Chapter S1 Review Clickers. The Cosmic Perspective Seventh Edition. Celestial Timekeeping and Navigation Pearson Education, Inc.

Similar documents
Chapter S1 Lecture. The Cosmic Perspective Seventh Edition. Celestial Timekeeping and Navigation Pearson Education, Inc.

Chapter S1 Celestial Timekeeping and Navigation. How do we define the day, month, year, and planetary time periods?

PHAS 1511: Foundations of Astronomy

Practice Questions: Seasons #1

HNRS 227 Fall 2007 Chapter 14. Earth in Space presented by Prof. Geller 25 October 2007

Aileen A. O Donoghue Priest Associate Professor of Physics

A Warm Up Exercise. The Motion of the Sun. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise

Introduction To Modern Astronomy I: Solar System

Astronomy 291. Professor Bradley M. Peterson

Chapter 0 2/19/2014. Lecture Outline. 0.1 The Obvious View. Charting the Heavens. 0.1 The Obvious View. 0.1 The Obvious View. Units of Chapter 0

Astronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION

PHYS 160 Astronomy Test #1 Fall 2017 Version B

Name: 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.

Seasons. What causes the seasons?

Knowing the Heavens. Goals: Constellations in the Sky

Summary Sheet #1 for Astronomy Main Lesson

Knowing the Heavens. Goals: Constellations in the Sky

Discovering the Night Sky

Discovering the Night Sky

Knowing the Heavens. Chapter Two. Guiding Questions. Naked-eye (unaided-eye) astronomy had an important place in ancient civilizations

CELESTIAL COORDINATES

Astronomy 103: First Exam

LOCATING CELESTIAL OBJECTS: COORDINATES AND TIME. a. understand the basic concepts needed for any astronomical coordinate system.

Coordinates on the Sphere

Oberth: Energy vs. Momentum

A User s Guide to the Sky

TAKEN FROM HORIZONS 7TH EDITION CHAPTER 3 TUTORIAL QUIZ

Astronomy 120 Winter 2005 Highlights of Astronomy. First Midterm Examination

James T. Shipman Jerry D. Wilson Charles A. Higgins, Jr. Chapter 15 Place and Time

The Celestial Sphere. Chapter 1. Constellations. Models and Science. Constellations. Diurnal vs. Annular Motion 9/16/2010

Computer Activity #3 SUNRISE AND SUNSET: THE SEASONS

2. Descriptive Astronomy ( Astronomy Without a Telescope )

Practice Questions: Seasons #2

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself Pearson Education, Inc.

Chapter 1: Discovering the Night Sky. The sky is divided into 88 unequal areas that we call constellations.

Which table correctly shows the dates on which the apparent paths of the Sun were observed? A) B) C) D)

Phys Lab #1: The Sun and the Constellations

1.4j interpret simple shadow stick data to determine local noon and observer s longitude

Lecture 2: Motions of the Earth and Moon. Astronomy 111 Wednesday August 30, 2017

Lecture 4: DM: time and Diurnal Motion

C) the seasonal changes in constellations viewed in the night sky D) The duration of insolation will increase and the temperature will increase.

Venus Project Book, the Galileo Project, GEAR

Reminder: Seasonal Motion

The Earth, Moon, and Sky. Lecture 5 1/31/2017

Earth Moon Motions A B1

Astronomy 311 Professor Menningen January 2, Syllabus overview books & supplies course goals assignments & grading About the professor

Dr. Tariq Al-Abdullah

Introductions. Astronomy and Cosmologies week 1, Spring 2013, Chamberlain & Zita. how does the Sun appear to move? the sky as it does?

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

Brock University. Test 1, October 2016 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: October 3, 2016

The Celestial Sphere. From our perspective on Earth the stars appear embedded on a distant 2 dimensional surface the Celestial Sphere.

PHSC 1053: Astronomy Time and Coordinates

Chapter 2 Lecture. The Cosmic Perspective Seventh Edition. Discovering the Universe for Yourself

Name: Exam 1, 9/30/05

The following terms are some of the vocabulary that students should be familiar with in order to fully master this lesson.

Time and Diurnal Motion

Earth Science, 13e Tarbuck & Lutgens

Exercise 2: The UW planetarium

Early history of astronomy. Early history of astronomy. Positions in the sky. Lecture 3: The Sun & Constellations

ASTR 1P01 Test 1, May 2018 Page 1 BROCK UNIVERSITY. Test 1: Spring 2018 Number of pages: 10 Course: ASTR 1P01, Section 1 Number of students: 598

Practice Seasons Moon Quiz

Lunar Eclipse Wednesday (January 31 st ) Morning. Topics for Today s Class. PHYS 1403 Stars and Galaxies

Brock University. Test 1, September 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: September 29, 2014

Time and Diurnal Motion

CA1 2.11: Designing an Equatorial Sundial Activity

Midterm Review #2-2018

The. Astronomy is full of cycles. Like the day, the month, & the year In this section we will try to understand these cycles.

Summer solstice June 21, 2014

CHAPTER 2 A USER'S GUIDE TO THE SKY

COMPUTER ACTIVITY 3: THE SEASONS: LENGTH OF THE DAY

The celestial sphere, the coordinates system, seasons, phases of the moon and eclipses. Chapters 2 and S1

Time and Diurnal Motion. 1a. The Earth Is Flat. 1c. Aristotle ( BC) 1b. The Earth Is Round. Time and Diurnal Motion

5 - Seasons. Figure 1 shows two pictures of the Sun taken six months apart with the same camera, at the same time of the day, from the same location.

Daily Motions. Daily Motions. Solar and Sidereal Days. Annual Motions of the Sun. Coordinate system on Earth. Annual Motion of the Stars.

drinking straw, protractor, string, and rock. observer on Earth. Sun across the sky on March 21 as seen by an

ASTR 1P01 Test 1, September 2017 Page 1 BROCK UNIVERSITY

Chapter 3: Coordinates & time; much of this chapter is based on earlier work by Katherine Bracher

Coordinate Systems. Basis for any 3D Coordinate System. 2. Locate the x-y plane (the fundamental plane ) Usual approach to define angles:

2. 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.

Earth Science Seasons Test Name Per Date

Constellations In ancient times, constellations only referred to the brightest stars that appeared to form groups, representing mythological figures.

Time and Diurnal Motion. 1a. The Earth Is Flat. 1c. Aristotle ( BC) 1b. The Earth Is Round. Time and Diurnal Motion

What causes the seasons? 2/11/09

Before you Sit. Please Pick-up: Blue Information Sheet for Evening Observing. 1 Red and 1 Blue ticket for Observing/ Planetarium

The Earth and the Sky

Chapter 1 Image Slides. Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Physics 312 Introduction to Astrophysics Lecture 3

Geometry of Earth Sun System

Precession and The Celestial Poles

a. exactly 360 b. less than 360 c. more than 360 On Figure 1, draw the Earth the next day and justify your answer above.

Discovering the Universe for Yourself (Chapter 2) Years, Seasons, and Months: The Motions of Sun, Earth, and Moon

A. the spinning of Earth on its axis B. the path of the Sun around Earth

Geography Class 6 Chapters 3 and

Earth-Sun Relationships. The Reasons for the Seasons

Introduction to Astronomy

6/17. Universe from Smallest to Largest:

Astronomy 122 Section 1 TR Outline. The Earth is Rotating. Question Digital Computer Laboratory

Chapter 1 Review Clickers. The Cosmic Perspective Seventh Edition. A Modern View of the Universe Pearson Education, Inc.

The sky and the celestial sphere

FOR DISCUSSION TODAY: THE ANNUAL MOTION OF THE SUN

Transcription:

Review Clickers The Cosmic Perspective Seventh Edition Celestial Timekeeping and Navigation

How long does Earth take to make one full rotation, relative to the distant stars? a) 14 hours b) 24 hours c) about 23 hours and 56 minutes d) one year

How long does Earth take to make one full rotation, relative to the distant stars? a) 14 hours b) 24 hours c) about 23 hours and 56 minutes d) one year

Why do we call a day 24 hours, if Earth rotates once in 23 hours, 56 min? a) For simplicity it is about 24 hours. b) We measure a day by the position of the Sun, so Earth's revolution around the Sun affects the length of day. c) In order to have an even number of days in each month. d) Earth's epicycle is about 4 minutes.

Why do we call a day 24 hours, if Earth rotates once in 23 hours, 56 min? a) For simplicity it is about 24 hours. b) We measure a day by the position of the Sun, so Earth's revolution around the Sun affects the length of day. c) In order to have an even number of days in each month. d) Earth's epicycle is about 4 minutes.

How much do sidereal and solar clocks differ after one day? a) 4 minutes b) about an hour c) about two hours d) 24 hours

How much do sidereal and solar clocks differ after one day? a) 4 minutes b) about an hour c) about two hours d) 24 hours

How much do sidereal and solar clocks differ after one month? a) 4 minutes b) about an hour c) about two hours d) 24 hours

How much do sidereal and solar clocks differ after one month? a) 4 minutes b) about an hour c) about two hours d) 24 hours

The constellation Orion rises in the early evening December 1. When will it rise on January 1? a) about the same time b) depends on where you are in the US c) about four minutes earlier d) two hours earlier

The constellation Orion rises in the early evening December 1. When will it rise on January 1? a) about the same time b) depends on where you are in the US c) about four minutes earlier d) two hours earlier

The constellation Orion rises in the early evening December 1. When will it rise in August? a) about the same time b) depends on where you are in the US c) in the early morning, before dawn d) it won't rise in August

The constellation Orion rises in the early evening December 1. When will it rise in August? a) about the same time b) depends on where you are in the US c) in the early morning, before dawn d) it won't rise in August

The time of apparent noon varies with longitude. For convenience, we pretend that it doesn't for nearby places by using a) the equation of time. b) the analemma. c) time zones. d) precession.

The time of apparent noon varies with longitude. For convenience, we pretend that it doesn't for nearby places by using a) the equation of time. b) the analemma. c) time zones. d) precession.

The English poet Kipling, while in the tropics, wrote, "The sun comes up like thunder over China cross the bay." What astronomical truth inspired this? a) None; it's just poetry b) Sunrise is louder in the tropics. c) Sunrise is faster in the tropics. d) Sunrise is earlier in the tropics.

The English poet Kipling, while in the tropics, wrote, "The sun comes up like thunder over China cross the bay." What astronomical truth inspired this? a) None; it's just poetry b) Sunrise is louder in the tropics. c) Sunrise is faster in the tropics. d) Sunrise is earlier in the tropics.

Suppose that you live at latitude 40 degrees north in the US. How high does the Sun get at noon on June 21? a) 40 degrees above the southern horizon b) 50 degrees above the southern horizon c) 73 degrees above the southern horizon d) straight overhead

Suppose that you live at latitude 40 degrees north in the US. How high does the Sun get at noon on June 21? a) 40 degrees above the southern horizon b) 50 degrees above the southern horizon c) 73 degrees above the southern horizon d) straight overhead

During the month of March, the Sun's declination a) is increasing. b) is decreasing. c) remains constant. d) goes up and down over the course of each day. e) cannot be determined.

During the month of March, the Sun's declination a) is increasing. b) is decreasing. c) remains constant. d) goes up and down over the course of each day. e) cannot be determined.