Today. 03 Geodesy. Sphericity. Columbus. Eratosthenes. Pythagoras GEOG 101 8/16/16. Instructor: Pesses 1

Size: px
Start display at page:

Download "Today. 03 Geodesy. Sphericity. Columbus. Eratosthenes. Pythagoras GEOG 101 8/16/16. Instructor: Pesses 1"

Transcription

1 Today 03 Geodesy Part I Introducing Geography Geography 101 Physical Geography: Earth s Surface Landscapes M. Pesses, Antelope Valley College Geodesy Land Division Geodesy ô Science dealing with the measurement of the shape of & locations on the Earth Sphericity In 1492 Not the first to think Earth was round ô Accepted idea around AD 100 Columbus What shape is the Earth? Pythagoras Eratosthenes Greek Mathematician/ Philosopher ô BC ô Observed Earth was round ô But how? Librarian at Alexandria, Egypt ô 247 BC Instructor: Pesses 1

2 Syene, Egypt ô On Summer Solstice, sun cast no shadows ô Directly overhead 23.5 North So what? Eratosthenes knew that the sun was not directly overhead in Alexandria on that same day ô Proof that the Earth was round Measuring the Earth Measuring the Earth Eratosthenes found that the sun s rays were coming in about 7.2 off of 90 ô Roughly 1/50 of a 360 circle Measured the distance & multiplied by 50 ô His circumference, approx. 24,662 miles ô Today measured at 24,901 miles Sphericity But is the Earth REALLY round? Instructor: Pesses 2

3 Newton If the Earth is spinning on an axis ô Equator moves faster than poles Oblate spheroid ô Centrifugal force at the Equator Speed of Earth s Rotation Latitude Speed (kmph) Speed (mph) Nearest geographic point North Pole Seward, Alaska; St. Petersburg, Russia Chibougamau, Québec; Kiev, Ukraine Beijing, China; Valdivia, Chile Pôrto Alegre, Brazil; New Orleans, Louisiana Quito, Ecuador; Pontianak, Indonesia But Is it really an oblate spheroid? Geoid Geoid Literally means earth shaped An average sea-level assuming a fluid Earth with Earth s gravitational pull The rock of the Earth is bumpy Sea level is not the same everywhere ô Mean Sea Level (MSL) is seeking equilibrium with gravity Instructor: Pesses 3

4 GEOG 101 8/16/16 GPS Global Positioning System (GPS) cm accuracy Cardinal Direction Getting around our geoid Wind Direction The Compass Location How does one know where he or she is on a sphere? Instructor: Pesses Points north Crucial to human development Longitude & Latitude An imaginary grid that covers the surface of the Earth 4

5 DMS Reported in Degrees, Minutes, Seconds (DMS) & the direction. ô 360 (degrees) around a sphere ô 60 (minutes) in a degree ó 1/60 ô 60 (seconds) in a minute (though we won t use these in this class ) Lines of Latitude Also called parallels Gives us North and South coordinates Lines run from East to West ô Example: N Lines of Latitude Latitude is the measured angle north or south of the Equator Finding Your Latitude Finding Your Latitude Angle measured between the horizon & solar noon Corrected with celestial charts & the analemma We can use other stars too Polaris ô The North Star directly over the North Pole ô Use the Southern Cross in the Southern Hemisphere Instructor: Pesses 5

6 Finding Your Latitude Lines of Longitude Measure the angle between Polaris & the horizon to find your latitude The Earth rotates on its axis; we use this to map out longitude. Lines of Longitude Lines of Longitude Meridians Great circles ô The shortest route between 2 points on a sphere. Origin Point Origin Point The Prime Meridian runs through Greenwich, England Given the numerical value of 0. Other meridians numbered in degrees, to the east & the west from Greenwich. ô The direction is important Instructor: Pesses 6

7 Finding Longitude It s one thing to look up longitude on a globe, but what about finding it on a ship in the ocean? Finding Longitude Determined by measuring the difference between the time at the prime meridian & solar noon at the meridian in question Rotation Rotation The sun moves through the sky every 24 hours, travels 360 (360/24 = 15 per hour) Earth rotates to the East If your time is later than Greenwich s, you have travelled East If earlier, travelled West Finding Longitude Finding Longitude So 3pm in Greenwich & noon at your location means you are at 45 West So 3pm in Greenwich & noon at your location means you are at 45 West ô 3 hours x 15 degrees = 45 degrees traveled Instructor: Pesses 7

8 Finding Longitude Harrison s Chronometer So 3pm in Greenwich & noon at your location means you are at 45 West ô 3 hours x 15 degrees = 45 degrees traveled But can you see the problem with this technique? The Graticule Coordinate System This system of latitude and longitude is referred to as the graticule Parallels & meridians cross at right angles (90 ) A grid used to organize a map or globe for the purposes of determining location and/or distance. GPS PLSS Global Positioning System (G.P.S.) Has made finding your location much easier Public Land Survey System (P.L.S.S.) ô Developed by Thomas Jefferson to facilitate westward expansion of the US ô Often referred to as Township and Range Instructor: Pesses 8

9 GEOG 101 8/16/16 Baselines & Meridians These give your origin point ô ô ô 6 mile grids are built off of the meridian and base line Townships (or Tiers) are counted north-south Range are counted east-west Sections Each township and range square is divided into 36 sections. Each section is therefore 1 square mile or 640 acres Influence on the Landscape Best seen from the air Instructor: Pesses Other land divisions French long lots in Louisiana 9

10 Next Time How maps work ô Projections ô Scale Instructor: Pesses 10

The Earth Really is Flat! The Globe and Coordinate Systems. Long History of Mapping. The Earth is Flat. Long History of Mapping

The Earth Really is Flat! The Globe and Coordinate Systems. Long History of Mapping. The Earth is Flat. Long History of Mapping The Earth Really is Flat! The Globe and Coordinate Systems Intro to Mapping & GIS The Earth is Flat Day to day, we live life in a flat world sun rises in east, sets in west sky is above, ground is below

More information

Solar Angles and Latitude

Solar Angles and Latitude Solar Angles and Latitude Objectives The student will understand that the sun is not directly overhead at noon in most latitudes. The student will research and discover the latitude ir classroom and calculate

More information

Earth In Space Chapter 3

Earth In Space Chapter 3 Earth In Space Chapter 3 Shape of the Earth Ancient Greeks Earth casts a circular shadow on the moon during a lunar eclipse Shape of the Earth Ancient Greeks Ships were observed to disappear below the

More information

Measuring the Earth Using a GPS M. Scott Wilkerson & M. Beth Wilkerson, DePauw University, May 10, 2007

Measuring the Earth Using a GPS M. Scott Wilkerson & M. Beth Wilkerson, DePauw University, May 10, 2007 Measuring the Earth Using a GPS M. Scott Wilkerson & M. Beth Wilkerson, DePauw University, May 10, 2007 Modified from: Kerski, J.J., 2007, Measuring the Earth s Circumference with GPS, Copyright ESRI,

More information

Celestial Observations

Celestial Observations Celestial Observations Earth experiences two basic motions: Rotation West-to-East spinning of Earth on its axis (v rot = 1770 km/hr) (v rot Revolution orbit of Earth around the Sun (v orb = 108,000 km/hr)

More information

The Globe Latitudes and Longitudes

The Globe Latitudes and Longitudes INDIAN SCHOOL MUSCAT MIDDLE SECTION DEPARTMENT OF SOCIAL SCIENCE The Globe Latitudes and Longitudes NAME: CLASS VI SEC: ROLL NO: DATE:.04.2015 I NAME THE FOLLOWING: 1. A small spherical model of the Earth:

More information

Earth Coordinates & Grid Coordinate Systems

Earth Coordinates & Grid Coordinate Systems Earth Coordinates & Grid Coordinate Systems How do we model the earth? Datums Datums mathematically describe the surface of the Earth. Accounts for mean sea level, topography, and gravity models. Projections

More information

Earth-Sun Relationships. The Reasons for the Seasons

Earth-Sun Relationships. The Reasons for the Seasons Earth-Sun Relationships The Reasons for the Seasons Solar Radiation The earth intercepts less than one two-billionth of the energy given off by the sun. However, the radiation is sufficient to provide

More information

Newton s Law of Gravity

Newton s Law of Gravity Gravitational Potential Energy On Earth, depends on: object s mass (m) strength of gravity (g) distance object could potentially fall Gravitational Potential Energy In space, an object or gas cloud has

More information

Tropical Horticulture: Lecture 2

Tropical Horticulture: Lecture 2 Lecture 2 Theory of the Tropics Earth & Solar Geometry, Celestial Mechanics The geometrical relationship between the earth and sun is responsible for the earth s climates. The two principal movements of

More information

Pre and post-visit activities - Navigating by the stars

Pre and post-visit activities - Navigating by the stars Pre and post-visit activities - Navigating by the stars Vocabulary List Adult Education at Scienceworks Pre-visit Activity 1: What is longitude and latitude? Activity 2: Using the Southern Cross to find

More information

Geography I Pre Test #1

Geography I Pre Test #1 Geography I Pre Test #1 1. The sun is a star in the galaxy. a) Orion b) Milky Way c) Proxima Centauri d) Alpha Centauri e) Betelgeuse 2. The response to earth's rotation is a) an equatorial bulge b) polar

More information

FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES

FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES FIRST GRADE 1 WEEK LESSON PLANS AND ACTIVITIES UNIVERSE CYCLE OVERVIEW OF FIRST GRADE UNIVERSE WEEK 1. PRE: Describing the Universe. LAB: Comparing and contrasting bodies that reflect light. POST: Exploring

More information

Basic Coordinates & Seasons Student Guide

Basic Coordinates & Seasons Student Guide Name: Basic Coordinates & Seasons Student Guide There are three main sections to this module: terrestrial coordinates, celestial equatorial coordinates, and understanding how the ecliptic is related to

More information

The Celestial Sphere. Questions for Today. The Celestial Sphere 1/18/10

The Celestial Sphere. Questions for Today. The Celestial Sphere 1/18/10 Lecture 3: Constellations and the Distances to the Stars Astro 2010 Prof. Tom Megeath Questions for Today How do the stars move in the sky? What causes the phases of the moon? What causes the seasons?

More information

Stellarium a valuable resource for teaching astronomy in the classroom and beyond

Stellarium a valuable resource for teaching astronomy in the classroom and beyond Stellarium 1 Stellarium a valuable resource for teaching astronomy in the classroom and beyond Stephen Hughes Department of Physical and Chemical Sciences, Queensland University of Technology, Gardens

More information

The following words and their definitions should be addressed before completion of the reading:

The following words and their definitions should be addressed before completion of the reading: Seasons Vocabulary: The following words and their definitions should be addressed before completion of the reading: sphere any round object that has a surface that is the same distance from its center

More information

Use WITH Investigation 4, Part 2, Step 2

Use WITH Investigation 4, Part 2, Step 2 INVESTIGATION 4 : The Sundial Project Use WITH Investigation 4, Part 2, Step 2 EALR 4: Earth and Space Science Big Idea: Earth in Space (ES1) Projects: Tether Ball Pole Sundial Globe and a Light Indoors

More information

compass Encyclopedic Entry

compass Encyclopedic Entry This website would like to remind you: Your browser (Apple Safari 7) is out of date. Update your browser for more security, comfort and the best experience on this site. Encyclopedic Entry compass For

More information

Coordinate Systems. Orbits and Rotation

Coordinate Systems. Orbits and Rotation Coordinate Systems Orbits and Rotation Earth orbit. The earth s orbit around the sun is nearly circular but not quite. It s actually an ellipse whose average distance from the sun is one AU (150 million

More information

Navigation: Latitude and Longitude

Navigation: Latitude and Longitude Sextants and Chronometers Help Sailors Find Their Position at Sea Latitude lines run horizontally across the globe and are used to measure distances north and south of the equator. Sailors used a sextant

More information

Shadows, Angles, and the Seasons

Shadows, Angles, and the Seasons Shadows, Angles, and the Seasons If it's cold in winter, why is Earth closer to the Sun? This activity shows the relationship between Earth-Sun positions and the seasons. From The WSU Fairmount Center

More information

Reasons for Seasons. Question: TRUE OR FALSE. Question: TRUE OR FALSE? What causes the seasons? What causes the seasons?

Reasons for Seasons. Question: TRUE OR FALSE. Question: TRUE OR FALSE? What causes the seasons? What causes the seasons? Reasons for Seasons Question: TRUE OR FALSE? Earth is closer to the Sun in summer and farther from the Sun in winter. Question: TRUE OR FALSE? Earth is closer to the Sun in summer and farther from the

More information

6. The greatest atmospheric pressure occurs in the 1) troposphere 3) mesosphere 2) stratosphere 4) thermosphere

6. The greatest atmospheric pressure occurs in the 1) troposphere 3) mesosphere 2) stratosphere 4) thermosphere 1. The best evidence of the Earth's nearly spherical shape is obtained through telescopic observations of other planets photographs of the Earth from an orbiting satellite observations of the Sun's altitude

More information

Sun Earth Relationships

Sun Earth Relationships 1 ESCI-61 Introduction to Photovoltaic Technology Sun Earth Relationships Ridha Hamidi, Ph.D. Spring (sun aims directly at equator) Winter (northern hemisphere tilts away from sun) 23.5 2 Solar radiation

More information

CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS

CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS INTRODUCTION CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS This is a scientific presentation to provide you with knowledge you can use to understand the sky above in relation to the earth. Before

More information

An Introduction to Coordinate Systems in South Africa

An Introduction to Coordinate Systems in South Africa An Introduction to Coordinate Systems in South Africa Centuries ago people believed that the earth was flat and notwithstanding that if this had been true it would have produced serious problems for mariners

More information

Solar System. 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X?

Solar System. 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X? Solar System 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X? A) Earth B) Sun C) Moon D) Polaris 2. Which object orbits Earth in both the Earth-centered

More information

Motions of Earth, Moon, and Sun

Motions of Earth, Moon, and Sun Motions of Earth, Moon, and Sun Apparent Motions of Celestial Objects An apparent motion is a motion that an object appears to make. Apparent motions can be real or illusions. When you see a person spinning

More information

Seasons on Earth LESSON

Seasons on Earth LESSON LESSON 4 Seasons on Earth On Earth, orange and red autumn leaves stand out against the blue sky. NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION (NOAA) PHOTO LIBRARY/NOAA CENTRAL LIBRARY INTRODUCTION Nearly

More information

EARTH'S MOTIONS. 2. The Coriolis effect is a result of Earth's A tilted axis B orbital shape C revolution D rotation

EARTH'S MOTIONS. 2. The Coriolis effect is a result of Earth's A tilted axis B orbital shape C revolution D rotation EARTH'S MOTIONS 1. Which hot spot location on Earth's surface usually receives the greatest intensity of insolation on June 21? A Iceland B Hawaii C Easter Island D Yellowstone 2. The Coriolis effect is

More information

1-2. What is the name given to the path of the Sun as seen from Earth? a.) Equinox b.) Celestial equator c.) Solstice d.

1-2. What is the name given to the path of the Sun as seen from Earth? a.) Equinox b.) Celestial equator c.) Solstice d. Chapter 1 1-1. How long does it take the Earth to orbit the Sun? a.) one sidereal day b.) one month c.) one year X d.) one hour 1-2. What is the name given to the path of the Sun as seen from Earth? a.)

More information

CELESTIAL MOTIONS. In Charlottesville we see Polaris 38 0 above the Northern horizon. Earth. Starry Vault

CELESTIAL MOTIONS. In Charlottesville we see Polaris 38 0 above the Northern horizon. Earth. Starry Vault CELESTIAL MOTIONS Stars appear to move counterclockwise on the surface of a huge sphere the Starry Vault, in their daily motions about Earth Polaris remains stationary. In Charlottesville we see Polaris

More information

Lab Activity on the Causes of the Seasons

Lab Activity on the Causes of the Seasons Lab Activity on the Causes of the Seasons 2002 Ann Bykerk-Kauffman, Dept. of Geological and Environmental Sciences, California State University, Chico * Objectives When you have completed this lab you

More information

Lines on Maps and Globes. Cross Curricular Writing Activity Social Studies Grade 4

Lines on Maps and Globes. Cross Curricular Writing Activity Social Studies Grade 4 Lines on Maps and Globes Cross Curricular Writing Activity Social Studies Grade 4 Fourth Grade Social Studies Standard Map: Chart/Globe The learner will be able to use maps, charts, graphs, and globes

More information

Noon Sun Angle = 90 Zenith Angle

Noon Sun Angle = 90 Zenith Angle Noon Sun Angle Worksheet Name Name Date Subsolar Point (Latitude where the sun is overhead at noon) Equinox March 22 nd 0 o Equinox September 22 nd 0 o Solstice June 22 nd 23.5 N Solstice December 22 nd

More information

Today. Solstices & Equinoxes Precession Phases of the Moon Eclipses. Ancient Astronomy. Lunar, Solar FIRST HOMEWORK DUE NEXT TIME

Today. Solstices & Equinoxes Precession Phases of the Moon Eclipses. Ancient Astronomy. Lunar, Solar FIRST HOMEWORK DUE NEXT TIME Today Solstices & Equinoxes Precession Phases of the Moon Eclipses Lunar, Solar Ancient Astronomy FIRST HOMEWORK DUE NEXT TIME The Reason for Seasons Hypothesis check: How would seasons in the northern

More information

SECOND GRADE 1 WEEK LESSON PLANS AND ACTIVITIES

SECOND GRADE 1 WEEK LESSON PLANS AND ACTIVITIES SECOND GRADE 1 WEEK LESSON PLANS AND ACTIVITIES UNIVERSE CYCLE OVERVIEW OF SECOND GRADE UNIVERSE WEEK 1. PRE: Discovering stars. LAB: Analyzing the geometric pattern of constellations. POST: Exploring

More information

UTM Zones for the US UTM UTM. Uniform strips Scalable coordinates

UTM Zones for the US UTM UTM. Uniform strips Scalable coordinates UTM UTM Uniform strips Scalable coordinates Globally consistent, most popular projection/coordinate system for regional to global scale geospatial data (i.e. satellite images global scale datasets USGS/EDC)

More information

Orientation to the Sky: Apparent Motions

Orientation to the Sky: Apparent Motions Chapter 2 Orientation to the Sky: Apparent Motions 2.1 Purpose The main goal of this lab is for you to gain an understanding of how the sky changes during the night and over the course of a year. We will

More information

Measuring Your Latitude from the Angle of the Sun at Noon

Measuring Your Latitude from the Angle of the Sun at Noon Measuring Your Latitude from the Angle of the Sun at Noon Background: You can measure your latitude in earth's northern hemisphere by finding out the altitude of the celestial equator from the southern

More information

1. In the diagram below, the direct rays of the Sun are striking the Earth's surface at 23 º N. What is the date shown in the diagram?

1. In the diagram below, the direct rays of the Sun are striking the Earth's surface at 23 º N. What is the date shown in the diagram? 1. In the diagram below, the direct rays of the Sun are striking the Earth's surface at 23 º N. What is the date shown in the diagram? 5. During how many days of a calendar year is the Sun directly overhead

More information

EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1

EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1 Instructor: L. M. Khandro EDMONDS COMMUNITY COLLEGE ASTRONOMY 100 Winter Quarter 2007 Sample Test # 1 1. An arc second is a measure of a. time interval between oscillations of a standard clock b. time

More information

Periods of Western Astronomy. Chapter 1. Prehistoric Astronomy. Prehistoric Astronomy. The Celestial Sphere. Stonehenge. History of Astronomy

Periods of Western Astronomy. Chapter 1. Prehistoric Astronomy. Prehistoric Astronomy. The Celestial Sphere. Stonehenge. History of Astronomy Periods of Western Astronomy Chapter 1 History of Astronomy Western astronomy divides into 4 periods Prehistoric (before 500 B.C.) Cyclical motions of Sun, Moon and stars observed Keeping time and determining

More information

Today FIRST HOMEWORK DUE NEXT TIME. Seasons/Precession Recap. Phases of the Moon. Eclipses. Lunar, Solar. Ancient Astronomy

Today FIRST HOMEWORK DUE NEXT TIME. Seasons/Precession Recap. Phases of the Moon. Eclipses. Lunar, Solar. Ancient Astronomy Today FIRST HOMEWORK DUE NEXT TIME Seasons/Precession Recap Phases of the Moon Eclipses Lunar, Solar Ancient Astronomy How do we mark the progression of the seasons? We define four special points: summer

More information

Stage 4. Geography. Blackline Masters. By Karen Devine

Stage 4. Geography. Blackline Masters. By Karen Devine 1 Devine Educational Consultancy Services Stage 4 Geography Blackline Masters By Karen Devine Updated January 2010 2 This book is intended for the exclusive use in NSW Secondary Schools. It is meant to

More information

Plotting a Course Through History A Navigation History Timeline

Plotting a Course Through History A Navigation History Timeline Mariners know how to navigate from here to there and back again. But we seldom stop to wonder who figured out how to determine position in the middle of an ocean, who developed the concept of latitude

More information

Where on Earth are the daily solar altitudes higher and lower than Endicott?

Where on Earth are the daily solar altitudes higher and lower than Endicott? Where on Earth are the daily solar altitudes higher and lower than Endicott? In your notebooks, write RELATIONSHIPS between variables we tested CAUSE FIRST EFFECT SECOND EVIDENCE As you increase the time

More information

Lecture 2. Map Projections and GIS Coordinate Systems. Tomislav Sapic GIS Technologist Faculty of Natural Resources Management Lakehead University

Lecture 2. Map Projections and GIS Coordinate Systems. Tomislav Sapic GIS Technologist Faculty of Natural Resources Management Lakehead University Lecture 2 Map Projections and GIS Coordinate Systems Tomislav Sapic GIS Technologist Faculty of Natural Resources Management Lakehead University Map Projections Map projections are mathematical formulas

More information

Essential Question. Enduring Understanding

Essential Question. Enduring Understanding Earth In Space Unit Diagnostic Assessment: Students complete a questionnaire answering questions about their ideas concerning a day, year, the seasons and moon phases: My Ideas About A Day, Year, Seasons

More information

ASTRONOMY 161. Introduction to Solar System Astronomy

ASTRONOMY 161. Introduction to Solar System Astronomy ASTRONOMY 161 Introduction to Solar System Astronomy Seasons & Calendars Monday, January 8 Season & Calendars: Key Concepts (1) The cause of the seasons is the tilt of the Earth s rotation axis relative

More information

The Four Seasons. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. The Moon s Phases

The Four Seasons. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. The Moon s Phases The Four Seasons A Warm Up Exercise What fraction of the Moon s surface is illuminated by the Sun (except during a lunar eclipse)? a) Between zero and one-half b) The whole surface c) Always half d) Depends

More information

Study Guide: Sun, Earth and Moon Relationship Assessment

Study Guide: Sun, Earth and Moon Relationship Assessment I can 1. Define rotation, revolution, solstice and equinox. *Rotation and Revolution Review Worksheet 2. Describe why we experience days and years due to the rotation and r evolution of the Earth around

More information

Name Period 4 th Six Weeks Notes 2015 Weather

Name Period 4 th Six Weeks Notes 2015 Weather Name Period 4 th Six Weeks Notes 2015 Weather Radiation Convection Currents Winds Jet Streams Energy from the Sun reaches Earth as electromagnetic waves This energy fuels all life on Earth including the

More information

4 The Rhumb Line and the Great Circle in Navigation

4 The Rhumb Line and the Great Circle in Navigation 4 The Rhumb Line and the Great Circle in Navigation 4.1 Details on Great Circles In fig. GN 4.1 two Great Circle/Rhumb Line cases are shown, one in each hemisphere. In each case the shorter distance between

More information

World Map Lesson 4 - The Global Grid System - Grade 6+

World Map Lesson 4 - The Global Grid System - Grade 6+ World Map Lesson 4 - The Global Grid System - Grade 6+ Activity Goal To use the global grid system of latitude and longitude to find specific locations on a world map. Materials Needed: A pencil, a ruler,

More information

How do you find a place on a globe? How do you look up a place based on latitude and longitude?

How do you find a place on a globe? How do you look up a place based on latitude and longitude? Why are globes tilted? Most Replogle globes are made to tilt at an angle of 23.5º to match the actual tilt of the earth in relationship to our sun. Incidentally, it is this tilting of the earth relative

More information

DETERMINING SOLAR ALTITUDE USING THE GNOMON. How does the altitude change during the day or from day to day?

DETERMINING SOLAR ALTITUDE USING THE GNOMON. How does the altitude change during the day or from day to day? Name Partner(s) Section Date DETERMINING SOLAR ALTITUDE USING THE GNOMON Does the Sun ever occur directly overhead in Maryland? If it does, how would you determine or know it was directly overhead? How

More information

Relationship Between the Earth, Moon and Sun

Relationship Between the Earth, Moon and Sun Relationship Between the Earth, Moon and Sun Rotation A body turning on its axis The Earth rotates once every 24 hours in a counterclockwise direction. Revolution A body traveling around another The Earth

More information

Geometry and Geography

Geometry and Geography Geometry and Geography Tom Davis tomrdavis@earthlink.net http://www.geometer.org/mathcircles March 12, 2011 1 Pedagogical Advice I have been leading mathematical circles using this topic for many years,

More information

Activity 10 - Universal Time

Activity 10 - Universal Time Activity 10 - Universal Time Teacher s Guide Scientists use the Universal Time reference to talk about data that is taken around the globe. Universal Time is the time kept in the time zone centered on

More information

Astromechanics. 1 solar day = 1.002737909350795 sidereal days

Astromechanics. 1 solar day = 1.002737909350795 sidereal days Astromechanics 13. Time Considerations- Local Sidereal Time The time that is used by most people is that called the mean solar time. It is based on the idea that if the Earth revolved around the Sun at

More information

ASTR 1030 Astronomy Lab 65 Celestial Motions CELESTIAL MOTIONS

ASTR 1030 Astronomy Lab 65 Celestial Motions CELESTIAL MOTIONS ASTR 1030 Astronomy Lab 65 Celestial Motions CELESTIAL MOTIONS SYNOPSIS: The objective of this lab is to become familiar with the apparent motions of the Sun, Moon, and stars in the Boulder sky. EQUIPMENT:

More information

Lines of Latitude and Longitude

Lines of Latitude and Longitude ED 5661 Mathematics & Navigation Teacher Institute Keith Johnson Lesson Plan Lines of Latitude and Longitude Lesson Overview: This lesson plan will introduce students to latitude and longitude along with

More information

Answers for the Study Guide: Sun, Earth and Moon Relationship Test

Answers for the Study Guide: Sun, Earth and Moon Relationship Test Answers for the Study Guide: Sun, Earth and Moon Relationship Test 1) It takes one day for the Earth to make one complete on its axis. a. Rotation 2) It takes one year for the Earth to make one around

More information

Full credit for this chapter to Prof. Leonard Bachman of the University of Houston

Full credit for this chapter to Prof. Leonard Bachman of the University of Houston Chapter 6: SOLAR GEOMETRY Full credit for this chapter to Prof. Leonard Bachman of the University of Houston SOLAR GEOMETRY AS A DETERMINING FACTOR OF HEAT GAIN, SHADING AND THE POTENTIAL OF DAYLIGHT PENETRATION...

More information

Celestial Sphere. Celestial Coordinates. Lecture 3: Motions of the Sun and Moon. ecliptic (path of Sun) ecliptic (path of Sun)

Celestial Sphere. Celestial Coordinates. Lecture 3: Motions of the Sun and Moon. ecliptic (path of Sun) ecliptic (path of Sun) Lecture 3: Motions of the and Moon ecliptic (path of ) ecliptic (path of ) The 23.5 degree tilt of Earth s spin axis relative to its orbital axis around the causes the seasons Celestial Sphere Celestial

More information

Moon Phases & Eclipses Notes

Moon Phases & Eclipses Notes Moon Phases & Eclipses Notes Melka 2014-2015 The Moon The Moon is Earth s one natural satellite. Due to its smaller size and slower speed of rotation, the Moon s gravity is 1/6 of the Earth s gravitational

More information

Tides and Water Levels

Tides and Water Levels Tides and Water Levels What are Tides? Tides are one of the most reliable phenomena in the world. As the sun rises in the east and the stars come out at night, we are confident that the ocean waters will

More information

Sunlight and its Properties. EE 495/695 Y. Baghzouz

Sunlight and its Properties. EE 495/695 Y. Baghzouz Sunlight and its Properties EE 495/695 Y. Baghzouz The sun is a hot sphere of gas whose internal temperatures reach over 20 million deg. K. Nuclear fusion reaction at the sun's core converts hydrogen to

More information

Shadows and Solar Zenith

Shadows and Solar Zenith Shadows and Solar Zenith Name Lab Partner Section Introduction: The solar zenith angle is defined to be the angle between the sun and a line that goes straight up (to the zenith) In reality the sun is

More information

Gravitational potential

Gravitational potential Gravitational potential Let s assume: A particle of unit mass moving freely A body of mass M The particle is attracted by M and moves toward it by a small quantity dr. This displacement is the result of

More information

CHAPTER 8 - LAND DESCRIPTIONS

CHAPTER 8 - LAND DESCRIPTIONS CHAPTER 8 - LAND DESCRIPTIONS Notes: While the location of land is commonly referred to by street number and city, it is necessary to use the legal description in the preparation of those instruments relating

More information

Searching Land Records thru the BLM General Land Office Records.

Searching Land Records thru the BLM General Land Office Records. Searching Land Records thru the BLM General Land Office Records. Land Records can be an exciting addition to your family history search. The United States Government transferred ownership of land to millions

More information

The Analemma for Latitudinally-Challenged People

The Analemma for Latitudinally-Challenged People The Analemma for Latitudinally-Challenged People Teo Shin Yeow An academic exercise presented in partial fulfillment for the degree of Bachelor of Science with Honours in Mathematics Supervisor : Associate

More information

The Orbit TelleriumThe Orbit TelleriumThe Orbit Tellerium

The Orbit TelleriumThe Orbit TelleriumThe Orbit Tellerium The Orbit TelleriumThe Orbit TelleriumThe Orbit Tellerium 16 Appendix 4 Moon Chart: For each day draw the shape of the Moon, record the time and mark the position of the Moon in the sky in relation to

More information

The ecliptic - Earth s orbital plane

The ecliptic - Earth s orbital plane The ecliptic - Earth s orbital plane The line of nodes descending node The Moon s orbital plane Moon s orbit inclination 5.45º ascending node celestial declination Zero longitude in the ecliptic The orbit

More information

Exploring Solar Energy Variations on Earth: Changes in the Length of Day and Solar Insolation Through the Year

Exploring Solar Energy Variations on Earth: Changes in the Length of Day and Solar Insolation Through the Year Exploring Solar Energy Variations on Earth: Changes in the Length of Day and Solar Insolation Through the Year Purpose To help students understand how solar radiation varies (duration and intensity) during

More information

The Reasons for the Seasons

The Reasons for the Seasons The Reasons for the Seasons (The Active Learning Approach) Materials: 4 Globes, One light on stand with soft white bulb, 4 flashlights, Four sets of "Seasons" Cards, Four laminated black cards with 1 inch

More information

Measuring the Diameter of the Sun

Measuring the Diameter of the Sun Chapter 24 Studying the Sun Investigation 24 Measuring the Diameter of the Sun Introduction The sun is approximately 150,000,000 km from Earth. To understand how far away this is, consider the fact that

More information

Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti

Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti INSTRUCTIONS: Please, use the `bubble sheet and a pencil # 2 to answer the exam questions, by marking

More information

The Size & Shape of the Galaxy

The Size & Shape of the Galaxy name The Size & Shape of the Galaxy The whole lab consists of plotting two graphs. What s the catch? Aha visualizing and understanding what you have plotted of course! Form the Earth Science Picture of

More information

The Map Grid of Australia 1994 A Simplified Computational Manual

The Map Grid of Australia 1994 A Simplified Computational Manual The Map Grid of Australia 1994 A Simplified Computational Manual The Map Grid of Australia 1994 A Simplified Computational Manual 'What's the good of Mercator's North Poles and Equators, Tropics, Zones

More information

Location and Distance on Earth (Chapter 22 part 1)

Location and Distance on Earth (Chapter 22 part 1) GEOLOGY 306 Laboratory Instructor: TERRY J. BOROUGHS NAME: Location and Distance on Earth (Chapter 22 part 1) For this assignment you will require: a calculator, protractor, and a metric ruler, and an

More information

Seasonal & Daily Temperatures. Seasons & Sun's Distance. Solstice & Equinox. Seasons & Solar Intensity

Seasonal & Daily Temperatures. Seasons & Sun's Distance. Solstice & Equinox. Seasons & Solar Intensity Seasonal & Daily Temperatures Seasons & Sun's Distance The role of Earth's tilt, revolution, & rotation in causing spatial, seasonal, & daily temperature variations Please read Chapter 3 in Ahrens Figure

More information

Public Land Survey System - Definition

Public Land Survey System - Definition Public Land Survey System - Definition The Public Land Survey System (PLSS) is a method used in the United States to locate and identify land, particularly for titles and deeds of farm or rural land. The

More information

A guide to coordinate systems in Great Britain

A guide to coordinate systems in Great Britain A guide to coordinate systems in Great Britain An introduction to mapping coordinate systems and the use of GPS datasets with Ordnance Survey mapping D00659 v2.3 Mar 2015 Crown copyright Page 1 of 43 Contents

More information

USING MAPS AND GLOBES

USING MAPS AND GLOBES USING MAPS AND GLOBES Grade Level or Special Area: 4 th Grade Written by: Krystal Kroeker, Colorado Springs Charter Academy, Colorado Springs, CO Length of Unit: Five lessons (approximately one week (five

More information

Motions of Earth LEARNING GOALS

Motions of Earth LEARNING GOALS 2 Patterns in the Sky Motions of Earth The stars first found a special place in legend and mythology as the realm of gods and goddesses, holding sway over the lives of humankind. From these legends and

More information

User s Guide MARK 15 #026 MARK 25 #025 INDEX SHADES INDEX MIRROR. HORIZON MIRROR (Beam Converger on Mark 25 only) ADJUSTMENT SCREW HORIZON SHADES

User s Guide MARK 15 #026 MARK 25 #025 INDEX SHADES INDEX MIRROR. HORIZON MIRROR (Beam Converger on Mark 25 only) ADJUSTMENT SCREW HORIZON SHADES User s Guide INDEX SHADES INDEX MIRROR HORIZON MIRROR (Beam Converger on Mark 25 only) ADJUSTMENT SCREW HORIZON SHADES TELESCOPE MICROMETER DRUM QUICK RELEASE LEVERS LED ILLUMINATION (Mark 25 only) INDEX

More information

OBJECTIVES. Identify the means by which latitude and longitude were created and the science upon which they are based.

OBJECTIVES. Identify the means by which latitude and longitude were created and the science upon which they are based. Name: Key OBJECTIVES Correctly define: isolines, gradient, topographic map, contour interval, hachured lines, profile, latitude, longitude, hydrosphere, lithosphere, atmosphere, elevation, model EARTH

More information

Activity 3: Observing the Moon

Activity 3: Observing the Moon Activity 3: Observing the Moon Print Name: Signature: 1.) KEY. 2.). 3.). 4.). Activity: Since the dawn of time, our closest neighbor the moon has fascinated humans. In this activity we will explore the

More information

Plotting Earthquake Epicenters an activity for seismic discovery

Plotting Earthquake Epicenters an activity for seismic discovery Plotting Earthquake Epicenters an activity for seismic discovery Tammy K Bravo Anne M Ortiz Plotting Activity adapted from: Larry Braile and Sheryl Braile Department of Earth and Atmospheric Sciences Purdue

More information

UTM: Universal Transverse Mercator Coordinate System

UTM: Universal Transverse Mercator Coordinate System Practical Cartographer s Reference #01 UTM: Universal Transverse Mercator Coordinate System 180 174w 168w 162w 156w 150w 144w 138w 132w 126w 120w 114w 108w 102w 96w 90w 84w 78w 72w 66w 60w 54w 48w 42w

More information

Which month has larger and smaller day time?

Which month has larger and smaller day time? ACTIVITY-1 Which month has larger and smaller day time? Problem: Which month has larger and smaller day time? Aim: Finding out which month has larger and smaller duration of day in the Year 2006. Format

More information

Weekend Cabin Retreat Project Site Plans

Weekend Cabin Retreat Project Site Plans Weekend Cabin Retreat Project Site Plans Sacramento City College EDT 300/ENGR 306 EDT 300/ENGR 306 - Site Plans 1 Cabin Project Site Plan/Bubble Diagram - Assignment 1 =10-0 Floor Plan - Assignment 1/4

More information

How To Understand General Relativity

How To Understand General Relativity Chapter S3 Spacetime and Gravity What are the major ideas of special relativity? Spacetime Special relativity showed that space and time are not absolute Instead they are inextricably linked in a four-dimensional

More information

Topographic Maps Practice Questions and Answers Revised October 2007

Topographic Maps Practice Questions and Answers Revised October 2007 Topographic Maps Practice Questions and Answers Revised October 2007 1. In the illustration shown below what navigational features are represented by A, B, and C? Note that A is a critical city in defining

More information

Motion & The Global Positioning System (GPS)

Motion & The Global Positioning System (GPS) Grade Level: K - 8 Subject: Motion Prep Time: < 10 minutes Duration: 30 minutes Objective: To learn how to analyze GPS data in order to track an object and derive its velocity from positions and times.

More information