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The Comet's Tale
THE COMET’S TALE Newsletter of the Comet Section of the British Astronomical Association Volume 5, No 1 (Issue 9), 1998 May A May Day in February! Comet Section Meeting, Institute of Astronomy, Cambridge, 1998 February 14 The day started early for me, or attention and there were displays to correct Guide Star magnitudes perhaps I should say the previous of the latest comet light curves in the same field. If you haven’t day finished late as I was up till and photographs of comet Hale- got access to this catalogue then nearly 3am. This wasn’t because Bopp taken by Michael Hendrie you can always give a field sketch the sky was clear or a Valentine’s and Glynn Marsh. showing the stars you have used Ball, but because I’d been reffing in the magnitude estimate and I an ice hockey match at The formal session started after will make the reduction. From Peterborough! Despite this I was lunch, and I opened the talks with these magnitude estimates I can at the IOA to welcome the first some comments on visual build up a light curve which arrivals and to get things set up observation. Detailed instructions shows the variation in activity for the day, which was more are given in the Section guide, so between different comets. Hale- reminiscent of May than here I concentrated on what is Bopp has demonstrated that February. The University now done with the observations and comets can stray up to a offers an undergraduate why it is important to be accurate magnitude from the mean curve, astronomy course and lectures are and objective when making them. -
The Comet's Tale
THE COMET’S TALE Journal of the Comet Section of the British Astronomical Association Number 33, 2014 January Not the Comet of the Century 2013 R1 (Lovejoy) imaged by Damian Peach on 2013 December 24 using 106mm F5. STL-11k. LRGB. L: 7x2mins. RGB: 1x2mins. Today’s images of bright binocular comets rival drawings of Great Comets of the nineteenth century. Rather predictably the expected comet of the century Contents failed to materialise, however several of the other comets mentioned in the last issue, together with the Comet Section contacts 2 additional surprise shown above, put on good From the Director 2 appearances. 2011 L4 (PanSTARRS), 2012 F6 From the Secretary 3 (Lemmon), 2012 S1 (ISON) and 2013 R1 (Lovejoy) all Tales from the past 5 th became brighter than 6 magnitude and 2P/Encke, 2012 RAS meeting report 6 K5 (LINEAR), 2012 L2 (LINEAR), 2012 T5 (Bressi), Comet Section meeting report 9 2012 V2 (LINEAR), 2012 X1 (LINEAR), and 2013 V3 SPA meeting - Rob McNaught 13 (Nevski) were all binocular objects. Whether 2014 will Professional tales 14 bring such riches remains to be seen, but three comets The Legacy of Comet Hunters 16 are predicted to come within binocular range and we Project Alcock update 21 can hope for some new discoveries. We should get Review of observations 23 some spectacular close-up images of 67P/Churyumov- Prospects for 2014 44 Gerasimenko from the Rosetta spacecraft. BAA COMET SECTION NEWSLETTER 2 THE COMET’S TALE Comet Section contacts Director: Jonathan Shanklin, 11 City Road, CAMBRIDGE. CB1 1DP England. Phone: (+44) (0)1223 571250 (H) or (+44) (0)1223 221482 (W) Fax: (+44) (0)1223 221279 (W) E-Mail: [email protected] or [email protected] WWW page : http://www.ast.cam.ac.uk/~jds/ Assistant Director (Observations): Guy Hurst, 16 Westminster Close, Kempshott Rise, BASINGSTOKE, Hampshire. -
Investigating the Neutral Sodium Emissions Observed at Comets
Investigating the neutral sodium emissions observed at comets K. S. Birkett M.Sci. Physics, Imperial College London, UK (2012) Department of Space and Climate Physics University College London Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey. RH5 6NT. United Kingdom THESIS Submitted for the degree of Doctor of Philosophy, University College London 2017 2 I, Kimberley Si^anBirkett, confirm that the work presented in this thesis is my own. Where information has been derived from other sources, I confirm that this has been indicated in the thesis. 3 Abstract Neutral sodium emission is typically very easy to detect in comets, and has been seen to form a distinct neutral sodium tail at some comets. If the source of neutral cometary sodium could be determined, it would shed light on the composition of the comet, therefore allowing deeper understanding of the conditions present in the early solar system. Detection of neutral sodium emission at other solar system objects has also been used to infer chemical and physical processes that are difficult to measure directly. Neutral cometary sodium tails were first studied in depth at comet Hale-Bopp, but to date the source of neutral sodium in comets has not been determined. Many authors considered that orbital motion may be a significant factor in conclusively identifying the source of neutral sodium, so in this work details of the development of the first fully heliocentric distance and velocity dependent orbital model, known as COMPASS, are presented. COMPASS is then applied to a range of neutral sodium observations, includ- ing spectroscopic measurements at comet Hale-Bopp, wide field images of comet Hale- Bopp, and SOHO/LASCO observations of neutral sodium tails at near-Sun comets. -
The Astronomer Wilhelm Tempel
Further information by The Astronomer Wilhelm Tempel www.lutz-clausnitzer.de In the second half of the 19th century Wilhelm Tempel ranked among the most popular research scientists because of his many discoveries in astronomy. (Prof. Dr. Dieter B. Herrmann, astronomy historian, Berlin) Tempel's Discoveries Twelve comets, of which the following four are short period comets: 9P/Tempel 1, destination of Deep Impact 10P/Tempel 2 11P/Tempel-Swift-LINEAR 55P/Tempel-Tuttle, comet of the Leonids Five minor planets: (64) Angelina (65) Cybele Birth house in Niedercunnersdorf near Loebau, today Gartenweg 26 (74) Galatea Milestones of Tempel’s Life (81) Terpsichore (97) Clotho 1821 Born, grew up, went to school in Niedercun- nersdorf (Saxony, Germany) Many nebulae. His surveys of these laid the groundwork for future explanation. They are 1837 Began apprenticeship as a lithographer in Meißen 1840 Began work as a lithographer in North Europe now known to be gaseous nebulae (made of 1858 Purchased a telescope in Venice (Italy) and gas and dust), star clusters and distant galax- ies. His most spectacular discovery was the made first discoveries 1860 Worked as a lithographer and astronomer Merope Nebula (today NGC 1435) in the star cluster of the Pleiades. in Marseille (France) 1871 Teamed up with Schiaparelli, also an astro- nomer, in Milan (Italy) 1875 Became Director of the Royal Observatory From his Observing Logs Arcetri (Italy) until his death in 1889 Observatory Arcetri near Florence in the year 1872 Ernst Wilhelm Leberecht Tempel 1868 in Marseille with his telescope Honors The total eclipse on 18.July 1860 The moon crater Copernicus 1861 Paris Academy of the Sciences, Lalande Prize 1870 Two comet prizes from the Vienna Academy 1872 Knighted by Emperor Auguste Souverain of the Imperial Rose Order of Brazil A lithography of the Orion Nebula 1879 Humbertus Prize from the Academy in Rome 1881 Paris Academy of the sciences Valz Prize 1881 Received commendation as an Associate of the Royal Astronomical Society of London 1898 Moon crater “Tempel” named by J. -
DI Fact Sheet 5H.Id
FIRST LOOK INSIDE A COMET! http://deepimpact.jpl.nasa.gov http://deepimpact.umd.edu What’s deep inside a comet? Comets are time capsules that hold clues about the formation and evolution of the solar system. They are composed of ice, gas and dust, primitive debris from the solar system’s distant and coldest regions that formed 4.5 billion years ago. Deep Impact, a NASA Discovery Mission, is the first space mission to probe beneath the surface of a comet and reveal the secrets of its interior. On July 4, 2005, the Deep Impact spacecraft arrives at Comet Tempel 1 to impact it with a 370-kg (~820- lbs) mass. On impact, the crater produced is expected to range in size from that of a house to that of a football stadium, and two to fourteen stories deep. Scientists expect to see ice and dust debris ejected from the crater revealing fresh material beneath. A dramatic brightening caused by sunlight reflecting off the expelled material and the possible opening of a gas jet is anticipated. Images from cameras and a spectrometer are sent to Earth covering the approach, the impact and its aftermath. The effects of the collision with the comet will also be observable from certain locations on Earth and in some cases with smaller telescopes. The data is analyzed and combined with that from other missions, from telescopes around the world and in Earth orbit. These results will lead to a better understanding of both the solar system’s formation and implications of comets colliding with Earth. -
In This Issue: Rod’S Previous Book, the Urban Astronomer’S Guide Has Also Been Very Popular
The Rosette Gazette Volume 25,, IssueIssue 01 Newsletter of the Rose CityCity AstronomersAstronomers January, 2012 The Past, Present, and Future of the Schmidt Cassegrain Telescope by Rod Mollise “Uncle” Rod Mollise is familiar to amateur astronomers as the author of numerous books and magazine articles on every aspect of astronomy, amateur and professional. He is most well‐known, however, for his books on Schmidt Cassegrain Telescopes, SCTs, especially his latest one, Choosing and Using a New CAT (Springer), which has become the standard reference for these popular instruments. In This Issue: Rod’s previous book, The Urban Astronomer’s Guide has also been very popular. That’s no 1….General Meeting surprise, since it is designed to help the majority of amateurs who must observe from light polluted urban and suburban sites see deep sky wonders. 2….Special Interest Groups In addition to his books, Rod’s writing can be found in magazines including Sky and Telescope, Sky and Telescope’s SKYWATCH, Astronomy Technology Today, Amateur ……Observing Reports Astronomy Magazine, and others. Look for Unk Rod on numerous online forums, too, 3….Club Officers especially his popular blog, Uncle Rod’s Astro Blog. He is also one of the editors of the acclaimed online double star magazine, The University of South Alabama’s The Journal of …...Magazines Double Star Observations. …...RCA Library Rod Mollise is an engineer by profession, working on the U.S. Navy’s LPD Landing Ship 4….The Observers Corner program in Pascagoula, Mississippi, where he serves as the Combined Test Team’s Navigation Systems Engineer. Despite long 8.....Dawn Takes A Closer hours devoted to the new ships, he also finds time to teach Look astronomy to undergraduates at the University of South Alabama in 10...RCA Board Minutes Mobile. -
THE ASTEROIDS and THEIR DISCOVERERS Rock Legends
PAUL MURDIN THE ASTEROIDS AND THEIR DISCOVERERS Rock Legends The Asteroids and Their Discoverers More information about this series at http://www.springer.com/series/4097 Paul Murdin Rock Legends The Asteroids and Their Discoverers Paul Murdin Institute of Astronomy University of Cambridge Cambridge , UK Springer Praxis Books ISBN 978-3-319-31835-6 ISBN 978-3-319-31836-3 (eBook) DOI 10.1007/978-3-319-31836-3 Library of Congress Control Number: 2016938526 © Springer International Publishing Switzerland 2016 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifi cally the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfi lms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specifi c statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. The publisher, the authors and the editors are safe to assume that the advice and information in this book are believed to be true and accurate at the date of publication. Neither the publisher nor the authors or the editors give a warranty, express or implied, with respect to the material contained herein or for any errors or omissions that may have been made. Cover design: Frido at studio escalamar Printed on acid-free paper This Springer imprint is published by Springer Nature The registered company is Springer International Publishing AG Switzerland Acknowledgments I am grateful to Alan Fitzsimmons for taking and supplying the picture in Fig. -
Comet Kohoutek (NASA 990 Convair )
Madrid, UCM, Oct 27, 2017 Comets in UV Shustov B., Sachkov M., Savanov I. Comets – major part of minor body population of the Solar System There are a lot of comets in the Solar System. (Oort cloud contains cometary 4 bodies which total mass is ~ 5 ME , ~10 higher than mass of the Main Asteroid Belt). Comets keep dynamical, mineralogical, chemical, and structural information that is critically important for understanding origin and early evolution of the Solar System. Comets are considered as important objects in the aspect of space threats and resources. Comets are intrinsically different from one another (A’Hearn+1995). 2 General comments on UV observations of comets Observations in the UV range are very informative, because this range contains the majority of аstrophysically significant resonance lines of atoms (OI, CI, HI, etc.), molecules (CO, CO2, OH etc.), and their ions. UV background is relatively low. UV imaging and spectroscopy are both widely used. In order to solve most of the problems, the UV data needs to be complemented observations in other ranges including ground-based observations. 3 First UV observations of comets from space Instruments Feeding Resolu Spectral range Comets Found optics tion Orbiting Astronomical 4x200mm ~10 Å 1100-2000 Å Bennett OH (1657 Å) Observatory (OAO-2) ~20 Å 2000-4000 Å С/1969 Y1 OI (1304 Å) 2 scanning spectrophotometers Launched in 1968 Orbiting Geophysical ~100cm2 Bennett Lyman-α Observatory (OGO-5) С/1969 Y1 halo Launched in 1968 Aerobee sounding D=50mm ~1 Å 1100-1800 Å Tago- Lyman-α halo rocket Sato- wide-angle all-reflective Kosaka spectrograph С/1969 Y1 Launched in 1970 Skylab 3 space station D=75mm Kohoutek Huge Lyman- Launched in 1973 С/1969 Y1 α halo NASA 990 Convair D=300mm Kohoutek OH (3090Å) aircraft. -
SMCAS Events Continue Virtually …
The SAN MATEO COUNTY ASTRONOMICAL SOCIETY Sept. – Dec. • 2020 Issue 669th General Meeting: September 19 770th General Meeting: October 24 771st General Meeting: November 21 772nd General Meeting: December 19 Founded in 1960, the San Mateo County Astronomical Society is a 501(c)(3) non-profit organiza- SMCAS Events Continue tion for amateur astronomers and interested members of the Virtually … public. Visitors may attend Society meetings and lectures on the first Friday of each month, September to June, and Star Parties two Saturdays a month. All events are free for visitors and guests. Family memberships are offered at a nominal annual cost. Detailed membership information is found at http://www.smcasas- tro.com/membership.html where those who want can join via PayPal. Membership also includes access to our Event Horizon newsletter, discounted costs and subscriptions to calendars and magazines, monthly star parties of the Society and the College of San Mateo, use of loaner telescopes, field trips, social occasions and general meetings presenting guest speakers and programs. For additional information, please email us at [email protected] or call (650) See page 3 or page 5 for more details 678-2762. Membership forms are available NOTE: CSM is closed due to the pandemic. SMCAS near the end of this newsletter events are online until further notice. beginning on page 17. 1 Table of Contents From the Prez (President’s Corner)............................................................................ 3 Upcoming Events ....................................................................................................... 5 SMCAS Presentations Now in Conjunction with Star Parties................................... 5 CalStar 2020 ● September 17 to 20 ● Lake San Antonio Park ................................. 6 Solar System Rise and Set Times.............................................................................. -
A Model of the Physical Properties of Comet Encke
https://ntrs.nasa.gov/search.jsp?R=19730024004 2020-03-23T01:27:56+00:00Z NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Technical Report 32-1590 A Model of the Physical Properties of Comet Encke F. W, Taylor C. M. Michaux R, L Newburn, Jr. Hm 3- £r" JET PROPULSION LABORATORY CALIFORNIA INSTITUTE OF TECHNOLOGY PASADENA, CALIFORNIA October 1, 1973 NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Technical Report 32-1590 A Model of the Physical Properties of Comet Encke F. W. Taylor C. M. Michaux R. L. Newburn, Jr. JET PROPULSION LABORATORY CALIFORNIA INSTITUTE OF TECHNOLOGY PASADENA, CALIFORNIA October 1, 1973 Preface The work described in this report was performed by the Space Sciences Division of the Jet Propulsion Laboratory. Comet Encke is presently regarded as the likely target of NASA's first cometary mission, probably a slow flyby projected to take place in 1980. This document presents a model of Encke which is intended to be useful for the design of scientific experiments and spacecraft systems for such a mission. Data on the physical properties of comets are generally very sparse, and Encke is no exception. Much of the numerical information contained herein is, there- fore, based on calculations of a highly conjectural nature, and the results have large uncertainties associated with 'them. The user is cautioned that this is a model and not a specification, and must be treated as such if it is to be useful. The starting point for this work was an earlier study of Encke (Ref. 9) prepared by the TRW Systems Group under contract to JPL. -
Ice& Stone 2020
Ice & Stone 2020 WEEK 53: DECEMBER 27-31 Presented by The Earthrise Institute # 53 Authored by Alan Hale This week in history DECEMBER 27 28 29 30 31 1 2 DECEMBER 27, 1984: A team of American meteorite hunters finds the meteorite ALH 84001 in the Allan Hills region of Antarctica. This meteorite was found to have come from Mars, and in 1996 a team led by NASA scientist David McKay reported the presence of possible “microfossils” and other evidence of potential biological activity within it. This is the subject of a previous “Special Topics” presentation. DECEMBER 27, 2020: The main-belt asteroid (41) Daphne (around which a small moon, named Peneius, was discovered in 2008) will occult the 7th-magnitude star HD 49385 in Monoceros. The predicted path of the occultation crosses Oregon, the northern Pacific Ocean, the southern part of the island of Sakhalin, far southeastern Russia, far northeastern China, northern Mongolia, and east-central Kazakhstan. DECEMBER 27 28 29 30 31 1 2 DECEMBER 28, 1969: Amateur astronomer John Bennett in South Africa discovers the comet now known as Comet Bennett 1969i. Around the time of its perihelion passage in March 1970 it became a bright naked-eye comet and it is the first Great“ Comet” that I ever observed; it is a previous “Comet of the Week.” DECEMBER 28, 1973: Comet Kohoutek 1973f passes through perihelion at a heliocentric distance of 0.142 AU. Although it did not become the “Great Comet” that had been originally expected, it was nevertheless a moderately conspicuous naked-eye object and was an important comet scientifically. -
The Work of Max Ernst on Wilhelm Tempel
Tribute to an astronomer: the work of Max Ernst on Wilhelm Tempel Yaël Nazé (Research associate FNRS, ULg) Abstract: In 1964-1974, the German artist Max Ernst created, with the help of two friends, a series of works (books, movie, paintings) related to the astronomer Wilhelm Tempel. Mixing actual texts by Tempel and artistic features, this series pays homage to the astronomer by recalling his life and discoveries. Moreover, the core of the project, the book Maximiliana or the Illegal Practice of Astronomy , actually depicts the way science works, making this artwork a most original tribute to a scientist. 1. Art and the astronomer Amongst the many artworks related to astronomy, a subset is linked to astronomers themselves rather than celestial objects or theories (Soderlund 2010, Nazé 2015). These paintings or sculptures fall in two broad categories. The first comprises portraits intended to represent specific people. The likeness to the actual scientist depicted varies greatly from artwork to artwork. Some portraits bear a close resemblance to the person represented – usually, these are contemporaneous and the artist actually met the scientist (e.g. Galileo by Justus Sustermans in 1636). Others have only a remote resemblance to the model, which usually happens when portraits are made well after the subject’s death. For example, the famous School of Athens by Raphaël, despite being a masterpiece, cannot be considered to show the actual faces of Plato, Aristotle, or Archimedes. In this context, plain errors are sometimes made: the portrait by Ford Madox Brown of William Crabtree Observing the Transit of Venus , for example, displays a man of great age while Crabtree was only 29 at the time of the event! https://fr.wikipedia.org/wiki/L'Astronome_%28Vermeer%29#/media/File:VERMEER_ - _El_astr%C3%B3nomo_%28Museo_del_Louvre,_1688%29.jpg Figure 1: The astronomer (c.