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The Evolution of the Roman Calendar Dwayne Meisner, University of Regina
The Evolution of the Roman Calendar Dwayne Meisner, University of Regina Abstract The Roman calendar was first developed as a lunar | 290 calendar, so it was difficult for the Romans to reconcile this with the natural solar year. In 45 BC, Julius Caesar reformed the calendar, creating a solar year of 365 days with leap years every four years. This article explains the process by which the Roman calendar evolved and argues that the reason February has 28 days is that Caesar did not want to interfere with religious festivals that occurred in February. Beginning as a lunar calendar, the Romans developed a lunisolar system that tried to reconcile lunar months with the solar year, with the unfortunate result that the calendar was often inaccurate by up to four months. Caesar fixed this by changing the lengths of most months, but made no change to February because of the tradition of intercalation, which the article explains, and because of festivals that were celebrated in February that were connected to the Roman New Year, which had originally been on March 1. Introduction The reason why February has 28 days in the modern calendar is that Caesar did not want to interfere with festivals that honored the dead, some of which were Past Imperfect 15 (2009) | © | ISSN 1711-053X | eISSN 1718-4487 connected to the position of the Roman New Year. In the earliest calendars of the Roman Republic, the year began on March 1, because the consuls, after whom the year was named, began their years in office on the Ides of March. -
Whorfian, Feminist, and Marxist Readings Sam Whittaker University of Windsor
University of Windsor Scholarship at UWindsor Electronic Theses and Dissertations Theses, Dissertations, and Major Papers 8-3-2017 Language, Thought, and bpNichol's The Martyrology: Whorfian, Feminist, and Marxist Readings Sam Whittaker University of Windsor Follow this and additional works at: https://scholar.uwindsor.ca/etd Recommended Citation Whittaker, Sam, "Language, Thought, and bpNichol's The aM rtyrology: Whorfian, Feminist, and Marxist Readings" (2017). Electronic Theses and Dissertations. 6601. https://scholar.uwindsor.ca/etd/6601 This online database contains the full-text of PhD dissertations and Masters’ theses of University of Windsor students from 1954 forward. These documents are made available for personal study and research purposes only, in accordance with the Canadian Copyright Act and the Creative Commons license—CC BY-NC-ND (Attribution, Non-Commercial, No Derivative Works). Under this license, works must always be attributed to the copyright holder (original author), cannot be used for any commercial purposes, and may not be altered. Any other use would require the permission of the copyright holder. Students may inquire about withdrawing their dissertation and/or thesis from this database. For additional inquiries, please contact the repository administrator via email ([email protected]) or by telephone at 519-253-3000ext. 3208. Language, Thought, and bpNichol's The Martyrology: Whorfian, Feminist, and Marxist Readings By Sam Whittaker A Thesis Submitted to the Faculty of Graduate Studies through the Department of English Language, Literature, and Creative Writing in Partial Fulfilment of the Requirements for the Degree of Master of Arts at the University of Windsor Windsor, Ontario, Canada 2017 © 2017 Sam Whittaker Language, Thought, and bpNichol's The Martyrology: Whorfian, Feminist, and Marxist Readings by Sam Whittaker APPROVED BY: J. -
Lessons from Reading Clavius
Christopher Clavius, S.J. Calendar Reform Lessons from Clavius Conclusion Lessons from reading Clavius Anders O. F. Hendrickson Concordia College Moorhead, MN MathFest, Pittsburgh August 5, 2010 Christopher Clavius, S.J. Calendar Reform Lessons from Clavius Conclusion Outline 1 Christopher Clavius, S.J. 2 Calendar Reform 3 Lessons from Clavius 4 Conclusion Christopher Clavius, S.J. Calendar Reform Lessons from Clavius Conclusion Christopher Clavius, S.J. (1538–1612) Christopher Clavius, S.J. Calendar Reform Lessons from Clavius Conclusion Clavius’s life Born in Bamberg c. 1538 1555 received into the Society of Jesus by St. Ignatius Loyola 1556–1560 studied philosophy at Coimbra 1561–1566 studied theology at the Collegio Romano 1567–1612 professor of mathematics at Collegio Romano 1570 published Commentary on the Sphere of Sacrobosco 1574 published edition of Euclid’s Elements c. 1572–1582 on papal calendar commission c. 1595 retired from teaching, focused on research 1612 died in Rome Christopher Clavius, S.J. Calendar Reform Lessons from Clavius Conclusion Clavius as teacher As a teacher, Clavius Taught elementary (required) courses in astronomy Led a seminar for advanced students Fought for status of mathematics in the curriculum Christopher Clavius, S.J. Calendar Reform Lessons from Clavius Conclusion Calendar Reform: Solar How to keep the calendar in synch with solar year (365.24237 days, equinox to equinox): Julian calendar: 365.25 days Gregorian calendar: omit 3 leap days every 400 years; hence 365.2425 days Christopher Clavius, S.J. Calendar Reform Lessons from Clavius Conclusion Calendar Reform: Lunar Easter is the first Sunday after the first full moon on or after the vernal equinox. -
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. -
The Calculation of Doomsday Based on Anno Domini
SCIENTIFIC CULTURE, Vol. 1, No. 2, (2015), pp. 22-32 Copyright © 2015 SC Open Access. Printed in Greece. All Rights Reserved. The calculation of doomsday based on Anno Domini Sepp Rothwangl Waldwirtschaft Hubertushof Scheibsgraben 49, A-8661 Wartberg, Astria (CALENdeRsign.com;[email protected]) Received: 10/01/2015 Accepted: 15/02/2015 ABSTRACT Anno Domini, or the year Christ’s birth, was an invention made some 1400 years ago by Dionysius Exiguus, who adjusted a new Easter Computus in order to avert end time fever with the pretext to solve a dispute upon the correct date of Easter. Right at the beginning of Christianity, early Christians expected in the near future the return of Christ, which was associated with the end of the world, together with the Seventh Day of the Lord. Such a scenario ocurred already in the cosmic year Anno Mundi (AM) 6,000 based upon a teleological concept by interpreting the Bible. AM produced a calendrical end time with its year 6000 due to equating the Six Days of Genesis with the verse of the Bible saying one Day of the Lord was the same as 1000 years of mankind. To combat the end of the world fever caused by this time concept at the beginning of the 6th century Dionysius Exiguus created a new temporal hinge point for counting the years: Anno Domini. Obviously this chronology is not in harmony with ancient historical works, as even former Pope Benedict XVI recognized, but is an end time prophecy by interpreting the Gospel, the Apocalypse, the scientific cosmology of antiquity, and astronomical values. -
The Late Republic in 5 Timelines (Teacher Guide and Notes)
1 180 BC: lex Villia Annalis – a law regulating the minimum ages at which a individual could how political office at each stage of the cursus honorum (career path). This was a step to regularising a political career and enforcing limits. 146 BC: The fall of Carthage in North Africa and Corinth in Greece effectively brought an end to Rome’s large overseas campaigns for control of the Mediterranean. This is the point that the historian Sallust sees as the beginning of the decline of the Republic, as Rome had no rivals to compete with and so turn inwards, corrupted by greed. 139 BC: lex Gabinia tabelleria– the first of several laws introduced by tribunes to ensure secret ballots for for voting within the assembliess (this one applied to elections of magistrates). 133 BC – the tribunate of Tiberius Gracchus, who along with his younger brother, is seen as either a social reformer or a demagogue. He introduced an agrarian land that aimed to distribute Roman public land to the poorer elements within Roman society (although this act quite likely increased tensions between the Italian allies and Rome, because it was land on which the Italians lived that was be redistributed). He was killed in 132 BC by a band of senators led by the pontifex maximus (chief priest), because they saw have as a political threat, who was allegedly aiming at kingship. 2 123-121 BC – the younger brother of Tiberius Gracchus, Gaius Gracchus was tribune in 123 and 122 BC, passing a number of laws, which apparent to have aimed to address a number of socio-economic issues and inequalities. -
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. -
CALENDARS by David Le Conte
CALENDARS by David Le Conte This article was published in two parts, in Sagittarius (the newsletter of La Société Guernesiaise Astronomy Section), in July/August and September/October 1997. It was based on a talk given by the author to the Astronomy Section on 20 May 1997. It has been slightly updated to the date of this transcript, December 2007. Part 1 What date is it? That depends on the calendar used:- Gregorian calendar: 1997 May 20 Julian calendar: 1997 May 7 Jewish calendar: 5757 Iyyar 13 Islamic Calendar: 1418 Muharaim 13 Persian Calendar: 1376 Ordibehesht 30 Chinese Calendar: Shengxiao (Ox) Xin-You 14 French Rev Calendar: 205, Décade I Mayan Calendar: Long count 12.19.4.3.4 tzolkin = 2 Kan; haab = 2 Zip Ethiopic Calendar: 1990 Genbot 13 Coptic Calendar: 1713 Bashans 12 Julian Day: 2450589 Modified Julian Date: 50589 Day number: 140 Julian Day at 8.00 pm BST: 2450589.292 First, let us note the difference between calendars and time-keeping. The calendar deals with intervals of at least one day, while time-keeping deals with intervals less than a day. Calendars are based on astronomical movements, but they are primarily for social rather than scientific purposes. They are intended to satisfy the needs of society, for example in matters such as: agriculture, hunting. migration, religious and civil events. However, it has also been said that they do provide a link between man and the cosmos. There are about 40 calendars now in use. and there are many historical ones. In this article we will consider six principal calendars still in use, relating them to their historical background and astronomical foundation. -
Calendar of Roman Events
Introduction Steve Worboys and I began this calendar in 1980 or 1981 when we discovered that the exact dates of many events survive from Roman antiquity, the most famous being the ides of March murder of Caesar. Flipping through a few books on Roman history revealed a handful of dates, and we believed that to fill every day of the year would certainly be impossible. From 1981 until 1989 I kept the calendar, adding dates as I ran across them. In 1989 I typed the list into the computer and we began again to plunder books and journals for dates, this time recording sources. Since then I have worked and reworked the Calendar, revising old entries and adding many, many more. The Roman Calendar The calendar was reformed twice, once by Caesar in 46 BC and later by Augustus in 8 BC. Each of these reforms is described in A. K. Michels’ book The Calendar of the Roman Republic. In an ordinary pre-Julian year, the number of days in each month was as follows: 29 January 31 May 29 September 28 February 29 June 31 October 31 March 31 Quintilis (July) 29 November 29 April 29 Sextilis (August) 29 December. The Romans did not number the days of the months consecutively. They reckoned backwards from three fixed points: The kalends, the nones, and the ides. The kalends is the first day of the month. For months with 31 days the nones fall on the 7th and the ides the 15th. For other months the nones fall on the 5th and the ides on the 13th. -
Roman Coins – Mass Media for Image Cultivation
Roman Coins – Mass Media for Image Cultivation Unlike modern coins, Roman money was characterized by an enormous diversity of coin images. This reflected not so much the desire for change, however, but rather an often very purposeful policy of concrete self-interests. At the time of the Roman Republic, coins were issued on behalf of the senate by a committee of moneyers. These men decided independently what motifs their coins were to bear, and, from the late 2nd century BC, used this liberty often for family propaganda. Later, during the time of the Firs and second triumvirate (60 to 32 BC), coins were issued by several powerful Romans or their adherents. These pieces were not republican any more, but imperatorial, and used mainly for the representation of political dispositions and ambitions. In imperial times finally (from 27 BC), the rulers of Rome were in charge of the issuance of money. Naturally, they used the large Roman coins for the artful conversion of political propaganda and self-manifestation as well. 1 von 20 www.sunflower.ch Roman Republic, L. Caecilius Metellus Diadematur (or Delmaticus), Denarius, 128 BC Denomination: Denarius Mint Authority: Moneyer Lucius Caecilius Metellus Diadematus (?) Mint: Rome Year of Issue: -128 Weight (g): 3.94 Diameter (mm): 18.0 Material: Silver Owner: Sunflower Foundation This denarius bears on the obverse a traditional motif, the head of Roma, the goddess and personification of Rome, wearing a winged attic helmet; behind her is the mark XVI for the value of 16 asses. The reverse depicts a goddess driving a biga, a two-horse racing chariot. -
The Gregorian Calendar in New Spain: a Problem in Sixteenth-Century Chronology." New Mexico Historical Review 58, 3 (1983)
New Mexico Historical Review Volume 58 Number 3 Article 3 7-1-1983 The Gregorian Calendar in New Spain: A Problem in Sixteenth- Century Chronology Harry Kelsey Follow this and additional works at: https://digitalrepository.unm.edu/nmhr Recommended Citation Kelsey, Harry. "The Gregorian Calendar in New Spain: A Problem in Sixteenth-Century Chronology." New Mexico Historical Review 58, 3 (1983). https://digitalrepository.unm.edu/nmhr/vol58/iss3/3 This Article is brought to you for free and open access by UNM Digital Repository. It has been accepted for inclusion in New Mexico Historical Review by an authorized editor of UNM Digital Repository. For more information, please contact [email protected], [email protected], [email protected]. THE GREGORIAN CALENDAR IN NEW SPAIN: A PROBLEM IN SIXTEENTH-CENTURY CHRONOLOGY HARRY KELSEY AFTER AYEAR-LONG JOURNEY TO NEW MEXICO, Antonio de Espejo arrived in Santa Barbara, Nueva Vizcaya, in the fall of 1583, weary, confused, but full of information about the new country he had seen. Almost immediately he began to compose a report, signing and dating it "at the end of the month of October" 1583. 1 This dating may seem imprecise for a formal report, and the truth is that Espejo did not know how to write the date. He seemed sure about the date of his return, 20 September, and he knew that he had been back for twenty-fivedays, more or less. He recorded all this very carefully in a covering letter. But Espejo was confused about the date. He could do no better in his calculations than to call it "the end of October."2 The reason for his confusion is simple. -
The Antikythera Mechanism, Rhodes, and Epeiros
The Antikythera Mechanism, Rhodes, and Epeiros Paul Iversen Introduction I am particularly honored to be asked to contribute to this Festschrift in honor of James Evans. For the last nine years I have been engaged in studying the Games Dial and the calendar on the Metonic Spiral of the Antikythera Mechanism,1 and in that time I have come to admire James’s willingness to look at all sides of the evidence, and the way in which he conducts his research in an atmosphere of collaborative and curious inquiry combined with mutual respect. It has long been suggested that the Antikythera Mechanism may have been built on the is- land of Rhodes,2 one of the few locations attested in ancient literary sources associated with the production of such celestial devices. This paper will strengthen the thesis of a Rhodian origin for the Mechanism by demonstrating that the as-of-2008-undeciphered set of games in Year 4 on the Games Dial were the Halieia of Rhodes, a relatively minor set of games that were, appro- priately for the Mechanism, in honor of the sun-god, Helios (spelled Halios by the Doric Greeks). This paper will also summarize an argument that the calendar on the Metonic Spiral cannot be that of Syracuse, and that it is, contrary to the assertions of a prominent scholar in Epirote stud- ies, consistent with the Epirote calendar. This, coupled with the appearance of the extremely minor Naan games on the Games Dial, suggests that the Mechanism also had some connection with Epeiros. The Games Dial and the Halieia of Rhodes The application in the fall of 2005 of micro-focus X-ray computed tomography on the 82 surviv- ing fragments of the Antikythera Mechanism led to the exciting discovery and subsequent publi- cation in 2008 of a dial on the Antikythera Mechanism listing various athletic games now known as the Olympiad Dial (but which I will call the Games or Halieiad Dial—more on that below), as well as a hitherto unknown Greek civil calendar on what is now called the Metonic Spiral.3 I begin with my own composite drawing of the Games Dial (Fig.