Spectral Characterization of Bennu Analogs Using PASCALE: A New Experimental Set‐Up for Simulating the Near‐Surface Conditions of Airless Bodies
Autor: | Neil Bowles, Devin L. Schrader, T. Warren, S. B. Calcutt, V. E. Hamilton, A. Clack, Jon Temple, K. L. Donaldson Hanna, Dante S. Lauretta, Timothy J. McCoy |
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Rok vydání: | 2021 |
Předmět: |
Atmospheres
010504 meteorology & atmospheric sciences Planetary Atmospheres Clouds and Hazes Permafrost Atmospheric Composition and Structure Biogeosciences 01 natural sciences Meteorites and Tektites Spectral line Planetary Sciences: Solar System Objects Physics and Chemistry of Materials Earth and Planetary Sciences (miscellaneous) Planetary Sciences: Astrobiology Permafrost Cryosphere and High‐latitude Processes Planetary Atmospheres Composition of Meteorites Meteorite Mineralogy and Petrology Asteroids Characterization (materials science) Planetary Mineralogy and Petrology Surfaces Geophysics Meteorite Asteroid Comets: Dust Tails and Trails Bennu Planetary Sciences: Comets and Small Bodies airless bodies Cryosphere Composition Research Article spectroscopy Materials science Mineralogy Planetary Geochemistry Cryobiology Geochemistry and Petrology Chondrite Comets Emissivity Spectroscopy Planetary Sciences: Solid Surface Planets Planetary Sciences: Fluid Planets Mineralogy and Petrology 0105 earth and related environmental sciences Albedo Geochemistry Space and Planetary Science thermal infrared Other laboratory Natural Hazards |
Zdroj: | Journal of Geophysical Research. Planets |
ISSN: | 2169-9100 2169-9097 |
DOI: | 10.1029/2020je006624 |
Popis: | We describe the capabilities, radiometric stability, and calibration of a custom vacuum environment chamber capable of simulating the near‐surface conditions of airless bodies. Here we demonstrate the collection of spectral measurements of a suite of fine particulate asteroid analogs made using the Planetary Analogue Surface Chamber for Asteroid and Lunar Environments (PASCALE) under conditions like those found on Earth and on airless bodies. The sample suite includes anhydrous and hydrated physical mixtures, and chondritic meteorites (CM, CI, CV, CR, and L5) previously characterized under Earth‐ and asteroid‐like conditions. And for the first time, we measure the terrestrial and extra‐terrestrial mineral end members used in the olivine‐ and phyllosilicate‐dominated physical mixtures under the same conditions as the mixtures and meteorites allowing us better understand how minerals combine spectrally when mixed intimately. Our measurements highlight the sensitivity of thermal infrared emissivity spectra to small amounts of low albedo materials and the composition of the sample materials. As the albedo of the sample decreases, we observe smaller differences between Earth‐ and asteroid‐like spectra, which results from a reduced thermal gradient in the upper hundreds of microns in the sample. These spectral measurements can be compared to thermal infrared emissivity spectra of asteroid (101955) Bennu's surface in regions where similarly fine particulate materials may be observed to infer surface compositions. Key Points Thermal infrared spectra of fine particulate minerals, physical mixtures of those minerals, and meteorites were measured under simulated Bennu conditionsComparisons of mineral, physical mixture, and meteorite spectra highlight the spectral behavior when materials are mixed in increasing complexityAs albedo decreases the spectral effects due to thermal gradients due to the vacuum environment of airless bodies are reduced |
Databáze: | OpenAIRE |
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