3-D Constellations Activity F7 Grade Level: 4–12

Total Page:16

File Type:pdf, Size:1020Kb

3-D Constellations Activity F7 Grade Level: 4–12 Star Finding and Constellations • F7 3-D Constellations Activity F7 Grade Level: 4–12 Source: Adapted with permission from the activity “Building Three-Dimensional Models of the Constellations” in Project STAR: The Universe in Your Hands, © 1993, 2001 by the President and Fellows of Harvard College, published by Kendall/Hunt Publishing, Dubuque, IA. Adapted by Anna Hurst for the Astronomy from the Ground Up project at the Astronomical Society of the Pacific. Updated 2010 by Andrew Fraknoi. This version was produced in 2010 by the Astronomical Society of the Pacific.http:// www.astrosociety.org What’s This Activity About? Tips and Suggestions Because the stars in the best known star patterns, such • The table in this activity already calculates the conver- as the constellation figure of Orion the hunter, and the sion of the distances in light years to the length of the asterism of the Big Dipper, look (after much association string needed (in centimeters and inches). Older stu- in our minds) like they belong together, many students dents who need math practice can do this conversion actually believe that the stars in these sky figures are as- on their own. sociated. Yet most stars in a bright constellation pattern • Note that some of the stars in the Big Dipper turn out are at quite different distances from us and only happen to be at about the same distance from us, since they to lie in the same part of our sky. This activity helps stu- are part of a moving group of stars that were probably dents realize that the sky is a three-dimensional place born together. This collection of stars is called the Ursa and things that look like they are together on the “dome Major Moving Group and its central part is about 80 of the sky” can actually be far apart. light years away. Thus, if you are trying to make the point that most stars in a constellation are NOT re- What Will Students Do? lated, it’s probably best to start by doing Orion. Later, Students use string and everyday materials, as well as let the students think about why the distances of five a photograph of the star patterns of Orion and the Big (or six, if you count Mizar and Alcor separately) of the Dipper to make a 3-D model, using the distances given stars in the Dipper are at roughly the same distance. in the activity. • Since the materials for making these models are easy to lose, it’s probably best to buy more than the students will need. What Will Students Learn? Concepts Inquiry Skills Big Ideas • Constellations • Ordering • Patterns of change • 3-D nature of the sky • Measuring • Modeling and simulations • Visualizing • Scale • Modeling The Universe at Your Fingertips • Astronomical Society of the Pacific Page 1 Star Finding and Constellations F7• 3-D Constellations Meissa 3-D Constellations 1050 LY Betelgeuse Bellatrix 640 LY 240 LY Mintaka 915 LY Alnitak Alnilam 800 LY 1340 LY Orion Nebula Rigel 800 LY Saiph 700 LY Type of Activity: Indoor classroom or drop-in See the list of sources for materials on page 4. station, facilitated Setting Up the Activity Set up Time: 30–45 minutes This works best with participants sitting at tables. You Time to Do: 30 minutes will need to pre-cut the lengths of thread and the pieces Audience age: 8 years and older of cardboard. Set out one piece of cardboard, a constel- Group size: various lation photograph, a constellation chart, a pen or needle, the appropriate number of threads and pony beads, and What’s This Activity About? a ruler for each participant, as well as tape for the table The stars appear to be painted on the dome of the sky to share. above our heads. Those that make up the Big Dipper, Suggestions for Introducing the Activity Orion and other well-known star patterns appear close to If possible, look at Orion and the Big Dipper, if not in the each other in space — but are they really close together? real sky, then in a planetarium or on a photograph. The This activity demonstrates that the pattern we see in the stars in Orion make a clear figure of a hunter. Do you sky is just an accident of our place in space. The stars in a think all the bright stars are at the same distance? The constellation can actually be quite distant from each oth- stars in the Big Dipper appear almost equally bright to us. er, so that the same constellation would thus look much Do you think all the stars that you see in the Big Dipper different from a different part of the Galaxy. are almost the same distance from Earth? Imagine you Materials could observe the Big Dipper from a planet orbiting the For each constellation model: star at the end of the Big Dipper’s handle. Do you think the Big Dipper would look the same from that planet as • Copies of constellation photographs it does when you observe the Dipper from Earth? • Copies of constellation charts (see pages 5–6) Doing the Activity • Meter stick 1. Participants should carefully tape the constellation • Thick sewing needle or ballpoint pen (with long, ex- photograph to the piece of cardboard. posed writing point) 2. They then place a bead on each string by first pass- • Steel washer ing the thread through it, then around and through it • Piece of corrugated cardboard about 30 cm x 30 cm again. By stringing the bead this way, they will be able (1 ft. x 1 ft.) to slide the bead along the length of the string, but it will stay in place when they let go. • Pony beads (number equal to number of stars in con- stellation) 3. Using the needle or pen, participants should punch holes through the photo and the cardboard at the posi- • 1-meter long pieces of black button thread (number of tion of each star which has a distance written next to it pieces equal to number of stars in constellation) on the corresponding chart. They then slide a piece of • Tape thread through each hole, leaving about 1 inch at the The Universe at Your Fingertips • Astronomical Society of the Pacific Page 2 Star Finding and Constellations F7• 3-D Constellations back and5. the The rest distance at the front. to the (The stars front on the is thephotos side iswith indicated Earth. on the Use constellation a scale of 2.5 charts cm =on 100 pages LY. For7 example, if a and 8. A star labeled “75 l.y.” is 75 light years from the Earth. A light year is the distance the constellationlight photo.)travel in Tape one year,the one-inch about 10^13 length km. of star is 100 LY away, slide the bead representing that star thread to the back of the cardboard to hold it in place. to 2.5 cm (1 inch) from the washer. If you have a star To cover 6.up To this make messy a three-dimensionalside, you can tape themodel constella of the- constellation,that is 830 participants LY away, slide must that slide bead the out beads 21 cm (8.3 inch- tion chart overalong it. the string until they are the correct scale distancees) away. from See the Earth. table Use on apage scale 4 forof 2.5the scaledcm distances = 100 l.y. For example, if a star is 100 l.y. away, slide the bead representing that star to 4. Participants should then bring together the ends of all to the stars in Orion and the Big Dipper. (Older stu- 2.5 cm (1 inch) from the washer. If you have a stardents that can is 830do the l.y. conversion away, slide calculations that bead themselves.) the strings onout the 21 front cm (8.3side inches)and tie away.them intoSee thea tight table on page 4 for the scaled distances to the stars Participants can use the rulers to position their beads at knot around ina steelOrion washer and the about Big Dipper.56 cm (22 Participants in) from can use the rulers to position their beads at their the sheet of approximatecardboard. Have scaled them distances. cut off the extra their approximate scaled distances. thread. This thread length is used because the camera 7. When the beads are positioned, participants should 7. When the beads are positioned, participants should hold the washer with one hand and the that took the pictures of these constellations had a focal hold the washer with one hand and the photo upright photo upright with the other hand. They then stretch the strings and hold the washer next length of 56 cm.to an If eye.you holdLooking the pictureat the photo at a distance through of the washer,with theythe othershould hand. be able They to seethen the stretch beads the strings and 56 cm from youroutlining eyes, the shapeconstellation of the constellation. will appear the This mayhold work the better washer in pairs,next to with an oneeye. partner Looking at the pho- same size as itholding does in up the the sky. cardboard so that it is easier for theto throughother partner the washer, to view they the constellation.should be able to see the 5. The distanceAs to mentionedthe stars on above, the photos the scale is indicated of the photo on is suchbeads that outlining if you hold the the shape cardboard of the 56 constellation. cm This the constellationfrom charts your oneye, pages your 5 view and 6.of A the star constellation labeled is maythe same work asbetter you inwould pairs, have with at one night partner holding up looking at the constellation with your naked eye.
Recommended publications
  • The Dunhuang Chinese Sky: a Comprehensive Study of the Oldest Known Star Atlas
    25/02/09JAHH/v4 1 THE DUNHUANG CHINESE SKY: A COMPREHENSIVE STUDY OF THE OLDEST KNOWN STAR ATLAS JEAN-MARC BONNET-BIDAUD Commissariat à l’Energie Atomique ,Centre de Saclay, F-91191 Gif-sur-Yvette, France E-mail: [email protected] FRANÇOISE PRADERIE Observatoire de Paris, 61 Avenue de l’Observatoire, F- 75014 Paris, France E-mail: [email protected] and SUSAN WHITFIELD The British Library, 96 Euston Road, London NW1 2DB, UK E-mail: [email protected] Abstract: This paper presents an analysis of the star atlas included in the medieval Chinese manuscript (Or.8210/S.3326), discovered in 1907 by the archaeologist Aurel Stein at the Silk Road town of Dunhuang and now held in the British Library. Although partially studied by a few Chinese scholars, it has never been fully displayed and discussed in the Western world. This set of sky maps (12 hour angle maps in quasi-cylindrical projection and a circumpolar map in azimuthal projection), displaying the full sky visible from the Northern hemisphere, is up to now the oldest complete preserved star atlas from any civilisation. It is also the first known pictorial representation of the quasi-totality of the Chinese constellations. This paper describes the history of the physical object – a roll of thin paper drawn with ink. We analyse the stellar content of each map (1339 stars, 257 asterisms) and the texts associated with the maps. We establish the precision with which the maps are drawn (1.5 to 4° for the brightest stars) and examine the type of projections used.
    [Show full text]
  • Constellation Creation
    Constellation Creation Constellations are fun to identify in the night sky, have helped humans navigate and chart the seasons for thousands of years, are the stuff of great legends and myths, but what can these patterns really tell us about stars? Students create constellation models as a team to find out. Grades Next Generation Science Standards • 5-8 • ESS1.A: The Universe and its Stars. The sun is a star that appears larger and brighter than other stars because it is closer. Stars range greatly in their distance from Earth. Time • 5-ESS1-1. Support an argument that differences in the apparent brightness of the sun • Prep 15 min compared to other stars is due to their relative distances from Earth. • 30 min activity plus pre-activity • MS-ESS1-3– Analyze and interpret data to determine scale properties of objects in the solar class time system. discussion Materials Utah Science 7 copies of Orion and Big Dipper sheet in color, cut in half Standards 12 blue stars, 1 Betelgeuse, 1 Mizar prints in color • 6.1.3 Use computational thinking to analyze data and Cardboard or poster board determine the scale and Glue properties of objects in the solar system. Scissors or razor blade Popsicle sticks Extra copies of the Orion and Big Dipper sheet for your Earth observers Do Ahead • You want to have 7 stars for each constellation that students can hold. Cut out 6 blue stars and one Betelgeuse for Orion, glue onto board, glue Orion constellation on back, attach popsicle stick for holding. • Cut out 6 blue stars and 1 Mizar for the Big Dipper, glue onto board, glue Big Dipper on back, attach popsicle stick for holding.
    [Show full text]
  • Winter Constellations
    Winter Constellations *Orion *Canis Major *Monoceros *Canis Minor *Gemini *Auriga *Taurus *Eradinus *Lepus *Monoceros *Cancer *Lynx *Ursa Major *Ursa Minor *Draco *Camelopardalis *Cassiopeia *Cepheus *Andromeda *Perseus *Lacerta *Pegasus *Triangulum *Aries *Pisces *Cetus *Leo (rising) *Hydra (rising) *Canes Venatici (rising) Orion--Myth: Orion, the great ​ ​ hunter. In one myth, Orion boasted he would kill all the wild animals on the earth. But, the earth goddess Gaia, who was the protector of all animals, produced a gigantic scorpion, whose body was so heavily encased that Orion was unable to pierce through the armour, and was himself stung to death. His companion Artemis was greatly saddened and arranged for Orion to be immortalised among the stars. Scorpius, the scorpion, was placed on the opposite side of the sky so that Orion would never be hurt by it again. To this day, Orion is never seen in the sky at the same time as Scorpius. DSO’s ● ***M42 “Orion Nebula” (Neb) with Trapezium A stellar ​ ​ ​ nursery where new stars are being born, perhaps a thousand stars. These are immense clouds of interstellar gas and dust collapse inward to form stars, mainly of ionized hydrogen which gives off the red glow so dominant, and also ionized greenish oxygen gas. The youngest stars may be less than 300,000 years old, even as young as 10,000 years old (compared to the Sun, 4.6 billion years old). 1300 ly. ​ ​ 1 ● *M43--(Neb) “De Marin’s Nebula” The star-forming ​ “comma-shaped” region connected to the Orion Nebula. ● *M78--(Neb) Hard to see. A star-forming region connected to the ​ Orion Nebula.
    [Show full text]
  • Creating a Constellation
    CLASSROOM ACTIVITY Creating a Constellation General Information Level: elementary 1st and 2nd cycles. Students per group: individual activity. How long: two 60-minute periods. Where: in class. When: before visiting the Planetarium. Type of activity: discovery led by the teacher. Key words: constellations — stars — legends — mythology. Skills honed: observing, classifying, inventing concepts, researching, developing motor skills, writing, communicating, fostering creativity. Starting Point What is a constellation? What picture does a group of stars evoke? Can I create my own constellation and think up a story about it? Preconceptions Students, particularly younger ones, might not know what a constellation is. They may also believe that the constellations are the same for all people on Earth and that everyone who looks at a specific group of stars sees the same thing in it. Basic Concepts From time immemorial, people have pondered the heavens. In the patterns formed by neighbour- ing stars, different cultures have seen animals, mythical creatures, legendary heroes, and objects of cultural importance. These groups of randomly linked stars are known as constellations. Creating a Constellation © 2000 Planétarium de Montréal — 2001.12.08 1 Goals Students create their own constellation from a group of stars and invent stories explaining their constellation. They then compare their creations with what other students have thought up and what other cultures have seen in the same group of stars. By the end of this activity, students should be able to: • Defi ne constellation (a pattern formed by a group of stars). • Create a constellation using a specifi c group of stars. • Make up a brief story about their constellation.
    [Show full text]
  • IBAK Sewer and Manhole Inspection Systems
    IBAK Sewer and Manhole Inspection Systems Table of contents Hindsight – Insight – Foresight ..................................... 4 Cable drums and cable winches IBAK Sewer and Manhole Inspection Systems ............ 6 Extension Kit ............................................................... 44 IBAK KT 180 ............................................................... 46 Cameras IBAK KW 180 .............................................................. 48 IBAK HYDRUS .............................................................. 8 IBAK KW 305/310/505 ................................................ 50 IBAK NANO / NANO L ................................................. 10 IBAK KW LISY Synchron ............................................ 52 IBAK JUNO ................................................................. 12 IBAK POLARIS ............................................................ 14 Compact push system IBAK ORION .............................................................. 16 IBAK HSP .................................................................... 54 IBAK ORION L ............................................................ 18 IBAK MiniLite .............................................................. 56 IBAK ORPHEUS 2 ...................................................... 20 IBAK ORPHEUS 2 HD ................................................ 22 Control units/systems IBAK ARGUS 5 ........................................................... 24 IBAK BK 3.5 ...............................................................
    [Show full text]
  • Winter Observing Notes
    Wynyard Planetarium & Observatory Winter Observing Notes Wynyard Planetarium & Observatory PUBLIC OBSERVING – Winter Tour of the Sky with the Naked Eye NGC 457 CASSIOPEIA eta Cas Look for Notice how the constellations 5 the ‘W’ swing around Polaris during shape the night Is Dubhe yellowish compared 2 Polaris to Merak? Dubhe 3 Merak URSA MINOR Kochab 1 Is Kochab orange Pherkad compared to Polaris? THE PLOUGH 4 Mizar Alcor Figure 1: Sketch of the northern sky in winter. North 1. On leaving the planetarium, turn around and look northwards over the roof of the building. To your right is a group of stars like the outline of a saucepan standing up on it’s handle. This is the Plough (also called the Big Dipper) and is part of the constellation Ursa Major, the Great Bear. The top two stars are called the Pointers. Check with binoculars. Not all stars are white. The colour shows that Dubhe is cooler than Merak in the same way that red-hot is cooler than white-hot. 2. Use the Pointers to guide you to the left, to the next bright star. This is Polaris, the Pole (or North) Star. Note that it is not the brightest star in the sky, a common misconception. Below and to the right are two prominent but fainter stars. These are Kochab and Pherkad, the Guardians of the Pole. Look carefully and you will notice that Kochab is slightly orange when compared to Polaris. Check with binoculars. © Rob Peeling, CaDAS, 2007 version 2.0 Wynyard Planetarium & Observatory PUBLIC OBSERVING – Winter Polaris, Kochab and Pherkad mark the constellation Ursa Minor, the Little Bear.
    [Show full text]
  • TAAS Monthly Observing Challenge December 2015 Deep Sky Object
    TAAS Monthly Observing Challenge December 2015 Deep Sky Object NGC 772 (GX) Aries ra: 01h 59m 20.1s dec: +19° 00’ 26” Magnitude (visual) = 10.3 Size = 7.2’ x 4.3’ Position angle = 130° Description: NGC 772 (also known as Arp 78) is an unbarred spiral galaxy approximately 130 million light-years away in the constellation Aries. Around 200,000 light years in diameter, NGC 772 is twice the size of the Milky Way Galaxy, and is surrounded by several satellite galaxies – including the dwarf elliptical, NGC 770 – whose tidal forces on the larger galaxy have likely caused the emergence of a single elongated outer spiral arm that is much more developed than the others arms. Halton Arp includes NGC 772 in his Atlas of Peculiar Galaxies as Arp 78, where it is described as a "Spiral galaxy with a small high-surface brightness companion". Two supernovae (SN 2003 hl & SN 2003 iq) have been observed in NGC 772. Source: https://www.wikipedia.org/wiki/NGC_772 AL: Herschel 400 Challenge Object NGC 2371 / 2372 (PN) Gemini ra: 07h 25m 34.8s dec: +29° 29’ 22” Magnitude (visual) = 11.2 Size = 62” Description: NGC 2371-2 is a dual lobed planetary nebula located in the constellation Gemini. Visually, it appears like it could be two separate objects; therefore, two entries were given to the planetary nebula by William Herschel in the "New General Catalogue", so it may be referred to as NGC 2371, NGC 2372, or variations on this name. Source: https://www.wikipedia.org/wiki/NGC_2371-2 AL: Herschel 400, Planetary Nebula Binocular Object NGC 1807 (OC) Taurus ra: 05h 10m 46.0s dec: +16° 31’ 00” Magnitude (visual) = 7.0 Size = 12’ Description: NGC 1807 is an open cluster at the border of the constellations Taurus and Orion near the open cluster NGC 1817.
    [Show full text]
  • Educator's Guide: Orion
    Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations.
    [Show full text]
  • Constellation Studies - Equatorial Sky in Winter
    Phys1810: General Astronomy 1 W2014 Constellation Studies - Equatorial Sky in Winter Preparation before the observing session - Read "Notes on Observing" thoroughly. - Find all the targets listed below using Starry Night and your star charts. - Note: The observatory longitude is 97.1234° W, the latitude is 49.6452° N and elevation is 233 meters. - Observe any predicted events and record your observations during the observing session In the list of constellations below, the name of the constellation is underlined followed by the genitive case of the name in parenthesis followed by the three-letter abbreviation. Note that references to stars such as α UMa, spoken as alpha Ursae Majoris (note genitive case), literally means alpha of Ursa Major. The Greek letters are usually assigned in order of brightness in the constellation (α -- brightest). Note that the constellation, Ursa Major, is a major exception to this rule. As soon as you get to the observatory the following 3 constellations should be sketched on a full page diagram making sure that their relative positions to each other and to the horizon are drawn as accurately as possible - this means completing the sketch in about 15 minutes. You need to repeat the sketch one hour later. Be sure to indicate the time and the location of the horizon on your diagram. Ursa Major (Ursae Majoris) UMa: (The Great Bear, The Big Dipper, The Plow) Through all ages, Ursa Major has been known under various names. It is linked with the nymph Kallisto, the daughter of Lycaon, a king of Arcadia in Greek mythology. Moving along the asterism of the dipper from the lip identify the stars Dubhe (α UMa), Merak (β UMa), Phecda (γ UMa), Megrez (δ UMa), Alioth (ε UMa), Mizar (ζ UMa), and Alkaid (η UMa).
    [Show full text]
  • The Mongolian Big Dipper Sūtra
    JIABS Journal of the International Association of Buddhist Studies Volume 29 Number 1 2006 (2008) The Journal of the International Association of Buddhist Studies (ISSN 0193-600XX) is the organ of the International Association of Buddhist Studies, Inc. It welcomes scholarly contributions pertaining to all facets of Buddhist Studies. EDITORIAL BOARD JIABS is published twice yearly, in the summer and winter. KELLNER Birgit Manuscripts should preferably be sub- KRASSER Helmut mitted as e-mail attachments to: Joint Editors [email protected] as one single file, complete with footnotes and references, BUSWELL Robert in two different formats: in PDF-format, and in Rich-Text-Format (RTF) or Open- CHEN Jinhua Document-Format (created e.g. by Open COLLINS Steven Office). COX Collet GÓMEZ Luis O. Address books for review to: HARRISON Paul JIABS Editors, Institut für Kultur - und Geistesgeschichte Asiens, Prinz-Eugen- VON HINÜBER Oskar Strasse 8-10, AT-1040 Wien, AUSTRIA JACKSON Roger JAINI Padmanabh S. Address subscription orders and dues, KATSURA Shōryū changes of address, and UO business correspondence K Li-ying (including advertising orders) to: LOPEZ, Jr. Donald S. Dr Jérôme Ducor, IABS Treasurer MACDONALD Alexander Dept of Oriental Languages and Cultures SCHERRER-SCHAUB Cristina Anthropole SEYFORT RUEGG David University of Lausanne CH-1015 Lausanne, Switzerland SHARF Robert email: [email protected] STEINKELLNER Ernst Web: www.iabsinfo.net TILLEMANS Tom Fax: +41 21 692 30 45 ZÜRCHER Erik Subscriptions to JIABS are USD 40 per year for individuals and USD 70 per year for libraries and other institutions. For informations on membership in IABS, see back cover.
    [Show full text]
  • Focus on Zeta Ursae Majoris - Mizar
    Vol. 3 No. 2 Spring 2007 Journal of Double Star Observations Page 51 Stargazers Corner: Focus on Zeta Ursae Majoris - Mizar Jim Daley Ludwig Schupmann Observatory (LSO) New Ipswich, New Hampshire Email: [email protected] Abstract: : This is a general interest article for both the double star viewer and armchair astronomer alike. By highlighting an interesting pair, hopefully in each issue, we have a place for those who love doubles but may have little interest in the rigors of measurements and the long lists of results. Your comments about these mini-articles are welcomed. Arabs long ago named Alcor “Saidak” or “the proof” as Introduction they too used it as a test of vision. Alcor shares nearly My first view of a double star through a telescope the same space motion with Mizar and about 20 other was an inspiring sight and just as with many new stars in what is called the Ursa Major stream or observers today, the star was Mizar. As a beginning moving cluster. The Big Dipper is considered the amateur telescope maker (1951) I followed tradition closest cluster in the solar neighborhood. Alcor’s and began to use closer doubles for resolution testing apparent separation from Mizar is more than a quar- the latest homemade instrument. Visualizing the ter light year and this alone just about rules out this scale of binaries, their physical separation, Keplerian wide pair from being a physical (in a binary star motion, orbital period, component diameters and sense) system and the most recent line-of-sight dis- spectral characteristics, all things I had heard and tance measurements give a difference between them read of, seemed a bit complicated at the time and, I of about 3 light years, ending any ideas of an orbiting might add, more so now! Through the years I found pair.
    [Show full text]
  • The Story of Astronomy
    www.astrosociety.org/uitc No. 42 - Spring 1998 © 1998, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. The Story of Astronomy Mindy Kalchman University of Toronto Lorne Brown Storyteller It was dark. The night sky hung clear over the tiny city in the valley; the stars awesome in their brilliance. A small group of men stood on the top of the hill, looking across the city and the valley to another hill on the other side, some fifteen kilometers away. There, a similar group had assembled, their lights flickering in the distance. "We're ready," said the leader of the first group, a bearded man with intense eyes. "Check your lantern." What was happening? Was this a covert military operation? A band of thieves and robbers plotting plunder? Actually, it was a scientific experiment. The leader was the great Galileo himself, who would later be denounced for claiming that the Earth revolves around the Sun. The experiment was simplicity itself: a lantern would be uncovered on one hill. Fifteen kilometers away, a second lantern would be uncovered, shining back to the first. Light would have thus traveled thirty kilometers, twice across the valley where the Italian city of Florence nestled. By timing how long it took the light to travel this distance, Galileo could calculate the speed of light. He was going to catch the ghost of the universe! Oral traditions have since time immemorial satisfied generations of children and adults with stories of wonder, fantasy, truth, and mystery. Stories are irreplaceable stimulants for the imagination and an often endless source of entertainment.
    [Show full text]