Intro to Astronomy. Looking at Our Space Neighborhood

Size: px
Start display at page:

Download "Intro to Astronomy. Looking at Our Space Neighborhood"

Transcription

1 Intro to Astronomy Looking at Our Space Neighborhood

2 Astronomy: The Original Science Ancient cultures used the movement of stars, planets and the moon to mark time Astronomy: the study of the universe This led to the development of the first calendar Year: Earth orbits the sun one time ( days) Month: about one orbit of the moon around Earth (29.25 days) Day: one rotation of Earth on its axis

3 Who s Who of Early Astronomy Ptolemy 140 A.D. Greek astronomer Thought Earth was at the center of the universe and other planets & the sun revolved around it Incorrect, but predicted motion of planets better than anyone else had Copernicus 1543 A.D. Polish astronomer Said the Sun was at the center of the universe and all planets orbit the sun Very controversial! Not quickly accepted

4 Who s Who of Early Astronomy Tycho Brahe late 1500 s Danish astronomer Favored Ptolemy s Earth-centered theory Used tools to make detailed astronomical observations that helped future astronomers Johannes Kepler early 1600 s Assistant to Tycho Brahe Used Brahe s data to show that all planets revolve around the sun in elliptical orbits Gave three laws of planetary motion that are still used today

5 Who s Who of Early Astronomy Galileo Galilei 1609 One of the first to use a telescope to see space Discovered craters and mountains on the Moon and four of Jupiter s moons Showed that planets are not stars, but more similar to Earth Sir Isaac Newton 1687 Showed that all objects in the universe attract each other by gravitational force (depends on mass & distance) Explained why all planets orbit largest object the Sun Newton s Cannon why object orbit Earth

6 Modern Astronomy Edwin Hubble 1924 Astronomers thought our galaxy (Milky Way) included every object in space Edwin proved the existence of other galaxies New technology continues to improve our understanding of space New galaxies, planets and moons are continually being discovered

7 Earth s Motion Early Astronomers First Focus

8 How Does Earth s Motion Affect Time? Axis the imaginary line that goes from the North to South Pole Rotation Earth s spin on its axis (think of a top) Earth s rotation causes day and night One rotation takes about 24 hours 1 day!

9 How Does Earth s Motion Affect Time? Revolution Earth s movement around the Sun One revolution is one year Earth s path around the Sun is called its orbit Earth s orbit is an oval (ellipse), not a circle days (rotations) per year (revolution) That s why we have leap year every 4 years!

10 How Does Earth s Motion Affect Seasons? 4 Seasons: summer, winter, spring, fall Seasons in Northern Hemisphere happen at different times than Southern Hemisphere Earth has seasons because its axis is tilted 23.5 as it moves around the sun

11 The Moon Our Closest Neighbor in the Neighborhood

12 Structure & Origin of the Moon 3,476 km in diameter (about distance across the US) ¼ the diameter of Earth 1/8 the mass of Earth (less dense than Earth) Collision Theory suggests that an object about the size of Mars hit Earth and the scattered material formed the moon 4.5 billion years ago

13 Features of the Moon Galileo made the first detailed observations of moon s features in 1609 with a telescope Craters pits that cover the surface, caused by impacts of meteoroids Highlands mountainous structures that cast large shadows Marias flat, dark areas that Galileo thought were oceans (maria = seas in Latin) Low, dry areas that were flooded with molten rock billions of years ago

14 Our Closest Neighbor 384,400 km from Earth (about 30 Earth s lined up) Revolves around Earth as Earth revolves around the Sun The positions of the moon, Earth and Sun cause the phases of the moon, eclipses and tides on Earth

15 Motions of the Moon Has its own axis tilted 5 Rotation (day): 27.3 Earth days Revolution (year): 27.3 Earth days So one year and one day on the moon are the same length! Earth & moon have synchronous rotation Near side of the moon always faces Earth You never see the far side of the moon from Earth

16 Phases of the Moon The moon does not produce light it reflects light from the sun The shapes of the moon you see are called phases Half of the moon is always lit, but sometimes Earth gets in the way The phase of the moon you see depends on how much of the sunlit side of the moon faces Earth

17 Cycle of Moon Phases Start: New Moon The lit side faces away from Earth so no moon is seen Phases in Order: 1. New Moon 2. Waxing Crescent 3. First Quarter 4. Waxing Gibbous 5. Full Moon 6. Waning Gibbous 7. Third Quarter 8. Waning Crescent then back to New Moon! One complete cycle takes about 28 days (1 month)

18 Eclipses Eclipse: when moon s shadow hits Earth or Earth s shadow hits the moon Two Types: (named for what is being blocked) Solar Lunar

19 Solar Eclipses When a new moon passes between Earth and the Sun, blocking light from reaching Earth Total Solar Eclipses where light is completely blocked by the moon Only people in the darkest part of moon s shadow (umbra) experience this Partial Solar Eclipse where part of the sun is visible; more common People in the lighter part of moon s shadow (penumbra) experience this

20 Lunar Eclipses Occurs at a full moon when Earth is directly between the moon and the sun, blocking light from reaching the moon Earth s shadow also has an umbra (darkness) and penumbra (partial darkness) Total Lunar Eclipse - where light is completely blocked by the Earth Can be seen anywhere on Earth where the moon is visible Partial Lunar Eclipse - where the Sun, Earth and moon are not perfectly in line moon passes partly into Earth s umbra

21 Tides Tide rise and fall of water every 12.5 hours Caused by gravity pulling the moon and Earth together Occur because of differences in how much the moon pulls on different parts of Earth (and the water on it)

22 High & Low Tide Water on Earth closer to the moon is pulled, forming high tide Water on the other side of the planet has much weaker pull and resists due to inertia, forming another high tide Low tides occur between the two high tides

23 Spring & Neap Tides Spring Tide: Occur when the moon, sun and Earth are in line Gravity of sun and moon combine to produce greatest difference in high/low tide Neap Tide: when the earth and sun are at right angles to earth and the moon Produces a tide with the least difference between high/low tide It s like a tug of war between the sun and the moon!

Physical Science. Chapter 22 The Earth in Space. Earth s Rotation

Physical Science. Chapter 22 The Earth in Space. Earth s Rotation Physical Science Chapter 22 The Earth in Space Earth s Rotation Axis imaginary line passing through the North and South Pole Earth s axis is tilted at 23 ½ degrees Rotation: the Earth spinning on its axis

More information

Physical Science. Chapter 22 The Earth in Space

Physical Science. Chapter 22 The Earth in Space Physical Science Chapter 22 The Earth in Space Earth s Rotation Axis imaginary line passing through the North and South Pole Earth s axis is tilted at 23 ½ degrees Rotation: the Earth spinning on its axis

More information

Name Period Chapter 12 &13 Study Guide

Name Period Chapter 12 &13 Study Guide Name Period Chapter 12 &13 Study Guide Multiple Choice Identify the choice that best completes the statement or answers the question. 1. When are tides highest? a. during the moon s first quarter phase

More information

Astronomy- The Original Science

Astronomy- The Original Science Astronomy- The Original Science Imagine that it is 5,000 years ago. Clocks and modern calendars have not been invented. How would you tell time or know what day it is? One way to tell the time is to study

More information

PHASES, ECLIPSES, AND TIDES

PHASES, ECLIPSES, AND TIDES PHASES, ECLIPSES, AND TIDES MOTIONS OF THE MOON The changing relative positions of the moon, Earth, and sun cause the phases of the moon, eclipses, and tides. The moon rotates once on its axis in the same

More information

Earth in Space. Guide for Reading How does Earth move in space? What causes the cycle of seasons on Earth?

Earth in Space. Guide for Reading How does Earth move in space? What causes the cycle of seasons on Earth? Earth in Space How does Earth move in space? What causes the cycle of seasons on Earth? The study of the moon, stars, and other objects in space is called astronomy. Ancient astronomers studied the movements

More information

Earth in Space. The Sun-Earth-Moon System

Earth in Space. The Sun-Earth-Moon System in Space The --Moon System What do you think? Read the two statements below and decide whether you agree or disagree with them. Place an A in the Before column if you agree with the statement or a D if

More information

1 Astronomy: The Original Science

1 Astronomy: The Original Science CHAPTER 18 1 Astronomy: The Original Science SECTION Studying Space BEFORE YOU READ After you read this section, you should be able to answer these questions: How do astronomers define a day, a month,

More information

Chapter Introduction Lesson 1 Earth s Motion Lesson 2 Earth s Moon Lesson 3 Eclipses and Tides Chapter Wrap-Up. Jason Reed/Photodisc/Getty Images

Chapter Introduction Lesson 1 Earth s Motion Lesson 2 Earth s Moon Lesson 3 Eclipses and Tides Chapter Wrap-Up. Jason Reed/Photodisc/Getty Images Chapter Introduction Lesson 1 Earth s Motion Lesson 2 Earth s Moon Lesson 3 Eclipses and Tides Chapter Wrap-Up Jason Reed/Photodisc/Getty Images What natural phenomena do the motions of Earth and the Moon

More information

7.4 Universal Gravitation

7.4 Universal Gravitation Circular Motion Velocity is a vector quantity, which means that it involves both speed (magnitude) and direction. Therefore an object traveling at a constant speed can still accelerate if the direction

More information

SPACE REVIEW. 1. The time it takes for the Earth to around the sun is one year. a. rotate b. revolve

SPACE REVIEW. 1. The time it takes for the Earth to around the sun is one year. a. rotate b. revolve SPACE REVIEW 1. The time it takes for the Earth to around the sun is one year. a. rotate b. revolve 2. Which planet is known as the "Red Planet"? a. Earth b. Mars c. Uranus d. Venus 3. One complete revolution

More information

Chapter 22 Exam Study Guide

Chapter 22 Exam Study Guide Chapter 22 Exam Study Guide Name: Hour: Date: Multiple Choice Identify the choice that best completes the statement or answers the question. Write the letter that best answers the question or completes

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

refractors satellite electromagnetic radiation

refractors satellite electromagnetic radiation Chapter 19 Exploring Space space probe reflectors mirror refractors satellite electromagnetic radiation light lens thrust 1. All radiation is classified by wavelength in the. 2. Two types of telescopes

More information

LESSON 2 THE EARTH-SUN-MOON SYSTEM. Chapter 8 Astronomy

LESSON 2 THE EARTH-SUN-MOON SYSTEM. Chapter 8 Astronomy LESSON 2 THE EARTH-SUN-MOON SYSTEM Chapter 8 Astronomy OBJECTIVES Investigate how the interaction of Earth, the Moon, and the Sun causes lunar phases. Describe conditions that produce lunar and solar eclipses.

More information

SPI Use data to draw conclusions about the major components of the universe.

SPI Use data to draw conclusions about the major components of the universe. SPI 0607.6.1 - Use data to draw conclusions about the major components of the universe. o Stars are huge, hot, brilliant balls of gas trillions of kilometers away. A Galaxy is a collection of billions

More information

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

Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest). Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest). Rotation The movement of one object as it turns or spins around a central point or axis. Revolution The movement

More information

Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1

Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1 Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1 Chapter 1 1. A scientific hypothesis is a) a wild, baseless guess about how something works. b) a collection of ideas that seems to explain

More information

Chapter. Origin of Modern Astronomy

Chapter. Origin of Modern Astronomy Chapter Origin of Modern Astronomy 22.1 Early Astronomy Ancient Greeks Astronomy is the science that studies the universe. It includes the observation and interpretation of celestial bodies and phenomena.

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

Name: Earth and Space Assessment Study Guide. Assessment Date : Term Rotation Revolution

Name: Earth and Space Assessment Study Guide. Assessment Date : Term Rotation Revolution Name: Earth and Space Assessment Study Guide Assessment Date : Earth s Rotation and Revolution Term Rotation Revolution Brief Definition Earth s Time to Complete One complete spin on an axis 24 hours (or

More information

The Sun Earth Moon System

The Sun Earth Moon System The Sun Earth Moon System Planet Earth Shape Spherical Oval shaped West to east* Rotation Fifteen degree /hour* Rotation is just less than 24 hours Magnetic field North and south magnetic poles Protect

More information

Chapter 19 Exploring Space. I. Fill in the blank

Chapter 19 Exploring Space. I. Fill in the blank Chapter 19 Exploring Space 1. All radiation is classified by wavelength in the electromagnetic spectrum. 2. Two types of telescopes that collect visible light are refractors and reflectors. 3. An uncrewed

More information

Solar System Glossary. The point in an object s elliptical orbit farthest from the body it is orbiting

Solar System Glossary. The point in an object s elliptical orbit farthest from the body it is orbiting Solar System Glossary Apogee Atmosphere Asteroid Axis Autumn Barred spiral The point in an object s elliptical orbit farthest from the body it is orbiting The air that surrounds Earth and other planets

More information

Orbital Mechanics. CTLA Earth & Environmental Science

Orbital Mechanics. CTLA Earth & Environmental Science Orbital Mechanics CTLA Earth & Environmental Science The Earth Spherical body that is flattened near the poles due to centrifugal force (rotation of the Earth) 40,074 KM across at the Equator 40,0007 KM

More information

a. The imaginary line that passes through Earth at the N and S poles is

a. The imaginary line that passes through Earth at the N and S poles is I. Earth in Space (p. 660-665) A. How Earth Moves Chapter 19: Earth, Moon & Sun a. Earth moves in two major ways: rotation & revolution 1. Rotation a. The imaginary line that passes through Earth at the

More information

Chapter 18: Studying Space Astronomy: The Original Science

Chapter 18: Studying Space Astronomy: The Original Science Chapter 18: Studying Space 18.1 Astronomy: The Original Science What is Astronomy? Astronomy is the study of the universe People in ancient cultures used the seasonal cycles of the stars, planets, and

More information

8 th Grade Earth, Moon and Sun Systems Review

8 th Grade Earth, Moon and Sun Systems Review 8 th Grade Earth, Moon and Sun Systems Review #1 Click on the link to learn What causes Seasons? A #2 H G B D C What is season A in this diagram? E F A: Summer B: Fall C: Winter D: Spring D. Spring A #3

More information

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

The Earth & its good friend, the Moon. SNC1D7 - Space The Earth & its good friend, the Moon SNC1D7 - Space Key Questions! What causes... day and night? the seasons? the tides? What are eclipses? Let s eat some space oreos! How do we know the Earth is round?

More information

Name: Exam 1, 9/30/05

Name: Exam 1, 9/30/05 Multiple Choice: Select the choice that best answers each question. Write your choice in the blank next to each number. (2 points each) 1. At the North Pole in mid-november, the sun rises at a. North of

More information

ASTRONOMY. S6E1 a, b, c, d, e, f S6E2 a, b, c,

ASTRONOMY. S6E1 a, b, c, d, e, f S6E2 a, b, c, ASTRONOMY S6E1 a, b, c, d, e, f S6E2 a, b, c, UNIVERSE Age 13.7 billion years old The Big Bang Theory Protons and Neutrons formed hydrogen and helium. This created heat that formed the stars. Other elements

More information

Unit 6 Lesson 1 How Do the Sun, Earth, and Moon Interact? Copyright Houghton Mifflin Harcourt Publishing Company

Unit 6 Lesson 1 How Do the Sun, Earth, and Moon Interact? Copyright Houghton Mifflin Harcourt Publishing Company Unit 6 Lesson 1 How Do the Sun, Earth, and Moon Interact? Night and Day Earth rotates, or turns like a top. Earth s rotation causes day and night. Earth rotates around an imaginary line called an axis,

More information

Ch 22 Origin of Modern Astronomy Notes Ch 22.1 Early Astronomers Astronomy Astrology A. Ancient Greece B. Two Basic Theories Existed:

Ch 22 Origin of Modern Astronomy Notes Ch 22.1 Early Astronomers Astronomy Astrology A. Ancient Greece B. Two Basic Theories Existed: Ch 22 Origin of Modern Astronomy Notes Ch 22.1 Early Astronomers Astronomy: The science that studies the universe, dealing with properties of objects in space. Astrology: A belief that the positions of

More information

Effective August 2007 All indicators in Standard / 14

Effective August 2007 All indicators in Standard / 14 8-4.1 Summarize the characteristics and movements of objects in the solar system (including planets, moons, asteroids, comets, and meteors). Taxonomy level: 2.4-B Understand Conceptual Knowledge Previous/Future

More information

PHYS 160 Astronomy Test #1 Fall 2017 Version B

PHYS 160 Astronomy Test #1 Fall 2017 Version B PHYS 160 Astronomy Test #1 Fall 2017 Version B 1 I. True/False (1 point each) Circle the T if the statement is true, or F if the statement is false on your answer sheet. 1. An object has the same weight,

More information

Introduction To Modern Astronomy II

Introduction To Modern Astronomy II ASTR 111 003 Fall 2006 Lecture 03 Sep. 18, 2006 Introduction To Modern Astronomy II Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch1: Astronomy and the Universe Ch2: Knowing the Heavens

More information

D. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified

D. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified ASTRONOMY 1 EXAM 1 Name Identify Terms - Matching (20 @ 1 point each = 20 pts.) 1 Solar System G 7. aphelion N 14. eccentricity M 2. Planet E 8. apparent visual magnitude R 15. empirical Q 3. Star P 9.

More information

18.2 Earth Cycles Days and years Calendars Years and days Leap years Calendars throughout human history 20,000 years ago. 7,000 BC. 4,000 BC.

18.2 Earth Cycles Days and years Calendars Years and days Leap years Calendars throughout human history 20,000 years ago. 7,000 BC. 4,000 BC. 18.2 Reading 18.2 Earth Cycles Do you ever wonder where our calendar comes from? Or why the Moon gradually changes its shape? Or why we have seasons? The answers have to do with the relative positions

More information

Astronomy, PART 2. Vocabulary. A. Universe - Our Milky Way Galaxy is one of of galaxies in an expanding universe.

Astronomy, PART 2. Vocabulary. A. Universe - Our Milky Way Galaxy is one of of galaxies in an expanding universe. Astronomy, PART 2 Vocabulary Aphelion Asteroid Astronomical Unit Comet Constellation Crater Eccentricity Eclipse Equinox Geocentric model Gravitation Heliocentric model Inertia Jovian Perihelion Revolution

More information

Earth in Space Chapter 1

Earth in Space Chapter 1 Earth in Space Chapter 1 Section 1 Earth in Space How does Earth move in space? What causes the cycle of seasons on Earth? How the Earth Moves The study of the moon, stars, and other objects in space is

More information

Moon, Planet, Star, Solar System, Galaxy, Universe

Moon, Planet, Star, Solar System, Galaxy, Universe Dr. V s Study Guide : Astronomy Unit 1) Place the following in order of increasing size: The Galaxy, the Solar System, a Star, the Universe,a Moon and a Planet. Moon, Planet, Star, Solar System, Galaxy,

More information

because you asked for it just one more set of MOON REVIEW questions

because you asked for it just one more set of MOON REVIEW questions because you asked for it just one more set of MOON REVIEW questions 1. The diagram below shows the Moon as it revolves around Earth. The numbered locations represent different positions of the Moon in

More information

Astronomy 11. No, this course isn t all about Star Wars

Astronomy 11. No, this course isn t all about Star Wars Astronomy 11 No, this course isn t all about Star Wars Earth s Rotation How fast are people on the equator moving? s=d/t =circumference/24 hours =(40,000 km)/24 hours =1670 km/h That s Mach 1.4! What

More information

Most of the time during full and new phases, the Moon lies above or below the Sun in the sky.

Most of the time during full and new phases, the Moon lies above or below the Sun in the sky. 6/16 Eclipses: We don t have eclipses every month because the plane of the Moon s orbit about the Earth is different from the plane the ecliptic, the Earth s orbital plane about the Sun. The planes of

More information

EARTH SCIENCE UNIT 9 -NOTES ASTRONOMY

EARTH SCIENCE UNIT 9 -NOTES ASTRONOMY EARTH SCIENCE UNIT 9 -NOTES ASTRONOMY UNIT 9- ASTRONOMY 2 THE SOLAR SYSTEM I. The Solar System:. a. Celestial Body:. i. Examples:. b. MAIN COMPONENTS/MEMBERS OF THE SOLAR SYSTEM: i. 1. Planets are objects

More information

The Moon. A look at our nearest neighbor in Space! Free powerpoints at

The Moon. A look at our nearest neighbor in Space! Free powerpoints at The Moon A look at our nearest neighbor in Space! Free powerpoints at http://www.worldofteaching.com What is the Moon? A natural satellite One of more than 96 moons in our Solar System The only moon of

More information

1. The pictures below show the Sun at midday. Write winter, spring or summer under the correct picture.

1. The pictures below show the Sun at midday. Write winter, spring or summer under the correct picture. Test 2 1. The pictures below show the Sun at midday. Write winter, spring or summer under the correct picture. 2. Look carefully at the phases of the Moon. Number them (1 to 4) in the order that you would

More information

Term Info Picture. A celestial body that orbits a bigger celestial body (a moon) Earth s only natural satellite. It causes all of the tides.

Term Info Picture. A celestial body that orbits a bigger celestial body (a moon) Earth s only natural satellite. It causes all of the tides. Astronomy (Earth, Moon and Sun) S6E2. Obtain, evaluate, and communicate information about the effets of the relative positions of the sun, Earth and moon. A. Develop and use a model to demonstrate the

More information

Investigations in Earth and Space Science Semester Review: Unit 1 and Unit 2

Investigations in Earth and Space Science Semester Review: Unit 1 and Unit 2 IESS Unit 1: Solar Energy & Fluid Circulation Review Directions: Write the answer to each question in the box to the right of the question. Fold your paper along the line and use this as a review sheet!

More information

Unit 2: Celestial Mechanics

Unit 2: Celestial Mechanics Unit 2: Celestial Mechanics The position of the Earth Ptolemy (90 168 AD) Made tables that allowed a user to locate the position of a planet at any past, present, or future date. In order to maintain circular

More information

TIDES. A tide just after the first or third quarters of the moon There is the least difference between high and low water Spring Tides

TIDES. A tide just after the first or third quarters of the moon There is the least difference between high and low water Spring Tides TIDES Earth and Moon Interaction The Earth is pulled to the Sun by gravity. The moon is pulled to the Earth by gravity. The moon s gravity effects the Earth s tides. Neap Tides A tide just after the first

More information

2.1 Patterns in the Night Sky

2.1 Patterns in the Night Sky 2.1 Patterns in the Night Sky Our goals for learning: What are constellations? How do we locate objects in the sky? Why do stars rise and set? Why don t we see the same constellations throughout the year?

More information

THE SUN-EARTH-MOON SYSTEM

THE SUN-EARTH-MOON SYSTEM Date Period Name THE SUN-EARTH-MOON SYSTEM SECTION 27.1 Tools of Astronomy In your textbook, read about electromagnetic radiation and telescopes. Use each of the terms below just once to complete the passage.

More information

What is in outer space?

What is in outer space? What is in outer space? Celestial Objects are any natural objects that move through space. Star:_a huge sphere of gas in space _Nuclear fusion within stars give off enormous amounts of energy such as light

More information

12.1 Earth, Moon and Sun Interactions

12.1 Earth, Moon and Sun Interactions 12.1 Earth, Moon and Sun Interactions Humans have been aware of the relationships between the Earth, Sun and Moon for thousands of years, but only recently have we began to better understand the true nature

More information

3) During retrograde motion a planet appears to be A) dimmer than usual. B) the same brightness as usual C) brighter than usual.

3) During retrograde motion a planet appears to be A) dimmer than usual. B) the same brightness as usual C) brighter than usual. Descriptive Astronomy (ASTR 108) Exam 1 B February 17, 2010 Name: In each of the following multiple choice questions, select the best possible answer. In the line on the scan sheet corresponding to the

More information

1) Kepler's third law allows us to find the average distance to a planet from observing its period of rotation on its axis.

1) Kepler's third law allows us to find the average distance to a planet from observing its period of rotation on its axis. Descriptive Astronomy (ASTR 108) Exam 1 A February 17, 2010 Name: In each of the following multiple choice questions, select the best possible answer. In the line on the scan sheet corresponding to the

More information

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

A) M D) The Moon s distance from Earth varies in a cyclic manner. Base your answers to questions 1 and 2 on the diagram below, which shows Earth in orbit around the Sun, and the Moon in orbit around Earth. M 1, M 2, M 3, and M 4 indicate positions of the Moon in its

More information

The reason is that the Moon s rotation takes 27.3 days the same amount of time it takes to revolve once around Earth. Because these two motions take

The reason is that the Moon s rotation takes 27.3 days the same amount of time it takes to revolve once around Earth. Because these two motions take Moon Phases 6.E.1.1 Explain how the relative motion and relative position of the sun, Earth and moon affect the seasons, tides, phases of the moon, and eclipses. Motions of the Moon Just as Earth rotates

More information

Gravity. Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields

Gravity. Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields Gravity Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields Simulation Synchronous Rotation https://www.youtube.com/watch?v=ozib_l eg75q Sun-Earth-Moon System https://vimeo.com/16015937

More information

Chapter 17. Chapter 17

Chapter 17. Chapter 17 Chapter 17 Moons and Other Solar System Objects Sections 17.1-17.2 Chapter 17 Parallax http://www.youtube.com/watc h?v=xuqaildqpww The Moon July 20, 1969 humans first landed on moon What was the first

More information

Explain how Earth's movement and the moon's orbit cause the phases of the moon. Explain the difference between a solar eclipse and a lunar eclipse.

Explain how Earth's movement and the moon's orbit cause the phases of the moon. Explain the difference between a solar eclipse and a lunar eclipse. Explain how Earth's movement and the moon's orbit cause the phases of the moon. Explain the difference between a solar eclipse and a lunar eclipse. The Earth- Moon System Have you ever wondered why the

More information

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

18.1 Earth and Its Moon Earth s shape and orbit Earth s shape Earth s orbit around the Sun 18.1 Earth and Its Moon Revolving around Earth at a distance of 384,400 kilometers is our only moon. Since the invention of spacecraft, our knowledge of Earth and the Moon has grown tremendously. In fact,

More information

Define umbra and penumbra. Then label the umbra and the penumbra on the diagram below. Umbra: Penumbra: Light source

Define umbra and penumbra. Then label the umbra and the penumbra on the diagram below. Umbra: Penumbra: Light source Lesson 3 Eclipses and Tides LA.8.2.2.3, SC.8.E.5.9, SC.8.N.1.1 Skim or scan the heading, boldfaced words, and pictures in the lesson. Identify or predict three facts you will learn from the lesson. Discuss

More information

Topic 10: Earth in Space Workbook Chapters 10 and 11

Topic 10: Earth in Space Workbook Chapters 10 and 11 Topic 10: Earth in Space Workbook Chapters 10 and 11 We can imagine all the celestial objects seen from Earth the sun, stars, the Milky way, and planets as being positioned on a celestial sphere. Earth

More information

In the beginning. Origin of Modern Astronomy Ch 22. Early Astronomy Early Astronomy/ Ancient Greece

In the beginning. Origin of Modern Astronomy Ch 22. Early Astronomy Early Astronomy/ Ancient Greece In the beginning Origin of Modern Astronomy Ch 22 GOD created the HEAVENS and the EARTH. (Gen. 1:1) 22.1 Early Astronomy/ Ancient Greece Astronomy: The science that studies the universe, dealing with properties

More information

Basics of Kepler and Newton. Orbits of the planets, moons,

Basics of Kepler and Newton. Orbits of the planets, moons, Basics of Kepler and Newton Orbits of the planets, moons, Kepler s Laws, as derived by Newton. Kepler s Laws Universal Law of Gravity Three Laws of Motion Deriving Kepler s Laws Recall: The Copernican

More information

The Sun-Earth-Moon System. Learning Guide. Visit for Online Learning Resources. Copyright NewPath Learning

The Sun-Earth-Moon System. Learning Guide. Visit  for Online Learning Resources. Copyright NewPath Learning The Sun-Earth-Moon System Learning Guide Visit www.newpathlearning.com for Online Learning Resources. Copyright NewPath Learning Table of Contents Lesson 1 - How the Earth Moves... 2 Lesson 2 - Seasons

More information

Earth in the Universe

Earth in the Universe Earth in the Universe Date: 6.E.1 Understand the earth/moon/sun system, and the properties, structures, and predictable motions of celestial bodies in the Universe. 6.E.1.1 Explain how the relative motion

More information

The Sun-Earth-Moon System

The Sun-Earth-Moon System Name The Sun-Earth-Moon System Section 28.3 The Sun-Earth-Moon System Date Main Idea Details Read the title of Section 3. List three things that might be discussed in this section. 1. 2. 3. Review Vocabulary

More information

Name Period Date Earth and Space Science. Solar System Review

Name Period Date Earth and Space Science. Solar System Review Name Period Date Earth and Space Science Solar System Review 1. is the spinning a planetary object on its axis. 2. is the backward motion of planets. 3. The is a unit less number between 0 and 1 that describes

More information

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009 Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009 Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. Mark answer on Scantron.

More information

Ch. 22 Origin of Modern Astronomy Pretest

Ch. 22 Origin of Modern Astronomy Pretest Ch. 22 Origin of Modern Astronomy Pretest Ch. 22 Origin of Modern Astronomy Pretest 1. True or False: Early Greek astronomers (600 B.C. A.D. 150) used telescopes to observe the stars. Ch. 22 Origin of

More information

1 Describe the structure of the moon 2. Describe its surface features 3. Summarize the hypothesis of moon formation

1 Describe the structure of the moon 2. Describe its surface features 3. Summarize the hypothesis of moon formation Loulousis 1 Describe the structure of the moon 2. Describe its surface features 3. Summarize the hypothesis of moon formation moon -a body that revolves around a planet and that has less mass than the

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

d. Galileo Galilei i. Heard about lenses being used to magnify objects 1. created his own telescopes to 30 power not the inventor! 2. looked

d. Galileo Galilei i. Heard about lenses being used to magnify objects 1. created his own telescopes to 30 power not the inventor! 2. looked 1. Age of Reason a. Nicolaus Copernicus 1473-1543 i. Commenteriolus manuscript circulated from 1512 1. unpublished 2. Heliocentric hypothesis ii. On the Revolutions of the Planets published year of his

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

Introduction To Modern Astronomy I

Introduction To Modern Astronomy I ASTR 111 003 Fall 2006 Lecture 03 Sep. 18, 2006 Introduction To Modern Astronomy I Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch1: Astronomy and the Universe Ch2: Knowing the Heavens

More information

After you read this section, you should be able to answer these questions:

After you read this section, you should be able to answer these questions: CHAPTER 16 4 Moons SECTION Our Solar System California Science Standards 8.2.g, 8.4.d, 8.4.e BEFORE YOU READ After you read this section, you should be able to answer these questions: How did Earth s moon

More information

Earth Science, 13e Tarbuck & Lutgens

Earth Science, 13e Tarbuck & Lutgens Earth Science, 13e Tarbuck & Lutgens Origins of Modern Astronomy Earth Science, 13e Chapter 21 Stanley C. Hatfield Southwestern Illinois College Early history of astronomy Ancient Greeks Used philosophical

More information

Topic 1: Earth s Motion Topic 2: The Moon Earth s Satellite Topic 3: Solar System Topic 4: The Planets Topic 5: Stars & Galaxies

Topic 1: Earth s Motion Topic 2: The Moon Earth s Satellite Topic 3: Solar System Topic 4: The Planets Topic 5: Stars & Galaxies Topic 1: Earth s Motion Topic 2: The Moon Earth s Satellite Topic 3: Solar System Topic 4: The Planets Topic 5: Stars & Galaxies Topic 1: Earth s Motion Essential Question: What causes the cycle of seasons

More information

Position 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set.

Position 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set. Position 3 None - it is always above the horizon. N E W S Agree with student 2; star B never crosses horizon plane, so it can t rise or set. Imaginary plane No; the Earth blocks the view. Star A at position

More information

Create a bulleted list of everything you know about the moon!

Create a bulleted list of everything you know about the moon! The Moon Create a bulleted list of everything you know about the moon! If given the opportunity, would you want to go to the moon? A. YES! That would be really cool. B. NO! Why would anyone want to go

More information

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

Brock University. Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014 Brock University Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014 Number of hours: 50 min Time of Examination: 18:00 18:50 Instructor:

More information

lightyears observable universe astronomical unit po- laris perihelion Milky Way

lightyears observable universe astronomical unit po- laris perihelion Milky Way 1 Chapter 1 Astronomical distances are so large we typically measure distances in lightyears: the distance light can travel in one year, or 9.46 10 12 km or 9, 600, 000, 000, 000 km. Looking into the sky

More information

Announcements. Topics To Be Covered in this Lecture

Announcements. Topics To Be Covered in this Lecture Announcements! Tonight s observing session is cancelled (due to clouds)! the next one will be one week from now, weather permitting! The 2 nd LearningCurve activity was due earlier today! Assignment 2

More information

Astronomy Practice Test

Astronomy Practice Test Name: ate: 1. In laska, there are fewer hours of daylight in the winter than in the summer. Which statement best explains why this difference occurs?. The Sun burns hotter in the summer.. The Sun moves

More information

Guided Notes Astronomy. Earth s Moon Formation Orbit Craters Motions Phases Tides Eclipses

Guided Notes Astronomy. Earth s Moon Formation Orbit Craters Motions Phases Tides Eclipses Guided Notes Astronomy Earth s Moon Formation Orbit Craters Motions Phases Tides Eclipses K. Coder 2015 1. What is the Moon? The Moon: the Earth's only natural satellite. See ESRT page 15 for data on Earth

More information

Chapter 23: The Sun-Earth-Moon System. Grade 6 Earth Science Mr. Norton

Chapter 23: The Sun-Earth-Moon System. Grade 6 Earth Science Mr. Norton Chapter 23: The Sun-Earth-Moon System Grade 6 Earth Science Mr. Norton Chapter 23: The Sun-Earth-Moon System Section 1: Earth Section 2: The Moon Earth s Satellite Section 3: Exploring Earth s Moon Chapter

More information

Name Date Class. Phases of the Moon

Name Date Class. Phases of the Moon Name Date Class Chapter 1 PAGE KEELEY SCIENCE PROBES Many people have different ideas about what causes us to see different parts of the Moon (moon phases). Which idea below best matches your thinking?

More information

Name and Student ID Section Day/Time:

Name and Student ID Section Day/Time: AY2 - Overview of the Universe - Midterm #1 - Instructor: Maria F. Duran Name and Student ID Section Day/Time: 1) Imagine we ve discovered a planet orbiting another star at 1 AU every 6 months. The planet

More information

How Astronomers Learnt that The Heavens Are Not Perfect

How Astronomers Learnt that The Heavens Are Not Perfect 1 How Astronomers Learnt that The Heavens Are Not Perfect Introduction In this packet, you will read about the discoveries and theories which changed the way astronomers understood the Universe. I have

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

The Cause of the Seasons

The Cause of the Seasons The Cause of the Seasons Summer Winter Seasons are caused by the Earth s axis tilt, not the distance from the Earth to the Sun! Axis tilt changes directness of sunlight during the year. Why Does Flux Sunlight

More information

Test 1 Review Chapter 1 Our place in the universe

Test 1 Review Chapter 1 Our place in the universe Test 1 Review Bring Gator 1 ID card Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the scantrons Formulas will be projected on the screen You can use

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

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

Full Moon. Phases of the Moon

Full Moon. Phases of the Moon Phases of the Moon The Moon takes 29.5 days to orbit Earth. This is a lunar month. The gravity of the Earth keeps the Moon in orbit. The Moon does not produce light. We see the Moon because it reflects

More information

Earth in the Universe

Earth in the Universe Earth in the Universe 6.E.1 Understand the earth/moon/sun system, and the properties, structures, and predictable motions of celestial bodies in the Universe. 6.E.1.1 Explain how the relative motion and

More information