From Molecular Cores to Stars

Size: px
Start display at page:

Download "From Molecular Cores to Stars"

Transcription

1 rom Molecular ores to Stars xamining erbig-aro 6/7 00 The University of Texas at ustin or classroom instruction Production supported by a NS ducation/public Outreach grant

2 olor alibration Make sure that your video projector accurately reproduces these colors, especially yellow (Y) and green (). White Y Red Yellow reen Magenta lue yan

3 . What part of the electromagnetic spectrum are you seeing in each image? The tiny dots of light are stars. Most of the stars are far behind this nebula in the foreground that is made of gas and dust. i. Which image shows the infrared light? ii. Which image shows the visible light? iii. What evidence in the images supports your decision?

4 lue Primary olors reen Red

5 lue Primary olors reen Red

6 lue Primary olors reen Red

7 Primary olors lue reen Red

8 = + + = + = + = +

9 yan Secondary olors Yellow Magenta

10 yan Secondary olors Yellow Magenta

11 yan Secondary olors Yellow Magenta

12 Secondary olors yan Yellow Magenta

13 = + + = + = + = +

14 6/7 infrared 6/7 visible 8 µm. µm +.8 µm.6 µm What do the colors in the infrared image mean? The infrared image colors correspond to infrared wavelengths of light, not visible colors. Visible colors range in wavelength from 0. to 0.7 micrometers. The light wavelengths in the infrared image range from.6 to 8.0 micrometers. To make sense of the infrared image, astronomers assign visible colors to infrared wavelengths to produce a false color image, like the one you are examining:.6 micrometers = blue (shortest wavelength),.6 and.8 micrometers combined = green, and 8.0 micrometers = red (longest wavelength). Visual R alse colors wavelength in micrometers 8.0

15 6/7 infrared 6/7 visible 8 µm. µm +.8 µm.6 µm. xamine the infrared image of 6/7 i. Which false colors in the infrared image represent the hottest material? The coolest? ii. Why do you think the other stars in the infrared image are false blue and white? iii. f a feature appears white in the infrared image, what does that indicate about the energy distribution in infrared wavelengths? Visual R alse colors wavelength in micrometers 8.0

16 6/7 infrared 6/7 visible. ly 8 µm. µm +.8 µm.6 µm. xamine the visible light image of 6/7 i. What is the dark blob (centered at ) in the visible light image? xplain. ii. What are the points of light surrounding the dark blob in the visible light image? xplain. Visual R alse colors wavelength in micrometers 8.0

17 6/7 infrared 6/7 visible. ly 8 µm. µm +.8 µm.6 µm. ompare and contrast the two images List the prominent features in each image, and how you think they are related. R image feature Visible image feature Visual Relationship R alse colors wavelength in micrometers 8.0

18 6/7 infrared 6/7 visible. ly 8 µm. µm +.8 µm.6 µm. vidence of motion The tube shaped smoke ring in the infrared image (,,, ) is an outflow of gas and dust from the forming star. The gas is expanding rapidly, with maximum speeds approaching 00 kilometers per second. nclude supporting evidence in your explanations. Why do you think the gas and dust are emitting infrared light? Visual R alse colors wavelength in micrometers 8.0

19 lectron Microscope mage of Space ust 0. mm isplayed in a close-up under an electron microscope, this tiny bit of cosmic dust may be our first sample of a passing comet. Less than onetenth of a millimeter across, the particle is composed of millions of even tinier crystals. lthough chemically similar to some meteorites, its fluffy, crystalline structure is unlike that of any known meteorite.

20 The constellation of Orion What is inside the Orion Nebula? etelgeuse Orion s elt nimation redit: Zolt Levay (STSc) and ryan Preston (STSc and Max-Q igital) Orion Nebula Rigel nimation redit: NS and Walt eimer (STSc) STSc-00- mage by kira ujii

21 Side view of 6. What happens after star formation? These is a visible wavelength images of an object in the Orion Nebula taken with the ubble Space Telescope. i. What is the bright spot in the center of image? ii. What about the dark oval in image and the dark disk in image? iii. Where do you think the planets would form? mage redit: Mark Mcaughrean (Max-Planck-nstitute for stronomy),. Robert O'ell (Rice University), and NS

22 Wink slides: Switch, or wink, between the two following slides to compare and contrast the images.

23 8 µm. µm +.8 µm.6 µm

24

25 ust to ust ycle ig ang and e louds lump & ollapse ust & as Neutron Star Proto Star Proto Planetary isc Sub-stellar Supernova lack ole Star Planets Planetary nebula White warf

26 ig ang Spitzer Space Telescope ores to iscs Legacy Team and e louds lump & ollapse nter-stellar Medium Li, e, N, O, lack ole Proto Star Proto Planetary isc Sub-stellar Objects Supernova Neutron Star Star White warf Planetary Nebula Planets

Student Guide From Molecular Cores to Stars

Student Guide From Molecular Cores to Stars Team Members: Date: Student Guide From Molecular Cores to Stars Dust Hunt Driving Question: What are the characteristics of dust in our classroom, and how did it get here? Science Objectives: 1. Collect

More information

Instructions. Students will underline the portions of the PowerPoint that are underlined.

Instructions. Students will underline the portions of the PowerPoint that are underlined. STARS Instructions Students will underline the portions of the PowerPoint that are underlined. Nuclear Furnace 1. A star is like a gigantic nuclear furnace. 2. The nuclear reactions inside convert hydrogen

More information

Classifying Stars. Scientists classify stars by: 1. Temperature 2. Brightness

Classifying Stars. Scientists classify stars by: 1. Temperature 2. Brightness STARS Classifying Stars Scientists classify stars by: 1. Temperature 2. Brightness Star Temperature 1. The color of a star tells us about its temperature. Blue stars are the hottest, 7500 C- 40,000 C.

More information

Modern Astronomy Review #1

Modern Astronomy Review #1 Modern Astronomy Review #1 1. The red-shift of light from distant galaxies provides evidence that the universe is (1) shrinking, only (3) shrinking and expanding in a cyclic pattern (2) expanding, only

More information

27.1: Characteristics of Stars

27.1: Characteristics of Stars 27.1: Characteristics of Stars STAR NOTES: Part 1 What is a Star? A body of gases that gives off energy in the form of light and heat. 27.1: Characteristics of Stars Are all stars the same? No 1. Stars

More information

Chapter 11 Review. 1) Light from distant stars that must pass through dust arrives bluer than when it left its star. 1)

Chapter 11 Review. 1) Light from distant stars that must pass through dust arrives bluer than when it left its star. 1) Chapter 11 Review TRUE/FALSE. Write 'T' if the statement is true and 'F' if the statement is false. 1) Light from distant stars that must pass through dust arrives bluer than when it left its star. 1)

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

18. Which graph best represents the relationship between the number of sunspots and the amount of magnetic activity in the Sun?

18. Which graph best represents the relationship between the number of sunspots and the amount of magnetic activity in the Sun? 1. Which star has a surface temperature most similar to the surface temperature of Alpha Centauri? A) Polaris B) Betelgeuse C) Procyon B D) Sirius 2. Giant stars have greater luminosity than our sun mainly

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

3. c 4. a 5. f 6. b 7. e. 1. Stars are bright and hot. 2. Distances between stars are measured in light-years. 3. The sun is a yellow star.

3. c 4. a 5. f 6. b 7. e. 1. Stars are bright and hot. 2. Distances between stars are measured in light-years. 3. The sun is a yellow star. Stars, Galaxies, Use Target Reading Skills Check student definitions for accuracy. 1. Electromagnetic radiation is energy that can travel through space in the form of waves. 2. visible light 3. wavelength

More information

Directions: For numbers 1-30 please choose the letter that best fits the description.

Directions: For numbers 1-30 please choose the letter that best fits the description. Directions: For numbers 1-30 please choose the letter that best fits the description. 1. The main force responsible for the formation of the universe is: a. Gravity b. Frictional force c. Magnetic force

More information

Astronomy-part 3 notes Properties of Stars

Astronomy-part 3 notes Properties of Stars Astronomy-part 3 notes Properties of Stars What are Stars? Hot balls of that shine because nuclear fusion (hydrogen to helium) is happening at their cores. They create their own. Have different which allow

More information

ASTRONOMY 1 FINAL EXAM 1 Name

ASTRONOMY 1 FINAL EXAM 1 Name ASTRONOMY 1 FINAL EXAM 1 Name Multiple Choice (2 pts each) 1. Sullivan Star is an F spectral class star that is part of a binary star system. It has a MS lifetime of 5 billion years. Its life will eventually

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

ACTIVITIES for Grades 9-12

ACTIVITIES for Grades 9-12 ACTIVITIES for Grades 9-12 BEFORE YOUR VISIT Online Video: Journey to the Stars Trailer and Prelude To prepare for your Museum visit, watch the trailer and the prelude with your students. Class Discussion:

More information

Galaxies and Stars. 3. Base your answer to the following question on The reaction below represents an energy-producing process.

Galaxies and Stars. 3. Base your answer to the following question on The reaction below represents an energy-producing process. Galaxies and Stars 1. To an observer on Earth, the Sun appears brighter than the star Rigel because the Sun is A) hotter than Rigel B) more luminous than Rigel C) closer than Rigel D) larger than Rigel

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

Astronomy Part 1 Regents Questions

Astronomy Part 1 Regents Questions Regents Questions 1. The Sun revolves around the center of A) Polaris B) Aldebaran C) Earth D) the Milky Way Galaxy 4. In which sequence are the items listed from least total mass to greatest total mass?

More information

Cosmic Microwave Background Radiation

Cosmic Microwave Background Radiation Base your answers to questions 1 and 2 on the passage below and on your knowledge of Earth Science. Cosmic Microwave Background Radiation In the 1920s, Edwin Hubble's discovery of a pattern in the red

More information

chapter 31 Stars and Galaxies

chapter 31 Stars and Galaxies chapter 31 Stars and Galaxies Day 1:Technology and the Big Bang Studying the Stars A. Telescopes - Electromagnetic radiation emitted by stars and other objects include light, radio, and X-ray Space telescopes

More information

Stars. The composition of the star It s temperature It s lifespan

Stars. The composition of the star It s temperature It s lifespan Stars Stars A star is a ball of different elements in the form of gases The elements and gases give off electromagnetic radiation (from nuclear fusion) in the form of light Scientists study the light coming

More information

Stars & Galaxies. Chapter 27 Modern Earth Science

Stars & Galaxies. Chapter 27 Modern Earth Science Stars & Galaxies Chapter 27 Modern Earth Science Chapter 27, Section 1 27.1 Characteristics of Stars How do astronomers determine the composition and surface temperature of a star? Composition & Temperature

More information

CHAPTER 28 STARS AND GALAXIES

CHAPTER 28 STARS AND GALAXIES CHAPTER 28 STARS AND GALAXIES 28.1 A CLOSER LOOK AT LIGHT Light is a form of electromagnetic radiation, which is energy that travels in waves. Waves of energy travel at 300,000 km/sec (speed of light Ex:

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

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

29.2 M E A S U R I N G T H E S T A R S

29.2 M E A S U R I N G T H E S T A R S 29.2 M E A S U R I N G T H E S T A R S MAIN IDEA Stellar classification is based on measurement of light, spectra, temperature, and composition Describe the star life cycle Birth of a Star If enough matter

More information

Stars and Galaxies 1

Stars and Galaxies 1 Stars and Galaxies 1 Characteristics of Stars 2 Star - body of gases that gives off great amounts of radiant energy as light and heat 3 Most stars look white but are actually different colors Antares -

More information

CHAPTER 29: STARS BELL RINGER:

CHAPTER 29: STARS BELL RINGER: CHAPTER 29: STARS BELL RINGER: Where does the energy of the Sun come from? Compare the size of the Sun to the size of Earth. 1 CHAPTER 29.1: THE SUN What are the properties of the Sun? What are the layers

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

Light: Transverse WAVE

Light: Transverse WAVE Light Longitudinal WAVES Light: Transverse WAVE Light: Particle or wave Photon The Wave Nature of Light 1. Unlike other branches of science, astronomers cannot touch or do field work on their samples.

More information

One of the factors that misled Herschel into concluding that we are at the Universe's center was

One of the factors that misled Herschel into concluding that we are at the Universe's center was Homework 11! This is a preview of the draft version of the quiz Started: Apr 14 at 9:17am Quiz Instruc!ons Question 1 One of the factors that misled Herschel into concluding that we are at the Universe's

More information

Clicker Question: Clicker Question: What is the expected lifetime for a G2 star (one just like our Sun)?

Clicker Question: Clicker Question: What is the expected lifetime for a G2 star (one just like our Sun)? How Long do Stars Live (as Main Sequence Stars)? A star on Main Sequence has fusion of H to He in its core. How fast depends on mass of H available and rate of fusion. Mass of H in core depends on mass

More information

Universe Now. 9. Interstellar matter and star clusters

Universe Now. 9. Interstellar matter and star clusters Universe Now 9. Interstellar matter and star clusters About interstellar matter Interstellar space is not completely empty: gas (atoms + molecules) and small dust particles. Over 10% of the mass of the

More information

Universe Celestial Object Galaxy Solar System

Universe Celestial Object Galaxy Solar System ASTRONOMY Universe- Includes all known matter (everything). Celestial Object Any object outside or above Earth s atmosphere. Galaxy- A large group (billions) of stars (held together by gravity). Our galaxy

More information

c = l Light: The Cosmic Messenger 1/23/18

c = l Light: The Cosmic Messenger 1/23/18 Reading for today s and Thur class: ASTR 1040 Stars & Galaxies SDO: Post-flare ejection from solar surface Prof. Juri Toomre TAs: Peri Johnson, Ryan Horton Lecture 3 Tues 23 Jan 2018 zeus.colorado.edu/astr1040-toomre

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

Extrasolar Planets: Molecules and Disks

Extrasolar Planets: Molecules and Disks Extrasolar Planets: Molecules and Disks The basic question: Is our solar system typical of what we should affect around other stars (inhabited or not), or is it an unusual freak? One approach is to look

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

Test Name: 09.LCW.0352.SCIENCE.GR Q1.S.THEUNIVERSE-SOLARSYSTEMHONORS Test ID: Date: 09/21/2017

Test Name: 09.LCW.0352.SCIENCE.GR Q1.S.THEUNIVERSE-SOLARSYSTEMHONORS Test ID: Date: 09/21/2017 Test Name: 09.LCW.0352.SCIENCE.GR7.2017.Q1.S.THEUNIVERSE-SOLARSYSTEMHONORS Test ID: 243920 Date: 09/21/2017 Section 1.1 - According to the Doppler Effect, what happens to the wavelength of light as galaxies

More information

Midterm Results. The Milky Way in the Infrared. The Milk Way from Above (artist conception) 3/2/10

Midterm Results. The Milky Way in the Infrared. The Milk Way from Above (artist conception) 3/2/10 Lecture 13 : The Interstellar Medium and Cosmic Recycling Midterm Results A2020 Prof. Tom Megeath The Milky Way in the Infrared View from the Earth: Edge On Infrared light penetrates the clouds and shows

More information

Question: How do we use a Hertzsprung-Russell Diagram to explain star characteristics?

Question: How do we use a Hertzsprung-Russell Diagram to explain star characteristics? The Hertzsprung-Russell Diagram Assignment Introduction: The development of the H-R Diagram began with Danish astronomer Ejnar Hertzsprung who began plotting the stars around 1911. American astronomer

More information

Chapter 21: Stars Notes

Chapter 21: Stars Notes Branches of Earth Science Chapter 21: Stars Notes Astronomy: The study of planets, stars, and other objects in space. Lithosphere: the land masses of earth o Litho means rock Hydrosphere: waters of the

More information

ISP205-2 Visions of the Universe

ISP205-2 Visions of the Universe ISP205-2 Visions of the Universe The big questions Course details Example of how scientific discoveries are made Brief tour of the universe Reading for next class The Big Questions 1. Laws of physics.

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

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

Astronomy 10 Test #2 Practice Version

Astronomy 10 Test #2 Practice Version Given (a.k.a. `First ) Name(s): Family (a.k.a. `Last ) name: ON YOUR PARSCORE: `Bubble your name, your student I.D. number, and your multiple-choice answers. I will keep the Parscore forms. ON THIS TEST

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

TEK 8 Test Review. 15. Galaxies are best described as -

TEK 8 Test Review. 15. Galaxies are best described as - TEK 8 Test Review 1. List the three subatomic particles and give each of their masses. 2. Describe and draw an illustration (Bohr Model) of the most common element in the Universe. 3. Describe and draw

More information

The invisible universe

The invisible universe The Universe in my pocket The invisible universe No. 2 ES 001 Grażyna Stasińska Paris Observatory Galileo Galilei explains to the Doge of Venice how to use his telescope (Fresco by Giuseppe Bertini). The

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

At this point of its orbit, any solar satellite such as a comet or a planet is farthest away from the sun. What is the aphelion?

At this point of its orbit, any solar satellite such as a comet or a planet is farthest away from the sun. What is the aphelion? At this point of its orbit, any solar satellite such as a comet or a planet is farthest away from the sun. What is the aphelion? These small, rocky worlds orbit the sun generally between the orbits of

More information

The Hertzsprung-Russell Diagram

The Hertzsprung-Russell Diagram The Hertzsprung-Russell Diagram Name: Date: 1 Introduction As you may have learned in class, the Hertzsprung-Russell Diagram, or the HR diagram, is one of the most important tools used by astronomers:

More information

Astronomy 1143 Final Exam Review Answers

Astronomy 1143 Final Exam Review Answers Astronomy 1143 Final Exam Review Answers Prof. Pradhan April 24, 2015 What is Science? 1. Explain the difference between astronomy and astrology. 2. What number is the metric system based around? What

More information

GALAXIES AND STARS. 2. Which star has a higher luminosity and a lower temperature than the Sun? A Rigel B Barnard s Star C Alpha Centauri D Aldebaran

GALAXIES AND STARS. 2. Which star has a higher luminosity and a lower temperature than the Sun? A Rigel B Barnard s Star C Alpha Centauri D Aldebaran GALAXIES AND STARS 1. Compared with our Sun, the star Betelgeuse is A smaller, hotter, and less luminous B smaller, cooler, and more luminous C larger, hotter, and less luminous D larger, cooler, and more

More information

Stellar Evolution: from star birth to star death and back again

Stellar Evolution: from star birth to star death and back again Stellar Evolution: from star birth to star death and back again Prof. David Cohen Dept. of Physics and Astronomy This presentation is available at: astro.swarthmore.edu/~cohen/presentations/admitted_students_2006/

More information

Activity: Cosmic Colors and Spectroscopy

Activity: Cosmic Colors and Spectroscopy 1 Activity: Cosmic Colors and Spectroscopy Background: The energy of a photon of light depends on the wavelength (frequency) of the light higher frequency f = higher energy E = shorter wavelength λ) red

More information

Astronomy Unit Notes Name:

Astronomy Unit Notes Name: Astronomy Unit Notes Name: (DO NOT LOSE!) To help with the planets order 1 My = M 2 V = Venus 3 Eager = E 4 M = Mars 5 Just = J 6 Served = Saturn 7 Us = Uranus 8 N = N 1 Orbit: The path (usually elliptical)

More information

Astronomy. Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe.

Astronomy. Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe. Astronomy Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe. Universe = everything that exists Disclaimer: Astrology is NOT science!!!

More information

The Interstellar Medium (ch. 18)

The Interstellar Medium (ch. 18) The Interstellar Medium (ch. 18) The interstellar medium (ISM) is all the gas (and about 1% dust) that fills our Galaxy and others. It is the raw material from which stars form, and into which stars eject

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

8.8A describe components of the universe, including stars, nebulae, galaxies and use models such as HR diagrams for classification

8.8A describe components of the universe, including stars, nebulae, galaxies and use models such as HR diagrams for classification 8.8A describe components of the universe, including stars, nebulae, galaxies and use models such as HR diagrams for classification 8.8B recognize that the Sun is a medium-sized star near the edge of a

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

The Big Bang Theory (page 854)

The Big Bang Theory (page 854) Name Class Date Space Homework Packet Homework #1 Hubble s Law (pages 852 853) 1. How can astronomers use the Doppler effect? 2. The shift in the light of a galaxy toward the red wavelengths is called

More information

Chapter 17 Solar System

Chapter 17 Solar System Chapter 17 Solar System Rotation Earth spinning on its axis (like a top) "TOP" imaginary rod running through the center of the Earth from North pole to South pole The Earth is tilted on its axis at an

More information

Chapter Introduction Lesson 1 The View from Earth Lesson 2 The Sun and Other Stars Lesson 3 Evolution of Stars Lesson 4 Galaxies and the Universe

Chapter Introduction Lesson 1 The View from Earth Lesson 2 The Sun and Other Stars Lesson 3 Evolution of Stars Lesson 4 Galaxies and the Universe Chapter Introduction Lesson 1 The View from Earth Lesson 2 The Sun and Other Stars Lesson 3 Evolution of Stars Lesson 4 Galaxies and the Universe Chapter Wrap-Up What makes up the universe and how does

More information

Chapter 15 Star Birth. Star-Forming Clouds. Stars form in dark clouds of dusty gas in interstellar space

Chapter 15 Star Birth. Star-Forming Clouds. Stars form in dark clouds of dusty gas in interstellar space Chapter 15 Star Birth Star-Forming Clouds Stars form in dark clouds of dusty gas in interstellar space The gas between the stars is called the interstellar medium Visible light (Hubble Space Telescope)

More information

Stellar Astronomy Sample Questions for Exam 3

Stellar Astronomy Sample Questions for Exam 3 Stellar Astronomy Sample Questions for Exam 3 Chapter 7 1. A protostar is formed by a) the rapid expansion of gas from an exploding star. b) the gravitational collapse of a rotating interstellar cloud.

More information

Stars and Planets GPS S4E1 A-D: Students will compare and contrast the physical attributes of stars, star patterns, and planets. Ms.

Stars and Planets GPS S4E1 A-D: Students will compare and contrast the physical attributes of stars, star patterns, and planets. Ms. Stars and Planets GPS S4E1 A-D: Students will compare and contrast the physical attributes of stars, star patterns, and planets. Ms. D AngeloD Physical Attributes of Stars Number Size Color Pattern A star

More information

AST4930: Star and Planet Formation. Syllabus. AST4930: Star and Planet Formation, Spring 2014

AST4930: Star and Planet Formation. Syllabus. AST4930: Star and Planet Formation, Spring 2014 AST4930: Star and Planet Formation Lecture 1: Overview Assoc. Prof. Jonathan C. Tan jt@astro.ufl.edu Bryant 302 Syllabus AST4930: Star and Planet Formation, Spring 2014 Assoc. Prof. Jonathan C. Tan (jt

More information

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

The Universe. But first, let s talk about light! 2012 Pearson Education, Inc. The Universe But first, let s talk about light! Light is fast! The study of light All forms of radiation travel at 300,000,000 meters (186,000 miles) per second Since objects in space are so far away,

More information

The Universe. 3. Base your answer to the following question on The diagram below represents the bright-line spectrum for an element.

The Universe. 3. Base your answer to the following question on The diagram below represents the bright-line spectrum for an element. A) B) The Universe 1. According to the Big Bang theory, which graph hest represents the relationship between time and the size of the universe from the beginning of the universe to the present? C) D) 2.

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

Station #1 Galaxy Cards. Standard 4a: Students know galaxies are clusters of billions of stars and may have different shapes.

Station #1 Galaxy Cards. Standard 4a: Students know galaxies are clusters of billions of stars and may have different shapes. Station #1 Galaxy Cards Standard 4a: Students know galaxies are clusters of billions of stars and may have different shapes. Materials: Galaxy cards, your textbook Using your text book answers the following

More information

Light and Atoms. ASTR 1120 General Astronomy: Stars & Galaxies. ASTR 1120 General Astronomy: Stars & Galaxies !ATH REVIEW: #AST CLASS: "OMEWORK #1

Light and Atoms. ASTR 1120 General Astronomy: Stars & Galaxies. ASTR 1120 General Astronomy: Stars & Galaxies !ATH REVIEW: #AST CLASS: OMEWORK #1 ASTR 1120 General Astronomy: Stars & Galaxies!ATH REVIEW: Tonight, 5-6pm, in RAMY N1B23 "OMEWORK #1 -Due THU, Sept. 10, by 5pm, on Mastering Astronomy CLASS RECORDED STARTED - INFO WILL BE POSTED on CULEARN

More information

Test Natural Sciences 102 Section 8 noon --- VERSION A February 28, 2007

Test Natural Sciences 102 Section 8 noon --- VERSION A February 28, 2007 Correct responses indicated in boldface. 1. An astronomer is designing a new telescope to use in space. The Hubble Space Telescope operates at wavelengths close to 500nm ( 1nm = 10-9 meter). The new telescope

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

2019 Astronomy Team Selection Test

2019 Astronomy Team Selection Test 2019 Astronomy Team Selection Test Acton-Boxborough Regional High School Written by Antonio Frigo Do not flip over this page until instructed. Instructions You will have 45 minutes to complete this exam.

More information

Which of the following planets are all made up of gas? When a planets orbit around the Sun looks like an oval, it s called a(n)

Which of the following planets are all made up of gas? When a planets orbit around the Sun looks like an oval, it s called a(n) When a planets orbit around the Sun looks like an oval, it s called a(n) - ellipse - circle - axis - rotation Which of the following planets are all made up of gas? - Venus, Mars, Saturn and Pluto - Jupiter,

More information

M42 (The Orion Nebula) and M43

M42 (The Orion Nebula) and M43 3.4b demonstrate an understanding that emission nebulae, absorption nebulae and open clusters are associated with the birth of stars 3.4c demonstrate an understanding that planetary nebulae and supernovae

More information

Stellar Life Cycle in Giant Galactic Nebula NGC 3603

Stellar Life Cycle in Giant Galactic Nebula NGC 3603 Stellar Life Cycle in Giant Galactic Nebula NGC 3603 edited by David L. Alles Western Washington University e-mail: alles@biol.wwu.edu Last Updated 2009-11-20 Note: In PDF format most of the images in

More information

Solar System Formation/The Sun

Solar System Formation/The Sun Solar System Formation/The Sun Objective 4 Examine the orbital paths of planets and other astronomical bodies (comets and asteroids). Examine the theories of geocentric and heliocentric models and Kepler

More information

Chapter 19 Lecture. The Cosmic Perspective. Seventh Edition. Our Galaxy Pearson Education, Inc.

Chapter 19 Lecture. The Cosmic Perspective. Seventh Edition. Our Galaxy Pearson Education, Inc. Chapter 19 Lecture The Cosmic Perspective Seventh Edition Our Galaxy 19.1 The Milky Way Revealed Our goals for learning: Where are we located within our galaxy? What does our galaxy look like? How do stars

More information

BUT, what happens when atoms, with electrons attached, are packed really close together? The electrons from the neighboring atoms can have a small

BUT, what happens when atoms, with electrons attached, are packed really close together? The electrons from the neighboring atoms can have a small Quiz #5 There are two stars, star A and star B. Star A is approaching the Earth at 100 km/s and Star B is moving away from the Earth at 200 km/s. Compare the Doppler shift for these two stars by explaining

More information

Stellar Life Cycle in Giant Galactic Nebula NGC edited by David L. Alles Western Washington University

Stellar Life Cycle in Giant Galactic Nebula NGC edited by David L. Alles Western Washington University Stellar Life Cycle in Giant Galactic Nebula NGC 3603 edited by David L. Alles Western Washington University e-mail: alles@biol.wwu.edu Introduction NGC 3603 is a giant HII region in the Carina spiral arm

More information

Coriolis Effect - the apparent curved paths of projectiles, winds, and ocean currents

Coriolis Effect - the apparent curved paths of projectiles, winds, and ocean currents Regents Earth Science Unit 5: Astronomy Models of the Universe Earliest models of the universe were based on the idea that the Sun, Moon, and planets all orbit the Earth models needed to explain how the

More information

days to rotate in its own axis km in diameter ( 109 diameter of the Earth ) and kg in mass ( mass of the Earth)

days to rotate in its own axis km in diameter ( 109 diameter of the Earth ) and kg in mass ( mass of the Earth) The Sun - It is located at the centre of our solar system with all planets and objects (comets and asteroids) revolving around it Page 1 of 6 - It s gravitational pull keeps the planets and other objects

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

Life Cycle of a Star - Activities

Life Cycle of a Star - Activities Name: Class Period: Life Cycle of a Star - Activities A STAR IS BORN STAGES COMMON TO ALL STARS All stars start as a nebula. A nebula is a large cloud of gas and dust. Gravity can pull some of the gas

More information

FCAT Review Space Science

FCAT Review Space Science FCAT Review Space Science The Law of Universal Gravitation The law of universal gravitation states that ALL matter in the universe attracts each other. Gravity is greatly impacted by both mass and distance

More information

5E Lesson Plan Template

5E Lesson Plan Template Handout Authors: Ashley Thornburg Austin Ross Title of Lesson: The Life Cycle of Stars Date of Lesson: Wednesday March 14, 2012 Length of Lesson: 40-45 minutes Name/Level of Course: Science 8 th Source

More information

MIT Invitational, Jan Astronomy C. 2. You may separate the pages, but do not forget to put your team number at the top of all answer pages.

MIT Invitational, Jan Astronomy C. 2. You may separate the pages, but do not forget to put your team number at the top of all answer pages. MIT Invitational, Jan 2019 Astronomy C Competitors: School name: Team number: INSTRUCTIONS 1. Please turn in all materials at the end of the event. 2. You may separate the pages, but do not forget to put

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

Stars Star birth and kinds Elemental furnaces Star death and heavy elements

Stars Star birth and kinds Elemental furnaces Star death and heavy elements Stars Star birth and kinds Elemental furnaces Star death and heavy elements Matter was not uniformly distributed as the universe expanded after the Big Bang. This lumpy universe coalesced under the force

More information

Energy. mosquito lands on your arm = 1 erg. Firecracker = 5 x 10 9 ergs. 1 stick of dynamite = 2 x ergs. 1 ton of TNT = 4 x ergs

Energy. mosquito lands on your arm = 1 erg. Firecracker = 5 x 10 9 ergs. 1 stick of dynamite = 2 x ergs. 1 ton of TNT = 4 x ergs Energy mosquito lands on your arm = 1 erg Firecracker = 5 x 10 9 ergs 1 stick of dynamite = 2 x 10 13 ergs 1 ton of TNT = 4 x 10 16 ergs 1 atomic bomb = 1 x 10 21 ergs Magnitude 8 earthquake = 1 x 10 26

More information

OPTION E, ASTROPHYSICS TEST REVIEW

OPTION E, ASTROPHYSICS TEST REVIEW IB PHYSICS Name: DEVIL PHYSICS Period: Date: BADDEST CLASS ON CAMPUS OPTION E, ASTROPHYSICS TEST REVIEW S1. This question is about the nature of certain stars on the Hertzsprung-Russell diagram and determining

More information

Focusing on Light What is light? Is it a particle or a wave? An age-old debate that has persisted among scientists is related to the question, "Is

Focusing on Light What is light? Is it a particle or a wave? An age-old debate that has persisted among scientists is related to the question, Is Focusing on Light What is light? Is it a particle or a wave? An age-old debate that has persisted among scientists is related to the question, "Is light a wave or a stream of particles?" Very noteworthy

More information

If the whole universe has no meaning, we. should never have found out that it has no. meaning: just as, if there were no light in

If the whole universe has no meaning, we. should never have found out that it has no. meaning: just as, if there were no light in If the whole universe has no meaning, we should never have found out that it has no meaning: just as, if there were no light in the universe and therefore no creatures with eyes, we should never know it

More information

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

BROCK UNIVERSITY. Test 2: June 2016 Number of pages: 10 Course: ASTR 1P02, Section 2 Number of students: 359 BROCK UNIVERSITY Page 1 of 10 Test 2: June 2016 Number of pages: 10 Course: ASTR 1P02, Section 2 Number of students: 359 Examination date: 25 June 2016 Time limit: 50 min Time of Examination: 13:00 13:50

More information

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

Stars & Galaxies. Chapter 27, Section 1. Composition & Temperature. Chapter 27 Modern Earth Science Characteristics of Stars Stars & Galaxies Chapter 27 Modern Earth Science Chapter 27, Section 1 27.1 Characteristics of Stars Composition & Temperature Scientists use the following tools to study stars Telescope Observation Spectral

More information

Unit 1: Space. Section 2- Stars

Unit 1: Space. Section 2- Stars Unit 1: Space Section 2- Stars Stars Recall: stars are celestial bodies of hot gas that give off heat and light Stars The milky way contains hundreds of billions of stars and is only one of hundreds of

More information