Regolith and Environment Science and Oxygen and Lunar Volatile Extraction (RESOLVE): Lunar Advanced Volatile Analysis (LAVA) Capillary Fluid Dynamic Restriction Effects on Gas ChromatographyThe Resource Prospector (RP) mission with the Regolith and Environment Science and Oxygen Lunar Volatile Extraction (RESOLVE) payload aims to show the presence of water in lunar regolith, and establish a proving ground for NASAs mission to Mars. One of the analysis is performed by the Lunar Advanced Volatiles Analysis (LAVA) subsystem, which consists of a fluid network that facilitates the transport of volatile samples to a gas chromatograph and mass spectrometer (GC-MS) instrument. The understanding of fluid dynamics directed from the GC to the MS is important due to the influence of flow rates and pressures that affect the accuracy of and prevent the damage to the overall GC-MS instrument. The micro-scale capillary fluid network within the GC alone has various lengths and inner-diameters; therefore, determination of pressure differentials and flow rates are difficult to model computationally, with additional complexity from the vacuum conditions in space and lack of a lunar atmosphere. A series of tests were performed on an experimental set-up of the system where the inner diameters of the GC transfer line connecting to the MS were varied. The effect on chromatography readings were also studied by applying these lines onto a GC instrument. It was found that a smaller inner diameter transfer line resulted in a lower flow rate, as well as a lower pressure differential across the thermal conductivity detector (TCD) unit of the GC and a negligible pressure drop across the mock-up capillary column. The chromatography was affected with longer retention times and broader peak integrations. It was concluded that a 0.050 mm inner diameter line still proved most suitable for the systems flow rate preferences. In addition, it was evident that this small transfer line portrayed some expense to GC signal characteristics and the wait time for steady-state operation.
Document ID
20150018436
Acquisition Source
Kennedy Space Center
Document Type
Other
Authors
Gonzalez, Marianne (California State Univ. Long Beach, CA, United States)
Quinn, Jacqueline (NASA Kennedy Space Center Cocoa Beach, FL United States)
Captain, Janine (NASA Kennedy Space Center Cocoa Beach, FL United States)
Santiago-Bond, Josephine (NASA Kennedy Space Center Cocoa Beach, FL United States)
Starr, Stanley (NASA Kennedy Space Center Cocoa Beach, FL United States)
Date Acquired
September 28, 2015
Publication Date
August 3, 2015
Subject Category
Inorganic, Organic And Physical ChemistryFluid Mechanics And Thermodynamics
Report/Patent Number
KSC-E-DAA-TN25779Report Number: KSC-E-DAA-TN25779
Funding Number(s)
CONTRACT_GRANT: NNX13AJ45A
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
RESOLVELAVARPLunar Advanced Volatile AnalysisRegolith and Environment Science and Oxygen and Lunar Volatile ExtractionGCFluid dynamicsIntern ReportCapillaryResource ProspectorRP-15GC-MSGas ChromatographyCapillary SlipNIFS