!
!=
The specific gravity is defined asthe ratio of the density of a
substance to the density of somestandard substance at a specified
temperature.
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The weight of a unit volume of a
substance is called a specific weight.
Specific Weight
gs !" = )/( 3mN
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STATEThe word STATEin thermodynamics refers to the
condition of a system as described by its
properties. The properties can be measured orcalculated throughout the entire system which
described the condition or state of the system.
Changing one property, changes the state
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!Thermal equilibriumtemperature is the same throughout thesystem
!Mechanical equilibriumno change of pressure with time
!Phase equilibriummass of each phase reaches an
equilibrium level and stay there
!Chemical equilibriumchemical composition does not change
with time
EQUILIBRIUM Condition
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ST TE ND EQUILIBRIUMThe state of a system is described by its properties. Once a
sufficient number of properties are known, we would be able
to specify the state of any system and shall be able to
calculate all other properties of the system.
How many properties ?The number of properties required to specify a state of a simple,
homogeneous compressible system shall be given by the
The THERMODYNAMICS
STATE of a simple
homogeneouscompressible system is
completely specified bytwo independent,
intensive properties.
ST TE POSTUL TE
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PROCESSES and CYCLESAny change that a system undergoes from one equilibrium state to
another is called a PROCESS, and the series of states through
which a system passes during a processis called the PATHof theprocess. When the final state is identical with the initial state theprocess is defined as a CYCLE.
/0*0# 2 /0*0# 345678//9
/0*0# 2 /0*0# 3 /0*0# 27:7;8 9
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! Isothermal Processtemperature remains constant throughoutthe process
! Isobaric Processpressure remains constant throughoutthe process
! Isometric Processspecific volume remains constantthroughout the process
PROCESSES Condition
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EQUILIBRIUM PROCESSES
! Sufficiently slow process! Adjust itself internally! Represent idealized process! Easy to analyze! Deliver most work
as the piston-cylinder devices iscompressed suddenly, all the nearby
molecule will pile up in a small regionnear piston and creating a high-
pressure region thus the systemcan no longer be in an equilibrium
state..
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PROCESSES DI GR Mprovides mean to easily visualize processes.
Thermodynamic properties are used as
coordinates, such as temperature (T), pressure (P),and volume (V) or specific volume (v).
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STEADY-FLOW PROCESSESa process during which a working fluid flows through a
control volume (open-system) steadily at any time. Although
the properties of the working fluid may change from point topoint within the control volume system, but at any fixed point
they remain the same at any time.
%# ?
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ZEROTH LAW OF THERMODYNAMICSTwo bodies individually in THERMAL EQUILIBRIUMwith a third bodies are in thermal equilibrium with
each other.
T t S l
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Temperature Scales as a common basis for temperature
measurements, based on some reproducible
states such as freezing and boiling points of
water.Two-Points Scales! Celcius Scale C(0~100 C)and Fahrenheit Scale F(32~212 F)
Thermodynamics Temperature ScaleIndependent of the properties of any subtances
! Kelvin Scale Kand Rankine Scale RIdeal Gas Temperature ScaleBased on the principle that at low pressure, the temperature of a gas
is proportional with its pressure at constant volume, T=a + bP
Id l G T t S l
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Ideal Gas Temperature Scale
FIGURE 145
P versus T plotsof the experimental data obtained from a constant-volume gas thermometer using four different
gases at different (but low) pressures.
TEMPERATURE MEASUREMENTS
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TEMPERATURE MEASUREMENTSREFERENCE POINTS
Relationship between Kelvin and Celcius Scale
Relationship between Rankine and Farhrenheit Scale
Relationship between Two Unit System
PRESSURE
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PRESSUREdefined as the normal force exerted by a fluid per unit area
211
m
NPa =
Pa9.807x10m
N9.807x10
cm
N9.807
cm
kgf1
bars1.01325kPa101.325Pa101,325atm1
kPa100MPa0.1Pa101bar
4
2
4
22
5
===
===
===
A
FP =
PRESSURE
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PRESSURE
Absolute pressure
Is the actual pressure at a givenposition/location and measuredrelative to absolute zero pressure
Gage pressureIs the pressure difference between
the absolute pressure and local
atmospheric pressure
Vacuum pressureIs the pressure between the
atmospheric pressure and theabsolute pressure. It is the pressure
below the atmospheric pressure.
absatmvac
atmabsgage
PPP
PPP
!=
!=
PRESSURE
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PRESSUREVariation with depth
z
zg
PPP
!=
!=
"=!
#
$
12
PRESSURE
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PRESSUREVariation with depth
PRESSURE
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PRESSUREVariation with depth
Pascals Law
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Pascals Law
The ratio A2/A1is calledthe ideal mechanical
advantageof the hydrauliclift
PRESSURE measurement
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PRESSURE measurementmanometer
12
2
PP
ghPP atm
=
+= !
measuring pressure with fluid column
PRESSURE measurement
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PRESSURE measurementmanometer
1332211 PghghghPatm =+++ !!!
PRESSURE measurement
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PRESSURE measurementmanometer
( )( )ghPP
PgaghhagP
1221
21211
!!
!!!
"="
=""++
Barometric PRESSURE
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Barometric PRESSURE measuring atmospheric pressure
Universiti Kuala Lumpur
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Universiti Kuala Lumpur
Energy, Energy Transfer & General Energy Analysis
Chapter 2!"#$%&'()*%+,-
to accompanyThermodynamics: An Engineering Approach, 6th edition
by Yunus A. engel and Michael A. Boles
O tli
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Outline! Understanding energy and forms of Energy!
Concept of Energy Transfer! First Law of Thermodynamics! Energy Balance and Energy Transfer! Energy and the Environment
Understanding ENERGY
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Understanding ENERGY
Understanding ENERGY
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Understanding ENERGY! If we take the entire roomincluding the air and the
refrigerator (or fan)as the system, which is an
adiabatic closed system since the room is well-sealedand well-insulated, the only energy interaction involved
is the electrical energy crossing the system boundary
and entering the room.
!As a result of the conversionof electric energy consumed by
the device to heat, the room
temperature will rise.
Form of ENERGY
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Form of ENERGY!energy exists in numerous forms such as thermal,
mechanical, kinetic, potential, electric, magnetic, chemical,
and nuclear, and their sum constitutes the total energy ofthe systemdenoted as E (kJ).On a unit mass basis it is
denoted ase=E/m (kJ/kg)
Macroscopic
With respect to outsidereference frame
MicroscopicRelated to the molecular
structure of the system
Macroscopic ENERGY
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!Kinetic energy, KEThe energy that a system
possesses as a result of its motion
relative to some reference frame.
!Potential energy, PEThe energy that a systempossesses as a result of its
elevation in a gravitational field.
!Flowing Fluid
Macroscopic ENERGY
ke per unit mass
pe per unit mass
Mass flow rate
Energy flow rate
Microscopic ENERGY
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Microscopic ENERGYinternal energy = microscopic form of energy denoted as U
!related to the molecularstructure and the degree of
molecular activity
!viewed as the sum of kineticand potential energy of the
molecules
Total ENERGY
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Total energy of a system
Energy of a system per unit mass
Total energy per unit mass
Total ENERGY
Energy Transfer
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Energy Transfer
Mass
out
Massin
System Boundary
Control Volume
!energy may be transported across the system boundaryin several ways. In a closed system (fixed mass), energy is
transported in the form of heatand work. For controlvolume (open system), energy can cross the boundary in
the form of heat, workand energy transported by the
mass streamcrossing the control surface.
Heat
Work
Heat vs Work
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Heat vs WorkHeat,Qis defined as the form of energy that is transferredbetween two systems (or a system and its surroundings)
by virtue of temperature difference whereas Work, Wisthe energy transfer associated with a force acting through
a distance.
Sign Convention For Energy Transfer
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Sign Convention For Energy Transfer
by Heat and Work
Heat and work are directional quantities, thus theirmagnitude and direction are necessary to completely
describe them
Classical Sign Conventionheat transfer to a system and work done by a system are
positive
Energy Transfer by Heat
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Energy Transfer by Heat!form of energy that is transferred across a systemboundary by mean of temperature difference between
two systems!otherwise it is workno heat transfer if same temperature
Adiabatic Process
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Adiabatic Process!is defined as a process with perfectly insulated system
and the heat transfer is zero .0=Q
There are two methods toachieve adiabatic process:
! the system is well insulated! both the system and thesurrounding are at the sametemperature!no driving force
for heat transfer
Heat Transfer
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Heat Transfer
Heat transfer per unit mass Heat transfer per unit timeRate of Heat Transfer
t
QQ =!
!recall that heat is energy in transition across the
system boundary solely due to temperature difference
between the system and its surrounding. Therefore, thenet heat transferred to a system is defined as ...
QQQQ outinnet =
!= ( )kJ
mQq = !!
"
#$$%
&
kg
kJ!"
#$%
&
s
kJ
Heat Transfer
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!=2
1
t
tdtQQ !
tQQ != !
Heat Transferwhen the rate of heat transfer
varies with time, the amountof heat transfer during a
process is determined by
integrating the rate of heat
transfer over the time interval.
when the rate of heat transferremains constantduring a
process, the above reduces to
Is there any Heat Transfer?
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Is there any Heat Transfer?
Heat Transfer Mechanism
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is the transfer of energy from the more
energetic particles of a substance to theadjacent less energetic ones as a result of
interactions between the particles. In solid,
the interaction is due to the combination of
vibrations of molecules and the energy
transport by the free electrons. In liquid and
gases, the interaction take places during
collision of the molecules.
Conduction
Fouriers Law
the rate of heat conduction ina direction is proportional to
the temperature gradient in
that direction
Heat Transfer Mechanism
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Conduction
xTAkQcond!
!=
1!0!"x
Where,
= heat flow/time(W)
k = thermal conductivity (W/m.K)
A = area normal to heat flow (m2)
= temperature gradient (K/m)
dx
dTAkQcond 1!=
!
condQ!
dx
dT
Heat Transfer Mechanism
C
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!is the mode of heat transfer between a solid surface
and the adjacent liquid of gas that is in motion, and itinvolves the combined effects of conduction and fluid
motion.
Convection
E#*0 !$*)-F#$ G#,"*)+-%
+
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!the rate of heat transfer by convection is determined
from Newtons Law of Cooling
7&)H#,0+&)
fsconv TThAQ !=
!
Where,
= heat transfer rate (W)
A = heat transfer area(m2)
h = convection heat transfer coefficient (W/m2.K)
Ts = surface temperature (K)
Tf = temperature gradient (K)
convQ!
Heat Transfer Mechanism
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!is the energy emitted by
matter in the form ofelectromagnetic waves as a
result of the changes in the
electronic configurations of
the atoms or molecules.
Unlike, other mechanisms,
radiation does not requires
medium for it to occur. It isfaster and suffers no
attenuation in a vacuum.
Just like sun light reaches
earth.
Radiation
/0#F*)IJ&=K%*) ;*L
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!gives the maximum rate of radiation that can be emitted by a
surface at an absolute Temperature Ts
. The idealized surface that
emits radiation at maximum rate is called blackbodyand the radiation
emitted by a blackbody is called blackbody radiation.
5*'+*0+&)
Where,Ais the surface area and
4
max, semit ATQ !=!
428./1067.5 KmWX
!
="
Stefan_Boltzman Constant
4
semit ATQ !"=!
Real surface
! is the emissivity of the surface
where 10 !! "
Blackbody surface
Kirchhoffs Law
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!states that the emissivity and absorptivity of a surface
are equal at the same temperature and wavelength.
Radiation
is the rate at which radiation is
incident on the surface
is the absorptivity of the surface
incQ!
!
incabs QQ !!
!=
Energy Transfer by Work
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Energy Transfer by Work!work is the energy transfer associated with a forceacting through a distance. If the energy crossing the
boundary of a closed system is not heat, it must be work.Thermodynamics workis defined as energy in transition
across the system boundary and is done by a system if
the sole effect external to the boundaries could have beenthe raising of the weight. Mathematical, the differential of
work can be expressed as
A rising piston, a
rotating shaft, and anelectric wire crossingthe system boundariesare all associated withwork interactions.
Energy Transfer by Work
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!if the force Fis not constant, the work donebetween two states is obtained by adding (integrating)
the differential amounts of work,
!! ==2
1
2
112
FdsWW "
Energy Transfer by Work
!total work done during aprocess 1-2 is determined by
following the process path andadding the differential amounts
of work done along the path
Energy Transfer by Work
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Energy Transfer by Work
m
Ww =
!
!
"
#
$
$
%
&
kg
kJ
Power is the work doneper unit time (kW)
Is there any Work Done?
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Is there any Work Done?
Heat & Work similarities
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Heat & Work similarities! both are recognized at the boundaries as they crossesthe boundary, they are boundary phenomena
!system possess energy, not heat or work
! both are path function,their magnitudes depend on
the path followed during a
process as well as end
states.
Properties are point functionshave exact differentials(d ).
! both are associated with aprocess, not a state. They
have no meaning at a state.
Path functions have inexactdifferentials( )
M&$N O&)#
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M&$N O&)#8=#,0$+,*= M&$N
Electrical work
Electrical power
When potential differenceand current change with
time
When potential difference
and current remain
constant
M&$N O&)#
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M&$N O&)#/"*F0 L&$N
( )
TnW
nTrnr
TFsW
sh
sh
!! !
!!
2
22
=
="#$%
&'==
M&$N O&)#
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M&$N O&)#/P$+)B L&$N
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( )2
1
2
2
2
1
xxkWspring !
=
The First Law of Thermodynamics
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yThe first Law of Thermodynamics states that energy can
neither be created nor destroyed; it can only change
forms. Implicitly, it is a statement of theConversation of Energy
Energy Balance
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gy
systemoutin EEE !="
the conservation of energy principle
the net change in the total energy of the system during aprocess is equal to the difference between the total
energy entering and the total energy leaving the system
during the process
Energy Change of a System, systemE!
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gy g yThe image cannot be displayed. Your computer may not have enough memory to open the image, or the image may have been corrupted. Restart your computer,and then open the file again. If the red x still appears, you may have to delete the image and then insert it again.
y
PEKEUE
EEEEE initialfinalsystem
!+!+!=!
"="=!12
!the determination of the energy change of the systemconcentrates the evaluation of the energy system at initial
and final state of the process, and taking the difference !
(
( )
( )12
2
1
2
2
12
2
1
zzmgPE
VVmKE
uumU
!="
!="
!="where
Energy Change of a System, systemE!
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gy g yThe image cannot be displayed. Your computer may not have enough memory to open the image, or the image may have been corrupted. Restart your computer,and then open the file again. If the red x still appears, you may have to delete the image and then insert it again.!when the final and initial state is specified, the values of
the specific internal energy can be determined from the
property table or property relation.
When the system is stationary, thus, the kinetic andpotential energy is zero,
( )12
uumUE !="="
Therefore, the energy change reduces to
PEKEUE
EEEEE initialfinalsystem
!+!+!=!
"="=! 12=0 =0
Ein& Eout
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in out!energy can be transferred to or from a systemin the form of
heat, work and mass flow, and this energy interaction is only
recognized as it crosses the system boundary. It represent theenergy gained or lostby a system during a process.
Q"#*0 0$*)-F#$ 0& *-(-0#%A E8R! SRTUA+),$#*-#- 0"# #)#$B( &F0"# %&=#,>=#- *)' 0">-0"# +)0#$)*= #)#$B( &F 0"#-(-0#%A *)' "#*0 0$*)-F#$F$&% * -(-0#%A E8R!;6//A '#,$#*-#- +0 -+),#0"# #)#$B( 0$*)-F#$$#' &>0&F 0"# -(-0#% ,&%#- F$&%
0"# #)#$B( &F 0"#%&=#,>=#-V
Q#)#$B( +)0#$*,0+&)0"*0 +- )&0 ,*>-#' D( *0#%P#$*0>$# '+W#$#),#+- L&$NV M65X O6U86U* -(-0#% &$ L&$N0$*)-F#$ 0& * -(-0#%A+),$#*-#- 0"# #)#$B( &F0"# -(-0#%A *)' M65XO6U8 J:0"# -(-0#% &$L&$N 0$*)-F#$ F$&% 0"#-(-0#%A '#,$#*-#- 0"##)#$B( &F 0"# -(-0#%V
QL"#)GR// T/
8U!85TUS* -(-0#%A0"# #)#$B( &F 0"# -(-0#%+),$#*-#- D#,*>-# %*--,*$$+#- #)#$B(V ;+N#L+-#A
L"#) GR// T/;8R
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9090
in outThe image cannot be displayed. Your computer may not have enough memory to open the image, or the image may have been corrupted. Restart your computer,and then open the file again. If the red x still appears, you may have to delete the image and then insert it again.
systemoutmassinmassoutinoutinoutin EEEWWQQEE !="+"+"=" ,,
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!realizing that energy is transferred in several forms, theenergy balance can be written as !
Energy Balance
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gy
!"!#$!"!#$
energypotentialandenergykineticenergy,internalinchange
flowmassandworkheat,bynsferenergy tranet
systemoutin EEE !="
the conservation of energy principle
the net change in the total energy of the system during a
process is equal to the difference between the totalenergy entering and the total energy leaving the system
during the process
systemoutmassinmassoutinoutinoutin EEEWWQQEE !="+"+"=" ,,
Energy Balance
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gy
tWW != !
!"!#$%
!"!#$%%
energypotentialandenergykineticenergy,internalinchangeofrate
flowmassandworkheat,bynsferenergy tranetofrate
systemoutin EEE !="
tQQ != !
the conservation of energy principle
In the rate form, the energy balance is represented as
For constant rates, the total quantities during a timeinterval are related to the quantities per unit times as
follows:
tEE !!=! !
Energy Balance
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9393
gy
systemoutin eee !="
other form of energy balance equation
Energy balance per unit mass
Energy balance in differential form
systemoutin
systemoutin
deee
dEEE
=!
=!
""
""
Energy Balance
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gy
outin
outin
EE
EE
=
=
! 0
012
=!="=! EEEEE systemoutin
For a closed system undergoing a CYCLEWhere the initial and final states are identical then
the energy balance for a cyclesimplifies to
In terms of heat and work
innetoutnet
innetoutnet
QW
QW
,,
,,
!! =
=
Ex 2-10: Cooling of a Hot Fluid in a Tank
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9595
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PEKEUEEWWQQ
EEEEE
outmassinmassoutinoutin
systemoutin
!+!+!="+"+"
"=!="
,,
12
Energy Balance
where )
( )( )
12
2
1
2
2
12
2
1
zzmgPE
VVmKE
uumU
!="
!="
!="
Ex 2-10: Cooling of a Hot Fluid in a Tank
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9696
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)00()0100()5000(
,,
!+!+!=
!+!+!=! outmassinmassoutinoutinoutin EEWWQQEE
For Einand Eout
00)800(
)()()(
2
121212
++!=
!+!+!=
"+"+"="
U
PEPEKEKEUU
PEKEUEsystem
For "Esystem
Energy Balance becomes
kJU
UUUUEWQEE systeminshtoutoutin
400
800100500
2
2
12,
=
!=+!
!="="=+!=!
ENERGY AND ENVIRONMENT! Th i f f f
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! The conversion of energy from one formto another often affects the environmentand the air we breathe in many ways, and
thus the study of energy is not completewithout considering its impact on theenvironment.
! Pollutants emitted during the combustionof fossil fuels are responsible forsmog,acid rain, and global warming.
! The environmental pollution has reachedsuch high levels that it became a seriousthreat to vegetation, wild life, and humanhealth.
Ozone and Smog! Smog: Made up mostly of ground-level ozone (O3), but it also
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! Smog:Made up mostly of ground level ozone (O3), but it alsocontains numerous other chemicals, including carbon monoxide(CO), particulate matter such as soot and dust, volatile organiccompounds (VOCs) such as benzene, butane, and other
hydrocarbons.! Hydrocarbonsand nitrogen oxidesreact in the presence of sunlight
on hot calm days to form ground-level ozone.! Ozoneirritates eyes and damages the air sacs in the lungs where
oxygen and carbon dioxide are exchanged, causing eventualhardening of this soft and spongy tissue.!
It also causes shortness of breath, wheezing, fatigue, headaches,and nausea, and aggravates respiratory problems such as asthma.! The other serious pollutant in smog is carbon
monoxide, which is a colorless, odorless,poisonous gas.! It is mostly emitted by motor vehicles.! It deprives the bodys organs from getting
enough oxygen by binding with the red bloodcells that would otherwise carry oxygen. It isfatal at high levels.! Suspended particulate mattersuch as dustand
sootare emitted by vehicles and industrialfacilities. Such particles irritate the eyes and the
lungs.
Acid Rain
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! The sulfur in the fuel reacts with oxygen to form sulfur dioxide(SO2),which is an air pollutant.! The main source of SO2is the electric power plants that burn high-
sulfur coal.! Motor vehicles also contribute to SO2emissions since gasoline and
diesel fuel also contain small amounts of sulfur.
! The sulfur oxides and nitric oxidesreact with water vapor and otherchemicalshigh in the atmosphere inthe presence of sunlight to formsulfuric and nitric acids.! The acids formed usually dissolve
in the suspended water droplets inclouds or fog.! These acid-laden droplets, which
can be as acidic as lemon juice, arewashed from the air on to the soilby rain or snow. This is known asacid rain.
The Greenhouse Effect: Global Warming
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! Greenhouse effect:Glass allows the solar radiation to enter freelybut blocks the infrared radiation emitted by the interior surfaces.This causes a rise in the interior temperature as a result of the
thermal energy buildup in a space (i.e., car).! The surface of the earth, which warms up
during the day as a result of theabsorption of solar energy, cools down atnight by radiating part of its energy intodeep space as infrared radiation.
! Carbon dioxide (CO2),water vapor, andtrace amounts of some other gases suchas methane and nitrogen oxides act like ablanket and keep the earth warm at nightby blocking the heat radiated from theearth. The result is global warming.!
These gases are called greenhousegaseswith CO2being the primarycomponent.! CO2 is produced by the burning of fossil
fuels such as coal, oil, and natural gas.
!A 1995 report:The earth hasl d d b t 0 5C
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already warmed about0.5Cduring the last century, and theyestimate that the earths
temperature will rise another2Cby the year 2100.!A rise of this magnitude can
cause severe changes inweather patternswith storms
and heavy rains and flooding atsome parts and drought inothers, major floods due to themelting of ice at the poles, lossof wetlands and coastal areasdue to rising sea levels, and
other negative results.! Improved energy efficiency,
energy conservation, and usingrenewable energy sourceshelpminimize global warming.
Systematic Solution Method
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! Sketch the system and show energy interactionacrossthe boundary.
! Determine the property relation. Is the working substancean ideal gas or a real substance? Begin to set up and fill in
a property table.
! Determine the process and sketch the process diagram.Continue to fill in the property table.!Apply conservation of mass and conservation of energyprinciples.
! Bring in other information from the problem statement,called physical constraints, such as the volume doubles orthe pressure is halved during the process.
! Develop enough equationsfor the unknowns and solve.
Universiti Kuala Lumpur
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Chapter 3
Thermodynamics
Properties of Pure Substances
to accompanyThermodynamics: An Engineering Approach, 6th edition
by Yunus A. engel and Michael A. Boles
Outline
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! Concept of Pure Substance!
Physics of Phase Change! Property Diagram! Property Tables! Ideal Gas and the Ideal Gas Equation! Real Gas and Compressibility Factor
PURE SUBSTANCESh homogeneous d fixed chemical composition
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!has a homogeneousand fixed chemical compositionthroughout and may exist in more than one phase!but the chemical
composition is the same in all phases.
Phases of Pure Substance
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! 3-D pattern and repeated! attractive forces are large! spacing very close!zero! molecules are in fixedpositions
! oscillate about equilibriumposition
! molecule velocity dependson T
! attractive force weaker thansolid
! spacing slightly greater thansolid
! molecules able to rotate andtranslate freely! molecules are no longer infixed position
! attractive forces are theweakest
! high energy level! far apart from each other! non-existent order! molecule moves at random andcollide within each other
! molecules are no longer infixed position
Phase-Change Processes
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of a Pure Substance
Saturated
liquid
Saturated
vapor
Phase-Change Processes
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State 1 T=20 C and P=1 atmAt state 1, water exists in the liquid phase, or socalled compressed liquidor subcooled liquid,meaning that it is not about to vaporize.
Process 1-2 T=20~100 C and P=1 atmAs heat being transfer and the temperature rises, the
liquid water expand thus increases the specific
volume. To accommodate this changes, the piston
will move up. The pressure is kept constant at P=1
atm since it depends on the outside atmospheric
pressure and the weight of the piston.
As more heat is being transferred, the
temperature will keep rising until it reaches
T=100 C, at this point, the water still exists in theliquid phaseand additional heat transfer will cause
some of the liquid water to vaporize.
Phase-Change Processes
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Process 2 T=100 C and P=1 atmAt state 2, the liquid water has reached thetemperature, called saturation temperature, at
which it begins to boil and some of the liquid
water will start to vaporize (from liquid to vapor).
A liquid that is about to vaporize is called a
saturated liquid.
Process 2-3 T=100 C and P=1 atmOnce the boiling starts, additional heat transfer
does not increase the temperature of the liquid.
The temperature will remain at 100 C until all the
liquid is completely vaporized. This is where the
phase-change from liquid to vapor takes place if
the pressure remains constant at 1 atm. During
this process, the volume will increase and liquid
level will decrease as result of more liquid turning
to vapor. At this stage, the substance is called
saturated liquid-vapor mixture.
Phase-Change Processes
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Process 3 T=100 C and P=1 atmAt state 3, midway about the vaporization line, thecylinder contains equal amount of liquid and
vapor at constant temperature and pressure.
Process 3-4 T=100 C and P=1 atmAs heat is continued being transferred, the
vaporization process will continue until all liquid
turns into vapor completely. More vapor will
occupy the cylinder as vapor will gradually
increase and liquid decreases. At this stage, the
substance is called saturated liquid-vapormixture.
Phase-Change Processes
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Process 4 T=100 C and P=1 atmAt state 4, when the last drop of the liquid water is
completely vaporized, the entire cylinder now
contains with vapor that is on the border line of
the liquid phase. Any heat loss from this vapor
will cause some of this vapor to condense (from
vapor to liquid). A vapor that is about to condense
is called a saturated vapor.
Process 4-5 T=100~ C and P=1 atmAs heat is continued being transferred, both the
temperature and the volume will increase. At
temperature higher that the saturation
temperature, any heat loss will result intemperature drop but no condensation will take
place, as long as the temperature remains above
100 C. A vapor that is not about to condense is
called a superheated vapor.
Phase-Change Processes
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Process 5 T= 300 C and P=1 atmAs heat is continued being transferred, both thetemperature and the volume will continue to
increase.
Phase-Change Processes
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What happen if we reverse the process?If the entire process is
reversed by cooling offthe water and whilst
maintaining the pressure
at 1 atm, the liquid water
will return to state 1
retracing the same path .In doing so, the amount of
heat released will exactly
match the amount of heat
added during the heating
process.
Saturation Temperature and PressureAt a given pressure the temperature at which a pure substance changes
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At a given pressure, the temperature at which a pure substance changes
phase is called Saturation Temperature.Likewise, at a giventemperature, the pressure at which a pure substance changes phase is called
Saturation Pressure.
Water boils at 100 C at 1 atm
Saturation Temperature and Pressure
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Heat Transfer of Phase ChangeLatent Heat
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The amount of energy absorbedand releasedduring phase changeLatent Heat ofFusionEnergy absorbed during melting
Latent Heat ofVaporizationEnergy absorbed during vaporization
L=Latent Heat of SubstancemLQ
=
Latent Heat ofSublimationEnergy absorbed during sublimation
! Latent heat: Th t f
Heat Transfer of Phase ChangeLatent Heat
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! Latent heat:The amount of energyabsorbed or released during a phase-change process.
! Latent heat of fusion:The amountof energy absorbed during melting. It isequivalent to the amount of energyreleased during freezing.
! Latent heat of vaporization:Theamount of energy absorbed duringvaporization and it is equivalent to theenergy released during condensation.! The magnitudes of the latent heats
depend on the temperature or pressureat which the phase change occurs.!
At 1 atm pressure, the latent heat offusion of water is 333.7 kJ/kg and thelatent heat of vaporization is 2256.5 kJ/kg.! The atmospheric pressure, and thus
the boiling temperature of water,decreases with elevation.
Key Terms
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Saturated
liquid
Saturated
vapor
The T-v Diagram
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The T-v Diagram
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The T-v Diagram
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The P-v Diagram
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The P-v Diagramsolid liquid vapor
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solid-liquid-vapor
The P-T DiagramThe phase diagram
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The phase diagram
The P-v-T Surface Diagram
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Property Tablebecause the relationship among thermodynamics
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!because the relationship among thermodynamicsproperties are too complex to be expressed in term of a
simple equation, these data are normally tabulated in theform of table.
! Some thermodynamic properties can be measured easily, butothers cannot and are calculated by using the relations betweenthem and measurable properties.!
The results of these measurements and calculations are presentedin tables in a convenient format.
No Phase Table for H20
1 Saturated liquid and vapor A-4 and A5
2 Superheated vapor A-6
3 Compressed liquid A-7
Property Tableforsaturated liquid and saturated vapor Table A-4Ex1
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q px1chap3.ppt
Key Thermodynamics Properties
Enthalpy
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py!the combination of properties derived for the sake of
simplicity and convenience.
Pvuh
PVUH
+=
+=
Property Tableforsaturated liquid and saturated vapor
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130130
q p
Key Thermodynamics Properties
Enthalpy
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py!the combination of properties derived for the sake of
simplicity and convenience. The quantity hfgis called theenthalpy of vaporization (or latent heat of vaporization. It
represent the amount of energy needed to vaporize a unit
mass of saturated liquid at a given temperature or
pressure.
Pvuh
PVUH
+=
+=
Property Tableforsaturated liquid and saturated vapor
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Property Tableforsaturated liquid and saturated vapor
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Property Tableforsaturated liquid-vapor mixture
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q p
!for constant pressure heat addition process, there is a
mixture of saturated liquid and saturated vapor during thevaporization process.
Property Tableforsaturated liquid-vapor mixture
Q lit th ti f f t th t t l f
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Quality x the ratio of mass of vapor to the total mass ofthe mixture
Property Tableforsaturated liquid-vapor mixture
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Property TableForsuperheated vapor Table A-6
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Property TableForsuperheated vapor Table A-6
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Property TableForsuperheated vapor
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Property Tableforcompressed liquid Table A-7
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Property Tableforcompressed liquid Table A-7
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141141
In the absence of compressed liquid
data, approximatecompressedliquid as saturated liquid at the
temperature
Property Tableforcompressed liquid Table A-7
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How to choose the right Table?!the correct table to use to find the thermodynamics
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yproperties of a real substances can always be determined
by comparing the known state properties to the propertiesin the saturation region.
vf vg v=superheatedtable
v=vf+ x(vg-vf)
Using Steam Tables Ex 4-9 pg 135
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Sat. mixture
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vf vg
T= Tsat@P=200 kPa
u=uf+ x(ug-uf)
X=0.6
P=200 kPa
Step 1Step 3
intensive properties
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146
uf ug
T= Tsat@P=1000 kPa
P=1000 kPa
u=2950
4 30 Ten kg of R134A fill a 1 348 m3 rigid container at an initial
extensive properties System, rigid=v constant
m=mass (kg) V=volume (m3) V1=V2
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147
4-30 Ten kg of R134A fill a 1.348 m3rigid container at an initialtemperature of -40C. The container is then heated until the pressure is
200 kPa. Determine the final temperature and initial pressure.
State T P v Phase
1 -40
C
0.1348
m3/kg
2 200kPa
Working fluid
Step 1Find intensive
properties
kg
m
kg
m
m
Vv
mvV
33
1348.010
348.1===
=
State T P v Phase
1 -40C 51.25kPa
0.1348 m3/kg Since vf
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148
2 200kPa
v2=v10.1348 m3/kg
Since vg
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149
Vf=0.0007054 Vg=0.36081
v=vf+ x(vg-vf)=0.1348 m3/kg
T
T= C
P= 51.25kPa
P= 200kPa
T= Tsat@P=200kPa
-10.09C
Vf=0.0007533 Vg=0.099867
2
1
Step 2
T2
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P= 1000 kPa T= C
vf= m3/kg vg= m
3/kg
uf= kJ/kg ug= kJ/kg
State T P v Phase
1 -40C 51.25kPa
0.1348 m3/kg Since vf
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151
2 66.30C
200
kPa
v2=v1
0.1348 m3
/kg
Since vg
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State T P v Phase
1 200kPa
0.12322 m3/kg
Since vf
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v=vf+ x(vg-vf)=0.0616 m3/kg
T= Tsat@P=200kPa
-10.09C
Vf=0.0007533 Vg=0.099867
2 1
Step 2
T1
2 -10.09C
200kPa
v2=0.5v10.0616 m3/kg
Since vf
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Then,
( )
kg
kJ
uuxuu fgfmix
6.152
28.3848.2246140.028.38
2,
=
!+=
!+=
2 -10.09C
200kPa
v2=0.5v10.0616 m3/kg
152.6 Since vf
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A liquid will take theshape of its container
but exhibits a free
surface.
A gas will fill its containercompletely and does not
exhibit a free surface.
gasgas
containergas
PTVV
,
=
Ideal-GasEquation of State
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!an equation that relates pressure, volume and
temperature of a sample of matter. Its provides a morepractical and desirable approach in establishing
relationships between the properties of the gases and it
predicts the P-v-T behavior of a gas quite accurately
within some properly selected region.
RTPvv
T
RP =!"
#$%
&= ,
gas constant R
!is different for each gas and Ruis the universal gast t
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157157
M
RR
u=
!
!#
$
Kkmolmbar
KkmolmkPa
KkmolkJ
Ru
./.08314.0
./.314.8
./314.8
3
3
The image cannot be displayed. Your computer may not have enough memory to open the image, or the image may have been corrupted. Restart your computer, and then open the file again. If the red x still appears, you may have to delete the image and theninsert it again.
mol
gram
kmolN
kgmM ==
)(
)(
constant
Ideal-GasSeveral different forms of Equation of State
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158158
( )
vNV
NRRMNmR
mvV
u
=
==
=
Ideal-GasFor a fixed mass, the properties of an ideal gas at twodiff t t t l t d t h th b
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different states are related to each other by
2
22
1
11
RT
VP
RT
VPm ==
How to defineIdeal-Gas
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!determination based on
errors yield !
Compressibility Factora measure of deviation from ideal-gas behavior
real gases deviate from ideal-gases behavior
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161161
!real gases deviate from ideal-gases behaviorsignificantly especially near the saturation region and
critical point. This deviation can be accurately accounted
for by a correction factor called the
compressibility factor Z
ZRTPvRT
PvZ == ,
ideal
actual
v
vZ = wherePRTv
actual =
Compressibility Factor
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162162
Principle of Corresponding States!gases behave differently at a given temperature andpressure real gases, but they behave very much the
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163
pressure real gases, but they behave very much the
same at temperature and pressure normalized with
respect to their critical temperatures and pressures
cr
R
P
PP =
cr
R
T
TT =
!
!
!!#
$
...=Z
Generalized Compressibility Chart
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Observation from Generalized Compressibility Chart
! at very low pressures, PR
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! at high temperatures, TR > 2, ideal gasbehavior can be assumed with good accuracy
regardless of pressure (except when PR >> 1)
! the deviation of a gas from ideal-gas behavior isgreatest in the vicinity of the critical point
pseudo-reduced specific volume!when Pand v, or Tand vare given instead of Pand
T, the pseudo-reduced specific volume can be
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, p p
calculated to used the generalized compressibility
chart
crcr
actual
R
PRT
vv
/=
cr
R
P
PP =
!!
"
!!
#
$
...
=Z
Van der WaalsEquation of State
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( ) RTbvv
aP =!"
#
$%
&
'+
2
cr
cr
cr
cr
P
RTb
P
TRa
8,
64
27 22
==
Beattie-BridgemanEquation of State
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!"#$
%& '=!
"#$
%& '=
v
bBBv
aAAoo
1,1
( )232
1v
ABvTv
c
v
TRP u !+"
#$%
&' !=
Equation of State
Benedict-Webb-Rubin
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169169
2
33
/
22622 1
1 vuoouo
u
evTv
c
v
a
v
aTbR
vT
C
ATRBv
TR
P !!" #
$%
&'(
)+++
#+$%
&'(
)##+=
VirialEquation of State
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( ) ( ) ( ) ( ) .....5432 +++++= vTd
v
Tc
v
Tb
v
Ta
v
RTP
ComparisonEquation of State
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Enthalpy Changes
forLiquids
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Tconstant, pump 0=!T
Pconstant, heater 0=!P TCuh av!"!=!
( )1212 PPvhhPvh
!=!
"="
( )satTfTfTP
TfTP
PPvhh
hh
!+"
"
###
##
,
,
By taking state 2 to be compressed liquid at given P and T andstate 1 to be saturated liquid at the same T
Universiti Kuala Lumpur
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Energy Analysis of Closed System
Chapter 4
!"#$%&'()*%+,-
to accompanyThermodynamics: An Engineering Approach, 6th edition
by Yunus A. engel and Michael A. Boles
Outline
! Examine the PdV Works
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!Identify Energy Balance for Closed System
! Define Specific Heat, Internal Energy andEnthalpyfor Ideal Gas
! Describe incompressible substances! Analyze Energy Balance for Heat and WorkInteraction of a Closed System
Energy Transfer by Work!work is the energy transfer associated with a forceacting through a distance. If the energy crossing the
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g g gy g
boundary of a closed system is not heat, it must be work.
Thermodynamics workis defined as energy in transition
across the system boundary and is done by a system if
the sole effect external to the boundaries could have beenthe raising of the weight. Mathematical, the differential of
work can be expressed as
A rising piston, arotating shaft, and an
electric wire crossingthe system boundariesare all associated withwork interactions.
!if the force Fis not constant, the work donebetween two states is obtained by adding (integrating)
Energy Transfer by Work
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between two states is obtained by adding (integrating)
the differential amounts of work,
!! ==2
1
2
112
FdsWW "
!total work done during aprocess 1-2 is determined by
following the process path and
adding the differential amountsof work done along the path
Energy Transfer by WorkW
w = !!#
$$& kJ
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m
w = !!
"
$$
%kg
Power is the work doneper unit time (kW)
Work Done
the net work done by a closed system may be in two
By a closed system
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!the net work done by a closed system may be in two
forms:-1. Rotating shaft, electrical , that is otherworks not
associated with moving boundary works.
2. Moving Boundary Work
Thus, the net work done by a closed systemis defined as
( )
( ) bothernet
botherinoutnet
WW
WWWW
+=
+! !"=
Moving Boundary WorkPdVwork Consider, Fig 4-2, initial pressure P, volume
of piston V and total area A If the piston is
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!one form of mechanical
works. It is the expansion andcompression work of a
moving boundary in piston-
cylinder devices.
of piston Vand total areaA. If the piston is
allowed to move a distance ds, in a quasi-equilibrium manner, the work done during
a process is given by
PdVPAdsFdsWb
===!
work is done bythe gas on the
piston
Total work Done
Moving Boundary Work
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180
The total area A under the process
curve 1-2 is obtained by adding all the
differential areas.
!=
2
1
PdVWb
!by adding all the differentialworks from the initial stage 1
to the final stage 2.
!! ===
2
1
2
1
PdVdAAArea
therefore, the area under the
Moving Boundary Work
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181181
process curve on a P-V diagram
is equal, in magnitude, to the
work done during a quasi-equilibrium expansion or
compression process of a
closed system
Quasi-equilibrium processA process during which the
system remains nearly in
equilibrium at all times.
Wbis positive for expansionWbis negative for compression
Moving Boundary Work
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Energy is conserved
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( )dxFAPF
WWWW
crankatmfriction
crankatmfrictionb
! ++=
++=
2
1
Work DoneMoving boundary for Constant Volume
Total Work Done
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02
1
== ! PdVWb
!if the volume is held constant, dV=0, the boundary work equationbecomes
Work DoneMoving boundary for Constant Pressure
Total work Done
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!if the pressure is held constant, the boundary work equation
becomes
( )122
1
2
1 VVPdVPPdVWb !="="=
Work DoneMoving boundary for Constant Temperature Ideal Gas
Total work Done!if the temperature of an ideal gas system is held constant, then the
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!if the temperature of an ideal gas system is held constant, then the
equation of state provides the pressure volume relation, then
boundary work equation becomes
!!"
#$$%
&=== ''
1
22
1
2
1
lnV
VmRTdV
V
mRTPdVW
b
For an ideal gas in a closed system (mass, m=constant),
1
2
2
1
2
22
1
1121
thus
,,
V
V
P
P
RT
VP
RT
VPmm
=
==
!!"
#$$%
&=
2
1ln
P
PmRTW
b
Work DoneMoving boundary for Constant Temperature Ideal Gas
Total work DoneC
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1
2
11
1
2
2
1
2
1
2
1
ln
ln
V
VVP
V
VC
V
dVC
dVV
C
PdVWb
=
=
=
==
!
!!
V
C
P
or
CmRTPV
=
==
mRTVPVP ==2211
where
Work Done!for actual expansion and compression processes of
gases pressure and volume are often related by
Polytropic Process
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gases, pressure and volume are often related by
PVn=C, where n and C are constants.
Work DonePolytropic Process
The pressure for a polytropic process can be expressedas
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1
1
1
1
2
2
2
2
1
+!!=
==
+!+!
!""
n
VVC
dVCVPdVW
nn
nb
nCVP !=
as
Thus,
Work DonePolytropic Process
nn
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190190
nn
VPVPC 2211 ==
1
1
1122
!
"
"
=
n
n
VPVPWb
since
Work DonePolytropic Process for Ideal Gas
Ideal Gas mRTPV =
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191191
1
112
!
"
"
=
n
n
TTmR
Wb
Ideal Gas mRTPV
Work DonePolytropic Process for n=1
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!!#
$$&
=
== '' (
1
2
2
1
12
1
ln
V
VPV
dVCVPdVWb
Energy Balancethe conservation of energy principle
the net change in the total energy of the system during aprocess is equal to the difference between the total
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193193
systemoutin EEE !="
process is equal to the difference between the total
energy entering and the total energy leaving the systemduring the process
Energy Change of a System,The image cannot be displayed. Your computer may not have enough memory to open the image, or the image may have been corrupted. Restart your computer,and then open the file again. If the red x still appears, you may have to delete the image and then insert it again.
systemE!
!the determination of the energy change of the systemconcentrates the evaluation of the energy system at initial
and final state of the process and taking the difference
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194194
PEKEUE
EEEEE initialfinalsystem
!+!+!=!
"="=!12
and final state of the process, and taking the difference !
(
( )
( )12
2
1
2
2
12
2
1
zzmgPE
VVmKE
uumU
!="
!="
!="where
Energy Change of a System,The image cannot be displayed. Your computer may not have enough memory to open the image, or the image may have been corrupted. Restart your computer,and then open the file again. If the red x still appears, you may have to delete the image and then insert it again.
systemE!
!when the final and initial state is specified, the values ofthe specific internal energy can be determined from the
property table or property relation
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property table or property relation.
When the system is stationary, thus, the kinetic andpotential energy is zero,
( )12
uumUE !="="
Therefore, the energy change reduces to
PEKEUEEEEEE initialfinalsystem
!+!+!=!
"="=! 12=0 =0
Ein& EoutThe image cannot be displayed. Your computer may not have enough memory to open the image, or the image may have been corrupted. Restart your computer,and then open the file again. If the red x still appears, you may have to delete the image and then insert it again.!realizing that energy is transferred in several forms, the
energy balance can be written as !
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systemoutmassinmassoutinoutinoutin EEEWWQQEE !="+"+"=" ,,
The image cannot be displayed. Your computer may not have enough memory to open the image, or the image may have been corrupted. Restart your computer,and then open the file again. If the red x still appears, you may have to delete the image and then insert it again.
Energy Balancethe conservation of energy principle
the net change in the total energy of the system during aprocess is equal to the difference between the total
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!"!#$!"!#$
energypotentialandenergykineticenergy,internalinchange
flowmassandworkheat,bynsferenergy tranet
systemoutin EEE !="
process is equal to the difference between the total
energy entering and the total energy leaving the systemduring the process
systemoutmassinmassoutinoutinoutin EEEWWQQEE !="+"+"=" ,,
Energy Balancethe conservation of energy principle
In the rate form, the energy balance is represented as
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198198
tWW != !
!"!#$%
!"!#$%%
energypotentialandenergykineticenergy,internalinchangeofrate
flowmassandworkheat,bynsferenergy tranetofrate
systemoutin EEE !="
tQQ != !
For constant rates, the total quantities during a timeinterval are related to the quantities per unit times as
follows:
tEE !!=! !
Energy Balanceother form of energy balance equation
Energy balance per unit mass
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systemoutin eee !="Energy balance in differential form
systemoutin
systemoutin
deee
dEEE
=!
=!
""
""
Energy BalanceFor a closed system undergoing a CYCLE
Where the initial and final states are identical then
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200200
outin
outin
EE
EE
=
=
! 0
012 =!="=! EEEEE systemoutinthe energy balance for a cyclesimplifies to
In terms of heat and work
innetoutnet
innetoutnet
QW
QW
,,
,,
!! =
=
Energy Balance for Closed System!the energy balance for a closed system, based on the classical
thermodynamics sign convention, is represented as
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201201
PEKEUWQ
EWQ
outnetinnet
systemoutnetinnet
!+!+!="
!="
,,
,,
If the system is does not move with a velocity and hasno change in the elevation
12
,,
)( UUWWQQ
UWQ
inoutoutin
outnetinnet
!=!!!
"=!
Energy Balance for a Cycle!a thermodynamics cycle is composed of processes that cause
the working fluid to undergoes a series of processes such that the
final and initial states are identical therefore the change in the
Closed system
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202202
inoutoutin
outnetinnet
outnetinnet
WWQQ
WQ
UWQ
!=
!
=
"=!
,,
,,
final and initial states are identical, therefore, the change in the
internal energy of the working fluid is zero for whole number of cycle,thus the energy balance becomes
0
Systematic Solution Method! Sketch the system and show energy interactionacrossthe boundary.
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203203
y
! Determine the property relation. Is the working substancean ideal gas or a real substance? Begin to set up and fill ina property table.
! Determine the process and sketch the process diagram.Continue to fill in the property table.
!Apply conservation of mass and conservation of energyprinciples.
! Bring in other information from the problem statement,called physical constraints, such as the volume doubles or
the pressure is halved during the process.! Develop enough equationsfor the unknowns and solve.
Key Thermodynamics PropertiesEnthalpy
!the combination of properties derived for the sake of
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204204
simplicity and convenience. The quantity hfgis called theenthalpy of vaporization (or latent heat of vaporization. Itrepresent the amount of energy needed to vaporize a unit
mass of saturated liquid at a given temperature or
pressure.
Pvuh
PVUH
+=
+=
EnthalpyKey Thermodynamics Properties
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205205
dPP
hdT
T
hdh
TP
!
"
#$
%
&
'
'+!
"
#$
%
&
'
'=
),( PThh =
Key Thermodynamics PropertiesInternal Energy
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206206
dvv
udTT
udu
Tv
!
"
#$
%
&
'
'+!
"
#$
%
&
'
'=
),( vTuu =
Key Thermodynamics PropertiesSpecific Heat
! it take different amounts of energyto raise the temperature of identical
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207207
! is defined as the energy requiredto raise the temperatureof a unit
mass of a substance by one degreeat maintained volume cVor
pressure cP
p
masses of different substances byone degree due to energy storage
capabilities of various substances!
! is specified by two independentintensive properties, thus it is
different at different temperature and
pressure
Specific HeatAt constant volume cv
= 0
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dvvudT
Tudu
Tv
!"#$
%&''+!
"#$
%&''=
v
v
T
uc !
"
#$%
&
'
'=
!is the change in internal energy
with temperature at constant volume
Specific HeatAt constant pressure cp
hh
= 0
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dPP
hdT
T
hdh
TP
!"#$
%& ''
+!"#$
%& ''
=
P
P
T
hc !
"
#$
%
&
'
'=
!is the change in enthalpy with
temperature at constant pressure
Specific Heat-Summary
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210
Internal EnergyForIdeal Gases
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211211
)(Tuu =(Shown in experiments performed by
Joule in 1843.)
EnthalpyForIdeal Gases
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212212
( ) ( )( )Thh
RTTuTh
Pvuh
=
+=
+=
Specific HeatForIdeal Gasesfor constant volume cv
Tu =
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213213
( )dTTcdudT
du
T
uc
Tu
v
v
v
=
=!"#$
%& ''
=
=
Specific HeatForIdeal Gasesfor constant pressure cp
=
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214214
( )dTTcdhdT
dh
T
hc
Th
P
v
P
=
=!"#$
%&''=
=
Internal Energy and EnthalpyFor Ideal Gases
==
2T
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215215
( ) ( )
( ) ( ) !
!="=#
=
"=
#2
1
1
12
12
T
T P
T v
dTcThThh
dTcTuTuu
Specific Heat forIdeal Gas
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Internal Energy and EnthalpyFor Ideal Gases
( )12,12TTcuu avev !=!
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( )
( )12,12
12,12
TTchh avep
avev
!=!
Internal Energy and EnthalpyFor Ideal Gases
THREEmethods to determine the internal energy andenthalpy changesof ideal gases
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218
py g g
( )( )
12,12
12,12
TTchhh
TTcuuu
avep
avev
!=!="
!=!="
( ) ( )( ) ( ) !
!="=#
=
"=
#2
1
2
1
12
12
T
T p
T
T v
dTcThThh
dTcTuTuu
12
12
hhh
uuu
!="
!=
"! using property table
!using the temperaturefunction and performing
integration (Table A-2c)
! using average specificheat (Table A-2b)
Specific Heat RelationsofIdeal Gases
RTuh +=
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219219
Rcc
RdTdTcdTc
RdTdudh
vP
vP
+=
+=
+=
v
P
c
ck =Specific Heat
Ratio
Specific Heats
forSolids and Liquids
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cccvp
==
Internal Energy ChangesforSolids and Liquids
=
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( ) ( )
( )
( )12
2
1
12
TTcu
dTTcuuu
dTTcdTcduTuu
ave
v
!"#
=!=#
==
=
$
Enthalpy Changes
forSolids
Pvuh +=
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Tcuh
vdPTcvdPuh
vdPduPdvvdPdudh
ave
ave
!"!=!
+!"+!=!
+=++=
= 0 for incompressible
= 0 for solid
Enthalpy Changes
forLiquids constant pressure processPvuh +=
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vdPTcvdPuh
vdPduPdvvdPdudh
ave +!"+!=!
+=++=
Pconstant, heater
0=!P Tcuhave!"!=!
= 0
Enthalpy Changes
forLiquids constant temperature process
vdPTcvdPuh +!"+!=!
= 0
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avTconstant, pump
0=!T
( )1212 PPvhh
Pvh
!=!
"="
( )satTfTfTP
TfTP
PPvhh
hh
!+"
"
###
##
,
,
By taking state 2 to be compressed liquid at given P and T andstate 1 to be saturated liquid at the same T
Universiti Kuala Lumpur
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Mass and Energy Analysis of Control VolumesChapter 5
!"#$%&'()*%+,-
to accompanyThermodynamics: An Engineering Approach, 6th edition
by Yunus A. engel and Michael A. Boles
Outline! Develop the conservation of mass principle! Apply the conservation of mass principle to
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