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Instruction Manual
1 Contents 1. Constellation Watch Cosmo Sign.................................................. 4 2. Constellation Display of Entire Sky at 35° North Latitude ........ 5 3. Features ........................................................................................... 6 4. Setting the Time and Constellation Dial....................................... 8 5. Concerning the Constellation Dial Display ................................ 11 6. Abbreviations of Constellations and their Full Spellings.......... 12 7. Nebulae and Star Clusters on the Constellation Dial in Light Green.... 15 8. Diagram of the Constellation Dial............................................... 16 9. Precautions .................................................................................... 18 10. Specifications................................................................................. 24 3 1. Constellation Watch Cosmo Sign 2. Constellation Display of Entire Sky at 35° The Constellation Watch Cosmo Sign is a precisely designed analog quartz watch that North Latitude displays not only the current time but also the correct positions of the constellations as Right ascension scale Ecliptic Celestial equator they move across the celestial sphere. The Cosmo Sign Constellation Watch gives the Date scale -18° horizontal D azimuth and altitude of the major fixed stars, nebulae and star clusters, displays local i c r e o Constellation dial setting c n t s ( sidereal time, stellar spectral type, pole star hour angle, the hours for astronomical i o N t e n o l l r f -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
Scutum Apus Aquarius Aquila Ara Bootes Canes Venatici Capricornus Centaurus Cepheus Circinus Coma Berenices Corona Austrina Coro
Polaris Ursa Minor Cepheus Camelopardus Thuban Draco Cassiopeia Mizar Ursa Major Lacerta Lynx Deneb Capella Perseus Auriga Canes Venatici Algol Cygnus Vega Cor Caroli Andromeda Lyra Bootes Leo Minor Castor Triangulum Corona Borealis Albireo Hercules Pollux Alphecca Gemini Vulpecula Coma Berenices Pleiades Aries Pegasus Sagitta Arcturus Taurus Cancer Aldebaran Denebola Leo Delphinus Serpens [Caput] Regulus Equuleus Altair Canis Minor Pisces Betelgeuse Aquila Procyon Orion Serpens [Cauda] Ophiuchus Virgo Sextans Monoceros Mira Scutum Rigel Aquarius Spica Cetus Libra Crater Capricornus Hydra Sirius Corvus Lepus Deneb Kaitos Canis Major Eridanus Antares Fomalhaut Piscis Austrinus Sagittarius Scorpius Antlia Pyxis Fornax Sculptor Microscopium Columba Caelum Corona Austrina Lupus Puppis Grus Centaurus Vela Norma Horologium Phoenix Telescopium Ara Canopus Indus Crux Pictor Achernar Hadar Carina Dorado Tucana Circinus Rigel Kentaurus Reticulum Pavo Triangulum Australe Musca Volans Hydrus Mensa Apus SampleOctans file Chamaeleon AND THE LONELY WAR Sample file STAR POWER VOLUME FOUR: STAR POWER and the LONELY WAR Copyright © 2018 Michael Terracciano and Garth Graham. All rights reserved. Star Power, the Star Power logo, and all characters, likenesses, and situations herein are trademarks of Michael Terracciano and Garth Graham. Except for review purposes, no portion of this publication may be reproduced or transmitted, in any form or by any means, without the express written consent of the copyright holders. All characters and events in this publication are fictional and any resemblance to real people or events is purely coincidental. Star chartsSample adapted from charts found at hoshifuru.jp file Portions of this book are published online at www.starpowercomic.com. This volume collects STAR POWER and the LONELY WAR Issues #16-20 published online between Oct 2016 and Oct 2017. -
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. -
'Insect Succession Pattern on Decomposing Pig Carcasses In
Papers and Proceedings of the Royal Society of Tasmania, Volume 153, 2019 31 INSECT SUCCESSION PATTERN ON DECOMPOSING PIG CARCASSES IN TASMANIA: A SUMMER STUDY by Paola A. Magni, J. David North, Melle Zwerver, Ian R. Dadour (with one text- igure, two plates and one table) Magni, P.A., North, J.D., Zwerver, M., Dadour, I.R. 2019 (14:xii). Insect succession pattern on decomposing pig carcasses in Tasmania: a summer study. Papers and Proceedings of the Royal Society of Tasmania 153: 31–38. https://doi.org/10.26749/rstpp.153.31 ISSN 0080–4703. Discipline of Medical, Molecular & Forensic Sciences, Murdoch University, 90 South St, Murdoch, Western Australia 6150, Australia (PAM, IRD). Murdoch University Singapore, King’s Centre, 390 Havelock Road, Singapore 169662 (current address: PAM). Tasmania Police Forensic Services, 37–43 Liverpool Street, Hobart, Tasmania 7000, Australia (JDN). Tasmania Police, Devonport Police Station, 24 Wenvoe Street, Devonport, Tasmania 7310, Australia (MZ). *Author for correspondence: Email: [email protected]. Insect succession has been studied around the world using the predictable and mostly sequential arrival pattern of different insect species that are attracted to a decomposing carcass. In cases of suspicious death of humans and animals, carrion insects may be used to assist in crime scene reconstruction. The present research represents the first study in forensic entomology to be undertaken in Tasmania, investi-gating insect succession patterns on decomposing pig carcasses and providing a preliminary database of forensically important insects. Six pig carcasses were placed in two contrasting locations (rural and urban) in northern Tasmania. Insect successional waves were recorded over a 40-day study during the austral summer season. -
Chemical Abundances of Four Red Supergiants Star Clusters (Rsgcs) in Scutum-Crux Arm
Star Clusters: From the Milky Way to the Early Universe Proceedings IAU Symposium No. 351, 2019 c International Astronomical Union 2020 A. Bragaglia, M. Davies, A. Sills & E. Vesperini, eds. doi:10.1017/S1743921319006902 Chemical abundances of four red supergiants star clusters (RSGCs) in Scutum-Crux arm Sang-Hyun Chun Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of Korea email: [email protected] Abstract. We investigate the spectral properties of red supergiant stars in the four RSGCs (RSGC2, RSGC3, RSGC4, RSGC5, and Alicante 10) in the Scutum-Crux arm of the Milky Way. The high-resolution (R ∼ 45, 000) near-infrared (H and K bands) spectra for 41 red supergiants were obtained using IGRINS at Gemini South telescope. The calibration of effective tempera- tures and gravities are derived based on the EWTi and EWCO using supergiants in IGIRNS library. The resulted temperatures and gravities are consistent with previous results. Model spectra were synthesized using derived stellar parameters from which we estimate metallicities and chemical abundances like α-elements. In our preliminary result, we find that overall four RSGCs indeed have sub-solar metallicities as already known in previous studies. The metallicity properties of RSGCs are far off the nominal metallicity trend in this region, and this suggests recent low-metallicity gas fueling into the inner disk and bulge. Keywords. stars: abundances, stars: late-type, (stars:) supergiants, Galaxy: disk 1. Introduction Massive stars are important to investigate the structures and chemical evolution of galaxies because of their luminous brightness and chemical enrichment as supernova. -
Sydney Observatory Night Sky Map September 2012 a Map for Each Month of the Year, to Help You Learn About the Night Sky
Sydney Observatory night sky map September 2012 A map for each month of the year, to help you learn about the night sky www.sydneyobservatory.com This star chart shows the stars and constellations visible in the night sky for Sydney, Melbourne, Brisbane, Canberra, Hobart, Adelaide and Perth for September 2012 at about 7:30 pm (local standard time). For Darwin and similar locations the chart will still apply, but some stars will be lost off the southern edge while extra stars will be visible to the north. Stars down to a brightness or magnitude limit of 4.5 are shown. To use this chart, rotate it so that the direction you are facing (north, south, east or west) is shown at the bottom. The centre of the chart represents the point directly above your head, called the zenith, and the outer circular edge represents the horizon. h t r No Star brightness Moon phase Last quarter: 08th Zero or brighter New Moon: 16th 1st magnitude LACERTA nd Deneb First quarter: 23rd 2 CYGNUS Full Moon: 30th rd N 3 E LYRA th Vega W 4 LYRA N CORONA BOREALIS HERCULES BOOTES VULPECULA SAGITTA PEGASUS DELPHINUS Arcturus Altair EQUULEUS SERPENS AQUILA OPHIUCHUS SCUTUM PISCES Moon on 23rd SERPENS Zubeneschamali AQUARIUS CAPRICORNUS E SAGITTARIUS LIBRA a Saturn Centre of the Galaxy Antares Zubenelgenubi t s Antares VIRGO s t SAGITTARIUS P SCORPIUS P e PISCESMICROSCOPIUM AUSTRINUS SCORPIUS Mars Spica W PISCIS AUSTRINUS CORONA AUSTRALIS Fomalhaut Centre of the Galaxy TELESCOPIUM LUPUS ARA GRUSGRUS INDUS NORMA CORVUS INDUS CETUS SCULPTOR PAVO CIRCINUS CENTAURUS TRIANGULUM -
Ecology and Control of the Trachoma Vector Musca Sorbens
Durham E-Theses Ecology and control of the trachoma vector Musca sorbens Emerson, Paul Michael How to cite: Emerson, Paul Michael (2001) Ecology and control of the trachoma vector Musca sorbens, Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/3995/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk Ecology and control of the trachoma vector Musca sorbens Paul Michael Emerson The copyright of this thesis rests with the author. No quotation from it should be published without his prior written consent and information derived from it should be acknowledged. Department of Biological Sciences University of Durham Submitted for the degree of Doctor of Philosophy, December 2001 EcoBegy and control of the trachoma vector Musca sorbens Paul M. Emerson The work described in this thesis was conducted in rural Gambia and builds a body of evidence incriminating the fly Musca sorbens as a vector of the blinding disease, trachoma, which is caused by ocular infection with Chlamydia trachomatis. -
Terrestrial Arthropod Surveys on Pagan Island, Northern Marianas
Terrestrial Arthropod Surveys on Pagan Island, Northern Marianas Neal L. Evenhuis, Lucius G. Eldredge, Keith T. Arakaki, Darcy Oishi, Janis N. Garcia & William P. Haines Pacific Biological Survey, Bishop Museum, Honolulu, Hawaii 96817 Final Report November 2010 Prepared for: U.S. Fish and Wildlife Service, Pacific Islands Fish & Wildlife Office Honolulu, Hawaii Evenhuis et al. — Pagan Island Arthropod Survey 2 BISHOP MUSEUM The State Museum of Natural and Cultural History 1525 Bernice Street Honolulu, Hawai’i 96817–2704, USA Copyright© 2010 Bishop Museum All Rights Reserved Printed in the United States of America Contribution No. 2010-015 to the Pacific Biological Survey Evenhuis et al. — Pagan Island Arthropod Survey 3 TABLE OF CONTENTS Executive Summary ......................................................................................................... 5 Background ..................................................................................................................... 7 General History .............................................................................................................. 10 Previous Expeditions to Pagan Surveying Terrestrial Arthropods ................................ 12 Current Survey and List of Collecting Sites .................................................................. 18 Sampling Methods ......................................................................................................... 25 Survey Results .............................................................................................................. -
These Sky Maps Were Made Using the Freeware UNIX Program "Starchart", from Alan Paeth and Craig Counterman, with Some Postprocessing by Stuart Levy
These sky maps were made using the freeware UNIX program "starchart", from Alan Paeth and Craig Counterman, with some postprocessing by Stuart Levy. You’re free to use them however you wish. There are five equatorial maps: three covering the equatorial strip from declination −60 to +60 degrees, corresponding roughly to the evening sky in northern winter (eq1), spring (eq2), and summer/autumn (eq3), plus maps covering the north and south polar areas to declination about +/− 25 degrees. Grid lines are drawn at every 15 degrees of declination, and every hour (= 15 degrees at the equator) of right ascension. The equatorial−strip maps use a simple rectangular projection; this shows constellations near the equator with their true shape, but those at declination +/− 30 degrees are stretched horizontally by about 15%, and those at the extreme 60−degree edge are plotted twice as wide as you’ll see them on the sky. The sinusoidal curve spanning the equatorial strip is, of course, the Ecliptic −− the path of the Sun (and approximately that of the planets) through the sky. The polar maps are plotted with stereographic projection. This preserves shapes of small constellations, but enlarges them as they get farther from the pole; at declination 45 degrees they’re about 17% oversized, and at the extreme 25−degree edge about 40% too large. These charts plot stars down to magnitude 5, along with a few of the brighter deep−sky objects −− mostly star clusters and nebulae. Many stars are labelled with their Bayer Greek−letter names. Also here are similarly−plotted maps, based on galactic coordinates. -
Selecting New Kinds of Dung Beetles for Better Bush Fly Control
Journal of the Department of Agriculture, Western Australia, Series 4 Volume 25 Number 3 1984 Article 14 1-1-1984 Selecting new kinds of dung beetles for better bush fly control T J. Ridsdill-Smith Follow this and additional works at: https://researchlibrary.agric.wa.gov.au/journal_agriculture4 Part of the Entomology Commons Recommended Citation Ridsdill-Smith, T J. (1984) "Selecting new kinds of dung beetles for better bush fly control," Journal of the Department of Agriculture, Western Australia, Series 4: Vol. 25 : No. 3 , Article 14. Available at: https://researchlibrary.agric.wa.gov.au/journal_agriculture4/vol25/iss3/14 This article is brought to you for free and open access by Research Library. It has been accepted for inclusion in Journal of the Department of Agriculture, Western Australia, Series 4 by an authorized administrator of Research Library. For more information, please contact [email protected]. • Dung beetles By T. J. Ridsdill Smith, CSIRO Division of Biological control shredding fresh dung. Entomology, Perth Biological control is a strategy by which other Native dung beetles are found in south-western living organisms are used to control a species Australia, but they are largely restricted to that has become a pest. Once the introduced areas of natural uegetaf ion where they feed on species is successfully established, it is dung pellets of marsupials. self-perpetuating. When European man cleared the land, planted Dung beetles and bush fly larvae both feed in pastures and introduced cattle, he created a dung. When beetles are abundant in a dung pad new type of environment which did not suit they compete with the flies which are then killed most native beetles. -
The Effect of Colour on the Numbers of Houseflies Resting on Painted Surfaces
THE EFFECT OF COLOUR ON THE NUMBERS OF HOUSEFLIES RESTING ON PAINTED SURFACES By D. F. WATERHOUSE* [Accepted for Publication September 22, 1947] Summary A simple technique for determining the preference of houseflies for surfdces of various colours is described. This consists of liberating adults into a Peet·Grady testing chamher fitted with movable coloured corners. The numbers of flies rest· ing on the coloured corners are recorded at intervals to provide adequate data for comparison. The ascending order of preference for the particular colours lested was white and sky hlue (equal) ,light grey, green, yellow and medium grey (equal), dusky hIue, and red. From measurements of the visual reflectances of the various colours it was found. that the order of preference could he explained. largely hy a reaction to the intensity of the light reflected hy the coloured surfaces, darker surfaces heing preferred to lighter surfaces. I. INTRODUCTION Colour perception in insects has been reviewed extensively by Weiss (1943, 1944, 1946), who points out' that most of the available information indicates that light intensity is more important than wavelength' in producing reactions. However, von Frisch and others have shown that, for bees at least, there is a definite wavelength discrimination (Wigglesworth 1939). The present tests were initiated when a proposal was made during the war that army kitchens and hospitals should be painted dark blue to repel flies. While it is well known that the common bush fly, Musca vetustissima, will not enter darkened rooms, the reaction of the housefly, M. domestica, is quite dif ferent. Thus there is a general trend in the evidence of Freeborn and Berry (1935) and Atkeson et al.