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#126 Re: Terraformation » Nuke Mars - Use of nukes to release Martian CO2 » 2007-07-03 21:24:54

Hi m1omg,
  Thanks for your posts.  Altho, would it be possible to eliminate the second of your 2 posts by editing the first one?

  Mars has only 1.777 time the radiation as the Earth?  According to "The Case for Mars" a person would get 14.7 rem from the 500 day stay on Mars with much of their time spent in the habitat with a couple layers of sand bags on top, (to lower radiation dosage).
  See page 119 of that book, where 10.6 rem come from cosmic rays and 4.1 rem come from solar flares.

  On Earth, at sea level, in 500 days, people would get 0.205 rem (or ~0.40 rem if they live in Denver since it has less atmosphere to protect it from cosmic rays). 

  (This assumes an average yearly does of 150 milli rem per year, page 114 Case for Mars.)

  When you were talking about dangerous nuclitides, were you refering to Fogg's plan of using pipes of deterium fusion and no fission bomb to start it?  In that case, what nuclitides are you talking about?  (The ones produced by D-D and D-T fusion are both rare and generally have very short half lifes.)

  I am not a big fan of Fogg's bombs, I pointed it out as an alternative to the fission bombs others have been talking about.

  As for Nuclear Winter, much of the science on it is very weak, but in any case, since Fogg's bombs go off underground, there is very little dust that reaches the atmosphere.  (Which also cuts down on radiation.)

  See chapter 6 of "Terraforming: Engineering Planetary Environments" especially pages 277 to 283.

  By the way, when stating facts, please give references to where you get your numbers.  If in the last couple years they have learned that Mars gets only 1.777 times the radiation that someone on Earth gets, this is very good news.  However, I follow research on Mars quite closely and this is the first I've heard of it.

  Warm regards, Rick.

#127 Re: Terraformation » Place to put Book Reviews on Martian Terraforming. » 2007-07-01 04:32:23

Hi everyone, X.
  Thanks for the kind words X.  You might ask the local university libraries to order a copy of Mars A Warmer Wetter Planet.  They have significant budgets to order books and the librarians are delighted to get thoughtful requests.  Failing that you could try ordering it on Albris.  I got my copy there very inexpensively.

  I was hoping that someone else would do a review of Case for Mars since likely plenty of people have a copy, but anyway, this book does not deserve to wait longer...

"The Case For Mars: The Plan to Settle the Red PLanet and Why We Must" by Robert Zubrin, Published by Touchstone Books, (c) 1997, 339 pages, $15.00 softcover.

This is THE book on Terraforming that is currently in print. 

Robert Zubrin almost singlehandedly has transformed the idea of going to Mars from a $500 Billion boondoggle to a pratical plan.  (NASA has taken his Mars Direct plan and modified & expanded it but it still will cost less than $75 Billion dollars.)  If we used Mr Zubrin's origional plan we could have humans on Mars in less than a decade with 13% of NASA's current budget.

More than any single person, Mr Zubrin has transformed human thought on the Red Planet in the last 12 years.

This book is a powerful example how ideas can be nurtured and grow.  It has been the single largest recruiting tool for the Mars Society and other pro-space exploration groups.  Encourage your local libraries to buy copies.  Failing that, buy some copies of your own and donate them to all of your local high school's libraries.

In case you can't tell, I am IMPRESSED by this book.  It is aimed at a science literate layman.  Someone with highschool science will have no trouble understanding it.


The book starts off describing the Mars Direct mission.  As an engineer who has worked on real rocket programs, Mr Zubrin knows how to plan what is possible.  He then discusses the history of Mars and space exploration to that world.  Many of the problems with NASA and previous Mars programs are political.  Nothing new there but they are spelled out.  (The worst is the 'cost plus' accounting system used for buying rockets in the USA.  This alone has cost the USA hundreds of millions of dollars in lost commercial launches.)

He then goes over how his "Mars Direct" plan (that he invented with some other engineers at Martin Merrietta Astronautics) would work in detail.  Unlike many space programs that people have suggested this gives the details, showing tonne by tonne how the package will fit together.  His biggest innovation was realizing that Mars' CO2 atmosphere could be used (with a dense power source) to make rocket fuel, reducing manyfold the size of the initial launches.  (By not having to ship the rocket fuel to Mars, the size of the initial launches is reduced as we don't need fuel to launch the fuel.)  A feed stock of hydrogen must be shipped to Mars but thru simple chemistry plus power this is turned into 18 times its own mass of rocket fuel.

He then talks about the "dragons" that scare people into saying that a Mars launch is too dangerous and needs more studies.  He shows that these are  paper tigers.  Just one example is the idea that we need to study long term exposure to zero gravity.  Not only are these problems well understood (needing no further study) but by spinning the spacecraft at the end of a teather, connected to the upper stage of the rocket, the zero gravity can be simply avoided.

He also talks about the alluring siren of the moon.  Many people say we should go back to Luna before going to Mars (this is the current USA plan).  He points out that there is no practical need for a Lunar mission before going to Mars.

Starting in chapter 6 thru 9, he discusses building the initial base, the initial colony and finally the possibility of terraforming Mars.  These section of the book are dense with practical ideas on how we can use local materials to help the people there.  This is the biggest difference between Mars and Luna.  Luna is missing most of the elements that life needs, Mars is a rich planet where the materials we need are there in the air and dust.

Furthermore, Mars has been geologically active with both volcanos and water erosion.  Both of these will concentrate minerals suggesting that we will find useful ores on Mars when we start exploring it.

In the final sections of the book he argues that if we wish to have a free society having a frontier is key.  He suggests that Mars is the only likely frontier our society will have soon.

Then in a late chapter he talks about the Martian meteor ALH84001 which showed signs of life. 

After finishing this book, I turned back to chapter four and read it thru to the end again.  It was that exciting.

This is a book that is dense with ideas. 

Since the book has been published things have moved on.  For example, his company Pioneer Astronautics, has continued to work on Mars enabling technologies.  He has created a superiour SCUBA diving breathing system  which can be used in space suits.  He has also shown that even more mass can be saved by converting the hydrogen feed stock into aromic hydrocarbons for a 54 times increase of mass when converting it into rocket fuel.  Partly because of his continuing work, the cost of the Mars mission has continued to drop since he first promoted Mars Direct.

Our understanding of Mars has also grown since then.  The major things we have learned is that Mars has a lot more water than was thought when he wrote the book (which is good) and that the southern polar cap has about 1/4 of the CO2 than was thought (which is bad).  Terraforming can still be done using his methods, but using the perfluorocarbons (the super greenhouse gasses he discusses) will likely be manditory as well as just the polar solletta mirrors.

The Martian meteor ALH84001 now looks like the indications were NOT caused by life but (in my opinion) this question is not fully resolved.  More than anything that rock has shown how hard it is to distinguish life signs that are microscopic in size.  (If we were on the planet, the problem would be trivial to solve.)

The current Mars Sample Return mission that NASA is building is a direct result of this book and the Mars Direct plan.  Anyone with an interest in Terraforming should snap up a copy of this book.

Warm regards, Rick.

#128 Re: Terraformation » Orbital Mechanics and asteriods / iceteroids » 2007-06-30 23:39:55

Hi Everyone,
  Hop had shown in his posts above that the Hohmann journey to Mars from the Trojan asteriods requires a delta vee of 4.27 km/sec.  In Jupiter's oribt they are cold enough to have plenty of water.  However, I am not enchanted by the Trojan asteroids as they are too warm to keep their NH3 which is the volitile that Mars really wants more of.  So how much more would it cost us to go to the outer solar system?

  Not much (in terms of delta vee)...

  (By the way, most of the numbers in this post are from "Entering Space: Creating a Spacefaring Civilization" by Robert Zubrin.)

  Objects far out from the sun orbit at a slower speed.  It thus takes less delta vee to change their orbit from circular to eliptical.  Nor do you have to make the elipse reach Mars at one end (that is expensive).  All you have to do it give it a new orbit that moves it close to an outer gas giant and then use that body as a gravity assist to slow your iceteroid so it will fall into the inner solar system.

  Robert Zubrin suggests moving an asteriod in a 25 AU circular orbit so it gets a gravity assist at Uranus.  This will require a delta vee of 0.3 km/s!

  The down side of this is after falling so far towards the sun, the body will have picked up a lot of speed.  (We generally prefer nice small, slow impacts...)

  This can be handled two ways: one we can move small bodies so that even when they hit Mars hard, the impacts are minor and don't splash large amounts of atmosphere, etc.  Since it is MUCH easier to move small bodies than large ones, this is my choice.

  If you wanted to move a huge body (say because you decided you just had to build a good sized moon), then you could use another gravity assist at Jupiter to slow the fall towards the inner system and circularize the asteriod's orbit. 

  Large gravity wells are in many ways like free fuel when it comes to plotting orbits around the solar system.  We were lucky enough to get 4 huge gravity wells in the outer solar system.  It seems a shame not to use them.

  Warm regards, Rick.

#129 Re: Terraformation » Nuke Mars - Use of nukes to release Martian CO2 » 2007-06-30 23:13:49

This is a great thread that basically shows that you can't use nuclear weapons to warm Mars by hitting the polar caps.

Martyn J. Fogg had a different idea in his "Terraforming: Engineering Planetary Environments" book.  On page 281 to 283 he suggests non-fission boosted thermonuclear pipes to melt ground water and vaporize nitrate rocks.  Lacking Fission products they would produce little fallout as well as being more powerful than fission bombs.

He points out that the entire nuclear arsenal of Earth (approximately 10,000 megatonnes) is equal to 1/2 an hour of Martian sunlight.  However, there are things that sun light is good at (crops and general warming) and some things it is too dilute an energy source for (vaporizing nitrogen rich rocks and melting quickly deep ground water).

Fogg suggests using thousands of these fusion rods to quickly jump start terraforming.  I think that some mirrors, greenhouse gasses and a several hundred years will do the job.  But a few of these things for particular jobs (e.g. this city wants a lot of fresh water now) might be very useful.

Warm regards, Rick.

#130 Re: Terraformation » Adding mass to Mars - An idea to stop loosing atmosphere » 2007-06-30 22:53:29

Hi Karov, everyone.
  I think if we have the technology to do the thing you are talking about in the "Micro Black Hole being fed Dark Matter" post we would have the energy to move millions of Kuniper Belt objects on to Mars and increase its gravity the old fashioned way.

  Furthermore many of the points in that post are very speculative.  I have sneaking doubts about dark matter in general (I suspect it may turn out to be  something like lumious ether).  We don't know if micro black holes can exit or if they will radiate Hawking's Radiation like we hope.  Nor do we know if super symmetery works.


  The post on neutronium seems to me to be more possible.  Keep adding mass to a Boise - Einstein Condensate until it approaches neutronium level density.  De orbit it and let it sink to the center of Mars.

  I have no idea if such a thing would be stable or safe.  As mass compresses around it it would likely stir up a major amount of vulanism (which generally would be a good thing).

  In any case, we know how to build Boise - Einstein Condensate and it does not require exotic physics that we are unsure will work.


  Warm regards, Rick.

#131 Re: Terraformation » Could you safely bombard Mars with large bodies... » 2007-06-30 16:41:40

You could drop small bodies in the southern highlands while humans lived in the Northern lowlands.

You wouldn't want to hit Mars with big impacts but no reason you couldn't target carbonate or nitrate beds with smaller asteroids.

Edit: While I was researching another post, I came across this table in the Terraforming textbook.  I'm adding it to my post for your enjoyment.

Note: exponents are in brackets, e.g. 1.4(12) = 1.4x10^12.


Diameter of impactor  (km).... 1.............. 5............... 10.............. 100
____________________________________________________________
Impactor mass (kg).......... 1.4(12)....... 1.7(14)....... 1.4(15)...... 1.4(18)
Crater diameter (km)............ 16............. 66............. 122........... 931
Imported volatiles (kg)...... 6.8(10)....... 8.5(12)....... 6.8(15)..... 6.8(16)
Incr. in Pressure (Pa)......... 1.8(-3)......... 0.2............. 1.8........... 1770

Depth H2O depth (m)........ 4.7.(-7)...... 5.9(-5)........ 4.7(-4)......... 0.5
Devolatilized CO2 (kg)....... 4.0(12)...... 1.0(14)....... 4.1(140...... 4.1(16)
Pressure of above (Pa)........ 0.1............. 2.7............ 10.7.......... 1070

Depth equivalent of regolith meltwater (m)
.......................................... 8.1(-5)....... 0.01............ 0.08............. 81

Substantial Atmosphere Impact Erosion?
.......................................... No............... No........... Some..... Significant?

# of Impacters needed to produce 300 mbars of CO2
...................................... ~291,000..... ~112,000..... ~2,800......... <28

# of Impactors needed to produce 10 m of water globally
....................................... ~123,000........ ~980.......... ~120........... <1


The table includes bodies 50 km in size which I left out for room reasons.  There is another table that talks about comet impacts.  However these generally have such significant atmosphere erosion that they are not worthwhile larger than 10km in diameter.

Warm regards, Rick.

#132 Re: Terraformation » Iceteroids: What happens when they get to Mars? » 2007-06-30 16:39:02

Hi Nickname, thanks for replying.

Rick,
If we drop a big snowball on Mars the result will probably be a short term melt followed by a global snow and freeze.

In my opinion we would make Mars a much more difficult place to teraform with reflective snow all over the place that takes a long time to return to the poles if ever.

I don't see that.  Frost at the low latitudes sublimes and moves to those latitudes higher than 40 degrees or works its way deeper into the soil where it is more stable.

The rate is up for debate (also depending on how big an iceball you drop) but current Mars conditions don't have any problem with moving H2O to the poles.

Finally, if we use a carbonaceous chondrites they have plenty of water but are darker than Mars is.


Maybe we should just use whatever asteroid we find with interesting ingredients as a factory to create super greenhouse gas.

On the years of trip getting it back to Mars we can convert most of the asteroid into super greenhouse gas, ....

In a previous post I pointed out that the major expense with the super greenhouse gasses is finding the fluorine.  There is no reason to expect that any asteriod or comet would have a significant amount of F.  (In fact, I have not heard of any fluorine being detected on an asteriod or comet.  Anyone heard otherwise?)

You could make greenhouse gasses like CH4 or NH3 out of comet stuff, but they are only stable for a handful of years under current Martian conditions.

Fluorine minerals are likely to be concentrated by volcanic activity (at the top of magma melts) and to a lesser extent by fluorine salts.  Both of these methods of concentrating the element will work on Mars, but probably won't have worked on any asteriod or comet.  So I think it would be easier to build the perfluoricarbons on Mars rather than on a comet.


We must use some pretty serious planning with greenhouse gas.
We want to have enough of it to get us past the snowball Mars scenario, but not so much that its uncomfortably warm.
If we don't calculate it correctly we could easily see Mars covered in snow and decrease the temperature even with greenhouse gas locking in heat.
Escaping from snowball Mars would require so much greenhouse gas that the escape point needed to melt makes it permanently uncomfortably warm when it melts.

I've read a lot on terraforming Mars and I think that a big problem is than any time you get a decent amount of water on the equator, is that it will move to the poles and be locked up there.

For this reason, I've been leaning towards Zubrin's suggestion of big solletta's over both poles.  That adds heat where we need it.  We want the huge amounts of water in the polar regions to join into the hydrosphere.

As Mars gets hotter, more heat will escape, greenhouse gasses or no.  (The rate that a blackbody radiates goes up rapidly as you warm it.  Also the wavelengths get shorter so more heat will leak out above the wavelenths that the super greenhouse gasses are tuned for.)

I don't think that with 45% of Earth's insolation, we have too worry about Mars getting too hot any time soon.


The same mechanism is believed to have happened on Earth a few times with 50c global results after the melt with co2 accumulation from volcanic activity.
Earth has oceans and life to use up the excess co2, Mars has nothing to use up excess super greenhouse gasses.

A number I often see quoted is that a CO2 molicule stays, on average, for 200 years before it is absorbed by the biosphere.  However, most of what the biosphere absorbs it released back into the atomosphere a few years later when the plant dies and rots.

(Historically 100 times more carbon was in the atmosphere than in the biosphere.  It is now up to 200 times.)

The iceball Earth theory (which I think likely by the way) points to evidence that Earth froze solid and then seemed to suddenly melt with the temperature rocketing up to 50 C because of the huge amount of CO2 that had built up in the air.  But the CO2 was not drawn down by life.  (The continents were basically sterile.)  The CO2 was drawn down because there was a lot of unweathered rock exposed by glaciers.  The hot rainfall made powerful carbonic acid which disolved rocks.

If we keep these threads on topic, it is easier to find information.  This thread is intended to be a place where we talk about the details of moving rocks, not what happens when they get here.  Perhaps a moderator can move Nickname's post and my reply into its own thread?

Warm regards, Rick

#133 Re: Terraformation » Orbital Mechanics and asteriods / iceteroids » 2007-06-30 02:24:47

Why might we want to drop asteriods or comets on Mars?

1) Add mass to Mars & increase its gravity.  (This is so small an advantage as to be almost zero.)

2) Add volitiles to Mars.  Mars has been slowly losing water to space for billions of years.  From what I've read, a comet 1 km cubed in size would last tens of millions of years before its water was lost.  More Nitrogen, Argon and the like will help Mars perminantly.

3) Start volcanos.  This is a good thing bad thing.  Impacts large enough to start up volcanos will also blow away a fair bit of atmosphere.  By the time we start dropping giant comets on Mars the local population likely won't appreciate impact this large.

4) Land on Carbonates / Nitrates rock formations.  It is looking like Mars does not have much in the way of Carbonate rocks (too acidic?) but likely it has plenty of Nitrates caused by lighting reacting with nitrogen in the atmosphere.  If we drop a iceteroid with 5% NH3 on Mars on top of a nitrate bed we might get a nitrogen boost double what is in the comet itself.  (This is all speculative but likely in my view.)  If we don't have carbonate beds, we might be able to drop the comet on CO2 Clathrates and get a simular effect.  Basically by picking the impact points we can leverage the amount of mass in the comet.

5) Adjust the spin of the planet.  Again this result would be so small as to be almost zero unless we are talking about unreasonably huge numbers of rocks of very large sizes.

6) Adjust the albedo of Mars.  In another thread I calculated that if we darkened Mars with a carbonaceous chondrite asteroids to a depth of 1mm we would get a 5 degree C warming.  This might be enought to be significant for terraformers.

7) Melting the ice caps.  No question this would work but the problem is that water (or CO2) vaporized / melted will just refreeze.  Even the energy of fair sized asteriods would be dwarfed by the sunlight reflected by a 200 km^2 mirror hovering over the poles for a year or two.


Anyway those are the main reasons I see for dropping rocks.  If people would like to argue that we shouldn't drop rocks on Mars, perhaps we can move that question to a new thread?  In this thread the working assumption is that someone might want to do this and we will talk about how expensive it will be.

Warm regards, Rick.

#134 Re: Terraformation » Orbital Mechanics and asteriods / iceteroids » 2007-06-30 02:00:50

Hi Everyone,
  I was going back thru some old posts and found some good ones by Hop.  I'm bringing them forward and making a thread for talking about the delta vee and orbits needed to create artifical impacts on Mars.

  I'll make several posts on this subject later, first what Hop has to say:

*********************************************************

I would use the asteroids at Jupiter-Sun L4 and L5 points (aka Trojans)

These are far enough from the sun to be ice rich.

Delta vee to send them on a Hohmann journey to Mars is 4.27 km/sec. Likely the asteroid's own resources can provide fuel and reaction mass.

When a Trojan arrives in Low Mars Orbit, it is traveling 7.6 km/sec. If Mars' atmosphere sheds 2.8 km/sec or more, the body is captured into elliptical orbit. Then each periapsis the body would again graze the atmosphere, gradually losing angular momentum Until finally the Trojan penetrates the Martian atmosphere one last time at about 3.5 km/sec.

For one body of Trojans, Hohmann windows occur each 2.24 years. But Mars could receive Trojans twice as often since there are two populations (the leading and trailing or L4 and L5). It takes a Trojan about 3.1 years to fall to Mars from it's original 5.2 AU orbit.
_________________
Hop

>>> also... <<<

Another possibility is the outer Main belt. There is a healthy population at 3.15 AU and these also may be volatile rich.

Delta vee to send it to Mars is 3.23 km/sec. Velocity at arrival in Low Mars Orbit is 6.2 km/sec. The atmosphere would need to shed 1.4 km/sec or more to capture the asteroid to an elliptical orbit.

The synodic period is 2.83 years, but I don't think you'd need to wait that often to send asteroids Mars way since these asteroids are scattered in a ring about the sun. These take about 1.8 years to fall to Mars from their 3.15 AU orbit.
_________________
Hop

>>> and... <<<

If I remember right, Kim Stanley Robinson terraforms his Mars with KBOs. To send bodies at 40 AU to Mars you'd need 3.4 km/sec. Velocity on reaching Low Mars Orbit is 10.5 km/sec Sad. It would take about 47 years for a KBO to fall to Mars from a 40 A.U. orbit. Getting to KBOs would be very hard. We still haven't sent a Discovery mission to Pluto so far as I know.
_________________
Hop


Thanks Hop for your interesting posts.  Are you still active?  I've not seen anything receint by you.

Warm regards, Rick.

#135 Re: Terraformation » Harmony-the way to increase effectiveness of ecosystem » 2007-06-29 09:56:13

Hi Jarek, everyone.
  I was hoping an ecologist would post a reply to your post but it doesn't look like that will happen so I will take a stab at it.

  If we want the Martian ecology to take advantage of all the energy and physical resources avalible to it, competition IS very efficient.

  We have not had much success with planned ecologies.  Biosphere 2 was the biggest attempt and its ecology was so simple that it crashed.  Many species overran the planned limits and humans had to become top level preditor, painstakingly squishing bugs for hours a day to try to keep things in ballance.

  Having said that in general, I have some specific comments to things you said...

  The sun is not never ending.  It is building up Helium ash in its core and is slowly burning hotter.  In around 800 million years we will have a run away green house effect and lose our oceans.  (See "The Life and Death of Planet Earth" by P. D. Ward & D. Brownlee for the details of how the Earth's ecology & geochemic cycles will react to the increasing insolation.)

  Even if we somehow set up a stable 'super efficient' ecosystem where there was little competition between lifeforms it won't last.  Mars is a high radiation environment and any genetic drift will select for organisms that compete more efficiently than the handicapped critters we want.

  Parasites are perhaps the ultimate in wasteful creatures but they are key in limiting populations that grow too dense allowing more variety in species.  And variety is the key concept needed for viable ecosystems.

  I think we would be better off selecting (and perhaps bioengineering) critters that are more tolerant of Martian conditions and let them create their own ecosystem. 

  Warm regards, Rick

#136 Re: Terraformation » Angular Momentum and Planetary Dynamos » 2007-06-21 13:43:37

Is there a large impact crater at the antipodes [of Tharsis]?

Hellas Impact Basin is opposite Tharsis.

Warm Regards, Rick

#137 Re: Terraformation » Angular Momentum and Planetary Dynamos » 2007-05-11 22:55:03

... since Venus has such a weak magnetic field, the solar wind hits the atmosphere directly, ... do we lose the rest to solar wind? Does Venus afford any protections to cosmic radiation, solar wind, etc, in its current state?

Mars likely started off with an atmosphere of around 3 to 5 bar and it has taken billions of years to lose it.  (With much of the nitrogen being reacted by lightning into Nitrates).  It will likewise take millions of years to make a noticiable dent in Venus' new 3 bar atmosphere.  Very likely, the gasses from volcanoes will more than make up for any losses

Rick

#138 Re: Terraformation » Angular Momentum and Planetary Dynamos » 2007-05-11 19:21:39

To some extent it depends on the amount of time you want to wait.  Luna is 1/81st of Earth's mass but it took millions of years to add a couple hours on to our day.  In billions of years it added 14 hours onto the Earth's rotation rate.

People are presumably doing this because they want a new world in the lifetime of themselves or their great grand children.  Would anyone seriously plan to move a small planet's worth of mass around the solar system so that in a billion years (when the sun is even hotter) Venus will have a rotation rate of 230 Earth days (down from 243 Earth days)?

I am saying it CAN be done using the laws of physics.  I don't think it will ever be done because for a fraction of that energy expenditure you can move to other solar systems and likely find easier to terraform planets.

Warm regards, Rick.

#139 Re: Terraformation » Angular Momentum and Planetary Dynamos » 2007-05-11 15:54:20

Theoretically, you could change the rotation rate with a moon almost the size of Venus itself.  However, realisitcally, so much mass is not rotating very much that we are stuck with what we have got.

Rick

#140 Re: Terraformation » Angular Momentum and Planetary Dynamos » 2007-05-11 01:03:07

Bryan asked about the breeder reactors they found in the Congo basin.


I've read two articles in Scientific American about these.

The basic story goes like this.  Uranium is not water soluble
  However uranium oxide is a polar molecule so it DOES
dissolve in water.  The Congo basin has plenty of uranium
ores and as these weathered, the uranium oxidized and
was carried into the water.

When they reached the mouth of the river in the delta the
rotting plant material pulled all the oxygen out of the water.
  The uranium atoms lost their oxygen and being no longer
soluble, percipitated out of solution.  Thus long ropy strings
of uranium atoms were concentrated in the mud. 

When the mud was further compressed the uranium was
packed into an even smaller volume.  A mass of uranium
in a small enough volume will turn into a reactor if it has
something to act as a moderator.  Geological processes
later lifted the rocks into a series of hills.

These became the rich uranium mines in Oklo in the
Belgium Congo.


Now water acts as a neutron moderator.  (Fast neutrons
are hard for other uranium atoms to catch.  A moderator
slows them down.)  The sediments were under the water
table so when things were wet, the water moderating the
reactor caused the reactors to go critical.  This caused the
water to boil away so the reactor shut down.  After several
hours the rock would cool enough for water to percolate
back into the soil and the whole thing would go critical
again boiling off the water and causing the cycle to repeat. 

These reactors bred up a lot of plutonium while burning up
the U235.

They have found 15 reactors in the area.  The largest in its
several million year life cooked up 8 tonnes of plutonium if
I remember correctly.

I found a reference to it at this URL:

http://adamant.typepad.com/seitz/2006/0 … of_af.html

From that URL:
"Oklo was soon staked out by Legionnaires as a cadre of
Ecole Polytechnique alumni excavated the 15 natural
reactors within the mine that had gone critical and
fissioned away the U-235 1.8 billion years before. Once
they had been dug up, analyzed and entered into the
annals of science, the last of the usual suspects were put
back on the street, and the miners of Oklo returned to
excavating the still rich ore."

Look up breeder reactors in the Congo in the Scientific
American indexes and you can get the details.


While trying to find a URL talking about this I found:

Natural Breeder Reactor Found in Australia

Apparently they have found natural reactors in Australia
as well.

The natural world is so INTERESTING.  Far stranger and
wonderful than the things that people can think up in
Science Fiction novels.

Warm regards, Rick.

#141 Re: Terraformation » Angular Momentum and Planetary Dynamos » 2007-05-11 00:22:06

I know Ceres is spherical (at about these dimensions), but aren't Pallas and
Vesta nearly so as well, at about half the size. Even so, yes, a lot of matter.
Maybe if we include some FeNi and some plutonium it will heat up.

At this URL is 24 pictures of Vesta.

http://www.solarviews.com/raw/ast/vesta24.gif

I guess the question is how round is round?  To my eye, it is visibly not a sphere.

What do you mean by "do work on the solar wind"? Are you making the distinction between an induced magnetic field versus a permanent magnet? What is the functional difference? I understand that some (all?) of the Jovian moons have induced magnetic fields because of their orbits within Jupiter's magnetosphere.
Does this mean that if you took a moon out of Jupiter's gravity well that it
would lose its magnetic field? How does one make a permanent magnet??

I am not saying anything at all as to what causes the magnetic field.  The solar wind is made up of charged particles.  They will be accelerated by the magnetic field.  (Which does work on them.)  The sun's own magnetic field is coupled to the solar wind.  It is far from clear to me what would happen to a small moon that is given an artificial magnetic field. 
Will the accelerations on it cancel out as it orbits Venus?  To answer that we need to know where the poles of the magnet are, if the moon is tide locked with the planet, etc.
However, since the magnetic field is accelerating particles even a super conductor will need more power to pump up the energy lost accelerating the solar wind.

You can not make a regular moon a permanent magnet.  They are not made of ferromagnetic materials.

Venus has only the faintest of magnetic fields, but I'm not sure why this has
come about. Surely it has a molten core??

It likely does.  I think that the very weak magnetic field is caused by a very slow rotation relative to the sun's magnetosphere which is passes thru and (thru induction) is coupled with.


Ahaaa! Yes, and this was my biggest question. Does the "help" change depending upon the process used to acquire the moon? ...

Do Phobos and Deimos contribute more than marginally to the stability of Mars? Does the swarm of satellites buzzing around Earth affect our own orbital dynamics? (We have lifted mass and put it into orbit!)

I am confused by your question.  I think we may be talking about to different things. 

I'm talking about stabilizing Mars' climate by making a large moon (much more massive than Phobos and Demos).  Are you talking about changing the rotation rate?

The masses of the satellites are so tiny they almost certainly have no noticeable effect on Earth.

If we did create a moon for Venus, should it revolve in the "normal" manner or in keeping with the retrograde rotation of the planet itself? Which manner will lead it to increase its distance over time and which manner will lead it to fall into the Roche Limit and be destroyed, a la Triton at Neptune or Deimos at Mars?
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We could theoretically build a moon in any orbit that we wanted with any rotation that we wish.  We could put a moon into such an orbit that it would either spiral out or in.  The moon could either speed up or slow down Venus' rotation rate.  (Tho the kick would have to be pretty big to get it out of its tidal lock with the Earth.)

Magnetic axis, not magnetic angle. On Earth, yes, the magnetic axis and the rotational axis are not at identical angles, but both intersect at the geometric centre of Earth. What I am saying about Uranus is that its magnetic axis does not bisect the planet into two equal halves -- its centre is off-centre, geometrically. It's a chord.
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My understanding is that the Earth's magnetic axis does not go thru the center of the Earth either.

#142 Re: Terraformation » Are acid seas a problem for future terraforming? » 2007-05-09 00:44:34

I was reading "The Solar System: Mars" and it reports that analysis of data has shown that only tiny amounts of carbonates have been found on Mars.  This suggests that acid lakes / seas / oceans(?) were general and not rare exceptions.

Warm regards, Rick.

#143 Re: Terraformation » Place to put Book Reviews on Martian Terraforming. » 2007-05-09 00:40:43

"The Solar System: Mars" by Linda T. Elkins - Tanton, published by Chelsea House Publishers, (c) 2006, 206 pages, hardcover.

I have mixed feelings about this book.  On one hand it has information on Mars that is not already in my library.  On the other hand it does not have enough 'oomph' to really make me happy.

This is a book that is intended to be a serious scientific primer for high school students on Mars.  It is part of a series of new books talking about the solar system and we have learned so much about Mars in the last few years it gets its own book.

As a primer to the planet it is excellent.  However it is not a fun read.  It is a long series of facts and essays.  Well organized, but lacking the excitment of the best written science books.

Also there is not much of interest to terraformers in this book.

If you are looking for an up to date book to give you the facts on Mars this will make a good choice.  I fully intend to read the other books in the series for the rest of the solar system.

However I am seriously wondering if there is enough new material to make it worth my while putting it into my library.

Warm regards, Rick.

#144 Re: Terraformation » Terraformers Take Note - ...(unintended consequences) » 2007-05-09 00:21:39


It will take a million tonnes of coal a year (for one thousand years) , launched annualy and either dumped into the martian atmosphere or burned on the surface in coal power stations to supply energy to a civilization to melt the CO2 ice cap.

Our job as a species must be to spread the conditions for life across the Universe.

Wouldn't it be easier to float a couple of sollettas from Earth to Mars in order to warm its poles?  Likewise factories building super greenhouse gasses don't require huge mass transfers from one planet to another. 

Warm regards, Rick.

#145 Re: Terraformation » Terraformers Take Note - ...(unintended consequences) » 2007-05-09 00:10:07

Mars will indeed tend to revert. Thickening the atmosphere will greatly increase the tendency of dust storms. ...

Furthermore, once you release significant water into the atmosphere you will get clouds and that will increase Mars's albedo, reflecting more sunlight into space.

It won't be easy.

         -- RobS

Hi Rob, everyone.

Actually the dust storms are caused when the CO2 on the south pole sublimes.  If we raise the temperature 5 degrees then the CO2 will not form an ice cap and you won't get the wind to kick up the dust storms. 

However clouds and snow and ice will certainly reflect more heat back into space.  I've been playing around with inventing a Mars game (pun intended) and have been trying to figure out how to model this.

Warm regards, Rick.

#146 Re: Terraformation » Terraforming the Earth’s great Deserts - Turning the Sahara into a rainforest. » 2007-05-09 00:03:59

Because of the way the air circulates there are regions about 15 degrees off the equator that get little rain fall.  However the Sahara got enough rain to support grasslands and farms until over grazing caused massive desertfication. 

With massive efforts we might be able to get that grassland back but I doubt that the Sahara will ever become a rain forest.  (At least not until it moves to a different latitude via plate tectonics.)

Sadly it is far easier to grow deserts than to shrink them. 

Warm regards, Rick.

#147 Re: Terraformation » Angular Momentum and Planetary Dynamos » 2007-05-08 23:46:59


And now here are the concerns for each:
1) Can we move a mass the size of an asteroid both with the speed and the precision to bring it into orbit around another body? This means both overcoming its initial inertia and orbital mechanics and then braking imparted inertia to bring about orbit?

Bryan

Sure, if you can move an asteriod it is not that much more difficult to put it into an orbit.  The trick is to start with a distant orbit around Mars and then thrust for a few minutes at the furthest point of the elipse to circularize it and make it shrink.


a) As a subset of this method, would it be feasible to accrete matter onto either Phobos or Deimos? They are, after all, already in orbits and that is the most difficult part of the whole enterprise.
b) What is the mass of these sets of asteroids available for moon-building? Are there enough NVAs to create a satellite with enough gravity to form itself into a sphere? Likewise with the NMAs? Perhaps more with Mars than with Venus. I'd like to pair up Eros with Venus ....   wink

Bryan

Sure, but it is not that hard to get an orbit.

I don't have the numbers before me but I doubt that there are enough NMA to make a circular moon.  The moon has to get 800 to 900 km in diameter to squish into a sphere and that requires a LOT of asteriods.  However by heating them we can make it a lot easier for them to slump together.



2) Can we build a moon from scratch, a la Death Star fashion? I would not want to attempt this with Mars, but I have seen several proposals on here for Venus, as a depository for excess carbon. I'd rather see it take excess sulphur personally, but let's play with this. You'd want to begin with a hollow iron sphere positioned in orbit. Perhaps magnetise the whole sphere to encourage passive accretion by space dust?

Or would solar energy rob it of its field?


Bryan

Most space dust is not magnetic.

The solar wind would not rob a perminant magnet of its field.  An electro-magnet would do work on the solar wind and thus would require more energy to be constantly be fed into it.


Could we lift enough carbon and sulphur out of the Venus gravity well to make this work? At what point would there be enough matter on the surface of this moon to shield the hollow core from solar radiation and other interference? If it could be shielded, then a metallic magnetised core could be built inside.

Bryan

No reason we couldn't lift all of Venus out of Venus' gravity field with enough energy.  Speaking practically tho, I can not see this happening even with a He3 economy.

As for shielding the magnetic field generators inside; you can't have it both ways.  If you want to have a magnetic field to do work on the solar wind, than the solar wind will do work on you.  If you shield your inner magnets with mu metal or superconductors, then the field won't reach outside your shield.



3) Lobbing impactors at planets is the cheapest way to add energy into a planetary system, but the process is inherently chaotic and we cannot know all the consequences of our actions in advance. After all, it was impactors on Mars which brought pieces of Mars to our Antarctica. And impactors on Luna send bits of moonrock down here to us. I'm guessing impactors on Venus might have consequences only for Mercury, but can we be sure? Impactors affect angular momentum, but do not create moons, unless we are talking about Velikovskian collisions.

Bryan

Huge impacts on Venus would almost certainly put crud into space that would find its way to Earth.  However most will take millions of years to get here, be small and be spread out widely over time.  So it wouldn't worry me too much.


Which brings us to the related topic of angular momentum. Does giving a planet a moon help angular momentum? I expect not, but perhaps there are better informed people on here.

Bryan

I'm not sure what you mean by help angular momentum.  But a tiny amount of mass in orbit holds a giant amount of angular momentum.  For example, all the planets masses added together are less than 1/1000 the mass of the sun, but the planets hold more than 99% of the solar systems angular momentum.

Mars has no moon so its obliquity precess far more than the Earth's.  Even a relatively small amount of mass in an orbit will significantly stabilize the system.  So I think the answer to your question is a yes.


Earth got its Moon out of a cataclysmic collision in the early solar system. ...

I wonder if there will come a time in the far future when the radius of Luna will exceed the distance between its orbital path and L1? Then it could break free.

Bryan

Luna is actually composed of mantle level rocks with high melting points.  The L1 point will always stay between the Earth and Luna as is a mathematical construct based on the mass of Luna and Earth itself.  Yes, people say that before the solar system ends, Luna will escape Earth orbit and enter orbit around the sun.  From there it could either hit the Earth, end up in orbit again or get kicked further away.


Late collisions of massive objects were a feature of the solar system in the first 100 Ma or so. Each orbit had more than one contender for dominance because accretion was happening everywhere at once. Ever wonder how Uranus got knocked over on its side? Or why its magnetic axis is off center from its geometric axis (ie: not tilted, but displaced -- not passing through the core)? It got knocked over.

Bryan

The angle of the magnetic field has to do with the flow of charged particles and interference with the solar magnisphere.  Also a planetary magnetic field is temporary.  Uranus' magnetic field has built up the way it is thru recent chance and physics not because of a late impact.  However late impacts are the accepted reason why it is tilted on its side.



Venus also experienced a late collision of cataclysmic proportions. Its orbital plane is slightly tilted to the solar ecliptic. It is not merely tidally locked to the Sun, but slightly retrograde. Venus got punched head-on by its Langrange companion. Consequently its energy was not added into the planet but subtracted. It got stopped nearly dead in its tracks. This depleted its full store of angular momentum. It engulfed its impactor. And the full thick silicate crust remained behind, which is another reason for the runaway greenhouse.

Bryan

If you are talking about a large body in the Venus - Sun L4 or L5 point it can't be that large.  L4 & 5 are only stable if the small body in those points are 5% or less of the mass of the planet.



Having said all this, I do not know how we can impart more angular momentum to Mars or Venus through use of a moon. The only way I can see is to use iron-nickel impactors aimed off-center with the direction of rotation. With Venus, even this may not work -- because its motion is retrograde, the planet would have to be slowed, stopped, reversed, to get it spinning in the right direction. And it would be *very* unstable. And it would add heat to Venus. :shock:

Bryan

Sure this would work.  You would need a huge amount of mass and Venus (for terraforming) would actually like to lose mass.  But speading up the Martian day (to even out more the temperature swings) while adding mass and heat to Mars would be very welcome.


I'd like to ship all Earth's plutonium to Mars and drop it into the core. That would put starch in its sails.....

Bryan

99.9999% of the Plutonium on Earth is man made (with the exceptions of that natural breeder reactor in the Congo).  There is not enough made to put a dent on Mars' core.


Thanks for the interesting post StarDreamer.

Warm regards, Rick.

#148 Re: Terraformation » What would be the optimal orbit for the moon? » 2007-05-08 23:15:18

I am assuming that you are talking about the tilt of a large artifical Martian moon and not Luna. 

Tides will bring any moon into an orbit over the equator of the primary in a fairly short time period (speaking of geologic eras here).  These tides will generate heat in both the moon and Mars.  Since we want Mars to stay vocanically active, we are better off giving it as high an axal tilt as we can get away with.

Since we are talking about moving a lot of mass around it will have to be not far from the ecliptic.  Shame that.

Warm regards, Rick.

#149 Re: Terraformation » What would be a more efficient way to use excess mass? » 2007-05-08 23:10:18

A small moon can hold a tremendous amount of angular momentum which is directly useful in stabalizing the degree that the planet tilts over many thousands of years.  It will stretch the crust and add heat to Mars thru tides.  It can be put into a decaying orbit (via rotation periods and mass concentrations) so after many million years it will hit Mars adding heat an mass to the planet and (perhaps) starting volcanoes and a MASSOUTFLO event.

All of these advantages can be had for many orders of magnitude less than trying to build up Mars' mass by a significant amount.

Nice question.

Warm regards, Rick

#150 Re: Terraformation » How Quickly Does Mars Lose Air? » 2007-05-08 23:03:07

noosfractal,
I wonder if just having a metal dust ring spinning around the planet would make its own mag field?

If you put a charge on the dust it will create a magnetic field.

This magnetic field will accelerate your dust and it soon won't be in orbit anymore.

Rick

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