Chapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Pearson Education, Inc.

Similar documents
Stars. 1.1 A Modern View of the Universe. What Objects Do We Find in The Universe? 8/12/2010. Our goals for learning:

Chapter 1 Our Place in the Universe. Copyright 2012 Pearson Education, Inc.

9/5/16. Astronomy 1001 Syllabus Sec 1 T,Th AM; Sec 2 T,TH PM. Astronomy 1001 First Assignments: Chapter 1: A Modern View of the Universe

Chapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe

Star. Planet. Chapter 1 Our Place in the Universe. 1.1 A Modern View of the Universe Our goals for learning: What is our place in the universe?

Chapter 1 Our Place in the Universe

Star. Chapter 1: Our Place in the Universe. 1.1 A Modern View of the Universe Our goals for learning:

AST 103 Ch.1 Our Place in the Universe #2. Prof. Ken Nagamine Dept. of Physics & Astronomy UNLV

Bell Ringer. want to do someday? 1. Briefly describe the Doppler effect in one sentence. 2. What do you want to do someday, like, in life?

Plan. Questions? Syllabus; administrative details. Some Definitions. An Idea of Scale

AST 103 The Solar System

Required Material. Required Material. Pre-Course Assessment 1/27/09. Textbook: The Cosmic Perspective, 5 th edition by Bennett et al.

Required Material. Required Material 1/27/09. Textbook: The Cosmic Perspective, 5 th edition by Bennett et al.

Our Place in the Universe (Chapter 1) The Structure and Size of the Universe

Lecture 3: Chapter 1- Charting the Heavens. Assignment: Read Chapter 1 of Astronomy Today

Measures of Astronomical Distances. Measures of Astronomical Distances

Chapter 1 Review Clickers. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Pearson Education, Inc.

What is the solar system?

THE SIZE AND STRUCTURE OF THE UNIVERSE

The Universe and Galaxies. Adapted from:

Welcome Aboard!! CHANGE OF KOMATSU S OFFICE HOURS. Briefing Welcome to the Cosmic Tour: Some Guide Lines. Lecture 1 Our Place in the Universe

The Universe and Galaxies

Back of chapters have additional Resources and various tutorials to help you getting acquainted With the subject Also exercises you can do for extra

Universe Celestial Object Galaxy Solar System

Lecture 2: A Modern View of the Universe!

LESSON 1. Solar System

Introduction to Astronomy

TAKEN FROM HORIZONS 7TH EDITION CHAPTER 1 TUTORIAL QUIZ

Phys 214. Planets and Life

Phys 214. Planets and Life

o Terms to know o Big Bang Theory o Doppler Effect o Redshift o Universe

Answers. The Universe. Year 10 Science Chapter 6

Test Name: 09.LCW.0352.SCIENCE.GR Q1.S.THEUNIVERSE-SOLARSYSTEMHONORS Test ID: Date: 09/21/2017

A Cosmic Perspective. Scott Fisher, Ph.D. - Director of Undergraduate Studies - UO Department of Physics

PHYS 101: Elementary Astronomy. Dr. Jared Workman

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 1

Homework. Our Home World! Nights for 1 st Class Sky Observation Exercise (field near Leeds Business School)

A MODERN VIEW OF THE UNIVERSE

Miami Dade County Public Schools Educational Transformation Office and the Division of Academics: Department of Science

The Earth and the Universe

AY2 Introduction to Astronomy Winter quarter, 2013

ASTRONOMY 202 Spring 2007: Solar System Exploration

The Universe. Unit 3 covers the following framework standards: ES 8 and 12. Content was adapted the following:

Modern Astronomy Review #1

Cosmic Landscape Introduction Study Notes

Our Place in the Universe

Figure 19.19: HST photo called Hubble Deep Field.

A Modern View of the Universe

ISP205-2 Visions of the Universe

The Age of the Universe If the entire age of the Universe were 1 calendar year, then 1 month would be equivalent to roughly 1 billion years

Introduction to the Universe

CST Prep- 8 th Grade Astronomy

The Solar System. Sun. Rotates and revolves around the Milky Way galaxy at such a slow pace that we do not notice any effects.

LESSON topic: formation of the solar system Solar system formation Star formation Models of the solar system Planets in our solar system

A100H Exploring the Universe: Introduction. Martin D. Weinberg UMass Astronomy

A Modern View of the Universe

Start with known facts and reasonable guesses. More on order of magnitude Astronomy How many piano tuners are there in Boulder County?

Beyond Our Solar System Chapter 24

Introduction to the Universe. What makes up the Universe?

Astronomy. Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe.

A100 Exploring the Universe: Introduction. Martin D. Weinberg UMass Astronomy

Where in the Solar System Are Smaller Objects Found?

What Objects Are Part of the Solar System?

1UNIT. The Universe. What do you remember? Key language. Content objectives

Astronomy 1. 10/17/17 - NASA JPL field trip 10/17/17 - LA Griffith Observatory field trip

UNIT 1: EARTH AND THE SOLAR SYSTEM.

An Introduction to AST 112 Stars, Galaxies, and the Cosmos

Science Benchmark: 06 : 04 Standard 04: Stargazing universe, the light-year, speed of light Grade Benchmark Standard Page

Planetarium observing is over. Nighttime observing starts next week.

Stars and Galaxies 1

The Outer Planets. Video Script: The Outer Planets. Visual Learning Company

Writing very large numbers

Our Solar System. Lesson 5. Distances Between the Sun and the Planets

Cambridge University Press Origins of Life in the Universe Robert Jastrow and Michael Rampino Excerpt More information PART I

WHAT WE KNOW. Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So..

2. The distance between the Sun and the next closest star, Proxima Centuari, is MOST accurately measured in

Learning About Our Solar System

Chapter 23: Touring Our Solar System

The Formation of the Solar System

21/11/ /11/2017 Space Physics AQA Physics topic 8

Unit 1: The Earth in the Universe

It is a very human trait to wonder where we are in this universe. Usually, the only hint of the vastness of the universe comes at night.

THE UNIVERSE AND THE EARTH

Today. A little more scale... The Scientific Method. Naked Eye Observations: the Appearance of the Sky

Chapter 06 Let s Make a Solar System

Earth s Formation Unit [Astronomy] Student Success Sheets (SSS)

Nucleus Hydrogen nucleus. hydrogen. helium

Astronomy Unit Notes Name:

Astronomy 9 Concepts of the Cosmos

Outline. Question of Scale. Planets Dance. Homework #2 was due today at 11:50am! It s too late now.

The Big Bang Theory (page 854)

28-Aug-17. A Tour of Our Solar System and Beyond. The Sun

How did it come to be this way? Will I stop sounding like the

Which letter on the timeline best represents the time when scientists estimate that the Big Bang occurred? A) A B) B C) C D) D

The color of a star provides a measure of its A. size B. mass C. composition D. surface temperature

10.1 The Early Universe

V. Astronomy Section

Prentice Hall EARTH SCIENCE

The Earth in the Universe Geology

Starting from closest to the Sun, name the orbiting planets in order.

Transcription:

Chapter 1 Lecture The Cosmic Perspective Seventh Edition A Modern View of the Universe

Chapter Opener

1.1 The Scale of the Universe Our goals for learning: What is our place in the universe? How big is the universe?

What is our place in the universe?

Star A large, glowing ball of gas that generates heat and light through nuclear fusion

Planet Mars Neptune A moderately large object that orbits a star; it shines by reflected light. Planets may be rocky, icy, or gaseous in composition.

Moon (or Satellite) An object that orbits a planet Ganymede (orbits Jupiter)

Asteroid A relatively small and rocky object that orbits a star

Comet A relatively small and icy object that orbits a star

Solar (Star) System A star and all the material that orbits it, including its planets and moons

Nebula An interstellar cloud of gas and/or dust

Galaxy A great island of stars in space, all held together by gravity and orbiting a common center M31, the great galaxy in Andromeda

Universe The sum total of all matter and energy; that is, everything within and between all galaxies

Far away means back in time? Light travels at a finite speed (300,000 km/s). Destination Light travel time Moon Sun Sirius Andromeda Galaxy 1 second 8 minutes 8 years 2.5 million years Thus, we see objects as they were in the past: The farther away we look in distance, the further back we look in time.

Far away means back in time? Example: We see the Orion Nebula as it looked 1500 years ago.

Far away means back in time? Example: This photo shows the Andromeda Galaxy as it looked about 2 1/2 million years ago. Question: When will we be able to see what it looks like now?

Light-year The distance light can travel in 1 year About 10 trillion kilometers (6 trillion miles)

Light-year At great distances, we see objects as they were when the universe was much younger.

How far is a light-year? 1light-year = (speed of light) (1 year) km 365 days 24 hr 60 min 60 s = 300,000 s 1 yr 1 day 1 hr 1 min

How far is a light-year? 1light-year = (speed of light) (1 year) km 365 days 24 hr 60 min 60 s = 300,000 s 1 yr 1 day 1 hr 1 min =9,460,000,000,000 km

Can we see the entire universe?

Thought Question Why can't we see a galaxy 15 billion light-years away? (Assume the universe is 14 billion years old.) A. Because no galaxies exist at such a great distance. B. Galaxies may exist at that distance, but their light would be too faint for our telescopes to see. C. Because looking 15 billion light-years away means looking to a time before the universe existed.

Thought Question Why can't we see a galaxy 15 billion light-years away? (Assume the universe is 14 billion years old.) A. Because no galaxies exist at such a great distance. B. Galaxies may exist at that distance, but their light would be too faint for our telescopes to see. C. Because looking 15 billion light-years away means looking to a time before the universe existed.

What have we learned? What is our place in the universe? Earth is part of the solar system, which is the Milky Way Galaxy, which is a member of the Local Group of galaxies in the Local Supercluster.

How big is Earth compared to our solar system? Let's reduce the size of the solar system by a factor of 10 billion; the Sun is now the size of a large grapefruit (14 cm diameter). How big is Earth on this scale? A. an atom B. a ball point C. a marble D. a golf ball

How big is Earth compared to our solar system? Let's reduce the size of the solar system by a factor of 10 billion; the Sun is now the size of a large grapefruit (14 cm diameter). How big is Earth on this scale? A. an atom B. a ball point C. a marble D. a golf ball

The scale of the solar system On a 1-to-10- billion scale: The Sun is the size of a large grapefruit (14 cm). Earth is the size of a ball point, 15 meters away.

How far away are the stars? On our 1-to-10-billion scale, it's just a few minutes' walk to Pluto. How far would you have to walk to reach Alpha Centauri? A. 1 mile B. 10 miles C. 100 miles D. the distance across the United States (2500 miles)

How far away are the stars? Answer: D, the distance across the United States

How big is the Milky Way Galaxy? The Milky Way has about 100 billion stars. On the same 1- to-10-billion scale, how big is the Milky Way?

Thought Question Suppose you tried to count the more than 100 billion stars in our galaxy, at a rate of one per second. How long would it take you? A. a few weeks B. a few months C. a few years D. a few thousand years

Thought Question Suppose you tried to count the more than 100 billion stars in our galaxy, at a rate of one per second. How long would it take you? A. a few weeks B. a few months C. a few years D. a few thousand years

How big is the universe? The Milky Way is one of about 100 billion galaxies. 10 11 stars/galaxy x 10 11 galaxies = 10 22 stars There are as many stars as grains of (dry) sand on all Earth's beaches.

How big is the universe? Now let's step through the universe in powers of 10:

What have we learned? How big is the universe? The distances between planets are huge compared to their sizes on a scale of 1-to-10-billion, Earth is the size of a ball point and the Sun is 15 meters away. On the same scale, the stars are thousands of kilometers away. It would take more than 3000 years to count the stars in the Milky Way Galaxy at a rate of one per second, and they are spread across 100,000 light-years. The observable universe is 14 billion light-years in radius and contains over 100 billion galaxies with a total number of stars comparable to the number of grains of sand on all of Earth's beaches.

1.2 The History of the Universe Our goals for learning: How did we come to be? How do our lifetimes compare to the age of the universe?

How did we come to be?

How do our lifetimes compare to the age of the universe? The cosmic calendar: a scale on which we compress the history of the universe into 1 year.

What have we learned? How did we come to be? The matter in our bodies came from the Big Bang, which produced hydrogen and helium. All other elements were constructed from H and He in stars and then recycled into new star systems, including our solar system. How do our lifetimes compare to the age of the universe? On a cosmic calendar that compresses the history of the universe into 1 year, human civilization is just a few seconds old, and a human lifetime is a fraction of a second.

1.3 Spaceship Earth Our goals for learning: How is Earth moving through space? How do galaxies move within the universe?

How is Earth moving through space? Contrary to our perception, we are not "sitting still." We are moving with Earth in several ways, and at surprisingly fast speeds. The Earth rotates around its axis once every day.

How is Earth moving through space? Earth orbits the Sun (revolves) once every year: at an average distance of 1 AU 150 million kilometers. with Earth's axis tilted by 23.5º (pointing to Polaris) It rotates in the same direction it orbits, counterclockwise as viewed from above the North Pole.

How is our Sun moving in in the Milky Way Galaxy? Our Sun moves randomly relative to the other stars in the local solar neighborhood typical relative speeds of more than 70,000 km/hr but stars are so far away that we cannot easily notice their motion and orbits the galaxy every 230 million years.

How is our Sun moving in in the Milky Way Galaxy? More detailed study of the Milky Way's rotation reveals one of the greatest mysteries in astronomy:

How do galaxies move within the universe? Galaxies are carried along with the expansion of the universe. But how did Hubble figure out that the universe is expanding?

Hubble discovered that All galaxies outside our Local Group are moving away from us. The more distant the galaxy, the faster it is racing away. Conclusion: We live in an expanding universe.

Are we ever sitting still?

What have we learned? How is Earth moving through space? It rotates on its axis once a day and orbits the Sun at a distance of 1 AU = 150 million kilometers. Stars in the Local Neighborhood move randomly relative to one another and orbit the center of the Milky Way in about 230 million years.

What have we learned? How do galaxies move within the universe? All galaxies beyond the Local Group are moving away from us with expansion of the universe: the more distant they are, the faster they're moving.

1.4 The Human Adventure of Astronomy Our goals for learning: How has the study of astronomy affected human history?

How has the study of astronomy affected human history? The Copernican revolution showed that Earth was not the center of the universe (Chapter 3). Study of planetary motion led to Newton's laws of motion and gravity (Chapter 4). Newton's laws laid the foundation of the industrial revolution. Modern discoveries are continuing to expand our "cosmic perspective."

What have we learned? How has the study of astronomy affected human history? Throughout history, astronomy has provided an expanded perspective on Earth that has grown hand in hand with social and technological developments.