1. THERMAP: a mid-infrared spectro-imager for space missions to small bodies in the inner solar system
- Author
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Groussin, O., Licandro, J., Helbert, J., Reynaud, J. -L., Levacher, P., García-Talavera, M. Reyes, Alí-Lagoa, V., Blanc, P. -E., Brageot, E., Davidsson, B., Delbó, M., Deleuze, M., Delsanti, A., Garcia, J. J. Diaz, Dohlen, K., Ferrand, D., Green, S., Jorda, L., Álvarez, E. Joven, Knollenberg, J., Kührt, E., Lamy, P., Lellouch, E., Merrer, J. Le, Marty, B., Mas, G., Rossin, C., Rozitis, B., Sunshine, J., Vernazza, P., and Vives, S.
- Subjects
Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Earth and Planetary Astrophysics - Abstract
We present THERMAP, a mid-infrared (8-16 {\mu}m) spectro-imager for space missions to small bodies in the inner solar system, developed in the framework of the MarcoPolo-R asteroid sample return mission. THERMAP is very well suited to characterize the surface thermal environment of a NEO and to map its surface composition. The instrument has two channels, one for imaging and one for spectroscopy: it is both a thermal camera with full 2D imaging capabilities and a slit spectrometer. THERMAP takes advantage of the recent technological developments of uncooled microbolometers detectors, sensitive in the mid-infrared spectral range. THERMAP can acquire thermal images (8-18 {\mu}m) of the surface and perform absolute temperature measurements with a precision better than 3.5 K above 200 K. THERMAP can acquire mid-infrared spectra (8-16 {\mu}m) of the surface with a spectral resolution {\Delta}{\lambda} of 0.3 {\mu}m. For surface temperatures above 350 K, spectra have a signal-to-noise ratio >60 in the spectral range 9-13 {\mu}m where most emission features occur., Comment: 21 pages, 12 figures, 3 tables; Experimental Astronomy: in press
- Published
- 2015
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