ASTRO 6570 Lecture 1
|
|
- Herbert Freeman
- 5 years ago
- Views:
Transcription
1 ASTRO 6570 Lecture 1 Historical Survey
2 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 known reference: - Spherical shape of Earth s shadow during a lunar eclipse. - Stars rise to a different altitude depending on where you are on Earth. Obliquity of Earth - Angle between plane of the Sun s motion in the sky (the ecliptic) and the plane of Earth s equator. - Known in the 6 th century BCE measured angle differences for shadows at the summer solstice and the winter solstice Tropic of Cancer is at ; tropic of Capricorn is at Eratosthenes ( BCE) measured a difference of 11/83 of a circle = Real value NOW = has decreased by ~15 since antiquity.
3 Horizontal sundial tracks of shadow with time of day and season
4 Credit : Jean-Pol GRANDMONT Meridian Line at the Church of Santa Maria degli Angeli, Rome (~1700 AD).
5 ECLIPTIC and the ZODIAC: Looking from Earth, the Sun moves in the Ecliptic plane defined by solar eclipses since you can t see the stars around the Sun. Ecliptic plane corresponds to the Zodiac the constellations through which the Sun and planets pass during a year. Babylonian astronomers knew about the Zodiac in the 6 th century BC; Greeks in the 5 th century.
6 OBLIQUITY- angle between the plane of the planet s orbit about the Sun and the plane of the planet s equator Object Axial tilt ( ) Mercury ~0.01 Venus Earth Moon Mars Ceres ~4 Jupiter 3.13 Saturn Uranus Neptune Pluto Variations: Earth: from to with a period of 42,000 yrs Mars: from ~11 0 to 59 0 (huge!) Earth s obliquity is stabilized by the Moon; this may change in about 1.5 billion years as the Moon moves away from the Earth.
7 ECLIPTIC and the ZODIAC (cont d.): The Greek astronomer Hipparcos (130 BCE) discovered precession of the equinoxes. In 2500 years, at 50 per year, precession amounts to 35 deg, or just over 1 sign of the Zodiac (360/12). From Dr John Smetanka St Vincent College So the node was in Aries in the Greek period.
8 Astronomical coordinates: Right Ascension and Declination (analogous to Longitude and Latitude on Earth) Need to specify the date (epoch) due to precession of the Earth s equatorial plane, which slowly moves the Vernal equinox. Modern star catalogs give positions at the Epoch J2000 = 2000 Jan 0.5 UT.
9 SIZES and DISTANCES: 1. Size of the Earth Eratosthenes ( BCE librarian of Alexandria) Arc length = R x θ (radians) When the Sun was right overhead at Syene near Aswan on the Nile river as determined using a well, he measured the shadow angle at Alexandria on the Mediterranean coast of Egypt, using a Gnomen which measures angles as a fraction of a circle. He found an angle of 1/50 of a circle. The distance was estimated at 5,040 stadia (I stadium thought to be about m) => 250,000 stadia for the circumference of the Earth. => R = 6,270 km, which is VERY CLOSE to the true value of 6,370 km, but possibly somewhat accidental given the difficulty of the measurement.
10 Relative sizes of the MOON & SUN: Aristarchus (~ BCE) Quarter moon EMS = 90 0 From solar eclipses Aristarchus knew that the angular size of the Moon is approximately the same as that of the Sun. Therefore: Sun 19 x size of the Moon He also estimated the size of the Moon relative to that of Earth at ~1/4 using lunar eclipses, and thus concluded that the Sun is ~5 times larger than Earth.
11 PLANETARY ORBITS Motion of the Sun: The working assumption was that the Sun moved at uniform speed on a circle centered on Earth but inclined to Earth s equator by => Equal periods for all seasons. But early Greeks realized that the lengths of the seasons are not the same! Hipparcos (~130 BCE) measured: Spring = 94 ½ days; Autumn = 88 1/8 days; Summer = 92 ½ days Winter = 90 1/8 days [We know now that this is because the orbit of Earth is an ellipse and its velocity varies with its orbital location.] Greeks did not know this, so they had to sacrifice one assumption è They kept circles & constant speed, but gave up on Earth at center of circle. (Note that precession has since moved the Equinox back by ~35 deg wrt perihelion.)
12 Got here, 25 Jan
13 RETROGRADE LOOPS Question faced by Greek astronomers: If the planets are also in circular orbits about Earth then why, at opposition (opposite the Sun) do the outer planets appear to go backwards in the sky? In a heliocentric model of the solar system this is due to the relative orbital motions of Earth and the outer planet. Consider Earth and Mars: Periods = 1.0 yr and 1.9 yr. As Earth passes Mars, Mars appears to go backwards with respect to the stars. Copernicus (1543) showed that retrograde loops were a natural consequence of a Sun-centered solar system.
14 EPICYCLES Greeks solved the problem differently they made the planets move around the Earth on epicycles! First suggested by Apollonius but did not fully account for the observations. PTOLEMY (1 st half of 2 nd century AD in Alexandria) refined previous models, to reach the culmination of Greek astronomy: Epicycle center moves at uniform angular speed on a circle the Deferent about the Equant that is a point off-center from the circle, opposite the Earth. Mars, Jupiter and Saturn s epicycles are aligned with one another & with the Earth-Sun line. Complicated but provided very accurate predictions of the orbits of the planets. Ptolemaic theory held sway for ~1,400 years until the Copernican revolution in 1543.
15 Tycho Brahe Very accurate positional measurements of the planets Johannes Kepler Used Tycho Brahe s measurements to determine orbital laws.
16 Johannes Kepler ( ) - THE THREE LAWS (based on the very precise observations of Tycho Brahe) 1. Planetary orbits are ellipses with the Sun at one focus (1610). 2. The radius vector from the Sun to the planet sweeps out equal areas in equal times - i.e. r 2 dθ/dt = constant (1610). 3. The orbital period squared is proportional to the semi-major axis of the ellipse cubed (1619). i.e. a 3 /P 2 = C = constant N.B. If a the semi-major axis - is in units of AU and P the orbital period - is in years, Then C = 1 REMEMBER THIS! If a and P are in physical units then C = G (M sun + M planet )/4π 2 G = Gravitational constant Newton
17 CONCEPTS of the UNIVERSE Plato & Aristotle: crystal spheres around Earth Hipparchus & Ptolemy: Circular orbits and epicycles - good predictions but very complicated - by 1,500 AD there were 79 variables fitted Copernicus: Heliocentric system; circular orbits. (On the Revolutions of the Heavenly Spheres, 1543) Kepler: Heliocentric system with elliptical orbits. (The New Astronomy, 1610)
18 Galileo Galilei (1564 (?) 1642 Giordano Bruno 1600 Galileo s telescope about 2 cm effective aperture Jupiter and its moons (1609) years since the first telescope International Year of Astronomy
19 ORBITS: Confirmation of the heliocentric model of the solar system 1. Galileo (1609 and 1610) - Observed that Venus showed phases just like the Moon. - not correct with the epicycle model (Venus is never fully lit) - Discovered the Jovian (Galilean) satellites. - clearly in orbit about Jupiter a mini-solar system 2. Bradley (1783) - Detected stellar aberration a shift in apparent position of a star due to velocity of Earth in its orbit - Position shift is v Earth /c = 10-4 rad = 20 arcsec. 3. Bessel (1830) - Observed stellar parallax shift in apparent nearby star position when observed from Earth at different locations in its orbit. - Position shift is ~ a Earth /D = 1 arcsec at D = 1 pc = 206,265 AU.
20 Planetary symbols: Mostly Inherited from the Greeks. Still used by modern planetary scientists. Handy numbers (approximate only!): One AU = Earth Sun distance = 150 x 10 6 km Lunar orbit semi-major axis 60 Earth radii Earth radius 6,400 km 4 lunar radii Jupiter radius 10 Earth radii Solar radius 10 Jupiter radii 100 Earth radii Angular size of Moon and Sun or ~0.01 radians
21 ASTRONOMICAL DISTANCE SCALE: Astronomical Unit (AU): Mean distance from Earth to the Sun (1 AU = x 10 6 km) Light year: Distance light travels in one year (= x km) Parsec: Distance at which 1.0 AU subtends 1 arc sec, or ~ 206,265 AU (in physical units, 1 pc = x km ~ 3.26 light years) - common unit for distances in our galaxy and the universe Kiloparsec (kpc), megaparsec (Mpc) and gigaparsec (Gpc) are used on galactic and extragalactic scales. Velocity of light: = x 10 8 m s -1 = 300 m per microsec
22 Some Modern discoveries Uranus discovered by Herschel in Ceres and Pallas discovered by Piazzi in ~1801. Neptune discovered by Adams, Leverrier and Galle in Satellites of Mars seen by Hall, Pluto discovered by Tombaugh, Rings of Uranus (1977), Jupiter (1979) & Neptune (1986). Satellite of Pluto discovered by Christie, First Kuiper belt object (QB1) discovered in First extrasolar planets discovered, 1992, 1995 (51Peg b).
23 We are probably nearing the limit of all we can know about astronomy. - Simon Newcomb, leading US astronomer, 1888
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 informationEarth 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 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 informationThe 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 informationPractice 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 informationEarth 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 informationBenefit 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 informationLecture #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 information2) 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 information1. 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 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 informationEarly Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle
Planetary Motion Early Theories Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle Stars appear to move around Earth Observations showed
More informationASTR 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 informationGravitation 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 informationLecture 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 informationTest 1 Review Chapter 1 Our place in the universe
Test 1 Review Bring Gator 1 ID card Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the scantrons Formulas will be projected on the screen You can use
More information18. 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 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 informationHistory 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 informationOccam 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 informationLecture #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 informationAstronomy 1010 Planetary Astronomy Sample Questions for Exam 1
Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1 Chapter 1 1. A scientific hypothesis is a) a wild, baseless guess about how something works. b) a collection of ideas that seems to explain
More informationChapter 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 informationChapter 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 informationASTR-1010: Astronomy I Course Notes Section III
ASTR-1010: Astronomy I Course Notes Section III Dr. Donald G. Luttermoser Department of Physics and Astronomy East Tennessee State University Edition 2.0 Abstract These class notes are designed for use
More informationAncient 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 informationIn The Beginning and Cosmology Becomes a Science
In The Beginning and Cosmology Becomes a Science Naked-eye (unaided-eye) astronomy had an important place in ancient civilizations Positional astronomy the study of the positions of objects in the sky
More informationAnnouncements. 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 informationOrigin 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 informationAy 1 Lecture 2. Starting the Exploration
Ay 1 Lecture 2 Starting the Exploration 2.1 Distances and Scales Some Commonly Used Units Distance: Astronomical unit: the distance from the Earth to the Sun, 1 au = 1.496 10 13 cm ~ 1.5 10 13 cm Light
More informationIn The Beginning and Cosmology Becomes a Science
In The Beginning and Cosmology Becomes a Science Naked-eye (unaided-eye) astronomy had an important place in ancient civilizations Positional astronomy the study of the positions of objects in the sky
More informationPHYS 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 informationUnit 2: Celestial Mechanics
Unit 2: Celestial Mechanics The position of the Earth Ptolemy (90 168 AD) Made tables that allowed a user to locate the position of a planet at any past, present, or future date. In order to maintain circular
More informationAstronomy I Exam I Sample Name: Read each question carefully, and choose the best answer.
Name: Read each question carefully, and choose the best answer. 1. During a night in Schuylkill Haven, most of the stars in the sky (A) are stationary through the night. (B) the actual motion depends upon
More informationb. Remember, Sun is a second or third generation star the nebular cloud of dust and gases was created by a supernova of a preexisting
1. Evolution of the Solar System Nebular hypothesis, p 10 a. Cloud of atoms, mostly hydrogen and helium b. Gravitational collapse contracted it into rotating disc c. Heat of conversion of gravitational
More informationAST 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 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 informationPosition 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set.
Position 3 None - it is always above the horizon. N E W S Agree with student 2; star B never crosses horizon plane, so it can t rise or set. Imaginary plane No; the Earth blocks the view. Star A at position
More informationLearning 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 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 informationHow 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 informationAstronomy 1143 Quiz 1 Review
Astronomy 1143 Quiz 1 Review Prof. Pradhan September 7, 2017 I What is Science? 1. Explain the difference between astronomy and astrology. Astrology: nonscience using zodiac sign to predict the future/personality
More informationThe 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 informationScientific Method. Ancient Astronomy. Astronomy in Ancient Times
Scientific Method Chapter 2: The Copernican Revolution The Birth of Modern Science Ancient Astronomy Models of the Solar System Laws of Planetary Motion Newton s Laws Laws of Motion Law of Gravitation
More informationAst ch 4-5 practice Test Multiple Choice
Ast ch 4-5 practice Test Multiple Choice 1. The distance from Alexandria to Syene is about 500 miles. On the summer solstice the sun is directly overhead at noon in Syene. At Alexandria on the summer solstice,
More informationThe History of Astronomy. Please pick up your assigned transmitter.
The History of Astronomy Please pick up your assigned transmitter. When did mankind first become interested in the science of astronomy? 1. With the advent of modern computer technology (mid-20 th century)
More informationPhysics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits. Planetary Motion
Physics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits Planetary Motion Geocentric Models --Many people prior to the 1500 s viewed the! Earth and the solar system using a! geocentric
More informationObservational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws
Observational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws Craig Lage New York University - Department of Physics craig.lage@nyu.edu February 24, 2014 1 / 21 Tycho Brahe s Equatorial
More informationcosmogony 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 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 informationWednesday, 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 informationThe 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 informationClaudius Ptolemaeus Second Century AD. Jan 5 7:37 AM
Claudius Ptolemaeus Second Century AD Jan 5 7:37 AM Copernicus: The Foundation Nicholas Copernicus (Polish, 1473 1543): Proposed the first modern heliocentric model, motivated by inaccuracies of the Ptolemaic
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 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 informationCOSMIC DISTANCE LADDER
ASTC02 - PROF. HANNO REIN COSMIC DISTANCE LADDER ADAPTED FROM SLIDES BY TERENCE TAO (UCLA) HOW FAR AWAY IS COSMIC DISTANCE LADDER Work out the answer in steps (rungs) Starting with short distances ( human
More informationMonday, October 3, 2011
We do not ask for what useful purpose the birds do sing, for song is their pleasure since they were created for singing. Similarly, we ought not ask why the human mind troubles to fathom the secrets of
More informationA100 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 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 informationThe Birth of Astronomy. Lecture 3 1/24/2018
The Birth of Astronomy Lecture 3 1/24/2018 Fundamental Questions of Astronomy (life?) What is the shape of the Earth? How big is the planet we live on? Why do the stars move across the sky? Where is Earth
More informationThis 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 informationa. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU
1 AST104 Sp04: WELCOME TO EXAM 1 Multiple Choice Questions: Mark the best answer choice. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1. A galaxy
More informationTopic 10: Earth in Space Workbook Chapters 10 and 11
Topic 10: Earth in Space Workbook Chapters 10 and 11 We can imagine all the celestial objects seen from Earth the sun, stars, the Milky way, and planets as being positioned on a celestial sphere. Earth
More informationHistory of Astronomy. PHYS 1411 Introduction to Astronomy. Tycho Brahe and Exploding Stars. Tycho Brahe ( ) Chapter 4. Renaissance Period
PHYS 1411 Introduction to Astronomy History of Astronomy Chapter 4 Renaissance Period Copernicus new (and correct) explanation for retrograde motion of the planets Copernicus new (and correct) explanation
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 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 informationIntroduction 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 informationTest Bank for Life in the Universe, Third Edition Chapter 2: The Science of Life in the Universe
1. The possibility of extraterrestrial life was first considered A) after the invention of the telescope B) only during the past few decades C) many thousands of years ago during ancient times D) at the
More informationFirst 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 informationExam #1 Study Guide (Note this is not all the information you need to know for the test, these are just SOME of the main points)
Exam #1 Study Guide (Note this is not all the information you need to know for the test, these are just SOME of the main points) Moon Phases Moon is always ½ illuminated by the Sun, and the sunlit side
More informationDr. Tariq Al-Abdullah
1 Chapter 1 Charting the Heavens The Foundations of Astronomy 2 Learning Goals: 1. Our Place in Space 2. The Obvious view 3. Earth s Orbital Motion 4. The Motion of the Moon 5. The Measurement of Distance
More informationLecture 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 informationGravitation and the Motion of the Planets
Gravitation and the Motion of the Planets 1 Guiding Questions 1. How did ancient astronomers explain the motions of the planets? 2. Why did Copernicus think that the Earth and the other planets go around
More informationBROCK 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 informationPHYS 160 Astronomy Test #1 Name Answer Key Test Version A
PHYS 160 Astronomy Test #1 Name Answer Key Test Version A True False Multiple Choice 1. T 1. C 2. F 2. B 3. T 3. A 4. T 4. E 5. T 5. B 6. F 6. A 7. F 7. A 8. T 8. D 9. F 9. D 10. F 10. B 11. B 12. D Definitions
More informationChapter. Origin of Modern Astronomy
Chapter Origin of Modern Astronomy 22.1 Early Astronomy Ancient Greeks Astronomy is the science that studies the universe. It includes the observation and interpretation of celestial bodies and phenomena.
More informationChapter 1 The Copernican Revolution
Chapter 1 The Copernican Revolution The Horse Head nebula in the Orion constellation (Reading assignment: Chapter 1) Learning Outcomes How the geocentric model accounts for the retrograde motion of planets?
More informationThe cosmic distance ladder. Teacher s day, AustMS September Terence Tao (UCLA)
The cosmic distance ladder Teacher s day, AustMS06 27 September 2006 Terence Tao (UCLA) 1 Astrometry An important subfield of astronomy is astrometry, the study of positions and movements of celestial
More informationDeAnza College Winter First Midterm Exam MAKE ALL MARKS DARK AND COMPLETE.
FAMILY NAME : (Please PRINT!) GIVEN NAME : (Please PRINT!) Signature: ASTRONOMY 4 DeAnza College Winter 2018 First Midterm Exam MAKE ALL MARKS DARK AND COMPLETE. Instructions: 1. On your Parscore sheet
More informationToday FIRST HOMEWORK DUE. Ancient Astronomy. Competing Cosmologies. Geocentric vs. Heliocentric. Ptolemy vs. copernicus.
Today FIRST HOMEWORK DUE Ancient Astronomy Competing Cosmologies Geocentric vs. Heliocentric Ptolemy vs. copernicus Retrograde Motion Phases of Venus Galileo 1 3.1 The Ancient Roots of Science Our goals
More informationGravitation and the Waltz of the Planets
Gravitation and the Waltz of the Planets Chapter Four Guiding Questions 1. How did ancient astronomers explain the motions of the planets? 2. Why did Copernicus think that the Earth and the other planets
More informationGravitation and the Waltz of the Planets. Chapter Four
Gravitation and the Waltz of the Planets Chapter Four Guiding Questions 1. How did ancient astronomers explain the motions of the planets? 2. Why did Copernicus think that the Earth and the other planets
More informationAST 248, Lecture 2. James Lattimer. Department of Physics & Astronomy 449 ESS Bldg. Stony Brook University. January 28, 2015
AST 248, Lecture 2 James Lattimer Department of Physics & Astronomy 449 ESS Bldg. Stony Brook University January 28, 2015 The Search for Life in the Universe james.lattimer@stonybrook.edu Distances in
More informationAstronomy 291. Professor Bradley M. Peterson
Astronomy 291 Professor Bradley M. Peterson The Sky As a first step, we need to understand the appearance of the sky. Important points (to be explained): The relative positions of stars remain the same
More informationEvidence 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 informationA100 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 informationExam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are
Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are concept questions, some involve working with equations,
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 information9/12/2010. 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 informationThe 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 informationHow High Is the Sky? Bob Rutledge
How High Is the Sky? Bob Rutledge Homer s Physics: Feb 16 2007 The Sun 8 Light Minutes Away 2 The Pleiades 300 Light Years Away (and inside our galaxy) [The nearest star, Proxima Cen, is only 4.2 light
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 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 informationN = R * f p n e f l f i f c L
This Class (Lecture 32): Cultural Evolution Next Class: Lifetime ET: Astronomy 230 HW 7 due today! Outline Will a civilization develop that has the appropriate technology and worldview? The most important
More informationMost 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 informationAstr 1050 Mon. Jan. 31, 2017
Astr 1050 Mon. Jan. 31, 2017 Finish Ch. 2: Eclipses & Planetary Motion Seasons Angular Size formula Eclipses Planetary Motion Reading: For Today: Finish Chapter 2 For Monday: Start Chapter 3 Homework on
More information2.4 The Birth of Modern Astronomy
2.4 The Birth of Modern Astronomy Telescope invented around 1600 Galileo built his own, made observations: Moon has mountains and valleys Sun has sunspots, and rotates Jupiter has moons (shown): Venus
More informationEarly 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 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 information