NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Mars 2020 Entry, Descent, and Landing Instrumentation 2 (MEDLI2) Sensor SuiteThe Mars 2020 Entry, Descent, and Landing Instrumentation 2 (MEDLI2) sensor suite seeks to address the aerodynamic, aerothermodynamic, and thermal protection system (TPS) performance issues during atmospheric entry, descent, and landing of the Mars 2020 mission. Based on the highly successful instrumentation suite that flew on Mars Science Laboratory (MEDLI), the new sensor suite expands on the types of measurements and also seeks to answer questions not fully addressed by the previous mission. Sensor Package: MEDLI2 consists of 7 pressure transducers, 17 thermal plugs, 2 heat flux sensors, and one radiometer. The sensors are distributed across both the heatshield and backshell, unlike MEDLI (the first sensor suite), which was located solely on the heat-shield. The sensors will measure supersonic pressure on the forebody, a pressure measurement on the aftbody, near-surface and in-depth temperatures in the heatshield and backshell TPS materials, direct total heat flux on the aftbody, and direct radiative heating on the aftbody. Instrument Development: The supersonic pressure transducers, the direct heat flux sensors, and the radiometer all were tested during the development phase. The status of these sensors, including the piezo-resistive pressure sensors, will be presented. The current plans for qualification and calibration for all of the sensors will also be discussed. Post-Flight Data Analysis: Similar to MEDLI, the estimated flight trajectory will be reconstructed from the data. The aerodynamic parameters that will be reconstructed will be the axial force coefficient, freestream Mach number, base pressure, atmospheric density, and winds. The aerothermal quantities that will be determined are the heatshield and backshell aero-heating, turbulence transition across the heatshield, and TPS in-depth performance of PICA. By directly measuring the radiative and total heat fluxes on the back-shell, the convective portion of the heat flux will be estimated. The status of the current tools to perform the post-flight data analysis will be presented, along with plans for model improvements.
Document ID
20170009078
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Hwang, Helen H.
(NASA Ames Research Center Moffett Field, CA, United States)
Wright, Henry S.
(NASA Langley Research Center Hampton, VA, United States)
Kuhl, Christopher A.
(NASA Langley Research Center Hampton, VA, United States)
Schoenenberger, Mark
(NASA Langley Research Center Hampton, VA, United States)
White, Todd R.
(NASA Ames Research Center Moffett Field, CA, United States)
Karlgaard, Christopher D.
(Analytical Mechanics Associates, Inc. Hampton, VA, United States)
Mahzari, Milad
(NASA Ames Research Center Moffett Field, CA, United States)
Oishi, Tomo
(Jacobs Technology, Inc. Moffett Field, CA, United States)
Pennington, Steven
(Science Systems and Applications, Inc. Hampton, VA, United States)
Trombetta, Dominic
(NASA Langley Research Center Hampton, VA, United States)
Santo, Jose
(Jacobs Technology, Inc. Moffett Field, CA, United States)
Date Acquired
September 27, 2017
Publication Date
June 12, 2017
Subject Category
Spacecraft Instrumentation And Astrionics
Report/Patent Number
ARC-E-DAA-TN40069
Meeting Information
Meeting: International Planetary Probe Workshop
Location: The Hague
Country: Netherlands
Start Date: June 12, 2017
End Date: June 16, 2017
Sponsors: NASA Headquarters
Funding Number(s)
CONTRACT_GRANT: NNL12AA09C
CONTRACT_GRANT: NNA16BD26C
Distribution Limits
Public
Copyright
Public Use Permitted.
No Preview Available