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Yes, Graeme.
There is a theoretically sound way to create a 1g environment on Mars. It involves constructing a circular railway.
There was a discussion about it back in 2002 on http://www.newmars.com/forums/viewtopic.php?t=1766]THIS PAGE.
It might be worth doing this for people who are only on Mars for a limited 'tour-of-duty' and who wish to return to Earth eventually.
I don't think it's a practical idea for all future martian colonists, though. So, if humans can't adapt to permanent residence in 0.38g, I don't think colonisation will be an option.
"And frankly, Columbus' feverish zealousness to get to the Indies is a problem for the 'Nina', 'Pinta' and 'Santa Maria', that the "Indies or bust" mindset is liable to cut corners or promise what can't likely be done to push the project."
I guess that throughout history, there have been the 'feverish zealots' of science and technology who appeared foolish and desperate to many of their contemporaries.
Maybe many of them were fools and desperadoes whose ideas came to nothing. But there were many others who were ostracised and ridiculed, who eventually became historical icons of science and discovery.
Dr. Z has enemies. Manned space exploration has powerful enemies. But I wish we had more people like Dr. Zubrin.
A little 'feverish zeal' for space exploration in governments all over the world would be a nice change.
O.K.
On the way out, my preference would be to maintain 1g for about 5.5 of the 6 months, then reduce to 0.38g, allowing a week or two at that level before landing.
For the return trip, my ideal set-up would be to begin with a week at 0.38g, then increase the 'gravity' in about 0.05g steps on a weekly basis. This would bring the astronauts back up to a full 1g over a three month period. I think a controlled and monitored exercise regime tailored to the gradually increasing 'gravity' could be devised by NASA doctors to ensure the astronauts were fully re-adapted to terrestrial conditions.
The final three months in full Earth 'gravity' would ensure that the first martian explorers would step out of their landing capsule looking, and feeling, strong and healthy.
This latter point would not only be good for the crew but would be good for public relations. With no artificial gravity, the astronauts would have to be dragged out of the capsule on stretchers and would spend months in rehabilitation, probably suffering permanent bone-loss and long-term debility.
The public would see them leave in perfect health and arrive home as physical wrecks.
What would that do to the Mars exploration program? ???
It's not just a matter of money and convenience either; it's potentially much more serious than that. A trip to Mars is a looong trip! We're looking at about 180 days outward, about 500 days on Mars, and about 180 days homeward. That's nearly a year and a half in 0.38g and about a year in zero-g.
As I've said before, even being generous and pretending the whole 860 days were spent in 0.38g, coming home would be like an 80 kg (180 lb) man suddenly weighing 210 kg (465 lb). This would feel like he was carrying his twin brother on his back and a 25 kg (55lb) dumbell in each hand!!
And it ignores the fact that his heart would feel like it was pumping blood which suddenly weighed 2.63 times as much as normal blood.
I have expressed serious doubts that a human could tolerate returning to Earth after such a mission. It seems quite possible to me that one or more of the astronauts might actually die!
My previous ranting on this subject met with agreement from Adrian, as I recall. And Phobos, a well-loved former contributor to New Mars, immortalised the concept of artificial gravity for Mars Direct by agreeing we should "set that sucker on the spin cycle"!! :laugh:
Good point, Graeme.
I suppose a lot depends on how long it takes astronauts to adjust to different 'gravities'.
::Edit:: Apologies for the repeated post. ::
Good point, Graeme.
I suppose a lot depends on how long it takes astronauts to adjust to different 'gravities'.
Aahhh .. you're all nuts!!! :angry:
If Dr. Z says Mars Direct is feasible (albeit with slight modifications) and Robert Dyck thinks he can make it work, that's good enough for me!
When do we leave?!! ??? [ :laugh: ]
I'm not a Christian but, what the hell ... any excuse for a celebration!
We're flying my parents-in-law up from Victoria for a week. Having the usual traditional Christmas meal, Christmas tree, etc. ... in the middle of the usual sticky tropical summer!!
As for "favorite holiday songs", "Meet Me In St.Louis" is one of my all-time favourite movies and "Have Yourself a Merry Little Christmas" is, perhaps not surprisingly, my favourite Christmas song.
[This thread is really Josh's, Clark's, Bill's, and CC's, I know, but if I may just toss in two cents worth(?):- ... ]
It's one thing to "mollify" various space agencies by giving them a "truly important role" in future projects, it may be another thing entirely to persuade them to stump up the cash to make a "truly important" financial contribution!
And there's always the usual 'fly in the ointment' - endless committee meetings with representatives of governments who are all paddling their own canoes, usually in different directions.
I don't know what the best way forward might be, though I'm inclined to agree with Bill and Josh, in principle. Why throw good money after bad?
But trying to cobble together some kind of United Nations of Space Exploration will probably meet the same intractable problems which make today's U.N. the lame duck shambles of an organisation it is.
It's always going to be easier to sell a space program to tax payers if you say the cost will be shared among several countries to ease the pain. But, in the end, I think one country, with one plan, and with one administrative structure to carry it out, will be able to achieve its objective much more cheaply in the long run.
I'm keen to get out of the rope retailing business, too! :bars:
Oops!
I just thought of something. There may be a down-side to mildly acidic martian seas.
I've been straining my eyes to find evidence of fossils in the images returned from the MERs. But, if the seas on Mars were acidic, shellfish would probably never have evolved because building and maintaining a shell in that sort of low pH environment would have been impossible.
Shells make great fossils and Earth is full of them. But on Mars, perhaps only soft-bodied creatures like jellyfish may have evolved. And they're notorious for leaving little trace of their existence in the fossil record!
Hmmm. Could shellfish on Mars have used other dissolved chemicals to produce a shell, like sulphates for example?
Do we have any zoologists here?
[I know this is all just the most idle speculation but it's a topic that really interests me. And I really am crazy enough to actually examine the micro-images from Mars for anything reminiscent of a fossil!
]
Hi Earthfirst.
Well, I don't know much about growing citrus fruit but your comments about former martian oceans, and any potential oceans created by terraformers in the future, are well taken.
I also read about Mars probably having had mildly acidic oceans in the past, which might explain the apparent scarcity of carbonate rocks on its surface today.
This is potentially good news for terraformers looking to find CO2 reservoirs hidden in the regolith.
People like Drs. McKay and Zubrin have suggested there may be large quantities of carbon dioxide adsorbed onto granules in the martian soil. Estimates have ranged widely, between maybe 100 millibars worth and as much as 800 millibars. This is in addition to the few tens of millibars worth which may exist as solid CO2 at the poles - especially the south pole (though, there have been reports lately that even the south polar cap is more H2O than CO2).
The idea, of course, being that a relatively dense new atmosphere could be created on Mars by the simple expedient of warming the planet, tipping the balance, and producing a runaway greenhouse effect which would release most of that CO2.
What's always bothered me, though, is the possibility that virtually all of Mars' CO2 was turned into carbonate rock early in the piece, leaving little or none readily available to us now for terraforming.
This latest news, that the formation of carbonates in the martian seas was inhibited by a lower than expected pH, makes the prospect that useful amounts of CO2 are still there for terraforming purposes much more likely.
And, if we manage to re-create an Oceanus Borealis and a Hellas Sea, it seems likely these new bodies of water will assume the same mild acidity as the originals. If so, then Earthfirst's suggestion that we won't have to worry about the new atmosphere rapidly disappearing into the ocean is also likely to be true.
Good news all round. :up:
This is one more subject on which I've lectured long and hard here at New Mars over the past couple of years. Not that NASA, or anyone else for that matter, seems to think my angle on the problem is really practicable.
Anyhow, taking the 'centripetal gravity' solution to its ultimate and ideal conclusion, we need full terrestrial gravity simulation for as much of the flight as possible, together with a low spin rate in order to avoid sensory problems caused by the Coriolis Effect (disturbance of balance and disorientation etc.).
The answer is to have two craft, or one craft and a counterweight, tethered to each other by 1800 metres of kevlar cable and rotating around the centre of gravity at 1 rev/minute. This will give us 1g of 'gravity', just like home, and the minimal rotation rate will all but eliminate Coriolis problems.
Others have suggested gradually slowing the rotation rate on the way out to Mars, in order to reduce the 'gravity' to 0.38g just in time for the landing. In this way, the astronauts will be fully adjusted to martian surface gravity when they start work.
Conversely, the rotation rate could be increased gradually on the return journey, until a full 1g is achieved - thus preparing the astronauts for terrestrial conditions again.
I think this makes a lot of sense but I wonder whether it's still better to have 1g for as much of the mission as possible.
I admit this is the physiologically ideal situation but that it does make for a more mass. And people have raised understandable objections of excessive complexity, untried technology, as well as the extra kilograms.
But it does have the very attractive redeeming feature that all the seriously detrimental physiological effects of 180 days in zero-g outward and another 180 days in zero-g homeward (not to mention 500 days in 0.38g on Mars) are eliminated.
There may be good practical arguments in favour of reducing the radius of rotation and increasing the rate of spin, or never going higher than 0.38g on the outward leg and allowing zero-g on the way home, but I still think some form of rotation is going to be essential.
I while I may be forced to change my mind eventually, my present attitude is: If we're going to do it at all, let's do it right - 1800 metres and 1 rev/minute!
Beautiful!
Damned martian kids, hiding behind that hill and throwing stones!! :rant:
You'll notice I avoided the gas/plasma question by using the word "matter".
You're not as fast on your feet when you get older, so you have to plan ahead! :;): :laugh:
How low can we get the Pressurised Rover's mass, perhaps using new materials, before we lose too many desirable features and compromise reliability and safety?
???
Apparently, no one's 100% certain of the theoretical maximum temperature of matter. It depends to some extent on whether the Standard Model of physics is complete and, if it's not, and if there are more and more massive sub-atomic particles produced as ever-increasing energy is applied to a system, then the maximum may be relatively low - a few trillion degrees!
On the other hand, if quarks are the end of the trail, and injecting more and more energy into a system goes to increasing the kinetic energy of the particles, rather than the creation of more massive ones, the theoretical temperature can be very much higher - as high as 10^32 degrees Kelvin.
According to http://www.astronomycafe.net/qadir/q804.html]THIS ARTICLE :-
The thermal energy is then free to increase practically without limit until you eventually end up creating 'quantum black holes'. This happens at a temperature of 10^32 Kelvin; that's 1 followed by 32 zeros! Once you produce quantum black holes, you have reached what many theoreticians believe is the end of the road for physics as we know it. Here, spacetime itself dissolves into a witches' brew of quantum worm holes, black holes, multi-dimensional superstrings and twistors. Most theories of the early universe give this temperature as a true limiting temperature for physics in the universe.
I'm not sure if this was what you were looking for, Cindy, but it's mind-boggling stuff just the same!
Many thanks, Rob, for your input on sea-levels.
Your post caused me to re-think the way I've been interpreting articles on this subject and I've realised I've made an error - an error of degree rather than one of substance, but an error just the same.
I've located http://www.sciencemaster.com/jump/earth … l.php]THIS ARTICLE, which clarifies the situation.
Rob, of course, is perfectly correct in estimating a 200 ft rise in sea-level if the Antarctic ice cap were to melt. This had me confused because I was quite sure I'd been reading of a 200 metre (roughly 600 ft) rise.
The 200 metre rise I'd read about, refers to the total difference in sea-level between that which prevailed in the depths of the last glacial maximum, and that which would prevail if all the ice on Earth were to melt.
The fact is that during the maximum glaciation, sea-levels were some 125 metres lower than they are now.
If all the ice present now were to melt, everywhere on the planet, sea-levels would be some 80 metres higher than they are now.
The difference between the two figures is 205 metres, which explains the figure I've been working with.
I apologise if I've misled anyone as to the numerical effect of climate change on sea-levels due to this misunderstanding on my part.
Thanks again, Rob, for being instrumental in correcting my mistake.
Yes, indeed, Rob. A multiplicity of potential terraforming disasters in the making!
While dust storms are known to cause lower atmospheric cooling, I guess we can only hope that increased levels of water vapour in the air from the newly created seas will act as an atmospheric cleanser, as happens here on earth.
Localised dust storms, some of them no doubt quite large, will probably always occur - especially in the dryer southern reaches, far from water. But I'm hopeful that global monster dust storms will be a thing of the past.
It may be, too, that hardy (genetically engineered?) drought-resistant plants, introduced to the southern highlands, will help to inhibit aeolian erosion and minimise the quantity of raised dust.
While, as you suggest, the increased water vapour in our brand new martian atmosphere will increase global albedo through cloud formation, the resultant cooling will surely be more than offset. Water vapour is the major greenhouse gas in Earth's atmosphere, without which our global mean temperature would be some 30K lower than it is.
Of course, on a terraformed Mars, with a 500 millibar atmosphere of mainly CO2, and proportionately less ocean surface and less average humidity, the CO2 will be the main influence. But, despite the clouds, I think the overall effect of the extra water vapour will be decidedly in our favour.
Nevertheless, I agree with you Rob that Mars will "tend to revert". Custom-made greenhouse gases like perfluorocarbons will be a constant requirement and I think that soletta will be a must.
Cindy:-
It'd be impossible to view it all in one lifetime ...
>Flabber .. Flabber ..< (Sorry, that must have been my gast. )
Far from imagining being able to see all of terraforming on Mars in one lifetime, I'd settle for one teensy weensy little Hab on martian soil before I turn up my toes!!
:;): :laugh:
Groovy movies! :up:
Thanks SpaceNut.
That link is very interesting. I was aware of the increase in Earth's atmospheric oxygen about 2.2 billion years ago but this article explains the process in much better detail.
I hadn't considered the idea of Earth's volcanoes exuding a different mix of gases as the planet settled down into middle age, so to speak. The gradual change from predominantly H2/CO to H2O/CO2 is something I wasn't familiar with and it's solved a riddle which has been troubling me for years - i.e. since O2 producing cyanobacteria have existed in profusion since at least 3.5 billion years ago, why did it take until 2.2 billion years ago for the concentration of O2 in the atmosphere to become significant?
Answer: Different volcanic gases in the early stages maintaining a heavily reducing atmosphere.
Problem solved! Thanks again for this illuminating link - light has dawned.
Yes, Cindy, an interesting example of how a micro-climate can be influenced by human activity, even to the detriment of that very activity.
Dook's right, of course, in saying oceans on Mars would act as heat sinks and tend to moderate temperature swings. But I've wondered for a long time now whether there's something profound about the topography on Mars which might have been a significant contributor to its dessication and freezing.
If we look at Mars' surface and compare it to Earth's, it's almost like Mars has one enormous continental plate, taking up about 60% of the surface area and mainly occupying the south of the planet, and one huge oceanic plate taking up the other 40%. Even if earlier volcanism had been vigorous enough to drive tectonic plate movement, there was probably too much continental plate area, a kind of logjam, to allow much movement.
Without the movement of continental plates and subduction of oceanic plates we have here, recycling carbonate rocks down into the mantle where the CO2 could be returned to the atmosphere via volcanoes would not have occurred.
In addition, the only ocean would have been centred on the north pole. Without the benefit of a planetwide system of oceanic currents, transferring warmer water from the equator to the colder polar regions, there would have been a tendency for the Oceanus Borealis to freeze and stay frozen.
With the greater distance of Mars from the Sun, and the inexorable sequestering of more and more of the thick greenhouse-producing CO2 atmosphere into the crustal rocks without tectonic recycling, the martian air would have thinned and the planet would have been locked into a permanent deep freeze.
These things bother me because I'm a terraformer. Your comments on the micro-climate in Florida, Cindy, certainly give me food for thought about the macro-climate on Mars; and it's not necessarily a particularly palatable snack! You remind me of nagging doubts I've had for some years.
While changing the local climate in Florida may be as simple as draining some waterlands, even massive planetary engineering on Mars to create a benign climate for colonisation may prove to be a futile exercise. It's possible that the very structure of Mars has been a major player in its climatic deterioration in the distant past and will conspire against our terraforming efforts there in the future.
This potential problem has been addressed to some extent in as much as orbiting solettas have been suggested to concentrate solar heating on Mars' north pole. But I've yet to see anything much of what we've learned about terrestrial air and ocean currents being applied to a hypothetical terraformed Mars.
Once we've established a warmer wetter Red Planet, will it be a constant engineering struggle to keep the place from reverting to its old ways?!
???
[Sorry! Rambled on a bit with this one.]
Yup! I'm a hardline dolphin fan.
Happy Birthday Seth!!
And may there be many many more of them. :up:
Nice of you to drop in Fraser!
By the way, in that photo in the "About Fraser Cain" section of your site, who's the old guy behind you in the white shirt?
???