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												  On the Origin and Evolution of the Material in 67P/Churyumov-GerasimenkoOn the Origin and Evolution of the Material in 67P/Churyumov-Gerasimenko Martin Rubin, Cécile Engrand, Colin Snodgrass, Paul Weissman, Kathrin Altwegg, Henner Busemann, Alessandro Morbidelli, Michael Mumma To cite this version: Martin Rubin, Cécile Engrand, Colin Snodgrass, Paul Weissman, Kathrin Altwegg, et al.. On the Origin and Evolution of the Material in 67P/Churyumov-Gerasimenko. Space Sci.Rev., 2020, 216 (5), pp.102. 10.1007/s11214-020-00718-2. hal-02911974 HAL Id: hal-02911974 https://hal.archives-ouvertes.fr/hal-02911974 Submitted on 9 Dec 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Space Sci Rev (2020) 216:102 https://doi.org/10.1007/s11214-020-00718-2 On the Origin and Evolution of the Material in 67P/Churyumov-Gerasimenko Martin Rubin1 · Cécile Engrand2 · Colin Snodgrass3 · Paul Weissman4 · Kathrin Altwegg1 · Henner Busemann5 · Alessandro Morbidelli6 · Michael Mumma7 Received: 9 September 2019 / Accepted: 3 July 2020 / Published online: 30 July 2020 © The Author(s) 2020 Abstract Primitive objects like comets hold important information on the material that formed our solar system. Several comets have been visited by spacecraft and many more have been observed through Earth- and space-based telescopes.
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												  ABCD the 4Th Quarter 2013 CatalogABCD springer.com The 4th quarter 2013 catalog Medicine springer.com Dentistry 2 T. Eliades, University of Zurich, Zurich, Switzerland; G. Eliades, Dentistry University of Athens, Athens, Greece (Eds.) Medicine Plastics in Dentistry and K. Rötzscher (Ed.) Estrogenicity J. Sadek, Dalhousie University, Halifax, Canada Forensic and Legal Dentistry A Guide to Safe Practice A Clinician’s Guide to ADHD This book provides a timely and comprehensive This book both explains in detail diverse aspects of review of our current knowledge of BPA release from The Clinician’s Guide to ADHD combines the use- the law as it relates to dentistry and examines key dental polymers and the potential endocrinologi- ful diagnostic and treatment approaches advocated issues in forensic odontostomatology. A central aim cal consequences. After a review of the history and in different guidelines with insights from other is to enable the dentist to achieve a realistic assess- evolution of the issue within the broader biomedical sources, including recent literature reviews and web ment of the legal situation and to reduce uncer- context, the estrogenicity of BPA is explained. The resources. The aim is to provide clinicians with clear, tainties and liability risk. To this end, experts from basic chemistry of the polymers used in dentistry is concise, and reliable advice on how to approach this across the world discuss the dental law in their own then presented in a simplified and clinically relevant complex disorder. The guidelines referred to in com- countries, covering both civil and criminal law and manner. Key chapters in the book carefully evaluate piling the book derive from authoritative sources in highlighting key aspects such as patient rights, insur- the release of BPA from polycarbonate products and different regions of the world, including the United ance, and compensation.
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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 Brightness1 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.
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												  Mission to Catch Comet ISONMission to Catch Comet ISON Andrew Cheng (JHU/APL; [email protected]) Steve Arnold (JHU/APL) Pietro Bernasconi (JHU/APL) Karl Hibbitts (JHU/APL) Eliot Young (SwRI) Tibor Kremic (GRC) Comet ISON . Comet ISON discovered September, 2012 An Oort Cloud comet believed to be making its first apparition . ISON perihelion in November, 2013 A sun-grazer which may not survive perihelion passage intact Observe the comet before perihelion . An important target of opportunity To study volatile-rich material from the epoch of planet formation To learn how comets work 26 May 2013 2 Oort Cloud Comets • Provide clues to the origins of the Solar System • Consist of pris8ne, icy material that was never heated in the inner solar system In late 2013, ISON may become the brightest Oort Cloud comet to appear in decades Comet Ikeya-Seki, sun-grazer of 1965 Comet McNaught in 2007 26 May 2013 3 Comet ISON Observability • Comet ISON is observable from the Northern Hemisphere, with solar elongaon >40°, from September 15, 2013 through Nov 12, 2013 • ISON becomes steadily brighter through this period • ISON may remain spectacularly bright aer December, 2013 Vitali Nevski and Artyom Novichonok, discoverers (space.com) 26 May 2013 4 Comet ISON Brightness . Observations are consistent with V~12 at time of BRRISON flight . Due to small solar elongation, additional observations BRRISON flight prior to flight are not expected CIOC web site, sungrazer.nrl.navy.mil 12 June 2013 BRRISON Project Review 3 5 What is BRRISON? . BRRISON = Balloon Rapid Response for the comet ISON Goal is to observe the comet ISON from a balloon platform Leverages the balloon study concepts Coordinate the science measurements with the greater scientific community, including ground and space observations 12 months from comet discovery to mission .
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												  Early Observations of the Interstellar Comet 2I/Borisovgeosciences Article Early Observations of the Interstellar Comet 2I/Borisov Chien-Hsiu Lee NSF’s National Optical-Infrared Astronomy Research Laboratory, Tucson, AZ 85719, USA; [email protected]; Tel.: +1-520-318-8368 Received: 26 November 2019; Accepted: 11 December 2019; Published: 17 December 2019 Abstract: 2I/Borisov is the second ever interstellar object (ISO). It is very different from the first ISO ’Oumuamua by showing cometary activities, and hence provides a unique opportunity to study comets that are formed around other stars. Here we present early imaging and spectroscopic follow-ups to study its properties, which reveal an (up to) 5.9 km comet with an extended coma and a short tail. Our spectroscopic data do not reveal any emission lines between 4000–9000 Angstrom; nevertheless, we are able to put an upper limit on the flux of the C2 emission line, suggesting modest cometary activities at early epochs. These properties are similar to comets in the solar system, and suggest that 2I/Borisov—while from another star—is not too different from its solar siblings. Keywords: comets: general; comets: individual (2I/Borisov); solar system: formation 1. Introduction 2I/Borisov was first seen by Gennady Borisov on 30 August 2019. As more observations were conducted in the next few days, there was growing evidence that this might be an interstellar object (ISO), especially its large orbital eccentricity. However, the first astrometric measurements do not have enough timespan and are not of same quality, hence the high eccentricity is yet to be confirmed. This had all changed by 11 September; where more than 100 astrometric measurements over 12 days, Ref [1] pinned down the orbit elements of 2I/Borisov, with an eccentricity of 3.15 ± 0.13, hence confirming the interstellar nature.
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												  How We Found About COMETSHow we found about COMETS Isaac Asimov Isaac Asimov is a master storyteller, one of the world’s greatest writers of science fiction. He is also a noted expert on the history of scientific development, with a gift for explaining the wonders of science to non- experts, both young and old. These stories are science-facts, but just as readable as science fiction.Before we found out about comets, the superstitious thought they were signs of bad times ahead. The ancient Greeks called comets “aster kometes” meaning hairy stars. Even to the modern day astronomer, these nomads of the solar system remain a puzzle. Isaac Asimov makes a difficult subject understandable and enjoyable to read. 1. The hairy stars Human beings have been watching the sky at night for many thousands of years because it is so beautiful. For one thing, there are thousands of stars scattered over the sky, some brighter than others. These stars make a pattern that is the same night after night and that slowly turns in a smooth and regular way. There is the Moon, which does not seem a mere dot of light like the stars, but a larger body. Sometimes it is a perfect circle of light but at other times it is a different shape—a half circle or a curved crescent. It moves against the stars from night to night. One midnight, it could be near a particular star, and the next midnight, quite far away from that star. There are also visible 5 star-like objects that are brighter than the stars.
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												  Make a Comet Materials: Students Should First Line Their Mixing Bowls with Trash BagsBuild Your Own Comet Prep Time: 30 minutes Grades: 6-8 Lesson Time: 55 minutes Essential Questions: • What is a comet composed of? • What gives a comet its tail? • What makes a comet different from other Near-Earth Objects (NEOs)? Objectives: • Create a physical representation of a comet and its properties. • Observe distinguishable factors between comets and other NEOs. Standards: • MS – PS1-4: Develop a model that predicts and describes changes in particle motion, temperature, and state of a pure substance when thermal energy is added or removed. • CCSS.ELA-LITERACY.RST.6-8.3 - Follow precisely a multistep procedure when carrying out experiments, taking measurements, or performing technical tasks. Teacher Prep: • Materials per comet: o 5 lbs. dry ice, ice chest, paper cups, towels, small container (for scooping), wooden or plastic mixing spoon, trash bag, mixing bowl, heavy work gloves, 1 tablespoon or less of starch, 1 tablespoon or less of dark corn syrup (or soda), 1 tablespoon or less of vinegar, 1 tablespoon or less of rubbing alcohol, large beaker, water, 1 c dirt/sand, 1 L of water. • Additional materials: o Hammer or mallet, paper cups, towels, flashlight, hair dryer. • Most of the dry ice needs to be in a fine powder before the students arrive, so use the hammer to do this ahead of time. There should be about 50-60% fine powder in order to hold the comet together. It is best to separate the dry ice ahead of time with towels. • This can also be done as a class demonstration. Teacher Notes/Background: • This lesson was adapted from NASA’s Make Your Own Comet activity.
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												  The Professor Comet's Report Early Spring – April 2012The Professor Comet’s Report 1 Mr. Justin J McCollum (BS, MS Physics) Lab Physics Coordinator Dept. of Physics Lamar University Welcome to the comet report which is a monthly article on the observations of comets by the amateur astronomy community and comet hunters from around the world! This C/2009 P1 Garradd with article is dedicated to the latest reports of available comets for Barred Spiral Galaxy NGC 4236 observations, current state of those comets, future 14 March 2011! predictions, & projections for observations in comet astronomy! Early Spring – April 2012 The Professor Comet’s Report 2 The Current Status of the Predominant Comets for Apr 2012! Comets Designation Orbital Magnitude Trend Observation Constellations Visibility (IAU – MPC) Status Visual (Range in (Night Sky Location) Period Lat.) Garradd 2009 P1 C 7.0* - 7.5 Fading 90°N – 30°S SW region of Ursa Major moving All Night SSW towards the SE region of Lynx. Giacobini - 21P P 9 – 10 Fading Poor N/A Zinner Elongation Lost in the daytime Glare! LINEAR 2011 F1 C 11 .7* Brightening 90°N – 20°S Undergoing retrograde motion All Night between Boötes and Draco thru the late Spring. Gehrels 2 78P P 12.2* Fading 60˚N - 20˚S Moving eastwards across Taurus Early Evening and progressing along the N edge of the Hyades Star Cluster! McNaught 2011 Q2 C 12.5 Fading 70˚N – Eqn. Currently in the S central region Early Morning of Andromeda moving NE between the boundary between Andromeda & Pisces. NEAT 246P/2010 V2 P 12.3* - 13 Possible 65˚N - 60˚S Undergoing retrograde motion All Night Steadiness in the E half of the N central region of Virgo until late June.
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												  Comet Section Observing GuideComet Section Observing Guide 1 The British Astronomical Association Comet Section www.britastro.org/comet BAA Comet Section Observing Guide Front cover image: C/1995 O1 (Hale-Bopp) by Geoffrey Johnstone on 1997 April 10. Back cover image: C/2011 W3 (Lovejoy) by Lester Barnes on 2011 December 23. © The British Astronomical Association 2018 2018 December (rev 4) 2 CONTENTS 1 Foreword .................................................................................................................................. 6 2 An introduction to comets ......................................................................................................... 7 2.1 Anatomy and origins ............................................................................................................................ 7 2.2 Naming .............................................................................................................................................. 12 2.3 Comet orbits ...................................................................................................................................... 13 2.4 Orbit evolution .................................................................................................................................... 15 2.5 Magnitudes ........................................................................................................................................ 18 3 Basic visual observation ........................................................................................................
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												  The Comet's TaleTHE 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.
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												  Small Bodies of the Solar System Don Yeomansnews and views teakre Small bodies of the Solar System Don Yeomans ,-.......-..-.- "_.."..._..".."....".._..I........... ".........._ "_.""".." ".......... " "............_..._.." ....".."-..- ..-.... "....""... Discoveries of comets that behave like asteroids and asteroids that behave like comets are making us reassess our view of Earth's smallest neighbours. cientists have a strong urge to place Mother Nature's objects into neat Sboxes. For most of the past halfcentury, the comets and asteroids of the Solar System did seem to belong in two separate popula- tions -each within their own box. The rules werethatcomets,withawiderangeoforbits, were solid, dirty iceballs originating in the so-called Oort cloud at theedge of the Solar System. Asteroids were definedas bitsofrock anfimed mostly to a region between Mars and Jupiter and travelling roughly in the same plane and inthe same direction as the planets about theSun (Fig. 1).Fromtjme to Lime over the past 50 years, objects were bund that did not really belong in either )OX, but they were onlyconsidered as occa- iional exceptions to the rules. Within the Figure 1 The usual view of corneta and utcroida. The inna Soh System cuntlinr the Sun and the ,ast few years, however,Mother Nature has four terreatrid planar:Mercury, Venu%Euth and Ma.fie lump of mdc that make up thenuin ticked over the boxes entirely, spilling the asteroid bdt between him and Jupiterorbit the Sun in the meplane andthe medirection PJ the :ontents and demanding thatscientists rec- planets. Most tometa have highly dlipticnl orbits, whichmeans they spend most of their timein the )gnizE crossover objects - asteroids that outer reache of the Solar System with only briefpasages dose to the Sun.
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												  Initial Characterization of Interstellar Comet 2I/BorisovInitial characterization of interstellar comet 2I/Borisov Piotr Guzik1*, Michał Drahus1*, Krzysztof Rusek2, Wacław Waniak1, Giacomo Cannizzaro3,4, Inés Pastor-Marazuela5,6 1 Astronomical Observatory, Jagiellonian University, Kraków, Poland 2 AGH University of Science and Technology, Kraków, Poland 3 SRON, Netherlands Institute for Space Research, Utrecht, the Netherlands 4 Department of Astrophysics/IMAPP, Radboud University, Nijmegen, the Netherlands 5 Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, the Netherlands 6 ASTRON, Netherlands Institute for Radio Astronomy, Dwingeloo, the Netherlands * These authors contributed equally to this work; email: [email protected], [email protected] Interstellar comets penetrating through the Solar System had been anticipated for decades1,2. The discovery of asteroidal-looking ‘Oumuamua3,4 was thus a huge surprise and a puzzle. Furthermore, the physical properties of the ‘first scout’ turned out to be impossible to reconcile with Solar System objects4–6, challenging our view of interstellar minor bodies7,8. Here, we report the identification and early characterization of a new interstellar object, which has an evidently cometary appearance. The body was discovered by Gennady Borisov on 30 August 2019 UT and subsequently identified as hyperbolic by our data mining code in publicly available astrometric data. The initial orbital solution implies a very high hyperbolic excess speed of ~32 km s−1, consistent with ‘Oumuamua9 and theoretical predictions2,7. Images taken on 10 and 13 September 2019 UT with the William Herschel Telescope and Gemini North Telescope show an extended coma and a faint, broad tail. We measure a slightly reddish colour with a g′–r′ colour index of 0.66 ± 0.01 mag, compatible with Solar System comets.