Abstract
The need for advanced propulsion systems for space exploration has led to extensive research into the cooling mechanisms of rocket engines. This study investigates using methane as a coolant under transcritical temperature and supercritical pressure conditions, focusing on understanding heat transfer deterioration. The Reynolds-Averaged Navier–Stokes equations are solved numerically for pure methane flowing in a high aspect ratio cooling channel for different operating conditions. The GERG-2008 equation of state and extended corresponding states models are used to calculate the properties of methane. The Simulation results showed that the optimum height of wall roughness size is directly linked to the applied heat flux and mass flow rate for each specific operating pressure. The surface roughness of the cooling channels must be carefully designed and manufactured for each specific supercritical operating pressure to maximize heat transfer and minimize pressure drop. This research improves the cooling system designs for rocket engines, which could lead to more efficient and reliable propulsion systems for future space missions.
Original language | English |
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Pages (from-to) | 617-630 |
Number of pages | 14 |
Journal | Acta Astronautica |
Volume | 228 |
DOIs | |
State | Published - Mar 2025 |
Keywords
- Cooling channel
- Heat transfer
- Heat transfer deterioration
- Liquefied natural gas
- Liquid rocket engine
- Supercritical pressure
- Wall roughness