Lunar sample measurements were made both under ambient nitrogen pressure and under vacuum conditions. Average emittance values were analyzed for a number of samples which were determined to include silicate minerals, pyroxenes, and fine particle feldspar. Information is also provided on modifications made to emittance apparatus in order to work with smaller sample sizes and to prevent accidental loss or contamination of the lunar sample material
Mid‐infrared spectroscopic analysis of the Moon and other airless bodies requires a full accounting ...
Flameless atomic abosrption, X-ray photoemission spectroscopy, ferromagnetic resonance, scanning ele...
Space weathering processes induce changes to the physical, chemical, and optical properties of space...
Currently, few thermal infrared measurements exist of fine particulate ( < 63 μm) analogue samples (...
Here we present new laboratory spectral measurements of the major silicate minerals identified on th...
Presented here are infrared reflectance spectra of a typical set of Apollo samples to illustrate spe...
The infrared spectra of analogs of lunar soils were investigated to further the development of metho...
One of the key problems in determining lunar surface composition for thermal-infrared measurements ...
One of the key problems in determining lunar surface composition for thermal-infrared measurements i...
Here we present a comprehensive set of laboratory measurements from the ultraviolet (UV) to the far...
Two lunar soils: basalt and anorthosite, three glasses: synthetic glass, basalt glass, and obsidian ...
The Diviner Lunar Radiometer, onboard NASA's Lunar Reconnaissance Orbiter, has produced the first gl...
Laboratory investigations were made of the spectral emission properties of a limited number of sili...
Infrared spectrophotometry evaluated for compositional analysis of lunar and planetary soil
Past and continuing observations indicate an enrichment of volatile materials in lunar polar regions...
Mid‐infrared spectroscopic analysis of the Moon and other airless bodies requires a full accounting ...
Flameless atomic abosrption, X-ray photoemission spectroscopy, ferromagnetic resonance, scanning ele...
Space weathering processes induce changes to the physical, chemical, and optical properties of space...
Currently, few thermal infrared measurements exist of fine particulate ( < 63 μm) analogue samples (...
Here we present new laboratory spectral measurements of the major silicate minerals identified on th...
Presented here are infrared reflectance spectra of a typical set of Apollo samples to illustrate spe...
The infrared spectra of analogs of lunar soils were investigated to further the development of metho...
One of the key problems in determining lunar surface composition for thermal-infrared measurements ...
One of the key problems in determining lunar surface composition for thermal-infrared measurements i...
Here we present a comprehensive set of laboratory measurements from the ultraviolet (UV) to the far...
Two lunar soils: basalt and anorthosite, three glasses: synthetic glass, basalt glass, and obsidian ...
The Diviner Lunar Radiometer, onboard NASA's Lunar Reconnaissance Orbiter, has produced the first gl...
Laboratory investigations were made of the spectral emission properties of a limited number of sili...
Infrared spectrophotometry evaluated for compositional analysis of lunar and planetary soil
Past and continuing observations indicate an enrichment of volatile materials in lunar polar regions...
Mid‐infrared spectroscopic analysis of the Moon and other airless bodies requires a full accounting ...
Flameless atomic abosrption, X-ray photoemission spectroscopy, ferromagnetic resonance, scanning ele...
Space weathering processes induce changes to the physical, chemical, and optical properties of space...