THERMAP: a mid-infrared spectro-imager for space missions to small bodies in the inner solar system - Archive ouverte HAL
Article Dans Une Revue Experimental Astronomy Année : 2016

THERMAP: a mid-infrared spectro-imager for space missions to small bodies in the inner solar system

J. Helbert
  • Fonction : Auteur
  • PersonId : 977713
M. Delbo
K. Dohlen
L. Jorda
P. Vernazza

Résumé

We present THERMAP, a mid-infrared 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 microbolometer arrays, 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 \textgreater 60 in the spectral range 9-13 mu m where most emission features occur.

Dates et versions

hal-01440673 , version 1 (19-01-2017)

Identifiants

Citer

O. Groussin, J. Licandro, J. Helbert, J. L. Reynaud, P. Levacher, et al.. THERMAP: a mid-infrared spectro-imager for space missions to small bodies in the inner solar system. Experimental Astronomy, 2016, 41 (1), pp.95--115. ⟨10.1007/s10686-015-9475-9⟩. ⟨hal-01440673⟩
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