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Thermal Analysis Methods for Aerobraking HeatingAs NASA begins exploration of other planets, a method of non-propulsively slowing vehicles at the planet, aerobraking, may become a valuable technique for managing vehicle design mass and propellant. An example of this is Mars Reconnaissance Orbiter (MRO), which will launch in late 2005 and reach Mars in March of 2006. In order to save propellant, MRO will use aerobraking to modify the initial orbit at Mars. The spacecraft will dip into the atmosphere briefly on each orbit, and during the drag pass, the atmospheric drag on the spacecraft will slow it, thus lowering the orbit apoapsis. The largest area on the spacecraft, and that most affected by the heat generated during the aerobraking process, is the solar arrays. A thermal analysis of the solar arrays was conducted at NASA Langley, to simulate their performance throughout the entire roughly 6-month period of aerobraking. Several interesting methods were used to make this analysis more rapid and robust. Two separate models were built for this analysis, one in Thermal Desktop for radiation and orbital heating analysis, and one in MSC.Patran for thermal analysis. The results from the radiation model were mapped in an automated fashion to the Patran thermal model that was used to analyze the thermal behavior during the drag pass. A high degree of automation in file manipulation as well as other methods for reducing run time were employed, since toward the end of the aerobraking period the orbit period is short, and in order to support flight operations the runs must be computed rapidly. All heating within the Patran Thermal model was combined in one section of logic, such that data mapped from the radiation model and aeroheating model, as well as skin temperature effects on the aeroheating and surface radiation, could be incorporated easily. This approach calculates the aeroheating at any given node, based on its position and temperature as well as the density and velocity at that trajectory point. Run times on several different processors, computer hard drives, and operating systems (Windows versus Linux) were evaluated.
Document ID
20050232839
Acquisition Source
Langley Research Center
Document Type
Preprint (Draft being sent to journal)
Authors
Amundsen, Ruth M.
(NASA Langley Research Center Hampton, VA, United States)
Gasbarre, Joseph F.
(NASA Langley Research Center Hampton, VA, United States)
Dec, John A.
(NASA Langley Research Center Hampton, VA, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2005
Subject Category
Lunar And Planetary Science And Exploration
Meeting Information
Meeting: 16th Annual Thermal and Fluids Analysis Workshop
Location: Orlando, FL
Country: United States
Start Date: August 8, 2005
End Date: August 12, 2005
Funding Number(s)
OTHER: 23-892-10-01
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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