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E a S T 7 4 T H S T R E E T August 2021 Schedule
E A S T 7 4 T H S T R E E T KEY St udi o key on bac k SEPT EM BER 2021 SC H ED U LE EF F EC T IVE 09.01.21–09.30.21 Bolld New Class, Instructor, or Time ♦ Advance sign-up required M O NDA Y T UE S DA Y W E DNE S DA Y T HURS DA Y F RII DA Y S A T URDA Y S UNDA Y Atthllettiic Master of One Athletic 6:30–7:15 METCON3 6:15–7:00 Stacked! 8:00–8:45 Cycle Beats 8:30–9:30 Vinyasa Yoga 6:15–7:00 6:30–7:15 6:15–7:00 Condiittiioniing Gerard Conditioning MS ♦ Kevin Scott MS ♦ Steve Mitchell CS ♦ Mike Harris YS ♦ Esco Wilson MS ♦ MS ♦ MS ♦ Stteve Miittchellll Thelemaque Boyd Melson 7:00–7:45 Cycle Power 7:00–7:45 Pilates Fusion 8:30–9:15 Piillattes Remiix 9:00–9:45 Cardio Sculpt 6:30–7:15 Cycle Beats 7:00–7:45 Cycle Power 6:30–7:15 Cycle Power CS ♦ Candace Peterson YS ♦ Mia Wenger YS ♦ Sammiie Denham MS ♦ Cindya Davis CS ♦ Serena DiLiberto CS ♦ Shweky CS ♦ Jason Strong 7:15–8:15 Vinyasa Yoga 7:45–8:30 Firestarter + Best Firestarter + Best 9:30–10:15 Cycle Power 7:15–8:05 Athletic Yoga Off The Barre Josh Mathew- Abs Ever 9:00–9:45 CS ♦ Jason Strong 7:00–8:00 Vinyasa Yoga 7:00–7:45 YS ♦ MS ♦ MS ♦ Abs Ever YS ♦ Elitza Ivanova YS ♦ Margaret Schwarz YS ♦ Sarah Marchetti Meier Shane Blouin Luke Bernier 10:15–11:00 Off The Barre Gleim 8:00–8:45 Cycle Beats 7:30–8:15 Precision Run® 7:30–8:15 Precision Run® 8:45–9:45 Vinyasa Yoga Cycle Power YS ♦ Cindya Davis Gerard 7:15–8:00 Precision Run® TR ♦ Kevin Scott YS ♦ Colleen Murphy 9:15–10:00 CS ♦ Nikki Bucks TR ♦ CS ♦ Candace 10:30–11:15 Atletica Thelemaque TR ♦ Chaz Jackson Peterson 8:45–9:30 Pilates Fusion 8:00–8:45 -
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. -
What the Romans Knew Piero Scaruffi Copyright 2018 • Part II
What the Romans knew Piero Scaruffi Copyright 2018 http://www.scaruffi.com/know • Part II 1 What the Romans knew Archaic Roma Capitolium Forum 2 (Museo della Civiltà Romana, Roma) What the Romans Knew • Greek! – Wars against Carthage resulted in conquest of the Phoenician and Greek civilizations – Greek pantheon (Zeus=Jupiter, Juno = Hera, Minerva = Athena, Mars= Ares, Mercury = Hermes, Hercules = Heracles, Venus = Aphrodite,…) – Greek city plan (agora/forum, temples, theater, stadium/circus) – Beginning of Roman literature: the translation and adaptation of Greek epic and dramatic poetry (240 BC) – Beginning of Roman philosophy: adoption of Greek schools of philosophy (155 BC) – Roman sculpture: Greek sculpture 3 What the Romans Knew • Greek! – Greeks: knowing over doing – Romans: doing over knowing (never translated Aristotle in Latin) – “The day will come when posterity will be amazed that we remained ignorant of things that will to them seem so plain” (Seneca, 1st c AD) – Impoverished mythology – Indifference to metaphysics – Pragmatic/social religion (expressing devotion to the state) 4 What the Romans Knew • Greek! – Western civilization = the combined effect of Greece's construction of a new culture and Rome's destruction of all other cultures. 5 What the Romans Knew • The Mediterranean Sea (Mare Nostrum) – Rome was mainly a sea power, an Etruscan legacy – Battle of Actium (31 BC) created the “mare nostrum”, a peaceful, safe sea for trade and communication – Disappearance of piracy – Sea routes were used by merchants, soldiers, -
Ancient Rome
Ancient Rome William E. Dunstan ROWMAN & LITTLEFIELD PUBLISHERS, INC. Lanham • Boulder • New York • Toronto • Plymouth, UK ................. 17856$ $$FM 09-09-10 09:17:21 PS PAGE iii Published by Rowman & Littlefield Publishers, Inc. A wholly owned subsidiary of The Rowman & Littlefield Publishing Group, Inc. 4501 Forbes Boulevard, Suite 200, Lanham, Maryland 20706 http://www.rowmanlittlefield.com Estover Road, Plymouth PL6 7PY, United Kingdom Copyright ᭧ 2011 by Rowman & Littlefield Publishers, Inc. All maps by Bill Nelson. All rights reserved. No part of this book may be reproduced in any form or by any electronic or mechanical means, including information storage and retrieval systems, without written permission from the publisher, except by a reviewer who may quote passages in a review. The cover image shows a marble bust of the nymph Clytie; for more information, see figure 22.17 on p. 370. British Library Cataloguing in Publication Information Available Library of Congress Cataloging-in-Publication Data Dunstan, William E. Ancient Rome / William E. Dunstan. p. cm. Includes bibliographical references and index. ISBN 978-0-7425-6832-7 (cloth : alk. paper) ISBN 978-0-7425-6833-4 (pbk. : alk. paper) ISBN 978-0-7425-6834-1 (electronic) 1. Rome—Civilization. 2. Rome—History—Empire, 30 B.C.–476 A.D. 3. Rome—Politics and government—30 B.C.–476 A.D. I. Title. DG77.D86 2010 937Ј.06—dc22 2010016225 ⅜ϱ ீThe paper used in this publication meets the minimum requirements of American National Standard for Information Sciences—Permanence of Paper for Printed Library Materials, ANSI/ NISO Z39.48–1992. Printed in the United States of America ................ -
Sarah Provancher Jeanne Hilt (502) 439-7138 (502) 614-4122 [email protected] [email protected]
FOR IMMEDIATE RELEASE: Tuesday, June 5, 2018 CONTACT: Sarah Provancher Jeanne Hilt (502) 439-7138 (502) 614-4122 [email protected] [email protected] DOWNTOWN TO SHOWCASE FÊTE DE LA MUSIQUE LOUISVILLE ON JUNE 21 ST Downtown Louisville to celebrate the Summer Solstice with live music and more than 30 street performers for a day-long celebration of French culture Louisville, KY – A little taste of France is coming to Downtown Louisville on the summer solstice, Thursday, June 21st, with Fête de la Musique Louisville (pronounced fet de la myzic). The event, which means “celebration of music” in French, has been taking place in Paris on the summer solstice since 1982. Downtown Louisville’s “celebration of music” is presented by Alliance Francaise de Louisville in conjunction with the Louisville Downtown Partnership (LDP). Music will literally fill the downtown streets all day on the 21st with dozens of free live performances over the lunchtime hour and during a special Happy Hour showcase on the front steps of the Kentucky Center from 5:30-7:30pm. A list of performance venues with scheduled performers from 11am-1pm are: Fourth Street Live! – Classical musicians including The NouLou Chamber Players, 90.5 WUOL Young Musicians and Harin Oh, GFA Youth Guitar Summit Kindred Plaza – Hewn From The Mountain, a local Irish band 400 W. Market Plaza – FrenchAxe, a French band from Cincinnati Old Forester Distillery – A local jug band The salsa band Milenio is the scheduled performance group for the Happy Hour also at Fourth Street Live! from 5 – 7 pm. "In Paris and throughout France, the Fête de la Musique is literally 24 hours filled with music by all types of musicians of all skill levels. -
Regents and Midterm Prep Answers
Name__________________________________!Regents and Mid Term Preparation The Seasons Description Position Description Position March 21st B South Pole-24 Hrs of Dark C June 21st C High Kinetic Energy A December 21st A Low Kinetic Energy C September 23rd D Earth Close to Sun A Northern Hemisphere Winter A Earth Far from Sun C Northern Hemisphere Spring B Southern Hemisphere Spring D North Hemisphere Summer C Southern Hemisphere Fall B Northern Hemisphere Fall D Southern Hemisphere Winter C Greatest Orbital Velocity A South Hemisphere Summer A Least Orbital Velocity C 9 Hrs of Day in NYS A 23 1/2 N-Zenith C 12 Hrs of Day in NYS D,B 0 (Equator)-Zenith D,B 15 Hrs of Day in NYS C 23 1/2 S-Zenith A Winter Solstice A North Pole-24 Hrs Day C Vernal Equinox B South Pole-24 Hrs Day A Autumnal Equinox D North Pole-24 Hrs Dark A Summer Solstice C Name__________________________________!Regents and Mid Term Preparation Sunʼs Path in NYS 1. What direction does the sun rise in summer? _____NE___________________ 2. What direction does the sun rise in winter? _________SE_________________ 3. What direction does the sun rise in fall/spring? ________E_______________ 4. How long is the sun out in fall/spring? ____12________ 5. How long is the sun out in winter? _________9______ 6. How long is the sun out in summer? ________15_______ 7. What direction do you look to see the noon time sun? _____S________ 8. What direction do you look to see polaris? _______N_________ 9. From sunrise to noon, what happens to the length of a shadow? ___SMALLER___ 10. -
Vocabulary Unit 13
Vocabulary Unit 13 Origin of the days of the week Sunday: The name comes from the Latin dies solis, meaning "sun's day": the name of a pagan Roman holiday. It is also called Dominica (Latin), the Day of God. [French: dimanche; Italian: domenica; Spanish: domingo German: Sonntag;] Monday: The name comes from the Anglo-Saxon monandaeg, "the moon's day". This second day was sacred to the goddess of the moon. [French: lundi; Italian: lunedi. Spanish: lunes. German: Montag] Tuesday: This day was named after the Norse god Tyr. The Romans named this day after their war-god Mars: dies Martis. [French: mardi; Italian: martedi; Spanish: martes.] Wednesday: The day named to honor Wodan (Odin). The Romans called it dies Mercurii, after their god Mercury. [French: mercredi; Italian: mercoledi; Spanish: miércoles. German: Mittwoch] Thursday: The day named after the Norse god Thor. In the Norse languages this day is called Torsdag. The Romans named this day dies Jovis ("Jove's Day"), after Jove or Jupiter. [French: jeudi; Italian: giovedi; Spanish: jueves.] Friday: The day in honor of the Norse goddess, Frigg. To the Romans this day was sacred to the goddess Venus, and was known as dies veneris. [French: vendredi; Italian: venerdi; Spanish: viernes. German: Freitag] Saturday: This day was called dies Saturni, "Saturn's Day", by the ancient Romans in honor of Saturn. In Anglo- Saxon: sater daeg. [French: samedi; Italian: sabato; Spanish: sábado. Origin of the months of the year January: Named after the Roman god of beginnings and endings Janus (the month Januarius). Janus was the keeper of the gates of heaven. -
Summer Solstice
A FREE RESOURCE PACK FROM EDMENTUM Summer Solstice PreK–6th Topical Teaching Grade Range Resources Free school resources by Edmentum. This may be reproduced for class use. Summer Solstice Topical Teaching Resources What Does This Pack Include? This pack has been created by teachers, for teachers. In it you’ll find high quality teaching resources to help your students understand the background of Summer Solstice and why the days feel longer in the summer. To go directly to the content, simply click on the title in the index below: FACT SHEETS: Pre-K – Grade 3 Grades 3-6 Grades 3-6 Discover why the Sun rises earlier in the day Understand how Earth moves and how it Discover how other countries celebrate and sets later every night. revolves around the Sun. Summer Solstice. CRITICAL THINKING QUESTIONS: Pre-K – Grade 2 Grades 3-6 Discuss what shadows are and how you can create them. Discuss how Earth’s tilt cause the seasons to change. ACTIVITY SHEETS AND ANSWERS: Pre-K – Grade 3 Grades 3-6 Students are to work in pairs to explain what happens during Follow the directions to create a diagram that describes the Summer Solstice. Summer Solstice. POSTER: Pre-K – Grade 6 Enjoyed these resources? Learn more about how Edmentum can support your elementary students! Email us at www.edmentum.com or call us on 800.447.5286 Summer Solstice Fact Sheet • Have you ever noticed in the summer that the days feel longer? This is because there are more hours of daylight in the summer. • In the summer, the Sun rises earlier in the day and sets later every night. -
Public Construction, Labor, and Society at Middle Republican Rome, 390-168 B.C
University of Pennsylvania ScholarlyCommons Publicly Accessible Penn Dissertations 2012 Men at Work: Public Construction, Labor, and Society at Middle Republican Rome, 390-168 B.C. Seth G. Bernard University of Pennsylvania, [email protected] Follow this and additional works at: https://repository.upenn.edu/edissertations Part of the Ancient History, Greek and Roman through Late Antiquity Commons, and the History of Art, Architecture, and Archaeology Commons Recommended Citation Bernard, Seth G., "Men at Work: Public Construction, Labor, and Society at Middle Republican Rome, 390-168 B.C." (2012). Publicly Accessible Penn Dissertations. 492. https://repository.upenn.edu/edissertations/492 This paper is posted at ScholarlyCommons. https://repository.upenn.edu/edissertations/492 For more information, please contact [email protected]. Men at Work: Public Construction, Labor, and Society at Middle Republican Rome, 390-168 B.C. Abstract MEN AT WORK: PUBLIC CONSTRUCTION, LABOR, AND SOCIETY AT MID-REPUBLICAN ROME, 390-168 B.C. Seth G. Bernard C. Brian Rose, Supervisor of Dissertation This dissertation investigates how Rome organized and paid for the considerable amount of labor that went into the physical transformation of the Middle Republican city. In particular, it considers the role played by the cost of public construction in the socioeconomic history of the period, here defined as 390 to 168 B.C. During the Middle Republic period, Rome expanded its dominion first over Italy and then over the Mediterranean. As it developed into the political and economic capital of its world, the city itself went through transformative change, recognizable in a great deal of new public infrastructure. -
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. -
Equation of Time — Problem in Astronomy M
This paper was awarded in the II International Competition (1993/94) "First Step to Nobel Prize in Physics" and published in the competition proceedings (Acta Phys. Pol. A 88 Supplement, S-49 (1995)). The paper is reproduced here due to kind agreement of the Editorial Board of "Acta Physica Polonica A". EQUATION OF TIME | PROBLEM IN ASTRONOMY M. Muller¨ Gymnasium M¨unchenstein, Grellingerstrasse 5, 4142 M¨unchenstein, Switzerland Abstract The apparent solar motion is not uniform and the length of a solar day is not constant throughout a year. The difference between apparent solar time and mean (regular) solar time is called the equation of time. Two well-known features of our solar system lie at the basis of the periodic irregularities in the solar motion. The angular velocity of the earth relative to the sun varies periodically in the course of a year. The plane of the orbit of the earth is inclined with respect to the equatorial plane. Therefore, the angular velocity of the relative motion has to be projected from the ecliptic onto the equatorial plane before incorporating it into the measurement of time. The math- ematical expression of the projection factor for ecliptic angular velocities yields an oscillating function with two periods per year. The difference between the extreme values of the equation of time is about half an hour. The response of the equation of time to a variation of its key parameters is analyzed. In order to visualize factors contributing to the equation of time a model has been constructed which accounts for the elliptical orbit of the earth, the periodically changing angular velocity, and the inclined axis of the earth. -
Research on the Precession of the Equinoxes and on the Nutation of the Earth’S Axis∗
Research on the Precession of the Equinoxes and on the Nutation of the Earth’s Axis∗ Leonhard Euler† Lemma 1 1. Supposing the earth AEBF (fig. 1) to be spherical and composed of a homogenous substance, if the mass of the earth is denoted by M and its radius CA = CE = a, the moment of inertia of the earth about an arbitrary 2 axis, which passes through its center, will be = 5 Maa. ∗Leonhard Euler, Recherches sur la pr´ecession des equinoxes et sur la nutation de l’axe de la terr,inOpera Omnia, vol. II.30, p. 92-123, originally in M´emoires de l’acad´emie des sciences de Berlin 5 (1749), 1751, p. 289-325. This article is numbered E171 in Enestr¨om’s index of Euler’s work. †Translated by Steven Jones, edited by Robert E. Bradley c 2004 1 Corollary 2. Although the earth may not be spherical, since its figure differs from that of a sphere ever so slightly, we readily understand that its moment of inertia 2 can be nonetheless expressed as 5 Maa. For this expression will not change significantly, whether we let a be its semi-axis or the radius of its equator. Remark 3. Here we should recall that the moment of inertia of an arbitrary body with respect to a given axis about which it revolves is that which results from multiplying each particle of the body by the square of its distance to the axis, and summing all these elementary products. Consequently this sum will give that which we are calling the moment of inertia of the body around this axis.