Exercise - I. 1. The point in the sky that is located 90 degrees above the horizon is the
|
|
- Jonah Washington
- 5 years ago
- Views:
Transcription
1 Exercise - I 1. The point in the sky that is located 90 degrees above the horizon is the a) terrestrial horizon b) equator c) pole d) zenith e) ascending node 2. Which of the following would be the coordinates of a star that is rising in the southeast? a) azimuth 180 degrees, al:tude 0 degrees b) azimuth 180 degrees, al:tude 90 degrees c) azimuth 145 degrees, al:tude 0 degrees d) azimuth 60 degrees, al:tude 0 degrees e) azimuth 75 degrees, al:tude 90 degrees 3. The equivalent of terrestrial longitude in the equatorial (celesgal) coordinate system is a) declina:on. b) the horizon. c) precession. d) right ascension. e) space.
2 4. Where on the Earth does the celesgal equator pass through the zenith? a) Marburg b) the North Pole c) the South Pole d) the equator e) nowhere on Earth 5. The Sun's path on the celesgal sphere is a) the zenith. b) the equator. c) the meridian. d) the eclip:c. e) the yellow brick road. 6. The occurrence of seasons on the Earth results from a) the Earth being closer to the Sun in summer. b) the Earth changing its rota:on rate during the year. c) the Earth's axis poin:ng in different south and then north during the year. d) the Earth's axis being inclined to the eclip:c. e) the appearance of Sirius rising above the Nile.
3 7. Where is the Sun on December 21? a) RA = 0 h, Dec = 0 o b) RA = 6 h, Dec = 23.5 o c) RA = 6 h, Dec = 23.5 o d) RA = 18 h, Dec = 23.5 o e) RA = 18 h, Dec = 23.5 o 8. Greenwich mean Gme or universal Gme is the standard Gme for longitude? a) 90 degrees b) 45 degrees c) zero degree d) 180 degrees 9. If we take an apple, assume it is a sphere, and cut it in half; we slice through a great circle. If we make a mistake, miss the center and hence cut the apple into two unequal parts we will have sliced through a a) great circle b) spherical angle c) small circle d) prime meridian
4 10. If the plane does not contain the center of the sphere, it is known as a) Greenwich meridian b) great circle c) small circle d) principle vertex 11. Which of the following statements about the celesgal sphere is not true? a) The celes:al sphere is just another name for our universe. b) From any loca:on on earth, we can see only half the celes:al sphere at any one :me. c) When we look in the sky, the stars all appear to be located on the celes:al sphere. d) The earth is placed at the center of celes:al sphere. e) The celes:al sphere does not exist physically. 12. Which of the following statements about the celesgal equator is true at all lagtudes? a) It extends from your horizon due east, through your zenith, to your horizon due west. b) It lies along the band of light we call the milky way. c) It cuts the dome of your sky exactly in half. d) It represents an extension of earth s equator onto the celes:al sphere. e) It extends from your horizon due north, through your zenith,to your horizon due south.
5 13. Which of the following correctly describes the meridian in your sky? a) A half- circle extending from your horizon due north, through your zenith, to your horizon due south. b) A half circle extending from your horizon due east, through your zenith, to your horizon due west. c) A half circle extending from your horizon due east,through the north celes:al pole,to your horizon due west. d) The boundary between the por:on of the celes:al sphere you can see at any moment and the por:on that you cannot see. 14. You are standing on the earth s equator. Which way is Polaris, the North star? a) Directly overhead. b) 30 degrees up, due west. c) On the northern horizon. d) The answer depends on whether it s winter or summer. e) The answer depends on what :me of day (or night) it is. 15. What is eclipgc? a) The sun s apparent path along the celes:al sphere. b) The moon s apparent path along the celes:al sphere. c) The sun s daily path across the sky. d) When the moon passes in front of sun.
6 16. What is a circumpolar star? a) A star that makes a daily circle around the celes:al sphere. b) A star that is visible close to the north celes:al pole. c) A star that always remains above your horizon. d) A star that is close to the south celes:al pole. 17. DeclinaGon is measured from a) Horizon b) prime meridian c) celes:al equator d) zero point 18. For a star what remains the same for all Gmes? a) Azimuth b) hour angle c) right ascension d) declina:on
7 19. Parallax would be easier to measure if a) Earth's orbit were larger. b) the stars were farther away. c) Earth moved faster along its orbit. d) all of these e) none of these 20. If a star has a parallax of 0.02 seconds of arc, then its distance is a) 20 pc b) 50 pc c) 2 pc d) 5 pc e) 500 pc 21. Suppose you measure the parallax angle for a pargcular star to be 0.1 arc second. The distance to this star is a) 10 light-years. b) 10 parsecs. c) 0.1 light-year. d) 0.1 parsec. e) impossible to determine.
8 22. Suppose that you measure the parallax angle for a pargcular star to be 0.5 arc-second. The distance to this star is a) 0.5 light-year. b) 0.5 parsec. c) 5 light-years. d) 5 parsecs. e) 2 parsecs. 23. The most distant stars we can measure stellar parallax from Earth are approximately a) 50 parsecs away. b) 500 parsecs away. c) 5,000 parsecs away. d) halfway across the Milky Way Galaxy. e) in the Andromeda Galaxy. 24. A star with a parallax angle of 1/20 arc-second is a) 20 light-years away. b) 1/20 parsec away. c) 20 parsecs away. d) 10 parsecs away.
9 25. Suppose you are at the equator which has a lagtude of 0 0. The algtude of the north celesgal pole as seen from your posigon is a) 90 0 b) c) d) 0 0 e) 45 0
10 6. At la:tude of 50 0 N, a star has a declina:on =30 0 N. Find it s zenith distance when it s on observer s meridian. Answer: Zenith Distance = 20 0
11
12
13
14
15 500
16
17
18
19
20 Zenith Distance
21 Zenith Distance = 20 0
22 LaGtude = 50 0, DeclinaGon = 30 0 AlGtude = Dec + ( AlGtude of NCP); AlGtude of NCP = LaGtude of observer = AlGtude = = Zenith distance = AlGtude = = 20 0
Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations.
Chapter 1: Discovering the Night Sky Constellations: Recognizable patterns of the brighter stars that have been derived from ancient legends. Different cultures have associated the patterns with their
More informationWeek 2. Problem Set 1 is due Thursday via Collab. Moon awareness Weather awareness
Week 2 Lab 1 observa.ons start real soon (in progress?) Prelab done? Observa.ons should wrap up this week. Lab 2 + Prelab 2 will be out next week early and observa.ons will follow Lab 1 write-up guidance
More informationAppearance of the Sky Orientation Motion of sky Seasons Precession (?)
Today Appearance of the Sky Orientation Motion of sky Seasons Precession (?) The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The ecliptic is the Sun s apparent
More informationTopic Guide: The Celestial Sphere. GCSE (9-1) Astronomy. Pearson Edexcel Level 1/Level 2 GCSE (9-1) in Astronomy (1AS0)
Topic Guide: The Celestial Sphere GCSE (9-1) Astronomy Pearson Edexcel Level 1/Level 2 GCSE (9-1) in Astronomy (1AS0) The Celestial Sphere Contents Specification Points 1 The Astronomy 2 Equatorial coordinates
More informationAppearance of the Sky Orientation Motion of sky Seasons Precession (?)
Today Appearance of the Sky Orientation Motion of sky Seasons Precession (?) The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The ecliptic is the Sun s apparent
More informationA2 Principi di Astrofisica. Coordinate Celesti
A2 Principi di Astrofisica Coordinate Celesti ESO La Silla Tel. 3.6m Celestial Sphere Our lack of depth perception when we look into space creates the illusion that Earth is surrounded by a celestial sphere.
More informationMeridian Circle through Zenith, North Celestial Pole, Zenith Direction Straight Up from Observer. South Celestial Pole
Chapter 3 How Earth and Sky Work- Effects of Latitude In chapters 3 and 4we will learn why our view of the heavens depends on our position on the Earth, the time of day, and the day of the year. We will
More informationOberth: Energy vs. Momentum
1 2 The Oberth Effect 3 Oberth: Energy vs. Momentum 4 The Celestial Sphere From our perspective on Earth the stars appear embedded on a distant 2-dimensional surface the Celestial Sphere. 5 The Celestial
More informationChapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc.
Chapter 2 Lecture The Cosmic Perspective Seventh Edition Discovering the Universe for Yourself Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the
More informationChapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? Constellations. 2.1 Patterns in the Night Sky
Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we
More informationChapter 2 Discovering the Universe for Yourself
Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we
More informationCelestial Sphere Spectroscopy (Something interesting; e.g., advanced data analyses with IDL)
AST326, 2010 Winter Semester Celestial Sphere Spectroscopy (Something interesting; e.g., advanced data analyses with IDL) Practical Assignment: analyses of Keck spectroscopic data from the instructor (can
More informationLecture 4: August 30, 2010
Lecture 4: August 30, 2010 How many hospitals are there in the USA? Announcements: First homework has been posted Due Friday (10 th ) First Observatory Opportunity Thursday Night September 2, 8:30pm Will
More informationChapter 2 Discovering the Universe for Yourself
Chapter 2 Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations we
More informationAstronomy 311 Professor Menningen January 2, Syllabus overview books & supplies course goals assignments & grading About the professor
1 Astronomy 311 Professor Menningen January 2, 2014 Syllabus overview books & supplies course goals assignments & grading About the professor 2 How to Learn Astronomy Stay curious Interact with the same
More informationWhat do you think? 2/3/09. Mastering Astronomy Assignment 2. Constellations the 88 semi-rectangular regions that make up the sky
//09 Mastering Astronomy Assignment Due Feb 0, am Read Chapter Constellations the 88 semi-rectangular regions that make up the sky Northern constellations have Latinized Greek-mythology names: Orion, Cygnus,
More informationObserving the Universe for Yourself
Observing the Universe for Yourself Figure 6-20 Solar-System Formation What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars as well as the Milky Way. A constellation
More informationChapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc.
Chapter 2 Discovering the Universe for Yourself 1 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations
More informationChapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself
Chapter 2 Lecture The Cosmic Perspective Seventh Edition Discovering the Universe for Yourself Discovering the Universe for Yourself 2.1 Patterns in the Night Sky Our goals for learning: What does the
More informationMULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
Exam 1 Physics 101 Fall 2014 Chapters 1-3 Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Suppose we look at a photograph of many galaxies.
More informationAstronomy 122 Section 1 TR Outline. The Earth is Rotating. Question Digital Computer Laboratory
Astronomy 122 Section 1 TR 1300-1350 Outline 1320 Digital Computer Laboratory Leslie Looney Phone: 244-3615 Email: lwlw@wuiucw. wedu Office: Astro Building #218 Office Hours: T 10:30-11:30 a.m. or by appointment
More informationName: Date: 5. The bright stars Vega, Deneb, and Altair form A) the summer triangle. B) the winter triangle. C) the Big Dipper. D) Orion, the Hunter.
Name: Date: 1. If there are about 6000 stars in the entire sky that can be seen by the unaided human eye, about how many stars would be seen at a particular instant on a given dark night from a single
More information3) During retrograde motion a planet appears to be A) dimmer than usual. B) the same brightness as usual C) brighter than usual.
Descriptive Astronomy (ASTR 108) Exam 1 B February 17, 2010 Name: In each of the following multiple choice questions, select the best possible answer. In the line on the scan sheet corresponding to the
More information1) Kepler's third law allows us to find the average distance to a planet from observing its period of rotation on its axis.
Descriptive Astronomy (ASTR 108) Exam 1 A February 17, 2010 Name: In each of the following multiple choice questions, select the best possible answer. In the line on the scan sheet corresponding to the
More informationContrast the old definition of constellation with the. State why we see different constellations during. Summarize what is meant by the Celestial
Contrast the old definition of constellation with the astronomers definition of constellation State why we see different constellations during different times of the year. Summarize what is meant by the
More informationConstellations In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures.
Chapter 2: The Sky Constellations In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures. Constellations Today, constellations
More informationConstellations. In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures.
Chapter 2 The Sky Constellations In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures. Constellations A constellation is
More informationAstronomical coordinate systems. ASTR320 Monday January 22, 2018
Astronomical coordinate systems ASTR320 Monday January 22, 2018 Special public talk this week: Mike Brown, Pluto Killer Wednesday at 7:30pm in MPHY204 Other news Munnerlyn lab is hiring student engineers
More informationWeek 2. Lab 1 observa.ons in progress. Problem Set 1 is due Wednesday via Collab. Moon awareness Weather awareness. Prelab done?
Lab 1 observa.ons in progress Prelab done? Week 2 Observa.ons should wrap up this week. Lab + Prelab 2 will be out next week early and observa.ons will follow Lab 1 write-up guidance will be forthcoming
More informationObserving the Night Sky: Locating Objects
Observing the Night Sky: Locating Objects As I left the house this morning, there was a bright bluish light above and to the left of my neighbors house (approximately East) and a big very bright object
More information6/17. Universe from Smallest to Largest:
6/17 Universe from Smallest to Largest: 1. Quarks and Leptons fundamental building blocks of the universe size about 0 (?) importance: quarks combine together to form neutrons and protons. One of the leptons
More information10/17/2012. Observing the Sky. Lecture 8. Chapter 2 Opener
Observing the Sky Lecture 8 Chapter 2 Opener 1 Figure 2.1 Figure 2.2 2 Figure 2.6 Figure 2.4 Annotated 3 The Celestial Sphere The celestial sphere is the vast hollow sphere on which the stars appear fixed.
More informationA Sky Full of Stars - II.
A Sky Full of Stars - II. Learning Objectives! What is the latitude of the Equator and of the Earth s North and South Poles? What is the declination of the Celestial Equator and of the Celestial Poles?!
More information2.1 Patterns in the Night Sky
2.1 Patterns in the Night Sky Our goals for learning: What are constellations? How do we locate objects in the sky? Why do stars rise and set? Why don t we see the same constellations throughout the year?
More informationAstronomy 101: 9/18/2008
Astronomy 101: 9/18/2008 Announcements Pick up a golf ball at the front of the class or get one from Alex; you will need it for an in-class activity today. You will also need the question sheet from Alex.
More informationClassAction: Coordinates and Motions Module Instructor s Manual
ClassAction: Coordinates and Motions Module Instructor s Manual Table of Contents Section 1: Warm-up Questions...3 The Sun s Path 1 4 Section 2: General Questions...5 Sledding or Going to the Beach...6
More informationConstellations. In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures.
Chapter 2 The Sky Constellations In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures. Constellations (2) Today, constellations
More informationTime, coordinates and how the Sun and Moon move in the sky
Time, coordinates and how the Sun and Moon move in the sky Using the colors and magnitudes of quasars drawn from the SDSS Catalog Archive Server to distinguish quasars from stars using the light they emit
More informationDiscovering the Night Sky
Discovering the Night Sky Guiding Questions 1. What role did astronomy play in ancient civilizations? 2. Are the stars that make up a constellation actually close to one another? 3. Are the same stars
More informationDiscovering the Night Sky
Guiding Questions Discovering the Night Sky 1. What role did astronomy play in ancient civilizations? 2. Are the stars that make up a constellation actually close to one another? 3. Are the same stars
More informationPhys Lab #1: The Sun and the Constellations
Phys 10293 Lab #1: The Sun and the Constellations Introduction Astronomers use a coordinate system that is fixed to Earth s latitude and longitude. This way, the coordinates of a star or planet are the
More informationKnowing the Heavens. Chapter Two. Guiding Questions. Naked-eye (unaided-eye) astronomy had an important place in ancient civilizations
Knowing the Heavens Chapter Two Guiding Questions 1. What role did astronomy play in ancient civilizations? 2. Are the stars that make up a constellation actually close to one another? 3. Are the same
More informationIntroduction to Astronomy
Introduction to Astronomy AST0111-3 (Astronomía) Semester 2014B Prof. Thomas H. Puzia Theme Our Sky 1. Celestial Sphere 2. Diurnal Movement 3. Annual Movement 4. Lunar Movement 5. The Seasons 6. Eclipses
More information2. Modern: A constellation is a region in the sky. Every object in the sky, whether we can see it or not, is part of a constellation.
6/14 10. Star Cluster size about 10 14 to 10 17 m importance: where stars are born composed of stars. 11. Galaxy size about 10 21 m importance: provide a stable environment for stars. Composed of stars.
More informationCHAPTER 2 A USER'S GUIDE TO THE SKY
CHAPTER 2 A USER'S GUIDE TO THE SKY MULTIPLE CHOICE 1. Seen from the northern latitudes (mid-northern hemisphere), the star Polaris a. is never above the horizon during the day. b. always sets directly
More informationThe celestial sphere, the coordinates system, seasons, phases of the moon and eclipses. Chapters 2 and S1
The celestial sphere, the coordinates system, seasons, phases of the moon and eclipses Chapters 2 and S1 The celestial sphere and the coordinates system Chapter S1 How to find our way in the sky? Let s
More informationThe Celestial Sphere. From our perspective on Earth the stars appear embedded on a distant 2 dimensional surface the Celestial Sphere.
1 The Celestial Sphere From our perspective on Earth the stars appear embedded on a distant 2 dimensional surface the Celestial Sphere. 2 The Celestial Sphere Although we know better, it is helpful to
More informationThe sky and the celestial sphere
Chapter 1 The sky and the celestial sphere The Sun, and sometimes the Moon are, by and large, the only astronomical objects visible in the day sky. Traditionally, astronomy has been a nocturnal activity.
More informationIntroduction to the sky
Introduction to the sky On a clear, moonless night, far from city lights, the night sky is magnificent. Roughly 2000 stars are visible to the unaided eye. If you know where to look, you can see Mercury,
More informationMotions of the Earth
Motions of the Earth Our goals for learning: What are the main motions of the Earth in space? How do we see these motions on the ground? How does it affect our lives? How does the orientation of Earth's
More informationLecture #03. January 20, 2010, Wednesday
Lecture #03 January 20, 2010, Wednesday Causes of Earth s Seasons Earth-Sun geometry Day length Solar angle (beam spread) Atmospheric beam depletion Shape and Size of the Earth North Pole E Geoid: not
More informationWelcome to Astronomy 402/602
Welcome to Astronomy 402/602 Introductions Syllabus Telescope proposal Coordinate Systems (Lecture) Coordinate System Exercise Light (Lecture) Telescopes (Lecture) Syllabus Course goals Course expectations
More informationAstronomy 103: First Exam
Name: Astronomy 103: First Exam Stephen Lepp September 21, 2010 Each question is worth 2 points. Write your name on this exam and on the scantron. Short Answer Mercury What is the closest Planet to the
More informationName and Student ID Section Day/Time:
AY2 - Overview of the Universe - Midterm #1 - Instructor: Maria F. Duran Name and Student ID Section Day/Time: 1) Imagine we ve discovered a planet orbiting another star at 1 AU every 6 months. The planet
More informationName Class Date. For each pair of terms, explain how the meanings of the terms differ.
Skills Worksheet Chapter Review USING KEY TERMS 1. Use each of the following terms in a separate sentence: year, month, day, astronomy, electromagnetic spectrum, constellation, and altitude. For each pair
More informationThe Earth and the Sky
The Earth and the Sky In this class, we want to understand why the objects in the sky as seen from the Earth - appear as they do. Even though we haven t yet discussed the details, I am assuming that there
More informationPHYS 160 Astronomy Test #1 Fall 2017 Version B
PHYS 160 Astronomy Test #1 Fall 2017 Version B 1 I. True/False (1 point each) Circle the T if the statement is true, or F if the statement is false on your answer sheet. 1. An object has the same weight,
More informationIntroduction To Modern Astronomy I: Solar System
ASTR 111 003 Fall 2007 Lecture 02 Sep. 10, 2007 Introduction To Modern Astronomy I: Solar System Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-15) Chap. 16: Our Sun Chap. 28: Search for
More informationWelcome back. Scale. Week 2 Updates. PHYS 1302 Astronomy of the Solar System
Week 2 Updates Two in-class quizzes now completed Introductions List-serve Quick review of Chapter 1 Discuss Chapter 2 Chapter 3 next week (9/9). Welcome back Week 2 of PHYS 1302 Como se dice The h Syllabus:
More informationPHAS 1511: Foundations of Astronomy
PHAS 1511: Foundations of Astronomy Dr Roger Wesson Research interests: deaths of stars. Planetary nebulae, novae and supernovae. Astronomy: some maths You can see that distances in astronomy are huge.
More informationAileen A. O Donoghue Priest Associate Professor of Physics
SOAR: The Sky in Motion Life on the Tilted Teacup Ride Celestial Coordinates and the Day Aileen A. O Donoghue Priest Associate Professor of Physics Reference Points Poles Equator Prime Meridian Greenwich,
More informationBrock University. Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014
Brock University Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014 Number of hours: 50 min Time of Examination: 18:00 18:50 Instructor:
More informationIt s Full of Stars! Outline. A Sky Full of Stars. Astronomy 210. lights), about how many stars can we see with
Astronomy 210 Section 1 MWF 1500-1550 134 Astronomy Building Leslie Looney Phone: 244-3615 Email: lwlw@wuiucw. wedu Office: Astro Building #218 Office Hours: MTF 10:30-11:30 a.m. or by appointment This
More informationAST 443 / PHY 517. Astronomical Observa<onal Techniques. Prof. F.M. Walter
AST 443 / PHY 517 Astronomical Observa
More informationCELESTIAL COORDINATES
ASTR 1030 Astronomy Lab 27 Celestial Coordinates CELESTIAL COORDINATES GEOGRAPHIC COORDINATES The Earth's geographic coordinate system is familiar to everyone - the north and south poles are defined by
More informationDaily Motions. Daily Motions. Solar and Sidereal Days. Annual Motions of the Sun. Coordinate system on Earth. Annual Motion of the Stars.
Sun: rises in the east sets in the west travels on an arc across the sky 24 hours Daily Motions Solar Day = 24 hours Stars: stars travel on arcs in the sky moving from east to west. some stars rise and
More informationThe Nature of Stars. The Nature of Stars
The Nature of Stars The total number of stars is beyond our ability to count Only a few stars have been studied in detail. To understand the nature of stars, we will compare and catalog the stars by: Physical
More informationPhysics Lab #2: Learning Starry Night, Part 1
Physics 10293 Lab #2: Learning Starry Night, Part 1 Introduction In this lab, we'll learn how to use the Starry Night software to explore the sky, and at the same time, you ll get a preview of many of
More informationBrock University. Test 1, October 2016 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: October 3, 2016
Brock University Test 1, October 2016 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: October 3, 2016 Number of hours: 50 min Time of Examination: 17:00 17:50 Instructor:
More informationREVIEW CH #0. 1) Right ascension in the sky is very similar to latitude on the Earth. 1)
REVIEW CH #0 TRUE/FALSE. Write 'T' if the statement is true and 'F' if the statement is false. 1) Right ascension in the sky is very similar to latitude on the Earth. 1) 2) Latitude and right ascension
More informationdrinking straw, protractor, string, and rock. observer on Earth. Sun across the sky on March 21 as seen by an
1. The diagram below represents some constellations and one position of Earth in its orbit around the Sun. These constellations are visible to an observer on Earth at different times of the year. When
More informationEARTHS SHAPE AND POLARIS PRACTICE 2017
1. In the diagram below, letters A through D represent the locations of four observers on the Earth's surface. Each observer has the same mass. 3. Which diagram most accurately shows the cross-sectional
More informationChapter S1 Celestial Timekeeping and Navigation. How do we define the day, month, year, and planetary time periods?
Chapter S1 Celestial Timekeeping and Navigation S1.1 Astronomical Time Periods Our goals for learning:! How do we define the day, month, year, and planetary time periods?! How do we tell the time of day?!
More informationIntroduction To Astronomy Lesson 1
Introduction To Astronomy Lesson 1 Topics for this Lesson Earth Based Coordinates The Celestial Sphere and Sky Coordinates The North Star Measuring Distances on the Sky The Motion of Objects in the Sky
More informationDiscovering the Universe for Yourself
Constellations: region in the sky with well defined borders; the familiar patterns of stars merely help us locate these constellations. 88 names were chosen by the International Astronomical Union. Every
More information4 Solar System and Time
4 olar ystem and Time 4.1 The Universe 4.1.1 Introduction The Universe consists of countless galaxies distributed throughout space. The bodies used in astro navigation belong to the Galaxy known as the
More informationUNIT 3: EARTH S MOTIONS
UNIT 3: EARTH S MOTIONS After Unit 3 you should be able to: o Differentiate between rotation and revolution of the Earth o Apply the rates of rotation and revolution to basic problems o Recall the evidence
More informationThe Celestial Sphere. GEK1506 Heavenly Mathematics: Cultural Astronomy
The Celestial Sphere GEK1506 Heavenly Mathematics: Cultural Astronomy Helmer Aslaksen Department of Mathematics National University of Singapore aslaksen@math.nus.edu.sg www.math.nus.edu.sg/aslaksen/ The
More informationFundamentals of Satellite technology
Fundamentals of Satellite technology Prepared by A.Kaviyarasu Assistant Professor Department of Aerospace Engineering Madras Institute Of Technology Chromepet, Chennai Orbital Plane All of the planets,
More informationBrock University. Test 1, May 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: May 21, 2014
Brock University Test 1, May 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: May 21, 2014 Number of hours: 50 min Time of Examination: 14:00 14:50 Instructor: B.Mitrović
More informationCHAPTER 2 A USER'S GUIDE TO THE SKY
CHAPTER 2 A USER'S GUIDE TO THE SKY MULTIPLE CHOICE 1. In one way of naming stars, a letter indicates its brightness relative to the other stars in the constellation. a. English b. Arabic c. Greek d. Cyrillic
More informationlightyears observable universe astronomical unit po- laris perihelion Milky Way
1 Chapter 1 Astronomical distances are so large we typically measure distances in lightyears: the distance light can travel in one year, or 9.46 10 12 km or 9, 600, 000, 000, 000 km. Looking into the sky
More informationBefore you Sit. Please Pick-up: Blue Information Sheet for Evening Observing. 1 Red and 1 Blue ticket for Observing/ Planetarium
Before you Sit Please Pick-up: Blue Information Sheet for Evening Observing. 1 Red and 1 Blue ticket for Observing/ Planetarium Evening Observing Observing at the Brooks Observatory: Three different weeks
More informationPHYS1002: Founda0ons of Astronomy
PHYS1002: Founda0ons of Astronomy Simon.Driver@icrar.org Course Text: Astronomy: A Physical Perspec0ve, Marc Kutner 9 Lectures + 2 Assessments + Final Exam New course component Exams will be similar to
More informationKnowing the Heavens. Goals: Constellations in the Sky
Goals: Knowing the Heavens To see how the sky changes during a night and from night to night. To measure the positions of stars in celestial coordinates. To understand the cause of the seasons. Constellations
More informationChapter S1 Lecture. The Cosmic Perspective Seventh Edition. Celestial Timekeeping and Navigation Pearson Education, Inc.
Chapter S1 Lecture The Cosmic Perspective Seventh Edition Celestial Timekeeping and Navigation 2014 Pearson Education, Inc. Celestial Timekeeping and Navigation 2014 Pearson Education, Inc. S1.1 Astronomical
More informationKnowing the Heavens. Goals: Constellations in the Sky
Goals: Knowing the Heavens To see how the sky changes during a night and from night to night. To measure the positions of stars in celestial coordinates. To understand the cause of the seasons. Constellations
More informationTime and Diurnal Motion
Time and Diurnal Motion Time and Diurnal Motion A. Geography: mapping the earth 2 B. Equatorial Coordinates C. Local Horizon System Updated 2014Jan11 A. Geography: mapping the earth Geometry: measure the
More informationA Warm Up Exercise. The Motion of the Sun. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise
A Warm Up Exercise The Motion of the Sun Which of the following is NOT true of a circumpolar star? a) It rises and sets from my latitude b) Its direction can be far North c) Its direction can be far South
More informationAileen A. O Donoghue Priest Associate Professor of Physics
SOAR: The Sky in Motion Life on the Tilted Teacup Ride The Year Aileen A. O Donoghue Priest Associate Professor of Physics Celestial Coordinates Right Ascension RA or From prime meridian (0 h ) to 23 h
More informationBrock University. Test 1, October 2017 Number of pages: 9 Course: ASTR 1P01, Section 1 Number of Students: 470 Date of Examination: October 3, 2017
Brock University Test 1, October 2017 Number of pages: 9 Course: ASTR 1P01, Section 1 Number of Students: 470 Date of Examination: October 3, 2017 Number of hours: 50 min Time of Examination: 17:00 17:50
More informationUnderstanding Positional Astronomy Part 2 Celestial Co-ordinates Difficulty: Intermediate
Exercise: Understanding Positional Astronomy Part 2 Celestial Co-ordinates Difficulty: Intermediate Objectives In Part 1 you learned about Celestial Sphere and how the stars appear to move across the night
More informationLOCATING CELESTIAL OBJECTS: COORDINATES AND TIME. a. understand the basic concepts needed for any astronomical coordinate system.
UNIT 2 UNIT 2 LOCATING CELESTIAL OBJECTS: COORDINATES AND TIME Goals After mastery of this unit, you should: a. understand the basic concepts needed for any astronomical coordinate system. b. understand
More informationPhysics Lab #4:! Starry Night Student Exercises I!
Physics 10293 Lab #4: Starry Night Student Exercises I Introduction For today s lab, we are going to let the Starry Night software do much of the work for us. We re going to walk through some of the sample
More informationASTR 1P01 Test 1, September 2017 Page 1 BROCK UNIVERSITY
ASTR 1P01 Test 1, September 2017 Page 1 BROCK UNIVERSITY Test 1: Fall 2017 Number of pages: 10 Course: ASTR 1P01, Section 2 Number of students: 1300 Examination date: 30 September 2017 Time limit: 50 min
More informationPlanet Earth. Part 2
Planet Earth Part 2 Sun, Earth and Moon Motions The Solar System revolves around the Milky Way galaxy center. The Sun rotates on its own axis. Earth revolves around the Sun (1 year) and rotates on its
More informationLocal Coordinates. These are centered upon you, the observer.
Astronomy 30, Observing #3 Name: Lab Partners: Date: Materials: This lab, with the star chart completed from the pre-lab. Some sheets of paper for sketches. A pencil with eraser. A small flashlight, ideally
More informationThe Sky. Day sky: the Sun, occasionally the Moon. Night Sky: stars, and sometimes the Moon
The Sky Day sky: the Sun, occasionally the Moon Night Sky: stars, and sometimes the Moon So MANY objects.how Do We Make Sense of it ALL?? Goal How to describe the locations of objects in the sky To understand
More informationEarth s Orbit. Sun Earth Relationships Ridha Hamidi, Ph.D. ESCI-61 Introduction to Photovoltaic Technology
1 ESCI-61 Introduction to Photovoltaic Technology Sun Earth Relationships Ridha Hamidi, Ph.D. Spring (sun aims directly at equator) Winter (northern hemisphere 23.5 tilts away from sun) 2 Solar radiation
More informationCoordinates on the Sphere
Survey Observations Coordinates on the Sphere Any position on the surface of a sphere (such as the Earth or the night sky) can be expressed in terms of the angular coordinates latitude and longitude Latitude
More information