FROM SOLAR FUELS TO OXYGEN PRODUCTION ON MARS
20 November 2019
20 November 2019
Contatti:
Dipartimento di Fisica, Segreteria
via Sommarive, 14 - 38123 Povo (Trento)
Tel.
+39 0461 281504 - 1575 - 2042 - 1545
Fax
+39 0461 281696
Venue: Polo Ferrari 2, via Sommarive 9 - Room B103
At: 14:30
Prof. Vasco Guerra – Instituto de Plasmas e Fusao Nuclear (IPFN) - Instituto Superior Técnico Lisboa
Abstract
There is a renewed interest on CO2 plasmas nowadays, as their activation by selective excitation of the asymmetric stretching vibrational mode may enhance dissociation and favour CO2 conversion at a low energy cost.
This CO2 reforming process takes advantage of the so-called vibrational (V-V) up-pumping mechanism and can be tuned to the production of solar fuels on Earth or to the oxygen and rocket fuel production on Mars.
The current status of research on Earth and the similarities and differences with the application to Mars are discussed.
Scientific Coordinator:
prof. Paolo Tosi
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