Time and Diurnal Motion

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Presentation transcript:

Time and Diurnal Motion Updated 2014Jan11

Time and Diurnal Motion 2 Time and Diurnal Motion Geography: mapping the earth Equatorial Coordinates Local Horizon System

A. Geography: mapping the earth 3 A. Geography: mapping the earth Geometry: measure the earth! The earth is a ball Geographic Coordinates Definition of Time

1a. The Earth Is Round Pythagoras of Samos (569-475 BC) “the first pure mathematician” lunar eclipses imply shadow of earth is round Bottoms of ships vanish first as ship goes to sea

1b. Aristotle (384-322 BC) 5 notes change in altitude of north star as travel south Estimates circumference of earth is 74,000 km (true value is 40,000 km)

1c. Eratosthenes (275-194 BC) 6 236 BC Director Library of Alexandria 240 BC Was told that on midsummer day (June 21) in the town of Syene in southern Egypt (today Aswan, near a huge dam on the river Nile) the noontime Sun was reflected in a deep well, meaning that it was right overhead, at zenith. But at Alexandria, on same day it was NOT overhead!

Erastotenes [within 1% true value] 7 In Alexandria sunlight was at angle of 7.2 degrees. Hired soldier to march out distance between cities: 5040 Stadia Calculates circumference is 250,000 stades [within 1% true value]

2. Cartography Spherical coordinates probably first done by 8 Spherical coordinates probably first done by Pythagoras (470 BC), Aristotle (330 BC), Eratosthenes (240 BC) Hipparchus (120 BC).

2b. Latitude is measured up from equator Hayward is 37N40’08” 9 is measured up from equator Hayward is 37N40’08” Equator is 0 N pole is 90 What is latitude Of South Pole?

2c. Longitude is measured westward from Greenwich, England 10 is measured westward from Greenwich, England Hayward is 122W04’51” Greenwich is 0 What is the longitude of the north pole?

Greenwich Observatory England (established 1675) 11 Greenwich Observatory England (established 1675)

0° Longitude at Greenwich 12 0° Longitude at Greenwich

Airy Transit Telescope 13

3. Solar Time 14

3a) Sundials measure “solar” time 15 340 BC Berosus Sundial Shaped like a bowel. The “longitude” line on the bowel tells how many hours before or after noon the sun is. The transit of the sun (when sun crosses local prime merdian) happens at NOON (12 hours) local time.

3b) UT: Universal Time 16 GMT: Greenwich mean time, the solar time at Greenwich Observatory [nearly the same as UT: “Universal Time” and ET: “Ephemeris Time”]

3b) Time is Relative When its 6 pm here 9 pm 2 am 17 When its 6 pm here What time is it in Boston? What time is it in Greenwich? Definition of time depends upon your longitude 9 pm 2 am

3b) Time Zones are 15° (1 hr) wide 18

California is in Pacific Zone 19 Pacific Standard time: PST PST = GMT – 8 hours Pacific Daylight Time: PDT = PST+1

3c. Local Mean Time 20 At Lake Tahoe (120 degrees longitude) sun transits on average at 12:00 noon PST. At Hayward, sun transits on average 12:08 PST. This is because we are 2 degrees longitude west of Lake Tahoe. It takes 8 minutes for the sun to travel from Lake Tahoe to here. Local Mean Time: LMT = PST – 8 minutes Sun Transits (on average) at 12:00 LMT

3c. Longitude Measure longitude in terms of time 21 Measure longitude in terms of time If 360° is equal to 24 hour 15° is equal to 1 hour 1° is equal to 4 minutes 1’ is equal to 4 seconds Hayward’s Longitude is hence 8 hours, 8 minutes, 19.4 seconds West of Greenwich, England

3c) Relate Time & Longitude 22 LMT: Local mean time or sundial time the time at our location LMT=GMT - Longitude Hayward’s Longitude is 8h8m LMT =GMT – 8h8m LMT = PST – 8m