Back of chapters have additional Resources and various tutorials to help you getting acquainted With the subject Also exercises you can do for extra
|
|
- Gilbert Snow
- 5 years ago
- Views:
Transcription
1 Astronomy 100 Instructor: Prof. Irv Robbins Office:1N, room 233 Office Phone: Observatory Course requirements are at the Observatory Web site Via CSI web site then quick links to astrophysical observatory then by my NAME link, Also when logging into the Mastering Astronomy(MA) web site in the announcements There you will find tutorials, the course homework and chapter short exams First day notes you receive are a SUMMARY
2 Back of chapters have additional Resources and various tutorials to help you getting acquainted With the subject Also exercises you can do for extra credit->
3 KEEP IN MIND: THIS IS A WEB AUGMENTED COURSE ONLINE HOMEWORK 15% ONLINE EXAMS 20% =35% Mastering Astronomy website THESE ON LINE ASSIGNMENTS ARE AVAILABLE AS SOON AS A CHAPTER IS STARTED IN CLASS. YOU WILL SEE DUE DATES AND IN GENERAL HAVE 2 to 2 1/2 WEEKS BEFORE SIGNIFICANT LATE PENALITIES INCUR. Did the dude Say somtin? I think he means at 35% We better do it or Drop the class!
4 Observing Requirement -5% Report on 2 observations: use forms found on line or in back of the Lab manual CAN BE DONE AT ONE SESSION..ADDITIONAL ONES ARE EXTRA CREDIT. WHERE? CSI Observatory (open monthly see schedule on line Astrophysical Observatory website or local AAA observings Saturday nights in SI, Friday Night in Brooklyn or observatories in NJ These events are weather dependent so get it done early or a term paper as described at the web sites Is required. SEE LINKS AT MA AND OBSERVATORY WEB SITE
5 Extra Credit MAXIMUM of 5 points on final average ON UNDER THE GENERAL REQUIREMENTS LINK YOU WILL FIND ALSO ALL ASSIGNMENTS CONTAIN EXTRA CREDIT POSSIBILITIES. NOTE: IN CLASS MIDTERM and FINAL EXAMS 100 SHORT ANSWERS CRIB SHEETS (3) ALLOWED 2 PERIOD EXAMS=60% OF YOUR GRADE.
6 CHECK THESE LINKS OUT YOU WON T BE SORRY! HOW TO USE THE ONLINE CHAPTER REVIEWS AND TUTORIALS AND OTHER RESOURCES TO GET A GOOD GRADE HOW TO SUCCEED IN THIS ASTRONOMY COURSE
7 + ADDITIONAL VOLUNTEER EXTRA CREDIT ( depending on quality of work done). ATTENDANCE MONITOR, OBSERVING REPORT COLLECTOR AND GRADER Observatory Workers AUDIO MONITOR(sets up portable mic) Enter on the forms you receive in class, as well as, seating preference in room=your LEFT,RIGHT, Front, Back, Aisle seat (justify please). NORMALLY NO SPECICFIC SEAT WILL BE HONORED
8 Chapter 1 Our Place in the Universe
9 1.1 A Modern View of the Universe What is our place in the universe? Voids On the Large scale we first learned that Earth is a sphere some 2,500 years ago; we learned that Earth is a planet going around the Sun only about 400 years ago; and we learned that the Millky Way is only one of many galaxies with the work of Hubble some 80 years ago
10 Scale of the Universe Powers of Ten ---Eames film
11 Star A large, glowing ball of gas that generates heat and light through nuclear fusion
12 Planet Mars Neptune A moderately large object that orbits a star; it shines by reflected light. Planets may be rocky, icy, or gaseous in composition.
13 Moon (or satellite) An object that orbits a planet. Ganymede (orbits Jupiter) artificial objects (spacecraft) are usually called satellites and not moons
14 Asteroid A relatively small and rocky object that orbits a star. Ida (1) Note the non-spherical shape; small objects are often non-spherical because their gravity is not strong enough to compress the material into a sphere. (2) Asteroids are sometimes called minor planets because they orbit much like planets but are smaller than anything we consider to be a true planet.
15 Comet A relatively small and icy object that orbits a star. Halley s comet close-up. (1) the basic difference between an asteroid and a comet is composition; (2) (2) comets have tails ONLY when they come close to the Sun, not when they are much farther away.
16 A star and all the material that orbits it, including its planets and moons Solar (Star) System
17 Figure 1.9
18 Nebula Cloud like: Check out the Orion Nebula Birth place of stars An interstellar cloud of gas and/or dust Crab Nebula- Remnants of a Supernova Explosion But Andromeda Nebula is the nearest Spiral Galaxy to us (our Milky way)
19 Galaxy A great island of stars in space, all held 3 galaxies Large spiral Andromeda And 2 dwarfs elliptical together by gravity and orbiting a common center M31, The Great Galaxy in Andromeda common problems is confusion between the terms solar system and galaxy.
20 Universe The sum total of all matter and energy; that is, everything within and between all galaxies
21 How did we come to be? Hot & Dense Big Bang ->Expanding H&He->all other elements Galalxy recycles Birth Home, sweet home Life ->elements
22 Thus, we see objects as they were in the past: The farther away we look in distance, the further back we look in time. How can we know what the universe is like? We see by light (and other energies) Light travels at a finite speed (300,000 km/s). Or 186,000 mi/s circle earth about 8 times/sec Moon Sun Destination Light travel time 1 second 8 minutes Sirius 8 years Andromeda Galaxy 2.5 million years
23 Example: We see the Orion Nebula as it looked 1,500 years ago. M31, The Great Galaxy in Andromeda
24 Example: This photo shows the Andromeda Galaxy as it looked about 2 1/2 million years ago. Question: When will be able to see what it looks like now? photo also shows 100,000 years of time? M31, The Great Galaxy in Andromeda
25 Light-year The distance light can travel in one year. About 10 trillion km (6 trillion miles).
26 At great distances, we see objects as they were when the universe was much younger.
27 How far is a light-year? Distance=rate x time (60mi/hr x 3hr)=? Distance =km/s x s(in a year) 1light - year = (speed of light) (1 year) = 300,000 km s 365 days 24 hr 1 yr 1 day 60 min 1 hr 60 s 1 min Total number of seconds in a year Extra credit: Do this 1ly=?km Not accepted after a week!!!!
28 How far is a light-year? 1light - year = (speed of light) (1 year) = 300,000 km s = 9,460,000,000,000 km 365 days 24 hr 1 yr 1 day 60 min 1 hr 60 s 1 min Note: a light-year is a unit of distance NOT a unit of time.
29 Can we see the entire universe?
30 Thought Question Why can t we see a galaxy 15 billion light-years away? (Assume universe is 14 billion years old.) A. Because no galaxies exist at such a great distance. B. Galaxies may exist at that distance, but their light would be too faint for our telescopes to see. C. Because looking 15 billion light-years away means looking to a time before the universe existed.
31 Thought Question Why can t we see a galaxy 15 billion light-years away? (Assume universe is 14 billion years old.) A. Because no galaxies exist at such a great distance. B. Galaxies may exist at that distance, but their light would be too faint for our telescopes to see. C. Because looking 15 billion light-years away means looking to a time before the universe existed.
32 1.2 The Scale of the Universe How big is Earth compared to our solar system? Roughly 100 earth s span the sun s diameter! Let s reduce the size of the solar system by a factor of 10 billion; the Sun is now the size of a large grapefruit (14 cm diameter). How big is Earth on this scale? A. an atom B. a ball point C. a marble D. a golf ball
33 Let s reduce the size of the solar system by a factor of 10 billion; the Sun is now the size of a large grapefruit (14 cm diameter). How big is Earth on this scale? A. an atom B. a ball point C. a marble D. a golf ball 2 x too big For earth Here!
34 How big is the Universe? The Milky Way is one of about 100 billion galaxies stars/galaxy x galaxies = stars As many stars as grains of (dry) sand on all Earth s beaches
35 How do our lifetimes compare to the age of the Universe? The Cosmic Calendar: a scale on which we compress the history of the universe into 1 year.
36 How do our lifetimes compare to the age of the Universe? The Cosmic Calendar: a scale on which we compress the history of the universe into 1 year.
37 1.3 Spaceship Earth How is Earth moving in our solar system? Contrary to our perception, we are not sitting still. We are moving with the Earth in several ways, and at surprisingly fast speeds ~1000 mi/hr The Earth rotates around its axis once every day. That s a thousand miles/hr at the equator: most of us are moving in circles around the axis at speeds far faster than commercial jets travel, which is why jets cannot keep up with the Sun when going opposite Earth s rotation
38 Earth orbits the Sun (revolves) once every year: at an average distance of 1 AU 150 million km. with Earth s axis tilted by 23.5º (pointing to Polaris) and rotating in the same direction it orbits, counterclockwise as viewed from above the North Pole. ORBIT. surprisingly high speed of over 100,000 km/hr=62,000 mi/hr We better not hit something!
39 Our Sun moves randomly relative to the other stars in the local Solar neighborhood typical relative speeds of more than 70,000 km/hr but stars are so far away that we cannot easily notice their motion And orbits the galaxy every 230 million years.
40 More detailed study of the Milky Way s rotation reveals one of the greatest mysteries in astronomy: Most of Milky Way s light comes from disk and bulge. but most of the mass is in its halo Halo What mass? -> DARK MATTER?
41 How do galaxies move within the universe? Galaxies are carried along with the expansion of the Universe. But how did Hubble figure out that the universe is expanding?
42 Hubble discovered that: All galaxies outside our Local Group are moving away from us. The more distant the galaxy, the faster it is racing away. Conclusion: We live in an expanding universe.
43 Are we ever sitting still? Earth rotates on axis: > 1,000 km/hr Earth orbits Sun: > 100,000 km/hr Solar system moves among stars: ~ 70,000 km/hr Milky Way rotates: ~ 800,000 km/hr Milky Way moves in Local Group Heh Prof? How come I don t feel it? Universe expands
44 1.4 The Human Adventure of Astronomy How has the study of astronomy affected human history? Copernican Revolution showed that Earth was not the center of the universe (Chapter 3) Study of planetary motion led to Newton s Laws of motion and gravity (Chapter 4) Newton s laws laid the foundation of the industrial revolution Modern discoveries are continuing to expand our cosmic perspective Development of the scientific method has brought many Humans out of the age of superstition and enriched our lives With great material wealth (but not all earthlings participate at this time!)
45 Astronomy led to Physics (What is it?) Fundamental Science Concerned with the fundamental principles of the Universe Foundation of other physical sciences Has simplicity of fundamental concepts Divided into five major areas ALL AREAS ARE USED TO INTERPRATE OUR UNIVERSE Classical Mechanics Thermodynamics Electromagnetism Optics Relativity \ Modern Physics EINSTEIN STARTED Quantum Mechanics /
46
47 Our Earth is a dynamic Rocky Planet of constant Change in the family of the Sun (Solar System)
48 Nearest to us in our Solar System is The Moon-a large rocky body
49 Figure 1.8 Arizona?
50 The Sun Rules the Solar System
51 The Sun s energy is driven by Nuclear Fusion- made up of matter in the plasma state interacting with strong magnetic forces Haunting images from the Sun
52 Venus in the Pleades Cluster
53 Why is dark side lit? <-Jupiter & moons
54 Radar view of Venus breaks through the clouds to reveal a young volcanic world
55 Mars from the Hubble Space Telescope Clouds, deserts, craters and Ice cap are viewed
56 Size-wise Mars is humble yet has the greatest Volcanoes and canyons of the Solar System
57 Jupiter IO EUROPA GANYMEDE CALLISTO These are the size Of the planet Mercury
58 Saturn and its mysterious rings
59 Unnumbered Figure 1.1 PLUTO THE LITTLE PLANET THAT COUDN T
60 The Solar system also contains, Comets and Asteroids. Which can be lethal to life on planet Earth from time to time.
61 Asteroid Gaspra
62 Our Milky Way galaxy from Earth contains > 150 billion other Suns and their systems( NOTE: Dust, glowing gas and stars)
63 Our Milky Way Galaxy in Infared (IR) radiation Deep Sky: Spiral Galaxy M61 In VIRGO
64 Deep Sky: Lagoon Nebula= a Stellar nursery In the our Milky Way Galaxy New Stars are born from condensing gas and dust
65 Deep Sky: Horsehead Nebula Combination of Dust and Gas in Our Milky Way Galaxy..located in Orion s star birth area A Dark Nebula
66 Deep Sky: The Rosette Nebula -emission nebula-3000 light-years away in Our Galaxy. Stellar wind from the open cluster of stars, NGC 2244, has cleared a hole in the nebula's center. Green= oxygen Blue= sulfur Red=hydrogen NOTE: ELEPHANT S TRUNKS
67 Deep Sky (Hubble): Newborn stars and their Solar Systems are forming in theeagle Nebula. The giant pillars (elephant trunks) are light years in length and are so dense that interior gas contracts gravitationally to form stars. Stellar nurseries are exposed.. The Eagle Nebula, lies about 7000 light years away
68 Deep Sky:The Pleiades, the most famous open cluster on the sky. Also called the Seven Sisters, M45 or Subaru is very bright and easy to see even in NYC. The Pleiades contains over 3000 young stars, is about 400 light years away, and only 13 light years across. Note the blue reflection nebulae surrounding the bright stars.
69 Deep Sky: Over 200 globular star clusters orbit the center of our Milky Way Galaxy, 47 Tucanae is the second brightest, Known also as 47 Tuc or NGC 104, visible from the Southern Hemisphere. Light takes about 20,000 years to reach us. Red Giant stars (yellowish) are easy to see. Stars in the cluster are very ancient! with Simple Chemistry And ages 10 to12 Billion Years Old!
70 Deep Sky: The Planetary Nebula (show) Glowing gaseous shrouds shed by dying sun-like stars trying to stabilize as they run out of nuclear fuel.. Typically 1,000 times the size of our solar system These Ten have names like Owl, the Cat's Eye, the Ghost of Jupiter, Ring. This glorious final phase in the life of a star lasts only about 10,000 yrs. Note: The Star Remnant At center of The Planetary Nebulae. Called Planetary Because the Resemble planets In a telescope GOOD-BYE PLANETS!
71 Deep Sky: Supernova Remnant: The Crab Nebula, filled with mysterious filaments, is the result of a star that was seen to explode in 1054 AD. This spectacular supernova explosion was recorded by Chinese and Anasazi Indian astronomers. In the very center lies a pulsar: a neutron star rotating. 30 times a second.
72 Deep Sky: Andromeda Nebula = Andromeda Spiral Galaxy.. Note two dwarf elliptical galaxies
73 Very Deep Sky: The Virgo cluster of Galaxies. Our Galaxy is in this group.
74 A very distant cluster of mostly spiral galaxies, half-way across the universe
75 Hubble: Ultra Deep Field.. Oldest and most distant Galaxies ever Found. Formed 13 billion years ago. Hubble spent 3 month imaging the Same spot.
76 Some final perspective when life gets you down Tree of Life MONTY PYTHON UNIVERSE SONG Homer has the last word on the scale of the Universe
Chapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Pearson Education, Inc.
Chapter 1 Lecture The Cosmic Perspective Seventh Edition A Modern View of the Universe Chapter Opener 1.1 The Scale of the Universe Our goals for learning: What is our place in the universe? How big is
More informationAstronomy 160. Instructor: Prof. Irv Robbins Office: 1N, room 233. Observatory
Astronomy 160 Space Science II Instructor: Prof. Irv Robbins Office: 1N, room 233 Phone: 982-28182818 Observatory 982-3260 e-mail: profirobbins@aol.com Course material is located at the Observatory Website:
More informationAstronomy 120. Instructor: Prof. Robert Taranto Office: 1N, room 222 Phone: Observatory
Astronomy 120 Instructor: Prof. Robert Taranto Office: 1N, room 222 Phone: 982-2825 Observatory 982-3260 e-mail: proftaranto@aol.com Course material is located at the Observatory Web: Access via CSI website
More informationStars. 1.1 A Modern View of the Universe. What Objects Do We Find in The Universe? 8/12/2010. Our goals for learning:
1.1 A Modern View of the Universe Our goals for learning: What is our place in the universe? How did we come to be? How can we know what the universe was like in the past? Can we see the entire universe?
More informationChapter 1 Our Place in the Universe. Copyright 2012 Pearson Education, Inc.
Chapter 1 Our Place in the Universe 1 1.1 Our Modern View of the Universe Our goals for learning: What is our place in the universe? How did we come to be? How can we know what the universe was like in
More informationStar. Planet. Chapter 1 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 Our goals for learning: What is our place in the universe? How did we come to be? How can we know what the universe was like in the
More information9/5/16. Astronomy 1001 Syllabus Sec 1 T,Th AM; Sec 2 T,TH PM. Astronomy 1001 First Assignments: Chapter 1: A Modern View of the Universe
9/5/16 Astronomy 1001 Syllabus Sec 1 T,Th AM; Sec 2 T,TH PM Syllabus: http://www.astro.umn.edu/courses/1001/syllabi/ Lecture notes: http://www.astro.umn.edu/courses/1001/ lecnotes/ Exams: http://www.astro.umn.edu/courses/1001/
More informationChapter 1 Our Place in the Universe
Chapter 1 Our Place in the Universe 1.1 Our Modern View of the Universe Topics we will explore: What is our place in the universe? How did we come to be? How can we know what the universe was like in the
More informationChapter 1 Lecture. The Cosmic Perspective Seventh Edition. A Modern View of the Universe
Chapter 1 Lecture The Cosmic Perspective Seventh Edition A Modern View of the Universe 1.1 The Scale of the Universe Our goals for learning: What is our place in the universe? How big is the universe?
More informationStar. Chapter 1: Our Place in the Universe. 1.1 A Modern View of the Universe Our goals for learning:
Chapter 1: Our Place in the Universe 1.1 A Modern View of the Universe Our goals for learning: What is our physical place in the Universe? How did we come to be? How can we know what the Universe was like
More informationPlan. Questions? Syllabus; administrative details. Some Definitions. An Idea of Scale
Plan Questions? Syllabus; administrative details Some Definitions An Idea of Scale All material available from http://astroweb.case.edu/ssm/astr101/ which is the primary document for the course (not Canvas).
More informationBell Ringer. want to do someday? 1. Briefly describe the Doppler effect in one sentence. 2. What do you want to do someday, like, in life?
Bell Ringer 1. Briefly describe the Doppler effect in one sentence. 2. What do you want to do someday, like, in life? 3. How do you think science might apply to what you want to do someday? SCIENCE MATTERS
More informationAST 103 Ch.1 Our Place in the Universe #2. Prof. Ken Nagamine Dept. of Physics & Astronomy UNLV
AST 103 Ch.1 Our Place in the Universe #2 Prof. Ken Nagamine Dept. of Physics & Astronomy UNLV 1 Ch. 1.2 The Scale of the Universe Our goals for learning: How big is Earth compared to our solar system?
More informationRequired Material. Required Material. Pre-Course Assessment 1/27/09. Textbook: The Cosmic Perspective, 5 th edition by Bennett et al.
Astronomy 104 -- Astronomy of the Solar System Spring 2009, TR 11:10-12:30, TCCW129 Instructor: Dr. Ting-Hui Lee Office: TCCW 215 Phone: 745-6472 E-mail: ting-hui.lee@wku.edu Office hours: W 10:00-11:45,
More informationRequired Material. Required Material 1/27/09. Textbook: The Cosmic Perspective, 5 th edition by Bennett et al.
Astronomy 104 -- Astronomy of the Solar System Spring 2009, TR 11:10-12:30, TCCW129 Instructor: Dr. Ting-Hui Lee Office: TCCW 215 Phone: 745-6472 E-mail: ting-hui.lee@wku.edu Office hours: W 10:00-11:45,
More informationCST 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 informationThe Universe and Galaxies
The Universe and Galaxies 16.1 http://dingo.care-mail.com/cards/flash/5409/galaxy.swf Universe The sum of all matter and energy that exists, that has ever existed, and that will ever exist. We will focus
More informationUniverse 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 informationAY2 Introduction to Astronomy Winter quarter, 2013
AY2 Introduction to Astronomy Winter quarter, 2013 Instructor: Maria Fernanda (Feña) Duran (mfduran@ucolick.org) Teaching assistants: Jieun Choi (jchoi37@ucsc.edu) Katie Hamren (khamren@ucolick.org) Course
More informationAST 103 The Solar System
AST 103 The Solar System Prof. Ken Nagamine Dept. of Physics & Astronomy UNLV Pick up two items from the front table (one each): 1. Syllabus 2. ABCD card 1 Instructor Contact Info Prof. Ken Nagamine Office:
More informationIntroduction to the Universe. What makes up the Universe?
Introduction to the Universe What makes up the Universe? Objects in the Universe Astrophysics is the science that tries to make sense of the universe by - describing the Universe (Astronomy) - understanding
More informationBeyond 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 informationStars 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 informationPhys 214. Planets and Life
Phys 214. Planets and Life Dr. Cristina Buzea Department of Physics Room 259 E-mail: cristi@physics.queensu.ca (Please use PHYS214 in e-mail subject) Lecture 8. The scale of time and nature of worlds (Page
More informationIntroduction to the Universe
What makes up the Universe? Introduction to the Universe Book page 642-644 Objects in the Universe Astrophysics is the science that tries to make sense of the universe by - describing the Universe (Astronomy)
More informationThe 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 informationAstronomy 1504 Section 10 Final Exam Version 1 May 6, 1999
Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999 Reminder: When I write these questions, I believe that there is one one correct answer. The questions consist of all parts a e. Read the entire
More informationWhat 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 informationCoriolis 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 informationPrentice 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 informationAn Introduction to AST 112 Stars, Galaxies, and the Cosmos
An Introduction to AST 112 Stars, Galaxies, and the Cosmos What is Astronomy? 50 years ago, astronomy was the study of everything outside Earth s atmosphere: the planets, the Sun, stars, galaxies, the
More informationoutline 1. in the beginning. The Big Bang 2. galaxies -- different types 3. stars -- life cycle 4. the solar system -- sun and planets
Earth s Place in the Universe outline 1. in the beginning. The Big Bang 2. galaxies -- different types 3. stars -- life cycle 4. the solar system -- sun and planets the big bang the universe is expanding
More informationTHE UNIVERSE AND THE EARTH
ESO1 THE UNIVERSE AND THE EARTH Unit 1 What is the Universe like? Universe theories Ideas about the Universe: Geocentric theory Aristotle (B.C) and Ptolomy (A.D) Heliocentric theory Copernicus in 1542
More information8/30/2010. 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 informationChapter 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 informationRead each slide then use the red or some underlined words to complete the organizer.
Read each slide then use the red or some underlined words to complete the organizer. 1B Did it start as a bang! 1B The Expanding Universe A. The Big Bang Theory: Idea that all matter began in an infinitely
More informationIntroduction to Astronomy
Introduction to Astronomy Have you ever wondered what is out there in space besides Earth? As you see the stars and moon, many questions come up with the universe, possibility of living on another planet
More informationA star is a massive sphere of gases with a core like a thermonuclear reactor. They are the most common celestial bodies in the universe are stars.
A star is a massive sphere of gases with a core like a thermonuclear reactor. They are the most common celestial bodies in the universe are stars. They radiate energy (electromagnetic radiation) from a
More informationAstronomy 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 informationThe Night Sky. The Universe. The Celestial Sphere. Stars. Chapter 14
The Night Sky The Universe Chapter 14 Homework: All the multiple choice questions in Applying the Concepts and Group A questions in Parallel Exercises. Celestial observation dates to ancient civilizations
More informationLESSON 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 information1UNIT. The Universe. What do you remember? Key language. Content objectives
1UNIT The Universe What do you remember? What are the points of light in this photo? What is the difference between a star and a planet? a moon and a comet? Content objectives In this unit, you will Learn
More informationBeyond the Solar System 2006 Oct 17 Page 1 of 5
I. Stars have color, brightness, mass, temperature and size. II. Distances to stars are measured using stellar parallax a. The further away, the less offset b. Parallax angles are extremely small c. Measured
More informationSun Mercury Venus. Earth Mars Jupiter
Sun Mercury Venus Earth Mars Jupiter Venus is the hottest planet in our solar system. The thick clouds on Venus hold the heat in. The sun s lights reflect off Venus s clouds making it look like the brightest
More informationScience Practice Astronomy (AstronomyJSuber)
Name: Date: 1. The pull of gravity on Earth is a direct result of the A. mass of Earth. B. magnetic field of Earth. C. rotation of Earth on its axis. D. weight of Earth's atmosphere. This online assessment
More informationAstronomy: Exploring the Universe
Course Syllabus Astronomy: Exploring the Universe Course Description Why do stars twinkle? Is it possible to fall into a black hole? Will the sun ever stop shining? Since the first glimpse of the night
More informationChapter 33 The History of a Star. Introduction. Radio telescopes allow us to look into the center of the galaxy. The milky way
Chapter 33 The History of a Star Introduction Did you read chapter 33 before coming to class? A. Yes B. No You can see about 10,000 stars with the naked eye. The milky way Radio telescopes allow us to
More informationThe Universe and Galaxies. Adapted from:
The Universe and Galaxies Adapted from: http://www.west-jefferson.k12.oh.us/earthandspacescience.aspx Astronomy The study of objects and matter outside the Earth s atmosphere and of their physical and
More informationDirected 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 informationPHYS 1510H. Today s Lecture. Introductory Astronomy I 9/8/16
PHYS 1510H Introductory Astronomy I 1 Today s Lecture! Review of syllabus and course websites! Introduction to astronomy! Break (10 minutes)! Slide show overview of course! Distances in astronomy 2 1 Who
More informationCambridge University Press Origins of Life in the Universe Robert Jastrow and Michael Rampino Excerpt More information PART I
PART I The Universe CHAPTER 1 Our place in the Universe The realm of the galaxies All life as we know it exists within the bounds of the single planet that we call home. For centuries mankind has gazed
More informationLecture 2: A Modern View of the Universe!
Lecture 2: A Modern View of the Universe! Asteroid Ida and satellite Dactyl! Claire Max April 3 rd, 2014 Astro 18: Planets and Planetary Systems UC Santa Cruz Page 1 Topics for this class Some definitions
More informationThe Earth and the Universe
The Earth and the Universe The exploration of space is called astronomy. Most of our observations in space have come from using telescopes of different kinds. Observing the universe from the ground has
More informationChapter 06 Let s Make a Solar System
like? Big picture. Chapter 06 Let s Make a Solar System How did it come to be this way? Where did it come from? Will I stop sounding like the Talking Heads? The solar system exhibits clear patterns of
More informationOur Planetary System. Chapter 7
Our Planetary System Chapter 7 Key Concepts for Chapter 7 and 8 Inventory of the Solar System Origin of the Solar System What does the Solar System consist of? The Sun: It has 99.85% of the mass of the
More informationAstronomy: Exploring the Universe
Course Syllabus Astronomy: Exploring the Universe Course Code: EDL028 Course Description The universe is truly the last unknown frontier and offers more questions than answers. Why do stars twinkle? Is
More informationHow did it come to be this way? Will I stop sounding like the
Chapter 06 Let s Make a Solar System How did it come to be this way? Where did it come from? Will I stop sounding like the Talking Heads? What does the solar system look like? Big picture. The solar system
More informationASTR 380. The Universe: the context for Life
ASTR 380 The Universe: the context for Life Simple facts: The Universe is vast. The Universe is old. The elements for life are wide-spread. Our physical laws appear universal The Universe is mostly empty!
More informationEarth s Formation Unit [Astronomy] Student Success Sheets (SSS)
Page1 Earth s Formation Unit [Astronomy] Student Success Sheets (SSS) HS-ESSI-1; HS-ESS1-2; HS-ESS1-3; HS-ESSI-4 NGSS Civic Memorial High School - Earth Science A Concept # What we will be learning Mandatory
More informationThe Universe. is space and everything in it.
The Universe is space and everything in it. Galaxies A galaxy is a supercluster of stars, gas, and dust that are held together by gravity. There are three main types of galaxies: Irregular Elliptical Spiral
More informationWhat Objects Are Part of the Solar System?
What Objects Are Part of the Solar System? Lesson 1 Quiz Josleen divided some of the planets into two main groups. The table below shows how she grouped them. Paul created a poster showing the solar system.
More information28-Aug-17. A Tour of Our Solar System and Beyond. The Sun
A Tour of Our Solar System and Beyond The Sun diameter = 1,390,000 km = 864,000 mi >99.8% of the mass of the entire solar system surface temperature 5800 C 600 x 10 6 tons H -> 596 x 10 6 tons He per second
More informationAfter you read this section, you should be able to answer these questions:
CHAPTER 16 4 Moons SECTION Our Solar System California Science Standards 8.2.g, 8.4.d, 8.4.e BEFORE YOU READ After you read this section, you should be able to answer these questions: How did Earth s moon
More informationChapter 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 informationChapter 23: Touring Our Solar System
Chapter 23: Touring Our Solar System The Sun The is the center of our solar system. The Sun makes up of all the mass of our solar system. The Sun s force holds the planets in their orbits around the Sun.
More informationScale in the Universe and Star Life Cycles
Scale in the Universe and Star Life Cycles Author: Richard Beare - Faulkes Telescope Project Scale in the Universe and Star Life Cycles Measuring objects in the Solar System Jupiter 2.45 arcmin 4.59 AU
More informationPossible Extra Credit Option
Possible Extra Credit Option Attend an advanced seminar on Astrophysics or Astronomy held by the Physics and Astronomy department. There are seminars held every 2:00 pm, Thursday, Room 190, Physics & Astronomy
More informationLecture PowerPoints. Chapter 33 Physics: Principles with Applications, 7 th edition Giancoli
Lecture PowerPoints Chapter 33 Physics: Principles with Applications, 7 th edition Giancoli This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching
More informationChapter 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 informationWhat is the sun? The sun is a star at the center of our solar system.
What is the sun? The sun is a star at the center of our solar system. Galileo Galilei (1564-1642) Galileo was one of the first Europeans to observe the sun. How did Galileo look at the sun? He lined up
More informationTEACHER BACKGROUND INFORMATION
TEACHER BACKGROUND INFORMATION (The Universe) A. THE UNIVERSE: The universe encompasses all matter in existence. According to the Big Bang Theory, the universe was formed 10-20 billion years ago from a
More information21/11/ /11/2017 Space Physics AQA Physics topic 8
Space Physics AQA Physics topic 8 8.1 Solar System, Orbits and Satellites The eight planets of our Solar System Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune As well as the eight planets, the
More informationMotion of the planets
Our Solar system Motion of the planets Our solar system is made up of the sun and the 9 planets that revolve around the sun Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune & Pluto (maybe?)
More informationAstronomy 1. 10/17/17 - NASA JPL field trip 10/17/17 - LA Griffith Observatory field trip
Astronomy 1 10/17/17 - NASA JPL field trip 10/17/17 - LA Griffith Observatory field trip CH 1 Here and NOW Where do we fit in the Universe? How-small-we-really-are-in-this-universe Start here: The figure
More informationCosmology, 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 informationAnnouncement Test 2. is coming up on Mar 19. Start preparing! This test will cover the classes from Feb 27 - Mar points, scantron, 1 hr.
Announcement Test 2 is coming up on Mar 19. Start preparing! This test will cover the classes from Feb 27 - Mar 14. 50 points, scantron, 1 hr. 1 AST103 Ch. 7 Our Planetary System Earth, as viewed by the
More informationISP205-2 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 informationStarting from closest to the Sun, name the orbiting planets in order.
Chapter 9 Section 1: Our Solar System Solar System: The solar system includes the sun, planets and many smaller structures. A planet and its moon(s) make up smaller systems in the solar system. Scientist
More informationAstronomy Today. Eighth edition. Eric Chaisson Steve McMillan
Global edition Astronomy Today Eighth edition Eric Chaisson Steve McMillan The Distance Scale ~1 Gpc Velocity L Distance Hubble s law Supernovae ~200 Mpc Time Tully-Fisher ~25 Mpc ~10,000 pc Time Variable
More informationExam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti
Exam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti INSTRUCTIONS: Please, use the `bubble sheet and a pencil # 2 to answer the exam questions, by marking
More informationD. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified
ASTRONOMY 1 EXAM 1 Name Identify Terms - Matching (20 @ 1 point each = 20 pts.) 1 Solar System G 7. aphelion N 14. eccentricity M 2. Planet E 8. apparent visual magnitude R 15. empirical Q 3. Star P 9.
More informationEarth 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 informationOutline 8: History of the Universe and Solar System
Outline 8: History of the Universe and Solar System The Andromeda Galaxy One of hundreds of billions of galaxies, each with hundreds of billions of stars A warped spiral galaxy, 150 MLY away and 100,000
More informationLearning About Our Solar System
Learning About Our Solar System By debbie Routh COPYRIGHT 2004 Mark Twain Media, Inc. ISBN 978-1-58037-876-5 Printing No. 404007-EB Mark Twain Media, Inc., Publishers Distributed by Carson-Dellosa Publishing
More informationJoy of Science Experience the evolution of the Universe, Earth and Life
Joy of Science Experience the evolution of the Universe, Earth and Life Review Introduction Main contents Quiz Unless otherwise noted, all pictures are taken from wikipedia.org Review 1 The presence of
More informationCHAPTER 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 informationFigure 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 informationAstronomy 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 informationUniverse 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 informationWHAT WE KNOW. Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So..
ASTRONOMY THE BIG BANG THEORY WHAT WE KNOW Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So.. WHAT DOES THIS MEAN? If
More informationThe Space Around Us. A quick overview of the solar system. Reid Pierce Lincoln Jr. High Bentonville, Arkansas
The Space Around Us A quick overview of the solar system Reid Pierce Lincoln Jr. High Bentonville, Arkansas The Universe The Universe is defined as the summation of all particles and energy that exist
More informationEarth Science, 13e Tarbuck & Lutgens
Earth Science, 13e Tarbuck & Lutgens Beyond Our Solar System Earth Science, 13e Chapter 24 Stanley C. Hatfield Southwestern Illinois College Properties of stars Distance Distances to the stars are very
More information29:50 Stars, Galaxies, and the Universe Final Exam December 13, 2010 Form A
29:50 Stars, Galaxies, and the Universe Final Exam December 13, 2010 Form A There are 40 questions. Read each question and all of the choices before choosing. Budget your time. No whining. Walk with Ursus!
More informationA protostar forming in the Orion Nebula. This also has protoplanetary discs, and will probably become a planetary system.
A protostar forming in the Orion Nebula. This also has protoplanetary discs, and will probably become a planetary system. These are also called stellar nurseries. Consisting almost entirely of hydrogen,
More informationAnswers. The Universe. Year 10 Science Chapter 6
Answers The Universe Year 10 Science Chapter 6 p133 1 The universe is considered to be the whole of all matter, energy, planets, solar systems, galaxies, and space. Many definitions of the universe also
More informationWelcome Aboard!! CHANGE OF KOMATSU S OFFICE HOURS. Briefing Welcome to the Cosmic Tour: Some Guide Lines. Lecture 1 Our Place in the Universe
CHANGE OF KOMATSU S OFFICE HOURS (Previous) Tuesdays & Thursdays 3:30 to 4:30 (New) Tuesdays 4:45 to 5:30 Thursdays 3:30 to 4:30 YOURNAME 31AUG Welcome Aboard!! AUSTIN AST 301 YOURNAME 31AUG 2.5 MILLION
More informationKitt Peak Nightly Observing Program
Kitt Peak Nightly Observing Program Splendors of the Universe on YOUR Night! Many pictures are links to larger versions. Click here for the Best images of the OTOP Gallery and more information. Canis Major
More informationThis Week in Astronomy
Homework #8 Due Wednesday, April 18, 11:59PM Covers Chapters 15 and 16 Estimated time to complete: 40 minutes Read chapters, review notes before starting This Week in Astronomy Credit: NASA/JPL-Caltech
More informationFormation of the Solar System Chapter 8
Formation of the Solar System Chapter 8 To understand the formation of the solar system one has to apply concepts such as: Conservation of angular momentum Conservation of energy The theory of the formation
More informationThe Age of the Universe If the entire age of the Universe were 1 calendar year, then 1 month would be equivalent to roughly 1 billion years
Astro.101 Sept. 9, 2008 Announcements A few slots are still open in the class; see prof. to sign up Web-page computer has been down; o.k. now Turn in your student contract Don t forget to do the OWL tutorial
More information