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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. -
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. -
The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 a Good Way to Start – Find North
The expression "dog days" refers to the period from July 3 through Aug. 11 when our brightest night star, SIRIUS (aka the dog star), rises in conjunction* with the sun. Conjunction, in astronomy, is defined as the apparent meeting or passing of two celestial bodies. TAAS Fabulous Fifty A program for those new to astronomy Friday Evening, July 20, 2018, 8:00 pm All TAAS and other new and not so new astronomers are welcome. What is the TAAS Fabulous 50 Program? It is a set of 4 meetings spread across a calendar year in which a beginner to astronomy learns to locate 50 of the most prominent night sky objects visible to the naked eye. These include stars, constellations, asterisms, and Messier objects. Methodology 1. Meeting dates for each season in year 2018 Winter Jan 19 Spring Apr 20 Summer Jul 20 Fall Oct 19 2. Locate the brightest and easiest to observe stars and associated constellations 3. Add new prominent constellations for each season Tonight’s Schedule 8:00 pm – We meet inside for a slide presentation overview of the Summer sky. 8:40 pm – View night sky outside The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 A Good Way to Start – Find North Polaris North Star Polaris is about the 50th brightest star. It appears isolated making it easy to identify. Circumpolar Stars Polaris Horizon Line Albuquerque -- 35° N Circumpolar Stars Capella the Goat Star AS THE WORLD TURNS The Circle of Perpetual Apparition for Albuquerque Deneb 1 URSA MINOR 2 3 2 URSA MAJOR & Vega BIG DIPPER 1 3 Draco 4 Camelopardalis 6 4 Deneb 5 CASSIOPEIA 5 6 Cepheus Capella the Goat Star 2 3 1 Draco Ursa Minor Ursa Major 6 Camelopardalis 4 Cassiopeia 5 Cepheus Clock and Calendar A single map of the stars can show the places of the stars at different hours and months of the year in consequence of the earth’s two primary movements: Daily Clock The rotation of the earth on it's own axis amounts to 360 degrees in 24 hours, or 15 degrees per hour (360/24). -
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. -
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. -
September 2020 BRAS Newsletter
A Neowise Comet 2020, photo by Ralf Rohner of Skypointer Photography Monthly Meeting September 14th at 7:00 PM, via Jitsi (Monthly meetings are on 2nd Mondays at Highland Road Park Observatory, temporarily during quarantine at meet.jit.si/BRASMeets). GUEST SPEAKER: NASA Michoud Assembly Facility Director, Robert Champion What's In This Issue? President’s Message Secretary's Summary Business Meeting Minutes Outreach Report Asteroid and Comet News Light Pollution Committee Report Globe at Night Member’s Corner –My Quest For A Dark Place, by Chris Carlton Astro-Photos by BRAS Members Messages from the HRPO REMOTE DISCUSSION Solar Viewing Plus Night Mercurian Elongation Spooky Sensation Great Martian Opposition Observing Notes: Aquila – The Eagle Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society Baton Rouge Astronomical Society Newsletter, Night Visions Page 2 of 27 September 2020 President’s Message Welcome to September. You may have noticed that this newsletter is showing up a little bit later than usual, and it’s for good reason: release of the newsletter will now happen after the monthly business meeting so that we can have a chance to keep everybody up to date on the latest information. Sometimes, this will mean the newsletter shows up a couple of days late. But, the upshot is that you’ll now be able to see what we discussed at the recent business meeting and have time to digest it before our general meeting in case you want to give some feedback. Now that we’re on the new format, business meetings (and the oft neglected Light Pollution Committee Meeting), are going to start being open to all members of the club again by simply joining up in the respective chat rooms the Wednesday before the first Monday of the month—which I encourage people to do, especially if you have some ideas you want to see the club put into action. -
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. -
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. -
Religious Service Development of Folk Religion Temples in Taiwan: a Comprehensive Perspective∗
Rev. Integr. Bus. Econ. Res. Vol 4(1) 49 Religious Service Development of Folk Religion Temples in Taiwan: A Comprehensive Perspective∗ Kuo-Yan Wang School of Management, Xiamen University Tan Kah Kee College [email protected] ABSTRACT Buying a sense of happiness from divine power for the future is the reflection of cultural relativism and universal values, whether the religious belief and person perception. Folk religion temples in Taiwan, undergoing economic anxiety and social status chaos in the past two decades, have illustrated the phenomenon of commercialization, and this phenomenon is forming a service system with many tentacles due to the highly homogeneous of religious services. This article, therefore, is clearly distinguished the increasing sources of donation/profit at current folk temples in Taiwan, and further discussed the influence of folk belief adherents. The conclusion involves future research directions, which can be enriched for the issue of Chinese folk belief religious services development. Keywords: Folk belief, religious service, temple, secularism. 1. INTRODUCTION Zaidman (2003) observed that the New Age sect, in contrast with traditional Christianity, has opened at least 25 shops in Israel. Recently, Zaidman delved deeply into whether “New Age shops” harm spirituality, and concluded that such shops are making an effort to construct a “creation of a sacred place” in the commodity context (2007). Vokurka and McDaniel (2004) also categorized three common types of church marketing strategy: traditional, program-oriented, and worship-oriented, based on the responses of 247 Southern Baptist churches. Ivakhiv (2003) focused on “self-spirituality” in the phenomenon of “New Age pilgrimage” and found that New Age pilgrims usually have their own individual interests or objective knowledge, rather than traditional Christian pilgrims who sincerely embrace the stories or myths associated with sacred places. -
TAAS Fabulous Fifty
TAAS Fabulous Fifty Friday April 21, 2017 19:30 MDT (7:30 pm) Ursa Major Photo Courtesy of Naoyuki Kurita All TAAS and other new and not so new astronomers are invited Evening Events 7:30 pm Meet inside church for overview of winter sky 8:30 pm View night sky outside 9:00 pm Social session inside church 10:00 pm Optional additional viewing outside Objectives Provide new astronomers a list of 50 night sky objects 1. Locate with the naked eye 2. Showcases the night sky for an entire year 3. Beginner astronomer will remember from one observing session to the next 4. Basis for knowing the night sky well enough to perform more detailed observing Methodology 1. Divide the observing activities into the four seasons: Winter Dec-Jan-Feb Spring Mar-Apr-May Summer Jun-Jul-Aug Fall Sep-Oct-Nov Boötes Photo Courtesy of Naoyuki Kurita 2. Begin with the bright and easy to locate and identify stars and associated constellations 3. Add the other constellations for each season Methodology (cont.) 4. Add a few naked eye Messier Objects 5. Include planets as a separate observing activity M 44 “The Beehive” Photo Courtesy of Naoyuki Kurita 6. Include the Moon as a separate observing activity 7. Include meteor showers as separate observing activity Spring Constellations Stars Messier Object Ursa Major Dubhe Merak Leo Regulus M 44 “The Beehive” Boötes Arcturus M 3 The Spring Sky Map Ursa Major Boötes Leo What Are the Messier Objects (M)? 100 astronomical objects listed by French astronomer Charles Messier in 1771 Messier was a comet hunter, and frustrated by -
M31 Andromeda Galaxy Aq
Constellation, Star, and Deep Sky Object Names Andromeda : M31 Andromeda Galaxy Lyra : Vega & M57 Ring Nebula Aquila : Altair Ophiuchus : Bernard’s Star Auriga : Capella Orion : Betelgeuse , Rigel & M42 Orion Nebula Bootes : Arcturus Perseus : Algol Cancer : M44 Beehive Cluster Sagittarius: Sagittarius A* Canes Venatici: M51 Whirlpool Galaxy Taurus : Aldebaran , Hyades Star Cluster , M1 Crab Nebula & Canis Major : Sirius M45 Pleiades Canis Minor : Procyon Tucana : Small Magellanic Cloud (SMC) Cassiopeia : Cassiopeia A & Tycho’s “Star” Ursa Minor : Polaris Centaurus : Proxima Centauri Virgo : Spica Dorado/Mensa : Large Magellanic Cloud (LMC) Milky Way Galaxy Gemini : Castor & Pollux Hercules : M13 Globular Cluster Characteristics of Stars (Compared with Sun) Class Color Temp. ( 1000 K) Absolute Magnitude Solar Luminosity Solar Mass Solar Diameter O Blue 60 -30 -7 1,000,000 50 100 to 1000 B Blue -White 30 -10 -3 10,000 10 10 to 100 A White 10 -7.5 +2 100 2 2 to 10 F White -Yellow 7.5 -6.5 +4 10 1.5 1 to 2 G Yellow 6.5 -4.5 +4.6 1 1 1 K Orange 4.5 -3.5 +11 1/100 0.5 0.5 M Red 3.5 -2.8 +15 1/100,000 0.08 0.1 Magnitude Magnitude scales: The smaller the magnitude number, the brighter the star Every 5 magnitudes = 100 times the brightness of object Every magnitude = 2.512 times the brightness of object Apparent magnitude = the brightness of object as seen from the viewer’s viewpoint (Earth) Absolute magnitude = “true brightness” – brightness as seen from 10 parsecs (32.6 light years) away Distance Measurement 1 astronomical unit = distance between Earth and Sun = 150 million kilometres or 93 million miles 1 light year ≈ 6 trillion miles / 9.5 trillion km Parsec = parallax second of arc – distance that a star “jumps” one second of a degree of arc in the sky as a result of the earth’s revolution around the sun. -
Constellation Discovery Series: URSA MAJOR
Constellation Discovery Series: URSA MAJOR Translation: The large or great bear. Visibility: - Ursa Major is the third largest constellation and one of the brightest. Most of the constellation can be seen throughout most of the year, in most of the northern hemisphere. It is hard to see the rest of the bear, especially from light-polluted cities. Additional Facts: - The constellation of Ursa Major has been recognized as a bear, by many distinct civilizations. - More commonly known as its asterism (a star pattern that makes up part of a constellation or that includes stars from more than one constellation) the Big Dipper. - The two stars which form the outer bowl of the Big Dipper point towards the North Star, Polaris, which can be found as a part of another constellation, the Little Dipper. Examples: URSA MINOR Translation: The little or lesser bear. Visibility: It is easy to recognize because it contains the famous Little Dipper asterism. Additional Facts: - Ursa Minor is also notable for marking the location of the north celestial pole, as it is home to Polaris, the North Star, which is located at the end of the dipper’s handle. - Because the Earth's axis is precessing (similar to how a spinning top wobbles around), Polaris is only temporarily at the North Pole. In about 14,000 years, Vega will be the North Star and another 14,000 years after that, it will be Polaris again. - Precession is caused by the gravitational attraction of the Sun and the Moon. It only happens because the Earth is not quite spherical.