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The W.A.S.P the Warren Astronomical Society Paper
Vol. 49, no. 1 January, 2018 The W.A.S.P The Warren Astronomical Society Paper President Jeff MacLeod [email protected] The Warren Astronomical Society First Vice President Jonathan Kade [email protected] Second Vice President Joe Tocco [email protected] Founded: 1961 Treasurer Ruth Huellmantel [email protected] P.O. Box 1505 Secretary Parker Huellmantel [email protected] Outreach Diane Hall [email protected] Warren, Michigan 48090-1505 Publications Brian Thieme [email protected] www.warrenastro.org Entire board [email protected] Astronomy at the Beach Class of 2017 / Photo credit: Phyllis Voorheis 2017 Warren Astronomical Society Banquet The Warren Astronomical Society concluded the year with a bang-up finale, accompanied by an impromptu drum line. Booming drums aside, it was a delight to see new faces in the group. Plus, Jeff MacLeod managed to work in a bit of juggling. The prize table, once again, had a desirable selection of prizes, a choice one being a Vixen telescope which went to our president-elect, Jeff MacLeod. The way he clutched it, you could almost hear him whispering, “My Precious.” Many thanks to the product sponsors for the event: Apache-Sitgreaves Research Center, Celestron Corporation, Oberwerk Corporation, Sirius Astro Products, and Sky and Telescope Magazine, along with the many generous donations from our own members. Continued pg 3 1 Society Meeting Times January Discussion Astronomy presentations and lectures twice Group Meeting each month at 7:30 PM: Tuesday, January 23 from 6:30 - 8:30 PM First Monday at Cranbrook Institute of 22275 Michigan Ave. Science. Dearborn, Michigan Third Thursday at Macomb Community Coffee and cookies provided (donations College - South Campus Building J (Library) requested), bring snacks and drinks to share. -
Stsci Newsletter: 2011 Volume 028 Issue 02
National Aeronautics and Space Administration Interacting Galaxies UGC 1810 and UGC 1813 Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) 2011 VOL 28 ISSUE 02 NEWSLETTER Space Telescope Science Institute We received a total of 1,007 proposals, after accounting for duplications Hubble Cycle 19 and withdrawals. Review process Proposal Selection Members of the international astronomical community review Hubble propos- als. Grouped in panels organized by science category, each panel has one or more “mirror” panels to enable transfer of proposals in order to avoid conflicts. In Cycle 19, the panels were divided into the categories of Planets, Stars, Stellar Rachel Somerville, [email protected], Claus Leitherer, [email protected], & Brett Populations and Interstellar Medium (ISM), Galaxies, Active Galactic Nuclei and Blacker, [email protected] the Inter-Galactic Medium (AGN/IGM), and Cosmology, for a total of 14 panels. One of these panels reviewed Regular Guest Observer, Archival, Theory, and Chronology SNAP proposals. The panel chairs also serve as members of the Time Allocation Committee hen the Cycle 19 Call for Proposals was released in December 2010, (TAC), which reviews Large and Archival Legacy proposals. In addition, there Hubble had already seen a full cycle of operation with the newly are three at-large TAC members, whose broad expertise allows them to review installed and repaired instruments calibrated and characterized. W proposals as needed, and to advise panels if the panelists feel they do not have The Advanced Camera for Surveys (ACS), Cosmic Origins Spectrograph (COS), the expertise to review a certain proposal. Fine Guidance Sensor (FGS), Space Telescope Imaging Spectrograph (STIS), and The process of selecting the panelists begins with the selection of the TAC Chair, Wide Field Camera 3 (WFC3) were all close to nominal operation and were avail- about six months prior to the proposal deadline. -
Further Defining Spectral Type" Y" and Exploring the Low-Mass End of The
Submitted to The Astrophysical Journal Further Defining Spectral Type “Y” and Exploring the Low-mass End of the Field Brown Dwarf Mass Function J. Davy Kirkpatricka, Christopher R. Gelinoa, Michael C. Cushingb, Gregory N. Macec Roger L. Griffitha, Michael F. Skrutskied, Kenneth A. Marsha, Edward L. Wrightc, Peter R. Eisenhardte, Ian S. McLeanc, Amanda K. Mainzere, Adam J. Burgasserf , C. G. Tinneyg, Stephen Parkerg, Graeme Salterg ABSTRACT We present the discovery of another seven Y dwarfs from the Wide-field In- frared Survey Explorer (WISE). Using these objects, as well as the first six WISE Y dwarf discoveries from Cushing et al., we further explore the transition between spectral types T and Y. We find that the T/Y boundary roughly coincides with the spot where the J − H colors of brown dwarfs, as predicted by models, turn back to the red. Moreover, we use preliminary trigonometric parallax measure- ments to show that the T/Y boundary may also correspond to the point at which the absolute H (1.6 µm) and W2 (4.6 µm) magnitudes plummet. We use these discoveries and their preliminary distances to place them in the larger context of the Solar Neighborhood. We present a table that updates the entire stellar and substellar constinuency within 8 parsecs of the Sun, and we show that the cur- rent census has hydrogen-burning stars outnumbering brown dwarfs by roughly a factor of six. This factor will decrease with time as more brown dwarfs are iden- tified within this volume, but unless there is a vast reservoir of cold brown dwarfs arXiv:1205.2122v1 [astro-ph.SR] 9 May 2012 aInfrared Processing and Analysis Center, MS 100-22, California Institute of Technology, Pasadena, CA 91125; [email protected] bDepartment of Physics and Astronomy, MS 111, University of Toledo, 2801 W. -
Astronomy 2009 Index
Astronomy Magazine 2009 Index Subject Index 1RXS J160929.1-210524 (star), 1:24 4C 60.07 (galaxy pair), 2:24 6dFGS (Six Degree Field Galaxy Survey), 8:18 21-centimeter (neutral hydrogen) tomography, 12:10 93 Minerva (asteroid), 12:18 2008 TC3 (asteroid), 1:24 2009 FH (asteroid), 7:19 A Abell 21 (Medusa Nebula), 3:70 Abell 1656 (Coma galaxy cluster), 3:8–9, 6:16 Allen Telescope Array (ATA) radio telescope, 12:10 ALMA (Atacama Large Millimeter/sub-millimeter Array), 4:21, 9:19 Alpha (α) Canis Majoris (Sirius) (star), 2:68, 10:77 Alpha (α) Orionis (star). See Betelgeuse (Alpha [α] Orionis) (star) Alpha Centauri (star), 2:78 amateur astronomy, 10:18, 11:48–53, 12:19, 56 Andromeda Galaxy (M31) merging with Milky Way, 3:51 midpoint between Milky Way Galaxy and, 1:62–63 ultraviolet images of, 12:22 Antarctic Neumayer Station III, 6:19 Anthe (moon of Saturn), 1:21 Aperture Spherical Telescope (FAST), 4:24 APEX (Atacama Pathfinder Experiment) radio telescope, 3:19 Apollo missions, 8:19 AR11005 (sunspot group), 11:79 Arches Cluster, 10:22 Ares launch system, 1:37, 3:19, 9:19 Ariane 5 rocket, 4:21 Arianespace SA, 4:21 Armstrong, Neil A., 2:20 Arp 147 (galaxy pair), 2:20 Arp 194 (galaxy group), 8:21 art, cosmology-inspired, 5:10 ASPERA (Astroparticle European Research Area), 1:26 asteroids. See also names of specific asteroids binary, 1:32–33 close approach to Earth, 6:22, 7:19 collision with Jupiter, 11:20 collisions with Earth, 1:24 composition of, 10:55 discovery of, 5:21 effect of environment on surface of, 8:22 measuring distant, 6:23 moons orbiting, -
The W.A.S.P the Warren Astronomical Society Paper
Vol. 49, no. 2 February, 2018 The W.A.S.P The Warren Astronomical Society Paper President Jeff MacLeod [email protected] The Warren Astronomical Society First Vice President Jonathan Kade [email protected] Second Vice President Joe Tocco [email protected] Founded: 1961 Treasurer Ruth Huellmantel [email protected] Secretary Parker Huellmantel [email protected] P.O. Box 1505 Outreach Diane Hall [email protected] Warren, Michigan 48090-1505 Publications Brian Thieme [email protected] www.warrenastro.org Entire board [email protected] Astronomy at the Beach Star trails around Polaris, circa mid-1970s - Joe Tocco 1 Society Meeting Times February Discussion Astronomy presentations and lectures twice Group Meeting each month at 7:30 PM: Come on over, and talk astronomy, space news, and whatnot! First Monday at Cranbrook Institute of Science. Joe Tocco will host the February Discussion Group on Tuesday, the 27th, 6:30-8:30: Third Thursday at Macomb Community College - South Campus Building J (Library) MCMI Corporate Office Note: for the summer, we are meeting in 6540 Diplomat Drive room 151, lower level of the library. Sterling Heights, MI 48314 [email protected] Snack Volunteer 586-634-6240 cell Schedule • WiFi Feb 5 Cranbrook Mike O’Dowd • HD Projector with 5.1 Sound System Feb 15 Macomb Gerald Voorheis • Water, coffee, and selection of sodas and M a r 5 C ran b r o o k Ruth Huellmantel snacks provided • Adult beverages are welcomed BYOB If you are unable to bring the snacks on your scheduled day, or if you need to reschedule, Office is located just south of M-59 and just please email the board at board@ East of Mound Road. -
Instruction Manual
iOptron® GEM28 German Equatorial Mount Instruction Manual Product GEM28 and GEM28EC Read the included Quick Setup Guide (QSG) BEFORE taking the mount out of the case! This product is a precision instrument and uses a magnetic gear meshing mechanism. Please read the included QSG before assembling the mount. Please read the entire Instruction Manual before operating the mount. You must hold the mount firmly when disengaging or adjusting the gear switches. Otherwise personal injury and/or equipment damage may occur. Any worm system damage due to improper gear meshing/slippage will not be covered by iOptron’s limited warranty. If you have any questions please contact us at [email protected] WARNING! NEVER USE A TELESCOPE TO LOOK AT THE SUN WITHOUT A PROPER FILTER! Looking at or near the Sun will cause instant and irreversible damage to your eye. Children should always have adult supervision while observing. 2 Table of Content Table of Content ................................................................................................................................................. 3 1. GEM28 Overview .......................................................................................................................................... 5 2. GEM28 Terms ................................................................................................................................................ 6 2.1. Parts List ................................................................................................................................................. -
Lists and Charts of Autostar Named Stars
APPENDIX A Lists and Charts of Autostar Named Stars Table A.I provides a list of named stars that are stored in the Autostar database. Following the list, there are constellation charts which show where the stars are located. The names are in alphabetical orderalong with their Latin designation (see Appendix B for complete list ofconstellations). Names in brackets 0 in the table denote a different spelling to one that is known in the list. The star's co-ordinates are set to the same as accuracy as the Autostar co-ordinates i.e. the RA or Dec 'sec' values are omitted. Autostar option: Select Item: Object --+ Star --+ Named 215 216 Appendix A Table A.1. Autostar Named Star List RA Dec Named Star Fig. Ref. latin Designation Hr Min Deg Min Mag Acamar A5 Theta Eridanus 2 58 .2 - 40 18 3.2 Achernar A5 Alpha Eridanus 1 37.6 - 57 14 0.4 Acrux A4 Alpha Crucis 12 26.5 - 63 05 1.3 Adara A2 EpsilonCanis Majoris 6 58.6 - 28 58 1.5 Albireo A4 BetaCygni 19 30.6 ++27 57 3.0 Alcor Al0 80 Ursae Majoris 13 25.2 + 54 59 4.0 Alcyone A9 EtaTauri 3 47.4 + 24 06 2.8 Aldebaran A9 Alpha Tauri 4 35.8 + 16 30 0.8 Alderamin A3 Alpha Cephei 21 18.5 + 62 35 2.4 Algenib A7 Gamma Pegasi 0 13.2 + 15 11 2.8 Algieba (Algeiba) A6 Gamma leonis 10 19.9 + 19 50 2.6 Algol A8 Beta Persei 3 8.1 + 40 57 2.1 Alhena A5 Gamma Geminorum 6 37.6 + 16 23 1.9 Alioth Al0 EpsilonUrsae Majoris 12 54.0 + 55 57 1.7 Alkaid Al0 Eta Ursae Majoris 13 47.5 + 49 18 1.8 Almaak (Almach) Al Gamma Andromedae 2 3.8 + 42 19 2.2 Alnair A6 Alpha Gruis 22 8.2 - 46 57 1.7 Alnath (Elnath) A9 BetaTauri 5 26.2 -
Introducción
Annual Report CAB 2018 INTRODUCCIÓN El Centro de Astrobiología (CAB) se fundó en 1999 como un Centro Mixto entre el Consejo Superior de Investigaciones Científicas (CSIC) y el Instituto Nacional de Técnica Aeroespacial (INTA). Localizado en el campus del INTA en Torrejón de Ardoz (Madrid), el CAB se convirtió en el primer centro fuera de los Estados Unidos asociado al recién creado NASA Astrobiology Institute (NAI), convirtiéndose en miembro formal en el año 2000. La Astrobiología considera la vida como una consecuencia natural de la evolución del Universo, y en el CAB trabajamos para estudiar el origen, evolución, distribución y futuro de la vida en el Universo, tanto en la Tierra como en entornos extraterrestres. La aplicación del método científico a la Astrobiología requiere la combinación de teoría, simulación, observación y experimentación. Esta aplicación de la Ciencia fundamental a las cuestiones de la Astrobiología es el principal objetivo del CAB. La organización multi- y transdiciplinar del Centro fomenta la interacción de los ingenieros con investigadores experimentales, teóricos y observacionales de varios campos: astronomía, geología, bioquímica, biología, genética, teledetección, ecología microbiana, ciencias de la computación, física, robótica e ingeniería de las comunicaciones. La investigación en el CAB aborda la sistematización de la cadena de eventos que tuvieron lugar entre el Big Bang inicial y el origen de la vida, incluyendo la autoorganización del gas interestelar en moléculas complejas y la formación de sistemas planetarios con ambientes benignos para el florecimiento de la vida. El objetivo final es investigar la posible existencia de vida en otros mundos, reconociendo biosferas diferentes de la terrestre, para ayudarnos en la comprensión del origen de la vida. -
How Astronomical Objects Are Named
How Astronomical Objects Are Named Jeanne E. Bishop Westlake Schools Planetarium 24525 Hilliard Road Westlake, Ohio 44145 U.S.A. bishop{at}@wlake.org Sept 2004 Introduction “What, I wonder, would the science of astrono- use of the sky by the societies of At the 1988 meeting in Rich- my be like, if we could not properly discrimi- the people that developed them. However, these different systems mond, Virginia, the Inter- nate among the stars themselves. Without the national Planetarium Society are beyond the scope of this arti- (IPS) released a statement ex- use of unique names, all observatories, both cle; the discussion will be limited plaining and opposing the sell- ancient and modern, would be useful to to the system of constellations ing of star names by private nobody, and the books describing these things used currently by astronomers in business groups. In this state- all countries. As we shall see, the ment I reviewed the official would seem to us to be more like enigmas history of the official constella- methods by which stars are rather than descriptions and explanations.” tions includes contributions and named. Later, at the IPS Exec- – Johannes Hevelius, 1611-1687 innovations of people from utive Council Meeting in 2000, many cultures and countries. there was a positive response to The IAU recognizes 88 constel- the suggestion that as continuing Chair of with the name registered in an ‘important’ lations, all originating in ancient times or the Committee for Astronomical Accuracy, I book “… is a scam. Astronomers don’t recog- during the European age of exploration and prepare a reference article that describes not nize those names. -
Ulugh Beg's Catalogue of Stars, Rev. from All Persian Manuscripts
-'^. iJ47 .^'> ^*"> ; r^* \ •— SVt^ >.: -<^ »-»S . - -^r jltl)ata, £}eni loth THE GIFT OF •bonfvuaui' ^rOTAjdjjXKuy\ QB 6.047"^°'"*" ""'"""V Library "I"&.^Sj,S?.!SSy? Of Stars, rev. from 3 1924 012 303 800 :^g5J^v,^.>. lb ULUGH BEG'S CATALOGUE OF STARS Revised from all Persian Manuscripts Existing in Great Britain, with a Vocabulary of Persian and Arabic Words BY Edward Ball Knobel Treasurer and Past President of the Royal Astronomical Society The Carnegie Institution of Washington Washington, 1917 Cornell University Library x^ The original of this book is in the Cornell University Library. There are no known copyright restrictions in the United States on the use of the text. http://www.archive.org/details/cu31924012303800 ULUGH BEG'S CATALOGUE OF STARS Revised from all Persian Manuscripts Existing in Great Britain, with a Vocabulary of Persian and Arabic Words BY Edward Ball ^obel Treasurer and Past President of the Royal Astronomical Society The Carnegie Institution of Washington Washington, 1917 ^^ CARNEGIE INSTITUTION OF WASHINGTON Publication No. 250 PRESS OF GIBSON BROTHERS WASHINGTON PREFACE. The present work forms a sequel to the volume on Ptolemy's Catalogue of Stars. Dr. Peters most carefully studied the printed editions of Ulugh Beg's cata- logue and devoted much care to the identification of the stars. He computed the positions of the stars for the epoch 1437.5 from Piazzi's catalogue with Maedler's proper motions. Some 300 of the stars have been re-reduced from the recent catalogues of Danckwortt and Neugebauer with modern proper motions, but the resulting corrections are very small. Peters examined three Persian manuscripts at Paris in 1887, but his collation was incomplete; no doubt it was curtailed by want of time, as he was then more particularly engaged on the Ptolemy manuscripts. -
Instruction Manual
iOptron® GEM45 German Equatorial Mount Instruction Manual Product GEM45 (#7600A series) and GEM45EC (#7600ECA series, as shown) Please read the included GEM45 Quick Setup Guide (QSG) BEFORE taking the mount out of the case! This product is a precision instrument. Please read the included QSG before assembling the mount. Please read the entire Instruction Manual before operating the mount. You must hold the mount firmly when disengaging the gear switches. Otherwise personal injury and/or equipment damage may occur. Any worm system damage due to improper operation will not be covered by iOptron’s limited warranty. If you have any questions please contact us at [email protected] WARNING! NEVER USE A TELESCOPE TO LOOK AT THE SUN WITHOUT A PROPER FILTER! Looking at or near the Sun will cause instant and irreversible damage to your eye. Children should always have adult supervision while using a telescope. 2 Table of Contents Table of Contents ........................................................................................................................................ 3 1. GEM45 Introduction ............................................................................................................................... 5 2. GEM45 Overview ................................................................................................................................... 6 2.1. Parts List .......................................................................................................................................... 6 2.2. Identification -
Black Holes, Chaos in Universe, Processes in Space, Stars, Galaxies, Ordered Universe
International Journal of Astronomy 2020, 9(1): 12-26 DOI: 10.5923/j.astronomy.20200901.03 Black Hole & There is no Chaos in the Universe Weitter Duckss Independent Researcher, Zadar, Croatia Abstract This year's Nobel's Prize in physics has turned into another degradation of science. The first part of the article (3.) deals with chaos that includes very different star systems. Inside a system there are objects with a lot of satellites and those with none. Some planets in distant orbits and brown dwarfs are warmer than some stars. The objects and stars of the same mass have completely different temperatures and are often classified into almost all star types. There is light inside an atmosphere or on the surface of an object without an atmosphere, but it disappears just outside the atmosphere or the surface of the object without the atmosphere. There are galaxies with the blueshift and redshift; although the Universe expands faster and faster, there are 200 000 galaxies and clusters of galaxies that merge or collide. There are enormous differences in the quantity of redshift at the same distances for galaxies and larger objects, i.e., there are different distances – with the differences measured in billions of light-years – for the same quantities of redshift. The other part of the article (4.) removes chaos and returns order in the Universe by implementing identical principles in the whole of the volume and for all objects. Keywords Black holes, Chaos in universe, Processes in space, Stars, Galaxies, Ordered universe universality and removing any paradox that might negate the 1.