home *** CD-ROM | disk | FTP | other *** search
- Path: sparky!uunet!usc!news.bbn.com!hsdndev!dartvax!Frederick.A.Ringwald
- From: Frederick.A.Ringwald@dartmouth.edu (Frederick A. Ringwald)
- Newsgroups: sci.space
- Subject: Re: Dyson Spheres, again
- Message-ID: <1992Nov23.020045.15067@dartvax.dartmouth.edu>
- Date: 23 Nov 92 02:00:45 GMT
- References: <wf2gt=G00VoyMYglpu@andrew.cmu.edu>
- <ewright.722280175@convex.convex.com>
- Sender: news@dartvax.dartmouth.edu (The News Manager)
- Organization: Dartmouth College, Hanover, NH
- Lines: 80
- X-Posted-From: InterNews1.0b1@newshost.dartmouth.edu
-
- In article <ewright.722280175@convex.convex.com>
- ewright@convex.com (Edward V. Wright) writes:
-
- > Well, Dyson himself did not actually propose a solid sphere, which would
- > require materials that are not only unavailable but unreasonably strong,
- > given our understanding of physics. What he invisioned was a large number
- > of habitats in orbit about a star which, together, would completely
- > encircle the star in a ball-of-twine formation. From a distance, it would
- > look like a solid shell.
-
- Have you read Dyson's original article? I have it here in front of me.
- He says:
-
- "The material factors which ultimately limit the expansion of a
- technically advanced species are the supply of matter and the supply of
- energy...The reader may well ask in what sense can anyone speak of the
- mass of Jupiter or the total radiation from the sun as being accessible
- to exploitation...the mass if Jupiter, if distributed in a spherical
- shell revolving around the sun at twice the Earth's distance from it,
- would have a thickness such that the mass is 200 grams per square
- centimeter of surface area (2 to 3 meters, depending on the density). A
- shell of this thickness could be made comfortably habitable, and could
- contain all the machinery required for exploiting the solar radiation
- falling onto it from the inside."
-
- This sounds like a solid sphere to me. He goes on to say:
-
- "If the foregoing argument is accepted, the the search for
- extraterrestrial intelligent beings should not be confined to the
- neighborhood of visible stars. The most likely habitat for such bveings
- would be a dark object, having a size comparable with the Earth's
- orbit, and a surface temperature of 200 deg to 300 deg K. Such a dark
- object would be radiating as copiously as the star which is hidden
- inside it, but the radiation would be in the far infrared, around 10
- microns wavelength."
-
- The jist of my (month-old) posts was that even if Dyson's basic idea is
- right, the details probably aren't. A genuine Dyson sphere probably
- would have plenty of starlight shining through it: a solid shell 2 or 3
- meters in thickness simply would not be rigid enough to withstand the
- pressure of the sun's gravity, unless made of material with properties
- that don't look too plausible. In other words, a Dyson sphere probably
- would not be a dark object. It would more probably look like a normal
- F-K dwarf, with a slight IR excess that might be hard to distinguish
- from a quite-natural circumstellar dust shell or ring.
-
- Then again, never second-guess an alien intelligence. Ideas about
- completely reworking a planetary system, often involving draining
- matter off the star, come to me in the night, and force me to conclude
- that, like most things in SETI, there's an infinity of possibility even
- within the narrow confines of the known laws of physics. We really
- don't even know enough to ask intelligent questions. Jill Tarter is
- taking as flexible approach as she can with the NASA HRM survey, and it
- may well be that the SETI project that succeeds will be done by
- astronomers with SETI initially being the farthest thing from their
- minds. (Then again, watch out for fascinating false alarms, such as
- Martian canals, pulsars, and gamma ray bursts.)
-
- By the way, the idea of a swarm of independent space habitats wasn't
- Freeman Dyson's, it was Gerard O'Neil's, circa the late '60s, about ten
- years after Dyson's 1960 paper, which I quote above. I know,
- Tsiolkovsky, Bernal, and a legion of sci-fi writers had thought of it,
- too, but the credit still should go to O'Neill for getting the
- technical community to take the concept at least halfway seriously, as
- a place to live and not just an orbiting laboratory, and as something
- more than strictly sci-fi. After all, his 1974 paper did make the front
- cover of Physics Today.
-
- I recommend to anyone a look at Dyson's original paper; the reference
- is:
-
- Dyson, F. J. 1960, Science, vol. 131, p. 1667 (No. 3414, 1960 June 3).
-
- You'll see immediately it's a one-pager, in the fine tradition of Fermi
- (i.e., say your piece and get out). While looking up this paper, I came
- across an interesting ad, in the same volume: a 1960 announcement that
- Werner von Braun had just left the U.S. Army Redstone Arsenal to join
- NASA, with a photo of him talking with several Mercury astronauts,
- including Gordon Cooper and John Glenn - before their space flights, of
- course. (Thanks goodness hairsyles have changed!)
-