The LEMFEV concept addresses critical gaps in Mars exploration: it complements existing tools (rovers, orbiters) by enabling direct, repeatable, and flexible atmospheric and surface observations at scales and locations previously inaccessible.
- Single‑flight missions: in‑flight measurements and data transmission.
- Multiple‑flight missions: repeated sorties to cover larger areas and gather time‑series data.
- Wind tunnel experiments with liquid crystals to visualise airflow patterns.
- Stratospheric balloon test (planned for late 2024): the flying model will be raised to ~32 km altitude to simulate Martian atmospheric conditions.
- cameras (for different wavelength ranges, 1.5 kg);
- meteorological sensors (0.5 kg) — to track wind, temperature, humidity;
- LIDAR (0.5 kg);
- radiometer (0.5 kg);
- ground‑penetrating radar (1 kg);
- infrared (IR) spectrometer (1.5 kg).
Instrumentation (example payload, total mass: 5.5 kg):
The LEMFEV will operate at relatively low Reynolds numbers, which increases friction drag and may cause laminar bubbles.
The team optimises the airfoil section for each aircraft version to improve aerodynamic performance.
Liquid crystals will be used in wind tunnel tests to study the boundary layer, detect the laminar‑turbulent transition, and analyse flow separation.
Aerodynamic optimisation:
- Low atmospheric density (about 1 % of Earth’s) requires high wing loading and efficient aerodynamics.
- Low speed of sound affects flight dynamics and control.
- Extreme temperatures and dust storms demand robust materials and protective systems.
- Electrical phenomena in the Martian atmosphere must be accounted for in electronics design.
- Terrain complexity rules out conventional take‑off and landing — the design must include alternative solutions.
Design challenges and solutions: