The Antikythera Mechanism Evidence of a Lunar Calendar Parts 1&2
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Kythera Summer Edition 2018
KYTHERA Summer Edition 2018 FOUNDERρΙΔΡΥΤΗΣό ©METAXIA POULOS • PUBLISHERό DIMITRIS KYRIAKOPOULOS • EDITORό DEBORAH PARSONS • WRITERSό ELIAS ANAGNOSTOU, ANNA COMINOS, SALLY COMINOS-DAKIN, FIONA CUNNINGHAM, EVGENIA GIANNINI, DOMNA KONTARATOU, MARIA KOUKOULI, THEODOROS KOUKOULIS, DIMITRIS KOUTRAFOURIS, ALEXIA NIKIFORAKI, PIA PANARETOS, AGLAIA PAPAOICONOMOU, ASPASIA PATTY, DAPHNE PETROCHILOS, IPPOLYTOS PREKAS, YIANNIS PROTOPSALTIS, JOY TATARAKI, ELIAS TZIRITIS, NIKOS TSIOPE- LAS • ARTWORKό DAPHNE PETROHILOS• PHOTOGRAPHYό DIMITRIS BALTZIS, CHRISSA FATSEAS, VENIA KAROLIDOU, STEPHEN TRIFYLLIS, EVANGELOS TSIGARIDAS • PROOF READINGό PAULA CASSIMATIS, JOY TATARAKI • LAYOUT ζ DESIGNό MYRTO BOLOTA • EDITORIALρADVERTISINGξΣΥΝΤΑΞΗρΔΙΑΦΗΜΙΣΕΙΣό 69φφ-55σ7τς, e-mailό kse.σ99υ@yahoo.gr FREE COMMUNITY PAPER • ΕΛΛΗΝΟξΑΓΓΛΙΚΗ ΕΚΔΟΣΗ • ΑΝΕΞ ΑΡΤΗΤΗ ΠΟΛΙΤΙΣΤΙΚΗ ΕΦΗΜΕΡΙΔΑ • ΔΙΑΝΕΜΕΤΑΙ ΔΩΡΕΑΝ George & Viola Haros and family wish everyone a Happy Summer in Kythera Distributing quality food, beverage, cleaning and packaging products to the Foodservice Industry wwwοstgeorgefoodserviceοcomοau All the right ingredients Ανοιχτά από τις 9.00 π.μ. έως αργά το βράδυ για καφέ, μεζέ και φαγητό MYLOPOTAMOS Καλλιόπη Καρύδη τηλ.: 27360-33397 και όλα μέλι-γάλα pure Kytherian thyme honey τχςξγοατία ςξσ ΙΠΠΟΛΥΤΟΥ ΠΡΕΚΑ θυμαρίσιο μέλι αωορίαε! welcome! Κυθήρων Έλίπλίίωί“”ίμί’ίίίμίίΚξ ΜΗΤΑΤΑ Κύθηρα Ρίίίμίμωίμπωξ τηλ.: 27360-33010, 6978-350952, 6977-692745 Ωί:ίίΑίίΑμ ΤαίίJeanνAntoineίWatteauίίίΑπξ Έίίίπλίίίίίξ Σίίμίίίίίξί ηΗΛξΑΝξίσρς8θ What is it that has brought you to Aphrodite’s -
Society News Science News the Antikythera Mechanism Skinakas Observatory Spectroscopic Diagnostics of Galactic Nuclei Eclipsing Binaries
HIPPARCHOSHIPPARCHOS The Hellenic Astronomical Society Newsletter Volume 2, Issue 2 Society News Science News The Antikythera Mechanism Skinakas observatory Spectroscopic Diagnostics of Galactic Nuclei Eclipsing Binaries ISSN: 1790-9252 ʸ˱ˤ˳˶˱˹˯˩˭ˮˬ˰˱˙ ƋƜƠƦƓ6SHFLDO(GLWLRQ °ĆāąĆąõýĉýĊýĈØĉĊćąăąĂõ÷Ĉ çąÿąĈāóûÿĒĊÿý÷ĉĊćąăąĂõ÷ĆćóĆûÿă÷ûõă÷ÿĆûćõĆāąĀýØČôĉĊû Ċą 1H[6WDU 6( ă÷ ĉ÷Ĉ øąýþôĉûÿ ă÷ øćûõĊû čÿāÿòúûĈ ÷ĉĊóćûĈ Ćā÷ăôĊûĈù÷ā÷ĄõûĈĀ÷ÿòāā÷ĂûĊąĆòĊýĂ÷ûăĒĈĀąċĂĆÿąēÞ ăó÷ ąÿĀąùóăûÿ÷ 1H[6WDU 6( ĉċăúċòüûÿ ĆćďĊąČ÷ăô ûċčćýĉĊõ÷ Ăû ûĄûāÿùĂóăûĈ āûÿĊąċćùõûĈ Ā÷ÿ ÷ĆõĉĊûċĊą āĒùą ÷Ąõ÷Ĉ ĆćąĈ ĊÿĂô Ûûă Ćûćÿā÷ĂøòăûĊ÷ÿ ý Ćÿþ÷ăĒĊýĊ÷ ă÷ Ċą ĂûĊ÷ăÿĔĉûÿ ą ÷ùąć÷ĉĊôĈ ƌƞƢƜƨơƱƠƥ ăó÷ ąÿĀąùóăûÿ÷ 1H[6WDU 6( öÁ &HOHVWURQ ´¹ÅÀ«µ´¸ 1H[6WDU6( ĊýăĊûāûċĊ÷õ÷āóĄýĊýĈĊûčăąāąùõ÷ĈĒĆďĈĆāôćďĈ ÷ċĊąĂ÷ĊąĆąÿýĂóăą āûÿĊąċćùÿĀĒ ĉēĉĊýĂ÷ úċă÷ĊĒĊýĊ÷ ÷ă÷øòþĂÿĉýĈ Ăóĉď IODVK Ċąċ čûÿćÿĉĊýćõąċ ĊÿĈ ĀąćċČ÷õûĈ ãæäêÜâæ 1H[6WDU6( êëçæé 0DNVXWRY&DVVHJUDLQ¡¾»¿¾Ã¸¹Ë*R7R ûĆÿĉĊćĔĉûÿĈ 6WDU%ULJKW ;/7 Ċą ûĆ÷ă÷ĉĊ÷ĊÿĀĒ āąùÿĉĂÿĀĒ ÛàØãÜêèæéáØêæçêèæë PP l ûċþċùćòĂĂÿĉýĈĊąċĊýāûĉĀąĆõąċ6N\$OLJQpĀ÷ÿĆąāāòòāā÷ ÜéêØçæéêØéÞ PP ÜéêâæÚæé I £¢ ¢£¡¨¢¢ 6WDU%ULJKW;/7 ãûĊą1H[6WDU6(ûõĉĊûĉĊýþóĉýĊąċąúýùąēØĆāòûĆÿāóĄĊû ãÜÚïìÜâãÜÚÜßëäéÞ [ óă÷÷ăĊÿĀûõĂûăą÷ĆĒĊąĂûăąēĀ÷ÿĊąĊýāûĉĀĒĆÿąþ÷Ċąøćûÿùÿ÷ æèàØáæìØàäãÜÚÜßæé éêÞèàåÞ ØāĊ÷üÿĂąċþÿ÷Āô»´»¾Ã¬À ĉ÷ĈíćýĉÿùƹÿĔăĊ÷ĈĊýăĊûčăąāąùõ÷1H[6WDUĊ÷ĊýāûĉĀĒĆÿ÷ ¡¢¥ PP PP(/X[ 6( óčąċă Ċýă ÿĀ÷ăĒĊýĊ÷ ă÷ ûăĊąĆõĉąċă ĆûćõĆąċ ¡¤£¢ 6WDU3RLQWHU ÷ăĊÿĀûõĂûă÷ êą ĂĒăą Ćąċ óčûĊû ă÷ ĀòăûĊû ûõă÷ÿ ă÷ ĀąÿĊòĄûĊû £¡ ¢ 뺸¼¾Á ¨ PP »´kIOLSPLUURUl Ăóĉ÷÷ĆĒĊąĆćąĉąČþòāĂÿąĀ÷ÿă÷÷Ćąā÷ēĉûĊûĊąþó÷Ă÷ ÙØèæé NJ Ûûă ĄóćûĊû Ćąÿą ÷ăĊÿĀûõĂûăą ă÷ ûĆÿāóĄûĊû -
The Mathematics of the Chinese, Indian, Islamic and Gregorian Calendars
Heavenly Mathematics: The Mathematics of the Chinese, Indian, Islamic and Gregorian Calendars Helmer Aslaksen Department of Mathematics National University of Singapore [email protected] www.math.nus.edu.sg/aslaksen/ www.chinesecalendar.net 1 Public Holidays There are 11 public holidays in Singapore. Three of them are secular. 1. New Year’s Day 2. Labour Day 3. National Day The remaining eight cultural, racial or reli- gious holidays consist of two Chinese, two Muslim, two Indian and two Christian. 2 Cultural, Racial or Religious Holidays 1. Chinese New Year and day after 2. Good Friday 3. Vesak Day 4. Deepavali 5. Christmas Day 6. Hari Raya Puasa 7. Hari Raya Haji Listed in order, except for the Muslim hol- idays, which can occur anytime during the year. Christmas Day falls on a fixed date, but all the others move. 3 A Quick Course in Astronomy The Earth revolves counterclockwise around the Sun in an elliptical orbit. The Earth ro- tates counterclockwise around an axis that is tilted 23.5 degrees. March equinox June December solstice solstice September equinox E E N S N S W W June equi Dec June equi Dec sol sol sol sol Beijing Singapore In the northern hemisphere, the day will be longest at the June solstice and shortest at the December solstice. At the two equinoxes day and night will be equally long. The equi- noxes and solstices are called the seasonal markers. 4 The Year The tropical year (or solar year) is the time from one March equinox to the next. The mean value is 365.2422 days. -
Alexander Jones Calendrica I: New Callippic Dates
ALEXANDER JONES CALENDRICA I: NEW CALLIPPIC DATES aus: Zeitschrift für Papyrologie und Epigraphik 129 (2000) 141–158 © Dr. Rudolf Habelt GmbH, Bonn 141 CALENDRICA I: NEW CALLIPPIC DATES 1. Introduction. Callippic dates are familiar to students of Greek chronology, even though up to the present they have been known to occur only in a single source, Ptolemy’s Almagest (c. A.D. 150).1 Ptolemy’s Callippic dates appear in the context of discussions of astronomical observations ranging from the early third century B.C. to the third quarter of the second century B.C. In the present article I will present new attestations of Callippic dates which extend the period of the known use of this system by almost two centuries, into the middle of the first century A.D. I also take the opportunity to attempt a fresh examination of what we can deduce about the Callippic calendar and its history, a topic that has lately been the subject of quite divergent treatments. The distinguishing mark of a Callippic date is the specification of the year by a numbered “period according to Callippus” and a year number within that period. Each Callippic period comprised 76 years, and year 1 of Callippic Period 1 began about midsummer of 330 B.C. It is an obvious, and very reasonable, supposition that this convention for counting years was instituted by Callippus, the fourth- century astronomer whose revisions of Eudoxus’ planetary theory are mentioned by Aristotle in Metaphysics Λ 1073b32–38, and who also is prominent among the authorities cited in astronomical weather calendars (parapegmata).2 The point of the cycles is that 76 years contain exactly four so-called Metonic cycles of 19 years. -
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. -
The Dark Shades of the Antikythera Mechanism
Journal of Radioanalytical and Nuclear Chemistry https://doi.org/10.1007/s10967-018-6255-9 (0123456789().,-volV)(0123456789().,-volV) The dark shades of the Antikythera Mechanism 1 2 3 Aristeidis Voulgaris • Christophoros Mouratidis • Andreas Vossinakis Received: 19 June 2018 Ó Akade´miai Kiado´, Budapest, Hungary 2018 Abstract In this work we analyze the dark shades which are evident on the AMRP X-ray positive Computed Tomographies and Radiographies of the Antikythera Mechanism ancient prototype. During 2000 years under the sea, the Mechanism bronze parts were totally corroded. The decreased X-ray absorption of the corroded bronze, allowed the CTs capture even in the thick large side of Fragment A. During the photometric analysis of the CTs, apart from corroded bronze, at least two other different (corroded) metal materials were detected, which were used by the ancient manufacturer during the construction of the Antikythera Mechanism. From our analysis and correlating with the mechanical evidence resulting by the use of our functional reconstruction models of the Antikythera Mechanism, we conclude that the existing design of the Antikythera Mechanism is probably the first of such a sophisticated design of the ancient manufacturer. Keywords Metals of Antikythera Mechanism Á Bronze corrosion Á Atacamite X-ray absorption Introduction Mechanism via the 2D X-ray and Thulium 170 radiation began by C. Karakalos of National Centre of Scientific The Antikythera Mechanism was found in 1901, in a Research ‘‘Demokritos’’ (Greece), in the 1970s. Karakalos shipwreck at 50 m depth, on a gulf of Antikythera island, took several film radiographies @160 keV [3]. The first Greece, by Symian sponge divers. -
How Long Is a Year.Pdf
How Long Is A Year? Dr. Bryan Mendez Space Sciences Laboratory UC Berkeley Keeping Time The basic unit of time is a Day. Different starting points: • Sunrise, • Noon, • Sunset, • Midnight tied to the Sun’s motion. Universal Time uses midnight as the starting point of a day. Length: sunrise to sunrise, sunset to sunset? Day Noon to noon – The seasonal motion of the Sun changes its rise and set times, so sunrise to sunrise would be a variable measure. Noon to noon is far more constant. Noon: time of the Sun’s transit of the meridian Stellarium View and measure a day Day Aday is caused by Earth’s motion: spinning on an axis and orbiting around the Sun. Earth’s spin is very regular (daily variations on the order of a few milliseconds, due to internal rearrangement of Earth’s mass and external gravitational forces primarily from the Moon and Sun). Synodic Day Noon to noon = synodic or solar day (point 1 to 3). This is not the time for one complete spin of Earth (1 to 2). Because Earth also orbits at the same time as it is spinning, it takes a little extra time for the Sun to come back to noon after one complete spin. Because the orbit is elliptical, when Earth is closest to the Sun it is moving faster, and it takes longer to bring the Sun back around to noon. When Earth is farther it moves slower and it takes less time to rotate the Sun back to noon. Mean Solar Day is an average of the amount time it takes to go from noon to noon throughout an orbit = 24 Hours Real solar day varies by up to 30 seconds depending on the time of year. -
94 Erkka Maula
ORGANON 15 PROBLÊMES GENERAUX Erkka Maula (Finland) FROM TIME TO PLACE: THE PARADIGM CASE The world-order in philosophical cosmology can be founded upon time as well as .space. Perhaps the most fundamental question pertaining to any articulated world- view concerns, accordingly, their ontological and epistemological priority. Is the basic layer of notions characterized by temporal or by spatial concepts? Does a world-view in its development show tendencies toward the predominance of one set of concepts rather than the other? At the stage of its relative maturity, when the qualitative and comparative phases have paved the way for the formation of quantitative concepts: Which are considered more fundamental, measurements of time or measurements of space? In the comparative phase: Is the geometry of the world a geometry of motion or a geometry of timeless order? In the history of our own scientific world-view, there seems to be discernible an oscillation between time-oriented and space-oriented concept formation.1 In the dawn, when the first mathematical systems of astronomy and geography appear, shortly before Euclid's synthesis of the axiomatic thought, there were attempts at a geometry of motion. They are due to Archytas of Tarentum and Eudoxus of Cnidus, foreshadowed by Hippias of Elis and the Pythagoreans, who tend to intro- duce temporal concepts into geometry. Their most eloquent adversary is Plato, and after him the two alternative streams are often called the Heraclitean and the Parmenidean world-views. But also such later and far more articulated distinctions as those between the statical and dynamic cosmologies, or between the formalist and intuitionist philosophies of mathematics, can be traced down to the original Greek dichotomy, although additional concepts entangle the picture. -
Metonic Intercalations in Athens
METONIC INTERCALATIONSIN ATHENS ~W~7~JHENI published in 1940 the only knownAttic decreenaming in its preamble v v at least part of the name and demotic of the secretary of 298/7 I suggested that the calendar equation indicated an ordinary year of twelve months.' This deter- mination was taken over by Pritchett and Meritt in Chronology of Hellenistic Athens (p. xvi), by Pritchett and Neugebauer in Calendars of Athens (p. 80), and by Meritt in The Athenian Year (p. 232). There is one consideration which at the time did not seem so important as it does now and which I wish to discuss here. The incentive to a reconsideration has been the observation that the sequence of ordinary and intercalary years which called for OOIOI in 299/8-295/4 rather than OIOOI at the beginning of the 8th Metonic cycle was the first apparent deviation from Meton's norm for possibly a hundred years, except for the anomaly in 307/6 which had valid and obvious historical reasons and which could be amply explained.2 I noted, as a comment on the cycles, that " the eighth cycle has only the transposition of IO to OI in the years 298/7 and 297/6." 8 Otherwise the cycle in the festival calendar of Athens followed faithfully the normal Metonic cycle of intercalation. In the text of Hesperia, IX, 1940, pp. 80-83 (13), as now restored with a stoichedon line of 29 letters, the equation reads: [. 'EA..Xa0b],8oXt'v[o] sv6 [TE&per'] [ElKa6a& Tptp&et] Ka' eiKoo-xrre[&T2q irp] [VTlavea- -] - KTX. -
The Calendars of India
The Calendars of India By Vinod K. Mishra, Ph.D. 1 Preface. 4 1. Introduction 5 2. Basic Astronomy behind the Calendars 8 2.1 Different Kinds of Days 8 2.2 Different Kinds of Months 9 2.2.1 Synodic Month 9 2.2.2 Sidereal Month 11 2.2.3 Anomalistic Month 12 2.2.4 Draconic Month 13 2.2.5 Tropical Month 15 2.2.6 Other Lunar Periodicities 15 2.3 Different Kinds of Years 16 2.3.1 Lunar Year 17 2.3.2 Tropical Year 18 2.3.3 Siderial Year 19 2.3.4 Anomalistic Year 19 2.4 Precession of Equinoxes 19 2.5 Nutation 21 2.6 Planetary Motions 22 3. Types of Calendars 22 3.1 Lunar Calendar: Structure 23 3.2 Lunar Calendar: Example 24 3.3 Solar Calendar: Structure 26 3.4 Solar Calendar: Examples 27 3.4.1 Julian Calendar 27 3.4.2 Gregorian Calendar 28 3.4.3 Pre-Islamic Egyptian Calendar 30 3.4.4 Iranian Calendar 31 3.5 Lunisolar calendars: Structure 32 3.5.1 Method of Cycles 32 3.5.2 Improvements over Metonic Cycle 34 3.5.3 A Mathematical Model for Intercalation 34 3.5.3 Intercalation in India 35 3.6 Lunisolar Calendars: Examples 36 3.6.1 Chinese Lunisolar Year 36 3.6.2 Pre-Christian Greek Lunisolar Year 37 3.6.3 Jewish Lunisolar Year 38 3.7 Non-Astronomical Calendars 38 4. Indian Calendars 42 4.1 Traditional (Siderial Solar) 42 4.2 National Reformed (Tropical Solar) 49 4.3 The Nānakshāhī Calendar (Tropical Solar) 51 4.5 Traditional Lunisolar Year 52 4.5 Traditional Lunisolar Year (vaisnava) 58 5. -
Presentation a Representation B FRONT DIALS
AGAMEMNON TSELIKAS The Anticythera Mechanism. Research Facilities and Heritage Dynamics between Humanities and Technologies NANYANG TECHNOLOGICAL UNIVERSITY EXPLORING MARITIME HERITAGE DYNAMICS 18 – 20 November 2015 Greece, Southern Aegean Sea HISTORICAL DATA * Probably was constructed in Rhodes island in the astronomical school of Poseidonius mid-2nd BC century. * It was one item of a cargo of many valuable artistic objects (bronze and marble statues) on a ship which probably departed from Rhodes in direction to Italy between the years 80 and 60 BC and wrecked south of Antikythera island. The route of the ancient ship from Rhodes to Italy. HISTORICAL DATA * It was found in 1900 a few days before Easter, by sponge divers originated from the greek island Symi in Dodekanessos near Rhodes island. The route of the sponge ship from Symi island in direction probably to Lybia. Sponge divers in their island Symi. The island of Antikythera The islands of Rhodes and Symi Sponge divers, officials, and crew of the war ship "Mykali" during the hauling of antiquities from the wreck in Antikythera. Winter 1900-1901. It consists of 82 fragments. HISTORICAL DATA * Scientists who studied the the unknown object: 1902-1910 Staes, Svoronos, Rados, Albert Rem. 1930-1940 Admiral John Theofanides, Tsiner, Gynder, Chartner. 1950-1970 Derek de Solla Price (1922-1983, “Gears from the Greeks”) and Karakalos 1980-1990 Bromley and Michael Wright 1990 - Today Michael Wright and team of the Study of mechanism. Albert Rem Admiral John Theofanides The grandson of admiral Theophanidis holding the first effort of the reconstruction of the mechanism. Derek de Solla Price Michael Wright The new team of study the Antikythe ra mecha- nism Costas Xenakis, Pandelis Feleris, Rogger Hadland, David Beit, Gerasimos Makris, Michael Edmounds, Tony Freeth, Giannis Siradakis, Xenophon Mussas, Giannis Bitsakis, Agamemnon Tselikas, Mary Zafiropoulou, Helen Mangou, Bil Ambrisco, Tom Baltsbenter, Dan Gelmb, Rogger Hadland. -
The Historical Review/La Revue Historique
The Historical Review/La Revue Historique Vol. 10, 2013 The Crisis of the Long 1850s and Regime Change in the Ionian State and the Kingdom of Greece Gekas Sakis https://doi.org/10.12681/hr.306 Copyright © 2013 To cite this article: Gekas, S. (2013). The Crisis of the Long 1850s and Regime Change in the Ionian State and the Kingdom of Greece. The Historical Review/La Revue Historique, 10, 57-84. doi:https://doi.org/10.12681/hr.306 http://epublishing.ekt.gr | e-Publisher: EKT | Downloaded at 02/10/2021 16:38:35 | The crisis of The long 1850s and regime change in The ionian sTaTe and The kingdom of greece Sakis Gekas abstract: The overthrow of king othon in 1862 and the decolonization of the ionian islands led to the unification of the ionian state with the kingdom of greece. This article argues that the multifaceted crisis of the long 1850s (1847-1862) created a crisis of legitimacy for both the British Protectorate and the othonian regime. The change of regime represents a case where an economic, social and political crisis set in motion a process of democratization and not the rise of an authoritarian regime (as in the 1930s). The argument balances socio-economic structuralist factors with the contingency of political action that determined the union of the two states; this regime change was the optimal and favoured solution and the way out of the legitimacy crisis for all actors involved. Introduction from the late 1840s to the early 1860s commercial downturn, financial instability, foreign occupation, cholera outbreaks and food riots engulfed the ionian state and the kingdom of greece.