TA Final Review. Class Announcements. Objectives Today. Compare True and Apparent brightness. Finding Distances with Cepheids

Similar documents
According to the currents models of stellar life cycle, our sun will eventually become a. Chapter 34: Cosmology. Cosmology: How the Universe Works

THE UNIVERSE CHAPTER 20

Island Universes. Up to 1920 s, many thought that Milky Way encompassed entire universe.

Figure 19.19: HST photo called Hubble Deep Field.

ASTR 101 General Astronomy: Stars & Galaxies

BROCK UNIVERSITY. Test 2, March 2018 Number of pages: 9 Course: ASTR 1P02, Section 1 Number of Students: 465 Date of Examination: March 12, 2018

BROCK UNIVERSITY. Test 2: July 2015 Number of pages: 9 Course: ASTR 1P02, Section 2 Number of students: 318

Galaxies and the Universe

Quick Quizlet. Quizlettino. Cosmology: How the Universe Works

BROCK UNIVERSITY. Test 2: June 2016 Number of pages: 10 Course: ASTR 1P02, Section 2 Number of students: 359

Galaxies and Cosmology

The Big Bang Theory. Rachel Fludd and Matthijs Hoekstra

BROCK UNIVERSITY. Test 2, March 2015 Number of pages: 9 Course: ASTR 1P02 Number of Students: 420 Date of Examination: March 5, 2015

8/30/2010. Classifying Stars. Classifying Stars. Classifying Stars

Expanding Universe. 1) Hubble s Law 2) Expanding Universe 3) Fate of the Universe. Final Exam will be held in Ruby Diamond Auditorium

Homework 6 Name: Due Date: June 9, 2008

Formation of the Universe. What evidence supports current scientific theory?

The Expanding Universe

Name Date Period. 10. convection zone 11. radiation zone 12. core

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

Beyond Our Solar System Chapter 24

Stars & Galaxies. Chapter 27 Modern Earth Science

Chapter 25: Beyond our Solar System The Universe pp

Stars & Galaxies. Chapter 27, Section 1. Composition & Temperature. Chapter 27 Modern Earth Science Characteristics of Stars

The Contents of the Universe (or/ what do we mean by dark matter and dark energy?)

Hubble's Law. H o = 71 km/s / Mpc. The further a galaxy is away, the faster it s moving away from us. V = H 0 D. Modern Data.

Cosmic Microwave Background Radiation

Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE

The Big Bang Theory was first proposed in the late 1920 s. This singularity was incredibly dense and hot.

ASTRONOMY II Spring 1995 FINAL EXAM. Monday May 8th 2:00pm

Astronomy Hour Exam 2 March 10, 2011 QUESTION 1: The half-life of Ra 226 (radium) is 1600 years. If you started with a sample of 100 Ra 226

Beyond the Solar System 2006 Oct 17 Page 1 of 5

The Universe. But first, let s talk about light! 2012 Pearson Education, Inc.

2) On a Hertzsprung-Russell diagram, where would you find red giant stars? A) upper right B) lower right C) upper left D) lower left

Question 1. Question 2. Correct. Chapter 16 Homework. Part A

Part I: The Dawn of Time

29:50 Stars, Galaxies, and the Universe Final Exam December 13, 2010 Form A

Prentice Hall EARTH SCIENCE

LESSON 1. Solar System

The Night Sky. The Universe. The Celestial Sphere. Stars. Chapter 14

How do we measure properties of a star? Today. Some Clicker Questions - #1. Some Clicker Questions - #1

Directed Reading A. Section: The Life Cycle of Stars TYPES OF STARS THE LIFE CYCLE OF SUNLIKE STARS A TOOL FOR STUDYING STARS.

What is the solar system?

Implications of the Hubble Law: - it is not static, unchanging - Universe had a beginning!! - could not have been expanding forever HUBBLE LAW:

Today. Lookback time. ASTR 1020: Stars & Galaxies. Astronomy Picture of the day. April 2, 2008

Cosmology and the Evolution of the Universe. Implications of the Hubble Law: - Universe is changing (getting bigger!) - it is not static, unchanging

Lecture 37 Cosmology [not on exam] January 16b, 2014

Lecture PowerPoints. Chapter 33 Physics: Principles with Applications, 7 th edition Giancoli

Chapter 28 Stars and Their Characteristics

Astronomy 114. Lecture35:TheBigBang. Martin D. Weinberg. UMass/Astronomy Department

Normal Galaxies (Ch. 24) + Galaxies and Dark Matter (Ch. 25) Symbolically: E0.E7.. S0..Sa..Sb..Sc..Sd..Irr

Learning Objectives. distances to objects in our Galaxy and to other galaxies? apparent magnitude key to measuring distances?

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

(Astronomy for Dummies) remark : apparently I spent more than 1 hr giving this lecture

Revision Guide for Chapter 12

How Did the Universe Begin?

Stars and Galaxies 1

chapter 31 Stars and Galaxies

Chapter 30. Galaxies and the Universe. Chapter 30:

PHYSICS 107. Lecture 27 What s Next?

Light. Transverse electromagnetic wave, or electromagnetic radiation. Includes radio waves, microwaves, infra-red, visible, UV, X-rays, and gamma rays

Galaxies and the expansion of the Universe

Earth Science, 13e Tarbuck & Lutgens

Astronomy 102: Stars and Galaxies Examination 3 Review Problems

Final Exam Study Guide

Observing the Night Sky. Observing the Night Sky. Observing the Night Sky. Observing the Night Sky. Observing the Night Sky. Chapter 29 THE UNIVERSE

A 103 Notes, Week 14, Kaufmann-Comins Chapter 15

Astronomy 162, Week 10 Cosmology Patrick S. Osmer Spring, 2006

UNIT 3 The Study of the. Universe. Chapter 7: The Night Sky. Chapter 8: Exploring Our Stellar Neighbourhood. Chapter 9:The Mysterious.

Edwin Hubble Discovered galaxies other than the milky way. Galaxy:

Active Galaxies and Galactic Structure Lecture 22 April 18th

ASTR 1120 General Astronomy: Stars & Galaxies. OUR Universe: Accelerating Universe

The King's University College Astronomy 201 Mid-Term Exam Solutions

HUBBLE SPACE TELESCOPE

3. It is expanding: the galaxies are moving apart, accelerating slightly The mystery of Dark Energy

ASTR 1P02 Test 2, March 2017 Page 1 BROCK UNIVERSITY. Test 2: March 2017 Number of pages: 9 Course: ASTR 1P02, Section 2 Number of students: 1193

Lecture 14: Other Galaxies A2020 Prof. Tom Megeath. The Milky Way in the Infrared 3/17/10. NGC 7331: the Milky Way s Twins. Spiral Galaxy bulge halo

Doppler Effect. Sound moving TOWARDS. Sound moving AWAY 9/22/2017. Occurs when the source of sound waves moves towards or away

i>clicker Quiz #14 Which of the following statements is TRUE?

Answers. The Universe. Year 10 Science Chapter 6

GraspIT Questions AQA GCSE Physics Space physics

AST-1002 Section 0459 Review for Final Exam Please do not forget about doing the evaluation!

Galaxies & Introduction to Cosmology

Lecture #21: Plan. Normal Galaxies. Classification Properties Distances

The Doppler Effect is the change in frequency observed when a source of sound waves is moving relative to an observer.

The Milky Way Galaxy (ch. 23)

3. It became unstable and exploded 2. This point was. Timeline of Events 4. This outward expansion

Chapter 15 Galaxies and the Foundation of Modern Cosmology

The Tools of Cosmology. Andrew Zentner The University of Pittsburgh

Astronomy 113. Dr. Joseph E. Pesce, Ph.D. Distances & the Milky Way. The Curtis View. Our Galaxy. The Shapley View 3/27/18

Astronomy 113. Dr. Joseph E. Pesce, Ph.D. Dr. Joseph E. Pesce, Ph.D.

Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999

Astronomy Stars, Galaxies and Cosmology Exam 3. Please PRINT full name

Today. life the university & everything. Reminders: Review Wed & Fri Eyes to the web Final Exam Tues May 3 Check in on accomodations

25/11/ Cosmological Red Shift:

Exam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti

Hubble sequence galaxy classification scheme, originally based on appearance, but correlates with other properties as well.

Galaxies. The majority of known galaxies fall into one of three major classes: spirals (78 %), ellipticals (18 %) and irregulars (4 %).

The Universe. What is it? What is in it? How did it form? How will it end? How do we know?

Exam 3 Astronomy 100, Section 3. Some Equations You Might Need

Transcription:

Class Announcements Vocab Quiz 4 deadline is Saturday Midterm 4 has started, ends Monday Lab was in the Planetarium. You still need to do the 2 questions Check PS100 webpage, make sure your clicker is registered. TA Final Review Final Review TBA How much of the book would you estimate that you have read this year? a) 80-100% b) 60-80% c) 40-60% d) 20-40% e) 0-20% Objectives Today Distance Scales Cepheid Variables & Supernovae Understand structure of Milkyway Identify different types of galaxies Cosmological redshift Hubble Law Big Bang and evidence for it Estimate distances to galaxies Compare True and Apparent brightness Some stars, called Cepheids,, are very bright and unstable, pulsating with periods that are proportional to their true brightnesses. Finding Distances with Cepheids We can measure a Cepheid s s period and apparent brightness, and then infer the absolute brightness from the period-luminosity relationship. With the apparent and absolute brightness we can then get a distance to the star. This is only good for finding distances to the nearest 100 galaxies. You have to resolve the star to get the period. 1

What is the Milkyway? We know we are in a disk, band of stars across the sky. The sun is 2/3 the way from the galaxy center to the edge. Globular clusters were used to find the center of the galaxy. Variable stars were used to determine distances The Sun x Images of the Milkyway Globular Clusters x External Galaxies Galaxies: Huge Collections of Stars In 1920 the Shapley-Curtis debate ensues Planetary systems forming? External Galaxies? In 1923 using Cepheid variable stars, Edwin Hubble determined that the Andromeda galaxy was a separate system of stars. Soon it was realized that all spiral-shaped shaped nebula were galaxies of stars similar to the Milky Way. On average over 100 billion stars per galaxy! Huge! The universe itself is only 10 5 times larger than a typical galaxy. At least 50 billion of them. Galaxies fall into four main classifications according to their shapes. First Sketch of a galaxy. William Parsons, 1845 Large galaxies, red stars, no blue stars Ellipticals What does the absence of blue stars tell us? A. That there isn t t enough gas in these galaxies to make large stars B. That the galaxy is moving towards us C. That the galaxy is old D. That there aren t t any new stars forming 2

Gas, dust lanes, blue stars, young star forming regions Spirals Barred Spirals Irregular/Peculiar Gas, dust lanes, blue stars, young star forming regions, no definite shape Galaxy Clusters Galaxies are held together in small to large groups What holds them together? What force holds galactic clusters together? a) The weak nuclear force b) The strong nuclear force c) The electromagnetic force d) The gravitational force Cosmological Redshift Each atom emits at characteristic wavelengths (spectral lines) Certain patterns of prominent lines are observed in the spectra of all stars & galaxies E.g. hydrogen In the early 1900 s, it was found that wavelengths measured for distant galaxies do not match laboratory measurements Distant galactic lines are always shifted to longer wavelengths True for all galaxies but the few closest. Why? 3

Doppler Shift The Doppler effect causes waves to shift up to a higher frequency as they move towards you and down to lower frequency as they move away Sound examples race car engine train whistle Light examples cosmological redshift If all the galaxies are moving away, why are some of the galaxies close to the Milkyway blueshifted? a) They are spiral galaxies with lots of new stars b) Something is sucking nearby galaxies in c) I don t t know Hubble Law Hubble found that the speed at which a galaxy moves away from us is proportional to its distance. The farther away the galaxy is, the faster it recedes. Could this mean we are at the center of the universe? The Expanding Universe The farther away two galaxies are, the faster they move apart All galaxies appear to be moving away from all other galaxies. Expansion Distances from the Hubble Law We can use the Hubble Law to find distances to galaxies The larger the redshift,, the faster the velocity, the faster the velocity, the greater the distance. 4

The Big Bang The observed expansion of the universe has led to only one viable cosmological theory: The Big Bang. The universe began as a great infusion of pure energy about 14 billion years ago. Space expanded from that point in time. The energy cooled into matter. Evidence Supporting the Big Bang We see the expansion We see a faint glow left from the original fireball. Called the Cosmic Microwave Background or 3 3 K Background Radiation. Evidence Supporting the Big Bang It correctly predicts the chemical abundances of gas clouds. 75% hydrogen, 25% helium, a tiny amount of lithium. Fusion early after the big bang would produce that ratio of H to He. Big Bang Stellar Fusion Supernova 3 min 35 min Steps in Big-Bang Bang Theory (Interest only, not on test) Time Temp Structure 10-43 sec 10-35 sec 0.001 sec 5x10 5 yrs 10 10 yrs huge 10 26 10 11 10 9 10 8 3x10 4 3 All energy Elementary particles (electrons, quarks, etc.) Protons and neutrons Nuclei of 3 H, 3 He, 4 He, 5 Li Nuclei of 2 H Electrons attach to nuclei to form atoms Stars, galaxies, people Good Theories Give Good Predictions. What Does the Big Bang Predict About the Future? Gravity always pulls, never pushes. So the expansion must slow down unless there is another force pushing out. The Ultimate Fate of the Universe Not enough mass open universe Just right flat universe Too much mass closed universe (big- crunch?) Another force runaway universe. 5

Accelerating Expansion? Recent work compared distances measured two ways: From the apparent brightness of a known kind of supernova From the amount of cosmological redshift At large distances, the two methods do not agree (the supernova method gives bigger distances than the Hubble Law) This and other data are taken as evidence that the expansion is speeding up! None of the four known forces could cause this What Do We Observe? The expansion is accelerating! A runaway universe No one knows why No known force could cause this 6