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Detection of water ice on comet 67P/C-G

Detection of water ice on comet 67P/C-G


Date: 23 September 2015
Satellite: Rosetta
Depicts: VIRTIS spectra of Hapi region on comet 67P/C-G
Copyright: ESA/Rosetta/VIRTIS/INAF-IAPS/OBS DE PARIS-LESIA/DLR; M.C. De Sanctis et al. (2015)

Spectra of Comet 67P/Churyumov-Gerasimenko taken at infrared wavelengths with Rosetta's Visible, InfraRed and Thermal Imaging Spectrometer, VIRTIS, in September 2014.

The black spectrum corresponds to a patch of the comet surface that was well illuminated at the time of the measurement; the red spectrum corresponds to a less-illuminated patch; and the blue spectrum to a patch of the comet surface that was cast in shadow.

The black spectrum shows a weak dip between wavelengths of 2.8 and 3.6 micron, which is produced by organic compounds on the surface absorbing the comet's thermal radiation.

The shape changes gradually from the black to the red and then the blue spectrum. In the blue spectrum, the dip is much stronger and shifted towards shorter wavelengths (2.7 to 3.6 micron), showing the characteristic shape of an absorption feature caused by water ice on the surface.

The three spectra demonstrate that water ice is only found on patches of the comet that are cast in shadow, suggesting a cyclical behaviour of water ice during each comet rotation.

Last Update: 1 September 2019
10-Jul-2020 09:31 UT

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