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AEE465/565 – Rocket Propulsion – Professor Dr. Werner J.A. Dahm
Thrust Performance
Isentropic Nozzle Flow
Total-to-Static Relations:
Normal Shock Relations: (M = Mach before shock)
Thrust Equation:
𝑇 = π‘šΜ‡π‘ 𝑉𝑒 + (𝑝𝑒 − 𝑃∞ )𝐴𝑒
*First term is jet (momentum) thrust, the second term is
pressure thrust.
𝑇 = π‘šΜ‡π‘ π‘‰π‘’π‘ž
*Valid in all cases
Equivalent Velocity:
Total Relations:
2
𝑝𝑑 2
(𝛾 + 1) 𝑀
=[
]
(𝛾 − 1) 𝑀2 + 2
𝑝𝑑 1
πœŒπ‘‘
𝛾−1 2
= [1 +
𝑀 ]
𝜌
2
𝛾+1
]
2𝛾𝑀 2 − (𝛾 − 1)
𝛾
𝛾−1
𝑝2 2𝛾𝑀 2 − (𝛾 − 1)
=
𝑝1
𝛾+1
1
𝛾−1
𝑇2 [2𝛾𝑀 2 − (𝛾 − 1)][(𝛾 − 1)𝑀2 + 2]
=
(𝛾 + 1)2 𝑀2
𝑇1
Specific Impulse:
𝐼𝑠𝑝 =
𝑀22 =
1
𝛾+1 2
𝛾−1
2
)
π‘šΜ‡π‘ =
[𝛾 (
𝛾+1
√𝑅 𝑇𝑑
Thrust Coefficient:
𝑇
(𝑐𝑇 )π‘Žπ‘π‘‘π‘’π‘Žπ‘™ =
𝑝𝑑 𝐴∗
(𝛾 − 1)𝑀12 + 2
2𝛾𝑀12 − (𝛾 − 1)
𝛾+1
]
(𝑐𝑇 )π‘–π‘‘π‘’π‘Žπ‘™
]} +
(𝑝𝑒 − 𝑝∞ ) 𝐴𝑒
𝑝𝑑
𝐴∗
𝛾−1
𝛾
2
2 𝛾−1
𝑝𝑒
)(
) [1 − ( )
= 𝛾 {(
𝛾−1 𝛾+1
𝑝𝑑
1
2
]}
*Isentropic and fully expanded nozzle flow (𝑝𝑒 = 𝑝∞ )
1 𝛾+1
1
𝛾+1 2
(𝑐𝑇 )π‘–π‘‘π‘’π‘Žπ‘™ π‘£π‘Žπ‘π‘’π‘’π‘š
given Exit Mach number or solve numerically to
find Exit Mach from
1
2
𝛾+1
𝐴
1
2
𝛾 − 1 2 2 𝛾−1
) [1 +
= {(
𝑀 ]}
𝐴∗ 𝑀 𝛾 + 1
2
𝐴∗
𝛾−1
𝛾
Oblique Shock Jump Relations:
Isentropic Area-Mach Number Relation:
𝐴𝑒
(𝑐𝑇 )π‘–π‘ π‘’π‘›π‘‘π‘Ÿπ‘œπ‘π‘–π‘ =
2
2 𝛾−1
𝑝𝑒
)(
) [1 − ( )
𝛾 {(
𝛾−1 𝛾+1
𝑝𝑑
^This is valid for any choked nozzle.
*Find
π‘‰π‘’π‘ž
𝑇
=
𝑔0 π‘šΜ‡π‘ 𝑔0
*Equivalent time that 1 lbf of combustion products could
produce 1 lbf of thrust, units of seconds
(𝛾 + 1)𝑀2
𝜌2
=
𝜌1 (𝛾 − 1)𝑀 2 + 2
π‘šΜ‡(π‘₯) = π‘šΜ‡∗ = 𝜌∗ 𝑒∗𝐴∗
(𝑝𝑒 − 𝑝∞ ) 𝐴𝑒
𝑇
=
π‘šΜ‡π‘
π‘šΜ‡π‘
*Would be the exit velocity from a fully expanded nozzle
that produces same thrust as actual nozzle.
Shock Jump Relations:
Mass Flow Rate:
𝑝𝑑 𝐴∗
[
π‘‰π‘’π‘ž = 𝑉𝑒 +
1
𝛾−1
𝑇𝑑2
=1
𝑇𝑑1
𝑇𝑑
𝛾−1 2
= [1 +
𝑀 ]
𝑇
2
𝑝𝑑
𝛾−1 2
= [1 +
𝑀 ]
𝑝
2
𝛾
𝛾−1
2
2 𝛾−1
)(
) }
= 𝛾 {(
𝛾−1 𝛾+1
𝐴𝑒
𝐴∗
Angle-Mach Relations:
*Once 𝑀𝑒 is known, can solve or 𝑇𝑒 and 𝑝𝑒 using
isentropic relations (above).
Nozzle Choking Criterion:
𝛾
𝛾−1
𝑝𝑑
𝛾+1
)
=(
𝑝∗
2
𝑀22 sin2(πœƒ − 𝛿) =
π‘Žπ‘‘ 𝑀 ∗ = 1
Trajectories
Tsiolkovsky Rocket Equation (velocity increment):
𝑀0
Δπ‘‰π‘π‘’π‘Ÿπ‘› = π‘‰π‘’π‘ž ln ( ) − 𝑔0 𝑑𝑏
𝑀𝑓
(𝛾 − 1)𝑀12 sin2(πœƒ) + 2
2𝛾𝑀12 sin2(πœƒ) − (𝛾 − 1)
Total Relations:
𝛾
𝑝𝑑 2
*Unchoked if,
𝑝𝑑 1
𝛾
𝑝𝑑
𝛾 + 1 𝛾−1
)
<(
𝑝∗
2
Exit Velocity:
𝑉𝑒 = π‘Žπ‘’ 𝑀𝑒
*Fully expanded flow in a vacuum (infinite nozzle length)
(𝛾 + 1)𝑀12
cot(𝛿) = tan(πœƒ) [
− 1]
2(𝑀12 sin2(πœƒ) − 1)
=[
1
𝛾−1
(𝛾 + 1) 𝑀12 sin2 (πœƒ) 𝛾−1
𝛾+1
]
[
]
(𝛾 − 1) 𝑀12 sin2 (πœƒ) + 2
2𝛾𝑀12 sin2 (πœƒ) − (𝛾 − 1)
Shock Jump Relations:
𝑝2 2𝛾𝑀12 sin2(πœƒ) − (𝛾 − 1)
=
𝑝1
𝛾+1
π‘€β„Žπ‘’π‘Ÿπ‘’, π‘Žπ‘’ = √𝛾 𝑅 𝑇𝑒
𝛾−1
𝛾
2𝛾
𝑝𝑒
𝑉𝑒 = {
𝑅 𝑇 [1 − ( )
𝛾−1 𝑑
𝑝𝑑
𝑇2 [2𝛾𝑀12 sin2(πœƒ) − (𝛾 − 1)][(𝛾 − 1)𝑀12 sin2(πœƒ) + 2]
=
(𝛾 + 1)2 𝑀12 sin2(πœƒ)
𝑇1
1
2
]}
(𝛾 + 1)𝑀12 sin2(πœƒ)
𝜌2
=
𝜌1 (𝛾 − 1)𝑀12 sin2(πœƒ) + 2
Where,
π‘˜π½
(8314
)
𝑅̃
π‘šπ‘œπ‘™ βˆ™ 𝐾
=
π‘€π‘Š
π‘€π‘Š
*Therefore, lower π‘€π‘Š gives higher 𝑉𝑒 → higher thrust
𝑅=
Isentropic Model of Atmosphere:
Aerodynamic Drag:
1
𝐷 = πœŒπ‘‰ 2 𝐴𝐢𝐷
2
πœ‹
*Circular cross-section with diameter d has area 𝐴 = 𝑑 2
4
Gravitational Force:
𝑅𝑒 2
)
𝑔(𝑧) = 𝑔𝑒 (
𝑅𝑒 + 𝑧
*As a function of altitude 𝑧 in π‘š,
earth radius 𝑅𝑒 = 6378 (103 ) π‘š,
and acceleration of gravity at surface 𝑔𝑒 = 9.8 π‘š/𝑠 2
Time and Altitude at Burnout:
𝛾
𝑝(𝑧)
𝛾 − 1 𝑧 𝛾−1
( ∗ )]
≈ [1 −
𝑝𝑠
2
𝑧
*Where surface pressure, 𝑝𝑠 = 101.3 (103 )
Nozzle Expansion:
- Larger velocity increment due to high thrust for short
burn time than due to lower thrust for long burn time.
- Short burn at high thrust reduces energy consumed
lifting propellant (for vertical launch)
β„Žπ‘ = π‘‰π‘’π‘ž {1 −
𝑁
𝑀
*First term is dependent on Mass Ratio 𝑅 = ( 0 )
π‘š2
𝑀𝑓
∗
𝑧 = 8404 π‘š
𝑑𝑏 = (
Summerfeld Separation Criterion:
When nozzle flow is “highly” over expanded, when
ln(𝑅)
1
} 𝑑 − 𝑔 𝑑2
𝑅−1 𝑏 2 𝑒 𝑏
𝑀𝑃
)
π‘šΜ‡π‘
𝑑𝑏 = (𝑑 − 𝑑0 )
𝑝𝑒
𝑝∞
gets too small, flow in nozzle separates when,
𝑝𝑒
≲𝐾
𝑝∞
for 0.25 ≤ 𝐾 ≤ 0.4
*Boundary layer separation can cause highly turbulent
recirculating flow
Maximum Vehicle Altitude (vertical launch):
1 (Δ𝑉𝑏 )2
β„Žπ‘šπ‘Žπ‘₯ = β„Žπ‘ +
2 𝑔𝑒
β„Žπ‘šπ‘Žπ‘₯ =
π‘‰π‘’π‘ž2 (ln(𝑅))2
𝑅
− π‘‰π‘’π‘ž 𝑑𝑏 {
ln(𝑅) − 1}
2𝑔𝑒
𝑅−1
*Minimizing 𝑑𝑏 maximizes β„Žπ‘šπ‘Žπ‘₯
Rocket Staging
Staging Methods:
Velocity Increments for an Optimally Staged Rocket:
Δ𝑉 due to burnout of the 𝑖 th-stage,
(𝑉𝑏 )𝑖 = (π‘‰π‘’π‘ž ) ln(𝑅𝑖 ) − 𝑔0 (𝑑𝑏 )𝑖
𝑖
Final Δ𝑉 imparted on final payload 𝑀𝐿 of stage 𝑁,
𝑁
Circular Orbits: π‘Ÿ(πœƒ) = 𝑅 = π‘π‘œπ‘›π‘ π‘‘π‘Žπ‘›π‘‘, 𝑒 < 0, πœ€ = 0
Velocity:
πœ‡
𝑉=√
𝑅
Period:
𝑇𝑏 = ∑(𝑑𝑏 )𝑖
𝑅3
𝑇 = 2πœ‹√
πœ‡
𝑖=1
𝑁
1 + πœ†π‘–
(𝑉𝑏 )𝑁 = ∑ [(π‘‰π‘’π‘ž ) ln (
)] − π‘”π‘œ 𝑇𝑏
𝑖
πœ€π‘– + πœ†π‘–
𝑖=1
(Δ𝑉𝑏 )𝑁 = π‘‰π‘’π‘ž 𝑁 ln {πœ€ + (1 − πœ€) [
1 −1
𝑀𝐿 𝑁
𝑀0
] }
Escape from Circular Orbit:
πœ‡
Δ𝑉1 ≥ (√2 − 1)√
𝑅
− π‘”π‘œ 𝑇𝑏
Ideal Case (infinitely many stages):
(Δ𝑉𝑏 )𝑁→∞ = π‘‰π‘’π‘ž (1 − πœ€) ln [
*Equivalent Velocity π‘‰π‘’π‘ž
=
𝑇
π‘šΜ‡π‘
𝑀0
] − π‘”π‘œ 𝑇𝑏
𝑀𝐿
Parabolic Trajectories: (not orbit) 𝑒 = 0, π‘Ž = ∞, πœ€ = 1
𝑉∞ = 0
Escape Velocity:
2πœ‡
𝑉𝑒𝑠𝑐 = √
π‘Ÿ
≈ same for all stages
Escape from planet surface:
Orbital Dynamics
2πœ‡
𝑉𝑒𝑠𝑐 = √
π‘…π‘π‘™π‘Žπ‘›π‘’π‘‘
Gravitational Parameter:
𝑁 βˆ™ π‘š2
π‘€β„Žπ‘’π‘Ÿπ‘’ 𝐺 = 6.67 × 10−11
π‘˜π‘”
πœ‡ = 𝐺𝑀 ′
Radial Position (from vehicle to center of planet):
π‘Ž(1 − πœ€ 2 )
1 + πœ€ cos(πœƒ)
π‘Ÿ=
Semimajor Axis:
π‘Ž = π‘Ÿπ‘šπ‘–π‘›
1
1−πœ€
π‘Ž=
1
(π‘Ÿ + π‘Ÿπ‘ )
2 π‘Ž
Eccentricity:
πœ€=
π‘Ÿπ‘Ž − π‘Ÿπ‘
π‘Ÿπ‘Ž + π‘Ÿπ‘
πœ€ = √1 −
𝑏2
π‘Ž2
πœ€ =1−
π‘Ÿπ‘šπ‘–π‘›
π‘Ž
Circularization Burn:
Circularize at π‘Ÿπ‘Ž :
2π‘Ÿπ‘
πœ‡
Δ𝑉1 = √ βˆ™ [1 − √
]
π‘Ÿπ‘Ž
π‘Ÿπ‘Ž + π‘Ÿπ‘
Circularize at π‘Ÿπ‘ :
Vis-Viva:
Stage Mass Relation: 𝑁-stage vehicle, the 𝑖 th-stage has,
𝑀0𝑖 = 𝑀𝑃𝑖 + 𝑀𝑆𝑖 + 𝑀𝐿𝑖
Payload Ratio:
𝑀0(𝑖+1)
𝑀𝐿𝑖
𝑀𝐿𝑖
πœ†π‘– ≡
=
=
𝑀0𝑖 − 𝑀0(𝑖+1) 𝑀0𝑖 − 𝑀𝐿𝑖 𝑀𝑃𝑖 + 𝑀𝑆𝑖
*Equal for all similar stages, πœ†π‘– = πœ†(𝑖+1) = β‹― = πœ†π‘
πœ†π‘œπ‘π‘‘π‘–π‘šπ‘Žπ‘™ =
(𝑀𝐿⁄𝑀 )
2 1
𝑉 = πœ‡( − )
π‘Ÿ π‘Ž
2
0
1⁄
𝑁
Structural Coefficient:
𝑀𝑆𝑖
𝑀𝑆𝑖
𝑀𝑆𝑖
πœ€π‘– =
=
=
𝑀0𝑖 − 𝑀0(𝑖+1) 𝑀0𝑖 − 𝑀𝐿𝑖 𝑀𝑆𝑖 + 𝑀𝑃𝑖
*Equal for all similar stages, πœ€π‘– = πœ€(𝑖+1) = β‹― = πœ€π‘
𝑀0𝑖
𝑀0𝑖
1 + πœ†π‘–
=
=
𝑀0𝑖 − 𝑀𝑃𝑖 𝑀𝑆𝑖 + 𝑀𝐿𝑖 πœ€π‘– + πœ†π‘–
Inclination Change: (circular orbits)
π‘Ÿπ‘ = π‘Ž(1 − πœ€)
Perigee Velocity:
πœ‡ 1+πœ€
)
𝑉𝑝 = √ (
π‘Ž 1−πœ€
πœ‡ 2π‘Ÿπ‘Ž
𝑉𝑝 = √
π‘Ÿπ‘ (π‘Ÿπ‘Ž + π‘Ÿπ‘ )
1
*Both other angles are: πœ‹ − πœƒ
2
πœ‡
πœƒ
Δ𝑉1 = 2√ sin ( )
𝑅
2
Apogee Radius:
π‘Ÿπ‘Ž = π‘Ž(1 + πœ€)
Apogee Velocity:
πœ‡ 1−πœ€
)
π‘‰π‘Ž = √ (
π‘Ž 1+πœ€
2π‘Ÿπ‘
πœ‡
π‘‰π‘Ž = √
π‘Ÿπ‘Ž (π‘Ÿπ‘Ž + π‘Ÿπ‘ )
Orbital Period:
πœ‡ π‘Ÿπ‘Ž
π‘‰π‘Ž = √
π‘Ž π‘Ÿπ‘
Orbital Rendezvous:
Lead Angle:
𝛼𝐿 =
πœ‹ (𝑅1 + 𝑅2 )3
√
2
2(𝑅2)3
Transfer Time:
π‘Ž3
𝑇 = 2πœ‹√
πœ‡
Mass Ratio:
𝑅𝑖 =
πœ‡
2π‘Ÿπ‘Ž
Δ𝑉1 = √ βˆ™ [1 − √
]
π‘Ÿπ‘
π‘Ÿπ‘Ž + π‘Ÿπ‘
Perigee Radius:
1⁄
𝑁
𝑀
(1 − 𝐿⁄𝑀 )
0
Δ = −π‘Ž√πœ€ 2 − 1
Orbital Maneuvers
*Where b = semi-minor axis
πœ€ < 1 → 𝑒𝑙𝑙𝑖𝑝𝑠𝑒
πœ€ = 1 → π‘π‘Žπ‘Ÿπ‘Žπ‘π‘œπ‘™π‘Ž
πœ€ > 1 → β„Žπ‘¦π‘π‘’π‘Ÿπ‘π‘œπ‘™π‘Ž
πœ€ = 0 → π‘π‘–π‘Ÿπ‘π‘™π‘’
*For Parallel Staging: Mass of 1st stage propellant from
large tank is equal to the total mass of the large tank’s
propellant times the fraction of the 1st stage burn time
over the total burn time of the 1st and 2nd stages.
Hyperbolic Trajectories: (not orbit) 𝑒 > 0
Excess Velocity:
πœ‡
𝑉∞ = √2𝑒
𝑉∞ = √
−π‘Ž
Asymptote Angle:
1
πœƒ∞ = πœ‹ − cos −1 ( )
πœ€
Turning Angle:
1
𝛿 = 2 sin−1 ( )
πœ€
Miss Distance:
𝑇𝑇𝑋 = π‘‡π»π‘œβ„Žπ‘šπ‘Žπ‘›π‘› =
πœ‹ (𝑅1 + 𝑅2 )3
√
2
2πœ‡
Intercept Opportunity Times:
Energy (per unit mass):
𝑒=−
πœ‡
2π‘Ž
1
1
1
=
−
𝑇 (𝑇𝐢 )1 (𝑇𝐢 )2
𝑅𝑖
π‘€β„Žπ‘’π‘Ÿπ‘’ (𝑇𝐢 )𝑖 = 2πœ‹√
πœ‡
Orbital Transfers
Standard Gravitation Parameters
Hohmann Transfer:
Combustion Tap-Off Systems:
3
Circular Orbit Velocities:
πœ‡
(𝑉𝐢 )1 = √
𝑅1
πœ‡
(𝑉𝐢 )2 = √
𝑅2
Transfer Orbit Parameters: (Trans time, see Rendezvous)
π‘Ÿπ‘ = 𝑅1
π‘Ÿπ‘Ž = 𝑅2
πœ‡ 2𝑅2
𝑉𝑝 = √
𝑅1 𝑅1 + 𝑅2
Body
π‘š
πœ‡ = 𝐺𝑀 ′ [ 2 ]
𝑠
Sun
1.327 × 1020
Mercury
2.203 × 1013
Venus
3.249 × 1014
Earth
3.986 × 1014
(Moon)
4.903 × 1012
Mars
4.283 × 1013
Jupiter
1.267 × 1017
Saturn
3.793 × 1016
Uranus
5.794 × 1015
Neptune
Pluto
6.837 × 1015
1.108 × 1012
Propellant Feed Systems
Pressure-Fed Systems:
πœ‡ 2𝑅1
π‘‰π‘Ž = √
𝑅2 𝑅1 + 𝑅2
Velocity Increments:
*Uses combustion product gas from combustion chamber
to drive gas turbine that then drives pumps.
Open Systems:
- Turbine exit gas pressure low, dumped overboard
Closed Systems:
- Turbine exit gas dumped into nozzle at low pressure
location to add π‘šΜ‡π‘ at nozzle exit
*Moderate/high thrust (Saturn I-B/Blue Origin)
Gas Generator Systems:
πœ‡
2𝑅2
Δ𝑉1 = √ [√
− 1]
𝑅1
𝑅1 + 𝑅2
πœ‡
2𝑅1
Δ𝑉2 = √ [1 − √
]
𝑅2
𝑅1 + 𝑅2
Bielliptic Transfer:
Deliver Pressure > Tank Pressure,
π‘ƒβ„Ž = 𝜌(𝑔 + π‘Ž)β„Ž
Circular Orbit Velocities:
πœ‡
(𝑉𝐢 )1 = √
𝑅1
πœ‡
(𝑉𝐢 )2 = √
𝑅2
Transfer Orbit Parameters: (𝑅𝑇𝑋 can be chosen)
𝑅1 = 𝑅𝑝𝑇𝑋1
*Part of fuel and oxidizer are burned in preburner to
produce high-pressure gas that drives turbopumps.
- Preburner operated very fuel-rich to keep
temperature sufficiently low
- Fuel-rich exhaust dumped overboard (open) or
dumped into nozzle (closed)
- Power controlled by adjusting fuel/ox rates into
preburner
- Can achieve higher CC pressure than expander sys.
Staged Combustion Systems:
𝑅𝑇𝑋 = π‘…π‘Žπ‘‡π‘‹1
𝑅2 = 𝑅𝑝𝑇𝑋2
𝑅𝑇𝑋 = π‘…π‘Žπ‘‡π‘‹2
1
π‘Ž 𝑇𝑋1 = (𝑅1 + 𝑅𝑇𝑋 )
2
1
π‘Ž 𝑇𝑋2 = (𝑅2 + 𝑅𝑇𝑋 )
2
Expander Systems:
Transit Time:
𝑇𝑇𝑋 = πœ‹
√(π‘Ž 𝑇𝑋1 )3 + √(π‘Ž 𝑇𝑋2)3
√πœ‡
Velocity Increments:
2
1
πœ‡
)−√
Δ𝑉1 = √πœ‡ ( −
𝑅1 π‘Ž 𝑇𝑋1
𝑅1
2
1
2
1
) − √πœ‡ (
)
Δ𝑉2 = √πœ‡ (
−
−
𝑅𝑇𝑋 π‘Ž 𝑇𝑋2
𝑅𝑇𝑋 π‘Ž 𝑇𝑋1
πœ‡
2
1
)
Δ𝑉3 = √ − √πœ‡ ( −
𝑅2
𝑅2 π‘Ž 𝑇𝑋2
*Fuel is expanded to gaseous form to drive turbine that
powers pumps which then push propellant into CC.
- Low/moderate thrust applications
- Often used for upper stage engines
*All propellant is burned in two stages (nothing wasted).
First in fuel-rich preburner, then in main CC.
- Allows very high CC pressures (high thrust)
- Can be used with any liquid propellants
- More efficient than gas generator (all fuel burned)
- Requires very high-pressure turbopumps
Propellants and Aerothermochemistry
Propellant Types:
Hydrocarbon Combustion:
Turbines:
Liquid Propellants:
Fuels:
a) Cryogenic
- LH2 – liquid hydrogen (20 K) “deep cryogen”
- LCH4 – liquid methane (111 K)
b) Non-cryogenic
- RP-1 – kerosene [𝐢1 𝐻1.96 ]
- ethyl alcohol – [𝐢2 𝐻5 𝑂𝐻]
c) Hypergolic (πΈπ‘Ž ≤ 0) (reacts on contact with oxi.)
- hydrazine [𝑁2 𝐻4 ]
- monomethyl hydrazine (MMH)
- unsymmetrical dimethyl hydrazine (UDMH)
Oxidizers:
a) Cryogenic
- LOX – liquid oxygen
- LF2 – liquid fluorine
- FLOX – fluorine-enhanced LOX
- N2O4 – dinitrogen tetroxide
b) Non-cryogenic
- N2O – nitrous oxide
- N2O4 – dinitrogen tetroxide
- ClF5 – chlorine pentafluoride
Overall Stoichiometric Reaction:
π‘š
π‘š
1 𝐢𝑛 π»π‘š + (𝑛 + ) 𝑂2 → 𝑛𝐢𝑂2 + 𝐻2 𝑂
4
2
𝑛 = π‘π‘Žπ‘Ÿπ‘π‘œπ‘› π‘Žπ‘‘π‘œπ‘šπ‘ , π‘š = β„Žπ‘¦π‘‘π‘Ÿπ‘œπ‘”π‘’π‘› π‘Žπ‘‘π‘œπ‘šπ‘ 
Application of 1st Law:
(Δβ„Žπ‘‘ )1,2 = π‘ž1,2 − 𝑀1,2 = 0
Monopropellants:
* Both fuel and oxidizer are contained in the same
molecule; contact with a catalyst bed initiates reaction
(breaks oxidizer and fuel components apart).
* Usually used for RCS and in-space propulsion at low-mid
thrust applications.
- hydrazine (N2H4) + granular Al w/iridium coating
- hydrogen peroxide (H2O2) + many possible catalysts
- nitromethane (CH3NO2)
- ethylene oxide (C2H4O)
- nitrous oxide (N2O)
- hydroxylammonium nitrate (HAN) (H4N2O4)
Solid Propellants:
* Both fuel and oxidizer are initially in solid form.
Homogenous Propellants:
* Fuel and oxidizer are contained in the same
molecule or in a homogeneous mixture.
- nitroglycerine + nitrocellulose
C3H5(NO2)3 + C6H7O2(NO2)3
- Single/Double/Triple base propellants
Metal powders often added to increase heat of
combustion.
Heterogeneous (composite) Propellants:
* Heterogeneous mixture of oxidizing crystals held in
an organic plastic-like fuel “binder”
a) Fuel Component (common binders)
- hydroxyl-terminated polybutadiene (HTPB)
- rubber/asphalt
b) Oxidizer Component (ground crystals of one or
more of the following)
- ammonium perchlorate (AP)
- ammonium nitrate (AN)
- nitronium perchlorate (NP)
- potassium perchlorate (KP)
- potassium nitrate (PN)
- cyclotrimethylene trinitomine (RDX)
- cyclotetramethylene tetranitramine (HMX)
* The combination of fuel/ox specifies the propellant
(e.g. AP-HTPB, KP-HTPB, …)
Many possible combinations.
→ β„Žπ‘‘2 − β„Žπ‘‘1 = 0
→ 𝐢𝑝 (𝑇𝑑2 − 𝑇𝑑1 ) = 0
Mixture Ratio:
𝑀𝑂
π‘Ÿ = ( 2)
𝑀𝑓
∴ 𝑇𝑑2 = 𝑇𝑑1
Turbine Work:
Stoichiometric Mixture Ratio:
32𝑛 + 8π‘š
π‘Ÿπ‘  =
12𝑛 + π‘š
Equivalence Ratio:
π‘Ÿπ‘ 
πœ‘=
π‘Ÿ
πœ‘ = 1 → π‘ π‘‘π‘œπ‘–π‘β„Žπ‘–π‘œπ‘šπ‘’π‘‘π‘Ÿπ‘–π‘ π‘π‘œπ‘šπ‘π‘’π‘ π‘‘π‘–π‘œπ‘›
πœ‘ > 1 → 𝑓𝑒𝑒𝑙 − π‘Ÿπ‘–π‘β„Ž π‘π‘œπ‘šπ‘π‘’π‘ π‘‘π‘–π‘œπ‘›
πœ‘ < 1 → 𝑓𝑒𝑒𝑙 − π‘™π‘’π‘Žπ‘› π‘π‘œπ‘šπ‘π‘’π‘ π‘‘π‘–π‘œπ‘›
Molar Enthalpy of Combustion:
Δβ„ŽΜƒπΆ = [∑ π΅π‘œπ‘›π‘‘ πΈπ‘›π‘’π‘Ÿπ‘”π‘¦ ]
𝑖
− [∑ π΅π‘œπ‘›π‘‘ πΈπ‘›π‘’π‘Ÿπ‘”π‘¦ ]
π‘Ÿπ‘’π‘Žπ‘π‘‘
𝑖
π‘π‘Ÿπ‘œπ‘‘
Δβ„ŽΜƒπΆ < 0 → 𝑒π‘₯π‘œπ‘‘β„Žπ‘’π‘Ÿπ‘šπ‘–π‘
Δβ„ŽΜƒπΆ > 0 → π‘’π‘›π‘‘π‘œπ‘‘β„Žπ‘’π‘Ÿπ‘šπ‘–π‘
Convert to mass-specific enthalpy:
Δβ„ŽΜƒπΆ
Δβ„ŽπΆ =
π‘€π‘Šπ»πΆ
π‘€π‘Šπ»πΆ = 12𝑛 + 1π‘š [
π‘˜π‘π‘Žπ‘™
]
𝑔
Convert to [π‘˜π½⁄π‘˜π‘”]:
Δβ„ŽπΆ [
π‘˜π‘π‘Žπ‘™
1000 π‘π‘Žπ‘™ 1000𝑔 4.1814 𝐽
1 π‘˜π½
)(
)(
)(
)
]βˆ™(
𝑔
π‘˜π‘π‘Žπ‘™
π‘˜π‘”
π‘π‘Žπ‘™
1000𝐽
Turbopumps and Turbines
Turbopumps:
Shaft Power from Turbine:
π‘ŠΜ‡ = 𝜏 βˆ™ ΩΜ‡
Ideal Pump Work:
|𝑀|π‘–π‘‘π‘’π‘Žπ‘™ =
1
|π‘Š|π‘›π‘œπ‘›π‘–π‘‘π‘’π‘Žπ‘™ = πœ‚ 𝑇 Δ𝑝𝑑
𝜌
Temperature Change Across Turbine:
Δ𝑝𝑑
Δ𝑇 = (1 − πœ‚ 𝑇 )
𝜌 βˆ™ 𝑐𝑉
Turbine Work: (per unit mass)
|𝑀𝑇 | = |𝐢𝑃 (𝑇𝑑𝑒 − 𝑇𝑑𝑖 )|
Turbine Power:
π‘ŠΜ‡π‘‡ = π‘šΜ‡|𝑀𝑇 |
Turbine Stage Efficiency:
|𝑀|
πœ‚π‘† =
|𝑀|𝑆
Total Turbine Efficiency:
𝑇
1 − ( 𝑑3 )
𝑇𝑑1
πœ‚π‘‡ =
𝛾−1
𝑝𝑑3 𝛾
1−( )
𝑝𝑑1
Turbine Total Temperature Ratio:
1
(𝑝 − 𝑝𝑑1 )
𝜌 𝑑2
Ideal Pump Power:
1
|𝑀̇ |π‘–π‘‘π‘’π‘Žπ‘™ = π‘šΜ‡|𝑀|π‘–π‘‘π‘’π‘Žπ‘™ = π‘šΜ‡ (𝑝𝑑2 − 𝑝𝑑1 )
𝜌
Pump Efficiency:
|𝑀|π‘–π‘‘π‘’π‘Žπ‘™
|𝑀̇ |π‘–π‘‘π‘’π‘Žπ‘™
πœ‚π‘ƒ =
=
|𝑀|π‘Žπ‘π‘‘π‘’π‘Žπ‘™ |𝑀̇ |π‘Žπ‘π‘‘π‘’π‘Žπ‘™
Non-Ideal Pump Work:
11
(𝑝 − 𝑝𝑑1 )
|𝑀|π‘Žπ‘π‘‘π‘’π‘Žπ‘™ =
πœ‚π‘ƒ 𝜌 𝑑2
Non-Ideal Pump Power:
1 1
(𝑝 − 𝑝𝑑1 )
|𝑀̇ |π‘Žπ‘π‘‘π‘’π‘Žπ‘™ = π‘šΜ‡|𝑀|π‘Žπ‘π‘‘π‘’π‘Žπ‘™ = π‘šΜ‡
πœ‚π‘ƒ 𝜌 𝑑2
*π‘“π‘Ÿπ‘œπ‘š π‘‘β„Žπ‘’ π‘Žπ‘π‘œπ‘£π‘’
𝜌
Δ𝑝𝑑 = (𝑝𝑑2 − 𝑝𝑑1 ) = 𝑀𝑃 πœ‚π‘ƒ
π‘šΜ‡
1st Law for Liquid Flow Through Pump:
1
1
𝑐𝑉 = (𝑇2 − 𝑇1 ) + (𝑝2 − 𝑝1 ) + (𝑉22 − 𝑉12 ) = |𝑀|
𝜌
2
1
𝑐𝑉 = (𝑇2 − 𝑇1 ) + (𝑝𝑑2 − 𝑝𝑑1 ) = |𝑀|
𝜌
Temperature Change Across Pump:
1 − πœ‚π‘ƒ (𝑝𝑑2 − 𝑝𝑑1 )
(𝑇2 − 𝑇1 ) = (
)
πœ‚π‘ƒ
𝜌 βˆ™ 𝑐𝑉
𝛾−1
𝛾
𝑇𝑑3
𝑝𝑑3
= 1 − πœ‚ 𝑇 [1 − ( )
𝑇𝑑1
𝑝𝑑1
]
Turbine Total Pressure Ratio:
𝛾
𝑝𝑑3
1
𝑇𝑑3 𝛾−1
= [1 − (1 − )]
𝑝𝑑1
πœ‚π‘‡
𝑇𝑑1
Total-to-Static Temperature Relation:
𝛾 − 1 2 −1
𝑇3 = 𝑇𝑑3 [1 +
𝑀3 ]
2
Total-to-Static Pressure Relation:
𝛾
𝛾 − 1 2 −𝛾−1
𝑀3 ]
2
Entropy Change Across Turbine:
𝑇𝑑3
𝑝𝑑3
Δ𝑠 = 𝑠3 − 𝑠1 = 𝐢𝑝 ln ( ) − 𝑅 ln ( )
𝑇𝑑1
𝑝𝑑1
𝛾−1
)
𝑅 = 𝐢𝑝 (
𝛾
𝑅 = 𝐢𝑣 (𝛾 − 1)
Temperature-Velocity Relation:
𝑉2
(𝑇𝑑 − 𝑇) =
2 βˆ™ 𝐢𝑝
𝑝3 = 𝑝𝑑3 [1 +
Nozzle Design
Simple Conical Nozzles:
Axial Thrust:
1 + cos(𝛼)
π‘šΜ‡π‘ 𝑉𝑒 + (𝑝𝑒 − 𝑝∞ )𝐴𝑒
2
*See notes for Rao and TOP nozzle stuff
π‘‡π‘Žπ‘₯π‘–π‘Žπ‘™ =
Combustion Chamber Performance
DOF and Molecular Energy
Non-Isentropic Nozzle Flow
(𝐷𝑂𝐹)π‘Ÿπ‘œπ‘‘ = 0
Application of 1st Law:
(Δβ„Žπ‘‘ )2,𝑒 = π‘ž2,𝑒 − 𝑀2,𝑒 = 0
→ β„Žπ‘‘2 − β„Žπ‘‘π‘’ = 0
→ 𝐢𝑝 (𝑇𝑑2 − 𝑇𝑑𝑒 ) = 0
∴ 𝑇𝑑2 = 𝑇𝑑𝑒
→ (𝐷𝑂𝐹)π‘Žπ‘£π‘Žπ‘–π‘™ = 3
Temperature-Velocity Relation:
Monatomic Molecules:
(𝐷𝑂𝐹)π‘‘π‘Ÿπ‘Žπ‘›π‘  = 3
Combustion Chambers:
(𝐷𝑂𝐹)𝑣𝑖𝑏 = 0
Diatomic Molecules:
(𝐷𝑂𝐹)π‘‘π‘Ÿπ‘Žπ‘›π‘  = 3
(𝑇𝑑 − 𝑇) =
Total Pressure Ratio:
Δ𝑠
𝑝𝑑𝑒
= 𝑒− 𝑅
𝑝𝑑2
*where, 𝑝𝑑𝑒 < 𝑝𝑑2 and Δ𝑠 > 0
(𝐷𝑂𝐹)𝑣𝑖𝑏 = 2
(𝐷𝑂𝐹)π‘Ÿπ‘œπ‘‘ = 2
→ (𝐷𝑂𝐹)π‘Žπ‘£π‘Žπ‘–π‘™ = 7
Total-to-Static Pressure Ratio:
Nozzle Efficiency:
2(3𝑛 − 5) 𝑖𝑓 π‘™π‘–π‘›π‘’π‘Žπ‘Ÿ
(𝐷𝑂𝐹)π‘Ÿπ‘œπ‘‘ = {
2(3𝑛 − 6) 𝑖𝑓 π‘›π‘œπ‘›π‘™π‘–π‘›π‘’π‘Žπ‘Ÿ
5 + 2(3𝑛 − 5) 𝑖𝑓 π‘™π‘–π‘›π‘’π‘Žπ‘Ÿ
→ (𝐷𝑂𝐹)π‘Žπ‘£π‘Žπ‘–π‘™ = {
6 + 2(3𝑛 − 6) 𝑖𝑓 π‘›π‘œπ‘›π‘™π‘–π‘›π‘’π‘Žπ‘Ÿ
Thrust Coefficient:
𝑇
𝐢𝑇 =
𝑝𝑑2 βˆ™ 𝐴∗
Thrust:
𝑝𝑑2 βˆ™ 𝐴∗
) 𝐢𝑇
𝑇 = π‘šΜ‡π‘ (
π‘šΜ‡π‘
C* “Characteristic Velocity”:
𝑝𝑑2 βˆ™ 𝐴∗
𝐢∗ =
π‘šΜ‡π‘
1
𝛾+1 2
∗
πΆπ‘–π‘‘π‘’π‘Žπ‘™
𝑝𝑑2
2 𝛾−1
) ]
=
√𝑅𝑇𝑑2 [𝛾 (
𝑝𝑑1
𝛾+1
C* Efficiency:
πœ‚πΆ ∗ =
∗
πΆπ‘Žπ‘π‘‘π‘’π‘Žπ‘™
∗
πΆπ‘–π‘‘π‘’π‘Žπ‘™
Specific Heat and Gas Constant Relations:
Specific Heat - Constant Volume:
Specific Impulse:
𝐼𝑆𝑃
Energy Stored in One Molecule:
1
𝑒 ′ = π‘˜π‘‡(𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’
2
𝑅̃
8.314 𝐽⁄π‘šπ‘œπ‘™ βˆ™ 𝐾
(π΅π‘œπ‘™π‘‘π‘§π‘šπ‘Žπ‘›π‘› πΆπ‘œπ‘›π‘ π‘‘π‘Žπ‘›π‘‘)
π‘˜=
=
𝐴𝑣 6.022 × 1023 π‘π‘Žπ‘Ÿπ‘‘
π‘šπ‘œπ‘™
1
𝑒̃ = 𝐴𝑣 βˆ™ 𝑒 ′ = 𝑅̃𝑇 βˆ™ (𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’ (π‘π‘’π‘Ÿ π‘šπ‘œπ‘™π‘’)
2
1
𝑒 = 𝑒̃ ⁄π‘€π‘Š = 𝑅𝑇 βˆ™ (𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’ (π‘π‘’π‘Ÿ π‘šπ‘Žπ‘ π‘ )
2
*(𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’ depends on temperature
- Low T = only trans. active
- Med T = trans. and rot. active
- High T = trans., rot., and vib. are active
1
= 𝐢 ∗ 𝐢𝑇
𝑔
Pressure Ratio:
𝑝2 (1 + 𝛾𝑀12 )
=
𝑝1 (1 + 𝛾𝑀22 )
Temperature Ratio:
𝑇2
1 + 𝛾𝑀12
𝑀2 2
)
=[
2] βˆ™ (
𝑇1
1 + 𝛾𝑀2
𝑀1
Total Temperature Ratio:
𝛾−1 2
2
1+
𝑀2
𝑇𝑑2
1 + 𝛾𝑀12
𝑀2 2
2
)
( )
=[
]βˆ™(
2
𝛾−1 2
𝑇𝑑1
1
+
𝛾𝑀
𝑀1
2
1+
𝑀1
2
𝑇𝑑2
π‘ž1,2
=
+1
𝑇𝑑1 𝐢𝑝 𝑇𝑑1
Total Pressure Ratio:
𝛾
𝛾 − 1 2 𝛾−1
1+
𝑀2
𝑝𝑑2
1 + 𝛾𝑀12
2
)
=[
]
βˆ™(
𝛾
−
1
𝑝𝑑1
1 + 𝛾𝑀22
1+
𝑀12
2
Combustion Chamber-to-Throat Area Ratio:
1𝛾+1
𝐴𝐢
1
2
𝛾 − 1 2 2𝛾−1
{(
) [1 +
=
𝑀2 ]}
𝐴∗ 𝑀2 𝛾 + 1
2
Thermal Choking Criterion:
(1 + 𝛾𝑀12 )2
𝑇𝑑2
1
≥
𝑇𝑑1 2(1 + 𝛾) [1 + 𝛾 − 1 𝑀 2 ] 𝑀 2
1
1
2
*subtract 1 from result to get max allowable 𝑇𝑑2
1
𝐢̃𝑉 = 𝑅̃ (𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’
2
1
𝐢𝑉 = 𝑅 (𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’
2
Specific Heat - Constant Pressure:
1
𝐢̃𝑃 = 𝑅̃ [1 + (𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’ ]
2
1
𝐢𝑃 = 𝑅 [1 + (𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’ ]
2
Gas Constant Relations:
𝑅 = 𝐢𝑃 − 𝐢𝑉
𝑅̃ = 𝐢̃𝑃 − 𝐢̃𝑉
*given 𝐢𝑃 and 𝛾
𝑅 = 𝐢𝑃 (1 −
𝐢𝑉
1
𝛾−1
) = 𝐢𝑃 (1 − ) = 𝐢𝑃 (
)
𝐢𝑃
𝛾
𝛾
*given 𝐢𝑉 and 𝛾
𝐢𝑃
𝑅 = 𝐢𝑃 − 𝐢𝑣 = 𝐢𝑉 ( − 1) = 𝐢𝑉 (𝛾 − 1)
𝐢𝑉
Specific Heat Ratio:
2
𝛾 =1+
(𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’
Monatomic:
(𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’ = 3 (independent of temp.)
2
→𝛾 =1+
= 1.667
(3)
Diatomic:
- Medium temp
2
(𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’ = 5 → 𝛾 = 1 +
= 1.4
(5)
- High temp
2
(𝐷𝑂𝐹)π‘Žπ‘π‘‘π‘–π‘£π‘’ = 7 → 𝛾 = 1 +
= 1.286
(7)
𝛾
𝛾−1
(𝛾 − 1)𝑀𝑒2
𝑝𝑒
1
= {1 − [
]}
𝑝𝑑2
πœ‚π‘ 2 + (𝛾 − 1)𝑀𝑒2
Polyatomic Molecules:
(𝐷𝑂𝐹)π‘‘π‘Ÿπ‘Žπ‘›π‘  = 3
2 𝑖𝑓 π‘™π‘–π‘›π‘’π‘Žπ‘Ÿ (𝐢𝑂2 )
(𝐷𝑂𝐹)𝑣𝑖𝑏 = {
3 𝑖𝑓 π‘›π‘œπ‘›π‘™π‘–π‘›π‘’π‘Žπ‘Ÿ (π‘Žπ‘™π‘™ π‘œπ‘‘β„Žπ‘’π‘Ÿπ‘ )
𝑉2
2 βˆ™ 𝐢𝑃
πœ‚π‘ =
𝛾 − 1 2 −1
𝑀𝑒 ]
2
𝛾−1
𝑝 𝛾
1−( 𝑒)
𝑝𝑑2
1 − [1 +
Area-Mach Relation:
𝐴𝑒
=
𝐴∗
1 𝛾+1
𝛾
1
2
𝛾 − 1 2 2 𝛾−1
1 𝛾 − 1 2 −𝛾−1
{(
) [1 +
𝑀𝑒 ]}
βˆ™ {1 + (1 − )
𝑀𝑒 }
𝑀𝑒 𝛾 + 1
2
πœ‚π‘
2
*from resulting 𝑀𝑒 , get:
→ 𝑝𝑒 from total-to-static (above)
𝛾 − 1 2 −1
→ 𝑇𝑒 = 𝑇𝑑𝑒 [1 +
𝑀𝑒 ]
2
𝛾−1
)
→ π‘Žπ‘’ = √𝛾𝑅𝑇𝑒 π‘€β„Žπ‘’π‘Ÿπ‘’, 𝑅 = 𝐢𝑝 (
𝛾
→ 𝑉𝑒 = 𝑀𝑒 βˆ™ π‘Žπ‘’
→ 𝑇 = π‘šπ‘ 𝑉𝑒 + (𝑝𝑒 − 𝑝∞ )𝐴𝑒
Non-Isentropic Thrust Coefficient:
𝛾+1
2
2 𝛾−1
𝑝𝑒
𝐢𝑇 = 𝛾 {πœ‚π‘› (
)(
)
[1 − ( )
𝛾−1 𝛾+1
𝑝𝑑2
𝛾−1
𝛾
1
2
]} +
(𝑝𝑒 − 𝑝∞ ) 𝐴𝑒
𝑝𝑑2
𝐴∗
Injectors and Droplet Vaporization
Droplet Characterization:
Droplet Diameter Probability:
1
π‘ƒπ‘Ÿπ‘œπ‘ (𝐷 + 𝑑𝐷)
2
𝑑𝐷
*Sauter Mean Diameter (SMD): the droplet diameter with
same surface-to-volume ratio as the entire spray.
*Weber Number: ratio of inertia (mass) to surface tension
*Ohnesorge Number: ratio of friction to surface tension
𝑆𝑀𝐷
= 𝑐 βˆ™ π‘Šπ‘’ 𝑝 βˆ™ π‘‚β„Žπ‘ž
β„“
β„“
π‘Šπ‘’πΆπΆ 𝑝 π‘‚β„ŽπΆπΆ
(𝑆𝑀𝐷)𝐢𝐢 = (𝑆𝑀𝐷)π‘™π‘Žπ‘ βˆ™ ( 𝐢𝐢 ) (
) (
)
β„“π‘™π‘Žπ‘ π‘Šπ‘’π‘™π‘Žπ‘
π‘‚β„Žπ‘™π‘Žπ‘
𝑃(𝐷) =
Droplet Vaporization:
Heat of Vaporization: (heat flux into droplet)
π‘šΜ‡π‘‰ βˆ™ Δβ„Žπ‘‰ = 𝑄̇𝑖𝑛
π‘€β„Žπ‘’π‘Ÿπ‘’,
𝑑𝑇
Μ‡
𝑄𝑖𝑛 = −π‘˜ |
βˆ™ 4πœ‹π‘…2
π‘‘π‘Ÿ 𝑅(𝑑)
𝑑𝑅
π‘šΜ‡π‘‰ = −4πœ‹πœŒπΏ 𝑅2 (𝑑)
𝑑𝑑
Droplet Diameter: (as function of time)
8π‘˜
) ln(1 + 𝐡) βˆ™ 𝑑
𝐷 2 (𝑑) = 𝐷0 − (
𝜌𝐿 𝐢𝑃
𝐢𝑃 (𝑇∞ − 𝑇𝑉 )
𝐡≡
ΔhV
Vaporization time:
𝜌𝐿 𝐢𝑃
𝐷02
𝑑𝑉 = 𝐷02
=
8π‘˜ ln(1 + 𝐡) π‘˜π‘‰
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