The Human Condition. Worlds in Points of Light. Fields of Study. What to Expect. Lure of Naked-Eye Observing. Today. Remote.

Size: px
Start display at page:

Download "The Human Condition. Worlds in Points of Light. Fields of Study. What to Expect. Lure of Naked-Eye Observing. Today. Remote."

Transcription

1 Worlds in Points of Light (Naked Eye Observations) Star-like Worlds My Background Robert Dick February 28-April 4, 2018 Robert Dick, Bruce Penn., ON I have held the crescent Moon in the palm of my hand and bathed in the starlight of wonderland Path of the planets 1 Learning from light 2 Planet diversity 3 Remote sensing 4 Planetary evolution 5 Extra-solar planets 6 What to Expect Week (Naked-eye observing) (Astronomical instruments) (Planetary astronomy) (Magic instruments, intimacy) (Up-close and personal) (Check on reality) Science Fiction Philosophy Poetry Imagination Fields of Study Observations Common Sense Critical Thinking Curiosity Physics Chemistry Remote Sensing Geology The Human Condition ASTRONOMY Today Introductions Course Outline Overview of Sky (Celestial Sphere) Historical Perspective Early Astronomy Our Vision (Brightness) Vision (colour sensitivity) Lure of Naked-Eye Observing No expensive instruments Cheep past-time Simple experiments Changing patterns = changing geometry Intellectual mind-games (physics) Mathematics (algebra, calculus) Cultural insights Answers major questions (structure of the solar system, Universe) 1

2 Diurnal.jpg The Celestial Sphere R.A. Scale Course Starmap Declination Scale Date Scale Course Polar Maps Course Polar Map Polar Sky on March 5 Changes in Celestial Sphere Date Sky at 10 pm LST Fireball Celestial Sphere - A narrated Tour of the Night Sky - Diurnal Rotation 2

3 Moon s Orbit Meteors (meteorology) Independent from Ecliptic Moon is Spherical Rapid changes = close Orbit Tilted wobbles (precesses) occasional eclipses Random = uncertainty Robert Dick, Rideau Ferry, ON Starlight Theatre - Fireball, from Celestial Sphere - A Narrated Tour of the Night sky Project back to Inter-planetary orbit 400K km Shower = stream comet debris Tom Matheson, NJ Robert Dick, Baja, Mx 1991 Spherical Earth Solar Eclipse Lunar Eclipse Same Shadow Robert Dick, Rideau Ferry, ON Comets Note: Public interest No terror Orbits and origins - elongated orbits Newton s Laws Great Comet of 1680 Obscurity to prominence... then back to obscurity Robert Dick, Baja, Mx 1991 Utility of Astronomy Omens weather (clear, hazy) Navigation way-finding Time reckoning at night Geometry in motion Contemplation Astrology Importance for survival! 3

4 Astrology Greek Mythologies Existed before recorded history Practical Leisure Remuneration for astronomers Kept astronomy in the social consciousness The gods and wandering stars Planetoi = wandering star GREEK Hermes Aphrodite Ares Zeus Cronus Uranus Poseidon ROMAN Mercury Venus Mars Jupiter Saturn Caelus Neptune Greek Universe Ptolemaic System (Almagest) - perfect circles, - constant speeds Heavens Celestial Sphere Planets Atmosphere Earth/Mortals Depth into sky Made accurate with empirically derived data - planar solar system - deferents, epicycles, eccentrics equants Claudius Ptolemy Egypt, 2 nd C AD What they Deduced Ptolemaic System Predictive world system Philosophy-based (Aristotle) Immutable heavens Geometric purity Constant speed Circular motions Simplicity (?) Cultural Mystique Greek Discoveries Predicting the planets instructing the gods Works of Aristotle 1600-yrs religious dogma Heresy to question: - Earth-centred universe - circular and constant motion Hipparchus ( BCE) ( Polymath ) Recording observations Accurate star catalogue to replace older one precession Others Accurate measures of planet motion - geometry - brightness implies distance - epicycles,... 4

5 What They Taught Us Greek Experiment There are bright wandering objects They are constrained to narrow band (ecliptic) Their motion is smooth and predictable They vary in distance from us (brightness) There are two sets opposition, non-opposition [outer] [inner] Eratothenes 850 km/0.02 = 42,500 km [40,100 km] Diameter of Earth 200 BCE Conjunctions Oppositions 1/2 Aristarchus Moon Distance = Earth Lat. Earth Radius Star Angle D M = Lat. x E R = 5 x 6300 km * 1/12 = 380,000 km Aristarchus BCE BCE Eratothenes Moon s Distance 300 BCE Historical Perspective We start with the points of light. How much can our unaided eye show us (ancient and renaissance eras)? What observations can we make to confirm our present world view (stargazing)? Position, Brightness,... Motion Visual Techniques Record keeping - preservation of knowledge (Hipparchus BCE) Naked Eye - qualitative, cultural narratives (oral histories) - accuracy limited to ~1/2 degree (Moon) Visual Instruments (Sextans/Octants ~1000 ADE) - sights to fix eye s position in instrument - accuracy ~1/30-deg (~2 arc minutes (1600 ADE) 5

6 Arab Astronomy Date Time Stars Sextants (size = precision) Sun Based on Ptolemaic System - practical, unifying Translated Almagest to Arabic Samarkand Observatory and Sextant 15 th Century Diffused across Africa and southern Europe Enabled translation into Latin for posterity Astrolabe 220 BCE Present Visual Precision Natural Light Levels at Night Pupil diam. = 6mm Sextant arm = 1m 0.34 Better sight ~ 0.5mm /10 th brightness to read a book is natural limit (silvery grey) Scotopic 1/1000 th = walk-about at night - a practical limit - Photopic Tycho Brahe s Sextant 17 th Century 1m 1m 1cd 20,000 cd/m 2 Limits to Vision Brightness - Colour - Resolution Brightness Moon is bright, but ~ 1/1000 streetlight (1-4 million cd/m 2 ) Luminance Moon 6,000 cd/m 2 Moon Candle 20,000 Venus 15,000 Mars 4,000 Jupiter 800 Sun 3x10 9 1m LEDs Interesting Information Bronowski, Jacob - Assent of Man (A still-remarkable 13-part BBC Series) Pannekoek, A. - A History of Astronomy ( Dated interpretation of history) Interscience,

Worlds in Points of Light. What to Expect

Worlds in Points of Light. What to Expect Worlds in Points of Light What to Expect Vision and Intellect Week Path of the planets 1 Learning from light 2 Planet diversity 3 Remote sensing 4 Planetary evolution 5 Extra-solar planets 6 (Naked-eye

More information

Chapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Chapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter 2 The Rise of Astronomy Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Periods of Western Astronomy Western astronomy divides into 4 periods Prehistoric

More information

2X CLAUDIUS PTOLEMY BIOGRAPHY 1260L

2X CLAUDIUS PTOLEMY BIOGRAPHY 1260L 2X CLAUDIUS PTOLEMY BIOGRAPHY 1260L CLAUDIUS PTOLEMY AN EARTH-CENTERED VIEW OF THE UNIVERSE Born 85 CE Hermiou, Egypt Died 165 CE Alexandria, Egypt By Cynthia Stokes Brown The Earth was the center of the

More information

A100 Exploring the Universe: The Invention of Science. Martin D. Weinberg UMass Astronomy

A100 Exploring the Universe: The Invention of Science. Martin D. Weinberg UMass Astronomy A100 Exploring the Universe: The Invention of Science Martin D. Weinberg UMass Astronomy astron100-mdw@courses.umass.edu September 09, 2014 Read: Chap 3 09/09/14 slide 1 Problem Set #1: due this afternoon

More information

1. The Moon appears larger when it rises than when it is high in the sky because

1. The Moon appears larger when it rises than when it is high in the sky because 2-1 Copyright 2016 All rights reserved. No reproduction or distribution without the prior written consent of 1. The Moon appears larger when it rises than when it is high in the sky because A. you are

More information

Learning Objectives. one night? Over the course of several nights? How do true motion and retrograde motion differ?

Learning Objectives. one night? Over the course of several nights? How do true motion and retrograde motion differ? Kepler s Laws Learning Objectives! Do the planets move east or west over the course of one night? Over the course of several nights? How do true motion and retrograde motion differ?! What are geocentric

More information

The Copernican Revolution

The Copernican Revolution The Copernican Revolution Nicolaus Copernicus (1473-1543) De Revolutionibus Orbium Coelestium (1543) [ On the Revolutions of the Celestial Spheres ] The Ptolemaic Cosmology: Geocentric and Geostatic The

More information

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009 Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009 Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. Mark answer on Scantron.

More information

The History and Philosophy of Astronomy

The History and Philosophy of Astronomy Astronomy 350L (Fall 2006) The History and Philosophy of Astronomy (Lecture 3: Antiquity I) Instructor: Volker Bromm TA: Jarrett Johnson The University of Texas at Austin Astronomy and Cosmology in Antiquity:

More information

At Home Phases Demo. Astronomy 210. Section 1 MWF Astronomy Building. Geocentric vs. Heliocentric system. The Motion of the Planets

At Home Phases Demo. Astronomy 210. Section 1 MWF Astronomy Building. Geocentric vs. Heliocentric system. The Motion of the Planets Astronomy 210 Section 1 MWF 1500-1550 134 Astronomy Building This Class (Lecture 4): Early Cosmology HW #1 Due on Friday! Next Class: You missed the first planetarium show. Cosmic Revolution Music: Twilight

More information

A100 Exploring the Universe: The Rise of Science. Martin D. Weinberg UMass Astronomy

A100 Exploring the Universe: The Rise of Science. Martin D. Weinberg UMass Astronomy A100 Exploring the Universe: The Rise of Science Martin D. Weinberg UMass Astronomy weinberg@astro.umass.edu September 11, 2012 Read: Chap 3 09/11/12 slide 1 Problem Set #1 due this afternoon at 5pm! Read:

More information

Motions of the Planets ASTR 2110 Sarazin

Motions of the Planets ASTR 2110 Sarazin Motions of the Planets ASTR 2110 Sarazin Motion of Planets Retrograde Motion Inferior Planets: Mercury, Venus Always near Sun on Sky Retrograde motion when very close to Sun on sky (Every other time) Superior

More information

Chapter 02 The Rise of Astronomy

Chapter 02 The Rise of Astronomy Chapter 02 The Rise of Astronomy Multiple Choice Questions 1. The moon appears larger when it rises than when it is high in the sky because A. You are closer to it when it rises (angular-size relation).

More information

Chapter 3: Ancient Astronomy

Chapter 3: Ancient Astronomy Chapter 3: Ancient Astronomy Mesopotamian Astronomy(as early as 4000 BC) [fig 3-1 ziggeraut] Predictions of seasonal changes for agriculture source of modern zodiac divided circle into 360 degrees, each

More information

This Week... Week 3: Chapter 3 The Science of Astronomy. 3.1 The Ancient Roots of Science. How do humans employ scientific thinking?

This Week... Week 3: Chapter 3 The Science of Astronomy. 3.1 The Ancient Roots of Science. How do humans employ scientific thinking? Week 3: Chapter 3 The Science of Astronomy This Week... The Copernican Revolution The Birth of Modern Science Chapter 2 Walkthrough Discovering the solar system Creating a clockwork Universe 3.1 The Ancient

More information

Lecture 5. Motions of the Planets

Lecture 5. Motions of the Planets Lecture 5 Motions of the Planets; Geometric models of the Solar System Motion of Planets Opposition, Conjunction Retrograde Motion Scientific Method and "Models" Size of the Earth Geocentric vs Heliocentric

More information

The History of Astronomy. Theories, People, and Discoveries of the Past

The History of Astronomy. Theories, People, and Discoveries of the Past The History of Astronomy Theories, People, and Discoveries of the Past Early man recorded very little history. Left some clues in the form of petrographs. Stone drawings that show eclipses, comets, supernovae.

More information

18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton.

18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton. Name: Date: 1. The word planet is derived from a Greek term meaning A) bright nighttime object. B) astrological sign. C) wanderer. D) nontwinkling star. 2. The planets that were known before the telescope

More information

Earth Science, 13e Tarbuck & Lutgens

Earth Science, 13e Tarbuck & Lutgens Earth Science, 13e Tarbuck & Lutgens Origins of Modern Astronomy Earth Science, 13e Chapter 21 Stanley C. Hatfield Southwestern Illinois College Early history of astronomy Ancient Greeks Used philosophical

More information

The great tragedy of science the slaying of a beautiful hypothesis by an ugly fact. -Thomas Huxley. Monday, October 3, 2011

The great tragedy of science the slaying of a beautiful hypothesis by an ugly fact. -Thomas Huxley. Monday, October 3, 2011 The great tragedy of science the slaying of a beautiful hypothesis by an ugly fact. -Thomas Huxley 1 Chapter 4 The Origin of Modern Astronomy Outline I. The Roots of Astronomy A. Archaeoastronomy B. The

More information

Announcements. Topics To Be Covered in this Lecture

Announcements. Topics To Be Covered in this Lecture Announcements! Tonight s observing session is cancelled (due to clouds)! the next one will be one week from now, weather permitting! The 2 nd LearningCurve activity was due earlier today! Assignment 2

More information

Upon Whose Shoulders We Stand: A History of Astronomy Up to 200 A.D. Dick Mallot 3/17/2005

Upon Whose Shoulders We Stand: A History of Astronomy Up to 200 A.D. Dick Mallot 3/17/2005 Upon Whose Shoulders We Stand: A History of Astronomy Up to 200 A.D. Dick Mallot 3/17/2005 Who were these ancient astronomers? Where did real astronomy begin? What did we know about astronomy 2000+ years

More information

What was once so mysterious about planetary motion in our sky? We see apparent retrograde motion when we pass by a planet

What was once so mysterious about planetary motion in our sky? We see apparent retrograde motion when we pass by a planet What was once so mysterious about planetary motion in our sky? Planets usually move slightly eastward from night to night relative to the stars. You cannot see this motion on a single night. But sometimes

More information

Most of the time during full and new phases, the Moon lies above or below the Sun in the sky.

Most of the time during full and new phases, the Moon lies above or below the Sun in the sky. 6/16 Eclipses: We don t have eclipses every month because the plane of the Moon s orbit about the Earth is different from the plane the ecliptic, the Earth s orbital plane about the Sun. The planes of

More information

BROCK UNIVERSITY. 1. About 2300 years ago, Aristotle argued that the Earth is spherical based on a number of observations, one of which was that

BROCK UNIVERSITY. 1. About 2300 years ago, Aristotle argued that the Earth is spherical based on a number of observations, one of which was that BROCK UNIVERSITY Page 1 of 10 Test 2: November 2015 Number of pages: 10 Course: ASTR 1P01, Section 2 Number of students: 861 Examination date: 7 November 2015 Time limit: 50 min Time of Examination: 13:00

More information

Occam s Razor: William of Occam, 1340(!)

Occam s Razor: William of Occam, 1340(!) Reading: OpenStax, Chapter 2, Section 2.2 &2.4, Chapter 3, Sections 3.1-3.3 Chapter 5, Section 5.1 Last time: Scales of the Universe Astro 150 Spring 2018: Lecture 2 page 1 The size of our solar system,

More information

Review of previous concepts!! Earth s orbit: Year, seasons, observed constellations, Polaris (North star), day/night lengths, equinoxes

Review of previous concepts!! Earth s orbit: Year, seasons, observed constellations, Polaris (North star), day/night lengths, equinoxes Review of previous concepts!! Earth s orbit: Year, seasons, observed constellations, Polaris (North star), day/night lengths, equinoxes Celestial poles, celestial equator, ecliptic, ecliptic plane (Fig

More information

The astronomical system of Ptolemy of Alexandria (ca. 150 AD)

The astronomical system of Ptolemy of Alexandria (ca. 150 AD) 1 The astronomical system of Ptolemy of Alexandria (ca. 150 AD) Jan P. Hogendijk Dept of Mathematics, Utrecht May 12, 2011 2 The Almagest of Ptolemy (ca. A.D. 150) Basic work of Greek astronomy; much wiped

More information

Earth Science, 11e. Origin of Modern Astronomy Chapter 21. Early history of astronomy. Early history of astronomy. Early history of astronomy

Earth Science, 11e. Origin of Modern Astronomy Chapter 21. Early history of astronomy. Early history of astronomy. Early history of astronomy 2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 21 Earth Science 11e Tarbuck/Lutgens This work is protected by United States copyright laws and is provided solely for the use of instructors

More information

Lecture #5: Plan. The Beginnings of Modern Astronomy Kepler s Laws Galileo

Lecture #5: Plan. The Beginnings of Modern Astronomy Kepler s Laws Galileo Lecture #5: Plan The Beginnings of Modern Astronomy Kepler s Laws Galileo Geocentric ( Ptolemaic ) Model Retrograde Motion: Apparent backward (= East-to-West) motion of a planet with respect to stars Ptolemy

More information

History of Astronomy - Part I. Ancient Astronomy. Ancient Greece. Astronomy is a science that has truly taken shape only in the last couple centuries

History of Astronomy - Part I. Ancient Astronomy. Ancient Greece. Astronomy is a science that has truly taken shape only in the last couple centuries History of Astronomy - Part I Astronomy is a science that has truly taken shape only in the last couple centuries Many advances have been made in your lifetime However, astronomical concepts and ideas

More information

Lecture 3: History of Astronomy. Astronomy 111 Monday September 4, 2017

Lecture 3: History of Astronomy. Astronomy 111 Monday September 4, 2017 Lecture 3: History of Astronomy Astronomy 111 Monday September 4, 2017 Reminders Labs start this week Homework #2 assigned today Astronomy of the ancients Many ancient cultures took note of celestial objects

More information

2) The number one million can be expressed in scientific notation as: (c) a) b) 10 3 c) 10 6 d)

2) The number one million can be expressed in scientific notation as: (c) a) b) 10 3 c) 10 6 d) Astronomy Phys 181 Midterm Examination Choose the best answer from the choices provided. 1) What is the range of values that the coordinate Declination can have? (a) a) -90 to +90 degrees b) 0 to 360 degrees

More information

ASTR 2310: Chapter 2

ASTR 2310: Chapter 2 Emergence of Modern Astronomy Early Greek Astronomy Ptolemaic Astronomy Copernican Astronomy Galileo: The First Modern Scientist Kepler's Laws of Planetary Motion Proof of the Earth's Motion Early Greek

More information

Benefit of astronomy to ancient cultures

Benefit of astronomy to ancient cultures Benefit of astronomy to ancient cultures Usefulness as a tool to predict the weather (seasons) Usefulness as a tool to tell time (sundials) Central Africa (6500 B.C.) Alignments Many ancient cultures built

More information

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler Celestial motions The stars: Uniform daily motion about the celestial poles (rising and setting). The Sun: Daily motion around the celestial

More information

Ancient Astronomy. Lectures 5-6. Course website:

Ancient Astronomy. Lectures 5-6. Course website: Ancient Astronomy Lectures 5-6 Course website: www.scs.fsu.edu/~dduke/lectures Lectures 5-6 Almagest Books 9 13 geocentric vs. heliocentric point of view the wandering stars, or planets the two anomalies

More information

2X CLAUDIUS PTOLEMY BIOGRAPHY 780L

2X CLAUDIUS PTOLEMY BIOGRAPHY 780L 2X CLAUDIUS PTOLEMY BIOGRAPHY 780L CLAUDIUS PTOLEMY AN EARTH-CENTERED VIEW OF THE UNIVERSE Born 85 CE Hermiou, Egypt Died 165 CE Alexandria, Egypt By Cynthia Stokes Brown, adapted by Newsela Claudius Ptolemy

More information

BROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that

BROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that BROCK UNIVERSITY Page 1 of 10 Test 1: November 2014 Number of pages: 10 Course: ASTR 1P01, Section 2 Number of students: 30 Examination date: 10 November 2014 Time limit: 50 min Time of Examination: 9:00

More information

Origins of Modern Astronomy

Origins of Modern Astronomy PHYS 1411 Introduction to Astronomy Origins of Modern Astronomy Chapter 4 Topics in Chapter 4 Chapter 4 talks about the history of Astronomy and the development of the model of the solar system. Brief

More information

Observing the Universe for Yourself

Observing 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 information

Introduction to Science

Introduction to Science Introduction to Science Richard Johns Langara College, January 2014 The purpose of this book is to provide a basic understanding of some scientific theories, especially for students who haven t taken much

More information

Wednesday, January 28

Wednesday, January 28 Ptolemy to Copernicus Wednesday, January 28 Astronomy of the ancients Many ancient cultures took note of celestial objects and celestial lphenomena. They noted tdcertain ti patterns in the heavens and

More information

How the Greeks Used Geometry to Understand the Stars

How the Greeks Used Geometry to Understand the Stars previous index next How the Greeks Used Geometry to Understand the Stars Michael Fowler, University of Virginia 9/16/2008 Crystal Spheres: Plato, Eudoxus, Aristotle Plato, with his belief that the world

More information

Evidence that the Earth does not move: Greek Astronomy. Aristotelian Cosmology: Motions of the Planets. Ptolemy s Geocentric Model 2-1

Evidence that the Earth does not move: Greek Astronomy. Aristotelian Cosmology: Motions of the Planets. Ptolemy s Geocentric Model 2-1 Greek Astronomy Aristotelian Cosmology: Evidence that the Earth does not move: 1. Stars do not exhibit parallax: 2-1 At the center of the universe is the Earth: Changeable and imperfect. Above the Earth

More information

Planets & The Origin of Science

Planets & The Origin of Science Planets & The Origin of Science Reading: Chapter 2 Required: Guided Discovery (p.44-47) Required: Astro. Toolbox 2-1 Optional: Astro. Toolbox 2-2, 2-3 Next Homework Due. Sept. 26 Office Hours: Monday,

More information

Greek astronomy: Introduction

Greek astronomy: Introduction 1 Greek astronomy: Introduction Jan P. Hogendijk Mathematics Dept, Utrecht University May 12, 2011 2 Greek astronomy Rough periodization 600-400 B.C. Philosophical speculations on the universe 400-300

More information

ASTRO 6570 Lecture 1

ASTRO 6570 Lecture 1 ASTRO 6570 Lecture 1 Historical Survey EARLY GREEK ASTRONOMY: Earth-centered universe - Some radical suggestions for a sun-centered model Shape of the Earth - Aristotle (4 th century BCE) made the first

More information

First MIDTERM Exam: Mon, Sep. 22, covering chapters tutorials (review later today).

First MIDTERM Exam: Mon, Sep. 22, covering chapters tutorials (review later today). Announcements First MIDTERM Exam: Mon, Sep. 22, covering chapters 1 3 + tutorials (review later today). Interim grades online, coded by class ID. See course website Grades tab. Another great night for

More information

Hipparchus of Rhodes.

Hipparchus of Rhodes. Hipparchus of Rhodes Hipparchus worked from about 160 to 130 B.C. He was a mathematician who used geometry to try to solve the problem of retrograde motion. http://universe-review.ca/i08-18-hipparchus.jpg

More information

Ancient Cosmology: A Flat Earth. Alexandria

Ancient Cosmology: A Flat Earth. Alexandria Today Competing Cosmologies Geocentric vs. Heliocentric Ptolemy vs. copernicus Retrograde Motion Phases of Venus Galileo FIRST HOMEWORK DUE How d it work? Ancient Cosmology: A Flat Earth Here there be

More information

Chapter 3 The Science of Astronomy

Chapter 3 The Science of Astronomy Chapter 3 The Science of Astronomy 3.1 The Ancient Roots of Science Our goals for learning: In what ways do all humans employ scientific thinking? How did astronomical observations benefit ancient societies?

More information

Introduction to the sky

Introduction 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 information

HISTORY OF ASTRONOMY, PART 1. How our understanding of the Universe has changed

HISTORY OF ASTRONOMY, PART 1. How our understanding of the Universe has changed HISTORY OF ASTRONOMY, PART 1 How our understanding of the Universe has changed Focus Question: How and why has our understanding of the universe changed over time? The oldest science? As far back as the

More information

SCIENCE 9 CHAPTER 10 SECTION 1

SCIENCE 9 CHAPTER 10 SECTION 1 SCIENCE 9 CHAPTER 10 SECTION 1 Observing the Stars (pp. 352-365) Celestial Bodies Celestial body: a natural object in space, such as the Sun, the Moon, a planet, or a star Star: a celestial body of hot

More information

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

Lecture 2: Motions of the Earth and Moon. Astronomy 111 Wednesday August 30, 2017 Lecture 2: Motions of the Earth and Moon Astronomy 111 Wednesday August 30, 2017 Reminders Online homework #1 due Monday at 3pm Labs start next week Motions of the Earth ASTR111 Lecture 2 Observation:

More information

Directions: Read each slide

Directions: Read each slide Directions: Read each slide and decide what information is needed. Some slides may have red or yellow or orange underlined. This information is a clue for you to read more carefully or copy the information

More information

Lecture 2 : Early Cosmology

Lecture 2 : Early Cosmology Lecture 2 : Early Cosmology Getting in touch with your senses Greek astronomy/cosmology The Renaissance (part 1) 8/28/13 1 Sidney Harris Discussion : What would an unaided observer deduce about the Universe?

More information

2. See FIGURE B. This person in the FIGURE discovered that this planet had phases (name the planet)?

2. See FIGURE B. This person in the FIGURE discovered that this planet had phases (name the planet)? ASTRONOMY 2 MIDTERM EXAM PART I SPRING 2019 60 QUESTIONS 50 POINTS: Part I of the midterm constitutes the Take-Home part of the entire Midterm Exam. Additionally, this Take-Home part is divided into two

More information

The following notes roughly correspond to Section 2.4 and Chapter 3 of the text by Bennett. This note focuses on the details of the transition for a

The following notes roughly correspond to Section 2.4 and Chapter 3 of the text by Bennett. This note focuses on the details of the transition for a The following notes roughly correspond to Section 2.4 and Chapter 3 of the text by Bennett. This note focuses on the details of the transition for a geocentric model for understanding the universe to a

More information

Phys Homework Set 2 Fall 2015 Exam Name

Phys Homework Set 2 Fall 2015 Exam Name Exam Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) About how many stars are visible on a clear, dark night with the naked eye alone? 1)

More information

Phys Homework Set 2 Fall 2015 Exam Name

Phys Homework Set 2 Fall 2015 Exam Name Exam Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Increasing the temperature of a blackbody by a factor of 2 will increase its energy by

More information

Lecture #4: Plan. Early Ideas of the Heavens (cont d): Geocentric Universe Heliocentric Universe

Lecture #4: Plan. Early Ideas of the Heavens (cont d): Geocentric Universe Heliocentric Universe Lecture #4: Plan Early Ideas of the Heavens (cont d): Shape & size of the Earth Size & distance of Moon & Sun Geocentric Universe Heliocentric Universe Shape of the Earth Aristotle (Greece, 384 322 B.C.)

More information

Ancient Astronomy. Kickin it old school

Ancient Astronomy. Kickin it old school Ancient Astronomy Kickin it old school Ancient Egypt Ancient Egyptians Only basic nocturnal timekeeping Yearly calendar secondary to Nile River Floods Sometimes needed a 13 th leap month Regulated by the

More information

3) During retrograde motion a planet appears to be A) dimmer than usual. B) the same brightness as usual C) brighter than usual.

3) 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 information

1) Kepler's third law allows us to find the average distance to a planet from observing its period of rotation on its axis.

1) 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 information

Astronomy 100 Section 2 MWF Greg Hall. Outline. Total Lunar Eclipse Time Lapse. Homework #1 is due Friday, 11:50 a.m.!!!!!

Astronomy 100 Section 2 MWF Greg Hall. Outline. Total Lunar Eclipse Time Lapse. Homework #1 is due Friday, 11:50 a.m.!!!!! Astronomy 100 Section 2 MWF 1200-1300 100 Greg Hall Leslie Looney Phone: 217-244-3615 Email: lwl @ uiuc. edu Office: Astro Building #218 Office Hours: MTF 10:30-11:30 a.m. or by appointment Homework #1

More information

Astronomy 110 Lecture Fall, 2005 Astronomy 110 1

Astronomy 110 Lecture Fall, 2005 Astronomy 110 1 Astronomy 110 Lecture 5 + 6 Fall, 2005 Astronomy 110 1 Planets Known in Ancient Times Mercury difficult to see; always close to Sun in sky Venus very bright when visible morning or evening star Mars noticeably

More information

History of Astronomy. Historical People and Theories

History of Astronomy. Historical People and Theories History of Astronomy Historical People and Theories Plato Believed he could solve everything through reasoning. Circles and Spheres are good because they are perfect (never ending) and pleasing to the

More information

Dive into Saturn.

Dive into Saturn. Dive into Saturn http://www.pbs.org/wgbh/nova/space/death-dive-to-saturn.html Read Ch. 3 By next class time Do practice online quiz 01 Axis tilt changes directness of sunlight during the year. Why Does

More information

AST 2010 Descriptive Astronomy Study Guide Exam I

AST 2010 Descriptive Astronomy Study Guide Exam I AST 2010 Descriptive Astronomy Study Guide Exam I Wayne State University 1 Introduction and overview Identify the most significant structures in the universe: Earth, planets, Sun, solar system, stars,

More information

Topic 1: Celestial Objects, phenomena, and interactions are important to people in many different ways.

Topic 1: Celestial Objects, phenomena, and interactions are important to people in many different ways. Topic 1: Celestial Objects, phenomena, and interactions are important to people in many different ways. To complete this booklet you must do the following: Define each term within this booklet Answer Each

More information

ASTR 1010 Spring 2016 Study Notes Dr. Magnani

ASTR 1010 Spring 2016 Study Notes Dr. Magnani The Copernican Revolution ASTR 1010 Spring 2016 Study Notes Dr. Magnani The Copernican Revolution is basically how the West intellectually transitioned from the Ptolemaic geocentric model of the Universe

More information

Name: Exam 1, 9/30/05

Name: Exam 1, 9/30/05 Multiple Choice: Select the choice that best answers each question. Write your choice in the blank next to each number. (2 points each) 1. At the North Pole in mid-november, the sun rises at a. North of

More information

Ch 22 Origin of Modern Astronomy Notes Ch 22.1 Early Astronomers Astronomy Astrology A. Ancient Greece B. Two Basic Theories Existed:

Ch 22 Origin of Modern Astronomy Notes Ch 22.1 Early Astronomers Astronomy Astrology A. Ancient Greece B. Two Basic Theories Existed: Ch 22 Origin of Modern Astronomy Notes Ch 22.1 Early Astronomers Astronomy: The science that studies the universe, dealing with properties of objects in space. Astrology: A belief that the positions of

More information

Physics 107 Ideas of Modern Physics (uw.physics.wisc.edu/~rzchowski/phy107) Goals of the course. What will we cover? How do we do this?

Physics 107 Ideas of Modern Physics (uw.physics.wisc.edu/~rzchowski/phy107) Goals of the course. What will we cover? How do we do this? Physics 107 Ideas of Modern Physics (uw.physics.wisc.edu/~rzchowski/phy107) Main emphasis is Modern Physics: essentially post-1900 Why 1900? Two radical developments: Relativity & Quantum Mechanics Both

More information

Early Models of the Universe. How we explained those big shiny lights in the sky

Early Models of the Universe. How we explained those big shiny lights in the sky Early Models of the Universe How we explained those big shiny lights in the sky The Greek philosopher Aristotle (384 322 BCE) believed that the Earth was the center of our universe, and everything rotated

More information

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

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 information

Things to do today. Terminal, Astronomy is Fun. Lecture 24 The Science of Astronomy. Scientific Thinking. After this lecture, please pick up:

Things to do today. Terminal, Astronomy is Fun. Lecture 24 The Science of Astronomy. Scientific Thinking. After this lecture, please pick up: Things to do today After this lecture, please pick up: Review questions for the final exam Homework#6 (due next Tuesday) No class on Thursday (Thanksgiving) Final exam on December 2 (next Thursday) Terminal,

More information

In so many and such important. ways, then, do the planets bear witness to the earth's mobility. Nicholas Copernicus

In so many and such important. ways, then, do the planets bear witness to the earth's mobility. Nicholas Copernicus In so many and such important ways, then, do the planets bear witness to the earth's mobility Nicholas Copernicus What We Will Learn Today What did it take to revise an age old belief? What is the Copernican

More information

cosmogony geocentric heliocentric How the Greeks modeled the heavens

cosmogony geocentric heliocentric How the Greeks modeled the heavens Cosmogony A cosmogony is theory about ones place in the universe. A geocentric cosmogony is a theory that proposes Earth to be at the center of the universe. A heliocentric cosmogony is a theory that proposes

More information

1UNIT. The Universe. What do you remember? Key language. Content objectives

1UNIT. 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 information

Space Notes Covers Objectives 1 & 2

Space Notes Covers Objectives 1 & 2 Space Notes Covers Objectives 1 & 2 Space Introduction Space Introduction Video Celestial Bodies Refers to a natural object out in space 1) Stars 2) Comets 3) Moons 4) Planets 5) Asteroids Constellations

More information

Origin of Modern Astronomy Chapter 21

Origin of Modern Astronomy Chapter 21 Origin of Modern Astronomy Chapter 21 Early history of astronomy Ancient Greeks Used philosophical arguments to explain natural phenomena Also used some observa:onal data (looking at the night sky) Ancient

More information

The Puzzle of Planetary Motion versus

The Puzzle of Planetary Motion versus The Puzzle of Planetary Motion versus Finding Earth s place in the Universe Observing the Planets Five of the planets are bright enough to be seen by the unaided eye. This view shows the sky after sunset

More information

Chapter 2 Discovering the Universe for Yourself

Chapter 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 information

How big is the Universe and where are we in it?

How big is the Universe and where are we in it? Announcements Results of clicker questions from Monday are on ICON. First homework is graded on ICON. Next homework due one minute before midnight on Tuesday, September 6. Labs start this week. All lab

More information

Introduction To Modern Astronomy I

Introduction To Modern Astronomy I ASTR 111 003 Fall 2006 Lecture 03 Sep. 18, 2006 Introduction To Modern Astronomy I Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch1: Astronomy and the Universe Ch2: Knowing the Heavens

More information

D. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified

D. 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 information

[05] Historical Perspectives (9/12/17)

[05] Historical Perspectives (9/12/17) 1 [05] Historical Perspectives (9/12/17) Upcoming Items 1. Homework #2 due now. 2. Read Ch. 4.1 4.2 and do self-study quizzes. 3. Homework #3 due in one week. Ptolemaic system http://static.newworldencyclopedia.org/thumb/3/3a/

More information

Introduction To Modern Astronomy II

Introduction To Modern Astronomy II ASTR 111 003 Fall 2006 Lecture 03 Sep. 18, 2006 Introduction To Modern Astronomy II Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch1: Astronomy and the Universe Ch2: Knowing the Heavens

More information

The History of Astronomy

The History of Astronomy The History of Astronomy The History of Astronomy Earliest astronomical record: a lunar calendar etched on bone from 6500 B.C. Uganda. Also we find early groups noted the Sun, Moon, Mercury, Venus, Earth,

More information

Days of the week: - named after 7 Power (moving) objects in the sky (Sun, Moon, 5 planets) Models of the Universe:

Days of the week: - named after 7 Power (moving) objects in the sky (Sun, Moon, 5 planets)   Models of the Universe: Motions of the Planets ( Wanderers ) Planets move on celestial sphere - change RA, Dec each night - five are visible to naked eye Mercury, Venus, Mars, Jupiter, Saturn Days of the week: - named after 7

More information

9/12/2010. The Four Fundamental Forces of Nature. 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force

9/12/2010. The Four Fundamental Forces of Nature. 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force The Four Fundamental Forces of Nature 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force The Universe is made of matter Gravity the force of attraction between matter

More information

Planetary Motion from an Earthly Perspective

Planetary Motion from an Earthly Perspective 1 Planetary Motion from an Earthly Perspective Stars appear fixed from night-to-night providing the familiar background of the constellations and asterisms. We see the same star patterns that were visible

More information

Astronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric

Astronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric Around 2500 years ago, Pythagoras began to use math to describe the world around him. Around 200 years later, Aristotle stated that the Universe is understandable and is governed by regular laws. Most

More information

In the beginning. Origin of Modern Astronomy Ch 22. Early Astronomy Early Astronomy/ Ancient Greece

In the beginning. Origin of Modern Astronomy Ch 22. Early Astronomy Early Astronomy/ Ancient Greece In the beginning Origin of Modern Astronomy Ch 22 GOD created the HEAVENS and the EARTH. (Gen. 1:1) 22.1 Early Astronomy/ Ancient Greece Astronomy: The science that studies the universe, dealing with properties

More information

PHYS 155 Introductory Astronomy

PHYS 155 Introductory Astronomy PHYS 155 Introductory Astronomy - observing sessions: Sunday Thursday, 9pm, weather permitting http://www.phys.uconn.edu/observatory - Exam - Tuesday March 20, - Review Monday 6:30-9pm, PB 38 Marek Krasnansky

More information

Planets in the Sky ASTR 101 2/16/2018

Planets in the Sky ASTR 101 2/16/2018 Planets in the Sky ASTR 101 2/16/2018 1 Planets in the Sky 2018 paths of Jupiter among stars (2017/2018) Unlike stars which have fixed positions in the sky (celestial sphere), planets seem to move with

More information

Chapter 4. The Origin Of Modern Astronomy. Is okay to change your phone? From ios to Android From Android to ios

Chapter 4. The Origin Of Modern Astronomy. Is okay to change your phone? From ios to Android From Android to ios Chapter 4 The Origin Of Modern Astronomy Slide 14 Slide 15 14 15 Is Change Good or Bad? Do you like Homer to look like Homer or with hair? Does it bother you when your schedule is changed? Is it okay to

More information