Modeling transmission windows in Titan’s lower troposphere: Implications for infrared spectrometers aboard future aerial and surface missions
نویسندگان
چکیده
From orbit, the visibility of Titan's surface is limited to a handful narrow spectral windows in near-infrared (near-IR), primarily from absorption methane gas. This has ability identify specific compounds on -- date bulk composition remains unknown. Further, understanding would provide insight into geologic processes, photochemical production and evolution, biological potential surface. One approach obtain wider coverage with which study by decreasing integrated column absorbers (primarily methane) scatterers between observer only possible if future missions operate at lower altitudes atmosphere. Herein, we use radiative transfer model measure detail through atmosphere different mission altitudes, consider impacts this have for interpreting reflectance measurements Over our modeled range 0.4 - 10 micron, find that increases width transmission as large 317% can be obtained performing remote observations However, any appreciable widening requires onboard illumination. make note are not currently observable but could identified using low altitudes. These simple nitriles such cyanoacetylene, building blocks amino acids urea. Finally, discuss implications identifications these Titan science.
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ژورنال
عنوان ژورنال: Icarus
سال: 2021
ISSN: ['0019-1035', '1090-2643']
DOI: https://doi.org/10.1016/j.icarus.2020.114228