Thermal infrared emissivity measurements under a simulated lunar environment: Application to the Diviner Lunar Radiometer Experiment
Donaldson Hanna, Kerri L. and Wyatt, Michael and Thomas, Ian R. and Bowles, Neil and Greenhagen, Benjamin and Maturilli, Alessandro and Helbert, Jörn (2012) Thermal infrared emissivity measurements under a simulated lunar environment: Application to the Diviner Lunar Radiometer Experiment. Journal of Geophysical Research, 117, . DOI: 10.1029/2011JE003862 .
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Here we present new laboratory spectral measurements of the major silicate minerals identified on the Moon (plagioclase solid series endmembers: albite and anorthite; clinopyroxene and orthopyroxene; and the olivine endmember forsterite) under lunar environmental conditions. We make the first characterization of thermal infrared spectral changes between ambient and lunar environment conditions over the 7 – 25 μm wavelength range for a fine-grained mineral suite and evaluate their application to lunar remote sensing data sets. The lunar environment introduces observable effects in thermal infrared emissivity spectra of fine grain minerals, which include: (1) a shift in the Christensen Feature (CF) position to shorter wavelengths, (2) an increase in the overall spectral contrast, and (3) decreases in the spectral contrast of the Reststrahlen Bands (RB) and Transparency Features (TF). Thus, our new measurements demonstrate the high sensitivity of minerals to environmental conditions under which they are measured and provide important constraints for interpreting new thermal infrared datasets of the Moon, including the Diviner Lunar Radiometer Experiment onboard NASA’s Lunar Reconnaissance Orbiter. Full resolution laboratory mineral spectra deconvolved to Diviner’s three spectral channels demonstrate that the spectral shape, CF position and band ratios can be used to distinguish between individual mineral groups and lunar lithologies. The integration of the thermal infrared CF position with near infrared spectral parameters allow us to make more robust mineralogical identifications and provide a framework for future integrations of data sets across two different wavelength regimes.
|Title:||Thermal infrared emissivity measurements under a simulated lunar environment: Application to the Diviner Lunar Radiometer Experiment|
|Journal or Publication Title:||Journal of Geophysical Research|
|In Open Access:||No|
|In ISI Web of Science:||No|
|HGF - Research field:||Aeronautics, Space and Transport|
|HGF - Program:||Space|
|HGF - Program Themes:||Space Science and Exploration|
|DLR - Research area:||Raumfahrt|
|DLR - Program:||R EW - Erforschung des Weltraums|
|DLR - Research theme (Project):||R - Vorhaben Exploration des Sonnensystems|
|Institutes and Institutions:||Institute of Planetary Research > Terahertz and Infrared Sensors|
|Deposited By:||Dr.rer.nat. Jörn Helbert|
|Deposited On:||30 May 2012 09:19|
|Last Modified:||22 Oct 2013 03:04|
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