I. Evidence of Earth s Spherical Shape

Similar documents
EARTH SCIENCE KEY UNIT 2-H

Benefit of astronomy to ancient cultures

The Earth & its good friend, the Moon. SNC1D7 - Space

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

EARTHS SHAPE AND POLARIS PRACTICE 2017

17. According to the data below, what is the exact shape of the Earth?

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

2.1 Patterns in the Night Sky

Astronomy 103: First Exam

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

Planetary Science Unit Map Grade 8

Mapping Earth Review Note Cards

Time and Diurnal Motion

Scientists observe the environment around them using their five senses.

Chapter 2 Discovering the Universe for Yourself

Time and Diurnal Motion

Lecture 2 : Early Cosmology

Lecture #03. January 20, 2010, Wednesday

Observing the Universe for Yourself

Time and Diurnal Motion. 1a. The Earth Is Flat. 1c. Aristotle ( BC) 1b. The Earth Is Round. Time and Diurnal Motion

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

Chapter 2 Discovering the Universe for Yourself

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

Topic Guide: Measuring the Solar System. GCSE (9-1) Astronomy. Pearson Edexcel Level 1/Level 2 GCSE (9-1) in Astronomy (1AS0)

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

lightyears observable universe astronomical unit po- laris perihelion Milky Way

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

Mid Term Prep-Shape of the Earth

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.) Ecliptic

Dr. Tariq Al-Abdullah

astronomy A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.

Practice Questions: Shape of the Earth

3. Lunar Motions & Eclipses. Lunar Phases: Static & Dynamic. Static & Dynamic Lunar Phases. Earth & Moon: Both Show Phases!

Brock University. Test 1, October 2017 Number of pages: 9 Course: ASTR 1P01, Section 1 Number of Students: 470 Date of Examination: October 3, 2017

2 OBSERVING THE SKY: THE BIRTH OF ASTRONOMY

All that is required to measure the diameter of the Earth is a person with stick and a brain.

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009

Brock University. Test 1, May 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: May 21, 2014

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself

Chapter: The Earth-Moon-Sun System

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

Astronomy. Today: Eclipses and the Motion of the Moon. First homework on WebAssign is due Thursday at 11:00pm

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.

Inventors and Scientists: Eratosthenes

Time and Diurnal Motion. 1a. The Earth Is Flat. 1c. Aristotle ( BC) 1b. The Earth Is Round. Time and Diurnal Motion

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

Astronomical Distances. Astronomical Distances 1/30

TAKEN FROM HORIZONS 7TH EDITION CHAPTER 3 TUTORIAL QUIZ

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

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

Astronomical Distances

4 ERATOSTHENES OF CYRENE

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

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

Astronomy Review. Use the following four pictures to answer questions 1-4.

4 ERATOSTHENES OF CYRENE

Eratosthenes method of measuring the Earth

a. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU

Discovering the Universe for Yourself

AST 2010 Descriptive Astronomy Study Guide Exam I

Discovering the Universe for Yourself (Chapter 2) Years, Seasons, and Months: The Motions of Sun, Earth, and Moon

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

ASTRO Fall 2012 LAB #2: Observing the Night Sky

18.1 Earth and Its Moon Earth s shape and orbit Earth s shape Earth s orbit around the Sun

chapter 10 questions_pictures removed.notebook September 28, 2017 Chapter 10 What We Know About the Universe Has Taken Us Thousands of Years to Learn

Size of the Earth and the Distances to the Moon and the Sun

D] The Lunar eclipse; The shadow cast by the Earth on the moon during Lunar eclipse is always circular proving the Erath is a sphere.

Chapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Early Ideas of the Universe

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Brock University. Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014

A) M D) The Moon s distance from Earth varies in a cyclic manner.

4 ERATOSTHENES OF CYRENE

Earth Science, 13e Tarbuck & Lutgens

Name: Class: Date: ID: A

The Celestial Sphere. From our perspective on Earth the stars appear embedded on a distant 2 dimensional surface the Celestial Sphere.

Chapter 1 Introduction to the Earth

Exercise 3: The history of astronomy

ASTRONOMY Merit Badge Requirements

3. The diagram below shows the Moon at four positions in its orbit around Earth as viewed from above the North Pole.

PHYS 160 Astronomy Test #1 Name Answer Key Test Version A

Knowing the Heavens. Goals: Constellations in the Sky

Period: Name: Astronomy Part 3A. Earth s Rotation: Video Notes Sheets. Earth Science with Mr. Sammartano Hommocks Middle School, Team 8-3

2.2 The Reason for Seasons

Knowing the Heavens. Goals: Constellations in the Sky

Earth Science Review Ch 1 & 2. Chapter 1 - Introduction to Earth Science

MIDTERM PRACTICE EXAM

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

Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest).

Observing the Night Sky: Locating Objects

Introduction To Modern Astronomy I: Solar System

Brock University. Test 1, October 2016 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: October 3, 2016

Space Notes Covers Objectives 1 & 2

How the Greeks Used Geometry to Understand the Stars

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

CA1 2.11: Designing an Equatorial Sundial Activity

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

CHAPTER 2 Strand 1: Structure and Motion within the Solar System

Sample Assessment Material Time: 2 hours

8R EARTH'S SHAPE PRACTICE

Transcription:

Earth s Shape

I. Evidence of Earth s Spherical Shape A. Two millennia ago Greek mathematicians determined Earth s shape was. spherical

1. Aristarchus (310 B.C. to 210 B.C.) a. Believed in universe. Sun-centered b. Attempted to determine the size of the Sun and Moon and distances to them.

2. Eratosthenes (274 B.C. to 195 B.C) a. Calculated Earth s circumference. b. Evidence of shape spherical (1) On the summer solstice at noon, the Sun s altitude is at not the same two locations on the same meridian of longitude. (2) Can be explained by a Earth. round

Eratosthenes c. Measurements of allowed shadow angles for a mathematical calculation of circumference using geometric relationships. Angle d = Angle e a = S 360 o C Where: a = Shadow Angle S = surface distance C = Circumference 7.2 o 5000 stadia = 360 o C C = (5000 stadia)(360o ) 7.2 o

B. Ships Sailing out to Sea a. Masts of ships are the to last disappear below the horizon. b. Caused by Earth s. curvature

Ships Gradually Disappear Below the Horizon

C. Sunlight at Sunset 1. As the Sun sets, the last sunlight is seen on objects. high

D. Lunar Eclipses Earth s shadow is. curved

E. Ferdinand Magellan s ships circumnavigated Earth in 1522. Only one of the five ships that set sail in 1519, the Victoria, completed the expedition Only 18 of the approximately 270 men returned. Magellan was killed in a battle in 1521 on the Philippine island of Cebu.

F. Photographs of Earth from Space Earthrise from the Moon Earth from Apollo 1. The evidence best for Earth s shape. 2. Clearly shown as being. spherical Earth and the Moon from the Galileo spacecraft

II. Earth s Shape is not a Perfect Sphere A. Earth s true shape is an. oblate spheroid 1. A perfect sphere s circumference is through the same the poles and equator. 2. Earth s Polar diameter (and circumference) is slightly smaller than at the equator.

Earth s Out of Round Shape isn t Noticeable The equatorial bulge in this diagram is exaggerated about 1,615 times! Perfect Sphere On the scale of the actual Earth photo and the drawing, Earth appears to be a perfect sphere. 3. As a result, Earth has a at the equator which can t be seen by the naked eye. 4. This is caused by Earth s.

Earth s Out of Round Shape isn t Noticeable The equatorial bulge in this diagram is exaggerated about 1,615 times! Perfect Sphere On the scale of the actual Earth photo and the drawing, Earth appears to be a perfect sphere. 3. As a result, Earth has a at the equator which can t be seen by the naked eye. 4. This is caused by Earth s.

Earth s Out of Round Shape isn t Noticeable The equatorial bulge in this diagram is exaggerated about 1,615 times! Perfect Sphere On the scale of the actual Earth photo and the drawing, Earth appears to be a perfect sphere. 3. As a result, Earth has a at slight bulge the equator which can t be seen by the naked eye. 4. This is caused by Earth s. rotation

B. Evidence of Earth s True Shape 1. Gravity Measurements

Force of Gravity a. Directional Component of Earth s Gravity Plumbob (1) Objects are attracted towards Earth s. center of mass (2) The direction of this force would always be at vertical every location on a perfectly spherical Earth. (3) Actual measurements show that the direction of the force of gravity is at not vertical every point

b. Magnitude of Gravity Measurements (1) The force of gravity should be at the same every location on a perfectly spherical Earth. (2) Actual measurements show that the force of gravity is at greater the poles than at the equator (factoring out the effect of elevation). Gravitometer to measure gravity

(a) According to Newton s Universal Law of Gravitation, the factor affecting force must be a change in. distance (b) As distance decreases, force. increases (c) As a result, the greater force at the poles is the result of a shorter distance to Earth s center of mass, indicating a smaller polar diameter F G (m 1 )(m 2 ) d 2 (d) Since weight is the effect of gravity on a mass, a person s weight is slightly at less the equator than at the poles

2. The Altitude of Polaris Sextant

Finding Polaris using the Big Dipper s Pointer Stars

a. The altitude to Polaris is equal to the observer s. latitude b. Precise measurements show that the altitude is than slightly different the latitude because Earth isn t perfectly spherical.