Mid-infrared reflectance spectroscopy of synthetic glass analogs for Mercury surface studies

نویسندگان

چکیده

We have synthesized and analyzed by mid-infrared reflectance spectroscopy silicate glasses that are representative for the on surface of Mercury. The glass compositions based high-pressure laboratory experiments resulting phase. spectra interest investigating Mercury using MERTIS (Mercury Radiometer Thermal Infrared Spectrometer) instrument board ESA/JAXA BepiColombo mission. Both powdered fractions polished blocks been analyzed. Powdered size 0–25 μm, 25-63 63-125 125–250 μm were measured in thermal infrared (2–20 μm). Spectra bulk (1.6 wt% - 19.0 MgO) show a single, dominating Reststrahlenband (RB, 9.3–9.8 μm), Christiansen Feature (CF; 7.6 8.1 dependent Transparency (TF; 11.6–11.9 Micro-FTIR analyses (3.4–26.5 characteristic bands at 7.8–8.2 (CF), 9.3–9.9 (RB). Only few olivine crystalline features observed. Spectral correlate with compositional characteristics, e.g. SiO2 content or SCFM (SiO2/(SiO2 + CaO FeO index. strongest correlation between band CF strong RB Mg/Si. No simple mixture from this study is able to reproduce entire ground spectrum However, Mg-rich identified 8.5 9.9 12.4 μm.

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ژورنال

عنوان ژورنال: Icarus

سال: 2021

ISSN: ['0019-1035', '1090-2643']

DOI: https://doi.org/10.1016/j.icarus.2021.114363