The OSIRIS-REx Thermal Emission Spectrometer (OTES) Instrument
P. R. Christensen, V. E. Hamilton, G. L. Mehall, D. Pelham, W., O'Donnell, S. Anwar, H. Bowles, S. Chase, J. Fahlgren, Z. Farkas, T. Fisher,, O. James, I. Kubik, I. Lazbin, M. Miner, M. Rassas, L. Schulze, K., Shamordola, T. Tourville, G. West, R. Woodward, D. Lauretta

TL;DR
The OSIRIS-REx Thermal Emission Spectrometer (OTES) is a compact, highly precise instrument designed to analyze Bennu's surface mineralogy and thermophysical properties, aiding sample site selection and studying the Yarkovsky effect.
Contribution
This paper details the design, calibration, and specifications of the OTES instrument, a novel Fourier transform spectrometer for planetary surface analysis.
Findings
High radiometric precision (<= 2.2 x 10^-8 W cm^-2 sr^-1/cm^-1)
Absolute radiance error <1% for 150-380 K temperatures
Compact design with 6.27 kg mass and 10.8 W power consumption
Abstract
The OSIRIS-REx Thermal Emission Spectrometer (OTES) will provide remote measurements of mineralogy and thermophysical properties of Bennu to map its surface, help select the OSIRIS-REx sampling site, and investigate the Yarkovsky effect. OTES is a Fourier transform spectrometer covering the spectral range 5.71 - 100 {\mu}m (1750 - 100 cm-1) with a spectral sample interval of 8.66 cm-1 and a 6.5-mrad field of view. The OTES telescope is a 15.2-cm diameter Cassegrain telescope that feeds a flat-plate Michelson moving mirror mounted on a linear voice-coil motor assembly. A single uncooled deuterated L-alanine doped triglycine sulfate (DLATGS) pyroelectric detector is used to sample the interferogram every two seconds. Redundant ~0.855 {\mu}m laser diodes are used in a metrology interferometer to provide precise moving mirror control and IR sampling at 772 Hz. The beamsplitter is a 38-mm…
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Taxonomy
TopicsAtmospheric and Environmental Gas Dynamics
