1 The Milky Way Galaxy We live on the quiet outskirts of a galaxy of approximately 100 Billion stars. This galaxy, the Milky Way, is roughly disk-shaped.

Slides:



Advertisements
Similar presentations
Chapter 15: The Milky Way Galaxy
Advertisements

Astro1010-lee.com UVU Survey of Astronomy Chapter 21 Our Milky Way.
Chapter 21: The Milky Way. William Herschel’s map of the Milky Way based on star counts In the early 1800’s William Herschel, the man who discovered the.
Our Galaxy `. Interstellar dust obscures our view at visible wavelengths along lines of sight that lie in the plane of the galactic disk.
ASTR-1020 Stellar Astronomy Day 26. Galaxy Classes.
Objectives: 1.Explain current theories of how galaxies form, and change over time. 2.Know the characteristics of the milky way galaxy. 3.Compare and contrast.
Introduction to Astrophysics Lecture 13: The Milky Way Galaxy.
Chapter 15 The Milky Way Galaxy.
© 2010 Pearson Education, Inc. Chapter 21 Galaxy Evolution.
The Milky Way Galaxy 19 April 2005 AST 2010: Chapter 24.
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 23 Our Galaxy CHAPTER 23 Our Galaxy.
GALAXIES Types Of Galaxies. How Far are Galaxies? Just as stars, galaxies are measured in light years. So what is a light year? Light travels at 186,000.
The Milky Way Center, Shape Globular cluster system
The Milky Way I AST 112 Credit: Stephane Vetter.
The Milky Way Galaxy.
Chapter 12. Final Exam Update Dec. 11 th,2013 Three parts: Part I : test SLO 5 questions. Part II: test SLO 5 questions Part III: Ch. 10,11,12,13,14.
Astronomy The scientific study of matter in outer space, especially the positions, dimensions, distribution, motion, composition, energy, and evolution.
Chapter 21 Section 4 Star Systems And Galaxies. Done By Nick White And Gina Heath.
GALAXIES. A GALAXY IS A massive group of stars held together by their mutual gravity.
Characteristics Of Stars Galaxy: A collection of stars, gases and dust. Universe: Contains billions of galaxies.
Our goals for learning How did Hubble prove galaxies lie beyond our galaxy? How do we observe the life histories of galaxies? How did galaxies form? Why.
Star Systems and Galaxies. hazy band of light stretched across the sky is the Milky Way, a spiral barred galaxy. It looks as if the Milky Way is very.
The Milky Way Galaxy.
The Milky Way Appears as a band of light stretching across the sky There are dark regions along the band, giving the appearance of a lack of stars This.
 Students will be able to determine the size and shape of our galaxy.  Students will be able to distinguish the different kinds of variable stars. 
Unit 1: The Big Picture. What is Astronomy? The study of stars & anything outside Earth –Not astrology…no horoscope reading here! Today we will go over.
Earth Science 25.3 The Universe The Universe. Earth Science 25.3 The Universe  On a clear and moonless night, away from city lights, you can see a marvelous.
Galaxies Cities of Stars.
Galaxies. A galaxy is a large group of stars, dust, and gases. They come in variable sizes and shapes. The largest have over a trillion stars.
1 Galaxies The Andromeda Galaxy - nearest galaxy similar to our own. Only 2 million light years away! Galaxies are clouds of millions to hundreds of billions.
© 2010 Pearson Education, Inc. Chapter 21 Galaxy Evolution.
Galaxies GALAXY -comes from the ancient Greeks and their word for “milk”- galactos.
Galaxies Miss Scillieri 6 th Grade Science Memorial School.
January 2nd 2013 Objective Warm-Up
Galactic Nucleus. Mass of the Galaxy The orbit of clusters can be used to estimate the mass of the galaxy. –Same used for planets and binary stars The.
Chapter 14 The Milky Way Galaxy What do you think? Where in the Milky Way is the solar system located? How fast is the Sun moving in the Milky Way? How.
THE FORMATION OF THE SOLAR SYSTEM. Its all about gravity Gravity can set the particles and dust in a nebula into motion The core of a young star (protostar)
THE MILKY WAY Intro Info.
When Giovanni Riccioli used a telescope like this one to observe a star in the handle of the Big Dipper, he discovered two stars that orbit each other.
Introduction to Galaxies 5/23/2013. BR: Milky Way Scale The Milky Way has a diameter of approximately 8.25 x 10 9 AU (8.25 billion AU). 206,265 AU = 3.26.
Galaxies GALAXIES Stars are not randomly sprinkled throughout the universe. Most astronomers agree that there are about 100 billion galaxies in the universe,
Answer the following question about yesterday’s activity at the bottom of page 21 Explain how you decided how many groups of galaxies you would have. What.
The Milky Way Galaxy. Sky Maps in Different Bands.
“OUR GALAXY” Definition of a Galaxy: a huge group of individual stars, star clusters, dust, and gas bound together by gravity.
UNIT 1 The Milky Way Galaxy.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 14 The Milky Way Galaxy.
Our Milky Way Galaxy. The Milky Way Almost everything we see in the night sky belongs to the Milky Way. We see most of the Milky Way as a faint band of.
Universe Tenth Edition
Our Galaxy Chapter Twenty-Five. Guiding Questions 1.What is our Galaxy? How do astronomers know where we are located within it? 2.What is the shape and.
Chapter 21 Galaxy Evolution Looking Back Through Time Our goals for learning How do we observe the life histories of galaxies? How did galaxies.
Nov 19, 2003Astronomy 100 Fall 2003 Next week is Thanksgiving Break. No homework until you get back. On Friday… Exam 2 Grades are posted. Nighttime observing.
7.2 Galaxies pp
Galaxies. The Hubble Tuning-Fork Diagram This is the traditional scheme for classifying galaxies:
The Milky Way Galaxy. What are each of these?
GALAXIES & BEYOND. What is a galaxy? A galaxy is a very large group of stars held together by gravity. Size: 100,000 ly+ Contain Billions of stars separated.
The Milky Way. The Milky Way: Our Home Galaxy What are the different components of the Milky Way? How do we see those components? What does a map of each.
Formation of the Solar System and The Universe. Our Solar System Sun is the center of a huge rotating system of: Sun is the center of a huge rotating.
Chapter 20: The Milky Way. William Herschel’s map of the Milky Way based on star counts In the early 1800’s William Herschel, the man who discovered the.
The Hubble Ultra Deep Field, or HUDF, catalogs thousands of galaxies in a small section of space in the southern constellation Fornax. Previous versions.
Galaxies.
© 2017 Pearson Education, Inc.
Formation of the Solar System and The Universe
© 2017 Pearson Education, Inc.
Galaxies.
Beyond Our Solar System – The Universe in a Nutshell!
Astronomy-Part 1 Notes The Structure of the Universe
Our Milky Way Galaxy.
When Giovanni Riccioli used a telescope like this one to observe a star in the handle of the Big Dipper, he discovered two stars that orbit each other.
When Giovanni Riccioli used a telescope like this one to observe a star in the Big Dipper, he discovered two stars that orbit each other. A group of stars.
Presentation transcript:

1 The Milky Way Galaxy We live on the quiet outskirts of a galaxy of approximately 100 Billion stars. This galaxy, the Milky Way, is roughly disk-shaped and is about 100,000 light years in diameter. Besides stars the Milky Way also contains enormous clouds of gas and dust The Milky Way as seen from some place on Earth far from city lights.

2 Parts of Our Galaxy Our Galaxy is a spiral galaxy. It is composed of: –a central bulge –a flat disk containing the spiral arms and –a halo of globular clusters there may also exist an extended halo of some unknown material commonly known as “dark matter”.

3 Gas and Dust in our galaxy account for about 15% of its mass. The spiral arms are composed mostly of clusters of bright young stars. The Sun orbits the center of the galaxy with a speed of about 220 kilometers per second. It takes the Sun 240 million years to go around the galaxy one time. The Milky Way as seen in infrared light. Dust and gas in our galaxy prevent us from seeing very far into the galaxy in visible light. In the infrared and radio we can see much farther. Using this information helps us to recognize that we live in a spiral galaxy. More Properties of the Milky Way

4 Learning About the Structure of the Milky Way William Herschel in 1784 recognized that the Sun was in a disk-shaped galaxy of stars. Because of dust and gas blocking the light of distant stars it appeared that the Sun was near the center of the galaxy. This same dust and gas makes it more difficult to observe other galaxies too especially along the disk of our galaxy and towards the center. Top. Herschel’s Map of the Milky Way Bottom. A picture of a dark dust cloud and a star cluster

5 Globular Clusters and the Center of the Galaxy In the 1920s an estimate was made for the size of the galaxy and the position of the Sun within it. It was found that certain dense clusters of stars known as globular clusters tended to be distributed in an elliptical region of space. The center would indicate the center of the galaxy. The Sun was found not to be at the center of this region. Later estimates placed this center at about 28,000 light years away. Globular Clusters contain some of the oldest stars in the galaxy.

6 There are several methods of determining the mass of the Milky Way. Astronomers comparing the estimated mass of all visible matter in the galaxy with the gravitational mass of the galaxy have found that most of the mass is not visible. This is where the theory that the galaxy must contain some kind of “dark matter” comes from. Using the same method used to measure the mass of planets and binary stars we can also use the modified form of Kepler’s 3rd Law to measure the mass of the Milky Way. Using the distance to the center of the galaxy and the orbital period of the Sun the mass of the galaxy is at least Solar masses. This method only measures the mass of the galaxy contained within the orbit of the Sun. Mass of the Milky Way

7 Spiral Arms - Density Waves The arms are traced out by massive bright, young stars. The arms do not “carry” stars with them but are regions of higher density that stars and gas pass through. An excess of mass in the arm exerts a slightly stronger gravitational pull. Clouds pulled into these arms collapse and form stars. Smaller stars live long enough to pass out of the arm as it sweeps by. Massive stars die before leaving the arm

8 Spiral Arms - SSF Another way that spiral arms form is due to supernova explosions of large stars. These explosions trigger the collapse of gas clouds causing new stars to form. The process continues as new large stars explode causing more clouds to collapse. As these stars orbit the galaxy the stars closer in orbit faster and form a spiral shape. This is called self- propagating star formation or SSF.

9 What is Lurking in the Center of Our Galaxy? Near the center of our galaxy there are roughly 10 million stars packed into one cubic light year. In the very center is an object smaller than the size of Jupiter’s orbit but with a mass several million times the mass of the Sun. Since so little light is visible from this object it is thought to be a very large black hole. This is called a supermassive black hole. Most other galaxies are also thought to have these huge black holes in their centers.