The paper deals with the aerodynamic analysis of a manned braking system entering the Mars atmosphere, with the aim to support planetary entry system design studies. The capsule configuration is an axisymmetric blunt body close to the Apollo capsule. Several fully three-dimensional Computational Fluid Dynamics analyses have been performed to assess the flowfield environment around the vehicle to address the aerodynamic performance of the entry capsule within mission exploration to Mars. To this end, a wide range of flow conditions including reacting and non-reacting flow, different angles of attack, and Mach numbers have been investigated and compared. Moreover, non-equilibrium effects on the flowfield around the capsule have been also investigated. Results show that real-gas effects, for all the angles of attach considered, increase both the aerodynamic drag and pitching moment, whereas the lift is only slighted affected. Finally, results comparisons highlight that experimental and CFD aerodynamic findings available for the Apollo capsule in air adequately represent the static coefficients of the capsule in the Mars atmosphere.
Nomenclatureforce, N L = Aerodynamic Lift, N M = Mach number / Aerodynamic Moment, Nm P = Pressure, Pa q = Dynamic Pressure, Pa R = Radius of curvature, m Re = Reynolds number S = Reference Area, m 2 Greek symbols α = Angle of attack, deg ρ = Density, kg/m 3 γ = Specific heats ratio Subscripts b = base ref = reference t2 = stagnation point downstream a normal shock w = wall 1 Professor, Chair of Fluid Dynamics, Dipartimento di Ingegneria Aerospaziale e Meccanica (DIAM), antonio.viviani@unina2.it, AIAA Senior Member.