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FY08 Technical Papers by GSMTPO Staff
AURA/NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation July 23, 2008 Revised as Complete and Submitted December 23, 2008 NGC 660, ~13 Mpc from the Earth, is a peculiar, polar ring galaxy that resulted from two galaxies colliding. It consists of a nearly edge-on disk and a strongly warped outer disk. Image Credit: T.A. Rector/University of Alaska, Anchorage NATIONAL OPTICAL ASTRONOMY OBSERVATORY NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation December 23, 2008 TABLE OF CONTENTS EXECUTIVE SUMMARY ............................................................................................................................. 1 1 SCIENTIFIC ACTIVITIES AND FINDINGS ..................................................................................... 2 1.1 Cerro Tololo Inter-American Observatory...................................................................................... 2 The Once and Future Supernova η Carinae...................................................................................................... 2 A Stellar Merger and a Missing White Dwarf.................................................................................................. 3 Imaging the COSMOS...................................................................................................................................... 3 The Hubble Constant from a Gravitational Lens.............................................................................................. 4 A New Dwarf Nova in the Period Gap............................................................................................................ -
Wildcard Innovations Argo Navis: So Just How Does It Stack up to the Sky Commander? Tom Trusock – 11/2004
Copyright © 2004 CloudyNights Telescope Reviews WildCard Innovations Argo Navis: So just how does it stack up to the Sky Commander? Tom Trusock – 11/2004 Reviewed: Argo Navis Ok – so I’m lazy. Features: • Digital Telescope Well – maybe that’s not quite true. There are Computer some nights I just don’t believe in excess work. • 2 serial interfaces I’m basically a visual observer, and while I do • Dual CPU’s enjoy the challenge of the hunt – I often just • 2 Meg Ram want to get to the target. Years ago, I settled on • Multitude of Catalogs DSC’s as my one of my preferred methods of finding DSO’s – especially faint fuzzies. If you are new to DSC (Digital Setting Circles) you might want to start off by reading “A Digital Setting Circles Primer”. I’ve owned at least a half dozen different units, among them units from JMI, Celestron, Sky Commander and now the newest kid on the block; the Argo Navis. Coming out of Australia, the Argo makes use of modern technology and components, utilizing not one, but two Motorola 5206e ColdFire 40mhz 32bit CPU’s (the same family of CPU’s used in the popular Palm series of Personal Digital Assistants) 2mb of re-programmable flash memory, 512kb of static Ram, WildCard Innovations Argo Navis and 8kb of non-volatile Ram. It’s powered from 4 AA batteries or an 8 to 16V external source. When used with external power, the Argo offers an LCD heater function to assist in keeping the display functional and dew off. -
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. -
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. -
FOR an ADVANCED Oaoi
.' ' ' > \ .\i I X-732-67-363 < I A COMPUTER, CONTROL SYSTEM I FOR AN ADVANCED OAOi ) I i I , 1 \ i J'OHN A. ,HRASTAR , P 1 (ACCESSION NUMBER) (THRU) I P > . -. c (PAGES) / + AUGUST 1967 - I . \ \ I, I \ / - k d - GO~DARD'SPACE FLIGHT CENTER ' GREENBELT, MARYLAND . .r A COMPUTER CONTROL SYSTEM FOR AN ADVANCED OAO John A. Hrastar August 1967 Goddard Space Flight Center Greenbelt, Maryland A COMPUTER CONTROL SYSTEM FOR AN ADVANCED OAO John A. Hrastar SUMMARY The purpose of the study covered by this report was to determine the feasibility of using an on-board digital computer and strap-down inertial reference unit for attitude control of an advanced OAO space- craft. An integrated, three axis control law was assumed which had been previously proven stable in the large. The principal advantage of this type of control system is the ability to complete three axis reori- entations over large angles. This system, although apparently complex, has the effect of simplifying the overall system. This is because a re- orientation is a simple extension of a hold or point operation, i.e., mode switching may be simplified. The study indicates that a system of this type is feasible and offers many advantages over present systems. The time for a reorientation using this type of control is considerably shorter than the time required using more conventional methods. The computer and inertial reference unit usedinthe study had the characteristics of systems presently under development. Feasibility, therefore is within the present state of the art, requiring only continued development of these systems. -
The Sky Tonight
MARCH POUTŪ-TE-RANGI HIGHLIGHTS Conjunction of Saturn and the Moon A conjunction is when two astronomical objects appear close in the sky as seen THE- SKY TONIGHT- - from Earth. The planets, along with the TE AHUA O TE RAKI I TENEI PO Sun and the Moon, appear to travel across Brightest Stars our sky roughly following a path called the At this time of the year, we can see the ecliptic. Each body travels at its own speed, three brightest stars in the night sky. sometimes entering ‘retrograde’ where they The brightness of a star, as seen from seem to move backwards for a period of time Earth, is measured as its apparent (though the backwards motion is only from magnitude. Pictured on the cover is our vantage point, and in fact the planets Sirius, the brightest star in our night sky, are still orbiting the Sun normally). which is 8.6 light-years away. Sometimes these celestial bodies will cross With an apparent magnitude of −1.46, paths along the ecliptic line and occupy the this star can be found in the constellation same space in our sky, though they are still Canis Major, high in the northern sky. millions of kilometres away from each other. Sirius is actually a binary star system, consisting of Sirius A which is twice the On March 19, the Moon and Saturn will be size of the Sun, and a faint white dwarf in conjunction. While the unaided eye will companion named Sirius B. only see Saturn as a bright star-like object (Saturn is the eighth brightest object in our Sirius is almost twice as bright as the night sky), a telescope can offer a spectacular second brightest star in the night sky, view of the ringed planet close to our Moon. -
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. -
Exploring the Brown Dwarf Desert C
Astronomy & Astrophysics manuscript no. draft c ESO 2018 March 5, 2018 MOA-2007-BLG-197: Exploring the brown dwarf desert C. Ranc1; 35, A. Cassan1; 35, M. D. Albrow2; 35, D. Kubas1; 35, I. A. Bond3; 36, V. Batista1; 35, J.-P. Beaulieu1; 35, D. P. Bennett4; 36, M. Dominik5; 35, Subo Dong6; 37, P. Fouqué7; 8; 35, A. Gould9; 37, J. Greenhilly10; 35, U. G. Jørgensen11; 35, N. Kains12; 5; 35, J. Menzies13; 35, T. Sumi14; 36, E. Bachelet15; 35, C. Coutures1; 35, S. Dieters1; 35, D. Dominis Prester16; 35, J. Donatowicz17; 35, B. S. Gaudi9; 37, C. Han18; 37, M. Hundertmark5; 11, K. Horne5; 35, S. R. Kane19; 35, C.-U. Lee20; 37, J.-B. Marquette1; 35, B.-G. Park20; 37, K. R. Pollard2; 35, K. C. Sahu12; 35, R. Street21; 35, Y. Tsapras21; 22; 35, J. Wambsganss22; 35, A. Williams23; 24; 35, M. Zub22; 35, F. Abe25; 36, A. Fukui26; 36, Y. Itow25; 36, K. Masuda25; 36, Y. Matsubara25; 36, Y. Muraki25; 36, K. Ohnishi27; 36, N. Rattenbury28; 36, To. Saito29; 36, D. J. Sullivan30; 36, W. L. Sweatman31; 36, P. J. Tristram32; 36, P. C. M. Yock33; 36, and A. Yonehara34; 36 (Affiliations can be found after the references) Received <date> / accepted <date> ABSTRACT We present the analysis of MOA-2007-BLG-197Lb, the first brown dwarf companion to a Sun-like star detected through gravitational microlensing. The event was alerted and followed-up photometrically by a network of telescopes from the PLANET, MOA, and µFUN collaborations, and observed at high angular resolution using the NaCo instrument at the VLT. -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
Stats2010 E Final.Pdf
Imprint Publisher: Max-Planck-Institut für extraterrestrische Physik Editors and Layout: W. Collmar und J. Zanker-Smith Personnel 1 PERSONNEL 2010 Directors Min. Dir. J. Meyer, Section Head, Federal Ministry of Prof. Dr. R. Bender, Optical and Interpretative Astronomy, Economics and Technology also Professorship for Astronomy/Astrophysics at the Prof. Dr. E. Rohkamm, Thyssen Krupp AG, Düsseldorf Ludwig-Maximilians-University Munich Prof. Dr. R. Genzel, Infrared- and Submillimeter- Scientifi c Advisory Board Astronomy, also Prof. of Physics, University of California, Prof. Dr. R. Davies, Oxford University (UK) Berkeley (USA) (Managing Director) Prof. Dr. R. Ellis, CALTECH (USA) Prof. Dr. Kirpal Nandra, High-Energy Astrophysics Dr. N. Gehrels, NASA/GSFC (USA) Prof. Dr. G. Morfi ll, Theory, Non-linear Dynamics, Complex Prof. Dr. F. Harrison, CALTECH (USA) Plasmas Prof. Dr. O. Havnes, University of Tromsø (Norway) Prof. Dr. G. Haerendel (emeritus) Prof. Dr. P. Léna, Université Paris VII (France) Prof. Dr. R. Lüst (emeritus) Prof. Dr. R. McCray, University of Colorado (USA), Prof. Dr. K. Pinkau (emeritus) Chair of Board Prof. Dr. J. Trümper (emeritus) Prof. Dr. M. Salvati, Osservatorio Astrofi sico di Arcetri (Italy) Junior Research Groups and Minerva Fellows Dr. N.M. Förster Schreiber Humboldt Awardee Dr. S. Khochfar Prof. Dr. P. Henry, University of Hawaii (USA) Prof. Dr. H. Netzer, Tel Aviv University (Israel) MPG Fellow Prof. Dr. V. Tsytovich, Russian Academy of Sciences, Prof. Dr. A. Burkert (LMU) Moscow (Russia) Manager’s Assistant Prof. S. Veilleux, University of Maryland (USA) Dr. H. Scheingraber A. v. Humboldt Fellows Scientifi c Secretary Prof. Dr. D. Jaffe, University of Texas (USA) Dr. -
A Blast Wave from the 1843 Eruption of Eta Carinae
1 A Blast Wave from the 1843 Eruption of Eta Carinae Nathan Smith* *Astronomy Department, University of California, 601 Campbell Hall, Berkeley, CA 94720-3411 Very massive stars shed much of their mass in violent precursor eruptions [1] as luminous blue variables (LBVs) [2] before reaching their most likely end as supernovae, but the cause of LBV eruptions is unknown. The 19th century eruption of Eta Carinae, the prototype of these events [3], ejected about 12 solar masses at speeds of 650 km/s, with a kinetic energy of almost 1050ergs[4]. Some faster material with speeds up to 1000-2000 km/s had previously been reported [5,6,7,8] but its full distribution was unknown. Here I report observations of much faster material with speeds up to 3500-6000 km/s, reaching farther from the star than the fastest material in earlier reports [5]. This fast material roughly doubles the kinetic energy of the 19th century event, and suggests that it released a blast wave now propagating ahead of the massive ejecta. Thus, Eta Carinae’s outer shell now mimics a low-energy supernova remnant. The eruption has usually been discussed in terms of an extreme wind driven by the star’s luminosity [2,3,9,10], but fast material reported here suggests that it was powered by a deep-seated explosion rivalling a supernova, perhaps triggered by the pulsational pair instability[11]. This may alter interpretations of similar events seen in other galaxies. Eta Carinae [3] is the most luminous and the best studied among LBVs [1,2]. -
SAS-2019 the Symposium on Telescope Science
Proceedings for the 38th Annual Conference of the Society for Astronomical Sciences SAS-2019 The Symposium on Telescope Science Joint Meeting with the Center for Backyard Astrophysics Editors: Robert K. Buchheim Robert M. Gill Wayne Green John C. Martin John Menke Robert Stephens May, 2019 Ontario, CA i Disclaimer The acceptance of a paper for the SAS Proceedings does not imply nor should it be inferred as an endorsement by the Society for Astronomical Sciences of any product, service, method, or results mentioned in the paper. The opinions expressed are those of the authors and may not reflect those of the Society for Astronomical Sciences, its members, or symposium Sponsors Published by the Society for Astronomical Sciences, Inc. Rancho Cucamonga, CA First printing: May 2019 Photo Credits: Front Cover: NGC 2024 (Flame Nebula) and B33 (Horsehead Nebula) Alson Wong, Center for Solar System Studies Back Cover: SA-200 Grism spectrum of Wolf-Rayet star HD214419 Forrest Sims, Desert Celestial Observatory ii TABLE OF CONTENTS PREFACE v SYMPOSIUM SPONSORS vi SYMPOSIUM SCHEDULE viii PRESENTATION PAPERS Robert D. Stephens, Brian D. Warner THE SEARCH FOR VERY WIDE BINARY ASTEROIDS 1 Tom Polakis LESSONS LEARNED DURING THREE YEARS OF ASTEROID PHOTOMETRY 7 David Boyd SUDDEN CHANGE IN THE ORBITAL PERIOD OF HS 2325+8205 15 Tom Kaye EXOPLANET DETECTION USING BRUTE FORCE TECHNIQUES 21 Joe Patterson, et al FORTY YEARS OF AM CANUM VENATICORIUM 25 Robert Denny ASCOM – NOT JUST FOR WINDOWS ANY MORE 31 Kalee Tock HIGH ALTITUDE BALLOONING 33 William Rust MINIMIZING DISTORTION IN TIME EXPOSED CELESTIAL IMAGES 43 James Synge PROJECT PANOPTES 49 Steve Conard, et al THE USE OF FIXED OBSERVATORIES FOR FAINT HIGH VALUE OCCULTATIONS 51 John Martin, Logan Kimball UPDATE ON THE M31 AND M33 LUMINOUS STARS SURVEY 53 John Morris CURRENT STATUS OF “VISUAL” COMET PHOTOMETRY 55 Joe Patterson, et al ASASSN-18EY = MAXIJ1820+070 = “MAXIE”: KING OF THE BLACK HOLE 61 SUPERHUMPS Richard Berry IMAGING THE MOON AT THERMAL INFRARED WAVELENGTHS 67 iii Jerrold L.