Ainhoa Muñiz Quintana: In charge of performance and propulsion for the project and in charge of communications for the group.
Atef El Nakib: In charge of component sizing and placement and stability and control. Also, Atef is in charge of the logistics of the group.
Alejandro Calleja Bezares: In charge of aerodynamics and modeling of the aircraft. Alejandro also did an extensive research on the environment.
Luis Andres: In charge of component of structural and fatgue analysis. Also, Luis is in charge of the scheduling for the group.
Chems Eddine Boudiaf: In charge of control surface study and flaps. Chems also did an extensive study on the inner components of the aircraft.
Jorge Martin de Valmaseda: In charge of electrical assembly and electrical components. Jorge is also in charge of navigation and radio connections
The goal of MEA is to design an aircraft that will be able to fly in the atmospheric conditions of Mars with the purpose of exploring new terrains and areas of interest such as future habitable land, and/or investigatory opportunities for scientists and astronauts. In order to aid with the flight mission and status of the aircraft, the plane is equipped with a controls system composed of sensors and cameras.
The goal of the mission is for a series of specific tasks to be completed in a precise sequence by the aircraft. The mission will be initiated with takeoff, climbing to a pressure of 639 Pa (1000 m), cruising for 100 km in one direction. After this, a loitering phase lasting 20 minutes will be entered by the aircraft before retracing its path back to the take-off point, where it will descend and land on the same runway as the take-off. Fig. 1 depicts the mission profile, and the total flight time for the aircraft is approximately 80 minutes.
The flight environment for Mars’s atmosphere is vastly different from that of Earth's, for one, the air is much thinner and it is more difficult for aircraft to generate lift and stay aloft since the atmospheric density of Mars is only about 1% of Earth's atmosphere2. The composition of the Martian atmosphere is also quite different, consisting primarily of carbon dioxide (95%) and small amounts of nitrogen and argon2. There is also evidence of trace amounts of methane and water vapor. Additionally, the average temperature on Mars is much colder than on Earth, with an average temperature of -62℃, dropping as low as -153℃, at the poles around noon3. Equipment and humans are exposed to high levels of radiation from the sun and cosmic rays since Mars does not have a protective magnetic field like Earth, which would cause a faster degradation of the equipment and be harmful to humans.. As a result, special considerations were considered when designing a vehicle for Mars exploration and travel, such as the use of lighter materials, an electric propulsion system, and special navigation techniques with their corresponding sensors.
The main dimensions of the aircraft are the 5 m length from the nose to the tail, a 2 m root chord, a 1 m root tip and the span of the wing is 7 m, it is also mounted 0.15 m below the x-axis with a 2º angle of attack. The difference in height between the wing and the horizontal tail is 1.38 m, having a tail span of around 4 m. The wing section fuselage of the aircraft has a diameter of 0.8 m, starting with a cone in the nose and finishing with a 0.3 m diameter truncated cone in the tail. These dimensions can be observed in Fig. 2, where it displays the 3D model of the aircraft.
The MEA is a sophisticated aircraft remotely controlled from Mars, designed for effective and efficient flight. Its internal components, including flight control, navigation, propulsion, power, and communication systems, manage stability, attitude, and maneuverability. Sensors like GPS, barometer, camera, angle of attack, thermal, and IMU provide important data for navigation, mapping, and detection of anomalies. The Pixhawk computer is a reliable interface for processing data from various sensors. The electric propulsion system and power system with batteries supply thrust and electricity. The communication system enables real-time control and data transmission between the aircraft and Ground Control Station (GCS). Integration of sensors and cameras ensures safe and efficient operation throughout the Mars mission.
First, a motor and a propeller that have a combined weight of approximately 7 kg were chosen, which caused a large load on the front of the aircraft. Since this aircraft will be flown remotely, a navigational camera in the front of the plane was necessary for visual interpretation of the terrain and to aid the pilot. With a nose to tail length of 5 m, the nose landing gear was placed 0.5 m aft the nose and the main landing gear were added to be behind the center of gravity of the aircraft to avoid having a significant change in the location of the center of gravity. Lastly, the thermal camera and batteries were placed towards the back of the aircraft to compensate for the moments that were caused by the different components located on the front of the fuselage, See Fig. 3. With this internal layout, the location of the center of gravity was calculated to be 1.925 m aft the nose of the aircraft. A good estimation of the location of the center of pressure of the aircraft would be the quarter chord of the Mean Aerodynamic Chord, which leaves a static margin of 0.095.
Side View
Side View and Dimensions
The NACA 0006 airfoil, a low-drag airfoil frequently used for unmanned aerial systems and small aircrafts, was chosen for MEA The low-drag qualities were crucial for maximizing the range and endurance of the aircraft. Many cambered airfoils were studied; however, they were directly disregarded due to the anomalies that arose when studying their graphs at low Reynolds Numbers. Moreover, when cambered airfoils were sized into wings, they failed to provide the general lift requirement for the aircraft to fly.
In addition to its low-drag characteristics, the NACA 0006 airfoil is also relatively easy to manufacture and has been extensively tested in various wind tunnels and flight tests. These factors make it a reliable choice for the lift system, ensuring that the aircraft will be able to operate effectively in the challenging Martian environment. Overall, the NACA 0006 airfoil is an excellent choice for MEA, providing a reliable and efficient lift system that will enable this aircraft to explore and investigate the Red Planet.
Designing wings for a plane flying on Mars presents unique challenges due to the planet's thin atmosphere, this means that the wings must be larger to generate enough lift to keep the plane aloft. Due to the low air density, a low-wing design was opted for. One of its main advantages is its ability to provide better stability and handling, particularly during take off and landing. Having the wings closer to the ground means that the change in the static margin would be minimal while reducing drag.
For the highest possible lift generation, the wing surface was maximized leading to a 7m wingspan and a mean aerodynamic chord (cW) of 1.56 m. Moreover, the wing was designed to have a root chord of 2m and a tip chord of 1m, creating a total wing area of 18.01 m2. The delta wing shape created a larger surface while smoothly connecting it to the fuselage creating better aerodynamics.
A T-tail was chosen for the design to improve performance during cruise conditions, and decrease the effects of turbulence and other disturbances on the horizontal stabilizer as well as drag. On another note, the range of angles of attack that MEA can operate within is relatively small, therefore stalling is more probable. Therefore, the T-tail design opted for this phenomena and now the horizontal stabilizer is not present within the wake of the wing which makes the recovery of the aircraft from stalling easier.
One step closer to space exploration!
For more information, don't hesitate to contact us:
atef.nakib@slu.edu | ainhoa.munizquintana@slu.edu | alejandro.callejabezares@slu.edu | jorge.martindevalmaseda@slu.edu