Sabatier Reactors (Methane Production up to 96% efficiency)
(CFM p155)
36cm x 5cm dia filled with Ru Ruthenium or Ni Nickel
Nichrome heating wires
Condensing system to separate H2O from CH4 and CO
Condensing system to separate CH4 from CO
Exothermic reaction starts and sustains at 400 degrees Celsius
3CO2 + 6H2 => CH4 + 2CO + 4H2O
Condense out 4H2O
Condense out CH4
When the H2O is electrolyzed and the H2 is cycled back into the reactor while the O2 is trapped in it’s tank, this yields a 4:1 CH4 to O2 ratio and an over all 18:1 for CH4 to H2 (seed quantity brought from earth).
The remaining CO is available for other uses.
http://advlifesupport.jsc.nasa.gov/documents/simaDocs/MSAD-01-0221.pdf4H2 + CO2 = CH4 + 2H2O DH= -40 kcal/mole (1)
Reaction (1), known for over a century as the "Sabatier reaction," is highly exothermic and has a large equilibrium constant (~109) driving it to the right. It occurs spontaneously in the presence of either a nickel or ruthenium catalyst (nickel is cheaper, ruthenium is better) at temperatures above 250 C. (Typical reactors operate with peak temperatures around 400 C in the forward reaction zone, declining to 200 C at the exit.) Because of the high equilibrium constant and high reaction rate when properly catalyzed, yields over 90% are readily obtained even with very small reactors. Reaction yields of 96% have been achieved in the Lockheed-Martin machine at stoichiometric mixture ratios, and 99.9% conversion rates of lean reagents have been achieved at non-stoichiometric mixture ratios17.
The methane and water produced by reaction (1) are easily separated in a condenser. The methane is then liquefied and stored, while the water is electrolyzed in accord with:
2H2O = 2H2 + O2 DH= +57 kcal/mole (2)
The oxygen so produced is liquefied and stored, while the hydrogen is recycled back into the Sabatier reactor to produce more methane and water, and so forth.
It will be noted that reaction (2) only produces two hydrogen molecules to recycle back to reaction (1), which requires an input of four hydrogens. Thus a net input of hydrogen is required to make the system run. This could, in principal, be acquired on Mars at large energy cost by condensing it out of the atmosphere1,18 in a relatively simple automated system, or mined from Martian permafrost with the aid of human explorers or a very advanced type of automated mining system. Alternatively, (and more practically for early missions) the hydrogen can simply be brought from Earth. In this case, the combination of reactions (1) and (2) will produce 12 kg of CH4/O2 bipropellant on Mars for every 1 kg of hydrogen imported.
The primary advantages of the SE system are simplicity, robustness, scalability, and energy efficiency. The Sabatier reactor is basically a simple steel pipe containing a catalyst bed, which can easily be scaled to support a mission of any size. For example, the Lockheed Martin unit demonstrated that a small Sabatier reactor 0.1 liter in volume would be sufficient to support the MSR mission propellant requirement of ~1 kg/day. Based on these results the entire Mars Direct manned mission propellant production could be done in three 10 liter pipe reactors. Operating at ~400 C with a filter to preclude catalyst poisoning by Martian dust, such reactors are basically bulletproof, especially since their small size makes it practical to support virtually any desired level of subsystem redundancy. Available water electrolysis units using solid polymer electrolytes are highly efficient (>90%) and extremely rugged, as they have been designed for nuclear submarine use with specifications that include resistance to depth charge attack. The power advantage of the SE system is illustrated in Table 1, which compares the achieved performance to date of the SE unit at Lockheed Martin with the best results from zirconia-electrolysis units at the University of Arizona. The results shown are for chemical process requirements only, since that is the only issue the University of Arizona machine addresses. It should be noted, however, that the power requirements for the gas acquisition to service the zirconia based system would be about 4 times greater than the SE system, because the zirconia system only removes one oxygen atom from each CO2 reacted, and only reacts about 46% of input CO2, while the SE system removes both oxygens from each CO2 and is more than 95% efficient.
The primary disadvantage of the SE system is the need to import hydrogen. This requirement is especially painful on the MSR mission, where the relatively small tank sizes employed increases the tank surface area/volume ratio, increasing heat-leak and thus boiloff, making transport of the required hydrogen to Mars difficult. The SE process, operating alone, produces 2 kg of oxygen for every one kg of methane. But the optimal mixture ratio to burn O2/CH4 in a rocket engine is not 2/1 but about 3.5/1, where an engine specific impulse as high as 380 s can be achieved. If the SE process is acting alone, the only way to achieve this mixture ratio is to throw away some of the methane produced. This drops the net propellant leverage actually achieved by the system from the theoretical 12/1 (propellant produced to hydrogen imported ratio) to an actual 10.3/1. Since the hydrogen required to produce 10.3 times its weight in CH4/O2 propellant actually occupies a volume equivalent to about 14 times its weight in CH4/O2 propellant, and at least 20% extra hydrogen will be needed at launch to allow for boil-off losses during flight to Mars, such limited leverage requires that the CH4/O2 tanks be drastically oversized if they are to be used to transport the required hydrogen feed stock. Oversizing the tanks to meet this requirement causes tank weights to increase, thereby increasing net propellant requirements, etc., with the net result being a severe negative impact on overall mission performance.
Thus we see that a simple SE system incorporating only reactions (1) and (2) cannot provide a really attractive Mars in-situ propellant production system. This situation changes, however, if a third reaction is introduced which allows the 3.5/1 mixture ratio to be achieved not by throwing away methane, but by adding oxygen. In this case, instead of the propellant production leverage falling from the theoretical SE 12/1 to 10.3/1, it rises to 18/1. Since this leverage is significantly greater than the density ratios of CH4/O2 bipropellant to H2 feed stock, this means that the hydrogen feed stock can be transported to Mars in the ascent vehicles propellant tanks, without any oversizing required. Put more simply, having a third, oxygen producing reaction available nearly doubles the propellant leverage of the SE system, and this doubling of performance is the difference between an attractive system and an inadequate one.
So, in short, what we need is an oxygen machine. The zirconia electrolysis nominally fits the bill, but as we have seen it is inadequate from a practical point of view, with power requirements greatly in excess of anything likely to be available on an MSR mission (a zirconia-electrolysis based MSR mission would need at least 5 RTG's, which are not to be had), and scalability problems that preclude use as a central technology for supporting a piloted Mars mission. What we need is a in-situ propellant production system that combines the simple steel-pipe reactor and high energy efficiency advantages of the SE system with the "infinite leverage oxygen machine" talking points of the zirconia-electrolysis approach. The only system that potentially meets these requirements is the reverse water gas shift (RWGS). In fact, as we shall see, a RWGS system may offer much more.