What Is Dark Matter? By NASA 2012

Size: px
Start display at page:

Download "What Is Dark Matter? By NASA 2012"

Transcription

1 Name: Class: What Is Dark Matter? By NASA 2012 In this informational text, the author describes what scientists know about dark matter today and the mysteries that continue to surround it. As you read, take notes on how scientists are able to study dark matter. [1] For the first 150 million years after the Big Bang, 1 there were no galaxies or stars or planets. The universe was featureless. As time passed, the first stars formed. Stars collected into galaxies. Galaxies began to cluster together. Those clusters are made up of the galaxies and all the material between the galaxies. Clumps of matter smashed into each other, and the planets in our solar system began to form around the sun. Something must hold our solar system, galaxies, and clusters of galaxies together. And gravity is that glue. In some clusters, the space between galaxies is filled with gas so hot, scientists cannot see it using visible light telescopes. The gas only can be seen as X-rays or gamma rays. 2 Scientists look at that gas and measure how much there is between galaxies in clusters. By doing this, they discovered that there must be five times more material in the clusters than we can detect. The invisible matter that we can t detect is called dark matter. "Gravitationell-lins-4" by NASA, N. Benitez (JHU), T. Broadhurst (Racah Institute of Physics/The Hebrew University), H. Ford (JHU), M. Clampin (STScI),G. Hartig (STScI), G. Illingworth (UCO/Lick Observatory), the ACS Science Team and ESA is in the public domain. The Swiss astronomer Fritz Zwicky first used the term dark matter in the 1930s. He studied the socalled Coma galaxy cluster 3 and, specifically, how fast it revolves. Clusters are like merry-go-rounds: their speed of revolution depends on the weight and position of the objects in the clusters, like the weight of the objects and their positions on a merry-go-round. The speed he measured implied the cluster had much more mass than the observable light suggested. 1. the cosmic explosion that marked the beginning of the universe, according to current theories 2. types of high energy and frequency electromagnetic radiation 3. a cluster of galaxies containing over 1,000 identified galaxies 1

2 [5] In the 1970s, U.S. astronomer Vera Rubin and her colleagues confirmed this result by studying galaxy rotation. They also discovered single galaxies, not just clusters, have more mass than their observable light suggested. The work of Rubin and her team helped to firmly establish the notion of dark matter. In many ways, scientists know more about what dark matter is not, though they do have a few ideas about what it could be. Dark matter possibly could be brown dwarfs, failed stars that never ignited because they lacked the mass needed to start burning. Dark matter could be white dwarfs, the remnants of cores of dead small- to medium-size stars. Or dark matter could be neutron stars or black holes, the remnants of large stars after they explode. However, problems exist with each of these suggestions. Scientists have strong evidence there aren t enough brown dwarfs or white dwarfs to account for all the dark matter. Black holes and neutron stars, too, are rare. Dark matter may not be made up of the matter we are familiar with at all. The matter that makes up dark matter could be different. It may be filled with particles predicted by theory but that scientists have yet to observe. Because scientists can t see dark matter directly, they have found other ways to investigate it. We can use indirect ways to study things, like looking at a shadow and making an educated guess about what s casting the shadow. One way scientists indirectly study dark matter is by using gravitational lensing. [10] Light going through a gravitational lens is similar to light going through an optical lens: 4 it gets bent. When light from distant stars passes through a galaxy or cluster, the gravity of the matter present in the galaxy or cluster causes the light to bend. As a result, the light looks like it is coming from somewhere else rather than from its actual origin. The amount of bending helps scientists learn about the dark matter present. Many NASA scientists use the Hubble Space Telescope to observe gravitational lensing. In addition to these indirect ways, scientists at NASA think they have a direct way to detect dark matter using the Fermi Gamma-Ray Space Telescope. This telescope looks at gamma rays, the highest energy form of light. When two dark matter particles crash into each other, they might release a gamma ray. The Fermi Telescope could theoretically 5 detect these collisions, which would appear as a burst of a gamma ray in the sky. Because Fermi has not been in space very long, scientists do not yet have enough data to form conclusions. That s what makes dark matter exciting: it s still one of the great mysteries of science. What Is Dark Matter by NASA (2012) is in the public domain. 4. a device that focuses or disperses a light beam 5. Theoretical (adjective): concerned with or involving the theory of a subject, rather than it practical application 2

3 Text-Dependent Questions Directions: For the following questions, choose the best answer or respond in complete sentences. 1. PART A: Which TWO sentences provide the best summary for the text? A. Dark matter will likely help scientists better understand the beginning of the universe. B. Scientists are excited to discover what dark matter truly is, so as to determine whether or not it is a threat. C. What scientists know about dark matter right now is built primarily on theory, rather than concrete facts. D. Scientists are unable to study dark matter directly because they are unsure whether or not it is dangerous. E. Dark matter is the thing in the universe that scientists know the least about, and will likely never understand completely. F. Dark matter is invisible, and therefore scientists must look at how dark matter affects matter around it to detect it. 2. PART B: Which TWO details from the text best support the answers to Part A? A. Clumps of matter smashed into each other, and the planets in our solar system began to form around the sun. (Paragraph 2) B. The Swiss astronomer Fritz Zwicky first used the term dark matter in the 1930s. He studied the so-called Coma galaxy cluster (Paragraph 4) C. Scientists have strong evidence there aren t enough brown dwarfs or white dwarfs to account for all the dark matter. (Paragraph 7) D. The matter that makes up dark matter could be different. It may be filled with particles predicted by theory but that scientists have yet to observe. (Paragraph 8) E. As a result, the light looks like it is coming from somewhere else rather than from its actual origin. The amount of bending helps scientists learn about the dark matter present. (Paragraph 9) F. Because Fermi has not been in space very long, scientists do not yet have enough data to form conclusions. (Paragraph 9) 3. How do paragraphs 6-7 contribute to the development of ideas in the text? A. They reveal how little scientist know for certain about dark matter. B. They should how much scientists are learning about dark matter. C. They prove that dark matter will forever be a mystery. D. They show why it s important to learn what dark matter is. 3

4 4. What connection does the author draw between the rotation of galaxy clusters and dark matter? 4

5 Discussion Questions Directions: Brainstorm your answers to the following questions in the space provided. Be prepared to share your original ideas in a class discussion. 1. Why do you think scientists want to learn more about dark matter? How would learning more about dark matter help scientists better understand the rest of the universe? 2. In the context of the text, who is in control: man or nature? How does the text emphasize how little humans know about natural occurrences in the universe? 5

Chapter 16 Dark Matter, Dark Energy, & The Fate of the Universe

Chapter 16 Dark Matter, Dark Energy, & The Fate of the Universe 16.1 Unseen Influences Chapter 16 Dark Matter, Dark Energy, & The Fate of the Universe Dark Matter: An undetected form of mass that emits little or no light but whose existence we infer from its gravitational

More information

Review of Lecture 15 3/17/10. Lecture 15: Dark Matter and the Cosmic Web (plus Gamma Ray Bursts) Prof. Tom Megeath

Review of Lecture 15 3/17/10. Lecture 15: Dark Matter and the Cosmic Web (plus Gamma Ray Bursts) Prof. Tom Megeath Lecture 15: Dark Matter and the Cosmic Web (plus Gamma Ray Bursts) Prof. Tom Megeath A2020 Disk Component: stars of all ages, many gas clouds Review of Lecture 15 Spheroidal Component: bulge & halo, old

More information

Today: Start Ch. 18: Cosmology. Homework # 5 due next Wed. (HW #6 is online)

Today: Start Ch. 18: Cosmology. Homework # 5 due next Wed. (HW #6 is online) Today: Start Ch. 18: Cosmology Homework # 5 due next Wed. (HW #6 is online) Dark Matter! A rotation curve is a graph of how fast a something is rotating, as a function of distance from the center.! We

More information

Dark Matter: Finding the Invisible

Dark Matter: Finding the Invisible Dark Matter: Finding the Invisible Laura Storch Boston University WR150 LA Image courtesy of Hubble Deep Field Overview: Dark Matter: -Why do we think it exists? -Observational evidence -What are its properties?

More information

What is the difference between a galaxy and a solar system?

What is the difference between a galaxy and a solar system? What is the difference between a galaxy and a solar system? By NASA, adapted by Newsela staff on 09.19.17 Word Count 819 Level 970L An image of the Milky Way galaxy taken In celebration of the International

More information

Chapter 22 What do we mean by dark matter and dark energy?

Chapter 22 What do we mean by dark matter and dark energy? Chapter 22 What do we mean by dark matter and dark energy? Unseen Influences Dark Matter: An undetected form of mass that emits little or no light, but whose existence we infer from its gravitational influence

More information

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

The Universe. Unit 3 covers the following framework standards: ES 8 and 12. Content was adapted the following: Unit 3 The Universe Chapter 4 ~ The Formation of the Universe o Section 1 ~ The Scale of the Universe o Section 2 ~ The Formation of the Universe o Section 3 ~ The Future of the Universe Chapter 5 ~ Galaxies

More information

Chapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization

Chapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization Objectives Describe characteristics of the universe in terms of time, distance, and organization Identify the visible and nonvisible parts of the electromagnetic spectrum Compare refracting telescopes

More information

GraspIT Questions AQA GCSE Physics Space physics

GraspIT Questions AQA GCSE Physics Space physics A. Solar system: stability of orbital motions; satellites (physics only) 1. Put these astronomical objects in order of size from largest to smallest. (3) Fill in the boxes in the correct order. the Moon

More information

How does the galaxy rotate and keep the spiral arms together? And what really lies at the center of the galaxy?

How does the galaxy rotate and keep the spiral arms together? And what really lies at the center of the galaxy? Ch 14: Mysteries of the Milky Way How does the galaxy rotate and keep the spiral arms together? And what really lies at the center of the galaxy? The Structure of the Galaxy We know that our galaxy has

More information

Directed Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past?

Directed Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past? Skills Worksheet Directed Reading Section: Viewing the Universe 1. How did observations of the sky help farmers in the past? 2. How did observations of the sky help sailors in the past? 3. What is the

More information

Cracking the Mysteries of the Universe. Dr Janie K. Hoormann University of Queensland

Cracking the Mysteries of the Universe. Dr Janie K. Hoormann University of Queensland Cracking the Mysteries of the Universe Dr Janie K. Hoormann University of Queensland Timeline of Cosmological Discoveries 16c BCE: flat earth 5-11c CE: Sun at the centre 1837: Bessel et al. measure distance

More information

Chapter 23: Dark Matter, Dark Energy & Future of the Universe. Galactic rotation curves

Chapter 23: Dark Matter, Dark Energy & Future of the Universe. Galactic rotation curves Chapter 23: Dark Matter, Dark Energy & Future of the Universe Galactic rotation curves Orbital speed as a function of distance from the center: rotation_of_spiral_galaxy.htm Use Kepler s Third Law to get

More information

Lecture 25: Cosmology: The end of the Universe, Dark Matter, and Dark Energy. Astronomy 111 Wednesday November 29, 2017

Lecture 25: Cosmology: The end of the Universe, Dark Matter, and Dark Energy. Astronomy 111 Wednesday November 29, 2017 Lecture 25: Cosmology: The end of the Universe, Dark Matter, and Dark Energy Astronomy 111 Wednesday November 29, 2017 Reminders Online homework #11 due Monday at 3pm One more lecture after today Monday

More information

AST1100 Lecture Notes

AST1100 Lecture Notes AST1100 Lecture Notes 4 Stellar orbits and dark matter 1 Using Kepler s laws for stars orbiting the center of a galaxy We will now use Kepler s laws of gravitation on much larger scales. We will study

More information

PHYSICS 107. Lecture 27 What s Next?

PHYSICS 107. Lecture 27 What s Next? PHYSICS 107 Lecture 27 What s Next? The origin of the elements Apart from the expansion of the universe and the cosmic microwave background radiation, the Big Bang theory makes another important set of

More information

Galaxies. Beyond the Book. FOCUS Book. Make a model that helps demonstrate how the universe is expanding. Follow these steps:

Galaxies. Beyond the Book. FOCUS Book. Make a model that helps demonstrate how the universe is expanding. Follow these steps: FOCUS Book Galaxies Make a model that helps demonstrate how the universe is expanding. Follow these steps: 1 Use markers to make dots on the outside of an uninflated balloon to represent galaxies full

More information

Earth Space Systems. Semester 1 Exam. Astronomy Vocabulary

Earth Space Systems. Semester 1 Exam. Astronomy Vocabulary Earth Space Systems Semester 1 Exam Astronomy Vocabulary Astronomical Unit- Aurora- Big Bang- Black Hole- 1AU is the average distance between the Earth and the Sun (93 million miles). This unit of measurement

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

TELESCOPES POWERFUL. Beyond the Book. FOCUS Book

TELESCOPES POWERFUL. Beyond the Book. FOCUS Book FOCUS Book POWERFUL TELESCOPES Why do we need telescopes in order to observe stars that are very far away? Why do stars look bright in the sky while most galaxies, which have billions of stars, are too

More information

GAMMA RAYS. 1 P a g e

GAMMA RAYS. 1 P a g e GAMMA RAYS 1 P a g e 2 P a g e 3 P a g e Death Stars Do the most powerful blasts of energy in the universe threaten Earth? You don't want to be anywhere near a giant star when it dies. In just a few seconds,

More information

Beyond the Book. FOCUS Book

Beyond the Book. FOCUS Book FOCUS Book You have learned that a nebula can turn into a star, and that the star can turn into a new nebula. Now design a comic, timeline, flowchart, or cycle diagram to explain this process. Include

More information

Planetarium/Observing: the clock is ticking! Don t forget to fill out your Planetarium/ Observing impression online.

Planetarium/Observing: the clock is ticking! Don t forget to fill out your Planetarium/ Observing impression online. Announcements HW #5 Due Wed, Dec. 10th. Planetarium/Observing: the clock is ticking! Don t forget to fill out your Planetarium/ Observing impression online. NOTE: Planetarium: Large dome you sit inside.

More information

Chapter 23 Lecture. The Cosmic Perspective Seventh Edition. Dark Matter, Dark Energy, and the Fate of the Universe Pearson Education, Inc.

Chapter 23 Lecture. The Cosmic Perspective Seventh Edition. Dark Matter, Dark Energy, and the Fate of the Universe Pearson Education, Inc. Chapter 23 Lecture The Cosmic Perspective Seventh Edition Dark Matter, Dark Energy, and the Fate of the Universe Curvature of the Universe The Density Parameter of the Universe Ω 0 is defined as the ratio

More information

The Formation of the Solar System

The Formation of the Solar System Earth and the Solar System The Formation of the Solar System Write a number beside each picture to rank each from the oldest (1) to the youngest (4). The universe includes everything that exists: all matter,

More information

Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe

Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe The Big Bang Theory The Big Bang Theory The Big Bang Theory is the most widely accepted scientific explanation

More information

CHAPTER 4 STARS, GALAXIES & THE UNIVERSE

CHAPTER 4 STARS, GALAXIES & THE UNIVERSE CHAPTER 4 STARS, GALAXIES & THE UNIVERSE LESSON 1: TELESCOPES ALL TYPES OF ELECTROMAGNETIC RADIATION TRAVEL AT THE SPEED OF LIGHT 186,000 miles per second!! Electromagnetic Radiation = energy that travels

More information

Science 30 Unit C Electromagnetic Energy

Science 30 Unit C Electromagnetic Energy Science 30 Unit C Electromagnetic Energy Outcome 2: Students will describe the properties of the electromagnetic spectrum and their applications in medical technologies, communication systems and remote-sensing

More information

ANSWER KEY. Stars, Galaxies, and the Universe. Telescopes Guided Reading and Study. Characteristics of Stars Guided Reading and Study

ANSWER KEY. Stars, Galaxies, and the Universe. Telescopes Guided Reading and Study. Characteristics of Stars Guided Reading and Study Stars, Galaxies, a the Universe Stars, Galaxies, and the Universe Telescopes Use Target Reading Skills Check student definitions for accuracy. 1. Electromagneticradiationisenergythatcan travel through

More information

What is a supernova? They Outshine Their Entire Galaxy. By NASA, adapted by Newsela staff on Word Count 675 Level 840L

What is a supernova? They Outshine Their Entire Galaxy. By NASA, adapted by Newsela staff on Word Count 675 Level 840L What is a supernova? By NASA, adapted by Newsela staff on 03.28.17 Word Count 675 Level 840L TOP: A vivid view of a supernova remnant captured by NASA's Spitzer and Chandra space observatories and the

More information

Homework 6 Name: Due Date: June 9, 2008

Homework 6 Name: Due Date: June 9, 2008 Homework 6 Name: Due Date: June 9, 2008 1. Where in the universe does the general expansion occur? A) everywhere in the universe, including our local space upon Earth, the solar system, our galaxy and

More information

DARK MATTER. Masses of Galaxies

DARK MATTER. Masses of Galaxies Masses of Galaxies Measure mass by: motion within a galaxy motion of different galaxies about each other gravitational lensing Gives - most mass isn t in stars and normal matter DARK MATTER 1 Mass of Galaxy

More information

THE ORIGIN OF THE UNIVERSE AND BLACK HOLES

THE ORIGIN OF THE UNIVERSE AND BLACK HOLES THE ORIGIN OF THE UNIVERSE AND BLACK HOLES WHAT IS COSMOGONY? Cosmogony (or cosmogeny) is any model explaining the origin of the universe. Cosmogony = Coming into existence WHAT IS COSMOLOGY Cosmology

More information

Chapter 23 Lecture. The Cosmic Perspective Seventh Edition. Dark Matter, Dark Energy, and the Fate of the Universe Pearson Education, Inc.

Chapter 23 Lecture. The Cosmic Perspective Seventh Edition. Dark Matter, Dark Energy, and the Fate of the Universe Pearson Education, Inc. Chapter 23 Lecture The Cosmic Perspective Seventh Edition Dark Matter, Dark Energy, and the Fate of the Universe Curvature of the Universe The Density Parameter of the Universe Ω 0 is defined as the ratio

More information

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

Observing the Night Sky. Observing the Night Sky. Observing the Night Sky. Observing the Night Sky. Observing the Night Sky. Chapter 29 THE UNIVERSE Hewitt/Lyons/Suchocki/Yeh Conceptual Integrated Science Constellations are groups of stars named over antiquity. A familiar constellation is Ursa Major, the Great Bear. Chapter 29 THE UNIVERSE The monthly

More information

Astro-2: History of the Universe. Lecture 5; April

Astro-2: History of the Universe. Lecture 5; April Astro-2: History of the Universe Lecture 5; April 23 2013 Previously.. On Astro-2 Galaxies do not live in isolation but in larger structures, called groups, clusters, or superclusters This is called the

More information

Moment of beginning of space-time about 13.7 billion years ago. The time at which all the material and energy in the expanding Universe was coincident

Moment of beginning of space-time about 13.7 billion years ago. The time at which all the material and energy in the expanding Universe was coincident Big Bang Moment of beginning of space-time about 13.7 billion years ago The time at which all the material and energy in the expanding Universe was coincident Only moment in the history of the Universe

More information

Figure 19.19: HST photo called Hubble Deep Field.

Figure 19.19: HST photo called Hubble Deep Field. 19.3 Galaxies and the Universe Early civilizations thought that Earth was the center of the universe. In the sixteenth century, we became aware that Earth is a small planet orbiting a medium-sized star.

More information

the evidence that the size of the observable Universe is changing;

the evidence that the size of the observable Universe is changing; Q1. Describe, in as much detail as you can: the evidence that the size of the observable Universe is changing; the evidence that, billions of years ago, all the matter in the Universe was tightly packed

More information

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

Today. life the university & everything. Reminders: Review Wed & Fri Eyes to the web Final Exam Tues May 3 Check in on accomodations life the university & everything Phys 2130 Day 41: Questions? The Universe Reminders: Review Wed & Fri Eyes to the web Final Exam Tues May 3 Check in on accomodations Today Today: - how big is the universe?

More information

GLAST. Exploring the Extreme Universe. Kennedy Space Center. The Gamma-ray Large Area Space Telescope

GLAST. Exploring the Extreme Universe. Kennedy Space Center. The Gamma-ray Large Area Space Telescope GLAST Gamma-ray Large Area Space Telescope The Gamma-ray Large Area Space Telescope Exploring the Extreme Universe Kennedy Space Center Dave Thompson GLAST Deputy Project Scientist David.J.Thompson@nasa.gov

More information

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

3. It is expanding: the galaxies are moving apart, accelerating slightly The mystery of Dark Energy II. Cosmology: How the universe developed Outstanding features of the universe today: 1. It is big, and full of galaxies. 2. It has structure: the galaxies are clumped in filaments and sheets The structure

More information

Exploring Dark Matter through Gravitational Lensing. Exploring the Dark Universe Indiana University June 2007

Exploring Dark Matter through Gravitational Lensing. Exploring the Dark Universe Indiana University June 2007 Exploring Dark Matter through Gravitational Lensing Exploring the Dark Universe Indiana University 28-29 June 2007 What is a Gravitational Lens? A gravitational lens is formed when the light from a distant,

More information

Stars, Galaxies, and the Universe

Stars, Galaxies, and the Universe Stars, Galaxies, and the Universe Chapter Test A Multiple Choice Write the letter of the correct answer on the line at the left. 1. What is a giant ball of hot gases that undergo nuclear fusion? a. a planet

More information

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

Directed Reading A. Section: The Life Cycle of Stars TYPES OF STARS THE LIFE CYCLE OF SUNLIKE STARS A TOOL FOR STUDYING STARS. Skills Worksheet Directed Reading A Section: The Life Cycle of Stars TYPES OF STARS (pp. 444 449) 1. Besides by mass, size, brightness, color, temperature, and composition, how are stars classified? a.

More information

Other Galaxy Types. Active Galaxies. A diagram of an active galaxy, showing the primary components. Active Galaxies

Other Galaxy Types. Active Galaxies. A diagram of an active galaxy, showing the primary components. Active Galaxies Other Galaxy Types Active Galaxies Active Galaxies Seyfert galaxies Radio galaxies Quasars Origin??? Different in appearance Produce huge amount of energy Similar mechanism a Galactic mass black hole at

More information

Writing very large numbers

Writing very large numbers 19.1 Tools of Astronomers Frequently in the news we hear about discoveries that involve space. Since the 1970s, space probes have been sent to all of the planets in the solar system and we have seen them

More information

Chapter 26 Section 1 pages Directed Reading Section: Viewing the Universe

Chapter 26 Section 1 pages Directed Reading Section: Viewing the Universe Name: Period: Chapter 26 Section 1 pages 659-666 Directed Reading Section: Viewing the Universe 1. How did observations of the sky help sailors in the past? 2. What is the main reason people study the

More information

3 The lives of galaxies

3 The lives of galaxies Discovering Astronomy : Galaxies and Cosmology 24 3 The lives of galaxies In this section, we look at how galaxies formed and evolved, and likewise how the large scale pattern of galaxies formed. But before

More information

New Ideas from Astronomy and Cosmology. Martin Buoncristiani Session 5 4/21/2011

New Ideas from Astronomy and Cosmology. Martin Buoncristiani Session 5 4/21/2011 New Ideas from Astronomy and Cosmology Martin Buoncristiani Session 5 Agenda Introduction Space, Time and Matter Early views of the cosmos Important Ideas from Classical Physics Two 20 th Century revolutions

More information

ASTR Astrophysics 1 - Stellar and Interstellar. Phil Armitage. office: JILA tower A909

ASTR Astrophysics 1 - Stellar and Interstellar. Phil Armitage. office: JILA tower A909 ASTR 3730 Astrophysics 1 - Stellar and Interstellar Phil Armitage office: JILA tower A909 email: pja@jilau1.colorado.edu Part one of a year-long introduction to astrophysics: Aim - develop physical understanding

More information

Astronomy Universe: all of space and everything in it

Astronomy Universe: all of space and everything in it Astronomy Universe: all of space and everything in it Most (90%) of the universe is made up of: dark matter: stuff we think is there due to amount of mass we think is there but is not detected by the instruments

More information

A supernova is the explosion of a star. It is the largest explosion that takes place in space.

A supernova is the explosion of a star. It is the largest explosion that takes place in space. What is a supernova? By NASA, adapted by Newsela staff on 03.28.17 Word Count 974 Level 1110L TOP: A vivid view of a supernova remnant captured by NASA's Spitzer and Chandra space observatories and the

More information

Dark Matter and Dark Energy

Dark Matter and Dark Energy Dark Matter and Dark Energy Jim Pivarski March 4, 2012 Matter as we know it is a minority of the universe. Jim Pivarski 2/51 Jim Pivarski 3/51 Jim Pivarski 4/51 This talk: What is dark matter? The astronomer

More information

The Tools of Cosmology. Andrew Zentner The University of Pittsburgh

The Tools of Cosmology. Andrew Zentner The University of Pittsburgh The Tools of Cosmology Andrew Zentner The University of Pittsburgh 1 Part Two: The Contemporary Universe 2 Contents Review of Part One The Pillars of Modern Cosmology Primordial Synthesis of Light Nuclei

More information

Dark Matter & Dark Energy. Astronomy 1101

Dark Matter & Dark Energy. Astronomy 1101 Dark Matter & Dark Energy Astronomy 1101 Key Ideas: Dark Matter Matter we cannot see directly with light Detected only by its gravity (possible future direct detection in the lab) Most of the matter in

More information

Cosmologists dedicate a great deal of effort to determine the density of matter in the universe. Type Ia supernovae observations are consistent with

Cosmologists dedicate a great deal of effort to determine the density of matter in the universe. Type Ia supernovae observations are consistent with Notes for Cosmology course, fall 2005 Dark Matter Prelude Cosmologists dedicate a great deal of effort to determine the density of matter in the universe Type Ia supernovae observations are consistent

More information

Dark matter: summary

Dark matter: summary Dark matter: summary Gravity and detecting Dark Matter Massive objects, even if they emit no light, exert gravitational forces on other massive objects. m 1 r 12 m 2 We study the motions (dynamics) of

More information

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

o Terms to know o Big Bang Theory o Doppler Effect o Redshift o Universe Standard 1: Students will understand the scientific evidence that supports theories that explain how the universe and the solar system developed. They will compare Earth to other objects in the solar system.

More information

Introduction. The Mystery of our universe today, is Dark Matter. Dark Matter is the heart of our

Introduction. The Mystery of our universe today, is Dark Matter. Dark Matter is the heart of our Introduction The Mystery of our universe today, is Dark Matter. Dark Matter is the heart of our galaxy, and it keeps the planets and stars from flying away or moving positions. Dark Matter is the pitch

More information

Astronomy 102: Stars and Galaxies Examination 3 Review Problems

Astronomy 102: Stars and Galaxies Examination 3 Review Problems Astronomy 102: Stars and Galaxies Examination 3 Review Problems Multiple Choice Questions: The first eight questions are multiple choice. Except where explicitly noted, only one answer is correct for each

More information

Finding Black Holes Left Behind by Single Stars

Finding Black Holes Left Behind by Single Stars Finding Black Holes Left Behind by Single Stars Finding Black Holes "Yesterday upon the stair I met a man who wasn't there. He wasn't there again today. I wish that man would go away." Hughes Mearns (1875-1965)

More information

Part two of a year-long introduction to astrophysics:

Part two of a year-long introduction to astrophysics: ASTR 3830 Astrophysics 2 - Galactic and Extragalactic Phil Armitage office: JILA tower A909 email: pja@jilau1.colorado.edu Spitzer Space telescope image of M81 Part two of a year-long introduction to astrophysics:

More information

Galaxies and the Universe

Galaxies and the Universe Standard 7.3.1: Recognize and describe that the Sun is a medium-sized star located near the edge of a diskshaped galaxy of stars and that the universe contains many billions of galaxies and each galaxy

More information

What is the Dark Matter? William Shepherd Niels Bohr International Academy Johannes Gutenberg University Mainz

What is the Dark Matter? William Shepherd Niels Bohr International Academy Johannes Gutenberg University Mainz What is the Dark Matter? William Shepherd Niels Bohr International Academy Johannes Gutenberg University Mainz Outline Evidence for the existence of dark matter Motion of visible matter Cosmological evidence

More information

The Milky Way Galaxy is Heading for a Major Cosmic Collision

The Milky Way Galaxy is Heading for a Major Cosmic Collision The Milky Way Galaxy is Heading for a Major Cosmic Collision Roeland van der Marel (STScI) [based on work with a team of collaborators reported in the Astrophysical Journal July 2012] Hubble Science Briefing

More information

CH 14 MODERN COSMOLOGY The Study of Nature, origin and evolution of the universe Does the Universe have a center and an edge? What is the evidence

CH 14 MODERN COSMOLOGY The Study of Nature, origin and evolution of the universe Does the Universe have a center and an edge? What is the evidence CH 14 MODERN COSMOLOGY The Study of Nature, origin and evolution of the universe Does the Universe have a center and an edge? What is the evidence that the Universe began with a Big Bang? How has the Universe

More information

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, March 2018 Number of pages: 9 Course: ASTR 1P02, Section 1 Number of Students: 465 Date of Examination: March 12, 2018 BROCK UNIVERSITY Page 1 of 9 Test 2, March 2018 Number of pages: 9 Course: ASTR 1P02, Section 1 Number of Students: 465 Date of Examination: March 12, 2018 Number of hours: 50 min Time of Examination:

More information

The sun, an engine of nuclear energy

The sun, an engine of nuclear energy The sun, an engine of nuclear energy By Big History Project, adapted by Newsela staff on 08.22.17 Word Count 905 Level 980L This image shows a view of all that remains of the oldest documented example

More information

GraspIT Questions AQA GCSE Physics Space physics

GraspIT Questions AQA GCSE Physics Space physics A. Solar system: stability of orbital motions; satellites (physics only) 1. Put these astronomical objects in order of size from largest to smallest. (3) Fill in the boxes in the correct order. the Moon

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

Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE

Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE Cosmology, Galaxies, and Stars OUR VISIBLE UNIVERSE Cosmology Cosmology is the study of the universe; its nature, origin and evolution. General Relativity is the mathematical basis of cosmology from which

More information

The phenomenon of gravitational lenses

The phenomenon of gravitational lenses The phenomenon of gravitational lenses The phenomenon of gravitational lenses If we look carefully at the image taken with the Hubble Space Telescope, of the Galaxy Cluster Abell 2218 in the constellation

More information

AST 301 Introduction to Astronomy

AST 301 Introduction to Astronomy AST 301 Introduction to Astronomy John Lacy RLM 16.332 471-1469 lacy@astro.as.utexas.edu Myoungwon Jeon RLM 16.216 471-0445 myjeon@astro.as.utexas.edu Bohua Li RLM 16.212 471-8443 bohuali@astro.as.utexas.edu

More information

Today. Gravitational Lenses 11/19/2013. Astronomy Picture of the Day

Today. Gravitational Lenses 11/19/2013. Astronomy Picture of the Day ASTR 1020: Stars & Galaxies November 15, 2013 Reading for Monday: Chapter 23, section 23.1-23.3. MasteringAstronomy homework on Galaxy Evolution is due tonight at midnight. Exam 3 is on Wednesday, Nov.

More information

Study Guide Chapter 2

Study Guide Chapter 2 Section: Stars Pages 32-38 Study Guide Chapter 2 Circle the letter of the best answer for each question. 1. What do scientists study to learn about stars? a. gravity c. space b. starlight d. colors COLOR

More information

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

8/30/2010. Classifying Stars. Classifying Stars. Classifying Stars Classifying Stars In the early 1900s, Ejnar Hertzsprung and Henry Russell made some important observations. They noticed that, in general, stars with higher temperatures also have brighter absolute magnitudes.

More information

Chapter 28 Stars and Their Characteristics

Chapter 28 Stars and Their Characteristics Chapter 28 Stars and Their Characteristics Origin of the Universe Big Bang Theory about 10-20 bya all matter in the universe existed in a hot dense state about the size of an atom (tiny). That matter sort

More information

Big Galaxies Are Rare! Cepheid Distance Measurement. Clusters of Galaxies. The Nature of Galaxies

Big Galaxies Are Rare! Cepheid Distance Measurement. Clusters of Galaxies. The Nature of Galaxies Big Galaxies Are Rare! Potato Chip Rule: More small things than large things Big, bright spirals are easy to see, but least common Dwarf ellipticals & irregulars are most common Faint, hard to see Mostly

More information

Black Holes Thursday, 14 March 2013

Black Holes Thursday, 14 March 2013 Black Holes General Relativity Intro We try to explain the black hole phenomenon by using the concept of escape velocity, the speed to clear the gravitational field of an object. According to Newtonian

More information

LESSON 1. Solar System

LESSON 1. Solar System Astronomy Notes LESSON 1 Solar System 11.1 Structure of the Solar System axis of rotation period of rotation period of revolution ellipse astronomical unit What is the solar system? 11.1 Structure of the

More information

SUPERNOVA! What is a supernova? How dangerous are they to life on Earth? How would the universe be different without supernovae?

SUPERNOVA! What is a supernova? How dangerous are they to life on Earth? How would the universe be different without supernovae? SUPERNOVA! What is a supernova? How dangerous are they to life on Earth? How would the universe be different without supernovae? 1 Stellar Evolution: The Deaths of Stars A hundred years ago, we believed

More information

CST Prep- 8 th Grade Astronomy

CST Prep- 8 th Grade Astronomy CST Prep- 8 th Grade Astronomy Chapter 15 (Part 1) 1. The theory of how the universe was created is called the 2. Which equation states that matter and energy are interchangeable? 3. All matter in the

More information

7. How many black holes do scientists think are in the Milky Way galaxy?

7. How many black holes do scientists think are in the Milky Way galaxy? Name: Block: Date: Science News for Students Black Hole Mysteries https://student.societyforscience.org/article/black-hole-mysteries 1. Is a black hole really a hole? Explain. 2. Why can't anything escape

More information

Grade 5. Practice Test. Telescopes: An Introduction Powerful Telescopes

Grade 5. Practice Test. Telescopes: An Introduction Powerful Telescopes Name Date Grade 5 Telescopes: An Introduction Powerful Telescopes Today you will read two passages. Read these sources carefully to gather information to answer questions and write an essay. Excerpt from

More information

Dark Matter. Jaan Einasto Tartu Observatory and ICRANet 16 December Saturday, December 15, 12

Dark Matter. Jaan Einasto Tartu Observatory and ICRANet 16 December Saturday, December 15, 12 Dark Matter Jaan Einasto Tartu Observatory and ICRANet 16 December 2012 Local Dark Matter: invisible matter in the Galaxy in Solar vicinity Global Dark Matter: invisible matter surrounding galaxies Global

More information

1 Astronomy: The Original Science

1 Astronomy: The Original Science CHAPTER 18 1 Astronomy: The Original Science SECTION Studying Space BEFORE YOU READ After you read this section, you should be able to answer these questions: How do astronomers define a day, a month,

More information

Astronomy 150: Killer Skies Lecture 35, April 23

Astronomy 150: Killer Skies Lecture 35, April 23 Assignments: ICES available online Astronomy 150: Killer Skies Lecture 35, April 23 HW11 due next Friday: last homework! note: lowest HW score dropped but: HW11 material will be on Exam 3, so be sure to

More information

Astronomers push the edges of final frontier, find farthest galaxy

Astronomers push the edges of final frontier, find farthest galaxy Astronomers push the edges of final frontier, find farthest galaxy By Associated Press, adapted by Newsela staff on 03.14.16 Word Count 688 This image provided by the Space Telescope Science Institute,

More information

Number of Stars: 100 billion (10 11 ) Mass : 5 x Solar masses. Size of Disk: 100,000 Light Years (30 kpc)

Number of Stars: 100 billion (10 11 ) Mass : 5 x Solar masses. Size of Disk: 100,000 Light Years (30 kpc) THE MILKY WAY GALAXY Type: Spiral galaxy composed of a highly flattened disk and a central elliptical bulge. The disk is about 100,000 light years (30kpc) in diameter. The term spiral arises from the external

More information

April 13, 2011 Exam 4, Friday. Review sheet posted. Sky Watch 4 due. Review session Thursday, 5 6 PM, Room WEL 3.502, right here! Reading: Chapter 9,

April 13, 2011 Exam 4, Friday. Review sheet posted. Sky Watch 4 due. Review session Thursday, 5 6 PM, Room WEL 3.502, right here! Reading: Chapter 9, April 13, 2011 Exam 4, Friday. Review sheet posted. Sky Watch 4 due. Review session Thursday, 5 6 PM, Room WEL 3.502, right here! Reading: Chapter 9, Sections 9.5.2, 9.6.1, 9.6.2. 9.7, 9.8; Chapter 10,

More information

Astro 406 Lecture 25 Oct. 25, 2013

Astro 406 Lecture 25 Oct. 25, 2013 Astro 406 Lecture 25 Oct. 25, 2013 Announcements: PS 7 due now PS 8 due next Friday ASTR 401: draft due next Monday thanks to the Planetarium-goers alternate makeup activity posted soon Next semester:

More information

What is the solar system?

What is the solar system? Notes Astronomy What is the solar system? 11.1 Structure of the Solar System Our solar system includes planets and dwarf planets, their moons, a star called the Sun, asteroids and comets. Planets, dwarf

More information

The State of the Universe

The State of the Universe The State of the Universe Harry Ringermacher, PhD General Electric Research Center Adj. Prof. of Physics, U. of S. Mississippi State of the Universe Universe is still going strong! - At least 100,000,000,000

More information

and Universe Awareness

and Universe Awareness Brought to you by s Chandra X-ray Observatory and Universe wareness Light Looking up at the night sky, you might think that space is dull, with lots of black, some white dots and just a hint of red if

More information

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES

SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES Q1. The figure below shows what scientists over 1000 years ago thought the solar system was like. Give one way that the historical model of the solar

More information

Examining Dark Energy With Dark Matter Lenses: The Large Synoptic Survey Telescope. Andrew R. Zentner University of Pittsburgh

Examining Dark Energy With Dark Matter Lenses: The Large Synoptic Survey Telescope. Andrew R. Zentner University of Pittsburgh Examining Dark Energy With Dark Matter Lenses: The Large Synoptic Survey Telescope Andrew R. Zentner University of Pittsburgh 1 Overview The contents of the Universe The accelerating Universe and Dark

More information

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

The Contents of the Universe (or/ what do we mean by dark matter and dark energy?) The Contents of the Universe (or/ what do we mean by dark matter and dark energy?) Unseen Influences Dark Matter: An undetected form of mass that emits little or no light but whose existence we infer from

More information

Module 3: Astronomy The Universe Topic 1 Content: Cosmology Presentation Notes

Module 3: Astronomy The Universe Topic 1 Content: Cosmology Presentation Notes Pretend that you have been given the opportunity to travel through time to explore cosmology. Cosmology is the study of how the universe formed and what will happen to it. Watch through your viewport as

More information

The Mystery of Dark Matter

The Mystery of Dark Matter The Mystery of Dark Matter Maxim Perelstein, LEPP/Cornell U. CIPT Fall Workshop, Ithaca NY, September 28 2013 Introduction Last Fall workshop focused on physics of the very small - elementary particles

More information