A Daily History of Holes, Dots, Lines, Science, History, Math, Physics, Art, the Unintentional Absurd, Architecture, Maps, Data Visualization, Blank and Missing Things, and so on. |1.6 million words, 7500 images, 4.9 million hits| Press & appearances in The Times, Le Figaro, Mensa, The Economist, The Guardian, Discovery News, Slate, Le Monde, Sci American Blogs, Le Pont, and many other places… 5000+ total posts since 2008.

  • Ration Book, 1944: Tanks, Ships, Cannons, Planes.

    JF Ptak Science Books  Quick Post

    There’s a lot to be said about the War Ration Books, but I’ll save that for another time. Right now, I just want to share their hope and beauty:

    WWII rations545

    WWII rations544

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  • A History of Writing for Children (1726)

    JF Ptak Science Books  Post 2373

    In the late 17th century John Comenius (1592-1670) wrote a book about universal (mostly practical) knowledge called The Visible World…, which also happens to be the first illustrated children’s book. It was a book about virtually anything, and everything, and certainly not a book about nothing, because sooner of later Comenius would get to the topic and deal with it, right or wrong.

    The book was originally written in 1676, and translated into English in 1726; in that edition the translator states the purpose of the work:   

    To entice witty children to it, that they may not conceit a torment to be in the school, but dainty/are., For it is apparent, that children (even from their infancy almost) are delighted with Pictures, and willingly please their eyes with these fights: And it will be very well worth the pains to have once brought it to pafs, that fcare-crows may be taken away out of Wifdom’s Gardens…”

    The sections on writing and writing instruments and books are very engaging–they are short and concise, and all of the practicing elements of the illustrations are labelled and identified, which is a major bonus. 

    On Writing

    Children--writing

    [Images from John Comenius,  Orbis Senfualium Piélus: Omnium Principalium in Mundo Rerun/ &f m Vita Alопит,  translated as Pictura et Nomenclatur, the Visible World, or A Nomenclature, and Pictures of all Chief Things that are int he World, translated into English by Charles Hoof…1726.  See an earlier post here for more on Comenius. Image Source:  PROJECT GUTENBERG.]

     

  • Interesting Graphic Display for Aircraft Losses, 1917

    JF Ptak Science Books   Quick PostGraphic aircraft losses 1917548

    This interesting graphic came in a browsing expedition in the July-December 1917 volume of the (Leipzig) Illustrirte Zeitung.  It appeared in the issue #3865 for July 17, 1917, in an article “Fliegererlebnisse” (“Aviation/Flying Experiences”) by Adolf Victor von Koerper. (Koerper was a very interesting man–aviator, early upper-echelon supporter of Adolf Hitler 1922-1926, and then accused and convicted and sentenced-to-death Hitler assassination conspirator.)  The chart shows the success of the German air force against the “Feindliche” (“Hostile”) aircraft, depicting losses (“verluste”) in airplanes and war balloons (“fesselballons”), for January-June, 1917.  According to this German losses were set at 314 aircraft and Allied forces at 1151, with a very high loss rate for (“Bloody”) April.  

  • Interesting Graphic: German Military Forces, 1929

    JF Ptak Science Books  Quick Post

    Graphic Army strength 1929551

    This is for issue #4523, August, 1929 of the Illustrirte Zeitung (Leipzig), “Der Rustungsstand der Machte fur den Landkrieg”, which showed the comparative strengths of leading nations against that of Germany.  As seen in the detail, in 1929 Germany was still abiding by the Treaty of Versailles, which was the peace treaty ending WWI and signed in 1919. The 440-clause treaty spent the first two dozen or so clauses discussing the creation of President Wilson’s League of Nations, while the rest was a distribution of punishment and reparations against/on Germany.  The German military as directed by Versailles was limited to 100,000 soldiers, and had 1926 machine guns, and 2886 cannons.  as stipulated Germany could have no tanks and no air force, and was limited to six ships and no subs, and had to keep the Rhineland free of all armed forces.  This would all be completely changed by 1934, when the Nazis were already well on the way to having a competitive (and modern) fighting force which counted 4.5 million troops.  It would only get worse.  

    Graphic Army strength 1929550

  • German Design, 1922

    JF Ptak Science Books  Quick Post

    Not every ad in the 1920’s  Illustrirte Zeitung was thick and black and heavy and beautifully designed–though there are plenty of them, and they do appeal to me.  This one appears in issue 4083 for May 1922.  

    German graphics Hamburg line556

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  • Astroengineering at Colossally-Advanced Super-Levels: the Dyson^1 Sphere I saw on Star Trek TNG

    -Or-

    How Many Legos Would it Take to Build a  Dyson Sphere Around our Solar System?

    JF Ptak Science Books    Post 2374

    This is the first time I’ve used a footnote in a title and the first time I started out any piece with a footnote—there’s a first time for everything, and then some, like what immediately follows: a  footnote to a footnote of a title.

    Footnote 1: Freeman Dyson has often said over the years that he really doesn’t think that the Dyson sphere should be named for him, but rather for Olaf Stephenson, whose 1937 scifi adventure opened the door to his idea.2

    In our house we sometimes work in silence and sometimes with distraction—the distraction recently has been in the form of Star Trek the Next Generation, and the episode in question was one where there is the discovery of a Dyson Sphere. The “sphere” by quantum electrodynamics Nobel Prize genius and (very) long-time resident of the Institute for Advanced Study at Princeton Freemnan Dyson first envisioned it back in 1959/1960 was a structure necessitated by a terrifically advanced civilization and its need to utilize all of the energy produced by a star. All. So a “sphere” of some sort (spherically symmetric thin shell object) would be constructed to do so, and in the original version by Dyson it would be built via an astroengineering feat of pulverized planet bits:

    “Intelligent beings in another solar system could have hidden their sun by knocking their planets apart and using the pieces to build a hollow ball around their sun”3

    At another level Dyson envisioned making this a more “fluid” environment for our solar system by knocking up Jupiter and distributing its mass to form a spherical shield. In the Star Trek episode, however, Enterprise just about bumps into the invisible sphere which is of god-like construction, solid complexity, and according to what I heard was the size of our solar system. That’s a big thing.

    And who would make such a thing? Gods? Certainly they would be so to us. Luckily the astronomer Nikolai Semenovich Kardashev4 came up with a way of classifying civilizations in a way that makes them conversationally accessible without the godlike qualities making a major entrance.

    The original scale of technological development ranked civilizations on a scale of I to III—our own place on the ride according to Dyson is about .7 It might be easier to describe Type I by describing what it isn’t, which is a Type II, where according to Kardashev there is the possibility of interstellar travel and stellar engineering, which is where the folks from Star Trek the Next Generation live. Type II is not Type III, where the change and influence can be brought to bear on a galaxy-wide order. And so Type IV is III expounded to the level of the universe, which gets us to Type V, wielding control and power on the multiverse level, which are civilizations that can make changes/control universe-sized domains. (In the speculative existence world such entities would be the Q from Star Trek, or the lovable and inexplicably powerful source of a magnetic anomaly near the center of the lunar crater Tycho, represented in the form of a curious black monolith.)

    Dyson’s gedanken experiment is overpowered by Star Trek—I’m not sure how to even begin to think of such a thing, or what the effort could come close to feeling like. The scope of it is something along the lines of constructing a hollow model of the Earth out of Legos, and then making it bigger. The Earth is 8,000 miles wide—if we made a sphere of Legos two orders of magnitude larger, we’d be making the Sun, which is about 800,000 miles wide. To make the Star Trek Dyson sphere out of Legos we’d need to make the thing 7 billion miles wide, which means the surface area would be 8×10^20 miles. Or in terms of Legos: 16×1036. 16,000,000,000,000,000,000,000,000,000,000,000,000, which is a big number. (Caveat: this is just a guesstimate, so please Lego folks don’t take me to the mat on this.) The real question would be how many layers of Legos would be necessary to perform the function of retaining that solar energy.

    What kept nagging at me though was the depiction of the sphere in Star Trek—they give a sense of the thing’s MASSIVENESS, but it is a question of how far away the starship Enterprise was from the structure. I do not recall anyone mentioning the distance of ship-to-sphere, but given the curvature of the object in relation to the Enterprise I would say that the distance would have to be measured in terms of solar system widths. The tv show failed me at this point—they could’ve made some pretty interesting comments about their distance and the size of the great beast, which may have gone some way in making the utter enormity of such a engineering sensation more comprehensible; but still I would think that our puny vocabulary would still come up short with the necessaries to describe it properly. It would be as unutterably difficult to describe as the Grand Canyon—though in this case the canyon’s size would be extended to be Earth-sized. There’s something else unresolved that whispers to me—in another episode that I saw they missed a teaching/”wow” opportunity by not making it abundantly clear that in all of the adventures of the Star Trek clan that they never left the Milky Way under their own power. I think at some point they wind up in M31 through some other power not their own. Perhaps it is not well known though that for all of their Warp 9 travel that they are still somewhat “local”, staying in their own galaxy, one of 225 billion galaxies in the universe–this universe.

    So when the narrator begins each episode calling space “the final frontier”, it is being pretty presumptive—all things considered, space is probably their first frontier, and then some.

    Footnotes:

    1. See above.

    2. Olaf Stephen was evidently the first to describe this energy-retaining structure built around a star—pretty impressive stuff from someone who was 13 years old in 1899—in his 1937 novel The Star Maker. The vastness for such an undertaking is in place, the result of a universal/cosmic consciousness and millions of years of higher development. Dyson has always credited Stephenson with this idea and suggested that the creation be better termed a “Stephenson Sphere”.

    3. A short contemporary review: “Shells Around Suns May Have Been Built”, in Science News,  June 18, 1960, page 389.

    http://www.islandone.org/LEOBiblio/SETI1.HTM

    See also: Freeman John Dyson, “Search for Artificial Stellar Sources of Infrared Radiation” Science, Vol. 131, June 3, 1960, pp. 1667-1668. ABSTRACT: If extraterrestrial intelligent beings exist and have reached a high level of technical development, one by-product of their energy metabolism is likely to be the large-scale conversion of starlight into far-infrared radiation. It is proposed that a search for sources of infrared radiation should accompany the recently initiated search for interstellar radio communications.”

    http://www.islandone.org/LEOBiblio/SETI1.HTM

    And this from Robert Bradbury, “Dyson Shells: A Retrospective”, Aeiveos Corp, 2001:  “In June of 1960,2 Freeman Dyson, proposed that growing civilizations would eventually have to harvest all of the power produced by their star. He suggested that even at the low growth rate of 1%, civilizations would require only 3000 years for this process. This would require the dismemberment of the planets to provide sufficient material to expand the living space of their biosphere”. He argued that we could do this to Jupiter using the power available from the Sun over 800 years…” 

    And this:  C. Sagan and R. G. Walker, “The infrared detectability of Dyson civilizations,” Astrophysical Journal 144, pp. 1216{1217, 1966.

    4. Kardashev, Nikolai (1964). “Transmission of Information by Extraterrestrial Civilizations”. Soviet Astronomy, volume 8: 217

    Since the Dyson Sphere would be basically invisible on some levels, see Richard Carrigan’s paper “IRAS-Based Whole-Sky Upper Limit on Dyson Sphere”, on how to find one, in the Astrophysical Journal, 698:2075–2086, 2009 June 20

    http://iopscience.iop.org/0004-637X/698/2/2075/pdf/0004-637X_698_2_2075.pdf

    And just because you can, consider this: Nemanja Kaloper, Antonio Padilla, Norihiro Tanahashi. “Galileon hairs of Dyson spheres, Vainshtein’s coiffure and Hirsute Bubbles “ Journal of High Energy Physics, October 2011, 2011:148.

    Also:

    Adler, Charles L. Wizards, aliens, and starships : physics and math in fantasy and science fiction. 2014

  • Robots: Swivels, Speed, and Stumps (1928)

    JF Ptak Science Books  Quick Post

    Sometimes the future of the past looks a little, well, dodgy, or at least it looks a little too quickly assembled. 

    I have a few robots to add to this blog’s collection of robots–both are from the same volume of Popular Mechanics for 1928.  The first features a large manikin-like robotic cut-out, with a few swivel joints, and performs a couple of tasks. More than likely this was all that it could do.

    Robot 1928560

  • An Enormous Bookplate and Some Found Book Art (1856)

    JF Ptak Science Books   Quick Post

    I purchased this volume of House of Representatives reports from 1856 a number of years ago, mostly for the extraordinary bookplate that appears on the front cover of the double-brick-sized volume.  It is about as big a bookplate as I’ve bumped into or seen in 30+ years of bookselling (though admittedly the folks in the sciences seem overall to have less interest in bookplates for their library as non-science readers/collectors, so my viewpoint may be problematic).  Still, it is a big bookplate, about 5×7 inches, and as I said is on the outside of the volume rather than on the front inside cover.  There was no mistaking to whom the volume belonged, until now, when it belongs to the non-House-of-Representatives-me–anyway it is quite an object.

    Bokplates546

  • Measuring Things with Mountains & the German Big Gun of WWI (1918)

    JF Ptak Science Books  Quick Post

    The story of the (very) long-range bombardment of Paris from points unknown is filled with questions in this article that appeared in the Scientific American on April 6, 1918.  The writer hadn’t an idea of the type of gun being used, the weight of the shell (yet), and just about all other details.  The author did wonder about the reasons for such a gun–that the idea of a long-range indescrimient bombing from a great distance just seemed to be beyond the wanting capacity of the countries fighting Germany.  

    The big gun was The Big Gun, later identified as the Paris Gun–a mysterious entity during the war, and after the war as well.  It turns out that when the Germany army retreated beginning in August that they also destroyed the weapon and just about anything connected to it.

    The gun was extremely powerful.  At 256 tons it launched a 236-pound shell to a height never before achieved by humans launching/propelling stuff into the air–it left the barrel of the gun at about 1 mile/second, traveled 75 overland miles, reached a height of 26 miles…and then came down, exploding, killing.

    One very effective way of explaining the incredible height that the shell reached was measuring the zenith of its trajectory in terms of mountains:

    WWI--german gun569

    Which is a detail from:

    WWI--german gun568

    And to give a more local understanding of the range of the gun:

    WWI--german gun567No doubt this map gave a true flavor and sense of dread to American readers on exactly what it meant to have to deal with a cannon whose reach was 75+ miles. 

     

  • The Future of Oil in 1921

    JF Ptak Science Books   Quick Post

    Oil production

    [Image source:http://www.railsandtrails.com/AutoFacts/1921p12-100-8.jpg]

    There wasn’t that much of a comparative draw on what was supposed to be the world’s total supply of oil, assumed to fill a barrel about 3×1 miles, or 65 billion barrels.  (Also I assume that they are talking about oil oil, total oil, not some derivative of crude/natural/refined petroleum products and so on.) That was supposed to be enough for 140 years at the  level of consumption, about 65 billion barrels, which sounds like a lot when you drinking up 500 million/year. And it should be noted that this was for U.S. consumption only–I don’t know what happened to the rest of the world on this one; probably it was a failure of gathering statistics rather than a myopic America-only viewpoint.

    But that was 1921, and there is no mention of the Middle East (which wouldn’t become a player for a few decades) and other oil-rich regions, and other factors too numerous to mention in this quick post, so it was very much a prediction of the moment more so than of the future. The other very problematic issue with the graph is assuming the “current rate of consumption”, which would absolutely and totally miss the explosion of oil-consuming vehicles and the production of pretroleum-inclusive products.  The bottom line is that in 2013 the total world production of all aspects of oil was about 32 billion barrels1, or half of what was thought to be the total world reserves of oil in 1921.    

    Footnotes

    1. U.S. Energy Information Administration, http://www.eia.gov/cfapps/ipdbproject/IEDIndex3.cfm?tid=5&pid=53&aid=1

  • Some Interesting and Early Computer Ephemera

    JF Ptak Science Books  Quick Post

     I’m sharing this little stash of computer memorabilia (dated from 1949-1954) because in its age it is so, well, “fresh”and new and uncomplicated–and that’s because it was, relative to what we experience now.  In 1954 there about 10,000 people working in the field of computing; 61 years later the growth in involvement of people working in the field is perhaps three orders of magnitude–the growth in the sheer volume of printed and digitally-circulated material is probably somewhere on the order of the differences between post-Gutenberg European printing and the printing industry in the year 1990.  The changes are spectacular, and they seem to be so much more appreciable when one looks at the foundation efforts from the early years, some of which can be seen and represented in documents like those that follow.

    First up is this computer-printed list of attendees for “Dinner Honoring Seminar on Computation, IBM Homestead, December 8, 1949. It is a hand-stapled, four-page list with some big names in the history of computing including Brillouin, Eckert, Grosch, Hamming, Tukey, Yowell, and others. 

     

    Computer sci bits162

     

    The next document is the draft consideration for the Constitution of the ACM and is a 3-page cover later dated July 1953 regarding the voting on the new Constitution and also on officers of the ACM. It also details printing costs and distribution of the Proceedings, and other associated housekeeping, including a 3-page offset-printed ballot for voting on the Constitution.  

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