Interstellar Colonization

"New World". Artwork by Frank Frazetta

Colonization is fairly straightforwards, though things can turn nasty if the new planets already have natives.

But there are other troubling problems with the concept of colonization, at least for interplanetary non-FTL non-interstellar colonization. Rick Robinsion presents the issues in a cogent manner here on his blog. Go read it right now, I'll wait.

I'd give you some tid-bits of Rick's commentary, except I'd wind up copying his entire essay.

If you are mapping your empire, you will need to figure some sizes. If you decide upon the empire's radius and want to know how many stars and stars with Terran-type planets, use the rules of thumb:

Nstars = Rly^3 * 0.01

NhStars = Rly^3 * 0.0022

where
Rly = empire radius in light years
Nstars = number of stars
NhStars = number of stars with human habitable planets

If you decide upon the number of stars in the empire and want to know it's radius:

Rly = cubeRoot(Nstars * 97)

Rly = cubeRoot(NhStars * 464)

(If your calculator does not have a cube root button, you can use the "Xy" button instead. Type in the number, hit Xy, type in 0.333333333 then hit the equal button.)

Note: the above equations are based upon the work of Jill Tarter and Margaret Turnbull. They were not trying to figure out which stars could host a human habitable planet. They were trying to figure out which stars could host a planet that was not so hideously uninhabitable that no possible form of life could live there. In other words, many of these planets could host alien life forms but would quickly kill an unprotected human being.

If my slide rule isn't lying to me, this works out to an average distance between adjacent stars of 9.2 light years, and an average distance of 15.4 light years between adjacent habitable stars.

Example: In his Flandry of Terra novels, Poul Anderson specified that the Terran Empire was four hundred light years in diameter. How many stars will it probably have? A sphere 400 light years in diameter has a 200 light year radius. 200^3 * 0.01 = 8,000,000 * 0.01 = 80,000 stars. Anderson cites a figure of about four million stars, which means one of us is a bit off the mark (probably me).

Example: You have decided that the NeoRoman Star Empire will contain 10,000 habitable planets. How wide is it? cubeRoot(10,000 * 464) = cubeRoot(5,643,000) = 167 light years radius = 334 light years in diameter.

Note that these rules of thumb were derived by me using an analysis of the Habcat database, and thus could be wildly inaccurate. If you can find better figures, use them, but these are better than no figures at all.

Once you have decided that your Terran Empire is X number of light years wide or contains Y number of stars, it would help to have a realistic number for the amount of years it will take for the empire to expand to that size. Or from the other side, if you have decided how long the empire has been around, it would help to be able to figure out how many stars and how wide it is. This is a little more difficult.

The SETI scientists are always fretting about the Fermi paradox. As a result, there have been a couple of attempts to model the speed of galactic colonization by a hypothetical alien race. These can be used, keeping in mind that they always assume slower-than-light starships. Such models have inhabited planets colonizing nearby worlds. When the population of the colonies grows large enough, they send out their own colonization missions.

A comprehensive but mathematically intensive model is Burning the Cosmic Commons by Robin Hanson. Another interesting model is Computer Simulation of Cultural Drift: Limitations on Interstellar Colonisation by William Sims Bainbridge. I would like to explain how to use them, but I'm still trying to digest the models myself.

Newman & Sagan (Galactic civilizations; population dynamics and interstellar diffusion. Icarus, 46, 293-327) attempted to apply the gas diffusion equation to interstellar migrations.

∂P/∂t = αP (1 - P/Ps) + γΔ2 ∂/∂x (P/Ps ∂P/∂x)

where
P = population of a settlement
Ps = the carrying capacity of a settlement
t = time
x = spatial coordinate
α = local population growth rate (percentage of current population)
γ = emigration rate (percentage of current population)
Δ = mean separation of settlements
∂ = partial differential (Yes, I know. Scary Calculus. But don't panic)

The solution to the equation is:

P/Ps = 1 - exp((x - vt) / L)

where
L = Δ sqrt(2γ / α) = gradient length scale
v = sqrt(αγ / 2) = wave speed

However, when Newman and Sagan analyzed the problem, they came to the belated realization that the local growth rate (α) greatly exceeds the emigration rate (γ) so that L <<Δ. Translated into English, this means that the galactic colonization resembled an explosion more than it did a slow gaseous diffusion. Which means the equation is worthless for this purpose. Back to the drawing board.

Eric M. Jones found a more promising approach. In Discrete calculations of interstellar migration and settlement ( Icarus Volume 46, Issue 3 , June 1981, Pages 328-336. Costs $15 for the article) he uses a Monte Carlo simulation (i.e., rules are established then a lot of dice are metaphorically thrown). Jones found the following equation will approximate the Monte Carlo results:

v = Δr/ [(Δ/vs) + (1/α) ln(2α/γ)]

where
Δr = average radial distance traveled (i.e., distance as meaured from the center of the empire)
Δ = average distance traveled
vs = ship speed
Δx/vs = average travel time (years)

Jones says one can usually assume that Δr = 0.7Δ and neglect the travel time, resulting in:

v = 0.7αΔ / ln(2α/γ)

Artwork by Wally Wood

Assuming the mean separation between settlements (Δ) is 7.2 light years (2.2 parsecs), local population growth rate (α) is 10-3 per year, and the emigration rate (γ) is 10-4 per year, this means the colonization wave will travel at about 2 x 10-3 light-years per year (5 x 10-4 parsecs per year). This would colonize the entire galaxy in a mere 60 million years.

The emigration rate could become much larger. In the 1840's the great Irish emigration reached a whopping 0.01/year. The population of Ireland at the time was about four million, so the emigration was an incredible 40,000 per year or about one hundred per day.

Using the upper equation, with my figure of 8.3 light years for Δ, and a slower-than-light ship speed of 10% c, I figure an expansion wave speed of 1.93 x 10-3 light-years per year. Unfortunately, upping the speed of the ships has little effect. At 50% c it's 1.97 x 10-3 ly/yr, at 100 c it's still 1.97 x 10-3 ly/yr, at ten times the speed of light it's 1.98 x 10-3 ly/yr, and at one thousand times the speed of light it is still 1.97 x 10-3 ly/yr!

At this speed, it would take about 50,000 years to expand to a 100 light year radius empire, which seems like an overly long time to me.

But maybe not. Mr. Jones is talking about a population growth of 10-3 or 0.1% per year. The United States has a growth rate closer to 0.6%, and some nations are crowding 3.0%. If our empire had a growth rate α of 0.6% and a modest emigration rate γ of 10-4 per year, it could reach 100 light years in radius in about 6900 years. And if it had a draconian γ of 10-2, it could reach that size in a mere 260 years.

When Worlds Collide

Issac Kuo questions the assumptions contained in Eric M. Jones's model:

One thing I don't like about these models is that they tend to be based around "average" trip distances and speeds. However, the rate of expansion will be determined by the "pioneering" trip distances and speeds.

The sorts of interstellar propulsion I find plausible involve an incredible amount of initial investment and economic buildup, but then the marginal costs for additional colonization missions are small. This suggests that the third generation of colonization missions might as well be long range missions. The second generation of colonies will have saturated the nearby systems so the only direction to expand is into long range missions.

For example, suppose it takes 5000 years to build up from an initial colony into something that can send out missions of their own. In the meantime, the home system could be sending out colonization missions at a rate of one per decade. By the time the first generation of colonies is up for sending out colonization missions, the nearest 50 systems have already been colonized. The first generation then sends colony ships to fill out the nearest 2500 systems.

Assuming no one has yet bothered to try any long range colonization missions, the result is a compact ball of 2500 colonized systems, of which only a thin shell on the outside can expand with short range missions.

It seems to me plausible that at least some of the "core" systems will embark on long range missions. Maybe some of those long range missions will merely just barely outrun the expanding border. That's a rather short-sighted strategy. Other long range missions will daringly punch across the galaxy, starting up seeds which won't run into the "slowpoke" border for dozens of millenia.

The result is an overall frontier of expansion that is defined by sporadic long range "seed dots". They fill out eventually, but it's entirely plausible for the overall rate of expansion to be entirely defined by far reaching long range high speed missions from the home system or early generation systems.


Rick Robinson:

Just glancing though your section there, the key challenge for a lot of purposes is time scale -- and oddly, it doesn't have much to do with ship speed; an STL civilization might expand over the long haul nearly as fast as an FTL one.

The key issue - and this comes up in all sorts of contexts -- is how long does it take for a planet to go from raw young colony to major world, the kind that could and might send out colonies of its own? This is the basic problem you have to solve for settings in which anyone has a space fleet of their own but Earth.

Let me try to put a few numbers on it.

The threshold for having a space fleet is arguably lower than for colonization, because a planet of 100 million people could probably maintain starships, but probably is not feeling a big population squeeze. To be sure, on some planets the habitable area will be pretty much filled, and even on the more earthlike ones the human presence is getting pervasive, so some impulse to colonize might be developing.

Whether a planet of 10 million people - the equivalent of a single large urban region -- could realistically have a diversified enough economy to maintain and operate a fleet of starships seems a bit iffy, unless they are putting a massive effort into it, so massive that it may stunt their other prospects.

The most likely scenario for a world of 10 million people sending out a colony might be that they've decided their current home sux, and they're going to try their shot at another one.

Looking at the other end, how many people for a viable colony. I'd say 10,000 at the low end, with 100,000 seeming a lot more comfortable. That's the population of one semirural county. How many machine shops and such does it have, how much can they specialize for efficiency, and oh yeah, you need raw material, a mining sector and all that.

If you can't make it you have to import it, paying starship freight instead of truck freight, and what have you got for sale? The market for colony-world curios is going to get crowded fast, and if you really do have something to sell, you'll probably need more than a one-county economy to produce it in commercial quantities.

So I would say that you usually have to put 100,000 people onto a colony planet for it to thrive. Colonies with fewer than that can hang on, but if subsidies are cut off they may die off outright, or be stuck in a marginal existence; only lucky ones will overcome it and do okay.

For a colony to really go as a largely self-sufficient post industrial world it had better have on order of a million people -- more or less the equivalent of Bakersfield and environs. I am certain that Australia has a Bakersfield, but I do not know what it is. Maybe our Oz contingent can inform us.

But once again, if they can't make it or pay starship freight for it they do without it, and the equivalent of Bakersfield has a tough challenge producing nearly all the needs of post industrial civilization. And for exports it is good to have one sizeable airport that can double as the shuttle port and provide steady employment for a lot of the techs.

Big proviso, so hold your pitchforks. This is predicated on the 23rd century, or 28th or whatever, having about the same productive efficiencies of scale that we are used to. If you have got replicators where you shovel dirt in one end and get a washing machine or air car out the other, things are different. But you still need a wide range of human skills, very hard for small communities to provide, maintain, and keep active.

So maybe my figures could all be squeezed down by an order of magnitude, so that a colony of 10,000 is fairly viable, a colony of 100,000 can maintain a full industrial base, and one of a million people can keep its own starships in service. That helps for story settings, but you wouldn't generally expect worlds like that to be active colonizers.

Finally, and most central to time scale, how fast do colony populations grow, either from immigration or birth rate? I would call a million emigrants from Earth each year a benchmark figure for large scale colonization. That's several thousand people each day, one huge ship or several merely big ones, and it still takes a century of sustained effort to plant 100 colonies, each of a million people.

From the colony's point of view, people are another expensive import, if you have to pay them to come. If they can afford a ticket and house stake they will only go to desirable colonies. If someone is paying to ship people to you, you may want to know why, because colonies could be a good place to dump dissidents, minor troublemakers, and similar riffraff.

On the export side, I'm more dubious of shipping off refugees, because by definition you're dealing with lots of them, and shipping them all off world is horribly expensive. Much more so than just plucking the town crank and town pickpocket off the streets and getting them to volunteer for emigration.

But by and large you expect that mass colonization involves people who weren't doing so great on Earth, because the supply of nut enthusiasts like people on this board who would actually like to colonize is limited, and a million people a year is a lot.

The other side of colonial growth is reproductive growth. Doubling the population each generation is about the historical sustained maximum. That corresponds to 10x per century, so Deseret World might go from 100,000 people to 10 million people in 200 years.

But even doubling per century is a pretty robust population growth rate. That's roughly 1.2x per generation. Unless you're growing 'em in vats, about half the women are having three or four kids, and one way or another the society encourages and accommodates itself to this.

It's no given that post industrial societies will generally have this population growth rate, though colony worlds may not follow the current trend in industrialized societies toward ZPG or even less.

If colony populations do tend to grow, I suspect the driving force is not the Heinleinian trope of ranchers with half a dozen marriageable -- and "husband-high" -- daughters, but the pervasive shortage of skilled specialists of all sorts. How this is transmitted to social attitudes I'm not sure, and no doubt can vary widely.

A colony with population doubling each century will go from 100,000 people to 10 million people in about 700 years, pushing us into the second half of the millennium.

Looking at it broadly, say that the age of colonization is around 2250-2350. That is a fairly common time frame for interstellar SF with a geocentric setting; (Star) Trek is vaguely in this era, AD2300 of course, and it's implied by some of Heinlein's interstellar stories.

After a century or so colonization from Earth sputters out, because all the low-hanging fruit has been plucked, and it is increasingly costly to reach virgin planets.

Emigration from Earth to the existing colonies can continue after that, but at some point the rate will likely fall. Successful colonies will no longer want people dumped on them, unsuccessful colonies can't absorb them, so emigration falls to the level of people who can pay to go and want to go, or who the colonies are willing to pay for.

So. At some point around 2400, colonization has tapered off and emigration is tapering off. We can guess that there are at least a dozen or so full colony planets - if you can reach any you can probably reach about that many (and you need a good handful for a decent scenario).

The upward limit is about 100 or so true colony worlds, set - regardless of how many worlds are in reach of your FTL - by the postulated size of the colonization wave. A hundred million people, a hundred worlds - an average of about a million immigrants per colony, though the distribution may well be oligarchic by a power law, a handful of colonies getting a large share of total immigrants, growing to populations of up to a few tens of millions, while most have less than a million and kind of struggle along.

Beyond and between the colonies there may be planets never made into self-sustaining colonies, but remaining as outposts, and likely with some permanent populations. If someone pulls the plug on these, though, don't miss the last bus out. Same with space stations and such.

As with the chronology, I think this is a fairly classical scale for a mid-interstellar setting -- when there are already established colony worlds, that you can get to by starliner, not just outpost transport or even colonization ship.

There are enough worlds for a diverse interstellar setting, but few enough that people who deal with space, at least, will have some notion of them all as distinct places. (The way "Spain" conveys something to you, or "New Delhi," but "Florianópolis" probably does not.

A few of these colonies already in 2400 have upwards of 10 million people and some potential to colonize themselves, but these were the immigration magnets, so they probably still feel short-handed if anything, not inclined to send lots of people off.

It will take 200 or 300 years for smaller colonies with rapid population growth rates to start pushing up into the 10 million population range, and might have the impulse and capability to colonize. But it might take closer to 500 years for a substantial number of the original colonies to have much motivation to colonize.

The early goers, though, will have filled in the next layer of easy pickings. Here is where your FTL really matters - whether you can light off freely into the vastness to hunt for a suitable planet, or are constrained by a colonization sphere that is starting to grow again.

But broadly speaking, it seems that secondary colonization couldn't be expected in any serious way until sometime well after 2500, and perhaps not in a big way till sometime around 2700-3000.


From "Hunters of the Sky Cave" by Poul Anderson

An interstellar domain can have no definite borders; stars are scattered too thinly, their types too intermingled. And there are too many of them. In very crude approximation, the Terrestrial Empire was a sphere of some 400 light-years diameter, centered on Sol, and contained an estimated four million stars. But of these less than half had even been visited. A bare 100,000 were directly concerned with the Imperium, a few multiples of that number might have some shadowy contact and owe a theoretical allegiance.

Consider a single planet; realize that it is a world, as big and varied and strange as this Terra ever was, with as many conflicting elements of race and language and culture among its natives; estimate how much government even one planet requires, and see how quickly a reign over many becomes impossibly huge.

Then consider, too, how small a percentage of stars are of any use to a given species (too hot, too cold, too turbulent, too many companions) and, of those, how few will have even one planet where that species is reasonably safe. The Empire becomes tenuous indeed.

And its inconceivable extent is still the merest speck in one outlying part of one spiral arm of one galaxy; among a hundred billion or more great suns, those known to any single world are the barest, tiniest handful.