The Solar System What’S in Our Solar System?

Total Page:16

File Type:pdf, Size:1020Kb

The Solar System What’S in Our Solar System? The Solar System What’s in Our Solar System? • Our Solar System consists of a central star (the Sun), the eight planets orbiting the sun, several dwarf planets, moons, asteroids, comets, meteors, interplanetary gas, dust, and all the “space” in between them. • Solar System: a star (sun) together with all the objects revolving around it (planets and their moons, asteroids, comets, and so on). What’s in Our Solar System? • The word solar comes from the Latin solaris, meaning “of the sun.” Sol is the Latin word for “sun.” • The eight planets of the Solar System are named for Greek and Roman Gods and Goddesses. Planetary System Planetary System: a planet with its moon(s), • The Earth and moon are a planetary system. • The word planet comes from a Greek word meaning “wandering.” To the ancients, the five visible planets to the naked eye appeared to move, unlike the other fixed stars that were “fixed.” • Orbit: the path followed by a planet, asteroid, or comet around a star, or a moon around a planet. The word comes from the Latin orbita, meaning a “wheel track.” Planets, Dwarf Planets, Moons, Asteroids, and Comets • Planet: a large body, spherical because of its own gravity, orbiting a star and not sharing its orbit with any other large bodies. • Dwarf Planet: a planet-like body that orbits the sun and does not clear its orbital zone of other massive bodies, and is not a moon. • Moon: object revolving around a planet. The word moon is from an ancient German root meaning “moon” or “month.” Planets, Dwarf Planets, Moons, Asteroids, and Comets • Asteroid: a rocky or metallic object a few feet or a few miles in dimeter. It may orbit alone or be in a belt of many other asteroids. The word asteroid comes from the Greek aster (“star”) and -oid (“-like”). They have no atmosphere or water. • Meteor: small rocky or metallic object heated to incandescent vapor as it falls or streaks into Earth’s atmosphere. Those streaks are called “shooting stars.” – Meteoroid: meteor in space – Meteorite: meteor that survived its passage through the atmosphere and strikes the ground. The Greek root for rock is “-ite.” • Comet: icy object that, when passing close enough to its star, displays a tail of evaporated material. The word comet comes from the Latin stella cometa, meaning “long-haired star”, referring to the tail. Composition and Structure of the Solar System The Solar System consists of: • The sun • Eight planets, including Earth • At least five dwarf planets, including Pluto • Over 100 moons • Large numbers of asteroids and comets Geocentric = Earth Centered (Aristotle, Ptolemy) Heliocentric = Sun Centered (Copernicus, Galileo) *Copernicus was the first astronomer to accurately describe out solar system. Composition and Structure of the Solar System • The sun is the largest object in our solar system. It’s the center of our solar system, and all other objects in our solar system revolve around it. • The cause of this arrangement is gravity. Gravity is a property of space and time that causes both weight and orbits. The word gravity comes from the Latin gravitas, meaning “weight” or “heaviness.” Because of gravity, small objects either drops onto larger, heavier objects or orbit around them. Composition and Structure of the Solar System The 8 Planets in order from -Most of the asteroids in our solar the sun outward: system are in two belts. • Mercury -Asteroid Belt: lies between the • Venus orbits of Mars & Jupiter. • Earth • Mars -Kuiper Belt: collection of icy objects that orbit beyond Neptune. • Jupiter • Saturn -Oort Cloud: a huge zone of icy • Uranus objects lying far beyond the Kuiper Belt. When something disturbs one • Neptune of these objects, it fall in toward the sun in elongated orbit and becomes a comet. Most of the comets in our solar system originate in the Oort Cloud. Motions of the Planets • Revolution: the planets all revolve around the sun in a single plane, like a disc. • Rotation: Each planet rotates on its axis. The axis is an imaginary rod running through the center of the planet and each of the geographic poles. – Axis is a Latin word meaning “axle.” – The axes of the planets are tilted varying amounts to the common plane of revolution. – Earth’s axis is tilted about 23.5° - this is what causes the seasons. Inner and Outer Planets • Inner Planets: • Outer Planets – Mercury – Jupiter – Venus – Saturn – Earth – Uranus – Mars – Neptune – Pluto The Relative Size of the Planets in the Solar System The Scale of the Solar System The illustration on the previous slide is not true to scale. In fact, it is wildly out of scale. To understand the true scale of the solar system, imagine the Earth is the size of your classroom globe, THEN: -The sun, at the center of the solar system, is a sphere 14 stories tall. -Mercury is a grapefruit and 1.25 miles from the sun. -Venus is a beach ball and 2.25 miles from the sun. -Earth, the size of a globe, is 3 miles from the sun. *The moon is a baseball and 40 feet from Earth. -Mars is a dodgeball and 4.5 miles from the sun. -Jupiter is as wide as five vans and 15.5 miles from the sun. -Saturn is as tall as a basketball hoop and 29 miles from the sun. -Uranus is as tall as the average male 8th grader (5’4) and 57 miles from the sun. -Neptune is as tall as the average male 6th grader and 90 miles from the sun. *Light takes 8 minutes to reach Earth, and 4 hours to reach Neptune. It takes light less than 3 seconds to travel from the Earth to the moon and back. The 8 Planets of the Solar System • Planets are categorized according to composition and size. There are two main categories of planets: – small Rocky Planets (Mercury, Venus, Earth, and Mars): rocky planets also known as “terrestrial planets” meaning earth-like. Terra is Latin for “earth.” These planets are composed mainly of rocks and metals. When the solar system was forming the heavier elements tended to collect closer to the sun. Venus, Earth, and Mars have atmospheres composed of gases. Earth is unique because it has a large amount of water. Rocky planets, being heavy, rotate more slowly. – Gas Giants (Jupiter, Saturn, Uranus, and Neptune): composed mostly of hydrogen and helium. Uranus and Neptune are sometimes called “ice giants,” because they contain ices of water, ammonia, and methane. Each of the gas planets has a small solid core. Being lighter, they rotate faster, this casues high winds andhuge storms. The gas planets have rings and multiple moons. The Sun • Diameter: 865,000 miles (109 times greater that Earth) • Distance from Earth: 93 Million Miles – This is know as 1AU (astronomical unit) and is used to measure interplanetary and interstellar distances. • Rotation: rotates on its axis in about 25 earth days. • Characteristics: – The sun is a fairly ordinary main sequence star. – Its very bright – 85% brighter than other stars in our galaxy – Its white in color, however it looks yellow because of our atmosphere. – Surface Temp: 10,000°F – Core Temp: 27 Million °F • A star’s temperature determines its “color.” The coldest stars are red. The hottest stars are blue. • Composition: 75% Hydrogen & 25% Helium The Sun • Other Facts: – The solar system is in a spiral arm of the Milky Way Galaxy. – The sun is located about 25,000 ly from the galactic center. – It orbits the galaxy in about 230 million years – The sun burns hydrogen in a process called nuclear fusion, in which hydrogen is converted to heat and light. Remember stars produce light. Planets reflect light. – The sun has a huge magnetic field that produces sunspots, solar flares, and the northern lights. – The sun contains 99.8% of all mass in our solar system. • Mythology: – The sun was worshipped as a god, often the principal god in most ancient societies. – The Romans celebrated the sun’s birthday as Sol Invictus (“unconquered sun”) about the same time as our Christmas. – Scientific observation began with ancient Hindus, Babylonians, and Greeks. Characteristics of Small Rocky Planets • They are made up mostly of rock and metal. • They are very heavy. • They move slowly in space. • They have no rings and few moons (if any). • They have a diameter of less than 13,000 km (8,077 miles). Mercury Diameter: 3,000 miles (3/8 size of Earth) – Smallest planet in the solar system – Smaller that the moons Ganymede and Titan Distance from Sun: 3 Million Miles (0.39 AU) Rotation: The period of rotation (one Mercury day) is 58.6 earth days. Orbit: the orbital period (one Mercury year) is ¼ earth year (88 earth days) Composition: Mercury is 70% metallic and 30% rocky material, with a dense iron core. Mercury Characterisitcs: • The surface temperature varies from -300°F (Nighttime) to 800°F (Daytime). • Mercury is the most heavily cratered body in the solar system. • Caloris Basin, on of the largest impact craters in the solar system, is 960 miles in diameter. Caloris is the Latin word for “heat.” • Mercury’s axis has 0° of tilt. Polar craters are in constant shadow and contain ice. • Mercury has no moons, no rings, no atmosphere, and a small magnetic field. Mythology and Observation • The Greeks and Romans named the planet after their swift-footed messenger god, Hermes/Mercury, because of its fast paced across the sky. • Mercury has been visited by the space probes Mariner 10 in 1974, and Mesenger in 2008 Venus • Diameter: 7,500 miles – Only slightly smaller that Earth; Venus is sometimes called “Earth’s sister.” • Distance from Sun: 67 Million miles (0.72 AU) • Rotation: Venus rotates once every 243 earth days, by far the slowest of the planets.
Recommended publications
  • Crater Copernicus John Paladini Took This Image of Crater Copernicus with His Home-Built 6" F/8 Refractor (10 Frames a Second Neximager Stack of About 100)
    WESTCHESTER AMATEUR ASTRONOMERS MAY 2010 Sky tch Crater Copernicus John Paladini took this image of crater Copernicus with his home-built 6" f/8 refractor (10 frames a second neximager stack of about 100). An impact crater, Copernicus is thought to be about 800 million years old. The crater is 93 km in diameter and about 3700m deep. The crater’s central peaks are visible in the above photo. They rise about 1200m above the crater’s floor. SERVING THE ASTRONOMY COMMUNITY SINCE 1983 Page 1 WESTCHESTER AMATEUR ASTRONOMERS MAY 2010 Events for May 2010 WAA Lectures the public. The scheduled rain/cloud date is May 15th. “No Place for the Timid: Participants and quests should read our General The Engineering Saves of NASA": Observing Guidelines. Friday May 7th, 8:00pm Miller Lecture Hall, Pace University Renewing Members. Pleasantville, NY Bill Forsyth - Hartsdale Alan Witzgall will be giving a behind the scenes look Donna Cincotta - Yonkers at NASA, featuring the engineering saves and Arumugam Manoharan - Yonkers technical support which make space flight possible. James Peale - Bronxville Alan is a well-known astronomy lecturer and science Paul Alimena - Rye writer; he is active in many metropolitan area astronomy organizations. Free and open to the public. Call: 1-877-456-5778 (toll free) for announcements, weather cancellations, or Upcoming Lectures questions. Also, don’t forget to periodically visit the June's lecture will be a teleconference featuring the WAA website at: senior astronomer from the SETI institute, Dr. Seth http://www.westchesterastronomers.org/. Shostak. It will take place at 7:00 pm on Thursday June 10th.
    [Show full text]
  • Apollonius of Rhodes Argonautica Book 3, Translated by Robert Cooper Seaton, Harvard University Press, Cambridge MA, 1912
    Apollonius of Rhodes Argonautica book 3, translated by Robert Cooper Seaton, Harvard University Press, Cambridge MA, 1912. (http://oaks.nvg.org/sa4ra16.html#tres) Come Now, Erato, stand by my side, and say next how Jason brought back the fleece to Iolcus aided by the love of Medea. For you share the power of Cypris, and by your love-cares charm unwedded maidens; wherefore to you too is attached a name that tells of love. Thus the heroes, unobserved, were waiting in ambush amid the thick reed-beds; but Hera and Athena took note of them, and, apart from Zeus and the other immortals, entered a chamber and took counsel together; and Hera first made trial of Athena: "Do you now first, daughter of Zeus, give advice. What must be done? Will you devise some scheme whereby they may seize the golden fleece of Aeetes and bear it to Hellas, or can they deceive the king with soft words and so work persuasion? Of a truth he is terribly overweening. Still it is right to shrink from no endeavour." Thus she spoke, and at once Athena addressed her: "I too was pondering such thoughts in my heart, Hera, when you did ask me outright. But not yet do I think that I have conceived a scheme to aid the courage of the heroes, though I have balanced many plans." She ended, and the goddesses fixed their eyes on the ground at their feet, brooding apart; and straightway Hera was the first to speak her thought: "Come, let us go to Cypris; let both of us accost her and urge her to bid her son (if only he will obey) speed his shaft at the daughter of Aeetes, the enchantress, and charm her with love for Jason.
    [Show full text]
  • Planets of the Solar System Information
    Planets of the Solar System Mercury Mercury is the smallest planet and the closest to the Sun. It travels very fast at a speed of 180 000 km/h in an elliptical orbit around the Sun. One orbit takes just 88 days. Mercury has the most eccentric orbit of all the planets, therefore its nearness to the Sun is variable. It can be as close as 47 million km and as far as 70 million km away, but is at an average distance of 57 910 000 km away from the Sun. With a diameter of 4 800km, Mercury is about 38% of the size of the Earth. Even though it is revolving very quickly around the sun it is rotating very slowly on its axis. One day on Mercury takes 59 Earth days. In the time it takes to complete two orbits Mercury only rotates three times! Average temperatures on Mercury reach 427°C Where did Mercury get its name? during the day and -173°C during the night. Mercury has no atmosphere to trap and store heat Mercury is named after the mythical Roman so it is very cold on the side of the planet that is Messenger of the Gods. He is often depicted facing away from the Sun. in art wearing winged sandles and a winged helmet. He was known for his speed. Venus Venus is the second closest planet at approximately 108 200 000 km away from the Sun. It is often referred to as our ‘sister planet’ because it has some similarities with Earth: It has a rocky surface dominated by volcanoes.
    [Show full text]
  • ASTRONAUTICS and AERONAUTICS, 1977 a Chronology
    NASA SP--4022 ASTRONAUTICS AND AERONAUTICS, 1977 A Chronology Eleanor H. Ritchie ' The NASA History Series Scientific and Technical Information Branch 1986 National Aeronautics and Space Administration Washington, DC Four spacecraft launched by NASA in 1977: left to right, top, ESA’s Geos 1 and NASA’s Heao 1; bottom, ESA’s Isee 2 on NASA’s Isee 1, and Italy’s Wo. (NASA 77-H-157,77-H-56, 77-H-642, 77-H-484) Contents Preface ...................................................... v January ..................................................... 1 February .................................................... 21 March ...................................................... 47 April ....................................................... 61 May ........................................................ 77 June ...................................................... 101 July ....................................................... 127 August .................................................... 143 September ................................................. 165 October ................................................... 185 November ................................................. 201 December .................................................. 217 Appendixes A . Satellites, Space Probes, and Manned Space Flights, 1977 .......237 B .Major NASA Launches, 1977 ............................... 261 C. Manned Space Flights, 1977 ................................ 265 D . NASA Sounding Rocket Launches, 1977 ..................... 267 E . Abbreviations of References
    [Show full text]
  • Apollonius Rhodius, the Argonautica
    i EB CLASSICA BRAR 1 1 APOLLONIUS RHODIUS ARGONAUTICA Translated by R. C. SEATON mmmmm]mmm\m[mmmm[^[r^\[f^\[r^\i7^\[?^\[?D\[fD\\o] Complete list of Loeb titles can be found at the end of each volume APOLLONIUS Of Rhodes' was a Greek grammarian and epic poet of Alexandria in Egypt and lived late in the 3rd century and early in the 2nd century [ES B.C. While still young he composed his extant epic poem of four books on the story of the Argonauts. When this work failed to win acceptance he went to Rhodes where he not only did well as a rhetorician but also made a success of his epic in a revised form, for which the Rhodians gave him the 'freedom' of their city; hence his surname. On returning to Alexandria he recited his poem again, with applause. In 196 Ptolemy Epiphanes made him the librarian of the Museum (the University) at Alexandria. His Argonautica is one oi the better minor epics, remarkable for originality, powers of observation, sincere feeling, and de- piction of romantic love. His Jason and Medea are natural and interesting, and did much to inspire Virgil (in a very different setting) in the fourth book of the Aeneid. L• ^' % Sb ^" ^ Ak- THE LOEB CLASSICAL LIBRARY EDITED BY li. CAPPS, Ph.D., LL.D. T. E. PAGE, Litt.D. W. II. D. ROUSE, Lirr.D. APOLLONTUS RHODIUS Digitized by tine Internet Arciiive in 2011 witii funding from University of Toronto littp://www.arcliive.org/details/apolloniusrliodiuOOapol APOLLONIUS RHODIUS THE ARGONAUTICA WITH AN ENGLISH TRANSLATION BY 11.
    [Show full text]
  • Scientific Goals for Exploration of the Outer Solar System
    Scientific Goals for Exploration of the Outer Solar System Explore Outer Planet Systems and Ocean Worlds OPAG Report v. 28 August 2019 This is a living document and new revisions will be posted with the appropriate date stamp. Outline August 2019 Letter of Response to Dr. Glaze Request for Pre Decadal Big Questions............i, ii EXECUTIVE SUMMARY ......................................................................................................... 3 1.0 INTRODUCTION ................................................................................................................ 4 1.1 The Outer Solar System in Vision and Voyages ................................................................ 5 1.2 New Emphasis since the Decadal Survey: Exploring Ocean Worlds .................................. 8 2.0 GIANT PLANETS ............................................................................................................... 9 2.1 Jupiter and Saturn ........................................................................................................... 11 2.2 Uranus and Neptune ……………………………………………………………………… 15 3.0 GIANT PLANET MAGNETOSPHERES ........................................................................... 18 4.0 GIANT PLANET RING SYSTEMS ................................................................................... 22 5.0 GIANT PLANETS’ MOONS ............................................................................................. 25 5.1 Pristine/Primitive (Less Evolved?) Satellites’ Objectives ...............................................
    [Show full text]
  • Astronomy Handbook
    ASTRONOMY HANDBOOK 63 Table of Contents Section 1 – The Night Sky Purple Section 2 – The North Polar Sky Green Secton 3 – The Winter Sky Pink Section 4 – The Spring Sky Yellow Section 5 – The Summer Sky Blue Section 6 – The Autumn Sky Orange Section 7 – Other Information Red 64 Section 1 – The Night Sky Table of Contents Page Subject Myths & Legends included? 2 Teaching Astronomy - 4 A Little History - 6 The Universe & Milky Way Estonian 9 The Stars & Our Sun Greek, Native American, Scandinavian 16 The Planets Greek, Native American 25 The Moon Native American, Chinese 36 Asteroids, Comets, Meteoroids Native American 39 Greek & Roman Gods - 40 Constellations: An Intro Native American 65 Teaching Astronomy Most schools that come to TOS like to take astronomy. It’s a great opportunity for the kids to sit quietly, look at stars and planets that they may not be able to see in a town or city, and listen to myths and legends about the night sky. This information offers a good foundation to astronomy. Please read it and absorb as much as you can before you arrive. During training we will concentrate on learning constellations and the stories associated with them. Astronomy lasts an hour-and-a-half. We will usually start off with a few games (which we will also show you during training) to burn off some of the kids’ energy, and to wait for it to get dark. Once the stars come out, you will gather your team and find somewhere around camp to look at the night sky.
    [Show full text]
  • Bulfinch's Mythology
    Bulfinch's Mythology Thomas Bulfinch Bulfinch's Mythology Table of Contents Bulfinch's Mythology..........................................................................................................................................1 Thomas Bulfinch......................................................................................................................................1 PUBLISHERS' PREFACE......................................................................................................................3 AUTHOR'S PREFACE...........................................................................................................................4 STORIES OF GODS AND HEROES..................................................................................................................7 CHAPTER I. INTRODUCTION.............................................................................................................7 CHAPTER II. PROMETHEUS AND PANDORA...............................................................................13 CHAPTER III. APOLLO AND DAPHNEPYRAMUS AND THISBE CEPHALUS AND PROCRIS7 CHAPTER IV. JUNO AND HER RIVALS, IO AND CALLISTODIANA AND ACTAEONLATONA2 AND THE RUSTICS CHAPTER V. PHAETON.....................................................................................................................27 CHAPTER VI. MIDASBAUCIS AND PHILEMON........................................................................31 CHAPTER VII. PROSERPINEGLAUCUS AND SCYLLA............................................................34
    [Show full text]
  • Planet Watch Constellation Watch the Night Sky Above
    THE NIGHT SKY ABOVE YORK FOR MARCH & APRIL 2014 �is chart is oriented for 9pm March 17th, 8pm March 31st, 7pm April 14th, but can be used at any time. To use the chart, hold it up to the sky. Turn the chart so that the direction you are looking is at the bottom of the chart. If you are looking to the south then have the ‘South Horizon’ at the bottom edge. As the Earth turns the stars appear to rotate anti-clockwise around the North Celestial Pole, marked by the star Polaris. Stars rise in the east and set in the west just like the Sun. �e sky makes a small westward shift every night as we orbit the Sun. be seen to be distinctly different colours. PLANET WATCH Rigel is a hot blue supergiant star and Jupiter is the brightest object (besides the Betelgeuse is a huge cool red giant, 8 times moon) in the evening sky in March and April. larger than Rigel. Although they appear to be It is the largest planet in the Solar System. the same brightness, Rigel is further away With a small telescope you can see the (772 light years compared to 644 light years), four Galilean moons of Jupiter. Io, Europa, meaning it is naturally brighter. �e sword Ganymede and Callisto were discovered by of Orion can be seen as three stars hanging Galileo when used his telescope to look at diagonally down from his belt. �e second the night sky. �ey are some interesting star down is not a star at all! It is a large places too.
    [Show full text]
  • Divine Riddles: a Sourcebook for Greek and Roman Mythology March, 2014
    Divine Riddles: A Sourcebook for Greek and Roman Mythology March, 2014 E. Edward Garvin, Editor What follows is a collection of excerpts from Greek literary sources in translation. The intent is to give students an overview of Greek mythology as expressed by the Greeks themselves. But any such collection is inherently flawed: the process of selection and abridgement produces a falsehood because both the narrative and meta-narrative are destroyed when the continuity of the composition is interrupted. Nevertheless, this seems the most expedient way to expose students to a wide range of primary source information. I have tried to keep my voice out of it as much as possible and will intervene as editor (in this Times New Roman font) only to give background or exegesis to the text. All of the texts in Goudy Old Style are excerpts from Greek or Latin texts (primary sources) that have been translated into English. Ancient Texts In the field of Classics, we refer to texts by Author, name of the book, book number, chapter number and line number.1 Every text, regardless of language, uses the same numbering system. Homer’s Iliad, for example, is divided into 24 books and the lines in each book are numbered. Hesiod’s Theogony is much shorter so no book divisions are necessary but the lines are numbered. Below is an example from Homer’s Iliad, Book One, showing the English translation on the left and the Greek original on the right. When citing this text we might say that Achilles is first mentioned by Homer in Iliad 1.7 (i.7 is also acceptable).
    [Show full text]
  • The Age of Chivalry
    1 A free download from http://manybooks.net The Age of Chivalry CHAPTER I<p> CHAPTER I CHAPTER II<p> CHAPTER II CHAPTER III<p> CHAPTER III CHAPTER IV<p> CHAPTER IV CHAPTER V<p> CHAPTER V CHAPTER VI<p> CHAPTER VI CHAPTER VII<p> CHAPTER VII CHAPTER VIII<p> CHAPTER VIII CHAPTER IX<p> CHAPTER IX CHAPTER X<p> CHAPTER X CHAPTER XI<p> CHAPTER XI CHAPTER XII<p> CHAPTER XII CHAPTER XIII<p> CHAPTER XIII CHAPTER XIV<p> CHAPTER XIV The Age of Chivalry 2 CHAPTER XV<p> CHAPTER XV CHAPTER XVI<p> CHAPTER XVI CHAPTER XVII<p> CHAPTER XVII CHAPTER XVIII<p> CHAPTER XVIII CHAPTER XIX<p> CHAPTER XIX CHAPTER XX<p> CHAPTER XX CHAPTER XXI<p> CHAPTER XXI CHAPTER XXII<p> CHAPTER XXII CHAPTER XXIII<p> CHAPTER XXIII CHAPTER I<p> CHAPTER I CHAPTER II<p> CHAPTER II CHAPTER III<p> CHAPTER III CHAPTER IV<p> CHAPTER IV CHAPTER V<p> CHAPTER V CHAPTER VI<p> CHAPTER VI CHAPTER VII<p> CHAPTER VII CHAPTER VIII<p> CHAPTER VIII CHAPTER IX<p> CHAPTER IX CHAPTER X<p> CHAPTER X CHAPTER XI<p> CHAPTER XI CHAPTER XII<p> CHAPTER XII CHAPTER XIII<p> CHAPTER XIII Information about Project Gutenberg The Legal Small Print The Age of Chivalry The Project Gutenberg EBook of The Age of Chivalry, by Thomas Bulfinch (#2 in our series by Thomas The Age of Chivalry 3 Bulfinch) Copyright laws are changing all over the world. Be sure to check the copyright laws for your country before downloading or redistributing this or any other Project Gutenberg eBook.
    [Show full text]
  • Apollodorus : the Library
    JU\r(^ Qksl 7^ani-hSin THE LOEB CLASSICAL LIBRARY EDITED BY E. CAPPS, Ph.D., LL.D. T. E. PAGE, Litt.D. W. H. D. ROUSE, Litt.D. APOLLODORUS THE LIBRARY I APOLLODOEUS THE LIBRARY WITH AN ENGLISH TRANSLATION BY SIR JAMES GEORGE FRAZER, F.B.A., F.R.S. FELLOW OF TRINITY COLLEGE, CAMBRIDGE IN TWO VOLUMES I LONDON : WILLIAM HEINEMANN NEW YORK : G. P. PUTNAM'S SONS MCMXXI FEB " 3 !940 TO MY OLD TEACHER AND FRIEND HENRY JACKSON, O.M. CONTENTS PAGK INTRODUCTION ix SUMMARY xlv SYMBOLS EMPLOYED IN THE CRITICAL NOTES llX 1 BOOK I • 127 BOOK II 295 BOOK Til Vll ERRATA. , Vol. , 73 For " Thestius " read " Agrius." Vol. II. P. 54. For "later version" read "earlier version." — INTRODUCTION I. The Author and His Book. Nothing is positively known, and little can be conjectured with any degree of probability, con- cerning the author of the Library. Writing in the ninth century of our era the patriarch Photius calls him Apollodorus the Gi'ammarian,^ and in the manu- scripts of his book he is described as Apollodorus the Athenian, Grammarian. Hence we may con- clude that Photius and the copyists identified our author with the eminent Athenian grammarian of that name, who flourished about 140 b.c. and wrote a number of learned works, now lost, including an elaborate treatise On the Gods in twenty-four books, and a poetical, or at all events versified. Chronicle in four books. 2 But in modern times good reasons have been given for rejecting this identification,^ ^ Photius, Bibliotheca, p.
    [Show full text]