What percent of the sun would a Dyson Sphere cover?
post by Raemon · 2024-07-03T17:27:50.826Z · LW · GW · 22 commentsThis is a question post.
Contents
Answers 23 gilch 18 Eccentricity 4 J Bostock None 22 comments
I disagreed with a bunch of the implications of this comment [LW(p) · GW(p)], but I was curious about the specific question "Would a dyson sphere made out of the solar system necessarily cover (most of) the sun?" (and therefore block out a substantial fraction of light coming to Earth).
The subquestions here seem to be (at first glance, not a physicist)
- What are efficient Dyson spheres probably made of?
- What percent of the solar system can be converted into Dyson-sphere material?
- Are gas giants harvestable?
- How long would it take to harvest that material?
- What would the radius of a Dyson sphere be? (i.e. how far away from the sun is optimal). How thick?
- If the sphere is (presumably) lots of small modules, how far apart are they?
I don't know if there's already been a canonical answer written up somewhere. The original motivating question was "if an AI is moderately 'nice', leaves Earth alone but does end up converting the rest of the solar system into a Dyson sphere, how fucked is Earth? (also, on what timescale?).
I don't know that this question actually makes sense (as another commenter mentioned, if the AI is that nice, it can probably also redirect sunlight to Earth at low cost. But, I'm still just curious about the details. (I have enough uncertainty about how the future plays out that it seems nice to understand some of the physical limits involved)
Answers
What are efficient Dyson spheres probably made of?
There are many possible Dyson sphere designs, but they seem to fall into three broad categories: shells, orbital swarms, and bubbles. Solid shells are probably unrealistic. Known materials aren't strong enough. Orbital swarms are more realistic but suffer from some problems with self-occlusion and possibly collisions between modules. Limitations on available materials might still make this the best option, at least at first.
But efficient Dyson spheres are probably bubbles. Rather than being made of satellites, they're made of statites, that is, solar sails that don't orbit, but hover. Since both gravitational acceleration and radiant intensity follow the inverse square law, the same design would function at almost any altitude above the Sun, with some caveats. These could be packed much more closely together than the satellites of orbital swarms while maybe using less material. Eric Drexler proposed 100 nm thick aluminum films with some amount of supporting tensile structure. Something like that could be held open by spinning, even with no material compressive structure. Think about a dancer's dress being held open while pirouetting and you get the idea.
The radiation needs to be mostly reflected downwards for the sails to hover, but it could still be focused on targets as long as the net forces keep the statites in place. Clever designs could probably approach 100% coverage.
What percent of the solar system can be converted into Dyson-sphere material? Are gas giants harvestable?
Eventually, almost all of it, but you don't need to to get full coverage. Yes, they're harvestable; at the energy scales we're talking about, even stellar material is harvestable via star lifting. The Sun contains over 99% of the mass of the Solar System.
How long would it take to harvest that material?
I don't know, but I'll go with the 31 years and 85 days [LW(p) · GW(p)] for an orbital swarm as a reasonable ballpark. Bubbles are a different design and may take even less material, but either way, we're talking about exponential growth in energy output that can be applied to the construction. At some point the energy matters more than the matter.
What would the radius of a Dyson sphere be? (i.e. how far away from the sun is optimal). How thick?
I'd say as close to the Sun as the materials can withstand (because this takes less material), so probably well within the orbit of Mercury. Too much radiation and the modules would burn up. Station keeping becomes more difficult when you have to deal with variable Solar wind and coronal mass ejections, and these problems are more severe closer in.
The individual statite sails would be very thin. Maybe on the order of 100 nm for the material, although the tensile supports could be much thicker. I don't know how many sails an optimal statite module would use (maybe just 1). But the configuration required for focus and station keeping probably isn't perfectly flat, so a minimal bounding box around a module could be much thicker still.
An energy efficient Dyson Sphere probably looks like a Matrioshka brain, with outer layers collecting waste heat from the inner layers. Layers could be much farther apart than the size of individual modules.
If the sphere is (presumably) lots of small modules, how far apart are they?
Statites could theoretically be almost touching, especially with active station keeping, which is probably necessary anyway. What's going to move them? Solar wind variation? Micrometor collisions? Gravitational interactions with other celestial bodies? Remember, statites work about the same regardless of altitude, so there can be layers with some amount of overlap.
"if an AI is moderately 'nice', leaves Earth alone but does end up converting the rest of the solar system into a Dyson sphere, how fucked is Earth?
Very, probably. And we wouldn't have to wait for the whole (non-Sun) Solar System to be converted before we're in serious trouble.
The planet Mercury is a pretty good source of material:
Mass: kg (which is about 70% iron)
Radius: m
Volume: m^3
Density: kg/m^3
Orbital radius: m
A spherical shell around the sun at roughly same radius as Mercury's orbit would have a surface area of m^2, and spreading out Mercury's volume over this area gives a thickness of about 1.4 mm. This means Mercury alone provides ample material for collecting all of the Sun's energy via reflecting light – very thin spinning sheets could act as a swarm of orbiting reflectors that focus sunlight onto large power plants or mirrors that direct it to elsewhere in the solar system. Spinning sheets could be made somewhere between 1-100 μm thick, with thicker cables or supports for additional strength, perhaps 1-10 km wide, and navigate using radiation pressure (using cables that bend the sheet, perhaps). Something like or mirrors would be enough to intercept and redirect all of the sun's light.
The gravitational binding energy of Mercury is on the order of J, or on the order of an hour of the Sun's output. This means in theory the time it takes for a new mirror to pay it's own manufacturing energy cost is in principle quite small; if each kg of material from Mercury is enough to make on the order of 1-100 square meters of mirror, then it will pay for itself in somewhere between minutes and hours (there are roughly 10,000 w/m^2 of solar energy at Mercury's orbit, and each kg of material on average requires on the order of J to remove). Only 40-80 doublings are required to consume the whole planet depending on how thick the mirrors are and how much material is used to start the process. Even with many orders of magnitude of overhead to account for inefficiency and heat dissipation, I believe Mercury could be disassembled to cover the entire sun with reflectors on the order of years and perhaps as quickly as months; certainly within decades.
Ooh boy this is a fun question:
For temperature reasons, a complete Dyson sphere is likely to be built outside the earth, as the energy output of the sun would force one at 1 A.U. to be 393K = 119 C. I assume the AI would prefer not to run all of its components this hot. A sphere like that would cook us like an oven unless the heat dissipating systems somehow don't radiate any energy back inwards (which is probably impossible).
A Dyson swarm might well be built at a mixture of inside and outside the earth's orbit. In that case the best candidate is to disassemble mercury, using solar energy to power electrolysis to turn the crust into metals, send up satellites to catch more sunlight, and focus that back down to the surface.
Mercury orbits at 60 million km from the sun. This means a circumference of 360 million km. The sun is 1.2 million km across, but because it's at 0.38 au from the sun, a band which blocks out the sun for the earth entirely would only need to be 0.8 million km. This gives a total surface area of 290e12 square kilometers to block out the sun entirely. Something like a Dyson belt.
If the belt is 1 m thick on average, this gives it a total volume of 290e18 cubic meters. Mercury has a volume of 60 billion cubic km = 60e18 cubic meters. This would blot out approximately 1/5 of the sun's radiation.
To put things in perspective, Mars is kinda maybe almost habitable with a lot of effort and gets less than 1/2 of the sun's radiation. I would make a wild guess that with 80% of the solar radiation we could scrape by with immense casualties due to massive decreases in agricultural yield. Temperature is somewhat tractable due to our ability to pump a bunch of sulfur hexafluoride into the atmosphere to heat things up.
As a caveat, I would suggest that if the AI is "nice" enough to spare Earth, it's likely to be nice enough to beam some reconstituted sunlight over to us. A priori I would say the niceness window for "unwilling to murder us while on earth, and we pose a direct threat, but unwilling to suffer the trivial cost of keeping the lights on" is extremely narrow.
↑ comment by Raemon · 2024-07-03T19:05:08.456Z · LW(p) · GW(p)
As a caveat, I would suggest that if the AI is "nice" enough to spare Earth, it's likely to be nice enough to beam some reconstituted sunlight over to us.
Yeah seems right. I still find myself curious, as well as strategically interested in "man, I just really don't know how the future is likely to play out, so getting more clarity on physical limits of this sort of system feels like it helps constrain possible future scenarios." That might just be cope though.
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comment by Garrett Baker (D0TheMath) · 2024-07-03T18:05:50.196Z · LW(p) · GW(p)
Armstrong & Sanders answer many of these questions in Eternity in Six Hours:
The most realistic design for a Dyson sphere is that of a Dyson swarm ([32, 33]): a collection of independent solar captors in orbit around the sun. The design has some drawbacks, requiring careful coordination to keep the captors from colliding with each other, issues with captors occluding each other, and having difficulties capturing all the solar energy at any given time. But these are not major difficulties: there already exist reasonable orbit designs (e.g. [34]), and the captors will have large energy reserves to power any minor course corrections. The lack of perfect efficiency isn't an issue either, with W available. And the advantages of Dyson swarms are important: they don't require strong construction, as they will not be subject to major internal forces, and can thus be made with little and conventional material.
The lightest design would be to have very large lightweight mirrors concentrating solar radiation down on focal points, where it would be transformed into useful work (and possibly beamed across space for use elsewhere). The focal point would most likely some sort of heat engine, possibly combined with solar cells (to extract work from the low entropy solar radiation).
The planets provide the largest source of material for the construction of such a Dyson swarm. The easiest design would be to use Mercury as the source of material, and to construct the Dyson swarm at approximately the same distance from the sun. A sphere around the sun of radius equal to the semi-major axis of Mercury's orbit ( m) would have an area of about m^2.
Mercury itself is mainly composed of 30% silicate and 70% metal [35], mainly iron or iron oxides [36], so these would be the most used material for the swarm. The mass of Mercury is kg; assuming 50% of this mass could be transformed into reflective surfaces (with the remaining material made into heat engines/solar cells or simply discarded), and that these would be placed in orbit at around the semi-major axis of Mercury's orbit, the reflective pieces would have a mass of:
Iron has a density of 7874 kg/m^3, so this would correspond to a thickness of 0.5 mm, which is ample. The most likely structure is a very thin film (of order 0.001 mm) supported by a network of more rigid struts.
They go on to estimate how long it'd take to construct, but the punchline is 31 years and 85 days.
Replies from: Raemon↑ comment by Raemon · 2024-07-03T18:27:40.010Z · LW(p) · GW(p)
A thing I'm still not sure about reading that is "what percent of the light is getting through?". Like, how dense are the reflector modules?
Later in the paper it says "The Dyson sphere is assumed to have an efficiency of one third", which could mean "realistically you only capture about 1/3rd of the energy in the first place" or "the capturing/redirecting process" loses 2/3rds of the energy.
Replies from: D0TheMath, Charlie Steiner↑ comment by Garrett Baker (D0TheMath) · 2024-07-03T18:45:27.766Z · LW(p) · GW(p)
They're probably basing their calculation on the orbital design discussed in citation 34: Suffern's Some Thoughts on Dyson Spheres whose abstract says
According to Dyson (1960), Malthusian pressures may have led extra-terrestrial civilizations to utilize significant fractions of the energy output from their stars or the total amount of matter in their planetary systems in their search for living space. This would have been achieved by constructing from a large number of independently orbiting colonies, an artificial biosphere surrounding their star. Biospheres of this nature are known as Dyson spheres. If enough matter is available to construct an optically thick Dyson sphere the result of such astroengineering activity, as far as observations from the earth are concerned, would be a point source of infra-red radiation which peaks in the 10 micron range. If not enough matter is available to completely block the stars’ light the result would be anomalous infra-red emission accompanying the visible radiation (Dyson 1960).
Bolded for your convenience. Presumably they justify that assertion somewhere in the paper.
↑ comment by Charlie Steiner · 2024-07-04T01:09:53.937Z · LW(p) · GW(p)
Imperfect efficiency isn't because it's transparent (as everyone keeps trying to say, it doesn't have to let through any sunlight at all) - it's because of Carnot efficiency. If you want to convert sunlight into electrical energy, you can't do it perfectly, which means your Dyson swarm heats up, which means it radiates light in the infrared.
So if 2/3 of the sun's energy is getting re-radiated in the infrared, Earth would actually stay warm enough to keep its atmosphere gaseous - a little guessing gives an average surface temperature of -60 Celsius.
Replies from: D0TheMath↑ comment by Garrett Baker (D0TheMath) · 2024-07-04T17:23:46.168Z · LW(p) · GW(p)
So if 2/3 of the sun's energy is getting re-radiated in the infrared, Earth would actually stay warm enough to keep its atmosphere gaseous - a little guessing gives an average surface temperature of -60 Celsius.
That is, until the Matrioshka brain gets built, in which case assuming no efficiency gains, the radiation will drop to 44% of its original, then 30%, then 20%, etc.
Replies from: Nick_Tarleton↑ comment by Nick_Tarleton · 2024-07-05T04:23:37.032Z · LW(p) · GW(p)
A shell in a Matrioshka brain (more generally, a Dyson sphere being used for computation) reradiates 100% of the energy it captures, just at a lower temperature.
Replies from: Charlie Steiner↑ comment by Charlie Steiner · 2024-07-05T16:49:18.589Z · LW(p) · GW(p)
Yeah, the energy radiated to infinity only gets reduced if it's being used for something long-term, like disassembling the sun or sending off energy-intensive intergalactic probes.
comment by jaan · 2024-07-04T05:56:45.671Z · LW(p) · GW(p)
dyson spheres are for newbs; real men (and ASIs, i strongly suspect) starlift.
Replies from: Wei_Dai↑ comment by Wei Dai (Wei_Dai) · 2024-07-04T07:05:40.943Z · LW(p) · GW(p)
Yes, advanced civilizations should convert stellar matter 100% into energy using something like the Hawking radiation of small black holes, then dump waste heat into large black holes.
Replies from: jaan, ryan_greenblatt↑ comment by jaan · 2024-07-05T06:28:13.089Z · LW(p) · GW(p)
interesting! still, aestivation seems to easily trump the black hole heat dumping, no?
Replies from: Wei_Dai↑ comment by Wei Dai (Wei_Dai) · 2024-07-05T07:13:33.510Z · LW(p) · GW(p)
From Bennett et el's reply to the aestivation paper:
Thus we come to our first conclusion: a civilization can freely erase bits without forgoing larger future rewards up until the point when all accessible bounded resources are jointly thermalized.
They don't mention black holes specifically, but my interpretation of this is that a civilization can first dump waste heat into a large black hole, and then later when the CMB temperature drops below that of the black hole, reverse course to use Hawking radiation of the black hole as energy source and CMB as heat sink.
If we only consider thermodynamics (and ignore how technologically feasible this is), I think this should net you the same amount of total computation over time, but allow you to do a lot of it earlier.
Replies from: ryan_greenblatt↑ comment by ryan_greenblatt · 2024-07-05T17:54:06.008Z · LW(p) · GW(p)
I don't think you can feasibly use the Hawking radiation of large black holes as an energy source in our universe (even if you are patient).
My understanding is that larger black holes decay over ~ years. I did a botec a while ago and found that you maybe get 1 flop every years or so on average if we assume perfect efficiency and very few bit erasures in our reversible computing approach (I think I assumed about 1 bit erasure per or something?). I don't think you can maintain a mega structure around a large black hole capable of harvesting this energy which also can survive this little energy. (I think quantum phenomena will decay your structure way too quickly.)
Replies from: Wei_Dai↑ comment by Wei Dai (Wei_Dai) · 2024-07-06T01:40:14.017Z · LW(p) · GW(p)
In that case, don't dump waste heat into black holes so large that it's impossible to use them as eventual energy sources. Instead dump waste heat into medium sized black holes, which can feasibly be used as eventual energy sources.
Replies from: ryan_greenblatt↑ comment by ryan_greenblatt · 2024-07-06T03:15:15.317Z · LW(p) · GW(p)
I think the size might have to be pretty precise to get this right (I think decay duration is cubic in mass), so they'd probably need to be engineered to have a particular size. (E.g. add mass to a small black hole until it hits the right size.)
But, yeah, with this constraint, I think it can maybe work. (I don't know the decay duration for the smallest naturally occurring black holes. But as long as this is sufficient low, the proposal works.)
↑ comment by ryan_greenblatt · 2024-07-04T15:34:33.574Z · LW(p) · GW(p)
(If the small black hole thing works out - it is non-obvious that this will be achievable even for technologically mature civilizations.)
Replies from: gilch, Wei_Dai↑ comment by gilch · 2024-07-04T21:05:59.035Z · LW(p) · GW(p)
Specifically, while the kugelblitz is a prediction of general relativity, quantum pair production from strong electric fields makes it infeasible in practice. Even quasars wouldn't be bright enough, and those are far beyond the energy level of a single Dyson sphere. This doesn't rule out primordial black holes forming at the time of the Big Bang, however.
It might still be possible to create micro black holes with particle accelerators, but how easy this is depends on some unanswered questions about physics. In theory, such an accelerator might need to be a thousand light years across at most, but this depends on achievable magnetic field strength. (Magnetars?) On the other hand, if compactified extra dimensions exist (like in string theory), the minimum required energy would be lower. One that small would evaporate almost instantly though. It's not clear if it could be kept alive long enough to get any bigger.
↑ comment by Wei Dai (Wei_Dai) · 2024-07-04T23:02:41.974Z · LW(p) · GW(p)
If it doesn't work, whoever designed this universe should be fired for ruining such an elegant scheme. :)
comment by quetzal_rainbow · 2024-07-03T18:50:50.370Z · LW(p) · GW(p)
Integral mass of inner planets is kg. Upper bound on density of planets is 5000 . If we set thickness of sphere to 1m, we are getting surface of , while surface area of the Sun is . Radius of such sphere is approximately ~ 0.1 AU, which is ~20x radius of the Sun. You can worry about too much heat, but if you can harvest atmospheres of planets, you can put all these gasses into cooling system, increasing overall efficiency.
comment by Dagon · 2024-07-03T18:17:58.382Z · LW(p) · GW(p)
This discussion is not new, and AI doesn't change much about the unknowns and impossibilities. Dyson sphere - Wikipedia says the idea's been around since 1937, though only named after Freeman Dyson in 1960, and injected into popular consciousness by Larry Niven's 1970 novel Ringworld. Ringworld is a more likely IMO structure than a Dyson sphere (because it solves the gravity problem, though it still handwaves the materials question), but really neither are likely to be all that interesting to non-biological intelligence.
If you don't need an ecosystem with a self-sustaining solar/plant/animal energy cycle, you're probably better off with many smaller solar-orbital structures, closer to asteroid-field than planets or large-surface stable structures. If you're thinking bigger than that, it's not clear that you need to concentrate in solar systems - break up the Sun as fuel for your diaspora of perenneal-ships.
↑ comment by Raemon · 2024-07-03T18:28:12.958Z · LW(p) · GW(p)
Nod, but, this doesn't answer the actual question.
Replies from: Dagon↑ comment by Dagon · 2024-07-03T19:04:28.958Z · LW(p) · GW(p)
Ok, but the question is unanswerable. It's not known how to convert conventional matter into whatever is strong enough for the Dyson sphere, so it's not known how much material is available, it's not known how much coverage it would have, or what diameter it could be built, or what diameter it would be useful.
The explorations I'd seen before assumed using all the non-solar matter in the system to build a sphere with a radius of Earth's orbit. Ringworld solutions tended to use this diameter as well.
Swarm or other partial modifications (which I don't know if there's a term for, but it's not Dyson sphere) will have other answers, but I don't think anyone can answer your questions because it's not currently feasible, and arguably not desirable.
There's no reason a "kind" superbeing couldn't build something that leaves Earth nearly unaffected, but it's unknown how much less efficient it would be than the naive "just use all the inner planets as source material, and to clear out interference".
Replies from: Raemon