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Small bodies can hold on to atmospheres for geological timescales if protected by an artificial magnetosphere
I agree a magnetosphere is a good idea, in fact Jupiter has a lot of radiation so you also need the magnetosphere to protect against that. Jupiter's strong magnetosphere collects radiation belts, great to protect Jupiter but bad for anyone in Jupiter's orbit. But if you terraform a planet, you really need to plan for more than just a few thousand years. There are limited resources on a planet, expending them just to be released into space is irresponsible. Terraforming has to be for the long-term, lasting millions of years if not hundreds of millions.
what would be the effect of solar UV on SF6? Would we find ourselves with an atmosphere of SO2 and hydrogen flouride after just a few centuries?
Good question. I checked, SF6 is inert toward oxygen, it takes a platinum catalyst to get them to react and a lot of energy. The abstract for this paper talks about electrical explosions of platinum, and temperatures above 5000°K.
http://stinet.dtic.mil/oai/oai?&verb=ge … =AD0680768I would also raise questions as to just how much rock is present on the surfcaces of Ganymede and Callisto. Is there actually enough material there to form a significant crust? I was under the impression that the surfcae of both worlds was icy, with small amounts of rock and dust present from meteorite fragments.
The visible surface is entirely rock, the belief that there's ice present is based on density calculated from gravity. In fact they don't have any direct evidence of ice on Ganymede or Callisto.
I've never been very keen on 'giant mirrors and lenses' in space. Where would the metal come from?
Jupiter's small moons, which are basically captured asteroids.
Maybe one way around this problem would be to engineer a ‘sub-zero’ ecosystem. The idea being to genetically modify plants to incorporate ammonia or some other anti-freeze within their cells and sap. The ecosystem could then function at sub-zero temperatures, with plants surviving in icy soils.
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If this proves possible, it would allow even the iciest of moons and trans-Neptune worlds, to be terraformed without melting their surfaces into global oceans.That works with temperatures just a couple degrees below freezing, so the antifreeze keeps water liquid. Ganymede's temperature currently is between 90°K and 160°K, that's -183°C to -113°C.
An interesting abstract on Callisto. The surfcae appears to be completely covered with rock and dust, with significant carbonaceous material also present.
You can terraform Ganymede and Callisto.
Europa has a pure ice crust about 7km deep, possibly as deep as 10km in places, which if melted would form a moon-wide ocean. Ganymede and Callisto have dirty ice about 500km deep inferred by gravity and density, with a rocky surface. Surface conditions of those two moons could be controlled to provide temperate conditions. After all, the Earth is 12,750km in diameter with a crust 24km thick; beneath that is magma. If the Earth can have a cold surface with ice insulated by a few kilometres of rock, then Jovian moons could have a temperate surface with cold ice interior insulated by rock and dirt.
Maybe one way around this problem would be to engineer a ‘sub-zero’ ecosystem. The idea being to genetically modify plants to incorporate ammonia or some other anti-freeze within their cells and sap. The ecosystem could then function at sub-zero temperatures, with plants surviving in icy soils.
The world would be artificially illuminated with ultraviolet light and the higher end of the visible spectrum, to deliver a maximum of photosynthetically available light, without raising the temperature of the world above freezing.
If this proves possible, it would allow even the iciest of moons and trans-Neptune worlds, to be terraformed without melting their surfaces into global oceans.
You can terraform Ganymede and Callisto.
Since Jovian moons are in orbit around Jupiter, their mean distance from the sun is the same. That is 5.2028 times the Earth's distance. The inverse square rule means they receive 1/27.06912784 as much sunlight per unit area as Earth, twilight. That's damn little, but it can be augmented. A series of concentric ring in polar orbit, connected and providing mutual support, can form a parabolic mirror. The centre of the parabola will be shadowed by the moon so it would be cut out. The rest of the parabola would have more depth than the diameter of the moon. This prohibits satellites, but would dramatically increase light. With a parabola diameter 3 times the diameter of the moon, total light gathering area including the planet itself will be 9 times the surface area. This will increase solar energy to 9 times current. That would still be 1/3.00768 per unit area that of the Earth, but sufficient. The planet would be brighter than an office except for a brief night when passing through the circle that doesn't receive reflected light. It's a big engineering project, but possible.
Europa has a pure ice crust about 7km deep, possibly as deep as 10km in places, which if melted would form a moon-wide ocean. Ganymede and Callisto have dirty ice about 500km deep inferred by gravity and density, with a rocky surface. Surface conditions of those two moons could be controlled to provide temperate conditions. After all, the Earth is 12,750km in diameter with a crust 24km thick; beneath that is magma. If the Earth can have a cold surface with ice insulated by a few kilometres of rock, then Jovian moons could have a temperate surface with cold ice interior insulated by rock and dirt.
The greater problem is holding on to an atmosphere. Ganymede has a surface gravity 0.146 Gs, Callisto has 0.127 Gs, and Europa has 0.13 Gs. An atmosphere of xenon would stay put, the question is where to find enough of it. Sulphur hexafluoride (SF6) is an even heavier gas, Io has plenty of sulphur but I don't know the abundance of fluorine. Xenon density is 5.894 g/L, SF6 is 6.164 g/L, nitrogen is 1.251 g/L and oxygen is 1.429 g/L. SF6 is also the strongest greenhouse gas we know, is highly inert, quite safe. It sublimes at -63.9°C. Unlike many other sulphur compounds, it's colourless and odourless. Solubility in water is low, so it wouldn't dissolve in an ocean.
Small bodies can hold on to atmospheres for geological timescales if protected by an artificial magnetosphere, see:
http://newmars.com/forums/viewtopic.php?t=5339
Even on a very small body, the entire atmosphere will not flash into space immiediately, but will slowly 'evapourate' from the top down. Only molecules able to achieve a free path, will be able to succesfully escape. This condition only applies to ions at the top of the ionosphere (exosphere). If the world is supplied with a powerful artificial magnetic field, the atmospheric ions would be recycled continuously, spirally down the field lines until they re-enter the atmosphere at the poles. This way, even relatively small bodies can retain synthetic atmospheres for geological timescales, although for bodies with surface gravity of less ~1% Earth, the amount of gas needed to produce an acceptable surface pressure becomes excessive.
I like the idea of using a strong greenhouse gas as a major atmospheric constituent. But what would be the effect of solar UV on SF6? Would we find ourselves with an atmosphere of SO2 and hydrogen flouride after just a few centuries?
As regards the use of mirrors, there is presumably a point, as one moves to bodies further from the sun, where it becomes more economic to artificially illuminate using a thermonuclear power source, rather than attempt to reflect the light of the sun.
I would also raise questions as to just how much rock is present on the surfcaces of Ganymede and Callisto. Is there actually enough material there to form a significant crust? I was under the impression that the surfcae of both worlds was icy, with small amounts of rock and dust present from meteorite fragments.
Condition 1: Precise atmospheric composition.
Second, the Earth had to be large enough to hold a strong magnetic field and active geology for billions of years, yet small enough and outside of the star's hot zone to avoid accumulating a hot, dry, dense atmosphere like Venus, or excessive volcanism that would plague a larger than earth terrestial planet.
Condition 2: precise size and distance from star.
Condition 3: Jupiter. Without a massive planet at about the right distance from the sun, the Earth would be slammed by comets on a regular basis.
Condition 4: A large moon. Our moon is very large, compared to its planetary companion. Lunar is as large as the moons of jupiter, a planet 300 times as heavy, and it formed under very unique conditions. Without it, the Earth's axial tilt would be unstable and it would be subject to frequent and very intense climatic swings.
Condition 5: A stable star. Only 15% of stars are as stable as our sun, most exhibit much more intense and frequent flaring activity, that would lead to climatic swings and would compress most planetary magnetic fields, leading to steady errosion of planetary atmospheres.
These helped us become exactly like we are, but I doubt they're a necessity for complex, intelligent life. Just complex, intelligent life very similar to us.
For instance, a less stable star isn't so bad if it's really long lived. If we had been a few billion years late, we'd be cooked. A red dwarf that has trillions of years of life in it would be quite a luxury for any multi-cellular life to develop. Considering the amount of red dwarfs out there, it seems like a safe bet that they'll have most of the life we find.
I don't buy this. If it were true, we would have expected a different intelligent species to have evolved on Earth, aeons before we did.
Also, the fact remain that if ET had evolved elsewhere in our galaxy even a short time ago by geological standards, they would have colonised every habitable star system in our galaxy by now. Their radio signals would be everywhere. Their space junk would be littered throughout our solar system. Also, how would they spontaneouly die out, if they had already colonised their solar systems or multiples of other solar systems?
The observations that we are seeing only make sense if we assume that ours is the only advanced technological society to have evolved in our galaxy, or none of the others were succesful in colonising space to a significant degree and thus, have not survived in any evident form.
You know your cat though. How many stray cats have you ever talked to?
The gulf of intelligence is likely to be the other way around. The more we learn about the Earth, the more we learn just how special it is and how small variations in certain attributes would render it unsuitable for complex, intelligent life.
Consider the following: For 90% of the Earth's existence it has held life, but for the first 4billion years, that life was single cellular and primitive. Multicellular life did not evolve until about 500 million years ago and the first land plants apperaed a few hundred million years ago. No-one knwos why, but it is suspected that a high concentration of oxygen in the atmosphere and low concentration of CO2, was a prerequisite for allowing multicellular metabolism.
Condition 1: Precise atmospheric composition.
Second, the Earth had to be large enough to hold a strong magnetic field and active geology for billions of years, yet small enough and outside of the star's hot zone to avoid accumulating a hot, dry, dense atmosphere like Venus, or excessive volcanism that would plague a larger than earth terrestial planet.
Condition 2: precise size and distance from star.
Condition 3: Jupiter. Without a massive planet at about the right distance from the sun, the Earth would be slammed by comets on a regular basis.
Condition 4: A large moon. Our moon is very large, compared to its planetary companion. Lunar is as large as the moons of jupiter, a planet 300 times as heavy, and it formed under very unique conditions. Without it, the Earth's axial tilt would be unstable and it would be subject to frequent and very intense climatic swings.
Condition 5: A stable star. Only 15% of stars are as stable as our sun, most exhibit much more intense and frequent flaring activity, that would lead to climatic swings and would compress most planetary magnetic fields, leading to steady errosion of planetary atmospheres.
There are probably even more conditions that make the earth special, without which intelligent, complex life and a civilisation could not have evolved.
The impression that these facts tend to create is that primitive life is probably everywhere, advanced life is probably very rare. There may be an intelligent civilisation with 100 light-years of earth. I may win the lottery next week!
One obvious point occures to me, if a civilisation had evolved elsewhere in our galaxy in the past, then given the age of the universe, wouldn't they have litterally conquered the galaxy by now? How come they havn't colonised our solar system long ago and how come the galaxy isn't awash with interstellar communication? If even one advanced civilisation had evolved and become space faring as little as 1 million years ago, we would expect them to be everywhere by now. This suggests that we are the first spacefaring civilisation to have evolved in this galaxy.
Electrified railways would seem like a good bet.
Attempting to power vehicles with chemical fuels derived from electricity produced by nuclear reactors, would be very expensive. This is due to the poor overall energy efficiency of the process and the simple fact that power sources must be transported from Earth.
For initial Mars missions this is tollerable given the overall cost of the mission and the modest initial transport requirements. As soon as we start looking at transporting people and materials on a large scale, the cost will begin to look burdensome.
Fitting a nuclear reactor within a train would run into problems of power-to-weight ratio, although it could be made to work in principle.
To power a train with electricity is easy - you just lay an extra (third) rail.
Railways have clear advantages over road vehicles in long-term economics. When you are paying through the nose for energy produced by imported nuclear reactors or home-made solar panels and wind-turbines, energy efficiency matters.
Given Venus's hostile environment, relatively deep gravity well and general lack of anything exceptional that it might export, I would anticipate that this will probably be a deadzone for future human colonization.
We have an entire other thread for this. Feel free to bring this up there, since you haven't yet. I've already spent a lot of time developing my case for Venus, and there's plenty more I haven't discussed yet.
Although if you want to talk about 'costing too much', you're on the wrong forum. Terraforming any planet is going to be incredibly expensive. We can't even imagine the costs properly. Every planet is a gravity well. Terraforming Mars at all would seem completely without economic merit, compared to mining all the low-gravity bodies, ignoring the neighboring planets, and calling it a day.
Sure, we could discuss terraforming from the point of view of having infinite money, resources, technologies unbounded by the laws of physics, etc. Then we would be gods, by any measure.
In the real world, whether it be the world of today or the solar system 5000 years hence, cost (in terms of required resources) and investmnet timeframe, are always going to be important. These hark back to basic laws of nature, they are not simply constructs of short-sighted capitalism.
We need to have some measure of reality in these discussions, for there to be any point having them at all.
In all terraforming scenarios the viability of a project = f(value of terraformed land/cost x return timeframe).
At some point it becomes easier simply to build your own world and craft it as you please.
I think the purpose of any sort of floating base would be primarily for terraforming. Nothing manned would be needed. Just automated facilities that grow and release bacteria that can sequester the thick CO2 atmosphere.
I wonder if it would be possible to set up a base on Maxwell Mount's summit (tallest mountain on the planet). It would be subject to far less atmosphere than the lower areas. Depends on the temperature.
Terraforming Venus with algae/bacteria is a dead duck from the start. What are you going to do with the trillions of tonnes of carbon and oxygen within the atmosphere? And where do you plan to get sufficient hydrogen and mineral trace elements to sustain the bacteria? Even if it were possible to reduce the carbon through organic processes, you would still be left with an atmosphere containing 60 bars of atomic oxygen and a mass of carbon sufficient to cover the planet to a depth of a hundred metres. Not an easy problem to solve.
The only plausible solution as far as I can see would be to completely block out the sun from the planet, allow it to cool to cryogenic temperatures (beneath the freezing point of nitrogen) and then simply fire the solidified CO2 into space electromagnetically.
It is uncertain who would want to undertake such a project and why. The cost of such large scale planetary engineering would be gigantic, the investment timescale measured in centuries or millenia, and unlike Mars, it would be impossible to terraform Venus in an easy and incremental way. If the solar system started running short of carbon in some distant point of the future, it might be possible to justify mining the Venusian atmosphere, with a potentially terraformed world as a long-distant side benefit.
From a financial viewpoint, it would be preferable to build a several thousand large O'Neill colonies, providing an equivelent surfcae area to Venus.
Maybe a 1 bar atmosphere won't be neccesary for Mars. On skylab, the crew survived perfectly well in a 1/3rd bar atmosphere, two-thirds oxygen, one third nitrogen.
The idea of decaying cometary objects in orbit is much better than slamming them into the surface. If Mars can be given a significant magnetic field, then the sun can do the hard work of breaking down the ammonia and water into breathable oxygen/nitrogen.
The most important hurdle in terraforming Mars is getting it to the point where it can support advanced plant life in open air. Once that is achieved, we can grow crops outside of domes, which massively improves the economics of habitation.
What would be the best way to start a continous human presence on Mars?
I presume expanding from the infrastructure (energy, rovers, drills, hab?) which will already be present on the surface after a succesful DRM-III type first mission is a good way to start, rather than setting up from scratch in a new location.What would your favorite Mars bases look like within, say, a 10 year time frame with this starting point?
A Gerard O'Neill type Near-Earth satellite power programme, would seem like the most realistic way to go, if you were looking to send a large number of people to Mars, with the sort of infrastructure needed for permanent colonisation.
Anything other than small-scale exploration would be very difficult if launched direct from Earth, due to mass requirements.
I would guess that medium-term Mars settlements would be subsurface, brick-built structures, with small surface domes for agriculture. probably quite cramped, rather like Antarctic research stations.
One of the problems is that some terraforming options are only really available before major settlements are established. For example, if you want to smash ammonia asteroids into Mars, you should probably do it when there are no people there.
Also, say you wait 200 years before raising the temperature enough to melt ice and create oceans. What about the people who own land (now for generations) in the areas that will be flooded? A dozen special interests will develop over 200 years that will lobby to halt the deluge. Buying them out might be your biggest terraforming expense.
True. You would probably end up displacing entire cities, maybe even entire new nations!
Some form of terraforming would appear desirable at an early stage on Mars. The present atmosphere is too thin to provide any plausible shielding against cosmic rays or solar flares and may even aggrevate the situation by breaking down into secondary particles.
Also, thickening the atmosphere could be accomplished relatively easily, with half a dozen CFC producing nuclear-powered factories on the surface. As soon as major flourine/chlorine salt mineral beds are identified, the factories could be shipped up from earth at an acceptable cost and landed enpiece at the location of the mineral bed. The atmosphere could be substantially thickened within a few decades, at an affordable price.
Again, there are strong economic imperitives, for the simple reason that the value of the land increases dramatically if radiation levels go down and especially if hardy food crops can be grown outside of man-made structures. The cost is affordable and the results are near-term enough for the project to be taken seriously.
Shifting large asteroids and producing a breathable atmosphere are longer term options that are probably unrealistic as conscious projects by any government. They are also unneccesary, given that humans can create a comfortable environment relatively cheaply and incrementally using plastic domes.
Mars will be paraterraformed long before any serious planetary terraforming is attempted.
Yes, I'm creating a second thread when the first one is still active, kind of. I'm a bad, bad man who must be punished most severely. Be that as it may, brief notes written in reply to lengthy queries have a way of being lost in the shuffle when the threads go off on extended tangents, like the one about planetary migration.
Let's focus this one a little more narrowly. We've presented with the almost poetic image of cities floating in the Venusian atmosphere, I guess slowly drifting downward as centuries or millenia of terraformation convert a Carbon Dioxide atmosphere into a Nitrogen-Oxygen one, the cities coming down to a new earth out of a new heaven (and don't ask me where the Nitrogen is coming from, because I have no idea). A few Christian fundamentalists might be absolutely intrigued by the parallel with the image of the new Jerusalem in Revelations, but as much fun as we could probably all have with the subject of the cultural implications of all of this, one can possibly shoot the idea down in one word.
Convection.
The heat engine on Venus is going to be a lot more powerful than the one on earth, and I have to wonder what is going to happen to one of those floating cities when it floats into a downdraft. Yes, it has bouyancy pushing it back up, but one can say the same of any unfortunate swimmer who gets himself caught in an undertow. He still goes down. Any reputable studies done of how much force our meterological undertow (convection powered downdrafts) would place on those bobbing cities, and how far down one of those cities might drop?
In the Mars vs. Venus vs. Titan competition, this strikes me as being a good reason to favor Mars. Yes, Mars can get very, very cold, BUT one can build underground. In fact, given the reality of radiation levels on the surface pre-terraformation, one would probably have to do so. Rock makes an excellent thermal insulator, so even if the surface is frigid, it doesn't follow that a great amount of energy will be needed to keep a subsurface habitat warm, or that a power failure would rapidly throw everybody into the deep freeze. There would be the difficulty of getting sunlight down to any gardens beneath the surface, but if one is willing to build parasols the size of planets, building a series of reflectors to concentrate and collimate sunlight and then bounce a few ferocious sunbeams underground would seem to be a trivial enterprise by comparison.
One which, by the way, might very well be practical with present-day technology, or something very close to it, unlike that planetary parasol. The beauty of one's Martian burrow is that one doesn't have to worry about where it's going to go. Out of these three choices, my vote would definitely be for Mars.
I think the downside of any scheme for a floating Venus city is the same as many other schemes suggested on this forum. It is difficult to imagine why any government or private group, would go to the trouble or expense of creating them.
For colonising the moon there is a clear commercial imperitive; the export of materials to construct solar power satellites and orbital colonies for Earth. These are things that the moon can export and that people will pay for. It would appear a little far-out to most people, but there is at least a plausible mechanism through which it would happen and that would allow a lunar colony to pay for its imports. The same is true for Near Earth Asteroids.
For Mars, the commercial imperitive is weaker, due to its heavier gravity, atmosphere and distance from Earth, but it is still likely that following heavy colonisation of near-Earth space, independant groups would travel to Mars and set up home at some point in the late 21st or early 22nd century. Mars has enough accessible resources and a comfortable enough surfcae environment to allow the colonies to be relatively independant of outside support, beyond a certain critical size.
None of these arguements appear to apply for a floating colony on Venus. It's thick, poisonous atmosphere and deep gravity well, make it difficult to escape from; there is no plausible export that it could provide that could not be provided by the asteroids at a far lower energy cost and there is no realistic hope of terraforming it with any technology that we can presently contemplate. It would remain critically dependant on outside imports, with no plausible export to pay its way and would be a precarious structure at best, with difficult engineering requiremnets.
Someone once said there are two kinds of people in this world -- those who divide everyone into two kinds of people and those who do not.
So let's talk about planets and moons. There are two kinds of world in this solar system -- those with atmospheres and those without. Earth, Venus, Titan and Mars are With. Luna, Ceres and the Jovian Moons are Without. Each kind presents its own group of problems, but, on the whole, With is a lot easier to work with than Without. If we insist on going Without, then let's begin with Luna, but, if we cannot get Luna right, then there's no sense in talking about Ceres or Europa or Ganymede or Callisto. Mars in its present condition is nearly Without, so if Mars is insurmountable, then all those truly Without are idle dreams.
In a related kind of way, there are two other kinds of world in this solar system -- those with heat and those without. Venus, Earth and Mars are With. Luna, Ceres, the Jovians and Titan are all Without, sometimes as a function of being airless and sometimes as a function of distance. Again, on the whole, With is a lot easier to work with than Without.
Let's use Earth as our analogy. What are the populations of Indonesia, India, Zaire and Brazil? Nearly two billion? Then what are the populations of Greenland, Spitzbergen and Antarctica? Some like it hot, but few love it cold. If Terran lifeforms have shown diminished attraction to polar conditions on Earth, then they will never take to those frigid little worlds out in space. Mars is at the limit in that direction, though under the ice on Europa is a slim possibility. Likewise, there is a greater variety of life under great pressures at the bottom of the sea and even deep within the rocks of the crust than there is floating in our atmosphere at low pressure. Heat and pressure quicken the pace and rhythms of life. Without these, the chemical reactions that power life slow and stop.
~~ Bryan
This makes sense. I know that many would argue that an icy terraformed world has long-term security advantages over a thin-shelled habitat, but in the short to medium term, an O'Neill type habitat is overwhelmingly attractive, in terms of initial cost and living conditions. It would appear to offer far more in terms of value for money. They are also incremental - you can buildf them one at a time, eventually building up a massive amount of land. Contrast this to any terraformed world, whose land will not be available for habitation until the enormous task of terraforming is completed, probably centuries in the future.
It is rather hard for me to imagine, what sort of society would go to so much cost and expense creating what is sure to be a cold and miserable little planet. It is easier to imagine an incremental terraforming approach on Mars, where the atmosphere would be initially thickened to provide cosmic ray shielding and could be accomplished relatively easily, simply by pumping CFCs into the existing atmosphere. But most other worlds (the jovians, satellites of saturn, uranus, neptune, pluto and the TNOs) will always be cold, miserable and rather unproductive even after full terraforming is complete. Mars isn't the only candidate, but it appears to be the only one that offers value for money.
I'm pretty sure Venus would be easier to terraform than Mars. Seeing as it lacks water, which is cheap, and Mars lacks nitrogen, which is quite expensive.
And as for the moon thing, it's not so cut-and-dried. Earth's moon has no ocean, and no atmosphere. Titan has practically no sunlight. Ganymede and Europa lack atmospheres, and Callisto lacks internal geology. They all have their own problems.
Terraforming Venus would be a nightmare of a project. How exactly do we dispose of a carbon dioxide atmosphere with a column density of 1000tonnes per square metre?
To introduce sufficient water to Venus would require the equivelent of several large kuiper belt objects, all of which would presumably need to cross Earth's orbit to get there.
Even after terraforming, the planet would still be unbearably hot, with the surface temperature teetering around the boiling point of water in equatorial regions. Then you have to deal with the fact that Venuses day-length is roughly comparable to its year (~250days).
Given Venus's hostile environment, relatively deep gravity well and general lack of anything exceptional that it might export, I would anticipate that this will probably be a deadzone for future human colonization.
It sounds ridiculous, but it would appear no less possible than terraforming Jupiter's other large moons. Amalthea has the dimensions 250x146x148km and its surfcae gravity is 0.02m/s2. This is 1/500th of Earth's gravity. The column density of the atmosphere would therefore need to be 5000tonnes/m2 for a 1bar average surface pressure. the total mass of the atmosphere would 5x10(17)kg - fully a quarter the mass of the satellite! The escape velocity of Amalthea is just 50m/s, so the atmosphere would escape very rapidly without a magnetic field holding it in place.
The views of Jupiter would be stunning!
One thing with Jupiter's moons is the deadly radiation - 10 minutes unshielded is enough to kill a human.
Europa is the worst off. Until you've got lots of well designed atmosphere, you're probably going to be living under the water.
You might want to think about Titan first. Saturn's local environment is relatively benign. Use large mirrors/Fresnel lenses to up your solar wattage.
Lasers? You would need a very impressive laser to illuminate an entire world and a wacking huge amount of electric power. I just can't see that being a very practical solution.
As for using lenses, the scale of the engineering required would be similarly huge. Sunlight intensity at Titan's distance from the sun is 1% that of earth and the lense would need to be continuously realigned as Titan orbited Saturn and Saturn orbited the sun.
It would probably be much easier to build a fusion reactor on the surface and artificially illuminate areas that have been heated with wasteheat from reactors.
In any event, Titan's existing hydrocarbon atmosphere would appera to be more of a hindrance than a help. Rhea, Japetus and Dione are also promissing potential candidates.
Europa sounds so great, and I've got to think that even if it lacks native life it could be seeded easily from earth. Given how many species live only between certain depth ranges we could even possibly introduce earth species without a threat to native species if any exist and things turn out right as to where they live.
Does anyone know if there's any information on the composition of the interior of Europa though? Is it a sphere of water below the ice, or is there a metallic core? If so is it solid or molten?
Even lacking native life and a course of chemicals for a chemosynthetic species at the bottom of the pyramid I think we could maybe slowly get things going. Dump enough biological waste into the water, and then build your ecosystem on some filter feeder like clams. That'd likely take a long time though.
There's a topic on the human missions board I think about colonizing earth's oceans that might have some applicability.
As a target for human colonisation, Europa strinkes me as the least promissing of all of the Jovians. It is relatively small, has a young and therfore mineral depleted icy crust and is right in the middle of Jupiter's radiation belts. Callisto is probably the most appealing target, Ganymede a distant second.
Actually, the sunlight intensity at Jupiter's orbit may be sufficient to allow at least some plant life to survive and may therefore support a limited ecosystem.
Jupiter's average distance from the sun is 5.46AU. The average sunlight intensity is therefore 45 watts/m2. On the equator of a terraformed Jovian moon, sunlight intensity would be perhaps 40 watt/m2 at midday, outside of Jupiters shadow. This is typical of Northern European mid-winter illumination levels. There are plenty of plants that will grow at these light-levels, if you are able to keep their roots warm. The rate of photosynthesis and therefore rate of growth will be reduced. This is inconvenient, but is not a show-stopper.
Using super greenhouse gases, it may be possible to keep the atmosphere of a terraformed Jovian relatively warm. In addition, the waste heat from a colony's nuclear/fusion reactor could be used to warm greenhouses full of food crops. The weak sunlight could be supplimented by artificial light, targeted at very specific and optimised frequencies for plant growth.
Many species of photosynthetic algae will thrive at very low sunlight levels, if provided with a liquid medium and sufficient nutrients. Genetic engineering could do wonders in this area and it is not difficult to imagine that a range of algal species could serve as the base for a larger food chain, just as plankton and complex land plants do on Earth.
I am still fishy about this idea of a global ocean world. It would appear to me that any useful meteoritic materials, which are no doubt abundantly available in the crusts of Jovian satellites, would sink to the core and be lost forever. There is also the crucial issue of recycling carbon, nitrogen and nutrients of any dead organisms that sink to the bottom of a 100 - 1000km deep ocean. I hate to imagine the sort of storms that might be generated in a global ocean that deep.
The Sea Dragon Big Dumb Booster idea may very well be the way to go. Large, but simple pressure-fed engines, with ablative liners, may end up being cheaper per unit of payload lifted than much smaller, high performance engines, which are really only suitable for ballistic missiles.
I have often wondered why NASA has not given more attention to the Big Dumb Booster concept. The shuttle has demonstrated that the technological requiremnets of a reusable vehicle almost automatically make it an expensive vehicle.
Instead, we want rockets rather like coke-cans, which we can use once and then throw away. This sort of design philosophy does not lend itself to complex, turbo-pump rockets made from ultra-expensive alloys. Ultimately I think, even a very large rocket could be extremely simple in design, with only a handful of moving parts (valves on the propellant lines, tank pressurisation equipment and a valve within the engine). Once the design is finalised, the whole thing could be constructyed in a ship yard from carbon steels or aluminium, very cheaply.
Looks wonderful.
But 2.5 bars at sea level? On Mars, that equates to an atmospheric column density 6.5 times that of Earth. Where do you plan to get that much gas? Bearing in mind that most of it cannot be oxygen.
~250km may be within the Ceres atmosphere. The column density of the atmosphere would need to be 40 times that of the Earth in order to provide similar surface pressure. Given that the Earths stratosphere extends to 50km above the surface, we can expect the Ceres atmosphere to be at least 200km deep. The ionosphere and exosphere will extend even further.
It would be interesting to know how this would effect atmospheric dynamics. Would we get super-high winds in the atmosphere? How much dust and suspended water would the atmosphere hold and how would that effect transparency?
Given that a superconducting magnetic field will prevent the atmosphere from leaking into space even on relatively small bodies, the ultimate descision over whether or not to terraform a body, would come down to whether the value of each square mile of land, is worth the cost of providing a breathable atmosphere over the land. As the candidate body's get smaller, surface gravity goes down and the required column density of gas increases progressively. This in turn, will increase the cost per unit area. Eventually, the mass of the atmosphere is a sizable proportion of the mass of the entire body. As gravity decreases, it is also arguable that the desirability of the land goes down.
As i said before, the question will come down to economics, as do all things in life. For bodies like Ceres, Vesta, Juno, Pallas, etc, my guess is that it will be much cheaper just to dome areas off with plastic enclosures. Even for Mars, there is a strong case for paraterraforming over planetary terraforming. the obvious advantage is is that you do the job in an incremental manor, with a relatively small budget to begin with.
Sounds good. There appear to be no fundamental barriers against the terraforming of smaller worlds.
Ceres would appear to be the most promising initial candidate. It is close enough to the sun to provide acceptable levels of sunlight for plant growth and massive enough to allow the accumulation of an atmosphere with acceptable surface pressure without the requirement for ridiculous quantities of gas. To provide a 1 bar pressure at the surface of Ceres, a mass of gas equivalent to 1% of the mass of the Ceres would be required. For smaller worlds, the amount of gas needed becomes excessive for the amount of surface area gained and you end up building a small gas planet.
Ceres could be terraformed relatively easily given the relatively abundant sunlight at its orbit. If a large comet were trapped in orbit around Ceres, the sun would gradually vaporise it into ammonia, water vapour and various other minor gases. The UV and solar wind particles would ionise the gases. If a superconducting ring were placed around the equator of Ceres, the ions would tumble along the field lines, entering the atmosphere at the poles.
By this means, Ceres could be provided with a breathable oxygen/nitrogen/water vapour atmosphere in a relatively short timeframe (~decades), due to the potentially enormous catchment area of the magnetic field. The sun does all of the hard work breaking down the water and ammonia into oxygen and nitrogen.
With a diameter of 950km, the surface area of Ceres is almost 3million square kilometres. At typical European/Japanese population densities, this would provide living space for perhaps 1 billion people.
Hi Antius, welcome to newmars.
I think the main reason for considering putting atmospheres around small bodies is long term stability.
I'm a fan of O'Neill cylinders but they have an inherent instability: a high pressure (i.e., 1 bar) atmosphere separated from vacuum by a relatively thin skin. I have no doubt we can engineer systems that cope with this instability in the vast majority of circumstances, but eventually the cylinder will encounter the astronomical equivalent of the hundred year wave. Even if the design can be made immune to natural menaces, the instability is there to be exploited by malicious actors (internal and external). The necessary docking ports are at least cumbersome, if not a point of special vulnerability.
If the magnetic field around an atmosphered small body is disabled, the atmosphere will eventually be lost, but your time to repair can probably be measured in years rather than hours. Also, atmospheric entry shouldn't be a huge issue in low gravity environments, particularly since aerobraking can be a big fuel saver, because then any mods required for atmospheric entry can be justified by fuel savings.
Some notes w.r.t. your other points:
- see the "Moving Ammonia Asteroids" section of Zubrin's _Technological Requirements for Terraforming Mars_
http://www.users.globalnet.co.uk/~mfogg/zubrin.htm
for an idea of economically bringing volatiles to small bodies- if we can engineer the other stuff, I'm sure we can engineer an atmosphere transparent in the important regions for plants, however, as you say the sunlight may be too faint in any case, in which case we may first want to use the small bodies' own volatiles to change it's orbit to something more viable
- an ocean world with artificial islands is not an unappealing habitat. Everyone gets beachfront
I'm highly sceptical. Firstly, if we are talking about heating an icy world to earth surface temperatures and melting it into a global ocean, where will the inhabitants get their mineral resources from? It would appear that they would sink to the bottom of a global ocean 100's of KM deep in mnay cases. Also, whatabout soil for growing crops? The only other alternative would be to cover the icy surfcae in an artificial (metal?) crust, before heating takes place. But then you run into the problem of what happens if the crust is pierced by a meteorite. This is also planetary engineering on a ridiculous scale.
Second, for most bodies, artificial lighting and artificial power would be a neccesity simply to grow food and keep the place warm enough for survival. This would appear to make the ecosystem just as vulnerable to catastrauphic disruption as any orbital habitat. A large meteorite hit would be just as catastrophic for a world like this as it would be for a space colony.
The other alternative would be to heavily insulate individual areas of the icy surface, dome them off and heat them, building our cities and cropland on the heavily insulated surface. This would allow the planets average temperature to remain below zero, but reach comfortable temperatures in particular locations. But again, it is difficult to justify the massive cost of paraterraforming such a barren world, for such a limited amount of holding capacity.
Given mechanical erosion protection ( solar wind, impacts ), the only thing relevant before the successfull atmosphere retention would be the RATIO: escape velocity VS. thermal velocity at the exobase. We know that if the particles` velocity in the exobase is kept under 20% of the escape velocity in the exobase, than an atmosphere could persist billions and billions of years, i.e. the same time order as the normal geological and astrodynamical lifespan of a planet, i.e. indeffintelly long, i.e. practically "forever". For smaller bodies that means REALLY cryogenic tempeatures necessary. Once, I calculated for 3-5% gees body Pluto as far as I remember, similar for Vesta, Juno, Ceres... and the results were that for nitrogen and oxigen 30-40k sufficed. Even sub-1k cryo-cooling is feasible I think.
Many proposed laser cooling, but much more appropriate would be kinda |plasma coolin`| -- i.e. version of the Peltier-Zeebeck effect working in fluid charged medium.The Non-charged component of the high atmosphere of the little body could be charged via channeling to meet the ficused solar wind, via collisions with the decelerated cooled charged ones, etc.
G.K.
30-50K is more than the average surface temperature of a body at Pluto's distance from the sun, so it would probably work. Much cooler than that and you need to go lower than natural background radiation will permit as far as i can see. Below about 20K is impossible without surrounding the world with some sort of physical barrier that blocked out incoming radiation.
Again, the question in my mind is: what is the point? Why not simply mine materials from such a body and use them to produce a bernal-sphere type free space colony, in which you have complete control over internal conditions and can tailor them as you desire? Why would we choose to colonise a body whose surfcae is nothing more than worthless ice?
Maybe there is a point that i have missed. In any event, the sirfcae would need to remain below zero to prevent it from melting into a global ocean.
A fascinating idea, one that has appeared several times before on this list, if memory serves. If I understand it correctly, the idea is to provide a minor planet/moon with an atmosphere. The sun will ionise the upper layers of the atmosphere, which will gradually escape into space, given that the average speed of the particles is greater than escape velocity. By giving the world a magnetic field, the ions are caught before they can escape and will basically spiral along the field lines, reentering the atmosphere at the poles.
It could work, but is loaded with problems. The first problem, is one of economics. Firstly, in order to provide Earth surface pressure on a world like Ceres, the planetoid would need to have something like 30% of the Earth's atmosphere. That's an awful lot of gas - equivelent in mass to a full 1% of the mass of Ceres. The easiest way to create such an atmosphere would be to trap a comet in high orbit about the planetoid. The sun would gradually vapourise and ionise the comet and the ions would be trapped within the magnetic field, gradually building up an oxygen/water vapour atmosphere (the H2 would escape into space).
The good thing about an atmosphere that deep is that it would trap IR radiation very efficiently, keeping the surfcae warm even at great distances from the sun. The bad thing is, it may not be transparent to the visible part of the spectrum, which is obviously important for plant growth.
For most candidate planetoids/moons, the surface must not be allowed to rise above zero, given that most outer solar system worlds are covered in ice to a depth of at least a few hundred kilometres. This may make an active ecosystem or comfortable environment difficult to maintain. Also, the sun is too dim beyond Jupiters orbit to allow significant plant growth without artificial light.
At the end of the day, i am left wondering why any future society would bother going to so much effort to create what is sure to be a cold and miserable little planet. Far more promissing to concentrate efforts on free space habitats, which have completely controllable internal environmental conditions and geography.