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Observing Ice Sublimation From Water-Doped Lunar Simulant at Cryogenic TemperaturesNASA's Resource Prospector (RP) mission is intended to characterize the three-dimensional nature of volatiles in lunar polar and permanently shadowed regions. The Near-Infrared Volatile Spectrometer System (NIRVSS) observes while a drill penetrates to a maximum depth of 1 m. Any 10 cm increment of soil identified as containing water ice can be delivered to a heating crucible with the evolved gas delivered to a gas chromatograph / mass spectrometer. NIRVSS consists of two components; a spectrometer box (SB) and bracket assembly (BA), connected by two fiber optic cables. The SB contains separate short- and long-wavelength spectrometers, SW and LW respectively, that collectively span the 1600-3400 nm range. The BA contains an IR emitter (lamp), drill observation camera (DOC, 2048 x 2048 CMOS detector), 8 different wavelength LEDs, and a longwave calibration sensor (LCS) measuring the surface emissivity at four IR wavelengths. Tests of various RP sub-systems have been under-taken in a large cryo-vacuum chamber at Glenn Re-search Center. The chamber accommodates a tube (1.2 m high x 25.4 cm diameter) filled with lunar simulant, NU-LHT-3M, prepared with known abundances of water. Thermocouples are embedded at different depths, and also across the surface of the soil tube. In the chamber the tube is cooled with LN2 as the pressure is reduced to approx. 5-6x10(exp -6) Torr. For the May 2016 tests two soil tubes were prepared with initially 2.5 Wt.% water. The shroud surrounding the soil tube was held at different temperatures for each tube to simulate a warm and cold lunar environment. Table 1 provides a summary of experimental conditions and Figure 1 shows the nominal view of the NIRVSS components, the drill foot, and the top of the soil tube. Once the average soil temperature reached approx. 178 K, drilling commenced. During drilling activities NIRVSS was alternating between obtaining spectra and obtaining images. Here we discuss NIRVSS spectral data obtained during controlled drill percussions.
Document ID
20180002066
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Roush, T. L.
(NASA Ames Research Center Moffett Field, CA, United States)
Teodoro, L. F. A.
(Bay Area Environmental Research Inst. Petaluma, CA, United States)
Colaprete, A.
(NASA Ames Research Center Moffett Field, CA, United States)
Cook, A. M.
(Millennium Engineering and Integration Co. Moffett Field, CA, United States)
Elphic, R.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
March 23, 2018
Publication Date
March 19, 2018
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
ARC-E-DAA-TN52117
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 19, 2018
End Date: March 23, 2018
Sponsors: Lunar and Planetary Inst.
Funding Number(s)
CONTRACT_GRANT: NNA13AC87C
CONTRACT_GRANT: NNX16AO96A
Distribution Limits
Public
Copyright
Public Use Permitted.
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