Computational Modeling of Mars Retropropulsion Concepts in the Langley Unitary Plan Wind TunnelFuture 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.
Document ID
20210024632
Acquisition Source
Langley Research Center
Document Type
Conference Paper
Authors
Karl T Edquist (Langley Research Center Hampton, Virginia, United States)
Stephen J Alter (Langley Research Center Hampton, Virginia, United States)
Christopher E Glass (Langley Research Center Hampton, Virginia, United States)
Bill Kleb (Langley Research Center Hampton, Virginia, United States)
Ashley M Korzun (Langley Research Center Hampton, Virginia, United States)
William A Wood (Langley Research Center Hampton, Virginia, United States)
Francisco Canabal (Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Robert E Childs (Science and Technology Corporation (United States) Hampton, Virginia, United States)
Logan D Halstrom (Ames Research Center Mountain View, California, United States)
Kristen V Matsuno (Ames Research Center Mountain View, California, United States)
Date Acquired
November 19, 2021
Subject Category
AerodynamicsFluid Mechanics And Thermodynamics
Meeting Information
Meeting: 2022 AIAA SciTech Forum
Location: San Diego, CA
Country: US
Start Date: January 3, 2022
End Date: January 7, 2022
Sponsors: American Institute of Aeronautics and Astronautics
Funding Number(s)
WBS: 335803.04.21.23 CONTRACT_GRANT: NNA16BD60C
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
Single Expert
Keywords
MarsSupersonic RetropropulsionLangley Unitary Plan Wind TunnelComputational Fluid Dynamics