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Do we have any figures for how much oxygen is contained in the regolith? It appears to be hyper-oxidised, so we should get some oxygen from terraforming, but do we know how much?
It's not going to be enough for advanced plants, but enough for a slight ozone layer? Hmmm.
Use what is abundant and build to last
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Approximate composition of Martian Soil elements by mass
Data taken at the Viking 1 landing site.
oxygen 40 - 45 percentage by mass
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What's the decomposition temperature?
Dissociation energy per kg?
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I think he's talking about superoxides and perchlorates. Minerals like rock and clay won't decompose easily.
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Yes, I'm talking about the superoxides and perchlorates. It's going to be difficult to get life going in Martian soil unless they're removed, anyway.
I've had an idea for a probe involving a mirror that could answer those questions. It would basically focus sunlight to heat surface material, and use a spectrometer to measure whatever is produced in the plume at different temperatures.
If the first meter contains 1% easily liberated oxygen by mass... well, that's enough for about 1 mb of oxygen.Enough for some ozone to form, and possibly for higher plants to survive (though they'd need to be engineered for the low pressure and cold temperatures...).
Use what is abundant and build to last
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With a fine grain soil one could add hydrogen in a chamber full of the minerals high in oxygen and what would happen is water would be created on heating which when brought high enough would evaporate into steam to which we can then cool the vapor with the standard distallation process collecting it in another holding tank.
http://www.lpi.usra.edu/meetings/lpsc2013/pdf/2046.pdf
Mars In Situ Resource Utilization (ISRU) and Planetary ProtectionPlanetary
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Why not brute force evaporation?
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Energy source?
Power level used?
measured results?
properties of the "Rocknest" wind drift sand. The upper surface of the drift is covered by coarse sand grains approximately 0.02 to 0.06 inches (0.5 to 1.5 millimeters) in size. These coarse grains are mantled with fine dust, giving the drift surface a light brownish red color. The coarse sand is somewhat cemented to form a thin crust about 0.2 inches (0.5 centimeters) thick
http://www.nasa.gov/content/goddard/cur … ce-sample/
Inside SAM, the "fines"—the dust, dirt and fine soil—were heated to 1,535 degrees F (835 C).
The southern subpolar region is well described by a two-layer model, according to which a soil with a water content of up to 55% by mass lies under a relatively dry soil with a water mass fraction of 2% and a thickness of 15–20 g/cm2. The distribution of water in Martian regolith northern subpolar region is in good agreement with the homogeneous model and does not require invoking the more complex two-layer soil model. The water-ice content in the subsurface layer of the northern subpolar region reaches 53 % by mass.
We show that there are two regions with a relatively high water content near the Martian equator. These are Arabia Terra and the Medusae Fossae formation region southwest of Olympus Mons. In these regions, a lower layer with 9–10% of water by mass may underlie the upper layer of relatively dry material 30 g/cm2 in thickness. The “moistest” spot near the equator is at about 30° E and 10° N. Its lower-layer soil may contain more than 16% of water by mass.
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This topic by Terraformer seems due for a return to view ...
The text below is from an article in the local newspaper today.
It caught my eye because it describes a situation that is rare on Earth, but which will be normal on Mars.
Everyone living in a habitat, riding in a transport vehicle with habitat atmosphere, or wearing a Mars suit, will be dependent upon a constant, never-ending supply of Oxygen. They'll also be dependent in exactly the same way on a never-ending supply of potable water and nourishing food. In addition to all those items, they'll be dependent upon a constant, never-ending supply of energy.
It seems to me that taking up residence on Mars is not for the faint of heart.
(th)
Search for oxygen tank refills routine for Peruvians
By Mauricio Muñoz
The Associated Press
VILLA EL SALVADOR, Peru — In
the middle of what was once a sandy
desert, on the outskirts of Peru’s cap-
ital, a new routine has emerged for
many of the residents of the densely
populated city of Villa El Salvador.
With the lives of friends or relatives
at stake because of the new corona-
virus, people are spending their days
searching for a place to buy oxygen,
preferably without having to spend
their life savings.
(th)
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The reasons for Mars is that the solar winds can blow the atmospher at high altitudes away from the planet. The trailing wind behind the planets blocking of the suns energy then is pulled from it due to the gravity of the planet. The not having any radiational shielding belts to help with a static shield is the last for why Mars has so little air remaining.
Upper air heating is the enemy for planetary loss.
Mars losing its atmosphere at a faster rate
So mars needs several things to combat the rates or it going into space....
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For SpaceNut re #10
Thanks for giving this topic a boost ... I'm hoping Calliban will be interested in the question I posed. It would definitely be interesting to see how many tons of Oxygen and Nitrogen would be needed to join the existing CO2 on Mars to yield a human-breathable atmosphere.
It would be interesting to learn what pressure the resulting mixture of gases would deliver at the surface, and if the partial pressure of Oxygen would be sufficient for humans to enjoy being out doors.
Naturally we can expect that the atmosphere will begin to waft away immediately after it is installed, but it would be interesting to learn the rate of loss to be expected. If a society is able to assemble the gases in the first place, then I would expect them to be able to replenish them as they are lost.
Edit#1: Another question related to the above is where the supply of gases might come from ... I would imagine comets would be a useful source of water from which Oxygen could be extracted, but Nitrogen (seems to me anyway) may be sourced from moons of various planets out-system from Mars.
Edit#2: Having NOT read the wealth of posts that are stored in the forum archive, I recognize that all these questions have probably been posed and answered before. This forum could use the services of a dedicated volunteer librarian who would go beyond my faltering efforts to try to tag interesting posts.
The forum could ** really ** use a permanent repository where items such as RobertDyck's recent restatement of his specifications for an optimum atmosphere for Mars and the Large Ship could be stored. It verges on ridiculous that RobertDyck, GW Johnson, kbd512 and other contributors have to keep repeating posts because of the flow-under-the-bridge nature of this medium.
At some point the resources and tools for permanent information storage may become available to members of this forum.
In the mean time, GW Johnson has shown and is showing how to use Wordpress as a permanent storage medium, but even his treasure trove of insights is not indexed.
(th)
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The half atmosphere of earth is a second target (7.35 psi) that we should head for after the first of partial pressure of approximate 3.0 psi.
Robert has calculated both gas mixes.
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For SpaceNut re #12 .... Bravo! You're right of course!
The amount of inert gas needed is NOT as great as I had originally imagined ...
If the habitats are fine at 1/2 Earth pressure at sea level, then the entire planet certainly should be.
Hopefully Calliban will be back with figures for the inputs needed to achieve the habitat equivalent atmosphere as specified by RobertDyck.
(th)
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Mars much like earths is a 2 sphere calculations in which the volume is the mass of the air we feel at the inner in PSI with regards to the height of the air column pushing down on the planets surface.
https://en.wikipedia.org/wiki/Boyle's_law
https://en.wikipedia.org/wiki/Charles%27s_law
https://en.wikipedia.org/wiki/Dalton%27s_law
Mars has a diameter of 4,222 miles (6,794 km), but from pole to pole, the diameter is 4,196 miles (6,752 km). Mars’ radius is, of course, half of planet’s diameter.
What is the easiest way to calculate the earth's atmospheric weight?
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According to this reference: 'Perchlorate (ClO4−) is widespread in Martian soils at concentrations between 0.5 and 1%. At such concentrations, perchlorate could be an important source of oxygen, but it could also become a critical chemical hazard to astronauts. In this paper, we review the dual implications of ClO4− on Mars, and propose a biochemical approach for removal of perchlorate from Martian soil that would be energetically cheap, environmentally friendly and could be used to obtain oxygen both for human consumption and to fuel surface operations.'
https://www.researchgate.net/profile/Al … 000000.pdf
Sounds good. The perchlorate is mostly in the form of calcium perchlorate, Ca(ClO4)2. This has a molar mass of 239, of which 128g is oxygen. Assume that Martian regolith has a bulk density of 2000kg/m2 and that 0.5% (on average) is perchlorate. That is an average of 10kg/m3. If we could fully reduce the perchlorate into calcium chloride and oxygen, then the top 1m of regolith, would release 5.4kg of oxygen per m2 of surface. If we could do that globally, it would add 0.2mbar of oxygen to the Martian atmosphere.
The regolith is between 5-10m in depth.
https://en.m.wikipedia.org/wiki/Martian_soil
If it all contains perchlorate at the same concentration as the surface, then it complete decomposition would add 1.5mbar of oxygen to the Martian atmosphere. Certainly enough to get terraforming started and a useful resource for future colonists. Perchlorates are sometimes used on Earth to produce oxygen candles, which burn to generate oxygen in enclosed spaces where easy replenishment of atmospheric oxygen is not possible (I.e submarines). It could also be used to manufacture solid rocket propellant and explosives.
Last edited by Calliban (2021-01-24 03:19:50)
"Plan and prepare for every possibility, and you will never act. It is nobler to have courage as we stumble into half the things we fear than to analyse every possible obstacle and begin nothing. Great things are achieved by embracing great dangers."
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These posts are oxygen pressure mixes from the Large scale colonizing
Total: 7.348 psi total
2.7 psi O2, 3.5 psi N2, 1.148 psi Ar
2.7 psi O2 + 3.5 psi N2 + 2.074 psi Argon = 8.274 psi total.
MCP suit partial pressure
Mount Everest partial
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If we could fully reduce the perchlorate into calcium chloride and oxygen, then the top 1m of regolith, would release 5.4kg of oxygen per m2 of surface. If we could do that globally, it would add 0.2mbar of oxygen to the Martian atmosphere.
This would result in a significant reduction in UV reaching the surface. Improves the lifespan of our plastic roofed gardens and farms. Also, reduced UV means methane, a potent greenhouse gas, will survive far longer. Mars currently emits 270 tonnes a year iirc, but maybe we can help that process along. Even in our oxygenated atmosphere it lasts on average 12 years before being oxidised, so i don't expect the small trace of oxygen here to make increasing its concentration difficult.
It may be that a self sustaining ecosystem with breathable air is not something we can achieve, due to the need for large amounts of biogenic greenhouse gases that would be destroyed if thet much oxygen were present. But maybe we can sustain ecopoiesis. I'm quite happy with that, humans can build vast habitats and paraterraform sections.
Last edited by Terraformer (2024-07-04 18:41:05)
Use what is abundant and build to last
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"Thermal Decomposition of Calcium Perchlorate/Iron-Mineral Mixtures: Implications of the Evolved Oxygen from the Rocknest Eolian Deposit in Gale Crater, Mars"
https://ntrs.nasa.gov/citations/20140012600
A major oxygen release between 300 and 500 C was detected by the Mars Curiosity Rover Sample Analysis at Mars (SAM) instrument at the Rocknest eolian deposit.
So all we have to do is... heat the regolith to between 300 and 500 degrees celcius.
Use what is abundant and build to last
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The temperature range is why I chose that for the getting water from the top level of soil on mars as there was going to be a bonus of gathering co2 + oxygen along with the water that would bake out.
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