Future human Mars missions will require powered descent starting at supersonic conditions, something which has never been done before at Mars. Computational powered descent flowfield simulations have been completed at full-scale Mars conditions, but the available ground test data are not appropriate for calibrating computational uncertainties for aerodynamic interference on proposed Mars descent vehicles. A test will be conducted in the NASA Langley Unitary Plan Wind Tunnel to begin addressing powered descent aerodynamics risks for large-scale human Mars entry concepts and to identify gaps in computational predictive capabilities. This paper covers pre-test computational flowfield predictions of two different models derived from full-scale reference vehicles: a blunt low lift-to-drag vehicle and a more slender geometry. Calculations of the blunt model include variations in nozzle configuration: nozzle location, size, area ratio, and pointing direction. There exist some significant differences between solvers, but some general trends are observed from simulations of the blunt model. First, aerodynamic axial force from the heatshield decreases with increasing thrust due to expanding plume blockage. Second, nozzles that point along the model axis result in lower aerodynamic axial force compared to nozzles that have a radial thrust component. Finally, placing the nozzles further away from the model nose preserves more heatshield axial force with increasing thrust com- pared to nozzles that are closer to the nose. For the slender model, the axial force from the heatshield is similar to the non-blowing axial force regardless of thrust magnitude, due to the nozzle arrangement on the heatshield. Once the test is completed, direct comparisons between the computations and test data will be made to determine computational uncertainties in a wind tunnel environment, to identify gaps in predictive capabilities, and to inform planning for future ground and flight test programs for Mars powered descent vehicles.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen


    Exportieren, teilen und zitieren



    Titel :

    Computational Modeling of Mars Retropropulsion Concepts in the Langley Unitary Plan Wind Tunnel


    Beteiligte:
    Karl T Edquist (Autor:in) / Stephen J Alter (Autor:in) / Christopher E Glass (Autor:in) / Bill Kleb (Autor:in) / Ashley M Korzun (Autor:in) / William A Wood (Autor:in) / Francisco Canabal (Autor:in) / Robert E Childs (Autor:in) / Logan D Halstrom (Autor:in) / Kristen V Matsuno (Autor:in)

    Kongress:

    2022 AIAA SciTech Forum ; 2022 ; San Diego, CA, US


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch




    Computational Modeling of Mars Retropropulsion Concepts in the Langley Unitary Plan Wind Tunnel

    Edquist, Karl T. / Alter, Stephen J. / Glass, Christopher E. et al. | AIAA | 2022



    Computational Modeling of Mars Retropropulsion Concepts in the Langley Unitary Plan Wind Tunnel

    Edquist, Karl T. / Alter, Stephen J. / Glass, Christopher E. et al. | TIBKAT | 2022


    Testing of Mars Retropropulsion Concepts in the Langley Unitary Plan Wind Tunnel

    Karl T. Edquist / Matthew N. Rhode / Bryan E. Falman et al. | NTRS