Ground-based Infrared Spectroscopy of Mercury's Near-Global Surface with IRTF/SPEX: Complementing MESSENGER Compositional Observations

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Scientific paper

Using SpeX at the NASA IRTF telescope we have obtained disk-resolved
spectra of Mercury and lunar sites in the wavelength range 0.8-5.5 mum.
These will be compared to MESSENGER data, searched for IR spectral
features, and modeled to determine surface properties.

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