PHYSICAL GEOGRAPHY. By Brett Lucas

Size: px
Start display at page:

Download "PHYSICAL GEOGRAPHY. By Brett Lucas"

Transcription

1 PHYSICAL GEOGRAPHY By Brett Lucas

2 INTRODUCTION

3 Introduction to Earth Geography as a Field of Learning Geography is from two Greek words, Geo Earth, and Graphien to write. Elements/Branches of Geography Physical & Human or Cultural (see next slide). This class is concerned with Physical Geography.

4 Elements of Geography

5 Introduction to Earth Environmental Spheres (next slide) The Solar System Size and Shape of Earth The Geographic Grid Earth Movements Annual March of the Seasons Telling Time

6 Environmental Spheres Lithosphere Litho, Greek for stone Atmosphere atmo, Greek for air Hydrosphere hydro, Greek for water Biosphere bio, Greek for life L Interacting spheres A B H

7 The Solar System Figure 1-6: Elliptical orbits Pluto is NO longer one of the planets in our solar system as of 2006

8 Size and Shape of Earth 3 rd Rock from the Sun (93 million miles) Size Diameter approx. 8,000 miles (12,800 km) at the equator 5 th largest in diameter

9 Size and Shape of Earth Earth s highest pt: 29,000 ft above sea level. Lowest point: 36,000 ft below sea level More bulgy at the equator: a difference of 0.3%. As a result, it s not a true/perfect sphere (circle), but an Oblate Spheroid, slightly flat on top and bottom.

10 Size and Shape of Earth

11 Size and Shape of Earth

12 Angle of Tilt See imaginary rotation axis. Interesting fact about Earth: The Earth tilts towards the east, at an angle of 23.5 degrees. This is called the inclination of the rotation axis.

13 The Geographic Grid The Combination of Latitude and Longitude Lines

14 Summary (Geographic Grid) Longitude (also called Meridians) Measures distance east and west around the globe, beginning at the Prime Meridian Important longitude lines: Prime Meridian & International Date Line degrees East or West Latitude (also called Parallels) Location on the Earth s surface between the equator and the north or south pole Important latitude line: Equator 0-90 degrees North or South

15 The Geographic Grid The Equator (next slide) the line thru the earth s middle Latitude (run north and south of Equator) Longitude E/W of the Prime/Greenwich Meridian They are used to establish location, for navigation and for telling time. The circle is 360 degrees around; therefore since there are 24 MAJOR longitude lines, each line is 15 degrees, same as ONE HOUR. So 360 degrees = 24 hours.

16 The Equator More interesting facts about Earth: Earth ALWAYS points to Polaris, the North Star Earth moves/ rotates from West to East.

17 Great and Small Circles A great circle is the largest circle than can be drawn on a sphere and they bisect the Earth into 2 equal halves e.g. The Equator The Prime Meridian The Sun s Circle of Illumination (see Blue Beauty NASA slides) Small circles are any other circles that can be drawn.

18 Latitude: Parallels There are 7 important parallels. Measures from 0º to 90º N and S of the equator. Also, the Tropics or tropical areas are hotter, due to the bulge.

19 Longitude: Meridians 0 degrees Longitude passes thru Greenwich, England. And it s then measured East and West Measures from 0º to 180º E & W of the Prime/Greenwich Meridian Established in 1884 at the International Meridian Conference in Washington, D.C. Also used for determining World Time (every 15 degrees is an hr)

20 Regions on Earth Regions on Earth (Latitude bands) Low latitude» 0º 30º N and S (close to Equator) Mid latitude» 30º 60º N and S High latitude» 60º 90º N and S (close to poles) Equatorial» within a few degrees of the equator Tropical» within the tropics between 23.5º N and 23.5º S Subtropical» 25º 30º N and S Polar» within a few degrees of the North and South Pole

21 Earth Movements Rotation on Axis (Daily) One complete rotation is 24 hrs Rotation Direction (West to East), see next slide Rotation Speed, see table and pg Revolution Around Sun (Annual) 365 days, 5hrs, 48 minutes and 46 seconds, simplified to or 365 ¼ days Leap Year

22 Rotation Direction West to East

23 Rotation Speed Note: Always constant speed, only DISTANCE at each location varies!

24 Annual March of Seasons Solstices Summer & Winter; unequal daylight (see next slides) Equinoxes 12 equal hours of daylight; start of Spring and Fall (anywhere between the 20 th and the 23 rd ) Also, see Table 1-7 (pg 22)

25 Solstices

26 Solstices

27 Equinoxes

28 Changes in Daylight

29 Time Zones Accurate calendars have been kept by great civilizations for 1000s of years the Egyptians, Mayas, Aztecs, Chinese, Indians, etc. Pg 23 (Babylon 2,000 B.C.) A.M. & P.M. are Latin words (pg 23). Meri (highest) is the root word for Meritorious. 3 units of natural time the year, month and day. Everything else is man-made (hour, minute, second, etc)

30 Time Zones Standard Time starts at the Greenwich Meridian (GMT) or Zulu. Now called UTC (Universal Time Coordinated). All areas to the east of the Prime Meridian are ahead in time, and all areas to the west are behind in time. Some countries have one time zone, while others have several. Russia has 9. International Date Line (further slides)

31 World Time Zones

32 U.S./Canada Time Zones

33 International Date Line Starts at 180 degrees; this is also where a NEW DAY (new DATE) begins i.e. 12 Midnight. It is the OPPOSITE of the Prime Meridian (zero degrees longitude) in Greenwich i.e. 12 Noon There is a difference of 12 hours between the Prime Meridian (zero degrees) and the International Date Line (180 degrees longitude)

The Earth is a Rotating Sphere

The Earth is a Rotating Sphere The Earth is a Rotating Sphere The Shape of the Earth Earth s Rotation ( and relative movement of the Sun and Moon) The Geographic Grid Map Projections Global Time The Earth s Revolution around the Sun

More information

Chapter 1 Introduction to the Earth

Chapter 1 Introduction to the Earth Chapter 1 Introduction to the Earth What is Geography? The study of the earth as the home of humankind. Greek - Eratosthenes Father of Geography Geo means Earth Graphy means to write Study how things are

More information

UNIT 1: THE PLANET EARTH

UNIT 1: THE PLANET EARTH UNIT 1: THE PLANET EARTH How many planets are there in our Solar System? What is the Equator? Why does life exist in our planet? Does The Earth move? What is a map? 1. Planet Earth TOPICS 2. Movements

More information

Cartesian Coordinates Need two dimensional system 2 number lines perpendicular to each other X-axis is horizontal Y-axis is vertical Position relative

Cartesian Coordinates Need two dimensional system 2 number lines perpendicular to each other X-axis is horizontal Y-axis is vertical Position relative General Physical Science Chapter 15 Place and Time Space and Time Einstein Space and time related Single entity Time is the 4 th dimension! Cartesian Coordinates Need some system to tell us where something

More information

Lecture #03. January 20, 2010, Wednesday

Lecture #03. January 20, 2010, Wednesday Lecture #03 January 20, 2010, Wednesday Causes of Earth s Seasons Earth-Sun geometry Day length Solar angle (beam spread) Atmospheric beam depletion Shape and Size of the Earth North Pole E Geoid: not

More information

Appearance of the Sky Orientation Motion of sky Seasons Precession (?)

Appearance of the Sky Orientation Motion of sky Seasons Precession (?) Today Appearance of the Sky Orientation Motion of sky Seasons Precession (?) The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The ecliptic is the Sun s apparent

More information

Introduction To Modern Astronomy I: Solar System

Introduction To Modern Astronomy I: Solar System ASTR 111 003 Fall 2007 Lecture 02 Sep. 10, 2007 Introduction To Modern Astronomy I: Solar System Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-15) Chap. 16: Our Sun Chap. 28: Search for

More information

Appearance of the Sky Orientation Motion of sky Seasons Precession (?)

Appearance of the Sky Orientation Motion of sky Seasons Precession (?) Today Appearance of the Sky Orientation Motion of sky Seasons Precession (?) The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The ecliptic is the Sun s apparent

More information

SUBJECT : GEOGRAPHY ROTATION AND REVOLUTION This paper consists of 5 printed pages.

SUBJECT : GEOGRAPHY ROTATION AND REVOLUTION This paper consists of 5 printed pages. SUBJECT : GEOGRAPHY ROTATION AND REVOLUTION 2017-2018 This paper consists of 5 printed pages. 1. Name the motions of the earth. A. They are Rotation and Revolution. 2. What is Rotation? A. Rotation is

More information

Seasons & Time.

Seasons & Time. Seasons & Time Earth s Movements Rotation Movement of Earth Around the Sun Elliptical Orbit Revolution 24 Hours (1 Day) 365 Days (1 Year) The Earth s Revolution & the Tilt of the axis cause variations

More information

THE EARTH AND ITS REPRESENTATION

THE EARTH AND ITS REPRESENTATION UNIT 7 THE EARTH AND ITS REPRESENTATION TABLE OF CONTENTS 1 THE EARTH AND THE SOLAR SYSTEM... 2 2 THE EARTH S MOVEMENTS... 2 2.1 Rotation.... 2 2.2 The revolution of the Earth: seasons of the year....

More information

The Earth-Moon-Sun System

The Earth-Moon-Sun System chapter 7 The Earth-Moon-Sun System section 2 Time and Seasons What You ll Learn how to calculate time and date in different time zones how to distinguish rotation and revolution what causes seasons Before

More information

Time, coordinates and how the Sun and Moon move in the sky

Time, coordinates and how the Sun and Moon move in the sky Time, coordinates and how the Sun and Moon move in the sky Using the colors and magnitudes of quasars drawn from the SDSS Catalog Archive Server to distinguish quasars from stars using the light they emit

More information

Lesson 20: The Earth in its Orbit

Lesson 20: The Earth in its Orbit 291 Lesson 20: The Earth in its Orbit Recall that the Earth s orbit around the un is an ellipse which is almost a perfect circle. The average distance from the un to the Earth is 152,100,000 km (to the

More information

Module 2: Mapping Topic 2 Content: Determining Latitude and Longitude Notes

Module 2: Mapping Topic 2 Content: Determining Latitude and Longitude Notes Introduction In order to more easily locate points on a globe or map, cartographers designed a system of imaginary vertical lines (also called parallels) and horizontal lines (also called meridians) that

More information

The Earth, Moon, and Sky. Lecture 5 1/31/2017

The Earth, Moon, and Sky. Lecture 5 1/31/2017 The Earth, Moon, and Sky Lecture 5 1/31/2017 From Last Time: Stable Orbits The type of orbit depends on the initial speed of the object Stable orbits are either circular or elliptical. Too slow and gravity

More information

Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations.

Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations. Chapter 1: Discovering the Night Sky Constellations: Recognizable patterns of the brighter stars that have been derived from ancient legends. Different cultures have associated the patterns with their

More information

Knowing the Heavens. Goals: Constellations in the Sky

Knowing the Heavens. Goals: Constellations in the Sky Goals: Knowing the Heavens To see how the sky changes during a night and from night to night. To measure the positions of stars in celestial coordinates. To understand the cause of the seasons. Constellations

More information

The Earth and its representation

The Earth and its representation GEOGRAPHY UNIT 1 The Earth and its representation THE SOLAR SYSTEM AND THE EARTH THE SOLAR SYSTEM The solar system is a planetary system. Is a group of astronomical objects who surround a star, in this

More information

Knowing the Heavens. Goals: Constellations in the Sky

Knowing the Heavens. Goals: Constellations in the Sky Goals: Knowing the Heavens To see how the sky changes during a night and from night to night. To measure the positions of stars in celestial coordinates. To understand the cause of the seasons. Constellations

More information

Discovering the Night Sky

Discovering the Night Sky Discovering the Night Sky Guiding Questions 1. What role did astronomy play in ancient civilizations? 2. Are the stars that make up a constellation actually close to one another? 3. Are the same stars

More information

Discovering the Night Sky

Discovering the Night Sky Guiding Questions Discovering the Night Sky 1. What role did astronomy play in ancient civilizations? 2. Are the stars that make up a constellation actually close to one another? 3. Are the same stars

More information

Knowing the Heavens. Chapter Two. Guiding Questions. Naked-eye (unaided-eye) astronomy had an important place in ancient civilizations

Knowing the Heavens. Chapter Two. Guiding Questions. Naked-eye (unaided-eye) astronomy had an important place in ancient civilizations Knowing the Heavens Chapter Two Guiding Questions 1. What role did astronomy play in ancient civilizations? 2. Are the stars that make up a constellation actually close to one another? 3. Are the same

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

Earth s Orbit. Sun Earth Relationships Ridha Hamidi, Ph.D. ESCI-61 Introduction to Photovoltaic Technology

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

More information

James T. Shipman Jerry D. Wilson Charles A. Higgins, Jr. Chapter 15 Place and Time

James T. Shipman Jerry D. Wilson Charles A. Higgins, Jr. Chapter 15 Place and Time James T. Shipman Jerry D. Wilson Charles A. Higgins, Jr. Chapter 15 Place and Time Place & Time Read sections 15.5 and 15.6, but ignore the math. Concentrate on those sections that help explain the slides.

More information

Motions of the Earth

Motions of the Earth Motions of the Earth Our goals for learning: What are the main motions of the Earth in space? How do we see these motions on the ground? How does it affect our lives? How does the orientation of Earth's

More information

Chapter S1 Celestial Timekeeping and Navigation. How do we define the day, month, year, and planetary time periods?

Chapter S1 Celestial Timekeeping and Navigation. How do we define the day, month, year, and planetary time periods? Chapter S1 Celestial Timekeeping and Navigation S1.1 Astronomical Time Periods Our goals for learning:! How do we define the day, month, year, and planetary time periods?! How do we tell the time of day?!

More information

November 20, NOTES ES Rotation, Rev, Tilt.notebook. vertically. night. night. counterclockwise. counterclockwise. East. Foucault.

November 20, NOTES ES Rotation, Rev, Tilt.notebook. vertically. night. night. counterclockwise. counterclockwise. East. Foucault. NOTES ES, Rev,.notebook, and Rotates on an imaginary axis that runs from the to the South North Pole Pole vertically North The of the axis points to a point in space near day Pole Polaris night Responsible

More information

The following terms are some of the vocabulary that students should be familiar with in order to fully master this lesson.

The following terms are some of the vocabulary that students should be familiar with in order to fully master this lesson. Lesson 211: EARTH'S SEASONS Students learn the complex geometry and planetary motions that cause Earth to have four distinct seasons. Fundamental Questions Attempting to give thorough and reasonable answers

More information

Astronomy 122 Section 1 TR Outline. The Earth is Rotating. Question Digital Computer Laboratory

Astronomy 122 Section 1 TR Outline. The Earth is Rotating. Question Digital Computer Laboratory Astronomy 122 Section 1 TR 1300-1350 Outline 1320 Digital Computer Laboratory Leslie Looney Phone: 244-3615 Email: lwlw@wuiucw. wedu Office: Astro Building #218 Office Hours: T 10:30-11:30 a.m. or by appointment

More information

Geographic Grid -Latitudes and Longitudes

Geographic Grid -Latitudes and Longitudes GEOGRAPHY STD 9 Geographic Grid -Latitudes and Longitudes 2018-2019 Q1. Define Geographic Grid. The network of latitudes and longitudes are known as Geographic Grid. They help us to locate places on the

More information

L.O: EARTH'S 23.5 DEGREE TILT ON ITS AXIS GIVES EARTH ITS SEASONS March 21 (SPRING), June 21(SUMMER), Sept 22 (AUTUMN) & Dec 21(WINTER)

L.O: EARTH'S 23.5 DEGREE TILT ON ITS AXIS GIVES EARTH ITS SEASONS March 21 (SPRING), June 21(SUMMER), Sept 22 (AUTUMN) & Dec 21(WINTER) L.O: EARTH'S 23.5 DEGREE TILT ON ITS AXIS GIVES EARTH ITS SEASONS March 21 (SPRING), June 21(SUMMER), Sept 22 (AUTUMN) & Dec 21(WINTER) 1. The apparent daily path of the Sun changes with the seasons because

More information

Astronomy 101: 9/18/2008

Astronomy 101: 9/18/2008 Astronomy 101: 9/18/2008 Announcements Pick up a golf ball at the front of the class or get one from Alex; you will need it for an in-class activity today. You will also need the question sheet from Alex.

More information

Astronomy 291. Professor Bradley M. Peterson

Astronomy 291. Professor Bradley M. Peterson Astronomy 291 Professor Bradley M. Peterson The Sky As a first step, we need to understand the appearance of the sky. Important points (to be explained): The relative positions of stars remain the same

More information

01) The Sun s rays strike the surface of the Earth at 90 degrees at the on December 22.

01) The Sun s rays strike the surface of the Earth at 90 degrees at the on December 22. Package Title: Testbank Course Title: Introducing Physical Geography 6e Chapter Number: 01 Question Type: Multiple Choice 01) The Sun s rays strike the surface of the Earth at 90 degrees at the on December

More information

A Sky Full of Stars - II.

A Sky Full of Stars - II. A Sky Full of Stars - II. Learning Objectives! What is the latitude of the Equator and of the Earth s North and South Poles? What is the declination of the Celestial Equator and of the Celestial Poles?!

More information

Planet Earth. Part 2

Planet Earth. Part 2 Planet Earth Part 2 Sun, Earth and Moon Motions The Solar System revolves around the Milky Way galaxy center. The Sun rotates on its own axis. Earth revolves around the Sun (1 year) and rotates on its

More information

Fundamentals of Satellite technology

Fundamentals of Satellite technology Fundamentals of Satellite technology Prepared by A.Kaviyarasu Assistant Professor Department of Aerospace Engineering Madras Institute Of Technology Chromepet, Chennai Orbital Plane All of the planets,

More information

Chapter S1 Lecture. The Cosmic Perspective Seventh Edition. Celestial Timekeeping and Navigation Pearson Education, Inc.

Chapter S1 Lecture. The Cosmic Perspective Seventh Edition. Celestial Timekeeping and Navigation Pearson Education, Inc. Chapter S1 Lecture The Cosmic Perspective Seventh Edition Celestial Timekeeping and Navigation 2014 Pearson Education, Inc. Celestial Timekeeping and Navigation 2014 Pearson Education, Inc. S1.1 Astronomical

More information

The position of the Sun on the celestial sphere at the solstices and the equinoxes.

The position of the Sun on the celestial sphere at the solstices and the equinoxes. 1 2 3 4 5 6 7 8 9 10 11 12 13 EARTH IN SPACE Tillery, Chapter 18 Artist's concept of the solar system. Shown are the orbits of the planets, Earth being the third planet from the Sun, and the other planets

More information

(1) How does the annual average sun angle at solar noon (that is, the sun angle at noon averaged over a full year) depend on latitude?

(1) How does the annual average sun angle at solar noon (that is, the sun angle at noon averaged over a full year) depend on latitude? (1) How does the annual average sun angle at solar noon (that is, the sun angle at noon averaged over a full year) depend on latitude? (A) * As latitude increases, average sun angle at solar noon decreases.

More information

Geography Class 6 Chapters 3 and

Geography Class 6 Chapters 3 and CHAPTER 3 MOTIONS OF THE EARTH The Earth is always travelling in Space. That makes each person on Earth, a Space Traveller. No one feels the movement of the Earth because humans are too tiny when compared

More information

Why does Earth rotate and what s the evidence? (besides watching it from space ships or satellites) Week 18 January 5, 2015

Why does Earth rotate and what s the evidence? (besides watching it from space ships or satellites) Week 18 January 5, 2015 Why does Earth rotate and what s the evidence? (besides watching it from space ships or satellites) Week 18 January 5, 2015 The sun determines our solar time everywhere on earth as Earth rotates. Can you

More information

Practice Seasons Moon Quiz

Practice Seasons Moon Quiz 1. Which diagram represents the tilt of Earth's axis relative to the Sun's rays on December 15? A) B) C) D) 2. The diagram below represents Earth in space on the first day of a season. 5. Base your answer

More information

Tonight. {01} The map. Relative space. What does a map do? Types of maps GEOG 201 2/17/2010. Instructor: Pesses 1

Tonight. {01} The map. Relative space. What does a map do? Types of maps GEOG 201 2/17/2010. Instructor: Pesses 1 Tonight {01} The map What makes a map Measuring the Earth Map Interpretation & GPS Spring 2010 M. Pesses What does a map do? Shows where things are Shows spatial (topological) relationships Shows patterns,

More information

NAVIGATION THEORY QUESTIONS Basics of Navigation

NAVIGATION THEORY QUESTIONS Basics of Navigation NAVIGATION THEORY QUESTIONS Basics of Navigation Q610065 look at it The angle between the plane of the ecliptic and the plane of equator is approx? 23.5 degrees In which two months of the year is the difference

More information

Chapter: The Earth-Moon-Sun System

Chapter: The Earth-Moon-Sun System Chapter 7 Table of Contents Chapter: The Earth-Moon-Sun System Section 1: Earth in Space Section 2: Time and Seasons Section 3: Earth s Moon 1 Earth in Space Earth s Size and Shape Ancient Measurements

More information

1/3/12. Chapter: The Earth-Moon-Sun System. Ancient Measurements. Earth s Size and Shape. Ancient Measurements. Ancient Measurements

1/3/12. Chapter: The Earth-Moon-Sun System. Ancient Measurements. Earth s Size and Shape. Ancient Measurements. Ancient Measurements // Table of Contents Chapter: The Earth-Moon-Sun System Section : Chapter 7 Section : Section : Earth s Size and Shape Ancient Measurements First, no matter where you are on Earth, objects fall straight

More information

PHAS 1511: Foundations of Astronomy

PHAS 1511: Foundations of Astronomy PHAS 1511: Foundations of Astronomy Dr Roger Wesson Research interests: deaths of stars. Planetary nebulae, novae and supernovae. Astronomy: some maths You can see that distances in astronomy are huge.

More information

Chapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc.

Chapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc. Chapter 2 Discovering the Universe for Yourself 1 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations

More information

Observing the Universe for Yourself

Observing the Universe for Yourself Observing the Universe for Yourself Figure 6-20 Solar-System Formation What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars as well as the Milky Way. A constellation

More information

Downloaded from

Downloaded from Geo Globe : Latitudes and Longitudes 1.Suppose the time at 30 east is 2 p.m. then what is the time at Greenwich? (A) 2 p.m. (B) 12 p.m. (C) 1 p.m. (D) Cannot find 2.What does the term 'Grid' mean

More information

Geometry of Earth Sun System

Geometry of Earth Sun System 12S56 Geometry of Earth Sun System Figure below shows the basic geometry Northern Hemisphere Winter ω equator Earth s Orbit Ecliptic ω ω SUN equator Northern Hemisphere Spring Northern Hemisphere Fall

More information

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

Chapter 1 Image Slides. Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Chapter 1 Image Slides. Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter 1 Image Slides Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display. CH. 1: CYCLES OF THE SKY CO a 1.1 The Celestial Sphere CO b The nearest star to us is about

More information

CHAPTER 2 A USER'S GUIDE TO THE SKY

CHAPTER 2 A USER'S GUIDE TO THE SKY CHAPTER 2 A USER'S GUIDE TO THE SKY MULTIPLE CHOICE 1. In one way of naming stars, a letter indicates its brightness relative to the other stars in the constellation. a. English b. Arabic c. Greek d. Cyrillic

More information

Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky

Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

Chapter 2 Discovering the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we

More information

MOTIONS OF THE EARTH. Figure 3.1 : Inclination of the Earth s axis and the orbital plane. Figure 3.2 : Day and Night on the Earth due to rotation

MOTIONS OF THE EARTH. Figure 3.1 : Inclination of the Earth s axis and the orbital plane. Figure 3.2 : Day and Night on the Earth due to rotation 3 Let s Do Take a ball to represent the earth and a lighted candle to represent the sun. Mark a point on the ball to represent a town X. Place the ball in such a way that the town X is in darkness. Now

More information

It s Full of Stars! Outline. A Sky Full of Stars. Astronomy 210. lights), about how many stars can we see with

It s Full of Stars! Outline. A Sky Full of Stars. Astronomy 210. lights), about how many stars can we see with Astronomy 210 Section 1 MWF 1500-1550 134 Astronomy Building Leslie Looney Phone: 244-3615 Email: lwlw@wuiucw. wedu Office: Astro Building #218 Office Hours: MTF 10:30-11:30 a.m. or by appointment This

More information

GEOGRAPHY STD.9 LATITUDE & LONGITUDE

GEOGRAPHY STD.9 LATITUDE & LONGITUDE GEOGRAPHY STD.9 LATITUDE & LONGITUDE 1. What is the Earth Grid? A. The complete network of meridians & parallels is called the earth Grid. 2. What is Latitude? A. The latitude of a place is the distance

More information

Aileen A. O Donoghue Priest Associate Professor of Physics

Aileen A. O Donoghue Priest Associate Professor of Physics SOAR: The Sky in Motion Life on the Tilted Teacup Ride The Year Aileen A. O Donoghue Priest Associate Professor of Physics Celestial Coordinates Right Ascension RA or From prime meridian (0 h ) to 23 h

More information

drinking straw, protractor, string, and rock. observer on Earth. Sun across the sky on March 21 as seen by an

drinking straw, protractor, string, and rock. observer on Earth. Sun across the sky on March 21 as seen by an 1. The diagram below represents some constellations and one position of Earth in its orbit around the Sun. These constellations are visible to an observer on Earth at different times of the year. When

More information

Reasons for the seasons - Rebecca Kaplan

Reasons for the seasons - Rebecca Kaplan Reasons for the seasons - Rebecca Kaplan https://www.youtube.com/watch?v=dd_8jm5ptlk https://www.timeanddate.com/worldclock/sunearth.html https://www.time.gov/ https://www.space.com/33790-harvest-moon-guide.html

More information

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc.

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc. Chapter 2 Lecture The Cosmic Perspective Seventh Edition Discovering the Universe for Yourself Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the

More information

3. The Sun s Position

3. The Sun s Position 3. The Sun s Position In order to understand how to collect energy from the sun, one must first be able to predict the location of the sun relative to the collection device. In this chapter we develop

More information

Name: Date: 5. The bright stars Vega, Deneb, and Altair form A) the summer triangle. B) the winter triangle. C) the Big Dipper. D) Orion, the Hunter.

Name: Date: 5. The bright stars Vega, Deneb, and Altair form A) the summer triangle. B) the winter triangle. C) the Big Dipper. D) Orion, the Hunter. Name: Date: 1. If there are about 6000 stars in the entire sky that can be seen by the unaided human eye, about how many stars would be seen at a particular instant on a given dark night from a single

More information

HEATING THE ATMOSPHERE

HEATING THE ATMOSPHERE HEATING THE ATMOSPHERE Earth and Sun 99.9% of Earth s heat comes from Sun But

More information

Introduction To Astronomy Lesson 1

Introduction To Astronomy Lesson 1 Introduction To Astronomy Lesson 1 Topics for this Lesson Earth Based Coordinates The Celestial Sphere and Sky Coordinates The North Star Measuring Distances on the Sky The Motion of Objects in the Sky

More information

GLOBE : LATITUDES AND LONGITUDES

GLOBE : LATITUDES AND LONGITUDES 2 Figure 2.1 : Globe Let s Do Take a big round potato or a ball. Pierce a knitting needle through it. The needle resembles the axis shown in a globe. You can now move the potato or the ball around this

More information

Seasons. What causes the seasons?

Seasons. What causes the seasons? Questions: Seasons What causes the seasons? How do we mark the progression of the seasons? What is the seasonal motion of the sun in the sky? What could cause the seasonal motion of the sun to change over

More information

HNRS 227 Fall 2007 Chapter 14. Earth in Space presented by Prof. Geller 25 October 2007

HNRS 227 Fall 2007 Chapter 14. Earth in Space presented by Prof. Geller 25 October 2007 HNRS 227 Fall 2007 Chapter 14 Earth in Space presented by Prof. Geller 25 October 2007 Key Points of Chapter 14 Shape, Size and Motions of the Earth Rotation and Revolution Precession Coordinate Systems

More information

Time Zones. Doug Fischer Geog 106 LRS

Time Zones. Doug Fischer Geog 106 LRS Time Zones Doug Fischer Geog 106 LRS Learning goals Students should be able to Explain time zones as a function of longitude Calculate time differences between different locations Demonstrate corrections

More information

Chapter 1. Essentials of Geography Pearson Education, Inc.

Chapter 1. Essentials of Geography Pearson Education, Inc. Chapter 1. Essentials of Geography Learning Objectives Define geography in general and physical geography in particular. Discuss human activities and human population growth as they relate to geographic

More information

EARTHS SHAPE AND POLARIS PRACTICE 2017

EARTHS SHAPE AND POLARIS PRACTICE 2017 1. In the diagram below, letters A through D represent the locations of four observers on the Earth's surface. Each observer has the same mass. 3. Which diagram most accurately shows the cross-sectional

More information

C) the seasonal changes in constellations viewed in the night sky D) The duration of insolation will increase and the temperature will increase.

C) the seasonal changes in constellations viewed in the night sky D) The duration of insolation will increase and the temperature will increase. 1. Which event is a direct result of Earth's revolution? A) the apparent deflection of winds B) the changing of the Moon phases C) the seasonal changes in constellations viewed in the night sky D) the

More information

The celestial sphere, the coordinates system, seasons, phases of the moon and eclipses. Chapters 2 and S1

The celestial sphere, the coordinates system, seasons, phases of the moon and eclipses. Chapters 2 and S1 The celestial sphere, the coordinates system, seasons, phases of the moon and eclipses Chapters 2 and S1 The celestial sphere and the coordinates system Chapter S1 How to find our way in the sky? Let s

More information

Mapping Earth Review Note Cards

Mapping Earth Review Note Cards Review Note Cards Spheres of Earth Atmosphere- Layer of gases Hydrosphere- All liquid water Lithosphere- Solid surface Biosphere-Living Portion Cryosphere-Ice Portion Evidence that the Earth is Round The

More information

Complete the following: a. Lines of latitude are parallel to the equator. Name:

Complete the following: a. Lines of latitude are parallel to the equator. Name: Name: Date: Social Studies Introduction: Basic Geography Period: Latitude Latitude is defined as a measurement of distance in degrees north and south of the equator. The word latitude is derived from the

More information

Earth s Motion. Lesson Outline LESSON 1. A. Earth and the Sun 1. The diameter is more than 100 times greater than

Earth s Motion. Lesson Outline LESSON 1. A. Earth and the Sun 1. The diameter is more than 100 times greater than Lesson Outline Earth s Motion LESSON 1 A. Earth and the Sun 1. The diameter is more than 100 times greater than Earth s diameter. a. In the Sun, atoms combine during, producing huge amounts of energy.

More information

Section 2. Locating Astronomical Objects in the Night Sky What Do You See? What Do You See? Think About It. Investigate.

Section 2. Locating Astronomical Objects in the Night Sky What Do You See? What Do You See? Think About It. Investigate. Section 2 Locating Astronomical Objects in the Night Sky Section 2 Locating Astronomical Objects in the Night Sky What Do You See? What Do You See? Learning Outcomes In this section, you will Construct

More information

A2 Principi di Astrofisica. Coordinate Celesti

A2 Principi di Astrofisica. Coordinate Celesti A2 Principi di Astrofisica Coordinate Celesti ESO La Silla Tel. 3.6m Celestial Sphere Our lack of depth perception when we look into space creates the illusion that Earth is surrounded by a celestial sphere.

More information

Reasons for the Seasons

Reasons for the Seasons Regents Earth Science Name: Unit 6: Astronomy Date: Section: LAB # Reasons for the Seasons Introduction: The units of time that mankind has devised are all imaginary. We base them on seasonal changes and

More information

Unit I: Earth Dimensions. Review Book pp.19-30

Unit I: Earth Dimensions. Review Book pp.19-30 Unit I: Earth Dimensions Review Book pp.19-30 Objective #1 Describe the actual shape of the Earth and explain 3 pieces of evidence for its actual shape. Earth s Shape The Earth appears to be the shape

More information

AUSTRALIAN HOMESCHOOLING SERIES SAMPLE. Earth and Space. Secondary Science 7C. Years 7 9. Written by Valerie Marett. CORONEOS PUBLICATIONS Item No 544

AUSTRALIAN HOMESCHOOLING SERIES SAMPLE. Earth and Space. Secondary Science 7C. Years 7 9. Written by Valerie Marett. CORONEOS PUBLICATIONS Item No 544 AUSTRALIAN HOMESCHOOLING SERIES Earth and Space Secondary Science 7C Years 7 9 Written by Valerie Marett CORONEOS PUBLICATIONS Item No 544 Secondary Science Earth and Space Contents The Earth. 2 Movements

More information

STANDARD. S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position.

STANDARD. S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position. STANDARD S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position. S6E2 b. Explain the alignment of the earth, moon, and sun during solar and lunar eclipses. c. Relate the

More information

CELESTIAL COORDINATES

CELESTIAL COORDINATES ASTR 1030 Astronomy Lab 27 Celestial Coordinates CELESTIAL COORDINATES GEOGRAPHIC COORDINATES The Earth's geographic coordinate system is familiar to everyone - the north and south poles are defined by

More information

10/17/2012. Observing the Sky. Lecture 8. Chapter 2 Opener

10/17/2012. Observing the Sky. Lecture 8. Chapter 2 Opener Observing the Sky Lecture 8 Chapter 2 Opener 1 Figure 2.1 Figure 2.2 2 Figure 2.6 Figure 2.4 Annotated 3 The Celestial Sphere The celestial sphere is the vast hollow sphere on which the stars appear fixed.

More information

4. Which object best represents a true scale model of the shape of the Earth? A) a Ping-Pong ball B) a football C) an egg D) a pear

4. Which object best represents a true scale model of the shape of the Earth? A) a Ping-Pong ball B) a football C) an egg D) a pear Name Test on Friday 1. Which diagram most accurately shows the cross-sectional shape of the Earth? A) B) C) D) Date Review Sheet 4. Which object best represents a true scale model of the shape of the Earth?

More information

Summary Sheet #1 for Astronomy Main Lesson

Summary Sheet #1 for Astronomy Main Lesson Summary Sheet #1 for Astronomy Main Lesson From our perspective on earth The earth appears flat. We can see half the celestial sphere at any time. The earth s axis is always perpendicular to the equator.

More information

Mid Term Prep-Latitude and Longitude

Mid Term Prep-Latitude and Longitude 1. What is the approximate altitude of Polaris at Syracuse, New York? A) 43 B) 47 C) 76 D) 90º 2. If an observer on Earth views Polaris on the horizon, the observer is located at the A) equator (0 ) B)

More information

The. Astronomy is full of cycles. Like the day, the month, & the year In this section we will try to understand these cycles.

The. Astronomy is full of cycles. Like the day, the month, & the year In this section we will try to understand these cycles. Understanding The Sky Astronomy is full of cycles Like the day, the month, & the year In this section we will try to understand these cycles. For Example Why do we think of stars as nighttime objects?

More information

Astronomy 100 Section 2 MWF Greg Hall

Astronomy 100 Section 2 MWF Greg Hall Astronomy 100 Section 2 MWF 1200-1300 100 Greg Hall Leslie Looney Phone: 217-244-3615 Email: lwl @ uiuc. edu Office: Astro Building #218 Office Hours: MTF 10:30-11:30 a.m. or by appointment Class Web Page

More information

Oberth: Energy vs. Momentum

Oberth: Energy vs. Momentum 1 2 The Oberth Effect 3 Oberth: Energy vs. Momentum 4 The Celestial Sphere From our perspective on Earth the stars appear embedded on a distant 2-dimensional surface the Celestial Sphere. 5 The Celestial

More information

Today in Space News: Earth s oldest rock found on the Moon.

Today in Space News: Earth s oldest rock found on the Moon. Today in Space News: Earth s oldest rock found on the Moon https://www.lpi.usra.edu/features/012419/oldest-rock/ Study Points Predict the approximate time of day/night you should look for first quarter

More information

6/17. Universe from Smallest to Largest:

6/17. Universe from Smallest to Largest: 6/17 Universe from Smallest to Largest: 1. Quarks and Leptons fundamental building blocks of the universe size about 0 (?) importance: quarks combine together to form neutrons and protons. One of the leptons

More information

Aim: What causes Seasons?

Aim: What causes Seasons? Notepack 28 Aim: What causes Seasons? Do Now: What is the difference between revolution and rotation? Earth s rotation The Earth rotates on its axis (imaginary vertical line around which Earth spins) every

More information

GEOGRAPHY AND HISTORY

GEOGRAPHY AND HISTORY GEOGRAPHY AND HISTORY YEAR 1, PART 1 www.vicensvives.es Contents 01 Our planet Earth 02 The representation of the Earth: maps 03 The Earth s relief 04 Rivers and seas 05 Weather and climate 06 Climates

More information

Modern Navigation. Thomas Herring

Modern Navigation. Thomas Herring 12.215 Modern Navigation Thomas Herring Review of Monday s Class Spherical Trigonometry Review plane trigonometry Concepts in Spherical Trigonometry Distance measures Azimuths and bearings Basic formulas:

More information