Quote from: Ace on 08/23/2019 11:50 pmAnother chemical reaction worth noting:Olivine (Fe,Mg)SiO4 has been reported as being a common component of Martian regolith in the form of basalts, at least in the Southern Highlands. Olivine is an igneous, ultramafic or mafic mineral that's also readily available on Earth, either in aphanitic (small crystals) form as a basalt, or phaneritic (larger crystals) as peridotite or gabbro.The interesting part is that when olivine is mixed with H2CO3 (carbonic acid), it forms oxygen gas and water. Carbonic acid is easy to make by bubbling CO2 through water. The reaction would allow you to recycle the water, while also generating oxygen. Should take a lot less energy than electrolysis.The downside is that you still need hydrogen for the Sabatier process, which suggests olivine might be best used as a secondary oxygen source -- but even in that role, it could still be very useful.That's interesting; if you could find methane on Mars, it might be the cheap way to get oxygen to go with it?However, a bit of digging suggest the rate may be quite slow, and the amount of carbonic acid held in water quite small? Catalysts perhaps? This does sound a bit too magical, if it was that simple, there would be no CO2 problem and therefore no global warming problem....
Another chemical reaction worth noting:Olivine (Fe,Mg)SiO4 has been reported as being a common component of Martian regolith in the form of basalts, at least in the Southern Highlands. Olivine is an igneous, ultramafic or mafic mineral that's also readily available on Earth, either in aphanitic (small crystals) form as a basalt, or phaneritic (larger crystals) as peridotite or gabbro.The interesting part is that when olivine is mixed with H2CO3 (carbonic acid), it forms oxygen gas and water. Carbonic acid is easy to make by bubbling CO2 through water. The reaction would allow you to recycle the water, while also generating oxygen. Should take a lot less energy than electrolysis.The downside is that you still need hydrogen for the Sabatier process, which suggests olivine might be best used as a secondary oxygen source -- but even in that role, it could still be very useful.
Silly basic questions here. There are clearly deposits of mostly-water at the poles, but if you want to use solar power you definitely don't want to be at the poles. Are there known deposits of high-quality "water ore" at latitudes with reasonable insolation? If not, what are some options if you want to extract water from some lower-quality ore such as a hydrate mineral, and are there some reasonable deposits of those near the equator? I've done a little research but not found anything clear-cut on these issues.
High areas around the poles are where you definitely want to be for Solar Power on the moon. You get better than every other fortnight insolation. If you are very near the pole only a few stations will keep you having one always in Sun and there is no air to attenuate at low angle.
...a methane plant on the moon would need a source of carbon dioxide
Quote from: wannamoonbase on 08/23/2019 12:47 pmI’ve thought for years that SpaceX would be wise to start testing sabatier hardware by making their own fuel for Raptor and SS/SH. Get some solar panels from Tesla build a couple reactors and start will some veto tanks at the launch sites.Yes, absolutely! There's no reason basic reactor flow and function shouldn't be ironed out on Earth long before use on Mars. Issues such as operating at scale are likely to present significant engineering challenges.
I’ve thought for years that SpaceX would be wise to start testing sabatier hardware by making their own fuel for Raptor and SS/SH. Get some solar panels from Tesla build a couple reactors and start will some veto tanks at the launch sites.