Particle Size Effects on Mid‐Infrared Spectra of Lunar Analog Minerals in a Simulated Lunar Environment

• Published in: Journal of geophysical research. Planets 2019-04, Vol.124 (4), p.970-988
• Main Authors: Shirley, K. A., Glotch, T. D.
• Format: Article
• Language: English
• Subjects: airless bodies; Asteroid missions; Asteroids; Data acquisition; Data interpretation; Diviner; Infrared analysis; Infrared instruments; Infrared radiometers; Infrared spectra; Laboratories; Lunar environments; Lunar regolith; Lunar spacecraft; Lunar surface; Mercury; Minerals; MIR spectroscopy; Moon; Particle size; particle size effects; Planetary composition; Planetary surfaces; Porosity; Regolith; Silicates; simulated lunar environment; Simulation; Size effects; Space missions; Spectral resolution; Spectroscopic analysis; Thermal environments; Wavelengths
• ISSN: 2169-9097; 2169-9100
• DOI: 10.1029/2018JE005533

Mid‐infrared spectroscopic analysis of the Moon and other airless bodies requires a full accounting of spectral variation due to the unique thermal environment in airless body regoliths and the substantial differences between spectra acquired under airless body conditions and those measured in an ambient environment on Earth. Because there exists a thermal gradient within the upper hundreds of microns of lunar regolith, the data acquired by the Diviner Lunar Radiometer Experiment are not isothermal with wavelength. While this complication has been previously identified, its effect on other known variables that contribute to spectral variation, such as particle size and porosity, have yet to be well characterized in the laboratory. Here we examine the effect of particle size on mid‐infrared spectra of silicates common to the Moon measured within a simulated lunar environment chamber. Under simulated lunar conditions, decreasing particle size is shown to enhance the spectral contrast of the Reststrahlen bands and transparency features, as well as shift the location of the Christiansen feature to longer wavelengths. This study shows that these variations are detectable at Diviner spectral resolution and emphasizes the need for simulated environment laboratory data sets, as well as hyperspectral mid‐infrared instruments on future missions to airless bodies. Plain Language Summary When trying to determine the composition of a planetary surface, it is important to have a basis for comparison. Currently, infrared data acquired from missions to airless bodies, like the Moon and asteroids, are mostly compared to data measured under ambient terrestrial conditions, and the difference in measurement environment complicates analysis. In this work, we measure minerals of varying particle size in the laboratory under a simulated lunar environment to understand how this variable affects the data, and whether we can detect the variations with the Lunar Reconnaissance Orbiter Diviner Lunar Radiometer Experiment. Acquiring infrared data under simulated lunar environment conditions will improve our interpretation of data not only from the Moon but also from other airless planetary bodies such as Mercury and asteroids. Key Points Particle size is an important variable affecting the position of the Christiansen feature under a simulated lunar environment Particle size variation is within the detectable limits of the Diviner Lunar Radiometer Experiment Future mid‐infrared missio