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ME 475/675 Introduction to
Combustion
Lecture 2
Announcement
• On Friday I will modify HW 1, which will be due on Monday
Ideal Stoichiometric Hydrocarbon Combustion
air
• CxHy + a(O2+3.76N2) οƒ  (x)CO2 + (y/2) H2O + 3.76a N2
• a = number of oxygen molecules per fuel molecule,
• Number of air molecules per fuel molecule is a(1+3.76)
𝑁𝑂2
𝑁𝐹𝑒𝑒𝑙
• If a = aST = x + y/4, then the reaction is Stoichiometric
• No O2 or Fuel in products
• This mixture produces nearly the hottest flame temperature
• If a < x + y/4, then reaction is fuel-rich (oxygen-lean, fuel left over)
• If a > x + y/4, then reaction is fuel-lean (oxygen-rich, O2 left over)
• Equivalence Ratio
• Φ=
π‘Žπ‘†π‘‘
π‘Žπ΄π‘π‘‘π‘’π‘Žπ‘™
=
𝑁𝑂2
𝑁𝐹𝑒𝑒𝑙 𝑆𝑑
• Φ = 1 → Stiochiometric
• Φ > 1 → Fuel Rich
• Φ < 1 → Fuel Lean
𝑁𝑂2
𝑁𝐹𝑒𝑒𝑙 π΄π‘π‘‘π‘’π‘Žπ‘™
=
𝑁𝐹𝑒𝑒𝑙,π΄π‘π‘‘π‘’π‘Žπ‘™
𝑁𝑂2 ,𝑆𝑑
𝑁𝐹𝑒𝑒𝑙,𝑆𝑑
𝑁𝑂2 ,π΄π‘π‘‘π‘’π‘Žπ‘™
Air to fuel mass ratio [kg air/kg fuel] of reactants
•
•
𝐴
𝐹
=
π‘šπ΄π‘–π‘Ÿ
π‘šπΉπ‘’π‘’π‘™
𝐴
𝐹 𝑆𝑑
=
𝑁 𝑂2
π‘π΄π‘–π‘Ÿ π‘€π‘Šπ΄π‘–π‘Ÿ
=
=
𝑁𝐹𝑒𝑒𝑙 π‘€π‘ŠπΉπ‘’π‘’π‘™
𝑁𝐹𝑒𝑒𝑙
(1+3.76)π‘€π‘Šπ΄π‘–π‘Ÿ
π‘Ž 𝑆𝑑
π‘€π‘ŠπΉπ‘’π‘’π‘™
• Need to find molecular weights
π‘π΄π‘–π‘Ÿ
𝑁𝑂
2
π‘€π‘Šπ΄π‘–π‘Ÿ
π‘€π‘ŠπΉπ‘’π‘’π‘™
=
(1+3.76)π‘€π‘Šπ΄π‘–π‘Ÿ
π‘Ž
π‘€π‘ŠπΉπ‘’π‘’π‘™
Molecular Weight of a Pure Substance
x
x
x
• Only one type of molecule:
• AxByCz…
• Molecular Weight
• MW = x(AWA) + y(AWB) + z(AWC) + …
• AWi = atomic weights
• Inside front cover of book
• Examples
• π‘€π‘Šπ‘‚2 = 2(AW𝑂 ) = 2(15.9994) = 32.00
π‘˜π‘”
π‘˜π‘šπ‘œπ‘™
• π‘€π‘Šπ»2𝑂 = 2(AW𝐻 ) + (AW𝑂 ) = 2(1.00794) +
• π‘€π‘Šπ‘ƒπ‘Ÿπ‘œπ‘π‘Žπ‘›π‘’ = π‘€π‘ŠπΆ3 𝐻8 = 3 12.011 + 8
• See page 701 for fuels
π‘˜π‘”
(15.9994) = 18.02
π‘˜π‘šπ‘œπ‘™
π‘˜π‘”
1.00794 = 44.097
π‘˜π‘šπ‘œπ‘™
x xx
x
x
x
Mixtures containing n components
• Total number of moles in system
• π‘π‘‡π‘œπ‘‘π‘Žπ‘™ =
𝑛
𝑖=1 𝑁𝑖
• Mole Fraction of species i
• πœ’π‘– = 𝑁
𝑁𝑖
π‘‡π‘œπ‘‘π‘Žπ‘™
=
𝑁𝑖
𝑛
𝑖=1 𝑁𝑖
• Mixture Molar Weight: π‘€π‘Šπ‘€π‘–π‘₯ =
• π‘€π‘Šπ‘€π‘–π‘₯ =
• π‘€π‘Šπ‘€π‘–π‘₯ =
π‘šπ‘–
𝑁𝑖
π‘šπ‘–
𝑁𝑖
=
=
x
x xx
x
x
x
o o
o x
x
• 𝑁𝑖 = number of moles of species 𝑖
• 𝑖 = 1, 2, . . 𝑛
o
𝑁𝑖 π‘€π‘Šπ‘–
=
π‘π‘‡π‘œπ‘‘π‘Žπ‘™
π‘šπ‘‡π‘œπ‘‘π‘Žπ‘™
=
π‘šπ‘– /π‘€π‘Šπ‘–
π‘šπ‘‡π‘œπ‘‘π‘Žπ‘™
π‘π‘‡π‘œπ‘‘π‘Žπ‘™
πœ’π‘– π‘€π‘Šπ‘– (weighted average)
1
π‘Œπ‘– /π‘€π‘Šπ‘–
• Example
• π‘šπ‘– = 𝑁𝑖 π‘€π‘Šπ‘– = mass of species 𝑖
• Total Mass
• π‘š π‘‡π‘œπ‘‘π‘Žπ‘™ =
• π‘€π‘Šπ΄π‘–π‘Ÿ =
• = 0.21 ∗ 2 ∗ 15.9994 + 0.79 ∗ 2 ∗ 14.0067
π‘˜π‘”
• = 0.21 ∗ 32.00 + 0.79 ∗ 28.00 = 28.85
π‘˜π‘šπ‘œπ‘™π‘’
• Remember and/or write inside front cover of your book
𝑛
𝑖=1 π‘šπ‘–
• Mass Fraction of species i
• π‘Œπ‘– = π‘š
π‘šπ‘–
π‘‡π‘œπ‘‘π‘Žπ‘™
=
π‘šπ‘–
𝑛
𝑖=1 π‘šπ‘–
• Useful facts:
• 𝑛𝑖=1 πœ’π‘– = 𝑛𝑖=1 π‘Œπ‘– = 1
• but πœ’π‘– ≠ π‘Œπ‘–
πœ’π‘– π‘€π‘Šπ‘– = 0.21π‘€π‘Šπ‘‚2 + 0.79π‘€π‘Šπ‘2
• Relationship between πœ’π‘– and π‘Œπ‘–
• π‘Œπ‘– =
•
π‘šπ‘–
=
π‘šπ‘‡π‘œπ‘‘π‘Žπ‘™
π‘€π‘Š
πœ’π‘– = π‘Œπ‘– π‘€π‘Šπ‘€π‘–π‘₯
𝑖
𝑁𝑖 π‘€π‘Šπ‘–
π‘π‘‡π‘œπ‘‘π‘Žπ‘™ π‘€π‘Šπ‘€π‘–π‘₯
= πœ’π‘–
π‘€π‘Šπ‘–
π‘€π‘Šπ‘€π‘–π‘₯
Stoichiometric Air/Fuel Mass Ratio
• For Hydrocarbon fuel CxHy
•
𝐴
𝐹 𝑆𝑑
=
π‘Žπ‘†π‘‘ (1+3.76)π‘€π‘Šπ΄π‘–π‘Ÿ
π‘€π‘ŠπΉπ‘’π‘’π‘™
π‘˜π‘”
28.85
π‘˜π‘šπ‘œπ‘™π‘’
• π‘€π‘Šπ΄π‘–π‘Ÿ = πœ’π‘– π‘€π‘Šπ‘– =
• π‘€π‘ŠπΉπ‘’π‘’π‘™ = π‘€π‘ŠπΆπ‘₯𝐻𝑦 = π‘₯ 12.011 + 𝑦(1.00794)
• aSt = x + y/4
•
𝐴
𝐹 𝑆𝑑
=
𝑦
π‘˜π‘”
(4.76)28.85
4
π‘˜π‘šπ‘œπ‘™π‘’
π‘˜π‘”
π‘˜π‘”
12.011π‘˜π‘šπ‘œπ‘™π‘’ +𝑦(1.00794π‘˜π‘šπ‘œπ‘™π‘’)
π‘₯+
π‘₯
• For 𝐢π‘₯ 𝐻𝑦 , 10 <
𝐴
𝐹 𝑆𝑑
< 35
• Constraints on y/x later
1
π‘˜π‘”
π‘₯
π‘˜π‘šπ‘œπ‘™π‘’
1
π‘˜π‘”
1.00794
π‘₯
π‘˜π‘šπ‘œπ‘™π‘’
1.00794
=
136.24 1+
𝑦 π‘₯
4
11.92+ 𝑦 π‘₯
Equivalence Ratio Φ
•Φ=
π‘Žπ‘†π‘‘
π‘Žπ΄π‘π‘‘π‘’π‘Žπ‘™
=
π‘Žπ‘†π‘‘ (1+3.76)π‘€π‘Šπ΄π‘–π‘Ÿ
π‘€π‘ŠπΉπ‘’π‘’π‘™
π‘Žπ΄π‘π‘‘π‘’π‘Žπ‘™ (1+3.76)π‘€π‘Šπ΄π‘–π‘Ÿ
π‘€π‘ŠπΉπ‘’π‘’π‘™
𝐴
=
𝐴
𝐹 𝑆𝑑
𝐹 π΄π‘π‘‘π‘’π‘Žπ‘™
=
πΉπ΄π‘π‘‘π‘’π‘Žπ‘™ 𝐴𝑆𝑑
𝐹𝑆𝑑 π΄π΄π‘π‘‘π‘’π‘Žπ‘™
• Φ = 1 → Stiochiometric
• Φ > 1 → Fuel Rich
• Φ < 1 → Fuel Lean
𝑦
•π‘Ž=
π‘₯+ 4
Φ
• CxHy + a(O2+3.76N2)
•%
•%
100%
Φ
𝐹𝑆𝑑
π΄π΄π‘π‘‘π‘’π‘Žπ‘™
Stoichiometric Air (%SA)=
=
∗ 100%
πΉπ΄π‘π‘‘π‘’π‘Žπ‘™ 𝐴𝑆𝑑
1
Excess Oxygen (%EO) = (%SA)-100% =
− 1 100%
Φ
Example
• For extra credit, this problem may be clearly reworked and turned in at the
beginning of the next class period.
• Problem 2.11, Page 91: In a propane-fueled truck, 3 percent (by volume)
oxygen is measure in the exhaust stream of the running engine. Assuming
“complete” combustion without dissociation, determine the air-fuel ratio
(mass) supplied to the engine.
• Also find
• Equivalence Ratio: Φ
• % Stoichiometric air: %SA
• % Excess Oxygen: %EA
• ID: Are reactants Fuel Rich, Fuel Lean, or Stoichiometric?
• Work on the board
Thermodynamic Systems (reactors)
• Closed systems
1π‘Š2
• Rigid tanks, piston/cylinders
• 1 = Initial state; 2 = Final state
• Mass: π‘š1 = π‘š2 = π‘š
• Chemical composition changes
1𝑄2
m, E
• But atoms are conserved
• 1st Law
•
1𝑄2
− 1π‘Š2 = Δ𝐸 = π‘š(𝑒2 − 𝑒1 )
• 𝑒=𝑒+
•
1𝑄2
𝑣2
2
+ 𝑔𝑧
− 1π‘Š2 = π‘š 𝑒2 − 𝑒1 +
𝑣22
2
−
𝑣12
2
+ 𝑔 𝑧2 − 𝑧1
• How to find internal energy 𝑒 for mixtures, and change 𝑒2 − 𝑒1 when composition changes due
to reactions (not covered in Thermodynamics I)
Open Systems (control volume)
• Steady State, Steady Flow (SSSF)
Inlet i
• Fixed volume, no moving boundaries
Outlet o
• Properties are constant and uniform
• Inside CV (Dm=DE=0), and
π‘šπ‘– 𝑒 + 𝑃𝑣
𝑖
Dm=DE=0
π‘š0 𝑒 + 𝑃𝑣
• At ports (β„Ž = 𝑒 + 𝑃𝑣)
• One inlet and one outlet: π‘šπ‘– = π‘šπ‘œ = π‘š
• Atoms are conserved
• Energy: 𝑄𝐢𝑉 − π‘ŠπΆπ‘‰ = π‘š β„Žπ‘œ − β„Žπ‘– +
𝑄𝐢𝑉
π‘£π‘œ2
2
−
𝑣𝑖2
2
π‘ŠπΆπ‘‰
+ 𝑔 π‘§π‘œ − 𝑧𝑖
• Composition and temperature of inlet and outlet are not the same due to
reaction
• Need to find β„Žπ‘œ − β„Žπ‘– (not covered in Thermodynamics I)
π‘œ
Combustion Thermochemistry
• We use thermodynamics to evaluate the internal energy, enthalpy and entropy of
a systems at different states
• The difference in energy and enthalpy between the products and reactants is
used with the first law to predict the heat of combustion (energy released during
combustion, due to changes in chemical bonds) if the products are assumed to
be at the same temperature as the reactants
• The adiabatic flame temperature (product temperature assuming all reaction
heat release stays in the system) can be determined by assuming the products
have the same energy level as the reactants
• The steady state product composition for a reaction may be determined from
entropy considerations
• Need to find
• The internal energy, enthalpy and entropy of mixtures of gases, and
• How to account for effects of chemical bonds
• These are not covered in ME 311 Thermodynamics I, but we we’ll cover them now
Ideal Gas Equation of State
• 𝑃𝑉 = π‘π‘…π‘ˆ 𝑇
• Universal Gas Constant
• π‘…π‘ˆ = 8.315
π‘˜π½
π‘˜π‘šπ‘œπ‘™π‘’ 𝐾
= 8315
• Inside book front cover
• kJ = kN*m=
𝐽
π‘˜π‘šπ‘œπ‘™π‘’ 𝐾
kPa*m3
• 𝑃𝑉 = π‘šπ‘…π‘‡ = 𝑁 ∗ π‘€π‘Š (π‘…π‘ˆ /π‘€π‘Š)𝑇
• Specific Gas Constant
• R =π‘…π‘ˆ /π‘€π‘Š
• MW = Molecular Weight of that gas
• 𝑃𝑣 = 𝑅𝑇; 𝑣 =
• 𝑃 = πœŒπ‘…π‘‡
𝑉
π‘š
=
1
𝜌
• Number of molecules
• N*NAV
• Avogadro's Number, 𝑁𝐴𝑉
• 6.022 ∗
26 π‘šπ‘œπ‘™π‘’π‘π‘’π‘™π‘’π‘ 
10
π‘˜π‘šπ‘œπ‘™π‘’
π‘šπ‘œπ‘™π‘’π‘π‘’π‘™π‘’π‘ 
1023
π‘šπ‘œπ‘™π‘’
• 6.022 ∗
• Number of molecules in 12 kg of C12
Partial Pressure 𝑃𝑖 and volume fraction
mixture of pressure 𝑃 and volume V
• Each specie acts as if it was the only
component at the given V and T
• Specie 𝑖: 𝑃𝑖 𝑉 = 𝑁𝑖 𝑅𝑒 𝑇
• Mixture: 𝑃 𝑉 = 𝑁 𝑅𝑒 𝑇
𝑃𝑖
Ratio:
𝑃
𝑁𝑖
𝑁
•
= = πœ’π‘–
• 𝑃𝑖 = πœ’π‘– 𝑃
• 𝑃𝑖 = πœ’π‘– 𝑃 = 𝑃 πœ’π‘– = 𝑃
𝑉𝑖
𝑉
of a specie in a
• Volume Fraction
• Each specie acts as if it was the only
component at the given P and T
• Specie 𝑖:𝑃𝑉𝑖 = 𝑁𝑖 𝑅𝑒 𝑇
• Mixture: 𝑃 𝑉 = 𝑁 𝑅𝑒 𝑇
•
𝑉𝑖
Ratio:
𝑉
=
𝑁𝑖
𝑁
= πœ’π‘–
End 2015
Extensive and Intensive System Properties
• Intensive Properties
• Extensive thermodynamic properties
depend on System Size (extent)
• Examples
• Volume V [m3]
• Internal Energy E [kJ]
• Enthalpy H = E + PV [kJ]
• Test: cut system in half
• Denoted with CAPITAL letters
• Independent of system size
• Examples
• Per unit mass (lower case)
• v = V/m [m3/kg]
• u = U/m [kJ/kg]
• h = H/m [kJ/kg]
• Denoted using lower-case letters
• Exceptions
• Temperature T [°C, K]
• Pressure P [Pa]
• Molar Basis (use bar
)
• V = vm = N𝑣
• U = um = N𝑒
• H = hm = Nβ„Ž
• N number of moles in the system
• Useful because chemical equations deal
with the number of moles, not mass
Calorific Equations of State for a pure substance
• 𝑒 = 𝑒 𝑇, 𝑣 = 𝑒(𝑇) ≠ 𝑓𝑛(𝑣)
• β„Ž = β„Ž 𝑇, 𝑃 = β„Ž(𝑇) ≠ 𝑓𝑛(𝑃)
For ideal gases
• Differentials (small changes)
• 𝑑𝑒 =
πœ•π‘’
πœ•π‘‡ 𝑣
𝑑𝑇 +
πœ•π‘’
=
πœ•π‘£ 𝑇
0;
• For ideal gas
•
πœ•π‘’
πœ•π‘‡ 𝑣
πœ•π‘’
πœ•π‘£ 𝑇
• Specific Heat [kJ/kg C]
• Energy input to increase temperature of one
kg of a substance by 1°C at constant volume
or pressure
• How are 𝑐𝑣 𝑇 and 𝑐𝑃 𝑇 measured?
𝑑𝑣
𝑐𝑝
𝑐𝑣
T [K]
Q [joules]
w
Q
= 𝑐𝑣 𝑇
m, T
Q
m, T
• 𝑑𝑒 = 𝑐𝑣 𝑇 𝑑𝑇
• π‘‘β„Ž =
πœ•β„Ž
πœ•π‘‡ 𝑃
𝑑𝑇 +
• For ideal gas
•
πœ•β„Ž
=
πœ•π‘ƒ 𝑇
0;
πœ•β„Ž
πœ•π‘‡ 𝑃
• π‘‘β„Ž = 𝑐𝑃 𝑇 𝑑𝑇
πœ•β„Ž
πœ•π‘ƒ 𝑇
= 𝑐𝑃 𝑇
𝑑𝑃
V = constant
P = wg/A = constant
• Calculate 𝑐𝑝 π‘œπ‘Ÿ 𝑣 =
𝑄
π‘šΔ𝑇 𝑝 π‘œπ‘Ÿ 𝑣
• 𝑐𝑝 = 𝑐𝑝 ∗ π‘€π‘Š; 𝑐𝑣 = 𝑐𝑣 ∗ π‘€π‘Š
π‘˜π½
π‘˜π‘”πΎ
π‘˜π½
π‘˜π‘šπ‘œπ‘™ 𝐾
Molar Specific Heat Dependence on Temperature
• Monatomic molecules: Nearly independent of temperature
• Only translational kinetic energy
• Multi-Atomic molecules: Increase with temperature and number of molecules
• Also possess rotational and vibrational kinetic energy
Internal Energy and Enthalpy
• Once cp(T) and cv(T) are known, internal energy change can be
calculated by integration
• 𝑒 𝑇 = π‘’π‘Ÿπ‘’π‘“ +
• β„Ž 𝑇 = β„Žπ‘Ÿπ‘’π‘“ +
𝑇
𝑐
π‘‡π‘Ÿπ‘’π‘“ 𝑣
𝑇
𝑐
π‘‡π‘Ÿπ‘’π‘“ 𝑃
𝑇 𝑑𝑇
𝑇 𝑑𝑇
• Appendix A (pp. 687-699, bookmark)
• 𝑐𝑝 𝑇 : π‘‘π‘Žπ‘π‘™π‘’π‘  π‘Žπ‘›π‘‘ π‘π‘’π‘Ÿπ‘£π‘’ 𝑓𝑖𝑑𝑠
• Note 𝑐𝑣 = 𝑐𝑝 − 𝑅𝑒
• 𝑐𝑝 =𝑐𝑝 /π‘€π‘Š
Mixture Properties
• Enthalpy
• π»π‘šπ‘–π‘₯ = π‘šπ‘– β„Žπ‘– = π‘š π‘‡π‘œπ‘‘π‘Žπ‘™ β„Žπ‘šπ‘–π‘₯
• π’‰π’Žπ’Šπ’™ (𝑻) =
• π»π‘šπ‘–π‘₯ =
π‘š 𝑖 β„Žπ‘–
π‘šπ‘‡π‘œπ‘‘π‘Žπ‘™
=
π’€π’Š π’‰π’Š (𝑻)
𝑁𝑖 β„Žπ‘– = π‘π‘‡π‘œπ‘‘π‘Žπ‘™ β„Žπ‘šπ‘–π‘₯
• π’‰π’Žπ’Šπ’™ (𝑻) =
𝑁𝑖 β„Žπ‘–
π‘π‘‡π‘œπ‘‘π‘Žπ‘™
=
• Internal Energy
• π’–π’Žπ’Šπ’™ (𝑻) = π’€π’Š π’–π’Š (𝑻)
• π’–π’Žπ’Šπ’™ 𝑻 = πŒπ’Š π’–π’Š 𝑻
πŒπ’Š π’‰π’Š (𝑻)
• Use these relations to calculate
mixture enthalpy and internal
energies (per mass or mole) as
functions of the properties of
the individual components and
their mass or molar fractions.
• u and h depend on temperature,
but not pressure
• Individual gas properties are on
pp. 687-699 as functions of gas
and T
Standardized Enthalpy and Enthalpy of Formation
• Needed for chemically-reacting systems because energy is required
to form and break chemical bonds
• Not considered in Thermodynamics I
• Needed to find 𝑒2 − 𝑒1 and β„Žπ‘œ − β„Žπ‘–
π‘œ
• β„Žπ‘– 𝑇 = β„Žπ‘“,𝑖
π‘‡π‘Ÿπ‘’π‘“ + Δβ„Žπ‘ ,𝑖 (𝑇)
• Standard Enthalpy at Temperature T =
• Enthalpy of formation at standard reference state: Tref and P°
• Sensible enthalpy change in going from Tref to T =
• Appendices A and B pp 687-702
𝑇
𝑐
π‘‡π‘Ÿπ‘’π‘“ 𝑃
+
𝑇 𝑑𝑇
Normally-Occurring Elemental Compounds
• For example:
• O2, N2, C, He, H2
π‘œ
• β„Žπ‘“,𝑖
π‘‡π‘Ÿπ‘’π‘“ = 0
• π‘‡π‘Ÿπ‘’π‘“ = 298K
• Use these as bases to tabulate the energy for form of more complex compounds
• Example:
• At 298K (1 mole) O2 + 498,390 kJ οƒ  (2 mole) O
• To form 2O atoms from one O2 molecule requires 498,390 kJ/kmol of energy
input to break O-O bond
•
•
π‘œ
β„Žπ‘“,𝑂
π‘œ
β„Žπ‘“,𝑖
π‘‡π‘Ÿπ‘’π‘“ =
498,390 kJ
2 π‘˜π‘šπ‘œπ‘™ 𝑂
=
π‘˜π½
249,195
π‘˜π‘šπ‘œπ‘™π‘‚
π‘‡π‘Ÿπ‘’π‘“ for other compounds are in Appendices A and B
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