Sutton Core
NOZZLE THEORY LAB
SUTTON ROCKET PROPULSION ELEMENTS • 9TH ED • CH. 2–3
FLAGHSIP SIMULATOR • PHASE 1
Nozzle Theory Lab
Real-time isentropic converging-diverging nozzle analysis. Change any parameter — everything updates instantly.
IDEAL ROCKET THEORY
CONSTANT γ • 1D ISENTROPIC FLOW
CONSTANT γ • 1D ISENTROPIC FLOW
CHAMBER CONDITIONS
Merlin, F-1 class — dense, moderate Isp
70.0 bar
3550 K
1.220
22.5
NOZZLE GEOMETRY
16.0
Typical: 12–20 sea level • 40–150 vacuum
Current pa = 1.013 bar
NOZZLE VISUALIZATIONParametric C-D • Mach-colored walls
OVER-EXPANDED Color = local Mach number (throat M=1 → exit). Plume reacts to pe vs pa.
Isp (VACUUM)
319.1s
Isp (SEA LEVEL)
277.6s
THRUST COEFF. CF
1.5507
c* (CHAR. VEL.)
1755.6m/s
EXIT MACH
3.68
pe / pc = 0.00636
EXIT PRESSURE
0.445 bar
Te = 1425.9 K
Flow regime: OVER-EXPANDED. When pe ≈ pa the nozzle is optimally expanded for that altitude. Under-expanded (pe > pa) wastes some performance at sea level but is ideal for vacuum. Over-expanded can cause flow separation.
PERFORMANCE CURVES (at current chamber conditions)
Specific Impulse vs Expansion Ratio
Current point at ε = 16.0 → Ispvac = 319.1s
Thrust Coefficient vs Expansion Ratio
Property Distribution — Throat (x=0) to Exit (x=1)
Mach rises rapidly in the diverging section. Pressure and temperature drop.
KEY EQUATIONS (SUTTON)
Area–Mach relation (isentropic)
Thrust coefficient
Reference: George P. Sutton & Oscar Biblarz, Rocket Propulsion Elements, 9th Edition, Chapters 2–3. All calculations use the ideal rocket assumptions (perfect gas, isentropic 1D flow, constant γ).