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We measured 3-micron reflectance spectra of 21 meteorites that represent allcarbonaceous chondrite types available in terrestrial meteorite collections.The measurements were conducted at the Laboratory for Spectroscopy underPlanetary Environmental Conditions (LabSPEC) at the Johns Hopkins UniversityApplied Physics Laboratory (JHU APL) under vacuum and thermally-desiccatedconditions (asteroid-like conditions). This is the most comprehensive 3-microndataset of carbonaceous chondrites ever acquired in environments similar to theones experienced by asteroids. The 3-micron reflectance spectra are extremelyimportant for direct comparisons with and appropriate interpretations ofreflectance data from ground-based telescopic and spacecraft observations ofasteroids. We found good agreement between 3-{\mu}m spectral characteristics ofcarbonaceous chondrites and carbonaceous chondrite classifications. The3-{\mu}m band is diverse, indicative of varying composition, thus suggestingthat these carbonaceous chondrites experienced distinct parent body aqueousalteration and metamorphism environments.

3-micron Reflectance Spectroscopy of Carbonaceous Chondrites under Asteroid-like Conditions