Chapter 1: Our Place in the Universe. 2005 Pearson Education Inc., publishing as Addison-Wesley



Similar documents
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

ASTR 115: Introduction to Astronomy. Stephen Kane

Scale of the Solar System. Sizes and Distances: How Big is Big? Sizes and Distances: How Big is Big? (Cont.)

Introduction to the Solar System

A Modern View of the Universe

NOTES: GEORGIA HIGH SCHOOL SCIENCE TEST THE SOLAR SYSTEM

Week 1-2: Overview of the Universe & the View from the Earth

1 A Solar System Is Born

Chapter 7 Our Planetary System. Agenda. Intro Astronomy. Intro Astronomy. What does the solar system look like? A. General Basics

Asteroids. Earth. Asteroids. Earth Distance from sun: 149,600,000 kilometers (92,960,000 miles) Diameter: 12,756 kilometers (7,926 miles) dotted line

A.4 The Solar System Scale Model

DESCRIPTION ACADEMIC STANDARDS INSTRUCTIONAL GOALS VOCABULARY BEFORE SHOWING. Subject Area: Science

So What All Is Out There, Anyway?

Summary: Four Major Features of our Solar System

UNIT V. Earth and Space. Earth and the Solar System

The Layout of the Solar System

Chapter 7 Our Planetary System. What does the solar system look like? Thought Question How does the Earth-Sun distance compare with the Sun s radius

Size and Scale of the Universe

Unit 8 Lesson 2 Gravity and the Solar System

The Solar System. Source

Page. ASTRONOMICAL OBJECTS (Page 4).

165 points. Name Date Period. Column B a. Cepheid variables b. luminosity c. RR Lyrae variables d. Sagittarius e. variable stars

The Expanding Universe

STUDY GUIDE: Earth Sun Moon

LER Ages. Grades. Solar System. A fun game of thinking & linking!

The Solar System: Cosmic encounter with Pluto

4 HOW OUR SOLAR SYSTEM FORMED 890L

Study Guide: Solar System

The Solar System. Unit 4 covers the following framework standards: ES 10 and PS 11. Content was adapted the following:

4 HOW OUR SOLAR SYSTEM FORMED 1020L

THE SOLAR SYSTEM - EXERCISES 1

Cosmic Journey: A Solar System Adventure General Information

The Main Point. Lecture #34: Solar System Origin II. Chemical Condensation ( Lewis ) Model. How did the solar system form? Reading: Chapter 8.

Science Standard 4 Earth in Space Grade Level Expectations

Georgia Performance Standards Framework for Science Grade 6. Unit Organizer: UNIVERSE AND SOLAR SYSTEM (Approximate Time 3 Weeks)

Solar System Formation

x Distance of the Sun to planet

Lecture 12: The Solar System Briefly

First Discoveries. Asteroids

Chapter 25.1: Models of our Solar System

Lecture 10 Formation of the Solar System January 6c, 2014

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

The Sun and the Stars

4 HOW OUR SOLAR SYSTEM FORMED 750L

Welcome to Class 4: Our Solar System (and a bit of cosmology at the start) Remember: sit only in the first 10 rows of the room

Astronomy Notes for Educators

Background Information Students will learn about the Solar System while practicing communication skills.

The Earth, Sun & Moon. The Universe. The Earth, Sun & Moon. The Universe

Name: João Fernando Alves da Silva Class: 7-4 Number: 10

Lecture 7 Formation of the Solar System. Nebular Theory. Origin of the Solar System. Origin of the Solar System. The Solar Nebula

Group Leader: Group Members:

galaxy solar system supernova (noun) (noun) (noun)

Motions of the Earth. Stuff everyone should know

Chapter 9 Asteroids, Comets, and Dwarf Planets. Their Nature, Orbits, and Impacts

DE2410: Learning Objectives. SOLAR SYSTEM Formation, Evolution and Death. Solar System: To Size Scale. Learning Objectives : This Lecture

THE SOLAR SYSTEM. Worksheets UNIT 1. Raül Martínez Verdún

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

Copyright 2006, Astronomical Society of the Pacific

Voyage: A Journey through our Solar System. Grades Lesson 2: The Voyage Scale Model Solar System

Name Class Date. true

The orbit of Halley s Comet

A SOLAR SYSTEM COLORING BOOK

Our Planetary System. Earth, as viewed by the Voyager spacecraft Pearson Education, Inc.

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015

Chapter 8 Formation of the Solar System Agenda

The facts we know today will be the same tomorrow but today s theories may tomorrow be obsolete.

The scale of the Universe, and an inventory

Grade 6 Standard 3 Unit Test A Astronomy. 1. The four inner planets are rocky and small. Which description best fits the next four outer planets?

Earth in the Solar System

Solar System Fundamentals. What is a Planet? Planetary orbits Planetary temperatures Planetary Atmospheres Origin of the Solar System

California Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping

3 HOW WERE STARS FORMED?

Chapter 8 Formation of the Solar System. What theory best explains the features of our solar system? Close Encounter Hypothesis

Study Guide due Friday, 1/29

Chapter 12 Asteroids, Comets, and Dwarf Planets. Asteroid Facts. What are asteroids like? Asteroids with Moons Asteroids and Meteorites

The Solar System. Olivia Paquette

The Sun and Solar Energy

HONEY, I SHRUNK THE SOLAR SYSTEM

FXA UNIT G485 Module Structure of the Universe. Δλ = v λ c CONTENTS OF THE UNIVERSE. Candidates should be able to :

Class 2 Solar System Characteristics Formation Exosolar Planets

Chapter 8 Welcome to the Solar System

The sun and planets. On this picture, the sizes of the sun and 8 planets are to scale. Their positions relative to each other are not to scale.

The Milky Way Galaxy is Heading for a Major Cosmic Collision

How Big is Our Solar System?

UC Irvine FOCUS! 5 E Lesson Plan

Chapter 6 Formation of Planetary Systems Our Solar System and Beyond

A Universe of Galaxies

5- Minute Refresher: Daily Observable Patterns in the Sky

Exploring Our Solar System Teacher s Guide

Planets and Dwarf Planets by Shauna Hutton

TELESCOPE AS TIME MACHINE

Scientists often deal with

1. Title: Relative Sizes and Distance in the Solar System: Introducing Powers of Ten

RETURN TO THE MOON. Lesson Plan

7 Scale Model of the Solar System

KINDERGARTEN 1 WEEK LESSON PLANS AND ACTIVITIES

Transcription:

Chapter 1: Our Place in the Universe

Topics Our modern view of the universe The scale of the universe Cinema graphic tour of the local universe Spaceship earth

1.1 A Modern View of the Universe Our goals for learning: What is our physical place in the Universe? How did we come to be? How can we know what the Universe was like in the past? Can we see the entire universe?

What is our physical place in the universe? Our Cosmic Address

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

Planet Mars Neptune A moderately large object which 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. Ida

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 The Trifid 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

How did we come to be? Our Cosmic Origins Big bang 14 billion years ago

How can we know what the universe was like in the past? Light travels at a finite speed (300,000 km/s). Destination Moon Sun Sirius Andromeda Galaxy Light travel time 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.

Example: This photo shows the Andromeda Galaxy as it looked about 2 1/2 million years ago. Question: When will be able to see what it looks like now? M31, The Great Galaxy in Andromeda

Definition: a light-year The distance light can travel in one year. About 10 trillion km (6 trillion miles).

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

Can we see the entire universe?

Thought Question Why can t we see a galaxy 15 billion light-years away? (Assume 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 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 is our place in the Universe? Earth orbits the Sun There are 100 billion other stars in the Milky Way There are about 40 other galaxies in the Local Group. What have we learned? The Local Group is part of the Local Supercluster. The Local Supercluster is one small piece of the Universe.

What have we learned? How did we come to be? Big Bang starts the expansion of the universe. Early universe contained only the elements hydrogen and helium. All other elements were made in stars and recycled into new generations of stars within galaxies. We are star stuff

What have we learned? How can we know what the universe was like in the past? Light takes time to travel through space (the speed of light = c = 300,000 km/s). Thus, when we look farther away, we see light that has taken a longer time to reach us. Can we see the entire universe? No - age limits the size of the observable universe. For a 14 billion year old universe, our observable universe is 14 billion light-years in radius.

1.2 The Scale of the Universe Our goals for learning: How big is Earth compared to our solar system? How far away are the stars? How big is the Milky Way Galaxy? How big is the Universe? How do our lifetimes compare to the age of the Universe?

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

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: 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 U.S. (2500 miles)

Answer: D, the distance across the U.S.

How big is the Milky Way Galaxy? The Milky Way has about 100 billion stars. On the same ten billion-toone scale.

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

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 As many stars as grains of (dry) sand on all Earth s beaches

Now let s step through the Universe in powers of 10:

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.

Cosmic Calendar Dec. 17: Cambrian explosion Dec. 16: rise of dinosaurs Dec. 30: extinction of dinosaurs

Cosmic Calendar

What have we learned? How big is the Earth compared to our solar system? On a scale of 1-to-10 billion, the Sun is about the size of a grapefruit. The Earth is the size of a ball point about 15 m away. The distance between planets are huge compared to their sizes. How far away are the stars? On the same scale, the stars are thousands of km away. How big is the Milky Way Galaxy? It would take more than 3,000 years to count the stars in the Milky Way Galaxy at a rate of one per second. The Milky Way Galaxy is about 100,000 light-years across.

What have we learned? How big is the universe? 100 billion galaxies in the observable Universe. 14 billion light-years in radius. As many stars as grains of sand on Earth s beaches. How do our lifetimes compare to the age of the universe? On a cosmic calendar that compresses the history of the Universe into one 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 in our solar system? How is our solar system moving in the Galaxy? How do galaxies move within the Universe? Are we ever sitting still?

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

Earth orbits the Sun (revolves) once every year: at an average distance of 1 AU 150 million km. with Earth s axis tilted by 23.5º (pointing to Polaris) and rotating in the same direction it orbits, counterclockwise as viewed from above the North Pole.

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.

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 in our solar system? Earth rotates on its axis once each day and orbits around the Sun once each year at an average distance of 1 A.U. ( 150 million km).

What have we learned? How is our solar system moving in the Milky Way Galaxy? Stars in the Local Neighborhood move randomly relative to each other. Our Solar System orbits the center of the Milky Way Galaxy about every 230 million years: the entire Galaxy rotates.

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.

What have we learned? Are we ever sitting still? No!