Galaxies – Review Questions!

Slides:



Advertisements
Similar presentations
Galaxies & the Universe
Advertisements

LECTURE 21, NOVEMBER 16, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
David - Doppler He is known for the principle he proposed he first proposed in concerning the colored light of double stars in He hypothesized that.
Week 8 Galaxies Reading: Chapter 15, Sections 1, 3 (9 pages)
Astronomy Review. What is gravity? The attractive force between two masses.
Galaxies and the Universe
Astronomy 1 – Fall 2014 Lecture 16; December 8, 2014.
Galaxies PHYS390 Astrophysics Professor Lee Carkner Lecture 20.
Galaxies What is a galaxy? How many stars are there in an average galaxy? About how many galaxies are there in the universe? What is the name of our galaxy?
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 24 Galaxies Galaxies.
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.
Distances. Parallax Near objects appear to move more than far objects against a distant horizon. Trigonometric parallax is used to measure distance to.
Chapter 31 Galaxies & the Universe Review & Recap It does this by precisely measuring the speed of gas and stars around a black hole. This provides clues.
Galaxies How big is the Universe? Types of galaxies Elliptical Spiral
Constellations are groups of stars, sometimes in patterns of animals, or objects. Constellations are important because they can help define where in the.
Spiral - Elliptical - Irregular
The Universe Chapter 20.
Part 5: The Galaxy and the Universe In this final part of the course, we will: 1. Look at the big spatial picture: Are there organizations of stars? What.
From Here to The Dawn of Time A. Herrold. To the edge of the solar system The orbit of Neptune is not at the edge of the solar system Past the planets.
Another galaxy: NGC The Milky Way roughly resembles it.
Chapter 15 Galaxies What do you think? Do galaxies all have spiral arms? Are most of the stars in a spiral galaxy in its arms? Are galaxies isolated.
Star Systems and Galaxies Galaxies and the Big Bang Theory.
Galaxy Review.
PHYS 205 Galaxies Where we live: Milkyway Galaxy Orion Arm System of Sol Third Planet.
Ch. 31 – Galaxies & the Universe   Have you seen the Milky Way at night? The Sun is one of over 100 billion stars that make up the Milky Way. The Sun.
Unit 6 Galaxies *Basic Galaxy Info. *Types of Galaxies -Characteristics of The Milky Way (Spiral Galaxies) *Red Shift & Hubble’s Law.
Galaxies.
Galaxies Chapter 16. Topics Types of galaxies Dark Matter Distances to galaxies Speed of galaxies Expansion of the universe and Hubble’s law.
 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. 
Sci. 4-3 Galaxies Pages A. Galaxies- large groupings of stars in space held together by the attraction of gravity.
Galaxies Please press “1” to test your transmitter.
Star Systems and Galaxies. Star Systems Many stars come in different types of groups. Star system = Group of 2 or more stars Double Stars: 2 stars held.
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.
Star Properties. Where do stars come from? Stars form in a cloud of dust and gas in space called a nebula.
Galaxies (And a bit about distances). This image shows galaxy M 100 in which the Hubble Space Telescope detected Cepheid variables.
Chapter 16 The Milky Way Galaxy 16.1 Overview n How many stars are in the Milky Way? – About 200 billion n How many galaxies are there? – billions.
The Nature of Galaxies Chapter 17. Other Galaxies External to Milky Way –established by Edwin Hubble –used Cepheid variables to measure distance M31 (Andromeda.
Galaxies A galaxy is a collection of millions to billions of stars, dust, and gas bound together by gravity. There are over 1 billion galaxies in the universe.
Galaxies Observing logs due April 27th!!.
Lecture Outlines Astronomy Today 7th Edition Chaisson/McMillan © 2011 Pearson Education, Inc. Chapter 23.
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,
The Expanding Universe. Basic Properties of Stars Magnitude Measuring the Stars –One of the most basic observable properties of a star is how bright it.
(there’s no place like home) The Milky Way Galaxy.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 14 The Milky Way Galaxy.
Star Systems & Galaxies
Universe Tenth Edition Chapter 24 Quasars and Active Galaxies Roger Freedman Robert Geller William Kaufmann III i  clicker Questions.
H205 Cosmic Origins  Today: Galaxies (Ch. 20)  Wednesday: Galaxy Evolution (Ch. 21)  EP 4 & Reflection 1 on Wednesday APOD.
Universe Tenth Edition Chapter 23 Galaxies Roger Freedman Robert Geller William Kaufmann III Clicker Questions.
Galaxies. Edwin Hubble ( ) Discovered that the universe goes beyond the Milky Way He was the first person to establish the distances to other.
Deep Space Objects Variable stars Caused by pulsations in the stars – expansions make them cooler and dimmer – Contractions make them hotter and brighter.
CHAPTER 31 THE GALAXIES & THE UNIVERSE. GALAXIES Scattered throughout the universe Made up of stars, dust and gas held together by gravity There are three.
The Milky Way and Other Galaxies Chapter 20.2 Notes.
Aim: How did the universe form?
Galaxies Star systems like our Milky Way
© 2017 Pearson Education, Inc.
Objectives Describe how astronomers classify galaxies.
Galaxy Types.
Galaxies and the Universe
Galaxies Island Universes.
Ch. 31 – Galaxies & the Universe
The Universe Chapter 25.3.
20.2 The Milky Way and Other Galaxies
Galaxies Chapter 16.
Announcements Observing for third exam starts today.
Galaxies How big is the Universe? Types of galaxies Groups of galaxies
Galaxies.
Presentation transcript:

Galaxies – Review Questions!

16-1.The stars in which type of galaxy can be uniformly distributed in a sphere? a) elliptical b) normal spiral c) barred spiral d) irregular

16-1.The stars in which type of galaxy can be uniformly distributed in a sphere? a) elliptical * b) normal spiral c) barred spiral d) irregular

16-2. Which type of galaxy is presently the most commonly observed type? a) normal spiral b) barred spiral c) elliptical d) irregular

16-2. Which type of galaxy is presently the most commonly observed type? a) normal spiral b) barred spiral c) elliptical * d) irregular

16-3. The smallest known galaxies are of which kind? a) elliptical b) barred spiral c) normal spiral d) irregular

16-3. The smallest known galaxies are of which kind? a) elliptical * b) barred spiral c) normal spiral d) irregular

16-12. Which type of galaxy has very little gas or dust? a) Elliptical b) Spiral c) Irregular d) All of the above

16-12. Which type of galaxy has very little gas or dust? a) Elliptical b) Spiral c) Irregular d) All of the above

16-4. The largest known galaxies are of which kind? a) elliptical b) normal Spiral c) barred Spiral d) irregular

16-4. The largest known galaxies are of which kind? a) elliptical * b) normal Spiral c) barred Spiral d) irregular

16-5. If a galaxy is moving away from us, its absorption lines will: a) change towards higher or lower wavelengths depending on the speed of the galaxy. b) remain at the same wavelengths as lines from galaxies not moving away from us. c) all change towards shorter wavelengths. d) all change towards longer wavelengths.

16-5. If a galaxy is moving away from us, its absorption lines will: a) change towards higher or lower wavelengths depending on the speed of the galaxy. b) remain at the same wavelengths as lines from galaxies not moving away from us. c) all change towards shorter wavelengths. d) all change towards longer wavelengths. *

16-6. What is located between a disk galaxy’s spiral arms? a) nothing b) only interstellar gas and dust c) almost as many stars as in the arms d) more stars than are in the arms

16-6. What is located between a disk galaxy’s spiral arms? a) nothing b) only interstellar gas and dust c) almost as many stars as in the arms d) more stars than are in the arms

16-7. Which observation correctly applies to galaxies in other superclusters? a) they are all moving towards us b) they are all moving away from us c) they are all larger than the Milky Way d) they are all smaller than the Milky Way

16-7. Which observation correctly applies to galaxies in other superclusters? a) they are all moving towards us b) they are all moving away from us * c) they are all larger than the Milky Way d) they are all smaller than the Milky Way

16-8. Spiral density waves describe which of the following? a) the ripples seen in comet tails b) the pulses of a pulsar c) the belts and zones in Jupiter’s upper layers d) ripples in the gas of our Galaxy

16-8. Spiral density waves describe which of the following? a) the ripples seen in comet tails b) the pulses of a pulsar c) the belts and zones in Jupiter’s upper layers d) ripples in the gas of our Galaxy *

16-9. The Andromeda galaxy, in our local cluster, is a) a spiral galaxy smaller than the Milky Way. b) a spiral galaxy larger than the Milky Way. c) an elliptical galaxy smaller than the Milky Way. d) an elliptical galaxy larger than the Milky Way.

16-9. The Andromeda galaxy, in our local cluster, is a) a spiral galaxy smaller than the Milky Way. b) a spiral galaxy larger than the Milky Way. c) an elliptical galaxy smaller than the Milky Way. d) an elliptical galaxy larger than the Milky Way.

a) measuring the distance to it using Cepheid variables. 16-10. Edwin Hubble first showed that Andromeda was a distant galaxy by a) measuring the distance to it using Cepheid variables. b) measuring the distance to it using RR Lyrae variables. c) precisely measuring its parallax angle. d) observing nova in the galaxy.

a) measuring the distance to it using Cepheid variables. * 16-10. Edwin Hubble first showed that Andromeda was a distant galaxy by a) measuring the distance to it using Cepheid variables. * b) measuring the distance to it using RR Lyrae variables. c) precisely measuring its parallax angle. d) observing nova in the galaxy.

Chapter 16 Thought/Writing Questions 1. List three methods of determining distances in the universe. 2. Why do spiral galaxies have spiral arms?

a) they have the highest blue shifts of any objects in the universe 17-1. Some quasars are among the most distant objects in the known universe. Which of the following statements about them must be correct? a) they have the highest blue shifts of any objects in the universe b) they have the smallest blue shifts of any objects in the universe c) they have the highest red shifts of any objects in the universe d) they have the smallest red shifts of any objects in the universe

a) they have the highest blue shifts of any objects in the universe 17-1. Some quasars are among the most distant objects in the known universe. Which of the following statements about them must be correct? a) they have the highest blue shifts of any objects in the universe b) they have the smallest blue shifts of any objects in the universe c) they have the highest red shifts of any objects in the universe * d) they have the smallest red shifts of any objects in the universe

17-6. The time for a fluctuation in brightness of a quasar allows astronomers to place an upper limit on its a) luminosity. b) size. c) age. d) distance.

17-6. The time for a fluctuation in brightness of a quasar allows astronomers to place an upper limit on its a) luminosity. b) size. c) age. d) distance.