Inside a comet’s nucleus
“The light molecules identified in the dust clouds around comets make us think there could be much more complex molecules in comet nuclei,” says Hervé Cottin from the LISA* inter-university laboratory for the study of atmospheric systems in Créteil.
“Such molecules could well have contributed to the appearance of life on Earth.”
“The principle of AMINO is to expose organic molecules to solar radiation so we can understand the surface or atmospheric chemistry of other objects in the solar system, like comets, meteorites, Mars and Saturn’s satellite Titan,” enthuses Hervé Cottin. “It’s an important experiment for exobiology.”
Lift-off at 1.38 p.m.
Uvolution, the 1st experiment of this type led by LISA, was performed in space inside a Foton capsule in September 2007. This experiment showed that UV radiation from the Sun could significantly alter organic molecules like certain amino acids.
The PROCESS experiment, installed outside the European Columbus laboratory until May 2009, will teach us more about these chemical reactions.
Wednesday 26 November, at 1.38 p.m. CET, AMINO lifted off to the ISS with a new complement of molecules to be tested.
It was launched on board a Progress ISS resupply ship atop a Soyuz booster from the Baikonur Cosmodrome in Kazakhstan.
Prepared by LISA, CNRS’s aeronomy research laboratory, the CBM molecular biophysics centre in Orléans and the Jacques Monod Institute, with support from CNES, the AMINO experiment is scheduled to run for 18 months.
* Laboratoire Interuniversitaire des Systèmes Atmosphériques