Dyson Spheres (New Scientist 17.5.25)
Timothy Collinson
(16 May 2025 16:40 UTC)
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Re: [TML] Dyson Spheres (New Scientist 17.5.25) Alex Goodwin (17 May 2025 05:20 UTC)
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Re: [TML] Dyson Spheres (New Scientist 17.5.25)
Timothy Collinson
(17 May 2025 17:02 UTC)
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Re: [TML] Dyson Spheres (New Scientist 17.5.25)
Alex Goodwin
(17 May 2025 17:21 UTC)
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Re: [TML] Dyson Spheres (New Scientist 17.5.25)
Timothy Collinson
(18 May 2025 14:13 UTC)
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Re: [TML] Dyson Spheres (New Scientist 17.5.25)
Alex Goodwin
(19 May 2025 03:42 UTC)
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Re: [TML] Dyson Spheres (New Scientist 17.5.25)
Timothy Collinson
(19 May 2025 11:06 UTC)
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Operation Kessler - was Re: [TML] Dyson Spheres (New Scientist 17.5.25)
Alex Goodwin
(19 May 2025 13:29 UTC)
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On 17/5/25 02:39, Timothy Collinson - timothy.collinson at port.ac.uk (via tml list) wrote: > I had a chance to grab a quick look at the latest New Scientist (17th > May 2025) whilst at work yesterday. > > Highlight (or, to be fair, perhaps the most useful(?) for Traveller), was: > > *Alien Dyson Spheres may self-destruct before we spot them* - Alex > Wilkins, p.10 > swarms of satellites would probably be plagued by an avalanche-like > cascade of collisions - at their orbital speeds that could be disastrous > even a swarm of fewer, larger satellites or those placed in thin > orbital shells to avoid satellites crossing paths, couldn't last much > longer than a million years unless actively managed, > arXiv, doi.org/pmg3 <http://doi.org/pmg3> > we are thus unlikely to come across them after alien civilization has > gone extinct as they are "only visible while being used" > Given an initial, exactly-centred-on-system-barycentre setup for a dyson _shell_, _any_ perturbation from that results in one chunk of the structure being a little closer to barycentre, and as a result, the chunk on the opposite side, will result in a net gravitational force pulling the closer chunk yet closer to barycentre unless counteracted. That's an additional failure mode to consider. ObTrav: The well-armed lunatics (ie, PCs) come across an Ancient-built dyson sphere (of whatever subtype) in the process of embuggerising itself via turbo-Kessler as outlined in that paper you linked to. > I did have one question though, is it still a Dyson Sphere when it's a > 'swarm' or is that something else? Oh hang on, I've got Blevins' book > _Megastructures, that will have the answer. > And indeed it does: > Dyson Spheres are made up of three kinds: > - Dyson Swarms/Rings > - Dyson Bubbles (statites with solar sails to keep them 'in place') > - Dyson Shells (what I was thinking of as a Dyson Sphere) > > My apologies if you all already knew that. But it might save someone > looking it up. > > (Also: Highly recommend _Megastructures_!) > > My mind still boggles at the amount of real estate any of the above > would offer a budding traveller. > > tc > For a prototypical dyson shell around a G2 class dwarf (such as the star closest to Terra), a 1 AU shell would give 549,316,406.25 x the surface area of a planet like Terra- call it 550 million times more surface area. Coruscant-level population (of 1 quintillion - billions being pop code A, trillions being pop code D, quadrillions being pop code G, and quintillions being pop code K (skipping I)) on the planet would, assuming linear scale up with area, result in approx 550 septillion population (sextillions being pop code N, septillions being pop code R (skipping O), so hundreds of septillions would be pop code T). That's assuming only _one_ significant layer of habitation, on both sides. I leave infrastructure for such a population centre to the reader. Alex