Monthly Newsletter of the Durban Centre - May 2018
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The Comet's Tale, and Therefore the Object As a Whole Would the Section Director Nick James Highlighted Have a Low Surface Brightness
1 Diebold Schilling, Disaster in connection with two comets sighted in 1456, Lucerne Chronicle, 1513 (Wikimedia Commons) THE COMET’S TALE Comet Section – British Astronomical Association Journal – Number 38 2019 June britastro.org/comet Evolution of the comet C/2016 R2 (PANSTARRS) along a total of ten days on January 2018. Composition of pictures taken with a zoom lens from Teide Observatory in Canary Islands. J.J Chambó Bris 2 Table of Contents Contents Author Page 1 Director’s Welcome Nick James 3 Section Director 2 Melvyn Taylor’s Alex Pratt 6 Observations of Comet C/1995 01 (Hale-Bopp) 3 The Enigma of Neil Norman 9 Comet Encke 4 Setting up the David Swan 14 C*Hyperstar for Imaging Comets 5 Comet Software Owen Brazell 19 6 Pro-Am José Joaquín Chambó Bris 25 Astrophotography of Comets 7 Elizabeth Roemer: A Denis Buczynski 28 Consummate Comet Section Secretary Observer 8 Historical Cometary Amar A Sharma 37 Observations in India: Part 2 – Mughal Empire 16th and 17th Century 9 Dr Reginald Denis Buczynski 42 Waterfield and His Section Secretary Medals 10 Contacts 45 Picture Gallery Please note that copyright 46 of all images belongs with the Observer 3 1 From the Director – Nick James I hope you enjoy reading this issue of the We have had a couple of relatively bright Comet’s Tale. Many thanks to Janice but diffuse comets through the winter and McClean for editing this issue and to Denis there are plenty of images of Buczynski for soliciting contributions. 46P/Wirtanen and C/2018 Y1 (Iwamoto) Thanks also to the section committee for in our archive. -
The State of Anthro–Earth
The Rosette Gazette Volume 22,, IssueIssue 7 Newsletter of the Rose City Astronomers July, 2010 RCA JULY 19 GENERAL MEETING The State Of Anthro–Earth THE STATE OF ANTHRO-EARTH: A Visitor From Far, Far Away Reviews the Status of Our Planet In This Issue: A Talk (in Earth-English) By Richard Brenne 1….General Meeting Enrico Fermi famously wondered why we hadn't heard from any other planetary 2….Club Officers civilizations, and Richard Brenne, who we'd always suspected was probably from another planet, thinks he might know the answer. Carl Sagan thought it was likely …...Magazines because those on other planets blew themselves up with nuclear weapons, but Richard …...RCA Library thinks its more likely that burning fossil fuels changed the climates and collapsed the 3….Local Happenings civilizations of those we might otherwise have heard from. Only someone from another planet could discuss this most serious topic with Richard's trademark humor 4…. Telescope (in a previous life he was an award-winning screenwriter - on which planet we're not Transformation sure) and bemused detachment. 5….Special Interest Groups Richard Brenne teaches a NASA-sponsored Global Climate Change class, serves on 6….Star Party Scene the American Meteorological Society's Committee to Communicate Climate Change, has written and produced documentaries about climate change since 1992, and has 7.…Observers Corner produced and moderated 50 hours of panel discussions about climate change with 18...RCA Board Minutes many of the world's top climate change scientists. Richard writes for the blog "Climate Progress" and his forthcoming book is titled "Anthro-Earth", his new name 20...Calendars for his adopted planet. -
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. -
The Planetary Report) Watching As a Bust
The Board of Dlrec:tolll The naming of comets can, indeed, be a very difficult matter. Traditionally these small, CARL SAGAN BRUCE MURRAY President Vice President icy solar system bodies were named for their discoverers. But because some people are Director" Laboratory Professor of Planetary very persistent (for example, there are four Comets Meier) a particular name is needed for Planetary Studies. Science, California Camell University Institute of Technology for each individu.al comet. Thus, at discovery a comet is assigned a letter designation LOUIS FRIEDMAN HENRY TANNER based on the order of discovery or recovery in a certain year. So, Comet 1982i was the Executive Director Corporate Secretary and 9th comet found in 1982. Later, comets are assigned new names based on their peri Assistant Treasurer, Cafifom;a THOMAS O. PAINE Institute of Technology helion (closest approach to the Sun). 1984 XXll1 was the 23rd comet to pass perihelion Former Administrator. NASA: Chairman, National JOSEPH RYAN in 1984. Confused? Here is a poetic attempt to explain. Commission on Space O'Melveny & Myers Board of Advlsolll DIANE ACKERMAN GARRY E. HUNT poet and author Space -Scientist, THE NAMING OF COMETS (With apologies to T. S. Eliot) United Kingdom ISAAC ASIMOV aulhor HANS MARK BY DAVID H. LEW Chancellor, RICHARD BERENDZEN University of Texas System Presid8nt, American University JAMES MICHENER The naming of Comets is a difficult matter, JACQUES BLAMONT author Chief Scien#st, Centre National It isn't just one of your holiday games; d'Etudes Spatlales, France PHILIP MORRISON Institute Professor, You may think at first I'm mad as a hatter RAY BRADBURY Massachusetts poet and author Institute of Technofogy When I tell you, a comet has THREE DIFFERENT NAMES. -
Ionic Emissions in Comet C/2016 R2 (Pan-STARRS)
MNRAS 000,1–12 (2019) Preprint 23 April 2020 Compiled using MNRAS LATEX style file v3.0 Ionic emissions in comet C/2016 R2 (Pan-STARRS) Kumar Venkataramani1;2? Shashikiran Ganesh1 and Kiran S.Baliyan1 1 Astronomy & Astrophysics Division, Physical Research Laboratory, Ahmedabad, India. 2 Department of Physics, Leach Science Center, Auburn University, Auburn, AL, USA. 23 April 2020 ABSTRACT We carried out observations of a peculiar comet, C/2016 R2 (Pan-STARRS), using a low resolution spectrograph mounted on the 1.2m telescope at Mount Abu Infrared Observatory, India. The comet was observed on two dates in January 2018, when it was at a heliocentric distance of 2.8 AU. Study based on our observations revealed that the optical spectrum of this comet is quite unusual as compared to general cometary spectra. Most of the major cometary emissions like C2,C3 and CN were absent in comet C/2016 R2. However, the comet spectrum + + showed very strong emission bands from ionic species like CO and N2 . A mean N2/CO ratio of 0.09 ± 0.02 was derived from the spectra and an extremely low depletion factor of 1.6 ± 0.4 has been estimated for this ratio as compared to the solar nebula. We have also detected minor + + emission features beyond 5400 Å, albeit marginally. The column densities of CO and N2 were calculated from their emission bands. The optical spectrum suggests that the cometary ice is dominated by CO. The low depletion factor of N2/CO ratio in this comet, as compared to the solar nebula and the unusual spectrum of the comet are consequences of distinctive processing at the location of its formation in the early solar nebula. -
UNIVERSITY of HAWAII at MANOA Institute for Astrononmy Pan-STARRS Project Management System
Pan-STARRS Document Control PSDC-xxx-xxx-00 UNIVERSITY OF HAWAII AT MANOA Institute for Astrononmy Pan-STARRS Project Management System Appearance of and response to interesting and rare objects discovered by MOPS Richard J. Wainscoat Pan-STARRS Solar System Group Institute for Astronomy October 28, 2006 c Institute for Astronomy 2680 Woodlawn Drive, Honolulu, Hawaii 96822 An Equal Opportunity/Affirmative Action Institution Pan-STARRS Moving Object Processing System PSDC-xxx-xxx-00 Revision History Revision Number Release Date Description 00 2006.10.20 First draft Interesting and rare objects—definition and followup ii October 28, 2006 Pan-STARRS Moving Object Processing System PSDC-xxx-xxx-00 TBD / TBR Listing Section No. Page No. TBD/R No. Description Interesting and rare objects—definition and followup iii October 28, 2006 Contents 1 Overview 1 2 Referenced Documents 1 3 Facilities available for followup observations 1 4 Fuzzy objects—comets or outgassing asteroids 2 4.1 Introduction .................................................. 2 4.2 Signature ................................................... 2 4.3 Response ................................................... 2 4.4 Followup ................................................... 2 4.5 Naming of Comets discovered by Pan-STARRS ............................... 3 5 Objects with high inclination, retrograde, or highly eccentric orbits 3 5.1 Introduction .................................................. 3 5.2 Signature ................................................... 3 5.3 Response .................................................. -
January 12-18, 2020
3# Ice & Stone 2020 Week 3: January 12-18, 2020 Presented by The Earthrise Institute This week in history JANUARY 12 13 14 15 16 17 18 JANUARY 12, 1910: A group of diamond miners in the Transvaal in South Africa spot a brilliant comet low in the predawn sky. This was the first sighting of what became known as the “Daylight Comet of 1910” (old style designations 1910a and 1910 I, new style designation C/1910 A1). It soon became one of the brightest comets of the entire 20th Century and will be featured as “Comet of the Week” in two weeks. JANUARY 12, 2005: NASA’S Deep Impact mission is launched from Cape Canaveral, Florida. Deep Impact would encounter Comet 9P/Tempel 1 in July of that year and – under the mission name “EPOXI” – would encounter Comet 103P/Hartley 2 in November 2010. Comet 9P/Tempel 1 is a future “Comet of the Week” and the Deep Impact mission – and its results – will be discussed in more detail at that time. JANUARY 12, 2007: Comet McNaught C/2006 P1, the brightest comet thus far of the 21st Century, passes through perihelion at a heliocentric distance of 0.171 AU. Comet McNaught is this week’s “Comet of the Week.” JANUARY 12 13 14 15 16 17 18 JANUARY 13, 1950: Jan Oort’s paper “The Structure of the Cloud of Comets Surrounding the Solar System, and a Hypothesis Concerning its Origin,” is published in the Bulletin of the Astronomical Institute of The Netherlands. In this paper Oort demonstrates that his calculations reveal the existence of a large population of comets enshrouding the solar system at heliocentric distances of tens of thousands of Astronomical Units. -
Colours of Minor Bodies in the Outer Solar System II - a Statistical Analysis, Revisited
Astronomy & Astrophysics manuscript no. MBOSS2 c ESO 2012 April 26, 2012 Colours of Minor Bodies in the Outer Solar System II - A Statistical Analysis, Revisited O. R. Hainaut1, H. Boehnhardt2, and S. Protopapa3 1 European Southern Observatory (ESO), Karl Schwarzschild Straße, 85 748 Garching bei M¨unchen, Germany e-mail: [email protected] 2 Max-Planck-Institut f¨ur Sonnensystemforschung, Max-Planck Straße 2, 37 191 Katlenburg- Lindau, Germany 3 Department of Astronomy, University of Maryland, College Park, MD 20 742-2421, USA Received —; accepted — ABSTRACT We present an update of the visible and near-infrared colour database of Minor Bodies in the outer Solar System (MBOSSes), now including over 2000 measurement epochs of 555 objects, extracted from 100 articles. The list is fairly complete as of December 2011. The database is now large enough that dataset with a high dispersion can be safely identified and rejected from the analysis. The method used is safe for individual outliers. Most of the rejected papers were from the early days of MBOSS photometry. The individual measurements were combined so not to include possible rotational artefacts. The spectral gradient over the visible range is derived from the colours, as well as the R absolute magnitude M(1, 1). The average colours, absolute magnitude, spectral gradient are listed for each object, as well as their physico-dynamical classes using a classification adapted from Gladman et al., 2008. Colour-colour diagrams, histograms and various other plots are presented to illustrate and in- vestigate class characteristics and trends with other parameters, whose significance are evaluated using standard statistical tests. -
Kohoutek Is Coming! New York, New York September I0, 1973
INSTITUTE OF CURRENT rORLD AFFAIRS ATW-20 Kohoutek Is Coming! New York, New York September I0, 1973 Mr. Richard H. Nolte Institute of Current World Affairs 535 Fifth Avenue New York, New York 10017 Dear Mr. Nolte: Our planet earth is about to be visited by a ghost. The name of the visitor is "1973f" or "Kohoutek," and it is a great comet, perhaps the greatest of the century. Comets have been called the ghosts of the solar system because they are so insubstantial relative to their size and brightness. Percival Lowell called them "bagfuls of nothing," and, in fact, their most eye- catching features great tails of enormous length and brilliance seem to be nothing more than tenuous streamers of gas excited to lumin- escence by the radiation of the sun. The great comet now rushing at us from the far corners of space was discovered on March 7th of this year by Dr. Lubo Kohoutek of the Hamburg Observatory in Bergedorf, West Germany. It showed up on a photo- graphic plate as a faint, diffuse object with no tail in the constel- lation of Hydra. Subsequent observations made possible the calculation of the orbit of this body. We now know that it will reach perihelion, its closest approach to the un, on December 24th, and it should be spectacu- larly visible to the naked eye for about six weeks before and after that date. The word "comet" comes from the Greek "hairy star." Comets are members of the solar system. Like planets they revolve in orbits around the sun. -
The Planetary Report
The On the Cover: Volume XVIII Deer fihd repose in a bucolic alpine meadow nestled in Olympic Table of National Park. But such scenes of seeming security and timeless Number 3 ness are illusory-as the dinosaurs discovered 65 million years May/June 1998 ago when.a comet or asteroid impact wiped them out Earth Contents resides in a swarm of smaller bodies, many with the potential to wreak havoc on civilization. We have discovered about 10 percent of the near-Earth objects, but one of th e many unknown objects may at any time appear and pass through our ne ighborhood- Features as did comet Hyakutake just last year. Such as-yet -undiscovered Opinion: co mets may pose the greatest danger to life as we know it. 4 The Green Space Project Deer photo: J. Lotter, Tom Stack & Associates To many of us, an alliance of our forces with those ofthe environmental movement has Comet Hyakutake: Johnny Horne seemed a natural thing to create. But not everyone feels that way. Noted science fiction author and Planetary Society member Kim Stanley Robinson explores this dilemma. 6 Deep Space 1: FroID Exploration Technology for the 21 st Century "Faster, better, cheaper" is the new and unofficial motto of NASA. The agency's New The Millennium program is soon to test the effectiveness of that motto in guiding technology Editor development with the launch of Deep Space 1. 9 The Mars Rock: SOlne of Its Chelnistry Is Froln Earth t may not be explicit, but there is a theme In August 1996 the announcement that scientists from NASA and Stanford University had I running through this issue: life on Earth found possible traces of ancient life on Mars touched off a flurry of experimentation and and its relationship to chunks of ice and controversy. -
Dust in Comet 103P/Hartley 2 Coma During EPOXI Mission Q ⇑ E
Icarus 222 (2013) 774–785 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Dust in Comet 103P/Hartley 2 coma during EPOXI mission q ⇑ E. Hadamcik a, , A.K. Sen b, A.C. Levasseur-Regourd c, R. Gupta d, J. Lasue e, R. Botet f a UPMC (U. P. & M. Curie, Sorbonne Universités), LATMOS/CNRS, 11 Bld d’Alembert, 78280 Guyancourt, France b Assam Univ., Silchar 788 001, India c UPMC (U. P. & M. Curie, Sorbonne Universités), LATMOS/CNRS, 4 Place Jussieu, 75005 Paris, France d IUCAA, Post Bag 4, Ganeshkhind, 411007 Pune, India e Univ. de Toulouse, UPS-OMP, IRAP, BP 44346, 31028 Toulouse, France f Univ. Paris-Sud, LPS/CNRS, Bat. 510, 91405 Orsay, France article info abstract Article history: The Deep Impact spacecraft flew by Comet 103P/Hartley 2 on 4 November 2010 (EPOXI mission). In situ Available online 16 July 2012 observations are complemented by a systematic ground- and space-based observation campaign. In the present work, imaging polarimetry is used to emphasize different dust regions in the coma and follow Keywords: their evolution over a period including the EPOXI fly-by. Comets, Dust On the intensity images, the coma is asymmetric with an important tailward feature. Jets in the sun- Comets, Coma ward direction are observed to present an extension that depends on the nucleus phase. The azimuthal Polarimetry integrated intensity presents a nominal radial decrease (À1 in log–log scale) for optocentric distances lar- ger than a few hundred kilometers. Through cometary continuum narrow band filters, the aperture polar- ization decreases with the optocentric distance. -
Kudo-Fujikawa\), C/2002 V1 \(NEAT\
A&A 528, A142 (2011) Astronomy DOI: 10.1051/0004-6361/201016250 & c ESO 2011 Astrophysics Molecular investigations of comets C/2002 X5 (Kudo-Fujikawa), C/2002 V1 (NEAT), and C/2006 P1 (McNaught) at small heliocentric distances N. Biver1, D. Bockelée-Morvan1, P. Colom1, J. Crovisier1, G. Paubert2,A.Weiss3, and H. Wiesemeyer3 1 LESIA, CNRS UMR 8109, UPMC, Université Paris-Diderot, Observatoire de Paris, 5 pl. Jules Janssen, 92195 Meudon, France e-mail: [email protected] 2 IRAM, Avd. Divina Pastora, 7, 18012 Granada, Spain 3 Max Planck Institute for Radio Astronomy, PO Box 20 24, 53010 Bonn, Germany Received 2 December 2010 / Accepted 14 January 2011 ABSTRACT We present unique spectroscopic radio observations of comets C/2002 X5 (Kudo-Fujikawa), C/2002 V1 (NEAT), and C/2006 P1 (McNaught), which came within rh ≈ 0.2 AU of the Sun in 2003 and 2007. The molecules OH, HCN, HNC, CS, and CH3OH + were detected in each of these comets when they were exposed to strong heating from the Sun. HC3NandHCO were detected in comets C/2002 X5 and C/2006 P1, respectively. We show that in these very productive comets close to the Sun screening of the photodissociation by the Sun UV radiation plays a non-negligible role. Acceleration of the gas expansion velocity and day-night −5 −1 asymmetry is also measured and modeled. The CS photodissociation lifetime was constrained to be about 2.5 × 10 s at rh = 1AU. The relative abundances are compared to values determined from more distant observations of C/2002 X5 or other comets.