The Mathematics of the Astrolabe and Its History
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Enthymema XXIII 2019 the Technê of Aratus' Leptê Acrostich
Enthymema XXIII 2019 The Technê of Aratus’ Leptê Acrostich Jan Kwapisz University of Warsaw Abstract – This paper sets out to re-approach the famous leptê acrostich in Aratus’ Phaenomena (783-87) by confronting it with other early Greek acrostichs and the discourse of technê and sophia, which has been shown to play an important role in a gamut of Greek literary texts, including texts very much relevant for the study of Aratus’ acrostich. In particular, there is a tantalizing connection between the acrostich in Aratus’ poem that poeticized Eudoxus’ astronomical work and the so- called Ars Eudoxi, a (pseudo-)Eudoxian acrostich sphragis from a second-century BC papyrus. Keywords – Aratus; Eudoxus; Ars Eudoxi; Acrostichs; Hellenistic Poetry; Technê; Sophia. Kwapisz, Jan. “The Technê of Aratus’ Leptê Acrostich.” Enthymema, no. XXIII, 2019, pp. 374-89. http://dx.doi.org/10.13130/2037-2426/11934 https://riviste.unimi.it/index.php/enthymema Creative Commons Attribution 4.0 Unported License ISSN 2037-2426 The Technê of Aratus’ Leptê Acrostich* Jan Kwapisz University of Warsaw To the memory of Cristiano Castelletti (1971-2017) Λεπτὴ μὲν καθαρή τε περὶ τρίτον ἦμαρ ἐοῦσα εὔδιός κ’ εἴη, λεπτὴ δὲ καὶ εὖ μάλ’ ἐρευθὴς πνευματίη· παχίων δὲ καὶ ἀμβλείῃσι κεραίαις 785 τέτρατον ἐκ τριτάτοιο φόως ἀμενηνὸν ἔχουσα ἠὲ νότου ἀμβλύνετ’ ἢ ὕδατος ἐγγὺς ἐόντος. (Arat. 783-87) If [the Moon is] slender and clear about the third day, she will bode fair weather; if slender and very red, wind; if the crescent is thickish, with blunted horns, having a feeble fourth-day light after the third day, either it is blurred by a southerly or because rain is in the offing. -
CURRICULUM VITA of ROBERT HAHN January 2015
CURRICULUM VITA OF ROBERT HAHN January 2015 I. PERSONAL A. Present University Department: Philosophy. II. EDUCATION Ph.D., Philosophy, Yale University, May 1976. M. Phil., Philosophy, Yale University, May 1976. M.A., Philosophy, Yale University, December 1975. B.A., Philosophy, Union College, Summa cum laude, June 1973. Summer Intensive Workshop in Ancient Greek, The University of California at Berkeley, 1973. Summer Intensive Workshop in Sanskrit, The University of Chicago, 1972. III. PROFESSIONAL EXPERIENCE 2002-present Professor of Philosophy, Southern Illinois University at Carbondale 1988-2001 Associate Professor of Philosophy, Southern Illinois University at Carbondale. 1982-1987 Assistant Professor of Philosophy, Southern Illinois University at Carbondale. 1981-1982 Assistant Professor of Philosophy, Denison University. 1978-1981 Assistant Professor of Philosophy and the History of Ideas, Brandeis University. 1979-1981 Assistant Professor, Harvard University, Extension. 1980 (Spring) Visiting Professor, The American College of Greece (Deree College), Athens, Greece. 1980 (Summer) Visiting Professor, The University of Maryland: European Division, Athens, Greece (The United States Air Force #7206 Air Base Group). 1977-1978 Assistant Professor of Philosophy, The University of Texas, Arlington. 1977 (Spring) Lecturer in Philosophy, Yale University. 1976 (Fall) Postdoctoral Research Fellow in Philosophy, The University of California at Berkeley. IV. TEACHING EXPERIENCE A. Teaching Interests and Specialties: History of Philosophy, History/Philosophy -
What Did Shakespeare Know About Copernicanism?
DOI: 10.2478/v10319-012-0031-x WHAT DID SHAKESPEARE KNOW ABOUT COPERNICANISM? ALAN S. WEBER Weill Cornell Medical College–Qatar Abstract: This contribution examines Shakespeare’s knowledge of the cosmological theories of Nicolaus Copernicus (1473-1543) as well as recent claims that Shakespeare possessed specialized knowledge of technical astronomy. Keywords: Shakespeare, William; Copernicus, Nicolaus; renaissance astronomy 1. Introduction Although some of his near contemporaries lamented the coming of “The New Philosophy,” Shakespeare never made unambiguous or direct reference to the heliocentric theories of Nicolaus Copernicus (1473-1543) in his drama or poetry. Peter Usher, however, has recently argued in two books Hamlet’s Universe (2006) and Shakespeare and the Dawn of Modern Science (2010) that Hamlet is an elaborate allegory of Copernicanism, which in addition heralds pre-Galilean telescopic observations carried out by Thomas Digges. Although many of Usher’s arguments are excessively elaborate and speculative, he raises several interesting questions. Just why did Shakespeare, for example, choose the names of Rosenskrantz and Guildenstern for Hamlet’s petard-hoisted companions, two historical relatives of Tycho Brahe (the foremost astronomer during Shakespeare’s floruit)? What was Shakespeare’s relationship to the spread of Copernican cosmology in late Elizabethan England? Was he impacted by such Copernican-related currents of cosmological thought as the atomism of Thomas Harriot and Nicholas Hill, the Neoplatonism of Kepler, and -
Earth-Centred Universe
Earth-centred Universe The fixed stars appear on the celestial sphere Earth rotates in one sidereal day The solar day is longer by about 4 minutes → scattered sunlight obscures the stars by day The constellations are historical → learn to recognise: Ursa Major, Ursa Minor, Cassiopeia, Pegasus, Auriga, Gemini, Orion, Taurus Sun’s Motion in the Sky The Sun moves West to East against the background of Stars Stars Stars stars Us Us Us Sun Sun Sun z z z Start 1 sidereal day later 1 solar day later Compared to the stars, the Sun takes on average 3 min 56.5 sec extra to go round once The Sun does not travel quite at a constant speed, making the actual length of a solar day vary throughout the year Pleiades Stars near the Sun Sun Above the atmosphere: stars seen near the Sun by the SOHO probe Shield Sun in Taurus Image: Hyades http://sohowww.nascom.nasa.g ov//data/realtime/javagif/gifs/20 070525_0042_c3.gif Constellations Figures courtesy: K & K From The Beauty of the Heavens by C. F. Blunt (1842) The Celestial Sphere The celestial sphere rotates anti-clockwise looking north → Its fixed points are the north celestial pole and the south celestial pole All the stars on the celestial equator are above the Earth’s equator How high in the sky is the pole star? It is as high as your latitude on the Earth Motion of the Sky (animated ) Courtesy: K & K Pole Star above the Horizon To north celestial pole Zenith The latitude of Northern horizon Aberdeen is the angle at 57º the centre of the Earth A Earth shown in the diagram as 57° 57º Equator Centre The pole star is the same angle above the northern horizon as your latitude. -
Configurations on Centers of Bankoff Circles 11
CONFIGURATIONS ON CENTERS OF BANKOFF CIRCLES ZVONKO CERINˇ Abstract. We study configurations built from centers of Bankoff circles of arbelos erected on sides of a given triangle or on sides of various related triangles. 1. Introduction For points X and Y in the plane and a positive real number λ, let Z be the point on the segment XY such that XZ : ZY = λ and let ζ = ζ(X; Y; λ) be the figure formed by three mj utuallyj j tangenj t semicircles σ, σ1, and σ2 on the same side of segments XY , XZ, and ZY respectively. Let S, S1, S2 be centers of σ, σ1, σ2. Let W denote the intersection of σ with the perpendicular to XY at the point Z. The figure ζ is called the arbelos or the shoemaker's knife (see Fig. 1). σ σ1 σ2 PSfrag replacements X S1 S Z S2 Y XZ Figure 1. The arbelos ζ = ζ(X; Y; λ), where λ = jZY j . j j It has been the subject of studies since Greek times when Archimedes proved the existence of the circles !1 = !1(ζ) and !2 = !2(ζ) of equal radius such that !1 touches σ, σ1, and ZW while !2 touches σ, σ2, and ZW (see Fig. 2). 1991 Mathematics Subject Classification. Primary 51N20, 51M04, Secondary 14A25, 14Q05. Key words and phrases. arbelos, Bankoff circle, triangle, central point, Brocard triangle, homologic. 1 2 ZVONKO CERINˇ σ W !1 σ1 !2 W1 PSfrag replacements W2 σ2 X S1 S Z S2 Y Figure 2. The Archimedean circles !1 and !2 together. -
1 Science LR 2711
A Scientific Response to the Chester Beatty Library Collection Contents The Roots Of Modern Science A Scientific Response To The Chester Beatty Library Collection 1 Science And Technology 2 1 China 3 Science In Antiquity 4 Golden Age Of Islamic Science 5 Transmission Of Knowledge To Europe 6 A Scientific Response To The Chester Beatty Library Collections For Dublin City Of Science 2012 7 East Asian Collections The Great Encyclopaedia of the Yongle Reign (Yongle Dadian) 8 2 Phenomena of the Sky (Tianyuan yuli xiangyi tushuo) 9 Treatise on Astronomy and Chronology (Tianyuan lili daquan) 10 Illustrated Scrolls of Gold Mining on Sado Island (Sado kinzan zukan) 11 Islamic Collections Islamic Medicine 12 3 Medical Compendium, by al-Razi (Al-tibb al-mansuri) 13 Encyclopaedia of Medicine, by Ibn Sina (Al-qanun fi’l-tibb) 14 Treatise on Surgery, by al-Zahrawi (Al-tasrif li-man ‘ajiza ‘an al-ta’lif) 15 Treatise on Human Anatomy, by Mansur ibn Ilyas (Tashrih al-badan) 16 Barber –Surgeon toolkit from 1860 17 Islamic Astronomy and Mathematics 18 The Everlasting Cycles of Lights, by Muhyi al-Din al-Maghribi (Adwar al-anwar mada al-duhur wa-l-akwar) 19 Commentary on the Tadhkira of Nasir al-Din al-Tusi 20 Astrolabes 21 Islamic Technology 22 Abbasid Caliph, Ma’mum at the Hammam 23 European Collections European Science of the Middle Ages 24 4 European Technology: On Military Matters (De Re Militari) 25 European Technology: Concerning Military Matters (De Re Militari) 26 Mining Technology: On the Nature of Metals (De Re Metallica) 27 Fireworks: The triumphal -
The Geography of Ptolemy Elucidated
The Grography of Ptolemy The geography of Ptolemy elucidated Thomas Glazebrook Rylands 1893 • A brief outline of the rise and progress of geographical inquiry prior to the time of Ptolemy. §1.—Introductory. IN tracing the early progress of Geography it is necessary to remember that, like all other sciences, it arose from “ small beginnings.” When men began to move from place to place they naturally desired to tell the tale of their wanderings, both for their own satisfaction and for the information of others. Such accounts have now perished, but their results remain in the earliest records extant ; hence, it is impossible to begin an investigation into the history of Geography at the true fountain-head, though it is in some instances possible to guess the nature of the source from the character of the resultant stream. A further difficulty lies in the question as to where the science of Geography begins. A Greek would probably have answered when some discoverer first invented a method for map- ping out the distance between certain places, which distance conversely could be ascertained directly from the map. In accordance with modern method, the science of Geography might be said to begin when the subject ceased to be dealt with mythically or dogmatically ; when facts were collected and reduced to laws, while these laws again, or their prior facts, were connected with other laws—in the case of Geography with those of Mathematics and Astro- nomy. Perhaps it would be better to follow the latter principle of division, and consequently the history of Geography may be divided into two main stages—“ Pre-Scientific” and Scientific Geography—though strictly speaking, the name of Geography should be applied to the latter alone. -
The Magic of the Atwood Sphere
The magic of the Atwood Sphere Exactly a century ago, on June Dr. Jean-Michel Faidit 5, 1913, a “celestial sphere demon- Astronomical Society of France stration” by Professor Wallace W. Montpellier, France Atwood thrilled the populace of [email protected] Chicago. This machine, built to ac- commodate a dozen spectators, took up a concept popular in the eigh- teenth century: that of turning stel- lariums. The impact was consider- able. It sparked the genesis of modern planetariums, leading 10 years lat- er to an invention by Bauersfeld, engineer of the Zeiss Company, the Deutsche Museum in Munich. Since ancient times, mankind has sought to represent the sky and the stars. Two trends emerged. First, stars and constellations were easy, especially drawn on maps or globes. This was the case, for example, in Egypt with the Zodiac of Dendera or in the Greco-Ro- man world with the statue of Atlas support- ing the sky, like that of the Farnese Atlas at the National Archaeological Museum of Na- ples. But things were more complicated when it came to include the sun, moon, planets, and their apparent motions. Ingenious mecha- nisms were developed early as the Antiky- thera mechanism, found at the bottom of the Aegean Sea in 1900 and currently an exhibi- tion until July at the Conservatoire National des Arts et Métiers in Paris. During two millennia, the human mind and ingenuity worked constantly develop- ing and combining these two approaches us- ing a variety of media: astrolabes, quadrants, armillary spheres, astronomical clocks, co- pernican orreries and celestial globes, cul- minating with the famous Coronelli globes offered to Louis XIV. -
Thinking Outside the Sphere Views of the Stars from Aristotle to Herschel Thinking Outside the Sphere
Thinking Outside the Sphere Views of the Stars from Aristotle to Herschel Thinking Outside the Sphere A Constellation of Rare Books from the History of Science Collection The exhibition was made possible by generous support from Mr. & Mrs. James B. Hebenstreit and Mrs. Lathrop M. Gates. CATALOG OF THE EXHIBITION Linda Hall Library Linda Hall Library of Science, Engineering and Technology Cynthia J. Rogers, Curator 5109 Cherry Street Kansas City MO 64110 1 Thinking Outside the Sphere is held in copyright by the Linda Hall Library, 2010, and any reproduction of text or images requires permission. The Linda Hall Library is an independently funded library devoted to science, engineering and technology which is used extensively by The exhibition opened at the Linda Hall Library April 22 and closed companies, academic institutions and individuals throughout the world. September 18, 2010. The Library was established by the wills of Herbert and Linda Hall and opened in 1946. It is located on a 14 acre arboretum in Kansas City, Missouri, the site of the former home of Herbert and Linda Hall. Sources of images on preliminary pages: Page 1, cover left: Peter Apian. Cosmographia, 1550. We invite you to visit the Library or our website at www.lindahlll.org. Page 1, right: Camille Flammarion. L'atmosphère météorologie populaire, 1888. Page 3, Table of contents: Leonhard Euler. Theoria motuum planetarum et cometarum, 1744. 2 Table of Contents Introduction Section1 The Ancient Universe Section2 The Enduring Earth-Centered System Section3 The Sun Takes -
Kaleidoscopic Symmetries and Self-Similarity of Integral Apollonian Gaskets
Kaleidoscopic Symmetries and Self-Similarity of Integral Apollonian Gaskets Indubala I Satija Department of Physics, George Mason University , Fairfax, VA 22030, USA (Dated: April 28, 2021) Abstract We describe various kaleidoscopic and self-similar aspects of the integral Apollonian gaskets - fractals consisting of close packing of circles with integer curvatures. Self-similar recursive structure of the whole gasket is shown to be encoded in transformations that forms the modular group SL(2;Z). The asymptotic scalings of curvatures of the circles are given by a special set of quadratic irrationals with continued fraction [n + 1 : 1; n] - that is a set of irrationals with period-2 continued fraction consisting of 1 and another integer n. Belonging to the class n = 2, there exists a nested set of self-similar kaleidoscopic patterns that exhibit three-fold symmetry. Furthermore, the even n hierarchy is found to mimic the recursive structure of the tree that generates all Pythagorean triplets arXiv:2104.13198v1 [math.GM] 21 Apr 2021 1 Integral Apollonian gaskets(IAG)[1] such as those shown in figure (1) consist of close packing of circles of integer curvatures (reciprocal of the radii), where every circle is tangent to three others. These are fractals where the whole gasket is like a kaleidoscope reflected again and again through an infinite collection of curved mirrors that encodes fascinating geometrical and number theoretical concepts[2]. The central themes of this paper are the kaleidoscopic and self-similar recursive properties described within the framework of Mobius¨ transformations that maps circles to circles[3]. FIG. 1: Integral Apollonian gaskets. -
Ibrāhīm Ibn Sinān Ibn Thābit Ibn Qurra
From: Thomas Hockey et al. (eds.). The Biographical Encyclopedia of Astronomers, Springer Reference. New York: Springer, 2007, p. 574 Courtesy of http://dx.doi.org/10.1007/978-0-387-30400-7_697 Ibrāhīm ibn Sinān ibn Thābit ibn Qurra Glen Van Brummelen Born Baghdad, (Iraq), 908/909 Died Baghdad, (Iraq), 946 Ibrāhīm ibn Sinān was a creative scientist who, despite his short life, made numerous important contributions to both mathematics and astronomy. He was born to an illustrious scientific family. As his name suggests his grandfather was the renowned Thābit ibn Qurra; his father Sinān ibn Thābit was also an important mathematician and physician. Ibn Sinān was productive from an early age; according to his autobiography, he began his research at 15 and had written his first work (on shadow instruments) by 16 or 17. We have his own word that he intended to return to Baghdad to make observations to test his astronomical theories. He did return, but it is unknown whether he made his observations. Ibn Sinān died suffering from a swollen liver. Ibn Sinān's mathematical works contain a number of powerful and novel investigations. These include a treatise on how to draw conic sections, useful for the construction of sundials; an elegant and original proof of the theorem that the area of a parabolic segment is 4/3 the inscribed triangle (Archimedes' work on the parabola was not available to the Arabs); a work on tangent circles; and one of the most important Islamic studies on the meaning and use of the ancient Greek technique of analysis and synthesis. -
Class 1: Overview of the Course; Ptolemaic Astronomy
a. But marked variations within this pattern, and hence different loops from one occasion to another: e.g. 760 days one time, 775 another, etc. b. Planetary speeds vary too: e.g. roughly 40 percent variation in apparent longitudinal motion per day of Mars from one extreme to another while away from retrograde 4. Each of the five planets has its own distinct basic pattern of periods of retrograde motion, and its own distinct pattern of variations on this basic pattern a. Can be seen in examples of Mars and Jupiter, where loops vary b. An anomaly on top of the anomaly of retrograde motion c. Well before 300 B.C. the Babylonians had discovered “great cycles” in which the patterns of retrograde loops and timings of stationary points repeat: e.g. 71 years for Jupiter (see Appendix for others) 5. The problem of the planets: give an account ('logos') of retrograde motion, including basic pattern, size of loops, and variations for each of the five planets a. Not to predict longitude and latitude every day b. Focus instead on salient events – i.e. phenomena: conjunctions, oppositions, stationary points, longitudinal distance between them c. For the Babylonians, just predict; for the Greeks, to give a geometric representation of the constituent motions giving rise to the patterns 6. Classical designations: "the first inequality": variation in mean daily angular speed, as in 40 percent variation for Mars and smaller variation for Sun; "the second inequality": retrograde motion, as exhibited by the planets, but not the sun and moon D. Classical Greek Solutions 1.