Abstract:Herein, it is argued that Mars has nearly ideal conditions for CO 2 decomposition by nonequilibrium plasmas. It is shown that the pressure and temperature ranges in the 96% CO 2 Martian atmosphere favour the vibrational excitation and subsequent up-pumping of the asymmetric stretching mode, which is believed to be a key factor for an efficient plasma dissociation, at the expense of the excitation of the other modes. Therefore, gas discharges operating at atmospheric pressure on Mars are extremely strong candid… Show more
“…A radically different and new approach to the question, proposed very recently, would be to use low-temperature plasmas [2]. The new results were obtained by simulations made at the N-PRIME team of IPFN (Instituto de Plasmas e Fusão Nuclear, Instituto Superior Técnico, Universidade de Lisboa, Portugal) [2,7] and are supported by experiments made at LPP (Laboratoire de Physique des Plasmas, Ecole Polytechnique, Palaiseau, France) and TU/e (Technische Universiteit Eindhoven, The Netherlands) in pulsed DC plasmas [8]. This early research focuses on the characterization and control of the degree of vibrational excitation, crucial to achieve an efficient plasma decomposition of CO 2 .…”
Sending a manned mission to Mars is one of the next major steps in space exploration.
Creating a breathable environment, however, is a substantial challenge. A sustainable
oxygen supply on the red planet can be achieved by converting carbon dioxide directly from
the Martian atmosphere. A new solution to do so is on the way: plasma technology.
“…A radically different and new approach to the question, proposed very recently, would be to use low-temperature plasmas [2]. The new results were obtained by simulations made at the N-PRIME team of IPFN (Instituto de Plasmas e Fusão Nuclear, Instituto Superior Técnico, Universidade de Lisboa, Portugal) [2,7] and are supported by experiments made at LPP (Laboratoire de Physique des Plasmas, Ecole Polytechnique, Palaiseau, France) and TU/e (Technische Universiteit Eindhoven, The Netherlands) in pulsed DC plasmas [8]. This early research focuses on the characterization and control of the degree of vibrational excitation, crucial to achieve an efficient plasma decomposition of CO 2 .…”
Sending a manned mission to Mars is one of the next major steps in space exploration.
Creating a breathable environment, however, is a substantial challenge. A sustainable
oxygen supply on the red planet can be achieved by converting carbon dioxide directly from
the Martian atmosphere. A new solution to do so is on the way: plasma technology.
A new approach to calculate the vibrational distribution function of molecules in a medium providing energy for vibrational excitation is proposed and demonstrated. The approach is an improvement of solution methods based on the drift-diffusion Fokker-Planck (FP) equation for a double differentiable function representing the vibrational populations on a continuum internal energy scale. A self-consistent numerical solution avoids approximations used in previous analytical solutions. The dissociation flux, a key parameter in the FP equation, is fixed using the kinetics of molecular dissociation from near-continuum levels, so that the vibrational kinetics becomes a functional problem. The approach is demonstrated for the kinetics of asymmetric stretching of CO, showing that it represents an alternative, potentially much more efficient in computational terms, to the presently usual state-to-state approach which is based on the kinetics of the populations of individual levels, and gives complementary insight into the dissociation process.
“…These include (a) reducing membrane thicknesses another order of magnitude using W mesh‐reinforced Ag foils 2.5 μm thick, (b) microporous substrates on which a pin hole free thin film of Ag would serve as the membrane (<1‐μm thickness), (c) adapting planar plasma glow discharge technology for reductions in voltage enabled by micrometer‐scale electrode gaps (Go & Pohlman, ), and (d) exploring pulsed power plasma techniques under development at the University of Lisbon. Pulsed power plasmas will be applicable to this approach to further reduce the energy budget (Guerra et al, ). Pulse widths 5 ms on and off to create plasmas that are more efficient in dissociating CO 2 have been reported (Silva et al, ).…”
A six Torr CO2 glow discharge in combination with a heated W mesh‐reinforced ultrathin Ag membrane is used to generate molecular oxygen. The Ag membrane is a commercially available 25‐μm‐thick Ag foil backed by a 25‐μm‐thick W electroformed mesh. The permeation flux is inversely dependent on the membrane thickness and exponentially dependent on the membrane temperature. Calculations show that a pressure differential of 1 atmosphere can be supported by the W mesh/Ag foil membrane at temperatures up to 350 °C. In this work, a glow discharge for pressures between 2 and 15 Torr CO2 and temperatures up to 500 °C were reported. The DC glow discharge was produced initially with a solid Ag rod cathode, 2 mm in diameter, and then with a 7‐mm‐diameter Ag rod machined into a hollow cathode, located 5 mm from, and normal to, the Ag membrane anode. The voltage was varied from 440 to 620 VDC with currents up to 41 mA. A stable flux of 1.61 × 1015 O2 molecules·cm−2·s−1 is observed for a membrane temperature of 450 °C and a CO2 pressure of 6 Torr. With ~4‐m2 surface area, this approach is competitive with the present mission qualified Mars Oxygen In‐Situ Resource Utilization Experiment (MOXIE) system planned by National Aeronautics and Space Administration (NASA) for the 2020 Mars rover mission which generates ≈12 g/hr O2. The proof of concept technique presented herein can be substantially improved by further reduction of the membrane thickness, refinement of the cathode, and glow discharge plasma.
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