LESSON 18: Time Learning ObjectivesLearning Objectives –Comprehend the longitude/time relationship, time conversion, zone time determination, and motions.

Slides:



Advertisements
Similar presentations
Time.
Advertisements

Locating Positions on Earth
Chapter S1 Celestial Timekeeping and Navigation
Latitude and Longitude Part II
Latitude and Longitude
Phys. 102: Introduction to Astronomy
Aim: How are time zones created?
Finding your longitude The trickier part of celestial navigation.
A100 Oct. 13 Keeping Time READ Essay 2 – Keeping Time in the text, pp
Meridian Transit.
The Earth Rotates.
AST 208 Topics Time and celestial coordinates. Telescopes.
Natural Environments: The Atmosphere GE 101 – Spring 2007 Boston University Myneni Lecture 03: Rotating Sphere Jan (1 of 15) Outline Further Reading:
An Earth Day Sidereal Day: 23 hr 56 min 4 sec Motion relative to background stars Mean Solar Day: 24 hours The average time between meridian crossings.
Latitude & Longitude.
Navigation Latitude & Longitude
Locating Positions on Earth
Latitude & Longitude.
Where on Earth are You?.
International Time Zones
Mapping.
LONGITUDE (to measure East-West), is all a matter of time…
Table of Contents Title: Chapter 2 - Mapping our World Page #: 17
Modern Navigation Thomas Herring MW 11:00-12:30 Room
RRB PAGES Local Time and Time Zones. Solar Noon and Time Zones Solar Noon: when the sun is at the highest point in the sky. This may not be the.
Social Studies 9 Chapter 2 Time Zones.  A time zone is a region of the Earth that has adopted the same standard time, usually referred to as the local.
The Celestial Sphere The 88 official constellations cover the celestial sphere. If you do not have a model of the celestial sphere to bring to class, you.
1 Homework Q & A Junior Navigation Chapter 9 Meridian Transit of the Sun.
EARTH’S ROTATION CHAPTER 4.2. Objectives Give evidence of Earth’s rotation. Give evidence of Earth’s rotation. Relate Earth’s rotation to the day- night.
Announcements Homework set 1 is due today
Do Not Write What is in Yellow APPARENT MOTIONS OF THE CELESTIAL OBJECTS.
The Seasons There would be no seasons if the Earth were not tilted on it’s axis!  Nick Devereux 2006.
Where is it? On the Celestial Sphere. Longitude and Latitude On Earth: Longitude is how far you are, in degrees, East or West of the “Prime Meridian”
Unit #1: Measuring The Earth Parallel Lines on flat map. Concentric circles on a globe as viewed from the North Pole Latitude.
Word of the Day Nautical Mile: One minute of arc length of latitude or longitude at the equator, or 1852m.
Terrestrial Coordinate System
Bell Question Define the following terms: 1. Rotation 2. Revolution 3. Precession 4. Nutation Answer the following question: 5. What would happen if the.
Bellwork Open your textbook to page H9 in the front. 1. What time zone do you live within? 2. What two states do not observe Daylight Savings Time? 3.
4.2 E ARTH ’ S R OTATION DAHS Mr. Sweet 1 O BJECTIVES Give evidence of Earth’s rotation. Relate Earth’s rotation to the day-night cycle and the time.
Scaling & Daily Motion. Scaling Often one is interested in how quantities change when an object or a system is enlarged or shortened Different quantities.
Time TIME.
Observer Scanner Training Navigational Elements Section 5 by 1st Lt. Alan Fenter.
ACTUAL Regents Do Now: What is the latitude of this observer? ① 90° N ② 66.5° N ③ 43° N ④ 23.5° N.
Celestial Navigation How to determine latitude and longitude using the stars!
Navigation Unit 1-Planet Earth. What is Navigation?  The science of locating a position on earth.
How are Earth’s surface features measured and modeled?
Longitude and Time.
Time Zones Astronomy Unit Ch Effect of Earth’s rotation Created based on the rate at which the sun appears to move across the sky ▫Sun rises in.
LESSON 15: Celestial Coordinate Systems Learning ObjectivesLearning Objectives –Know the ultimate goal of celestial navigation. –Know the definitions of.
Announcements No lab after lecture tonight because of the 1 st Quarter night last Tuesday Homework: Chapter 2 # 2, 3, 4, 5, 7 & 8 Binoculars are available.
Weather & Climate Lab 1B - 1E. Lab 1B: Earth Measures.
10. Spherical geometry Cambridge University Press 1  G K Powers 2013.
MOTIONS OF SKY. Goals To identify the different parts of the celestial sphere model To understand how to express the location of objects in the sky To.
1 Homework Q & A Junior Navigation Chapter 5 Celestial Coordinates.
Module 3 – Naval Skills Chapter 3 – Time and Navigation Section 2 – Kinds of Time Unit 4 - Marine Navigation.
EXTRATERRESTRIAL RADIATION  Two sources of variation in extraterrestrial radiation must be considered. The first is the variation in the radiation emitted.
How are latitude and longitude used for navigation?
GREENWHICH MARIDIAN.
Locating Positions on Earth
Time Zones.
Latitude and Longitude
FACTS ABOUT THE EARTH, THE SUN AND TELLING TIME
-Time is based on longitude lines.
Announcements Dark Sky night Saturday night is looking iffy. Check before heading out to see if it is cancelled. Homework: Chapter.
Aim: How do we use time zones to determine longitude?
How Do We Use Earth’s Motion to Determine the Length of a Day?
Julian Date/Time. The basis for all calculations
AIM: How is Longitude related to Time Zones?
Time Vocabulary: Time difference hour time zones elapsed
Time Vocabulary: Time difference hour time zones elapsed
Presentation transcript:

LESSON 18: Time Learning ObjectivesLearning Objectives –Comprehend the longitude/time relationship, time conversion, zone time determination, and motions of the sun as the basis of time.

Apparent Solar Time and Mean Solar Time Apparent solar time - reckoned with respect to the passage or the observable sun (the apparent sun).Apparent solar time - reckoned with respect to the passage or the observable sun (the apparent sun). Mean solar time - uses a hypothetical mean sun, whose hour circle moves at a constant rate along the celestial equator.Mean solar time - uses a hypothetical mean sun, whose hour circle moves at a constant rate along the celestial equator. The mean sun moves at the average rate of motion of the apparent sun.The mean sun moves at the average rate of motion of the apparent sun. –In 24 hrs, it moves through 360 deg of arc over the circumference of the earth, or through 15 deg of arc every hour, or through 15’ of arc every minute.

The Equation of Time Found in the bottom right hand corner of each daily page of the Nautical Almanac. The difference between the mean and apparent times is called the Equation of Time. It changes slightly from day to day.

Local Mean Time and Arc to Time Conversions Local Mean Time - time referenced to the observer’s meridian; also called LMT.Local Mean Time - time referenced to the observer’s meridian; also called LMT. –This time is in contrast to GMT (Greenwich Mean Time), time referenced to the Greenwich meridian; and to ZT (zone time), time referenced to the central meridian of the various time zones. Based on the relationship of the mean sun with the observer’s meridian. LMT differs from ZT by the amount of time required for the mean sun to traverse the difference in longitude between the observer’s meridian and the standard (central) meridian of the time zone.Based on the relationship of the mean sun with the observer’s meridian. LMT differs from ZT by the amount of time required for the mean sun to traverse the difference in longitude between the observer’s meridian and the standard (central) meridian of the time zone.

Local Mean Time and Arc to Time Conversions Since the mean sun moves through 15 deg of arc every hour, or through 15’ of arc every minute, these differences in longitude can be directly converted into differences in time.Since the mean sun moves through 15 deg of arc every hour, or through 15’ of arc every minute, these differences in longitude can be directly converted into differences in time. The “Conversion of Arc to Time” table in the Nautical Almanac aids in this calculation.The “Conversion of Arc to Time” table in the Nautical Almanac aids in this calculation. –Just remember that any location east of another has a later time, and any location to the west has an earlier time.

Arc-to-Time Conversion

LMT of Apparent Noon

Use arc-to-time conversion methodUse arc-to-time conversion method Zone Time of Noon = Local Apparent Noon (LAN)