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Mineralogical, Elemental and Tomographic Reconnaissance Investigation for CLPS (“METRIC”)METRIC comprises a suite of two instruments in a Lunar lander that perform X-ray diffraction (XRD) for mineral structure, X-ray fluorescence (XRF) for elemental composition, and X-ray Micro Computed Tomography (XCT) for 3D internal micromorphology. The instruments are accompanied by optical-near IR cameras to provide local geologic context. The Honeybee Robotics PlanetVac pneumatic sampling and transfer system [1],positioned on a lander footpad, will deliver sieved regolith to the X-ray instruments for analysis. The instrument suite is intended for delivery to the lunar surface on a Commercial Lunar Payload Services (CLPS) lander. The METRICXRD/F instrument draws on heritage from the Mars Science Laboratory CheMin instrument [2] and improves upon the design in multiple ways [3]. Like CheMin, Rietveld refinement and full-pattern fitting of METRIC XRD data can identify minerals at a detection limit of ~1 wt.%, quantify their abundances when present at >3 wt.%, and determine mineral composition (e.g., Fo#in olivine) from lattice parameters for minerals present at >5 wt.%[4,5]. An optimized XRF geometry provides for improved detection and quantification of major, minor and trace elements. The METRIC XCT instrument is a miniaturized X-ray Computed Tomography scanner[6]. Lunar regolith is delivered to a 3 mm diameter, 10 mm long graphite tube inside the instrument. The tube is rotated through 360°in 0.9deg.incrementsand a divergent point source X-ray beam is directed through the material. A Charge Coupled Device (CCD)records attenuation images whose brightness and contrast area function of average atomic number and density. Quantitative data, including particle and void sizes, 3D particle shape parameters, modal volumes and pore geometry can be derived from the resulting 3D reconstructions(voxel resolution: 30 μm). Crystal morphologies derived from METRIC XCT data complement the bulk mineralogy determined by the METRIC XRD/F and provide a measure of grain size distribution for the different phases. Taken together, the METRIC instrument suite determines crystal structure, elemental composition and morphology, three principal characteristics of geological materials that are highly useful in determining the origin and subsequent processing of lunar regolith.
Document ID
20220002240
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
E B Rampe
(Johnson Space Center Houston, Texas, United States)
K Cannon
(Colorado School of Mines Golden, Colorado, United States)
P Sarrazin
(eXaminArt Mountain View, California, United States)
D F Blake
(Ames Research Center Mountain View, California, United States)
R W Obbard
(Search for Extraterrestrial Intelligence Mountain View, California, United States)
P Lucey
(University of Hawaii System Honolulu, Hawaii, United States)
D Bergman
(Honeybee Robotics (United States) Brooklyn, New York, United States)
G J Taylor
(University of Hawaii System Honolulu, Hawaii, United States)
D T Vaniman
(Planetary Science Institute Tucson, Arizona, United States)
Date Acquired
February 9, 2022
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: 44th Committee on Space Research Scientific Assembly (COSPAR 2022)
Location: Athens
Country: GR
Start Date: July 16, 2022
End Date: July 24, 2022
Sponsors: COSPAR
Funding Number(s)
WBS: 981698
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Keywords
Moon
XRD
XRF
XCT
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