IQ The most obvious systematic motions in the sky are the daily, or diurnal, changes caused by the Earth’s rotation. T F.

Slides:



Advertisements
Similar presentations
Motions of the Earth and Sky
Advertisements

Unit 9: Earth Cycles Vocabulary.
Chapter 17 Earth’s Cycles
Moon Phases and eclipses.
Prof. D.C. Richardson Sections
Observing the Universe for Yourself
The Sun-Earth-Moon System
Unit III: The Earth in Space
Climate and Latitude Sun’s rays spread over large area = cooler
Topic 4 Motions of the Earth, Moon, and Sun
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Observing Astronomy 315 Professor Lee Carkner Lecture 3.
Prologue Welcome to PH109 Exploring the Universe Dr. Michael L. Cobb Fall, 2003.
The Sky From Earth. Let’s Step Outside Where are the stars? What direction are we facing?
Constellations. Celestial Sphere Our Point of View.
Discovering the Universe for Yourself (Chapter 2) Years, Seasons, and Months: The Motions of Sun, Earth, and Moon.
OBSERVING THE SKY Chapter 1 Chapter 3 Constellations and Navigation Constellations and Navigation ORIGINS OF ASTRONOMY.
Astronomy 104 Lunar Phases AndEclipses January 24, 2007.
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Question 1 Constellations appear to move across the sky at night because 1) the Earth orbits the Sun. 2) the Moon orbits the Earth. 3) stars are in constant.
Sky Motions Diurnal Motion Annual Motion.
Chapter 1 Cycles of the Sky
Motions of the Earth Stuff everyone should know Chapters 2, 3.
Copyright © 2009 Pearson Education, Inc. Chapter 2 Discovering the Universe for Yourself.
Discovering the Universe for Yourself
Constellations A constellation is a region of the sky.
Chapter 1: The Cycles of the Sky
AST 112 Motion of Objects in the Sky. The Celestial Sphere Imagine you’re where Earth is, but there’s no Earth. What do you see? Keep in mind: – Nearest.
Chapter 2 Discovering the Universe for Yourself
 Rotation  The amount of time it takes for Earth to spin around once.  ONE DAY  Revolution  The amount of time it takes for Earth to go around the.
Welcome to PH109 Exploring the Universe Dr. Michael L. Cobb Fall, 2013.
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.
The Earth, Sun, and Moon.
The Sun, Earth, and Moon System
1. annular eclipse - the moon is not close enough to the earth to completely block the sun, so the sun rings the moon.
Motions of the Earth and Sky I. Outline for Today History: flat vs. spherical earth Map of the sky Constellations Diurnal and Yearly Motion The seasons.
Investigating Astronomy Timothy F. Slater, Roger A. Freeman Chapter 1 Predicting the Motions of the Stars, Sun, and Moon.
© 2010 Pearson Education, Inc. Discovering the Universe for Yourself.
Last time: 2.1. Patterns in The Sky: Stars and constellations, TODAY: celestial coordinates 2.2 Seasons,…Precession 2.2 (cont.) The Moon and Eclipses.
Chapter 1 Predicting the Motions of the Stars, Sun, and Moon.
Chapter 2 Discovering the Universe for Yourself. What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars as.
Astronomy 105 ä Student Information Sheet ä Class Syllabus ä Lab Syllabus ä Course Supplies ä Text ä Lab Manual ä Scantron 882-ES ä Flashlight with red.
Mastering Astronomy.
1 Lines in the Sky In order to use the sky to measure time you need to measure the location of objects in the sky. We will look at two methods of measuring.
IQ Solar eclipses can happen only near New Moon. True False.
Phases of the Moon Reasons for the Seasons Constell- ations Eclipses Celestial Sphere Using terms $ 200 $ 200$200 $ 200 $ 200 $400 $ 400$400 $ 400$400.
Quiz #1 Review Thursday, 15 September 2011 I list here the main topics and the main points for each topic. Study also the indicated lecture notes.
Copyright © 2015, W. W. Norton & Company Prepared by Lisa M. Will, San Diego City College Lecture Slides CHAPTER 2: Patterns in the Sky—Motions of Earth.
The Daily Motion As the Earth rotates, the sky appears to us to rotate in the opposite direction. The sky appears to rotate around the N (or S) celestial.
The sky Our place in space ConstellationsMeasurement Celestial Sphere Polaris and precession $ 200 $ 200$200 $ 200 $ 200 $400 $ 400$400 $ 400$400.
Sky Motions  Diurnal Motion Annual Motion. DIURNAL MOTION o Daily East / West motion of the sky Due to the Earth’s rotation (15°/hour) [360°/24 hours.
Phases of the Moon Reasons for the Seasons Constell- ations Eclipses Celestial Sphere Using terms $ 200 $ 200$200 $ 200 $ 200 $400 $ 400$400 $ 400$400.
Our Location on the Earth North South EastWest North South East you are here West.
What is apparent motion? Important to understand what we see and what is actually happening. Apparent motion is what we see from Earth Actual motion is.
Astronomy vs. Astrology Astronomy: Astronomy: The scientific study of matter in outer space, especially the positions, dimensions, distribution, motion,
Motion of the Moon. Review Question Describe the path the Sun will take across the sky on the day of the autumnal equinox as viewed from the Earth’s equator.
Chapter 2: Discovering the Universe for Yourself
THIS IS Jeopardy.
8.5 Motions of Earth, the Moon, and Planets
November 8,2010 Celestial Motions.
Motions in the sky: The celestial sphere
IQ The most obvious systematic motions in the sky are the daily, or diurnal, changes caused by the Earth’s rotation. T F.
The Sun-Earth-Moon System
8.5 Motions of Earth, the Moon, and Planets
IQ Solar eclipses can happen only near New Moon. True False.
The Earth, Sun, and Moon.
Sun Earth & Moon System.
Naked Eye Astronomy The Cycles of the Sun Summer Winter
Motions of Earth, the Moon, and Planets
ASTRO UNIT 1 REVIEW.
Presentation transcript:

IQ The most obvious systematic motions in the sky are the daily, or diurnal, changes caused by the Earth’s rotation. T F

IQ True! The Earth’s rotation causes the entire sky to appear to sweep from east to west once each day. This is (generally) the “fastest” motion we notice. The Earth’s rotation axis points at the north and south poles of the “celestial sphere.” The Earth’s equator projects to the equator of the celestial sphere.

IQ Solar eclipses can happen only near: A. New Moon B. Full Moon C. First quarter Moon D. Third quarter Moon

IQ A. New Moon is the correct answer! A solar eclipse occurs when the Sun is blocked by the Moon. This can only happen when the moon is between the Earth and the Sun, which is New Moon.

IQ Lunar eclipses can only happen at: A. New Moon B. First quarter C. Full Moon D. Third quarter

IQ C. Full Moon is correct. A lunar eclipse occurs when the Earth blocks the Sun’s light from the Moon. This can only happen when the Moon is opposite the Sun as seen from the Earth - that is, the Earth is between the Sun and Moon. That happens only at Full Moon!

IQ The Full Moon always rises at: A: Midnight B. Sunset C. Sunrise D. It is always in the sky

IQ B. Sunset is correct. The phases of the moon refer to the pattern of illumination on the hemisphere facing Earth. Full Moon occurs when the entire hemisphere is illuminated, which can only occur when the Moon is directly opposite the Sun as seen from the Earth. The full moon must rise just as the sun sets.

IQ Polaris (the North Star) just happens to be near the Earth’s rotation axis. T F

IQ The answer is True. Polaris just happens to be near the pole. As time progresses, the Earth’s precession will move the rotation axis away from Polaris.

IQ The sun appears in the zenith from Albuquerque: A. On the summer solstice B. On the winter solstice Only when the sun is farthest from the Earth Never!

IQ D. Never! The sun can appear directly overhead, in the zenith, only if one lives within 23.5° of the equator. The latitude of ABQ is 32°, so the sun can never be directly overhead.

IQ Astrology is a science. True False

IQ False is the correct answer. Astrology does not use the scientific method to verify its techniques and predictions. Principally because of the Earth’s precession, the constellations and sky signs of astrology no longer match the true positions of astronomical objects.