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

Slides:



Advertisements
Similar presentations
Knowing the Heavens Chapter Two.
Advertisements

The Science of Astronomy
Apparent/Actual Motions Summary
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Observing Astronomy 315 Professor Lee Carkner Lecture 3.
Chapter 2b: The Sky.
Prologue Welcome to PH109 Exploring the Universe Dr. Michael L. Cobb Fall, 2003.
IQ The most obvious systematic motions in the sky are the daily, or diurnal, changes caused by the Earth’s rotation. T F.
Miscellaneous announcements… Course web site is up to date with all handouts and Homework 1 solutions. Start planning your two observing projects. Questions.
The Earth Rotates.
John T. McGraw, Professor Laurel Ladwig, Planetarium Manager
The Sky From Earth. Let’s Step Outside Where are the stars? What direction are we facing?
The night sky? With the naked eye, we can see more than 2000 stars as well as the Milky Way. Remind students that we often use the term “constellation”
OBSERVING THE SKY Chapter 1 Chapter 3 Constellations and Navigation Constellations and Navigation ORIGINS OF ASTRONOMY.
Observing and the Sky Astronomy 311 Professor Lee Carkner Lecture 3.
Physics 101 Astronomy Dr. Brian Davies Office: 532 Currens Hall, Office Hours: M Tu W F 11-noon
Motions of the Celestial Sphere. Constellations Sky looks like a dome with the star painted on the inside. 88 constellations such as Ursa Major, Orion,
Ancient astronomy & celestial sphere ASTR 1010 Lecture 3.
Motion in the Sky. Discussion How do we estimate how far away things are from us in everyday life?
Sky Motions Diurnal Motion Annual Motion.
Chapter 1 Cycles of the Sky
Section 3 Constellations  Sections of sky with recognizable star patterns  Used by ancient people for navigation  Also used to keep track of time.
Fix Astronomy Chapter 1 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Constellations.
Astro Pages14-18 Chapter 2-2 THE SKY AND ITS MOTION.
Introduction to Astronomy.  Observations lead to theories and laws  Laws are concise statements that summaries a large number of observations.  Theories.
The Celestial Sphere Stars at different distances all appear to lie on the celestial sphere. The 88 official constellations cover the celestial sphere.
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 1 If you could hover over the Earth’s north rotational pole.
Observational Astrophysics in the visible light Shai Kaspi Technion - March 2015.
Latitude and longitude
Trivia Question of the Day. Astronomy Picture of the Day Astronomy Picture of the Day.
Sept. 25, Apparent motions: Moon, Sun, stars & Orbits Review the daily (diurnal) vs. monthly (sidereal) sky How about the Moon and its phases? Celestial.
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 4 - Space Lesson 17: Earth Movements – Rotation and Revolution.
Chapter 6: Earth’s Motions in Space Ms. Johnson Foundations.
A scientific model.  Why do we use the model of the celestial sphere when studying the night sky, even though it does not accurately represent three-dimensional.
Physics 101 Astronomy Dr. Brian M. Davies Office: 532 Currens Hall, Office Hours are M W F 11-noon and Tues 10-11:30 a.m.
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.
 Celestial Sphere: an imaginary sphere on which all the celestial objects would appear  Celestial object: any object in the sky that genuinely appears.
At the scale of the Milky Way Galaxy, distances are described in terms of Light-years, which is the distance light travels in one year.
Celestial Sphere Facts: It’s an imaginary sphere with earth in the center. It is useful for locating constellations and stars on a star map.
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.
EARTH IN SPACE. A reminder about earth  The earth is almost a sphere  We locate points on the sphere with 3 coordinates – Longitude (180º W º.
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.
Earth and Space Science
Chapter 2 Celestial Motions. Fig. 2.1 The Celestial Sphere To understand the idea of the celestial sphere first think of the earth in space. The stars.
AstroLab-2 Locating Stars in the Sky Merav Opher-Fall 2004.
Constellations pg. 65. Constellation section of the sky with a recognizable star pattern. 88 listed 48 from Ptolemy.
Local and Sky Coordinates
MOTIONS OF SKY. Goals To identify the different parts of the celestial sphere model To understand how to express the location of objects in the sky To.
Our Location on the Earth North South EastWest North South East you are here West.
Chapter 4: Rising & Setting Stars © BRIEF
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 Unit 1 The celestial sphere and the seasons.
Knowing the Heavens Chapter Two.
Constellations pg. 71.
Rotating Earth Sunlight animations © Swinburne.
1.5. Describing the Position of Objects in Space
Motions in the sky: The celestial sphere
Chapter 1 Cycles of the Sky
IQ The most obvious systematic motions in the sky are the daily, or diurnal, changes caused by the Earth’s rotation. T F.
Celestial Motions Chapter 2.
Motions of Earth, Moon and Sun
Chapter 1 Cycles of the Sky
Chapter 1 Cycles of the Sky
12/29/2018 The Sky.
The Sky (Celestial Sphere)
ASTRO UNIT 1 REVIEW.
Celestial Motions Chapter 2.
Homework #1 has been posted
Presentation transcript:

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

2 Announcements: Get clickers registered! Homework #2 due Tuesday Reading: Chp 1: sections 1.2 and 1.3

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 3 Naked-Eye Astronomy Celestial Sphere Diurnal Motion

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 4 Stonehenge: 5100 years old A Mayan building faces sunset Astronomical Alignments in Egyptian Tombs

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 5 Vocabulary: longitude/latitude celestial sphere celestial pole/equator horizon/zenith constellation ecliptic/zodiac

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 6 Rotational axis

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 7 Latitude: angle measured in north/south direction zero degrees at equator +90 degrees at north pole -90 degrees at south pole Longitude: angle measured in east/west direction zero degrees at Greenwich, England measured to 180 degrees east and west

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 8

9 The Celestial sphere Figure 1.2 x zenith

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 10 Horizon: defined by plane perpendicular to your body Zenith: the point directly above your head. changes with time!!

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 11 Celestial Pole: North and South pole projected onto celestial sphere. Celestial Equator: Earth’s equator projected onto celestial sphere.

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 12 Constellation: Orion

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 13 Orion

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 16 Constellations: The stars that comprise a constellation are not actually physically associated in space. Each is at a different distance from the Earth. If you could travel to a different star, you would not see the same patterns in the sky!!

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 17 Observing Astronomical Phenomena Daily: Monthly: Yearly: Other: Objects rise in the East and set in the West. Different constellations visible at different times of year. Moon seen at different “phases”.

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 18 Day and Night: The Spinning Earth Virtual planetarium…

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 19 If you could hover over the Earth’s north rotational pole and look down at the Earth as it spins, you would see that the Earth spins in a ____________ direction. a) clockwise b) counter-clockwise

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 20 The Rising and Setting Stars Figure 1.4 Virtual planetarium…

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 21 Rising and Setting Stars: Stars only rise perpendicular to the horizon if you happen to be living on the equator In the Northern hemisphere, stars rise inclined toward the south (to the north if you are in the southern hemisphere). At the poles, stars will not rise or set, but circle around you!!

Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 22 Constellations change with seasons Figure 1.5