Pretest Ch 20: Origins of the Universe

Size: px
Start display at page:

Download "Pretest Ch 20: Origins of the Universe"

Transcription

1 Name: _Answer key Pretest: _2_/ 58 Posttest: _58_/ 58 Pretest Ch 20: Origins of the Universe Vocab/Matching: Match the definition on the left with the term on the right by placing the letter of the term on the blank. 1. P the Doppler effect applied to light, shows A. Albert Einstein galaxies are moving away from us B. Big Bang 2. M where the universe has a low amount of C. Closed universe mass and will continue expanding forever D. Cosmic microwave 3. O discovered CMBR in the 1960s and proved background radiation the Big Bang Theory E. Dark matter 4. S everything that exists; all the matter and F. Edwin Hubble energy G. Fred Hoyle 5. Q the small point that everything that exists H. Fundamental forces was condensed into I. Georges Lemaitre 6. H gravity, electromagnetism, strong and weak J. Hypothesis molecular forces K. Law 7. J a scientific guess, based on a small amount M. Open universe of experimental evidence, may change N. Oscillating universe over time O. Penzias & Wilson 8. F used red shift to discover the universe is P. Red shift expanding, in 1920 s Q. Singularity 9. B theory that all that exists now was once in R. Theory one small point and started expanding S. Universe 10. E we can not see it, but can measure its effects; black holes are an example 11. R an explanation for a natural phenomenon, has much evidence to back it up, tends to be complex 12. A had the idea that the universe must not be static (unchanging) but had no evidence 13. D microwave energy left over from the Big Bang event that we can still measure today 14. N this is just one Big Bang in a series of Big Bangs/Big Crunches/Big Bangs/Big Crunches

2 15. G gave the Big Bang Theory its name while trying to make fun of it 16. I started the Big Bang theory, though he had no evidence to support it 17. K a simple statement that describes what happens in natural phenomenon 18. C the amount of matter in the universe is finite (set); the universe will collapse back in on itself or stay one size forever. If the following statement applies to a hypothesis, put a letter H. If it applies to a scientific theory, put the letter T. If it applies to a scientific law, put the letter L. It is possible to have more than one letter or no letters at all on a blank. 19. H an educated guess about a phenomenon 20. H can become a law 21. H T L can be changed 22. L describes a phenomenon (answers what ) 23. is more important than a theory 24. L tends to be simple, often just a mathematical equation 25. _T L has a lot of evidence to back it up 26. T explains a phenomenon (answers why or how ) 27. _T L is considered to be true or a fact by the scientific community 28. H can become a theory 29. H may not have evidence to back it up 30. _H T L can be proven false with further evidence/experimentation/observation 31. T tends to be very detailed and complex 32. _H T L_ can be used to make predictions

3 33. The following list identifies some of the events that have taken place according to Big Bang Theory. Put this list in a proper sequential order in time A. Formation of atoms (nuclei + electrons) B. The 4 fundamental forces of nature become distinguishable C. Supernova create conditions for the nuclear production of elements heavier than iron D. The first particles form from energy E. Something, not yet understood, causes the early universe (all of space and energy) to begin a process of rapid expansion from a singularity F. The first stars form initiating the nuclear fusion process to create the elements up through iron. G. Formation of galaxies H. Formation of simple atomic nuclei (combinations of protons and neutrons) E B D H A G F C 34. What needed to happen in the universe before it was possible for the first atoms to form? Cool down so energy could become matter (quarks eventually form atomic nuclei (protons & neutrons) then atoms) 35. What is so special about the time seconds after the initial bang? sec We don t know what happened before that. The models we use rely on 4 fundamental forces of physics.gravity, electromagnetism, weak molecular force, strong molecular force. Those forces had not existed before then they were all one superforce so we can t use science to explain what was happening, because science (as we know it) wasn t working then.

4 36. According to Big Bang Theory what significant event occurred approximately 300,000 years after the initial bang? first atoms were made (H & He) cooled down enough (about 3000 K). That cleared up the soup and allowed light to shine through. We detect this now as CMBR. 37. A very common misconception about the Big Bang is that people tend to view it as some giant explosion. Scientist wouldn t describe it this way. What would be a more appropriate description for what occurred at the very beginning according to Big Bang Theory? Rapid expansion from size of atom to 8x solar system in less than a second. The list on the left contains a few significant pieces of evidence that support some aspect of Big Bang Theory. For each item listed, describe the way in which it supports Big Bang Theory, briefly describe how this information is known, and identify the scientist(s) associated with the evidence. Evidence How it supports BBT Scientist(s) How is this known The universe is expanding 38. if expanding now, was once small in the past 39. Hubble, Red shift. Light from galaxies is shifted towards red end of spectrum means its moving away from us (Doppler Effect for light) Einstein, 1916 Theory of general Relativity says that objects with gravity

5 have to be moving, so universe can t just stay the same Lemaitre, 1927 Based on Einstein, predicted it would expand, couldn t prove, people ignored him Cosmic Microwave Background Radiation 41. The energy left over from the formation of the universe. Over time, it has shifted towards microwave end of spectrum. This light existed in early universe, but was blocked by all the unorganized matter. By 300,000 years after the Event, the universe had cooled down enough for the light to be seen. 42. Penzias & Wilson, 1964 (was predicted by others before that, but they actually found it) 43. BBT predicts there would be some residual energy left over that s not coming from 1 place in space, but has expanded (as the universe did) to come from all over. That s what CMBR does comes from everywhere.

6 Abundance of light elements (hydrogen and helium) in the universe 44. The conditions in the early universe would only make the simplest of elements Hydrogen and Helium. Thus we should find a lot of hydrogen and helium in the universe today. There have been many contributors to identifying composition % of the universe is Hydrogen and 25% is Helium. Other heavier elements came from stars processes (fusion) and supernovas (star explosions) as predicted by Hoyle. 46. Measurements of the red shift of light from distant galaxies informs scientists that the universe is expanding. What is red shift? Why does this show something is moving away from us? Red shift Doppler Effect applied to light. As objects move away from us, their wavelengths are stretched out (become longer) this shifts it towards the red end of the spectrum. The more it shifts the faster it is moving. If things move towards us, the wavelengths are compressed (shortened) and shifted towards the blue end of the spectrum.

7 Given the notion that the universe is currently expanding as described by Big Bang Theory, there are, in general, three possible outcomes for the future. Identify/describe those three possibilities for the fate of the universe: 47. Keep expanding forever (open universe, Big Rip) 48. Expand to a certain point and stop (flat universe, Big Freeze) 49. Expand to a certain point and contract again (closed universe, Big Crunch/Oscillating Universe)

8 50. What will determine which of the above scenarios actually happens? The amount of mass in the universe. The problem is that there is a lot of matter we can t see, but know it s there because of its gravitational effects (dark matter). So it s hard to measure the amount of mass. Describe how #50 will do this for each of #47 - #49 above. 51. If the amount of mass is over a certain limit, the universe will collapse back in on itself (closed universe/big Crunch) 52. If the amount of mass is just right the universe will grow to a certain size and stay there (Flat universe/big Freeze) 53. If the amount of mass is under the certain limit, it will just keep expanding forever (open universe, Big Rip) 54. Which of the three outcomes identified in seems to be supported by current data? Universe expanding forever (open universe/big Rip) there appears to be too low of an amount of mass for the gravity to stop the expansion or to stop it and bring everything back together. Hubble found that galaxies are speeding up the farther away they are, the faster they move (speeding up, not slowing down)

9 55. What is a galaxy and what is ours called? Collection of billions of stars. Ours is called the Milky Way and is estimated to contain between 200,000,000,000 and 400,000,000,000 stars. It is 100,000 ly across (light takes 100,000 years to cross it!) There are three shapes to galaxies. Name and draw them. What kind is ours? Elliptical Spirals (2 kinds spiral or barred spiral)

10 Irregular gravity of nearby objects gives it odd shape

Your years of toil Said Ryle to Hoyle Are wasted years, believe me. The Steady State Is out of date Unless my eyes deceive me.

Your years of toil Said Ryle to Hoyle Are wasted years, believe me. The Steady State Is out of date Unless my eyes deceive me. Your years of toil Said Ryle to Hoyle Are wasted years, believe me. The Steady State Is out of date Unless my eyes deceive me. My telescope Has dashed your hope; Your tenets are refuted. Let me be terse:

More information

Astro 102 Test 5 Review Spring 2016. See Old Test 4 #16-23, Test 5 #1-3, Old Final #1-14

Astro 102 Test 5 Review Spring 2016. See Old Test 4 #16-23, Test 5 #1-3, Old Final #1-14 Astro 102 Test 5 Review Spring 2016 See Old Test 4 #16-23, Test 5 #1-3, Old Final #1-14 Sec 14.5 Expanding Universe Know: Doppler shift, redshift, Hubble s Law, cosmic distance ladder, standard candles,

More information

Origins of the Cosmos Summer 2016. Pre-course assessment

Origins of the Cosmos Summer 2016. Pre-course assessment Origins of the Cosmos Summer 2016 Pre-course assessment In order to grant two graduate credits for the workshop, we do require you to spend some hours before arriving at Penn State. We encourage all of

More information

Chapter 15 Cosmology: Will the universe end?

Chapter 15 Cosmology: Will the universe end? Cosmology: Will the universe end? 1. Who first showed that the Milky Way is not the only galaxy in the universe? a. Kepler b. Copernicus c. Newton d. Hubble e. Galileo Ans: d 2. The big bang theory and

More information

The Expanding Universe

The Expanding Universe Stars, Galaxies, Guided Reading and Study This section explains how astronomers think the universe and the solar system formed. Use Target Reading Skills As you read about the evidence that supports the

More information

165 points. Name Date Period. Column B a. Cepheid variables b. luminosity c. RR Lyrae variables d. Sagittarius e. variable stars

165 points. Name Date Period. Column B a. Cepheid variables b. luminosity c. RR Lyrae variables d. Sagittarius e. variable stars Name Date Period 30 GALAXIES AND THE UNIVERSE SECTION 30.1 The Milky Way Galaxy In your textbook, read about discovering the Milky Way. (20 points) For each item in Column A, write the letter of the matching

More information

The Origin and Evolution of the Universe

The Origin and Evolution of the Universe The Origin and Evolution of the Universe 9.7 People have been wondering about the Universe for a long time. They have asked questions such as Where did the Universe come from? How big is it? What will

More information

The Birth of the Universe Newcomer Academy High School Visualization One

The Birth of the Universe Newcomer Academy High School Visualization One The Birth of the Universe Newcomer Academy High School Visualization One Chapter Topic Key Points of Discussion Notes & Vocabulary 1 Birth of The Big Bang Theory Activity 4A the How and when did the universe

More information

Chapter 23 The Beginning of Time

Chapter 23 The Beginning of Time Chapter 23 The Beginning of Time 23.1 The Big Bang Our goals for learning What were conditions like in the early universe? What is the history of the universe according to the Big Bang theory? What were

More information

1 A Solar System Is Born

1 A Solar System Is Born CHAPTER 3 1 A Solar System Is Born SECTION Formation of the Solar System BEFORE YOU READ After you read this section, you should be able to answer these questions: What is a nebula? How did our solar system

More information

Big bang, red shift and doppler effect

Big bang, red shift and doppler effect Big bang, red shift and doppler effect 73 minutes 73 marks Page of 26 Q. (a) Scientists have observed that the wavelengths of the light from galaxies moving away from the Earth are longer than expected.

More information

The Cosmic Microwave Background and the Big Bang Theory of the Universe

The Cosmic Microwave Background and the Big Bang Theory of the Universe The Cosmic Microwave Background and the Big Bang Theory of the Universe 1. Concepts from General Relativity 1.1 Curvature of space As we discussed earlier, Einstein s equivalence principle states that

More information

Transcript 22 - Universe

Transcript 22 - Universe Transcript 22 - Universe A few introductory words of explanation about this transcript: This transcript includes the words sent to the narrator for inclusion in the latest version of the associated video.

More information

A Century of Paradigm Shifts in our Thinking About the Universe

A Century of Paradigm Shifts in our Thinking About the Universe A Century of Paradigm Shifts in our Thinking About the Universe George R. Blumenthal Chancellor, UC Santa Cruz Professor of Astronomy and Astrophysics Why start 100 years ago? Before 1910 there was no

More information

Modeling Galaxy Formation

Modeling Galaxy Formation Galaxy Evolution is the study of how galaxies form and how they change over time. As was the case with we can not observe an individual galaxy evolve but we can observe different galaxies at various stages

More information

Topic 3. Evidence for the Big Bang

Topic 3. Evidence for the Big Bang Topic 3 Primordial nucleosynthesis Evidence for the Big Bang! Back in the 1920s it was generally thought that the Universe was infinite! However a number of experimental observations started to question

More information

Evolution of the Universe from 13 to 4 Billion Years Ago

Evolution of the Universe from 13 to 4 Billion Years Ago Evolution of the Universe from 13 to 4 Billion Years Ago Prof. Dr. Harold Geller hgeller@gmu.edu http://physics.gmu.edu/~hgeller/ Department of Physics and Astronomy George Mason University Unity in the

More information

Unit 1.7: Earth and Space Science The Structure of the Cosmos

Unit 1.7: Earth and Space Science The Structure of the Cosmos Lesson Summary: This week students will search for evidence provided in passages that lend support about the structure and organization of the Cosmos. Then students will summarize a passage. Materials

More information

STAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves

STAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves Name: Teacher: Pd. Date: STAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves TEK 8.8C: Explore how different wavelengths of the electromagnetic spectrum such as light and radio waves are used to

More information

Big Bang and Steady State Theories - Past exam questions (6 mark)

Big Bang and Steady State Theories - Past exam questions (6 mark) Big Bang and Steady State Theories - Past exam questions (6 mark) (1) * Scientists believe that the Universe is expanding. Describe how careful observation of electromagnetic radiation from distant galaxies

More information

The Universe. The Solar system, Stars and Galaxies

The Universe. The Solar system, Stars and Galaxies The Universe The Universe is everything. All us, the room, the U.S. the earth, the solar system, all the other stars in the Milky way galaxy, all the other galaxies... everything. How big and how old is

More information

The Doppler Effect & Hubble

The Doppler Effect & Hubble The Doppler Effect & Hubble Objectives Explain the Doppler Effect. Describe Hubble s discoveries. Explain Hubble s Law. The Doppler Effect The Doppler Effect is named after Austrian physicist Christian

More information

Big Bang Cosmology. Big Bang vs. Steady State

Big Bang Cosmology. Big Bang vs. Steady State Big Bang vs. Steady State Big Bang Cosmology Perfect cosmological principle: universe is unchanging in space and time => Steady-State universe - Bondi, Hoyle, Gold. True? No! Hubble s Law => expansion

More information

Build Your Own Universe

Build Your Own Universe Build Your Own Universe You will need: At least 10,000,000,000,000,00 0,000,000,000,000,000,000,00 0,000,000,000,000,000,000,00 0,000,000,000,000,000,000,00 0,000 x Down quarks At least 10,000,000,000,000,000,

More information

What is the Sloan Digital Sky Survey?

What is the Sloan Digital Sky Survey? What is the Sloan Digital Sky Survey? Simply put, the Sloan Digital Sky Survey is the most ambitious astronomical survey ever undertaken. The survey will map one-quarter of the entire sky in detail, determining

More information

Astronomy & Physics Resources for Middle & High School Teachers

Astronomy & Physics Resources for Middle & High School Teachers Astronomy & Physics Resources for Middle & High School Teachers Gillian Wilson http://www.faculty.ucr.edu/~gillianw/k12 A cosmologist is.... an astronomer who studies the formation and evolution of the

More information

UNIT V. Earth and Space. Earth and the Solar System

UNIT V. Earth and Space. Earth and the Solar System UNIT V Earth and Space Chapter 9 Earth and the Solar System EARTH AND OTHER PLANETS A solar system contains planets, moons, and other objects that orbit around a star or the star system. The solar system

More information

The first minutes of the Universe released energy which changed to matter, forming stars and galaxies. Introduction

The first minutes of the Universe released energy which changed to matter, forming stars and galaxies. Introduction THE COSMIC ENGINE CHAPTER 18 The Universe begins The first minutes of the Universe released energy which changed to matter, forming stars and galaxies Introduction Cosmology, the study of the Universe

More information

FXA 2008. UNIT G485 Module 5 5.5.1 Structure of the Universe. Δλ = v λ c CONTENTS OF THE UNIVERSE. Candidates should be able to :

FXA 2008. UNIT G485 Module 5 5.5.1 Structure of the Universe. Δλ = v λ c CONTENTS OF THE UNIVERSE. Candidates should be able to : 1 Candidates should be able to : CONTENTS OF THE UNIVERSE Describe the principal contents of the universe, including stars, galaxies and radiation. Describe the solar system in terms of the Sun, planets,

More information

1.1 A Modern View of the Universe" Our goals for learning: What is our place in the universe?"

1.1 A Modern View of the Universe Our goals for learning: What is our place in the universe? Chapter 1 Our Place in the Universe 1.1 A Modern View of the Universe What is our place in the universe? What is our place in the universe? How did we come to be? How can we know what the universe was

More information

WHERE DID ALL THE ELEMENTS COME FROM??

WHERE DID ALL THE ELEMENTS COME FROM?? WHERE DID ALL THE ELEMENTS COME FROM?? In the very beginning, both space and time were created in the Big Bang. It happened 13.7 billion years ago. Afterwards, the universe was a very hot, expanding soup

More information

Study Guide: Solar System

Study Guide: Solar System Study Guide: Solar System 1. How many planets are there in the solar system? 2. What is the correct order of all the planets in the solar system? 3. Where can a comet be located in the solar system? 4.

More information

World of Particles Big Bang Thomas Gajdosik. Big Bang (model)

World of Particles Big Bang Thomas Gajdosik. Big Bang (model) Big Bang (model) What can be seen / measured? basically only light (and a few particles: e ±, p, p, ν x ) in different wave lengths: microwave to γ-rays in different intensities (measured in magnitudes)

More information

Solar Energy Production

Solar Energy Production Solar Energy Production We re now ready to address the very important question: What makes the Sun shine? Why is this such an important topic in astronomy? As humans, we see in the visible part of the

More information

Week 1-2: Overview of the Universe & the View from the Earth

Week 1-2: Overview of the Universe & the View from the Earth Week 1-2: Overview of the Universe & the View from the Earth Hassen M. Yesuf (hyesuf@ucsc.edu) September 29, 2011 1 Lecture summary Protein molecules, the building blocks of a living organism, are made

More information

The History and Philosophy of Astronomy

The History and Philosophy of Astronomy Astronomy 350L (Fall 2006) The History and Philosophy of Astronomy (Lecture 23: Steady State vs Big Bang) Instructor: Volker Bromm TA: Jarrett Johnson The University of Texas at Austin Steady State vs

More information

Carol and Charles see their pencils fall exactly straight down.

Carol and Charles see their pencils fall exactly straight down. Section 24-1 1. Carol is in a railroad car on a train moving west along a straight stretch of track at a constant speed of 120 km/h, and Charles is in a railroad car on a train at rest on a siding along

More information

23. The Beginning of Time. Agenda. Agenda. ESA s Venus Express. Conditions in the Early Universe. 23.1 Running the Expansion Backward

23. The Beginning of Time. Agenda. Agenda. ESA s Venus Express. Conditions in the Early Universe. 23.1 Running the Expansion Backward 23. The Beginning of Time Somewhere, something incredible is waiting to be known. Agenda Announce: Solar Altitude Lab (#2) due today Read Ch. 24 for Thursday Observation make-up next week Project Presentations

More information

Einstein s cosmological legacy: From the big bang to black holes

Einstein s cosmological legacy: From the big bang to black holes School of Mathematical and Computing Sciences Te Kura Pangarau, Rorohiko Einstein s cosmological legacy: From the big bang to black holes Matt Visser Overview: 2005 marks 100 years since Einstein discovered

More information

Class 2 Solar System Characteristics Formation Exosolar Planets

Class 2 Solar System Characteristics Formation Exosolar Planets Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System

More information

Where is Fundamental Physics Heading? Nathan Seiberg IAS Apr. 30, 2014

Where is Fundamental Physics Heading? Nathan Seiberg IAS Apr. 30, 2014 Where is Fundamental Physics Heading? Nathan Seiberg IAS Apr. 30, 2014 Disclaimer We do not know what will be discovered. This is the reason we perform experiments. This is the reason scientific research

More information

Answers for the Student Worksheet for the Hubble Space Telescope Scavenger Hunt

Answers for the Student Worksheet for the Hubble Space Telescope Scavenger Hunt Instructions: Answers are typed in blue. Answers for the Student Worksheet for the Hubble Space Telescope Scavenger Hunt Crab Nebula What is embedded in the center of the nebula? Neutron star Who first

More information

Particle Soup: Big Bang Nucleosynthesis

Particle Soup: Big Bang Nucleosynthesis Name: Partner(s): Lab #7 Particle Soup: Big Bang Nucleosynthesis Purpose The student explores how helium was made in the Big Bang. Introduction Very little helium is made in stars. Yet the universe is

More information

First Discoveries. Asteroids

First Discoveries. Asteroids First Discoveries The Sloan Digital Sky Survey began operating on June 8, 1998. Since that time, SDSS scientists have been hard at work analyzing data and drawing conclusions. This page describes seven

More information

Test 2 --- Natural Sciences 102, Professors Rieke --- VERSION B March 3, 2010

Test 2 --- Natural Sciences 102, Professors Rieke --- VERSION B March 3, 2010 Enter your answers on the form provided. Be sure to write your name and student ID number on the first blank at the bottom of the form. Please mark the version (B) in the Key ID space at the top of the

More information

Introduction to the Solar System

Introduction to the Solar System Introduction to the Solar System Lesson Objectives Describe some early ideas about our solar system. Name the planets, and describe their motion around the Sun. Explain how the solar system formed. Introduction

More information

7. In which part of the electromagnetic spectrum are molecules most easily detected? A. visible light B. radio waves C. X rays D.

7. In which part of the electromagnetic spectrum are molecules most easily detected? A. visible light B. radio waves C. X rays D. 1. Most interstellar matter is too cold to be observed optically. Its radiation can be detected in which part of the electromagnetic spectrum? A. gamma ray B. ultraviolet C. infrared D. X ray 2. The space

More information

3 HOW WERE STARS FORMED?

3 HOW WERE STARS FORMED? 3 HOW WERE STARS FORMED? David Christian explains how the first stars were formed. This two-part lecture begins by focusing on what the Universe was like in its first 200 million years of existence, a

More information

Welcome to Class 4: Our Solar System (and a bit of cosmology at the start) Remember: sit only in the first 10 rows of the room

Welcome to Class 4: Our Solar System (and a bit of cosmology at the start) Remember: sit only in the first 10 rows of the room Welcome to Class 4: Our Solar System (and a bit of cosmology at the start) Remember: sit only in the first 10 rows of the room What is the difference between dark ENERGY and dark MATTER? Is Earth unique,

More information

A Universe of Galaxies

A Universe of Galaxies A Universe of Galaxies Today s Lecture: Other Galaxies (Chapter 16, pages 366-397) Types of Galaxies Habitats of Galaxies Dark Matter Other Galaxies Originally called spiral nebulae because of their shape.

More information

The facts we know today will be the same tomorrow but today s theories may tomorrow be obsolete.

The facts we know today will be the same tomorrow but today s theories may tomorrow be obsolete. The Scale of the Universe Some Introductory Material and Pretty Pictures The facts we know today will be the same tomorrow but today s theories may tomorrow be obsolete. A scientific theory is regarded

More information

Science Standard 4 Earth in Space Grade Level Expectations

Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal

More information

Modeling the Expanding Universe

Modeling the Expanding Universe H9 Modeling the Expanding Universe Activity H9 Grade Level: 8 12 Source: This activity is produced by the Universe Forum at NASA s Office of Space Science, along with their Structure and Evolution of the

More information

Chapter 15.3 Galaxy Evolution

Chapter 15.3 Galaxy Evolution Chapter 15.3 Galaxy Evolution Elliptical Galaxies Spiral Galaxies Irregular Galaxies Are there any connections between the three types of galaxies? How do galaxies form? How do galaxies evolve? P.S. You

More information

Beginning of the Universe Classwork 6 th Grade PSI Science

Beginning of the Universe Classwork 6 th Grade PSI Science Beginning of the Universe Classwork Name: 6 th Grade PSI Science 1 4 2 5 6 3 7 Down: 1. Edwin discovered that galaxies are spreading apart. 2. This theory explains how the Universe was flattened. 3. All

More information

Chapter 1: Our Place in the Universe. 2005 Pearson Education Inc., publishing as Addison-Wesley

Chapter 1: Our Place in the Universe. 2005 Pearson Education Inc., publishing as Addison-Wesley Chapter 1: Our Place in the Universe Topics Our modern view of the universe The scale of the universe Cinema graphic tour of the local universe Spaceship earth 1.1 A Modern View of the Universe Our goals

More information

The Hidden Lives of Galaxies. Jim Lochner, USRA & NASA/GSFC

The Hidden Lives of Galaxies. Jim Lochner, USRA & NASA/GSFC The Hidden Lives of Galaxies Jim Lochner, USRA & NASA/GSFC What is a Galaxy? Solar System Distance from Earth to Sun = 93,000,000 miles = 8 light-minutes Size of Solar System = 5.5 light-hours What is

More information

Exploring the Universe Through the Hubble Space Telescope

Exploring the Universe Through the Hubble Space Telescope Exploring the Universe Through the Hubble Space Telescope WEEK FIVE: THE HUBBLE DEEP FIELD + LIMITATIONS OF HUBBLE, COLLABORATIONS, AND THE FUTURE OF ASTRONOMY Date: October 14, 2013 Instructor: Robert

More information

Remodelling the Big Bang

Remodelling the Big Bang Remodelling the Big Bang Dewey B. Larson Unquestionably, the most significant development that has taken place in cosmology in recent years is the replacement of the original Big Bang theory by a totally

More information

The Big Bang A Community in the Classroom Presentation for Grade 5

The Big Bang A Community in the Classroom Presentation for Grade 5 The Big Bang A Community in the Classroom Presentation for Grade 5 Richard Cupp Engineer STANARDS CONNECTION Grade 5 Physical Science: Elements and their combinations account for all the varied types of

More information

REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe

REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe REALIZING EINSTEIN S DREAM Exploring Our Mysterious Universe The End of Physics Albert A. Michelson, at the dedication of Ryerson Physics Lab, U. of Chicago, 1894 The Miracle Year - 1905 Relativity Quantum

More information

How To Understand General Relativity

How To Understand General Relativity Chapter S3 Spacetime and Gravity What are the major ideas of special relativity? Spacetime Special relativity showed that space and time are not absolute Instead they are inextricably linked in a four-dimensional

More information

THE BIG BANG HOW CLOSE CAN WE COME? Michael Dine Final Lecture Physics 171, 2009

THE BIG BANG HOW CLOSE CAN WE COME? Michael Dine Final Lecture Physics 171, 2009 THE BIG BANG HOW CLOSE CAN WE COME? Michael Dine Final Lecture Physics 171, 2009 New York Times: April, 2003 Reports a debate among cosmologists about the Big Bang. lll1.html Dr. Tyson, who introduced

More information

Introduction. The activity. Part 1 predictions and outcomes. Part 2 a dialogue concerning the origin of the Universe. And so to the Big Bang.

Introduction. The activity. Part 1 predictions and outcomes. Part 2 a dialogue concerning the origin of the Universe. And so to the Big Bang. Teacher Notes Introduction And so to the Big Bang. The activity Part 1 predictions and outcomes This introduces Big Bang theory by looking at some of its predictions. The first one was a failed prediction,

More information

The Sun and Solar Energy

The Sun and Solar Energy I The Sun and Solar Energy One of the most important forces behind global change on Earth is over 90 million miles distant from the planet. The Sun is the ultimate, original source of the energy that drives

More information

Cosmic Journey: Teacher Packet

Cosmic Journey: Teacher Packet Cosmic Journey: Teacher Packet Compiled by: Morehead State University Star Theatre with help from Bethany DeMoss Table of Contents Table of Contents 1 Corresponding Standards 2 Vocabulary 4 Sizing up the

More information

GRAVITY CONCEPTS. Gravity is the universal force of attraction between all matter

GRAVITY CONCEPTS. Gravity is the universal force of attraction between all matter IT S UNIVERSAL GRAVITY CONCEPTS Gravity is the universal force of attraction between all matter Weight is a measure of the gravitational force pulling objects toward Earth Objects seem weightless when

More information

The spectacular eruption of a volcano, the magnificent scenery of a

The spectacular eruption of a volcano, the magnificent scenery of a Section 1.1 1.1 What Is Earth Science 1 FOCUS Section Objectives 1.1 Define Earth science. 1.2 Describe the formation of Earth and the solar system. Build Vocabulary Word Parts Ask students to use a dictionary

More information

Background Biology and Biochemistry Notes A

Background Biology and Biochemistry Notes A Background Biology and Biochemistry Notes A Vocabulary dependent variable evidence experiment hypothesis independent variable model observation prediction science scientific investigation scientific law

More information

Stellar Evolution: a Journey through the H-R Diagram

Stellar Evolution: a Journey through the H-R Diagram Stellar Evolution: a Journey through the H-R Diagram Mike Montgomery 21 Apr, 2001 0-0 The Herztsprung-Russell Diagram (HRD) was independently invented by Herztsprung (1911) and Russell (1913) They plotted

More information

5. The Nature of Light. Does Light Travel Infinitely Fast? EMR Travels At Finite Speed. EMR: Electric & Magnetic Waves

5. The Nature of Light. Does Light Travel Infinitely Fast? EMR Travels At Finite Speed. EMR: Electric & Magnetic Waves 5. The Nature of Light Light travels in vacuum at 3.0. 10 8 m/s Light is one form of electromagnetic radiation Continuous radiation: Based on temperature Wien s Law & the Stefan-Boltzmann Law Light has

More information

SYLLABUS FORM WESTCHESTER COMMUNITY COLLEGE Valhalla, NY l0595. l. Course #:PHYSC 151 2. NAME OF ORIGINATOR /REVISOR: PAUL ROBINSON

SYLLABUS FORM WESTCHESTER COMMUNITY COLLEGE Valhalla, NY l0595. l. Course #:PHYSC 151 2. NAME OF ORIGINATOR /REVISOR: PAUL ROBINSON SYLLABUS FORM WESTCHESTER COMMUNITY COLLEGE Valhalla, NY l0595 l. Course #:PHYSC 151 2. NAME OF ORIGINATOR /REVISOR: PAUL ROBINSON NAME OF COURSE: ASTRONOMY 3. CURRENT DATE: OCTOBER 26, 2011. Please indicate

More information

TEACHER BACKGROUND INFORMATION THERMAL ENERGY

TEACHER BACKGROUND INFORMATION THERMAL ENERGY TEACHER BACKGROUND INFORMATION THERMAL ENERGY In general, when an object performs work on another object, it does not transfer all of its energy to that object. Some of the energy is lost as heat due to

More information

A Day Without Yesterday: Georges Lemaitre & the Big Bang

A Day Without Yesterday: Georges Lemaitre & the Big Bang A Day Without Yesterday: Georges Lemaitre & the Big Bang MARK MIDBON In January 1933, the Belgian mathematician and Catholic priest Georges Lemaitre traveled with Albert Einstein to California for a series

More information

The Universe Inside of You: Where do the atoms in your body come from?

The Universe Inside of You: Where do the atoms in your body come from? The Universe Inside of You: Where do the atoms in your body come from? Matthew Mumpower University of Notre Dame Thursday June 27th 2013 Nucleosynthesis nu cle o syn the sis The formation of new atomic

More information

Part 1 Composition of Earth Composition of solar system Origin of the elements Part 2 Geochronometry: Age of Earth Formation of Earth and Moon.

Part 1 Composition of Earth Composition of solar system Origin of the elements Part 2 Geochronometry: Age of Earth Formation of Earth and Moon. Part 1 Composition of Earth Composition of solar system Origin of the elements Part 2 Geochronometry: Age of Earth Formation of Earth and Moon. Differentiation of core and mantle. Isotope tracing: sequence

More information

TELESCOPE AS TIME MACHINE

TELESCOPE AS TIME MACHINE TELESCOPE AS TIME MACHINE Read this article about NASA s latest high-tech space telescope. Then, have fun doing one or both of the word puzzles that use the important words in the article. A TELESCOPE

More information

From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation?

From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation? From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation? From lowest energy to highest energy, which of the following correctly

More information

Kinetic Theory. Energy. Transfers and Efficiency. The National Grid

Kinetic Theory. Energy. Transfers and Efficiency. The National Grid AQA P1 Revision Infrared Radiation Heating and Insulating Buildings Kinetic Theory Energy Transfers and Efficiency Energy Transfer by Heating Transferring Electrical Energy Generating Electricity The National

More information

thermal history of the universe and big bang nucleosynthesis

thermal history of the universe and big bang nucleosynthesis thermal history of the universe and big bang nucleosynthesis Kosmologie für Nichtphysiker Markus Pössel (vertreten durch Björn Malte Schäfer) Fakultät für Physik und Astronomie, Universität Heidelberg

More information

Final. Mark Scheme. Additional Science / Physics (Specification 4408 / 4403) PH2FP. Unit: Physics 2

Final. Mark Scheme. Additional Science / Physics (Specification 4408 / 4403) PH2FP. Unit: Physics 2 Version.0 General Certificate of Secondary Education January 203 Additional Science / Physics (Specification 4408 / 4403) Unit: Physics 2 Final Mark Scheme Mark schemes are prepared by the Principal Examiner

More information

Objectives 404 CHAPTER 9 RADIATION

Objectives 404 CHAPTER 9 RADIATION Objectives Explain the difference between isotopes of the same element. Describe the force that holds nucleons together. Explain the relationship between mass and energy according to Einstein s theory

More information

Name: Date: Period: Gravity Study Guide

Name: Date: Period: Gravity Study Guide Vocabulary: Define the following terms. Law of Universal Gravitation Gravity Study Guide Weight Weightlessness Gravitational Field Black hole Escape velocity Math: Be able to use the equation for the law

More information

Chemical Building Blocks: Chapter 3: Elements and Periodic Table

Chemical Building Blocks: Chapter 3: Elements and Periodic Table Name: Class: Date: Chemical Building Blocks: Chapter 3: Elements and Periodic Table Study Guide Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.

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

The Location of the Missing Dark Matter A.G. Kelly.

The Location of the Missing Dark Matter A.G. Kelly. The Location of the Missing Dark Matter A.G. Kelly. Abstract. A source of most of the missing Dark Matter is proposed. If the formation of stars was at a time, and in a position, such that the light from

More information

Why Does the Sun Shine?

Why Does the Sun Shine? Why Does the Sun Shine? Is the Sun on Fire? Fire (oxidation) produces light and heat, just like the Sun. Source: chemical potential energy Suppose the Sun were made of carbon and oxygen. The Sun could

More information

Top 10 Discoveries by ESO Telescopes

Top 10 Discoveries by ESO Telescopes Top 10 Discoveries by ESO Telescopes European Southern Observatory reaching new heights in astronomy Exploring the Universe from the Atacama Desert, in Chile since 1964 ESO is the most productive astronomical

More information

Activity: Multiwavelength Bingo

Activity: Multiwavelength Bingo ctivity: Multiwavelength background: lmost everything that we know about distant objects in the Universe comes from studying the light that is emitted or reflected by them. The entire range of energies

More information

Chapter 1 Our Place in the Universe

Chapter 1 Our Place in the Universe Chapter 1 Our Place in the Universe Syllabus 4 tests: June 18, June 30, July 10, July 21 Comprehensive Final - check schedule Website link on blackboard 1.1 Our Modern View of the Universe Our goals for

More information

Indiana's Academic Standards 2010 ICP Indiana's Academic Standards 2016 ICP. map) that describe the relationship acceleration, velocity and distance.

Indiana's Academic Standards 2010 ICP Indiana's Academic Standards 2016 ICP. map) that describe the relationship acceleration, velocity and distance. .1.1 Measure the motion of objects to understand.1.1 Develop graphical, the relationships among distance, velocity and mathematical, and pictorial acceleration. Develop deeper understanding through representations

More information

An Introduction to Astronomy and Cosmology. 1) Astronomy - an Observational Science

An Introduction to Astronomy and Cosmology. 1) Astronomy - an Observational Science An Introduction to Astronomy and Cosmology 1) Astronomy - an Observational Science Why study Astronomy 1 A fascinating subject in its own right. The origin and Evolution of the universe The Big Bang formation

More information

Malcolm S. Longair. Galaxy Formation. With 141 Figures and 12 Tables. Springer

Malcolm S. Longair. Galaxy Formation. With 141 Figures and 12 Tables. Springer Malcolm S. Longair Galaxy Formation With 141 Figures and 12 Tables Springer Contents Part I Preliminaries 1. Introduction, History and Outline 3 1.1 Prehistory 3 1.2 The Theory of the Expanding Universe

More information

2. The Universe Is Expanding and Evolving

2. The Universe Is Expanding and Evolving 2. The Universe Is Expanding and Evolving We now know that the entire universe is both expanding and evolving. These two remarkable facts have been established beyond doubt over the past century. The simple

More information

1. The Kinetic Theory of Matter states that all matter is composed of atoms and molecules that are in a constant state of constant random motion

1. The Kinetic Theory of Matter states that all matter is composed of atoms and molecules that are in a constant state of constant random motion Physical Science Period: Name: ANSWER KEY Date: Practice Test for Unit 3: Ch. 3, and some of 15 and 16: Kinetic Theory of Matter, States of matter, and and thermodynamics, and gas laws. 1. The Kinetic

More information

Light as a Wave. The Nature of Light. EM Radiation Spectrum. EM Radiation Spectrum. Electromagnetic Radiation

Light as a Wave. The Nature of Light. EM Radiation Spectrum. EM Radiation Spectrum. Electromagnetic Radiation The Nature of Light Light and other forms of radiation carry information to us from distance astronomical objects Visible light is a subset of a huge spectrum of electromagnetic radiation Maxwell pioneered

More information

ELEMENTS OF PHYSICS MOTION, FORCE, AND GRAVITY

ELEMENTS OF PHYSICS MOTION, FORCE, AND GRAVITY 1 Pre-Test Directions: This will help you discover what you know about the subject of motion before you begin this lesson. Answer the following true or false. 1. Aristotle believed that all objects fell

More information

In studying the Milky Way, we have a classic problem of not being able to see the forest for the trees.

In studying the Milky Way, we have a classic problem of not being able to see the forest for the trees. In studying the Milky Way, we have a classic problem of not being able to see the forest for the trees. A panoramic painting of the Milky Way as seen from Earth, done by Knut Lundmark in the 1940 s. The

More information

Einstein s theory of relativity

Einstein s theory of relativity Department of Mathematics, Institute of Origins, December 5, 2008 Overview UCL Institute of Origins Origins UCL has established the Institute of Origins to promote world leading research in topics related

More information

Introduction and Origin of the Earth

Introduction and Origin of the Earth Page 1 of 5 EENS 1110 Tulane University Physical Geology Prof. Stephen A. Nelson Introduction and Origin of the Earth This page last updated on 30-Jul-2015 Geology, What is it? Geology is the study of

More information