Chapter 18 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. The Bizarre Stellar Graveyard Pearson Education, Inc.

Size: px
Start display at page:

Download "Chapter 18 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. The Bizarre Stellar Graveyard Pearson Education, Inc."

Transcription

1 Reading Quiz Clickers The Cosmic Perspective Seventh Edition The Bizarre Stellar Graveyard

2 18.1 White Dwarfs What is a white dwarf? What can happen to a white dwarf in a close binary system?

3 What supports a white dwarf against the crush of gravity? a) thermal pressure b) electron degeneracy pressure c) neutron degeneracy pressure d) proton degeneracy pressure

4 What supports a white dwarf against the crush of gravity? a) thermal pressure b) electron degeneracy pressure c) neutron degeneracy pressure d) proton degeneracy pressure

5 What is the mass limit of a white dwarf? a) 0.8 solar masses b) 1.1 solar masses c) 1.4 solar masses d) 2.0 solar masses e) 8.0 solar masses

6 What is the mass limit of a white dwarf? a) 0.8 solar masses b) 1.1 solar masses c) 1.4 solar masses d) 2.0 solar masses e) 8.0 solar masses

7 How big is a white dwarf? a) the size of a football field b) the size of a city c) the size of the Moon d) the size of Earth e) the size of Jupiter

8 How big is a white dwarf? a) the size of a football field b) the size of a city c) the size of the Moon d) the size of Earth e) the size of Jupiter

9 What is a nova? a) the explosion of the core of a high mass star b) a burst of hydrogen fusion on the surface of a white dwarf c) a burst of carbon fusion in a white dwarf d) a burst of helium fusion in a white dwarf e) radiation from a white dwarf accretion disk

10 What is a nova? a) the explosion of the core of a high mass star b) a burst of hydrogen fusion on the surface of a white dwarf c) a burst of carbon fusion in a white dwarf d) a burst of helium fusion in a white dwarf e) radiation from a white dwarf accretion disk

11 What happens in a white dwarf supernova? a) Carbon fuses throughout the white dwarf. b) Hydrogen fuses on the surface of the white dwarf. c) The white dwarf collapse into a neutron star. d) Helium fuses throughout the white dwarf.

12 What happens in a white dwarf supernova? a) Carbon fuses throughout the white dwarf. b) Hydrogen fuses on the surface of the white dwarf. c) The white dwarf collapse into a neutron star. d) Helium fuses throughout the white dwarf.

13 18.2 Neutron Stars What is a neutron star? How were neutron stars discovered? What can happen to a neutron star in a close binary system?

14 How big is a neutron star? a) the size of a football field b) the size of a city c) the size of the Moon d) the size of Earth e) the size of Jupiter

15 How big is a neutron star? a) the size of a football field b) the size of a city c) the size of the Moon d) the size of Earth e) the size of Jupiter

16 What is a pulsar? a) a high-mass star undergoing thermal pulses due to new shell fusion layers in the interior b) a white dwarf in a binary system periodically going nova as it accretes mass from the binary star c) a white dwarf in a binary system with a hot accretion spot that periodically comes into view as the stars orbit each other d) a rotating neutron star beaming radiation along its magnetic axis

17 What is a pulsar? a) a high-mass star undergoing thermal pulses due to new shell fusion layers in the interior b) a white dwarf in a binary system periodically going nova as it accretes mass from the binary star c) a white dwarf in a binary system with a hot accretion spot that periodically comes into view as the stars orbit each other d) a rotating neutron star beaming radiation along its magnetic axis

18 How do we know pulsars are neutron stars? a) The X-ray intensity is too strong to come from a white dwarf. b) Pulsars spin too fast to be as large as a white dwarf. c) The observed size of the accretion disk is too small to be a white dwarf. d) The radiation shows a gravitational redshift that requires a mass greater than the white dwarf limit.

19 How do we know pulsars are neutron stars? a) The X-ray intensity is too strong to come from a white dwarf. b) Pulsars spin too fast to be as large as a white dwarf. c) The observed size of the accretion disk is too small to be a white dwarf. d) The radiation shows a gravitational redshift that requires a mass greater than the white dwarf limit.

20 What produces X-ray bursts? a) radiation along the magnetic axis of a rapidly rotating neutron star b) radiation from hydrogen fusion on the surface of a neutron star in a binary system c) radiation from helium fusion on the surface of a neutron star in a binary system d) the collapse of a white dwarf into a neutron star e) the collapse of a neutron star into a black hole

21 What produces X-ray bursts? a) radiation along the magnetic axis of a rapidly rotating neutron star b) radiation from hydrogen fusion on the surface of a neutron star in a binary system c) radiation from helium fusion on the surface of a neutron star in a binary system d) the collapse of a white dwarf into a neutron star e) the collapse of a neutron star into a black hole

22 What is the maximum mass of a neutron star? a) 2-3 solar masses b) 5-7 solar masses c) 10 solar masses d) solar masses

23 What is the maximum mass of a neutron star? a) 2-3 solar masses b) 5-7 solar masses c) 10 solar masses d) solar masses

24 18.3 Black Holes: Gravity's Ultimate Victory What is a black hole? What would it be like to visit a black hole? Do black holes really exist?

25 What defines the event horizon? a) the physical surface of a black hole b) the boundary of the observable universe c) the distance from a black hole where the escape velocity equals the speed of light d) the point at which the mass in a star's core cannot be supported and collapses into a black hole

26 What defines the event horizon? a) the physical surface of a black hole b) the boundary of the observable universe c) the distance from a black hole where the escape velocity equals the speed of light d) the point at which the mass in a star's core cannot be supported and collapses into a black hole

27 Which of the following is not a property of a black hole that can be known? a) mass b) temperature c) charge d) angular momentum

28 Which of the following is not a property of a black hole that can be known? a) mass b) temperature c) charge d) angular momentum

29 What happens to time near a black hole? a) It passes more slowly for stationary frames. b) It passes more slowly for moving frames. c) It passes more slowly for all frames. d) It passes more quickly for moving frames. e) It passes more quickly for all frames.

30 What happens to time near a black hole? a) It passes more slowly for stationary frames. b) It passes more slowly for moving frames. c) It passes more slowly for all frames. d) It passes more quickly for moving frames. e) It passes more quickly for all frames.

31 How can we detect a black hole? a) Emission from a black hole accretion disk has a characteristic X-ray spectrum. b) Observing a massive star supernova reveals the mass of the stellar remnant, and if it exceeds 3 solar masses it must be a black hole. c) Observing the orbital motion of a star around a stellar remnant reveals the mass of the stellar remnant, and if it exceeds 3 solar masses it must be a black hole. d) Observation of an X-ray burst reveals the mass of the central object through the gravitational redshift of the X-rays.

32 How can we detect a black hole? a) Emission from a black hole accretion disk has a characteristic X-ray spectrum. b) Observing a massive star supernova reveals the mass of the stellar remnant, and if it exceeds 3 solar masses it must be a black hole. c) Observing the orbital motion of a star around a stellar remnant reveals the mass of the stellar remnant, and if it exceeds 3 solar masses it must be a black hole. d) Observation of an X-ray burst reveals the mass of the central object through the gravitational redshift of the X-rays.

33 18.4 The Origin of Gamma-Ray Bursts What causes gamma-ray bursts?

34 Where do gamma-ray bursts come from? a) the disk of the Milky Way b) the halo of the Milky Way c) the center of the Milky Way d) other galaxies

35 Where do gamma-ray bursts come from? a) the disk of the Milky Way b) the halo of the Milky Way c) the center of the Milky Way d) other galaxies

36 What is the cause of gamma-ray bursts? a) massive star supernovae resulting in black holes b) white dwarf supernovae c) black hole mergers d) all of the above e) A and C

37 What is the cause of gamma-ray bursts? a) massive star supernovae resulting in black holes b) white dwarf supernovae c) black hole mergers d) all of the above e) A and C

Chapter 18 Lecture. The Cosmic Perspective Seventh Edition. The Bizarre Stellar Graveyard Pearson Education, Inc.

Chapter 18 Lecture. The Cosmic Perspective Seventh Edition. The Bizarre Stellar Graveyard Pearson Education, Inc. Chapter 18 Lecture The Cosmic Perspective Seventh Edition The Bizarre Stellar Graveyard The Bizarre Stellar Graveyard 18.1 White Dwarfs Our goals for learning: What is a white dwarf? What can happen to

More information

White dwarfs are the remaining cores of dead stars. Electron degeneracy pressure supports them against the crush of gravity. The White Dwarf Limit

White dwarfs are the remaining cores of dead stars. Electron degeneracy pressure supports them against the crush of gravity. The White Dwarf Limit The Bizarre Stellar Graveyard Chapter 18 Lecture The Cosmic Perspective 18.1 White Dwarfs Our goals for learning: What is a white dwarf? What can happen to a white dwarf in a close binary system? Seventh

More information

Chapter 18 The Bizarre Stellar Graveyard

Chapter 18 The Bizarre Stellar Graveyard Chapter 18 The Bizarre Stellar Graveyard 18.1 White Dwarfs Our goals for learning What is a white dwarf? What can happen to a white dwarf in a close binary system? What is a white dwarf? White Dwarfs White

More information

Chapter 14: The Bizarre Stellar Graveyard

Chapter 14: The Bizarre Stellar Graveyard Lecture Outline Chapter 14: The Bizarre Stellar Graveyard 14.1 White Dwarfs Our goals for learning: What is a white dwarf? What can happen to a white dwarf in a close binary system? What is a white dwarf?

More information

Chapter 18 The Bizarre Stellar Graveyard. White Dwarfs. What is a white dwarf? Size of a White Dwarf White Dwarfs

Chapter 18 The Bizarre Stellar Graveyard. White Dwarfs. What is a white dwarf? Size of a White Dwarf White Dwarfs Chapter 18 The Bizarre Stellar Graveyard 18.1 White Dwarfs Our goals for learning What is a white dwarf? What can happen to a white dwarf in a close binary system? What is a white dwarf? White Dwarfs White

More information

11/1/17. Important Stuff (Section 001: 9:45 am) Important Stuff (Section 002, 1:00 pm) 14.1 White Dwarfs. Chapter 14: The Bizarre Stellar Graveyard

11/1/17. Important Stuff (Section 001: 9:45 am) Important Stuff (Section 002, 1:00 pm) 14.1 White Dwarfs. Chapter 14: The Bizarre Stellar Graveyard 11/1/17 Important Stuff (Section 001: 9:45 am) The Second Midterm is Thursday, November 9 The Second Midterm will be given in a different room: Willey 175 Bring 2 pencils and a photo-id. In accordance

More information

The Stellar Graveyard

The Stellar Graveyard Life and Death of High Mass Stars (M > 8 M sun ) AST 101 Introduction to Astronomy: Stars & Galaxies Last stage: Iron core surrounded by shells of increasingly lighter elements. Announcements MIDTERM #2

More information

11/1/16. Important Stuff (Section 001: 9:45 am) Important Stuff (Section 002, 1:00 pm) 14.1 White Dwarfs. Chapter 14: The Bizarre Stellar Graveyard

11/1/16. Important Stuff (Section 001: 9:45 am) Important Stuff (Section 002, 1:00 pm) 14.1 White Dwarfs. Chapter 14: The Bizarre Stellar Graveyard Important Stuff (Section 001: 9:45 am) The Second Midterm is Thursday, November 10 The Second Midterm will be given in a different room: Willey 175 Bring 2 pencils and a photo-id. In accordance with the

More information

The Bizarre Stellar Graveyard

The Bizarre Stellar Graveyard The Bizarre Stellar Graveyard 18.1 White Dwarfs Our goals for learning: What is a white dwarf? What can happen to a white dwarf in a close binary system? What is a white dwarf? White Dwarfs White dwarfs

More information

The Stellar Graveyard Neutron Stars & White Dwarfs

The Stellar Graveyard Neutron Stars & White Dwarfs The Stellar Graveyard Neutron Stars & White Dwarfs White Dwarfs White dwarfs are the remaining cores of low-mass (M < 8M sun ) stars Electron degeneracy pressure supports them against gravity Density ~

More information

Astronomy. Chapter 15 Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes

Astronomy. Chapter 15 Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes Astronomy Chapter 15 Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes are hot, compact stars whose mass is comparable to the Sun's and size to the Earth's. A. White dwarfs B. Neutron stars

More information

First: Some Physics. Tides on the Earth. Lecture 11: Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes A2020 Prof. Tom Megeath. 1.

First: Some Physics. Tides on the Earth. Lecture 11: Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes A2020 Prof. Tom Megeath. 1. Lecture 11: Stellar Remnants: White Dwarfs, Neutron Stars, and Black Holes A2020 Prof. Tom Megeath First: Some Physics 1. Tides 2. Degeneracy Pressure Concept 1: How does gravity cause tides? R F tides

More information

Chapter 13 Notes The Deaths of Stars Astronomy Name: Date:

Chapter 13 Notes The Deaths of Stars Astronomy Name: Date: Chapter 13 Notes The Deaths of Stars Astronomy Name: Date: I. The End of a Star s Life When all the fuel in a star is used up, will win over pressure and the star will die nuclear fuel; gravity High-mass

More information

Chapter 14: The Bizarre Stellar Graveyard. Copyright 2010 Pearson Education, Inc.

Chapter 14: The Bizarre Stellar Graveyard. Copyright 2010 Pearson Education, Inc. Chapter 14: The Bizarre Stellar Graveyard Assignments 2 nd Mid-term to be held Friday Nov. 3 same basic format as MT1 40 mult. choice= 80 pts. 4 short answer = 20 pts. Sample problems on web page Origin

More information

Chapter 13: The Stellar Graveyard

Chapter 13: The Stellar Graveyard Chapter 13: The Stellar Graveyard Habbal Astro110 http://chandra.harvard.edu/photo/2001/1227/index.html Chapter 13 Lecture 26 1 Low mass star High mass (>8 M sun ) star Ends as a white dwarf. Ends in a

More information

ASTR 101 General Astronomy: Stars & Galaxies. NEXT Tuesday 4/4 MIDTERM #2

ASTR 101 General Astronomy: Stars & Galaxies. NEXT Tuesday 4/4 MIDTERM #2 ASTR 101 General Astronomy: Stars & Galaxies NEXT Tuesday 4/4 MIDTERM #2 The Stellar Graveyard What s In The Stellar Graveyard? Lower mass stars (M< 8M sun ) à white dwarfs Gravity vs. electron degeneracy

More information

Astronomy 110: SURVEY OF ASTRONOMY. 11. Dead Stars. 1. White Dwarfs and Supernovae. 2. Neutron Stars & Black Holes

Astronomy 110: SURVEY OF ASTRONOMY. 11. Dead Stars. 1. White Dwarfs and Supernovae. 2. Neutron Stars & Black Holes Astronomy 110: SURVEY OF ASTRONOMY 11. Dead Stars 1. White Dwarfs and Supernovae 2. Neutron Stars & Black Holes Low-mass stars fight gravity to a standstill by becoming white dwarfs degenerate spheres

More information

Life and Evolution of a Massive Star. M ~ 25 M Sun

Life and Evolution of a Massive Star. M ~ 25 M Sun Life and Evolution of a Massive Star M ~ 25 M Sun Birth in a Giant Molecular Cloud Main Sequence Post-Main Sequence Death The Main Sequence Stars burn H in their cores via the CNO cycle About 90% of a

More information

Termination of Stars

Termination of Stars Termination of Stars Some Quantum Concepts Pauli Exclusion Principle: "Effectively limits the amount of certain kinds of stuff that can be crammed into a given space (particles with personal space ). When

More information

Evolution of High Mass stars

Evolution of High Mass stars Evolution of High Mass stars Neutron Stars A supernova explosion of a M > 8 M Sun star blows away its outer layers. The central core will collapse into a compact object of ~ a few M Sun. Pressure becomes

More information

Gravity simplest. fusion

Gravity simplest. fusion Gravity simplest fusion The life of a star has a complex relationship with gravity: 1. Gravity is what brings the original dust together to make a star 2. Gravity wants to crush the star Gravity pulls

More information

Chapter 19 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. Our Galaxy Pearson Education, Inc.

Chapter 19 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. Our Galaxy Pearson Education, Inc. Reading Quiz Clickers The Cosmic Perspective Seventh Edition Our Galaxy 19.1 The Milky Way Revealed What does our galaxy look like? How do stars orbit in our galaxy? Where are globular clusters located

More information

AST 101 Introduction to Astronomy: Stars & Galaxies

AST 101 Introduction to Astronomy: Stars & Galaxies AST 101 Introduction to Astronomy: Stars & Galaxies Life and Death of High Mass Stars (M > 8 M sun ) REVIEW Last stage: Iron core surrounded by shells of increasingly lighter elements. REVIEW When mass

More information

1. (15.1) What are the approximate mass and radius of a white dwarf compared with those of the Sun?

1. (15.1) What are the approximate mass and radius of a white dwarf compared with those of the Sun? SUMMARY White dwarfs, neutron stars, and black holes are the remnants of dead stars. A white dwarf forms when a low mass star expels its outer layers to form a planetary nebula shell and leaves its hot

More information

A100 Exploring the Universe: Stellar Remnants. Martin D. Weinberg UMass Astronomy

A100 Exploring the Universe: Stellar Remnants. Martin D. Weinberg UMass Astronomy A100 Exploring the Universe: Stellar Remnants Martin D. Weinberg UMass Astronomy astron100-mdw@courses.umass.edu October 28, 2014 Read: S3, Chap 18 10/28/14 slide 1 Exam #2: November 04 One week from today!

More information

Chapter 13 2/19/2014. Lecture Outline Neutron Stars. Neutron Stars and Black Holes Neutron Stars. Units of Chapter

Chapter 13 2/19/2014. Lecture Outline Neutron Stars. Neutron Stars and Black Holes Neutron Stars. Units of Chapter 13.1 Neutron Stars Lecture Outline Chapter 13 Neutron Stars and After a Type I supernova, little or nothing remains of the original star. After a Type II supernova, part of the core may survive. It is

More information

Lecture Outlines. Chapter 22. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 22. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 22 Astronomy Today 8th Edition Chaisson/McMillan Chapter 22 Neutron Stars and Black Holes Units of Chapter 22 22.1 Neutron Stars 22.2 Pulsars 22.3 Neutron-Star Binaries 22.4 Gamma-Ray

More information

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

Exam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti Exam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti INSTRUCTIONS: Please, use the `bubble sheet and a pencil # 2 to answer the exam questions, by marking

More information

Ch. 29 The Stars Stellar Evolution

Ch. 29 The Stars Stellar Evolution Ch. 29 The Stars 29.3 Stellar Evolution Basic Structure of Stars Mass effects The more massive a star is, the greater the gravity pressing inward, and the hotter and more dense the star must be inside

More information

A100 Exploring the Universe: Stellar Remnants. Martin D. Weinberg UMass Astronomy

A100 Exploring the Universe: Stellar Remnants. Martin D. Weinberg UMass Astronomy A100 Exploring the Universe: Stellar Remnants Martin D. Weinberg UMass Astronomy astron100-mdw@courses.umass.edu March 24, 2015 Read: S3, Chap 18 03/24/15 slide 1 Exam #2: March 31 One week from today!

More information

18.3 Black Holes: Gravity's Ultimate Victory

18.3 Black Holes: Gravity's Ultimate Victory 18.3 Black Holes: Gravity's Ultimate Victory Our goals for learning: What is a black hole? What would it be like to visit a black hole? Do black holes really exist? What is a black hole? Gravity, Newton,

More information

Neutron Stars. Chapter 14: Neutron Stars and Black Holes. Neutron Stars. What s holding it up? The Lighthouse Model of Pulsars

Neutron Stars. Chapter 14: Neutron Stars and Black Holes. Neutron Stars. What s holding it up? The Lighthouse Model of Pulsars Neutron Stars Form from a 8-20 M Sun star Chapter 14: Neutron Stars and Black Holes Leftover 1.4-3 M Sun core after supernova Neutron Stars consist entirely of neutrons (no protons) Neutron Star (tennis

More information

Notes for Wednesday, July 16; Sample questions start on page 2 7/16/2008

Notes for Wednesday, July 16; Sample questions start on page 2 7/16/2008 Notes for Wednesday, July 16; Sample questions start on page 2 7/16/2008 Wed, July 16 MW galaxy, then review. Start with ECP3Ch14 2 through 8 Then Ch23 # 8 & Ch 19 # 27 & 28 Allowed Harlow Shapely to locate

More information

High Mass Stars and then Stellar Graveyard 7/16/09. Astronomy 101

High Mass Stars and then Stellar Graveyard 7/16/09. Astronomy 101 High Mass Stars and then Stellar Graveyard 7/16/09 Astronomy 101 Astronomy Picture of the Day Astronomy 101 Something Cool Betelgeuse Astronomy 101 Outline for Today Astronomy Picture of the Day Something

More information

Astronomy 104: Stellar Astronomy

Astronomy 104: Stellar Astronomy Astronomy 104: Stellar Astronomy Lecture 19: Stellar Remnants (Hanging Out with the Degenerates) Spring Semester 2013 Dr. Matt Craig 1 1 Things To Do Today and Next Time Chapter 12.2 (Neutron Stars) Chapter

More information

Astro 1050 Fri. Apr. 10, 2015

Astro 1050 Fri. Apr. 10, 2015 Astro 1050 Fri. Apr. 10, 2015 Today: Continue Ch. 13: Star Stuff Reading in Bennett: For Monday: Finish Chapter 13 Star Stuff Reminders: Ch. 12 HW now on Mastering Astronomy, due Monday. Ch. 13 will be

More information

21. Neutron Stars. The Crab Pulsar: On & Off. Intensity Variations of a Pulsar

21. Neutron Stars. The Crab Pulsar: On & Off. Intensity Variations of a Pulsar 21. Neutron Stars Neutron stars were proposed in the 1930 s Pulsars were discovered in the 1960 s Pulsars are rapidly rotating neutron stars Pulsars slow down as they age Neutron stars are superfluid &

More information

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

AST-1002 Section 0459 Review for Final Exam Please do not forget about doing the evaluation! AST-1002 Section 0459 Review for Final Exam Please do not forget about doing the evaluation! Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the scantrons

More information

Stellar Evolution: Outline

Stellar Evolution: Outline Stellar Evolution: Outline Interstellar Medium (dust) Hydrogen and Helium Small amounts of Carbon Dioxide (makes it easier to detect) Massive amounts of material between 100,000 and 10,000,000 solar masses

More information

Dead & Variable Stars

Dead & Variable Stars Dead & Variable Stars Supernovae Death of massive Stars As the core collapses, it overshoots and bounces A shock wave travels through the star and blows off the outer layers, including the heavy elements

More information

Neutron Stars. Neutron Stars and Black Holes. The Crab Pulsar. Discovery of Pulsars. The Crab Pulsar. Light curves of the Crab Pulsar.

Neutron Stars. Neutron Stars and Black Holes. The Crab Pulsar. Discovery of Pulsars. The Crab Pulsar. Light curves of the Crab Pulsar. Chapter 11: Neutron Stars and Black Holes A supernova explosion of an M > 8 M sun star blows away its outer layers. Neutron Stars The central core will collapse into a compact object of ~ a few M sun.

More information

Physics HW Set 3 Spring 2015

Physics HW Set 3 Spring 2015 1) If the Sun were replaced by a one solar mass black hole 1) A) life here would be unchanged. B) we would still orbit it in a period of one year. C) all terrestrial planets would fall in immediately.

More information

Accretion Disks. Review: Stellar Remnats. Lecture 12: Black Holes & the Milky Way A2020 Prof. Tom Megeath 2/25/10. Review: Creating Stellar Remnants

Accretion Disks. Review: Stellar Remnats. Lecture 12: Black Holes & the Milky Way A2020 Prof. Tom Megeath 2/25/10. Review: Creating Stellar Remnants Lecture 12: Black Holes & the Milky Way A2020 Prof. Tom Megeath Review: Creating Stellar Remnants Binaries may be destroyed in white dwarf supernova Binaries be converted into black holes Review: Stellar

More information

This class: Life cycle of high mass stars Supernovae Neutron stars, pulsars, pulsar wind nebulae, magnetars Quark-nova stars Gamma-ray bursts (GRBs)

This class: Life cycle of high mass stars Supernovae Neutron stars, pulsars, pulsar wind nebulae, magnetars Quark-nova stars Gamma-ray bursts (GRBs) This class: Life cycle of high mass stars Supernovae Neutron stars, pulsars, pulsar wind nebulae, magnetars Quark-nova stars Gamma-ray bursts (GRBs)!1 Cas$A$ All$Image$&$video$credits:$Chandra$X7ray$ Observatory$

More information

1. Star: A object made of gas found in outer space that radiates.

1. Star: A object made of gas found in outer space that radiates. 1. Star: A object made of gas found in outer space that radiates. 2. Stars produce extremely great quantities of energy through the process of. The chemical formula for nuclear fusion looks like this:

More information

Protostars on the HR Diagram. Lifetimes of Stars. Lifetimes of Stars: Example. Pressure-Temperature Thermostat. Hydrostatic Equilibrium

Protostars on the HR Diagram. Lifetimes of Stars. Lifetimes of Stars: Example. Pressure-Temperature Thermostat. Hydrostatic Equilibrium Protostars on the HR Diagram Once a protostar is hot enough to start, it can blow away the surrounding gas Then it is visible: crosses the on the HR diagram The more the cloud, the it will form stars Lifetimes

More information

The April Brooks Observatory sessions

The April Brooks Observatory sessions The April Brooks Observatory sessions Because of our poor weather this semester, additional observing sessions have been scheduled for ASTR 1010, beginning at 8:45 PM each evening: Sunday, April 13 through

More information

Death of Stars Part II Neutron Stars

Death of Stars Part II Neutron Stars Death of Stars Part II Neutron Stars 1 REMEMBER THIS!? 2 Guiding Questions 1. What led scientists to the idea of a neutron star? 2. What are pulsars, and how were they discovered? 3. How did astronomers

More information

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

The Night Sky. The Universe. The Celestial Sphere. Stars. Chapter 14 The Night Sky The Universe Chapter 14 Homework: All the multiple choice questions in Applying the Concepts and Group A questions in Parallel Exercises. Celestial observation dates to ancient civilizations

More information

Prentice Hall EARTH SCIENCE

Prentice Hall EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 25 Beyond Our Solar System 25.1 Properties of Stars Characteristics of Stars A constellation is an apparent group of stars originally named for mythical

More information

Chapter 14. Outline. Neutron Stars and Black Holes. Note that the following lectures include. animations and PowerPoint effects such as

Chapter 14. Outline. Neutron Stars and Black Holes. Note that the following lectures include. animations and PowerPoint effects such as Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode (presentation mode). Chapter 14 Neutron

More information

Analyzing X-Ray Pulses from Stellar Cores Pencil & Paper Version

Analyzing X-Ray Pulses from Stellar Cores Pencil & Paper Version Analyzing X-Ray Pulses from Stellar Cores Pencil & Paper Version Purpose: To determine if two end products of stellar evolution GK Per and Cen X-3 could be white dwarfs or neutron stars by calculating

More information

L = 4 d 2 B p. 4. Which of the letters at right corresponds roughly to where one would find a red giant star on the Hertzsprung-Russell diagram?

L = 4 d 2 B p. 4. Which of the letters at right corresponds roughly to where one would find a red giant star on the Hertzsprung-Russell diagram? Fall 2016 Astronomy - Test 3 Test form B Name Do not forget to write your name and fill in the bubbles with your student number, and fill in test form B on the answer sheet. Write your name above as well.

More information

L = 4 d 2 B p. 1. Which outer layer of the Sun has the highest temperature? A) Photosphere B) Corona C) Chromosphere D) Exosphere E) Thermosphere

L = 4 d 2 B p. 1. Which outer layer of the Sun has the highest temperature? A) Photosphere B) Corona C) Chromosphere D) Exosphere E) Thermosphere Fall 2016 Astronomy - Test 3 Test form A Name Do not forget to write your name and fill in the bubbles with your student number, and fill in test form A on the answer sheet. Write your name above as well.

More information

Neutron Stars. Properties of Neutron Stars. Formation of Neutron Stars. Chapter 14. Neutron Stars and Black Holes. Topics for Today s Class

Neutron Stars. Properties of Neutron Stars. Formation of Neutron Stars. Chapter 14. Neutron Stars and Black Holes. Topics for Today s Class Foundations of Astronomy 13e Seeds Phys1403 Introductory Astronomy Instructor: Dr. Goderya Chapter 14 Neutron Stars and Black Holes Cengage Learning 2016 Topics for Today s Class Neutron Stars What is

More information

ASTR Midterm 2 Phil Armitage, Bruce Ferguson

ASTR Midterm 2 Phil Armitage, Bruce Ferguson ASTR 1120-001 Midterm 2 Phil Armitage, Bruce Ferguson SECOND MID-TERM EXAM MARCH 21 st 2006: Closed books and notes, 1 hour. Please PRINT your name and student ID on the places provided on the scan sheet.

More information

Special Relativity. Principles of Special Relativity: 1. The laws of physics are the same for all inertial observers.

Special Relativity. Principles of Special Relativity: 1. The laws of physics are the same for all inertial observers. Black Holes Special Relativity Principles of Special Relativity: 1. The laws of physics are the same for all inertial observers. 2. The speed of light is the same for all inertial observers regardless

More information

The Stellar Graveyard

The Stellar Graveyard ASTR 101 General Astronomy: Stars & Galaxies The Stellar Graveyard NEXT Thursday 10/22: MIDTERM #2 What s In The Stellar Graveyard? Lower mass stars (M< 8Msun)! white dwarfs Gravity vs. electron degeneracy

More information

Pulsars - a new tool for astronomy and physics

Pulsars - a new tool for astronomy and physics 1 Reading: Chapter 24, Sect. 24.5-24.6; Chap. 20, Chap. 25, Sec. 25.1 Exam 2: Thursday, March 22; essay question given on Tuesday, March 20 Last time:death of massive stars - supernovae & neutron stars

More information

Stars with Mⵙ go through two Red Giant Stages

Stars with Mⵙ go through two Red Giant Stages Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Death of Stars Nuclear reactions in small stars How stars disperse carbon How low mass stars die The nature of white dwarfs

More information

Chapter 21 Astronomy Today 7th Edition Chaisson/McMillan

Chapter 21 Astronomy Today 7th Edition Chaisson/McMillan Lecture Outlines Chapter 21 Astronomy Today 7th Edition Chaisson/McMillan Chapter 21 Stellar Explosions Units of Chapter 21 21.1 Life after Death for White Dwarfs 21.2 The End of a High-Mass Star 21.3

More information

Learning Objectives: Chapter 13, Part 1: Lower Main Sequence Stars. AST 2010: Chapter 13. AST 2010 Descriptive Astronomy

Learning Objectives: Chapter 13, Part 1: Lower Main Sequence Stars. AST 2010: Chapter 13. AST 2010 Descriptive Astronomy Chapter 13, Part 1: Lower Main Sequence Stars Define red dwarf, and describe the internal dynamics and later evolution of these low-mass stars. Appreciate the time scale of late-stage stellar evolution

More information

Recall what you know about the Big Bang.

Recall what you know about the Big Bang. What is this? Recall what you know about the Big Bang. Most of the normal matter in the universe is made of what elements? Where do we find most of this normal matter? Interstellar medium (ISM) The universe

More information

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

Astronomy Stars, Galaxies and Cosmology Exam 3. Please PRINT full name Astronomy 132 - Stars, Galaxies and Cosmology Exam 3 Please PRINT full name Also, please sign the honor code: I have neither given nor have I received help on this exam The following exam is intended to

More information

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

Astronomy 113. Dr. Joseph E. Pesce, Ph.D. Dr. Joseph E. Pesce, Ph.D. Astronomy 113 Dr. Joseph E. Pesce, Ph.D. Stellar Deaths/Endpoints 13-2 Low Mass Stars ³ Like the Sun (< 2 M ) ² Live about 10 billion years (sun is middle aged) ² Create elements through Carbon, Nitrogen,

More information

Stellar Evolution - Chapter 12 and 13. The Lives and Deaths of Stars White dwarfs, neutron stars and black holes

Stellar Evolution - Chapter 12 and 13. The Lives and Deaths of Stars White dwarfs, neutron stars and black holes Stellar Evolution - Chapter 12 and 13 The Lives and Deaths of Stars White dwarfs, neutron stars and black holes During the early stages of a star formation the objects are called a protostars. The internal

More information

Beyond the Solar System 2006 Oct 17 Page 1 of 5

Beyond the Solar System 2006 Oct 17 Page 1 of 5 I. Stars have color, brightness, mass, temperature and size. II. Distances to stars are measured using stellar parallax a. The further away, the less offset b. Parallax angles are extremely small c. Measured

More information

BANG! Structure of a White Dwarf NO energy production gravity = degenerate gas pressure as it cools, becomes Black Dwarf. Lives of High Mass Stars

BANG! Structure of a White Dwarf NO energy production gravity = degenerate gas pressure as it cools, becomes Black Dwarf. Lives of High Mass Stars Structure of a White Dwarf NO energy production gravity = degenerate gas pressure as it cools, becomes Black Dwarf Mass Limit for White Dwarfs S. Chandrasekhar (1983 Nobel Prize) -calculated max. mass

More information

Astronomy 104: Second Exam

Astronomy 104: Second Exam Astronomy 104: Second Exam Stephen Lepp October 29, 2014 Each question is worth 2 points. Write your name on this exam and on the scantron. Short Answer A The Sun is powered by converting hydrogen to what?

More information

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 9

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 9 Phys 0 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 9 MULTIPLE CHOICE 1. We know that giant stars are larger in diameter than the sun because * a. they are more luminous but have about the

More information

Life and Death of a Star 2015

Life and Death of a Star 2015 Life and Death of a Star 2015 Name Date 1. In the main-sequence, the core is slowly shrinking because A. the mass of the star is slowly increasing B. hydrogen fusing to helium makes the core more dense

More information

Agenda. Degenerate Objects. 18. The Bizarre Stellar Graveyard. Degeneracy Pressure A Star s Final Battle. Our goals for learning:

Agenda. Degenerate Objects. 18. The Bizarre Stellar Graveyard. Degeneracy Pressure A Star s Final Battle. Our goals for learning: 18. The Bizarre Stellar Graveyard Now, my suspicion is that the Universe is not only queerer than we suppose, but queerer than we can suppose. Agenda Announce: Extra Credit presentations on April 18 H-R

More information

3/18/14. Today on Stellar Explosions. Second Mid-Term Exam. Things to do SECOND MID-TERM EXAM. Making a millisecond pulsars spin it up!

3/18/14. Today on Stellar Explosions. Second Mid-Term Exam. Things to do SECOND MID-TERM EXAM. Making a millisecond pulsars spin it up! 3/18/14 ASTR 1040: Stars & Galaxies Binary mass transfer: accretion disk Today on Stellar Explosions Spinning up pulsars through mass transfer from (surviving!) companions White dwarf supernovae from mass

More information

Chapter 12 Review. 2) About 90% of the star's total life is spent on the main sequence. 2)

Chapter 12 Review. 2) About 90% of the star's total life is spent on the main sequence. 2) Chapter 12 Review TRUE/FALSE. Write 'T' if the statement is true and 'F' if the statement is false. 1) As a main-sequence star, the Sun's hydrogen supply should last about 10 billion years from the zero-age

More information

ASTRONOMY QUIZ NUMBER 11

ASTRONOMY QUIZ NUMBER 11 ASTRONOMY QUIZ NUMBER. Suppose you measure the parallax of a star and find 0. arsecond. The distance to this star is A) 0 light-years B) 0 parsecs C) 0. light-year D) 0. parsec 2. A star is moving toward

More information

Planetary Nebulae evolve to White Dwarf Stars

Planetary Nebulae evolve to White Dwarf Stars Planetary Nebulae evolve to White Dwarf Stars Planetary Nebulae When Red Giant exhausts its He fuel the C core contracts Low & medium-mass stars don t have enough gravitational energy to heat to core 6

More information

Chapter 18 Lecture. The Cosmic Perspective. The Bizarre Stellar Graveyard Pearson Education, Inc.

Chapter 18 Lecture. The Cosmic Perspective. The Bizarre Stellar Graveyard Pearson Education, Inc. Chapter 18 Lecture The Cosmic Perspective The Bizarre Stellar Graveyard 2014 Pearson Education, Inc. Stellar Remnants During the course of a stars evolution it will shed a significant fraction of its

More information

What is a star? A body of gases that gives off tremendous amounts of energy in the form of light & heat. What star is closest to the earth?

What is a star? A body of gases that gives off tremendous amounts of energy in the form of light & heat. What star is closest to the earth? Stars What is a star? A body of gases that gives off tremendous amounts of energy in the form of light & heat. What star is closest to the earth? Answer: The SUN It s about 150,000,000 km from earth =

More information

Stellar Evolution. Stars are chemical factories The Earth and all life on the Earth are made of elements forged in stars

Stellar Evolution. Stars are chemical factories The Earth and all life on the Earth are made of elements forged in stars Lecture 11 Stellar Evolution Stars are chemical factories The Earth and all life on the Earth are made of elements forged in stars A Spiral Galaxy (Milky Way Type) 120,000 ly A few hundred billion stars

More information

Lecture 23 Stellar Evolution & Death (High Mass) November 21, 2018

Lecture 23 Stellar Evolution & Death (High Mass) November 21, 2018 Lecture 23 Stellar Evolution & Death (High Mass) November 21, 2018 1 2 High Mass Stars (M > 5 M ) Section 13.3 Bennett, The Essential Cosmic Perspective, 7 th ed. High mass stars have: More mass Greater

More information

A Star is born: The Sun. SNC1D7-Space

A Star is born: The Sun. SNC1D7-Space A Star is born: The Sun SNC1D7-Space Exploring the Sun Our Sun, a star, is the most important celestial object for life on Earth. The solar nebula theory is the current theory used to explain the formation

More information

1 The Life Cycle of a Star

1 The Life Cycle of a Star CHAPTER 1 The Life Cycle of a Star Describe the life cycle of various size stars. Rings of glowing gas encircling Supernova 1987A, about 179,000 light-years away in the Large Magellanic Cloud, one of the

More information

Astronomy Ch. 22 Neutron Stars and Black Holes. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Astronomy Ch. 22 Neutron Stars and Black Holes. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Name: Period: Date: Astronomy Ch. 22 Neutron Stars and Black Holes MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) In a neutron star, the core

More information

Astronomy 102: Stars and Galaxies Examination 3 April 11, 2003

Astronomy 102: Stars and Galaxies Examination 3 April 11, 2003 Name: Seat Number: Astronomy 102: Stars and Galaxies Examination 3 April 11, 2003 Do not open the test until instructed to begin. Instructions: Write your answers in the space provided. If you need additional

More information

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. HW3 Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) A surface explosion on a white dwarf, caused by falling matter from the atmosphere of

More information

Chapter 18 Lecture. The Cosmic Perspective. The Bizarre Stellar Graveyard Pearson Education, Inc.

Chapter 18 Lecture. The Cosmic Perspective. The Bizarre Stellar Graveyard Pearson Education, Inc. Chapter 18 Lecture The Cosmic Perspective The Bizarre Stellar Graveyard 2014 Pearson Education, Inc. Stellar Remnants During the course of a stars evolution it will shed a significant fraction of its

More information

Abundance of Elements. Relative abundance of elements in the Solar System

Abundance of Elements. Relative abundance of elements in the Solar System Abundance of Elements Relative abundance of elements in the Solar System What is the origin of elements in the universe? Three elements formed in the first minutes after the big bang (hydrogen, helium

More information

NSCI 314 LIFE IN THE COSMOS

NSCI 314 LIFE IN THE COSMOS NSCI 314 LIFE IN THE COSMOS 2 BASIC ASTRONOMY, AND STARS AND THEIR EVOLUTION Dr. Karen Kolehmainen Department of Physics CSUSB COURSE WEBPAGE: http://physics.csusb.edu/~karen MOTIONS IN THE SOLAR SYSTEM

More information

Review Questions for the new topics that will be on the Final Exam

Review Questions for the new topics that will be on the Final Exam Review Questions for the new topics that will be on the Final Exam Be sure to review the lecture-tutorials and the material we covered on the first three exams. How does speed differ from velocity? Give

More information

Stellar Astronomy Sample Questions for Exam 4

Stellar Astronomy Sample Questions for Exam 4 Stellar Astronomy Sample Questions for Exam 4 Chapter 15 1. Emission nebulas emit light because a) they absorb high energy radiation (mostly UV) from nearby bright hot stars and re-emit it in visible wavelengths.

More information

The Nature of Pulsars! Agenda for Ast 309N, Nov. 1. To See or Not to See (a Pulsar) The Slowing & Fading of Pulsars!

The Nature of Pulsars! Agenda for Ast 309N, Nov. 1. To See or Not to See (a Pulsar) The Slowing & Fading of Pulsars! Agenda for Ast 309N, Nov. 1 Quiz 7 Card 10/30 feedback More on pulsars and other neutron stars Begin: the saga of interacting binary systems Card: questions for review Reading: - Kaler, ch. 7 Wheeler,

More information

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

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 Multiple choice test questions 2, Winter Semester 2015. Based on parts covered after mid term. Essentially on Ch. 12-2.3,13.1-3,14,16.1-2,17,18.1-2,4,19.5. You may use a calculator and the useful formulae

More information

The Stellar Graveyard

The Stellar Graveyard ASTR 1120 General Astronomy: Stars & Galaxies The Stellar Graveyard!EXT $ursday 10/15: #IDTERM #2!EXT Tuesday 10/20: "!earching for distant world"# GO DIRECTLY TO THE PLANETARIUM What s In The Stellar

More information

Final States of a Star

Final States of a Star Pulsars Final States of a Star 1. White Dwarf If initial star mass < 8 MSun or so. (and remember: Maximum WD mass is 1.4 MSun, radius is about that of the Earth) 2. Neutron Star If initial mass > 8 MSun

More information

Stellar remnants II. Neutron Stars 10/18/2010. (progenitor star 1.4 < M< 3 Msun) Stars, Galaxies & the Universe Announcements

Stellar remnants II. Neutron Stars 10/18/2010. (progenitor star 1.4 < M< 3 Msun) Stars, Galaxies & the Universe Announcements Stars, Galaxies & the Universe Announcements Exam #2 on Wednesday Review sheet and study guide posted by Thursday Use office hours and Astronomy Tutorial hours Covers material since Exam #1 (plus background

More information

Beyond Our Solar System Chapter 24

Beyond Our Solar System Chapter 24 Beyond Our Solar System Chapter 24 PROPERTIES OF STARS Distance Measuring a star's distance can be very difficult Stellar parallax Used for measuring distance to a star Apparent shift in a star's position

More information

The Death of Stars. White Dwarfs, Neutron Stars and Black Holes. White Dwarfs

The Death of Stars. White Dwarfs, Neutron Stars and Black Holes. White Dwarfs The Death of Stars White Dwarfs, Neutron Stars and Black Holes White Dwarfs Formed when stars like our Sun reach the end of their life When the Sun s fuel is spent, it will collapse. Don t worry, that

More information

Chapter 12: The Life Cycle of Stars (contʼd) How are stars born, and how do they die? 4/9/09 Habbal Astro Lecture 25 1

Chapter 12: The Life Cycle of Stars (contʼd) How are stars born, and how do they die? 4/9/09 Habbal Astro Lecture 25 1 Chapter 12: The Life Cycle of Stars (contʼd) How are stars born, and how do they die? 4/9/09 Habbal Astro 110-01 Lecture 25 1 12.3 Life as a High-Mass Star Learning Goals What are the life stages of a

More information

Ch. 16 & 17: Stellar Evolution and Death

Ch. 16 & 17: Stellar Evolution and Death Ch. 16 & 17: Stellar Evolution and Death Stars have lives: born, evolve, die Mass determines stellar evolution: Really Low Mass (0.08 to 0.4 M sun ) Low Mass: (0.4 to 4 M sun ) Long lives High Mass (4

More information

MIDTERM #2. ASTR 101 General Astronomy: Stars & Galaxies. Can we detect BLACK HOLES? Black Holes in Binaries to the rescue. Black spot in the sky?

MIDTERM #2. ASTR 101 General Astronomy: Stars & Galaxies. Can we detect BLACK HOLES? Black Holes in Binaries to the rescue. Black spot in the sky? ASTR 101 General Astronomy: Stars & Galaxies Can we detect BLACK HOLES? NEXT Friday 04/03: MIDTERM #2 [Image by A. Hamilton] Black spot in the sky? Black Holes in Binaries to the rescue Black Holes in

More information