Universe Tenth Edition Chapter 22 Our Galaxy Roger Freedman Robert Geller William Kaufmann III Clicker Questions.

Slides:



Advertisements
Similar presentations
Chapter 15: The Milky Way Galaxy
Advertisements

LECTURE 21, NOVEMBER 16, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
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.
Astronomy 1 – Fall 2014 Lecture 15; December 4, 2014.
ASTR-1020 Stellar Astronomy Day 26. Galaxy Classes.
Introduction to Astrophysics Lecture 13: The Milky Way Galaxy.
Slide 1 Andromeda galaxy M31Milky Way galaxy similar to M31.
Chapter 15 The Milky Way Galaxy.
1. A(n) ____ emits large amounts of energy but photographically appears to be a single point of light much like a star. a. a planet like Venus b. E galaxy.
The Milky Way Galaxy Astronomy 315 Professor Lee Carkner Lecture 16.
February 28, 2006 Astronomy Chapter 24: The Milky Way Galaxy M51 Whirlpool Galaxy 31 million LY distant 30,000 LY across.
The Milky Way Galaxy 19 April 2005 AST 2010: Chapter 24.
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 24 Galaxies Galaxies.
ASTR100 (Spring 2008) Introduction to Astronomy Galaxy Evolution & AGN Prof. D.C. Richardson Sections
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 23 Our Galaxy CHAPTER 23 Our Galaxy.
The Milky Way Galaxy Astronomy 315 Professor Lee Carkner Lecture 17.
Chapter 14: The Milky Way Galaxy. Even our unaided eyes tell us that we live in some kind of disk structure. We see the Milky Way in the summer time as.
Chapter 14: The Milky Way Galaxy The scenario for the formation of galaxies is very reminiscent of the formation process for solar systems. Giant cloud.
LECTURE 22, NOVEMBER 18, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
The Milky Way Center, Shape Globular cluster system
The Milky Way. Structure of the Milky Way The Milky Way.
The Milky Way I AST 112 Credit: Stephane Vetter.
The Milky Way Galaxy Immanuel Kant (1724 – 1804) German philosopher The infinitude of creation is great enough to make a world, or a Milky Way of worlds,
The Milky Way Galaxy. The Milky Way We see a band of faint light running around the entire sky. Galileo discovered it was composed of many stars. With.
Chapter 14 The Milky Way Galaxy. Units of Chapter 14 Our Parent Galaxy Measuring the Milky Way Galactic Structure The Formation of the Milky Way Galactic.
The Milky Way Galaxy.
Our Galaxy The Milky Way. 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.
The Milky Way Our Galaxy Please press “1” to test your transmitter.
The Milky Way and Other Galaxies Science A-36 12/4/2007.
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.
Spiral - Elliptical - Irregular
End of Ch. 13 III. Cycle of Birth and Death of Stars: Interstellar Medium Ch. 14.
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.
Ch. 14. The Milky Way Ch. 14. Ch. 14 OUTLINE Shorter than book 14.1 The Milky Way Revealed 14.2 Galactic Recycling (closely related to Ch. 13) 14.3 The.
 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. 
Galaxies GALAXY -comes from the ancient Greeks and their word for “milk”- galactos.
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.
Lecture Outlines Astronomy Today 7th Edition Chaisson/McMillan © 2011 Pearson Education, Inc. Chapter 23.
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.
Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.
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 © 2015, W. W. Norton & Company Prepared by Lisa M. Will, San Diego City College Lecture Slides CHAPTER 15: Our Galaxy: The Milky Way Understanding.
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.
Copyright © 2010 Pearson Education, Inc. Chapter 14 The Milky Way Galaxy Lecture Outline.
Universe Tenth Edition Chapter 24 Quasars and Active Galaxies Roger Freedman Robert Geller William Kaufmann III i  clicker Questions.
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.
Universe Tenth Edition Chapter 23 Galaxies Roger Freedman Robert Geller William Kaufmann III.
ASTR 113 – 003 Spring 2006 Lecture 09 March 29, 2006 Review (Ch4-5): the Foundation Galaxy (Ch 25-27) Cosmology (Ch28-29) Introduction To Modern Astronomy.
The Milky Way Galaxy. What are each of these?
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.
© 2017 Pearson Education, Inc.
© 2017 Pearson Education, Inc.
© 2017 Pearson Education, Inc.
Our Place in the Universe
III. Cycle of Birth and Death of Stars: Interstellar Medium
Even our unaided eyes tell us that we live in some kind of disk structure. We see the Milky Way in the summer time as we look toward the center (white.
Our Milky Way Galaxy.
Chapter 14 Spiral Galaxy.
The scenario for the formation of galaxies is very reminiscent of the formation process for solar systems. Giant cloud of gas and dust, shrinks under its.
The Milky Way Galaxy.
The scenario for the formation of galaxies is very reminiscent of the formation process for solar systems. Giant cloud of gas and dust, shrinks under its.
Presentation transcript:

Universe Tenth Edition Chapter 22 Our Galaxy Roger Freedman Robert Geller William Kaufmann III Clicker Questions

William Herschel tried to locate the center of our Galaxy by counting the number of stars in different directions. This did not work because A.stars are not uniformly distributed. B.more distant stars are obscured by dust and gas. C.there are very few stars near the center of our Galaxy. D.most of the brighter stars are in the outer regions of our Galaxy. E.interstellar reddening gave rise to an incorrect count. Q22.1

William Herschel tried to locate the center of our Galaxy by counting the number of stars in different directions. This did not work because A.stars are not uniformly distributed. B.more distant stars are obscured by dust and gas. C.there are very few stars near the center of our Galaxy. D.most of the brighter stars are in the outer regions of our Galaxy. E.interstellar reddening gave rise to an incorrect count. A22.1

It is possible to obtain high-resolution images of the center of our Galaxy A.at radio and visible wavelengths. B.equally at all wavelengths. C.only at radio wavelengths. D.at infrared and radio wavelengths. E.only at visible wavelengths. Q22.2

It is possible to obtain high-resolution images of the center of our Galaxy A.at radio and visible wavelengths. B.equally at all wavelengths. C.only at radio wavelengths. D.at infrared and radio wavelengths. E.only at visible wavelengths. A22.2

Which of the following best describes how globular clusters are distributed in our Galaxy? A.They are distributed about the center of our Galaxy within the disk. B.They are distributed above the center of our Galaxy in a ring shape. C.They are distributed spherically about the center of our Galaxy in the halo. D.They are only found in the spiral arms. E.They are only found in the nucleus. Q22.3

Which of the following best describes how globular clusters are distributed in our Galaxy? A.They are distributed about the center of our Galaxy within the disk. B.They are distributed above the center of our Galaxy in a ring shape. C.They are distributed spherically about the center of our Galaxy in the halo. D.They are only found in the spiral arms. E.They are only found in the nucleus. A22.3

The distance to and location of the center of our Galaxy was first estimated by mapping out the positions of A.globular clusters. B.the spiral arms. C.intense infrared sources. D.strong radio sources. E.x-ray sources. Q22.4

The distance to and location of the center of our Galaxy was first estimated by mapping out the positions of A.globular clusters. B.the spiral arms. C.intense infrared sources. D.strong radio sources. E.x-ray sources. A22.4

Our solar system is located A.near a globular cluster in the halo of our Galaxy. B.near a globular cluster in a spiral arm of our Galaxy. C.in a spiral arm of our Galaxy. D.in the nucleus of our Galaxy. E.in the disk of our Galaxy, but not within a spiral arm. Q22.5

Our solar system is located A.near a globular cluster in the halo of our Galaxy. B.near a globular cluster in a spiral arm of our Galaxy. C.in a spiral arm of our Galaxy. D.in the nucleus of our Galaxy. E.in the disk of our Galaxy, but not within a spiral arm. A22.5

Which of the following are not found in the halo of our Galaxy? A.Relatively young objects B.Relatively old objects C.Low-mass stars D.Population II stars E.Metal-poor stars Q22.6

Which of the following are not found in the halo of our Galaxy? A.Relatively young objects B.Relatively old objects C.Low-mass stars D.Population II stars E.Metal-poor stars A22.6

Which objects outline the shape of the spiral arms of our Galaxy? A.O and B stars B.H I clouds C.H II regions D.A and B, but not C E.All of A, B, and C Q22.7

Which objects outline the shape of the spiral arms of our Galaxy? A.O and B stars B.H I clouds C.H II regions D.A and B, but not C E.All of A, B, and C A22.7

Which of the following correctly describes our current understanding of our Galaxy ’ s spiral arms? A.The spiral arms are created by density waves that sweep around the Galaxy. B.The spiral arms are the sites for the formation of new stars. C.Stars that are formed in a spiral arm remain in that spiral arm. D.A and B are correct, but not C. E.All of A, B, and C are correct. Q22.8

Which of the following correctly describes our current understanding of our Galaxy ’ s spiral arms? A.The spiral arms are created by density waves that sweep around the Galaxy. B.The spiral arms are the sites for the formation of new stars. C.Stars that are formed in a spiral arm remain in that spiral arm. D.A and B are correct, but not C. E.All of A, B, and C are correct. A22.8

Most astronomers think that there is dark matter in our Galaxy because A.stars in the outer edges of our Galaxy move faster than expected. B.stars in the outer edges of our Galaxy move slower than expected. C.large amounts of matter can be seen at infrared wavelengths. D.large amounts of matter can be seen at radio wavelengths. E.large amounts of matter can be seen at x-ray wavelengths. Q22.9

Most astronomers think that there is dark matter in our Galaxy because A.stars in the outer edges of our Galaxy move faster than expected. B.stars in the outer edges of our Galaxy move slower than expected. C.large amounts of matter can be seen at infrared wavelengths. D.large amounts of matter can be seen at radio wavelengths. E.large amounts of matter can be seen at x-ray wavelengths. A22.9

What observation suggests that a supermassive black hole is at the center of our Galaxy? A.We do not see any light emanating from the center of our Galaxy. B.We see large amounts of gravitational radiation coming from the center of our Galaxy. C.Stars close to the center of our Galaxy are moving at high speeds. D.Light from the center of our Galaxy has a large gravitational redshift. E.Light from the center of our Galaxy has a large gravitational blueshift. Q22.10

What observation suggests that a supermassive black hole is at the center of our Galaxy? A.We do not see any light emanating from the center of our Galaxy. B.We see large amounts of gravitational radiation coming from the center of our Galaxy. C.Stars close to the center of our Galaxy are moving at high speeds. D.Light from the center of our Galaxy has a large gravitational redshift. E.Light from the center of our Galaxy has a large gravitational blueshift. A22.10