PRIME MERIDIAN a Place Is
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TYPHOONS and DEPRESSIONS OVER the FAR EAST Morning Observation, Sep Teinber 6, from Rasa Jima Island by BERNARDF
SEPTEMBER1940 MONTHLY WEATHER REVIEW 257 days west of the 180th meridian. In American coastal appear to be independent of the typhoon of August 28- waters fog was noted on 10 days each off Washington and September 5, are the following: The S. S. Steel Exporter California; on 4 days off Oregon; and on 3 days off Lower reported 0700 G. C. T. September 6, from latitude 20'18' California. N., longitude 129'30'E.) a pressure of 744.8 mm. (993.0 nib.) with west-northwest winds of force 9. Also, the TYPHOONS AND DEPRESSIONS OVER THE FAR EAST morning observation, Sep teinber 6, from Rasa Jima Island By BERNARDF. DOUCETTE, J. (one of the Nansei Island group) was 747.8 mm. (997.0 5. mb.) for pressure and east-northeast, force 4, for winds. [Weather Bureau, Manila, P. I.] Typhoon, September 11-19) 1940.-A depression, moving Typhoon, August %!-September 6,1940.-A low-pressure westerly, passed about 200 miles south of Guam and area far to the southeast of Guam moved west-northwest, quickly inclined to the north, intensifying to typhoon rapidly developing to typhoon intensity as it proceeded. strength, September 11 to 13. It was stationary, Sep- When the center reached the regions about 250 miles tember 13 and 14, about 150 miles west-northwest of west of Guam, the direction changed to the northwest, Guam, and then began a northwesterly and northerly and the storm continued along this course until it reached course to the ocean regions about 300 miles west of the the latitude of southern Formosa. -
2. Disc Resources
An early map of the world Resource D1 A map of the world drawn in 1570 shows ‘Terra Australis Nondum Cognita’ (the unknown south land). National Library of Australia Expeditions to Antarctica 1770 –1830 and 1910 –1913 Resource D2 Voyages to Antarctica 1770–1830 1772–75 1819–20 1820–21 Cook (Britain) Bransfield (Britain) Palmer (United States) ▼ ▼ ▼ ▼ ▼ Resolution and Adventure Williams Hero 1819 1819–21 1820–21 Smith (Britain) ▼ Bellingshausen (Russia) Davis (United States) ▼ ▼ ▼ Williams Vostok and Mirnyi Cecilia 1822–24 Weddell (Britain) ▼ Jane and Beaufoy 1830–32 Biscoe (Britain) ★ ▼ Tula and Lively South Pole expeditions 1910–13 1910–12 1910–13 Amundsen (Norway) Scott (Britain) sledge ▼ ▼ ship ▼ Source: Both maps American Geographical Society Source: Major voyages to Antarctica during the 19th century Resource D3 Voyage leader Date Nationality Ships Most southerly Achievements latitude reached Bellingshausen 1819–21 Russian Vostok and Mirnyi 69˚53’S Circumnavigated Antarctica. Discovered Peter Iøy and Alexander Island. Charted the coast round South Georgia, the South Shetland Islands and the South Sandwich Islands. Made the earliest sighting of the Antarctic continent. Dumont d’Urville 1837–40 French Astrolabe and Zeelée 66°S Discovered Terre Adélie in 1840. The expedition made extensive natural history collections. Wilkes 1838–42 United States Vincennes and Followed the edge of the East Antarctic pack ice for 2400 km, 6 other vessels confirming the existence of the Antarctic continent. Ross 1839–43 British Erebus and Terror 78°17’S Discovered the Transantarctic Mountains, Ross Ice Shelf, Ross Island and the volcanoes Erebus and Terror. The expedition made comprehensive magnetic measurements and natural history collections. -
AIM: Latitude and Longitude
AIM: Latitude and Longitude Latitude lines run east/west but they measure north or south of the equator (0°) splitting the earth into the Northern Hemisphere and Southern Hemisphere. Latitude North Pole 90 80 Lines of 70 60 latitude are 50 numbered 40 30 from 0° at 20 Lines of [ 10 the equator latitude are 10 to 90° N.L. 20 numbered 30 at the North from 0° at 40 Pole. 50 the equator ] 60 to 90° S.L. 70 80 at the 90 South Pole. South Pole Latitude The North Pole is at 90° N 40° N is the 40° The equator is at 0° line of latitude north of the latitude. It is neither equator. north nor south. It is at the center 40° S is the 40° between line of latitude north and The South Pole is at 90° S south of the south. equator. Longitude Lines of longitude begin at the Prime Meridian. 60° W is the 60° E is the 60° line of 60° line of longitude west longitude of the Prime east of the W E Prime Meridian. Meridian. The Prime Meridian is located at 0°. It is neither east or west 180° N Longitude West Longitude West East Longitude North Pole W E PRIME MERIDIAN S Lines of longitude are numbered east from the Prime Meridian to the 180° line and west from the Prime Meridian to the 180° line. Prime Meridian The Prime Meridian (0°) and the 180° line split the earth into the Western Hemisphere and Eastern Hemisphere. Prime Meridian Western Eastern Hemisphere Hemisphere Places located east of the Prime Meridian have an east longitude (E) address. -
Date Day Peculiarity Position of the Sun Northern Hemisphere Southern
Date Day Peculiarity Position of the Northern Southern sun hemisphere hemisphere March 21 Equinox Length of day Above the From March and night will Equator 21 to be equal ( 0° ) June 21 Spring Autumn June 21 Summer Northern Above the From June 21 Solstice Hemisphere Tropic of to September experiences its Cancer 23 longest day (231⁄2°N) and shortest night Summer Winter September 23 Equinox Length of day Above the From and night will Equator September 23 be equal ( 0° ) to December 22 Autumn Spring December 22 Winter Solstice Northern Above Tropic From Hemisphere of Capricorn December 22 experiences (231⁄2°S) to March 21 its shortest day and longest night. Winter Summer Utharayanam Dakshinayanam The Sun sets its northward apparent The Sun sets its movement southward apparent movement from Tropic of Capricorn (231⁄2°S) and from Tropic of Cancer (231⁄2°N) and it it culminates on Tropic of Cancer (231⁄2°N) culminates on Tropic of Capricorn (231⁄2°S) Following the winter solstice to June 21. Following the summer solstice to December 22 Causes Earth's revolution It is in an elliptical orbit that the Earth revolves around the Sun Tilt of the axis The axis of the Earth is tilted at an angle of ( the inclination of axis ) 661⁄2° from the orbital plane. If measured from the vertical plane this would be 231⁄2° Parallelism of the Earth's axis. The Earth maintains this tilt throughout its revolution. The apparent movement of the Sun. Since the parallelism is maintained same throughout the revolution, the position of the Sun in relation to the Earth varies apparently between Tropic of Cancer (231⁄2° North) and Tropic of Capricorn (231⁄2° South). -
The International Date Line!
The International Date Line! The International Date Line (IDL) is a generally north-south imaginary line on the surface of the Earth, passing through the middle of the Pacific Ocean, that designates the place where each calendar day begins. It is roughly along 180° longitude, opposite the Prime Meridian, but it is drawn with diversions to pass around some territories and island groups. Crossing the IDL travelling east results in a day or 24 hours being subtracted, so that the traveller repeats the date to the west of the line. Crossing west results in a day being added, that is, the date is the eastern side date plus one calendar day. The line is necessary in order to have a fixed, albeit arbitrary, boundary on the globe where the calendar date advances. Geography For part of its length, the International Date Line follows the meridian of 180° longitude, roughly down the middle of the Pacific Ocean. To avoid crossing nations internally, however, the line deviates to pass around the far east of Russia and various island groups in the Pacific. In the north, the date line swings to the east of Wrangel island and the Chukchi Peninsula and through the Bering Strait passing between the Diomede Islands at a distance of 1.5 km (1 mi) from each island. It then goes southwest, passing west of St. Lawrence Island and St. Matthew Island, until it passes midway between the United States' Aleutian Islands and Russia's Commander Islands before returning southeast to 180°. This keeps Russia which is north and west of the Bering Sea and the United States' Alaska which is east and south of the Bering Sea, on opposite sides of the line in agreement with the date in the rest of those countries. -
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. -
The Longitude of the Mediterranean Throughout History: Facts, Myths and Surprises Luis Robles Macías
The longitude of the Mediterranean throughout history: facts, myths and surprises Luis Robles Macías To cite this version: Luis Robles Macías. The longitude of the Mediterranean throughout history: facts, myths and sur- prises. E-Perimetron, National Centre for Maps and Cartographic Heritage, 2014, 9 (1), pp.1-29. hal-01528114 HAL Id: hal-01528114 https://hal.archives-ouvertes.fr/hal-01528114 Submitted on 27 May 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. e-Perimetron, Vol. 9, No. 1, 2014 [1-29] www.e-perimetron.org | ISSN 1790-3769 Luis A. Robles Macías* The longitude of the Mediterranean throughout history: facts, myths and surprises Keywords: History of longitude; cartographic errors; comparative studies of maps; tables of geographical coordinates; old maps of the Mediterranean Summary: Our survey of pre-1750 cartographic works reveals a rich and complex evolution of the longitude of the Mediterranean (LongMed). While confirming several previously docu- mented trends − e.g. the adoption of erroneous Ptolemaic longitudes by 15th and 16th-century European cartographers, or the striking accuracy of Arabic-language tables of coordinates−, we have observed accurate LongMed values largely unnoticed by historians in 16th-century maps and noted that widely diverging LongMed values coexisted up to 1750, sometimes even within the works of one same author. -
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. -
Prime Meridian ×
This website would like to remind you: Your browser (Apple Safari 4) is out of date. Update your browser for more × security, comfort and the best experience on this site. Encyclopedic Entry prime meridian For the complete encyclopedic entry with media resources, visit: http://education.nationalgeographic.com/encyclopedia/prime-meridian/ The prime meridian is the line of 0 longitude, the starting point for measuring distance both east and west around the Earth. The prime meridian is arbitrary, meaning it could be chosen to be anywhere. Any line of longitude (a meridian) can serve as the 0 longitude line. However, there is an international agreement that the meridian that runs through Greenwich, England, is considered the official prime meridian. Governments did not always agree that the Greenwich meridian was the prime meridian, making navigation over long distances very difficult. Different countries published maps and charts with longitude based on the meridian passing through their capital city. France would publish maps with 0 longitude running through Paris. Cartographers in China would publish maps with 0 longitude running through Beijing. Even different parts of the same country published materials based on local meridians. Finally, at an international convention called by U.S. President Chester Arthur in 1884, representatives from 25 countries agreed to pick a single, standard meridian. They chose the meridian passing through the Royal Observatory in Greenwich, England. The Greenwich Meridian became the international standard for the prime meridian. UTC The prime meridian also sets Coordinated Universal Time (UTC). UTC never changes for daylight savings or anything else. Just as the prime meridian is the standard for longitude, UTC is the standard for time. -
Civil Twilight Duration (Sunset to Solar Depression
Civil Twilight Duration (sunset to solar depression 6°) at the Prime Meridian, Sea Level, Northern Hemisphere (March 1, 2007 to March 31, 2008) Mar 1 Mar 15 Mar 29 Apr 12 Apr 26 May 10 May 24 7 Jun 21 Jun Jul 5 Jul 19 Aug 2 Aug 16 Aug 30 Sep 13 Sep 27 11 Oct 25 Oct Nov 8 Nov 22 Dec 6 Dec 20 Jan 3 Jan 17 Jan 31 14 Feb 28 Feb Mar 13 Mar 27 20 25 30 35 40 45 50 55 60 65 70 75 80 85 90 95 Civil Twilight Duration (daytime temporal minutes after sunset) after minutes temporal (daytime Duration Civil Twilight 23.5° N 30° N 100 40° N 45° N 105 50° N 55° N 58° N 59° N 110 60° N 61° N Northward Equinox North Solstice 115 Southward Equinox South Solstice 120 Analysis by Dr. Irv Bromberg, University of Toronto, Canada http://www.sym454.org/twilight/ Civil Twilight Duration (sunset to solar depression 6°) at the Prime Meridian, Sea Level, Southern Hemisphere (March 1, 2007 to March 31, 2008) Mar 1 Mar 15 Mar 29 Apr 12 Apr 26 May 10 May 24 7 Jun 21 Jun Jul 5 Jul 19 Aug 2 Aug 16 Aug 30 Sep 13 Sep 27 11 Oct 25 Oct Nov 8 Nov 22 Dec 6 Dec 20 Jan 3 Jan 17 Jan 31 14 Feb 28 Feb Mar 13 Mar 27 20 25 30 35 40 45 50 55 60 65 70 75 80 85 90 95 23.5° S 30° S Civil Twilight Duration (daytime temporal minutes after sunset) after minutes temporal (daytime Duration Civil Twilight 100 40° S 45° S 50° S 55° S 105 58° S 59° S 110 60° S 61° S Northward Equinox North Solstice 115 Southward Equinox South Solstice 120 Analysis by Dr. -
Earth-Moon-Sun-System EQUINOX Presentation V2.Pdf
The Sun http://c.tadst.com/gfx/750x500/sunrise.jpg?1 The sun dominates activity on Earth: living and nonliving. It'd be hard to imagine a day without it. The daily pattern of the sun rising in the East and setting in the West is how we measure time...marking off the days of our lives. 6 The Sun http://c.tadst.com/gfx/750x500/sunrise.jpg?1 Virtually all life on Earth is aware of, and responds to, the sun's movements. Well before there was written history, humankind had studied those patterns. 7 Daily Patterns of the Sun • The sun rises in the east and sets in the west. • The time between sunrises is always the same: that amount of time is called a "day," which we divide into 24 hours. Note: The term "day" can be confusing since it is used in two ways: • The time between sunrises (always 24 hours). • To contrast "day" to "night," in which case day means the time during which there is daylight (varies in length). For instance, when we refer to the summer solstice as being the longest day of the year, we mean that it has the most daylight hours of any day. 8 Explaining the Sun What would be the simplest explanation of these two patterns? • The sun rises in the east and sets in the west. • The time between sunrises is always the same: that amount of time is called a "day." We now divide the day into 24 hours. Discuss some ideas to explain these patterns.