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On the Origin and Evolution of the Material in 67P/Churyumov-Gerasimenko
On 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. -
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. -
October 2017 BRAS Newsletter
October 2017 Issue Next Meeting: Monday, October 9th at 7PM at HRPO nd (2 Mondays, Highland Road Park Observatory) October Program: BRAS President John Nagle will. reveal how he researches and puts together his Observing Notes column for our newsletter each. month. What's In This Issue? HRPO’s Great American Eclipse Event Summary (Page 2) President’s Message Secretary's Summary Outreach Report - FAE Light Pollution Committee Report Recent Forum Entries 20/20 Vision Campaign Messages from the HRPO Spooky Spectrum Observe The Moon Night Natural Sky Conference HRPO 20th Anniversary Observing Notes – Phoenix & Mythology Like this newsletter? See past issues back to 2009 at http://brastro.org/newsletters.html Newsletter of the Baton Rouge Astronomical Society October 2017 President’s Message The first Sidewalk Astronomy of the season was a success. We had a good time, and About 100 people (adult and children) attended. Ben Toman live streamed on the BRAS Facebook page. See his description in this newsletter. A copy of the proposed, revised By-Laws should be in your mail soon. Read through them, and any proposed changes need to be communicated to me before the November meeting. Wally Pursell (who wrote the original and changed by-laws) and I worked last year on getting the By-Laws updated to the current BRAS policies, and we hope the revised By-Laws will need no revisions for a long time. We need more Globe at Night observations – we are behind in the observations compared to last year at this time. We also need observations of variable stars to help in a school project by a new BRAS member, Shreya. -
Comet Section Observing Guide
Comet 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 ........................................................................................................ -
Polarimetry of Comets: Observational Results and Problems
POLARIMETRY OF COMETS: OBSERVATIONAL RESULTS AND PROBLEMS N. Kiselev & V. Rosenbush Main Astronomical Observatory of National Academy of Sciences of Ukraine 1st WG meeting in Warsaw, Poland, 7-9 May 2012 Outline of presentation Linear polarization of comets. Problems with the interpretation of diversity in the maximum polarization of comets. Circular polarization of comets. Next task Polarimetric data for comets up to the mid 1970s (Kiselev, 1981; Dobrovolsky et al.,1986) The polarization of molecular emissions was explained as being due to resonance fluorescence (Öhman, 1941; Le Borgne et al., 1986) 2 P90 sin P() 2 , where P90 = 0.077 1 P90 cos Curve (2) is polarization phase dependence for the resonance fluorescence according to Öhman’s formula. Curve (1) is a fit of polarization data in continuum according to Öhman’s formula. There are no observations of comets at phase angles smaller than 40 until 1975. Open questions: •What is polarization phase curve for dust near opposition ? •What is the maximum of polarization? •Is there a diversity in comet polarization? Comets: negative polarization branch Discovery of the NPB gave impetus to development of new optical mechanisms Observations of comet West to explain its origin. Among them, the revealed a negative branch of scattering of light by particles with aggregate structure. linear polarization at phase angles 22. (Kiselev&Chernova, 1976) Phase angle dependence of polarization for comets in the blue and red continuum (Kiselev, 2003) The observed difference in the All comets polarization of the two groups of comets is apparent. Why is this? There are three points of view: •The polarization of each comet is an individual (Perrin&Lamy, 1986). -
The Composition of Cometary Volatiles 391
Bockelée-Morvan et al.: The Composition of Cometary Volatiles 391 The Composition of Cometary Volatiles D. Bockelée-Morvan and J. Crovisier Observatoire de Paris M. J. Mumma NASA Goddard Space Flight Center H. A. Weaver The Johns Hopkins University Applied Physics Laboratory The composition of cometary ices provides key information on the chemical and physical properties of the outer solar nebula where comets formed, 4.6 G.y. ago. This chapter summa- rizes our current knowledge of the volatile composition of cometary nuclei, based on spectro- scopic observations and in situ measurements of parent molecules and noble gases in cometary comae. The processes that govern the excitation and emission of parent molecules in the radio, infrared (IR), and ultraviolet (UV) wavelength regions are reviewed. The techniques used to convert line or band fluxes into molecular production rates are described. More than two dozen parent molecules have been identified, and we describe how each is investigated. The spatial distribution of some of these molecules has been studied by in situ measurements, long-slit IR and UV spectroscopy, and millimeter wave mapping, including interferometry. The spatial dis- tributions of CO, H2CO, and OCS differ from that expected during direct sublimation from the nucleus, which suggests that these species are produced, at least partly, from extended sources in the coma. Abundance determinations for parent molecules are reviewed, and the evidence for chemical diversity among comets is discussed. 1. INTRODUCTION ucts are called daughter products. Although there have been in situ measurements of some parent molecules in the coma Much of the scientific interest in comets stems from their of 1P/Halley using mass spectrometers, the majority of re- potential role in elucidating the processes responsible for the sults on the parent molecules have been derived from remote formation and evolution of the solar system. -
Comets in UV
Comets in UV B. Shustov1 • M.Sachkov1 • Ana I. G´omez de Castro 2 • Juan C. Vallejo2 • E.Kanev1 • V.Dorofeeva3,1 Abstract Comets are important “eyewitnesses” of So- etary systems too. Comets are very interesting objects lar System formation and evolution. Important tests to in themselves. A wide variety of physical and chemical determine the chemical composition and to study the processes taking place in cometary coma make of them physical processes in cometary nuclei and coma need excellent space laboratories that help us understand- data in the UV range of the electromagnetic spectrum. ing many phenomena not only in space but also on the Comprehensive and complete studies require for ad- Earth. ditional ground-based observations and in-situ exper- We can learn about the origin and early stages of the iments. We briefly review observations of comets in evolution of the Solar System analogues, by watching the ultraviolet (UV) and discuss the prospects of UV circumstellar protoplanetary disks and planets around observations of comets and exocomets with space-born other stars. As to the Solar System itself comets are instruments. A special refer is made to the World Space considered to be the major “witnesses” of its forma- Observatory-Ultraviolet (WSO-UV) project. tion and early evolution. The chemical composition of cometary cores is believed to basically represent the Keywords comets: general, ultraviolet: general, ul- composition of the protoplanetary cloud from which traviolet: planetary systems the Solar System was formed approximately 4.5 billion years ago, i.e. over all this time the chemical composi- 1 Introduction tion of cores of comets (at least of the long period ones) has not undergone any significant changes. -
Ice & Stone 2020
Ice & Stone 2020 WEEK 16: APRIL 12-18, 2020 Presented by The Earthrise Institute # 16 Authored by Alan Hale This week in history APRIL 12 13 14 15 16 17 18 APRIL 13, 2029: The near-Earth asteroid (99942) Apophis will pass just 0.00026 AU from Earth, slightly less than 5 Earth radii above the surface and within the orbital distance of geosynchronous satellites. At this time this is the closest predicted future approach of a near-Earth asteroid. The process of determining future close approaches like this one is the subject of this week’s “Special Topics” presentation. APRIL 12 13 14 15 16 17 18 APRIL 14, 2020: The near-Earth asteroid (52768) 1998 OR2, which will be passing close to Earth later this month, will occult the 7th-magnitude star HD 71008 in Cancer. The predicted path of the occultation crosses central Belarus, central Poland, northwestern Czech Republic, southern Germany, western Switzerland, southeastern France, central Algeria, far eastern Mali, and western Niger. APRIL 12 13 14 15 16 17 18 APRIL 15, 2019: A team of scientists led by Larry Nittler (Carnegie Institution for Science) announces their discovery of an apparent cometary fragment encased within the meteorite LaPaz Icefield 02342 that had been found in Antarctica. This discovery provides information concerning the transport of primordial material within the early solar system. COVER IMAGEs CREDITS: Front cover: This artist’s concept shows the Wide-field Infrared Survey Explorer, or WISE spacecraft, in its orbit around Earth. From 2010 to 2011, the WISE mission scanned the sky twice in infrared light not just for asteroids and comets but also stars, galaxies and other objects. -
Seeing the Light: the Art and Science of Astronomy
Chapter 1 Seeing the Light: The Art and Science of Astronomy In This Chapter ▶ Understanding the observational nature of astronomy ▶ Focusing on astronomy’s language of light ▶ Weighing in on gravity ▶ Recognizing the movements of objects in space tep outside on a clear night and look at the sky. If you’re a city dweller Sor live in a cramped suburb, you see dozens, maybe hundreds, of twin- kling stars. Depending on the time of the month, you may also see a full Moon and up to five of the eight planets that revolve around the Sun. A shooting star or “meteor” may appear overhead. What you actually see is the flash of light from a tiny piece of comet dust streaking through the upper atmosphere. Another pinpoint of light moves slowly and steadily across the sky. Is it a space satellite, such as the Hubble Space Telescope, or just a high-altitude airliner? If you have a pair of binoculars, you may be able to see the difference. Most air- liners have running lights, and their shapes may be perceptible. If you liveCOPYRIGHTED in the country — on the seashore MATERIAL away from resorts and develop- ments, on the plains, or in the mountains far from any floodlit ski slope — you can see thousands of stars. The Milky Way appears as a beautiful pearly swath across the heavens. What you’re seeing is the cumulative glow from millions of faint stars, individually indistinguishable with the naked eye. At a great observation place, such as Cerro Tololo in the Chilean Andes, you can see even more stars. -
The Crab Nebula Imaged by the Hubble Space Telescope in 1999 and 2000
Astronomers’ Observing Guides Other titles in this series The Moon and How to Observe It Peter Grego Double & Multiple Stars, and How to Observe Them James Mullaney Saturn and How to Observe it Julius Benton Jupiter and How to Observe it John McAnally Star Clusters and How to Observe Them Mark Allison Nebulae and How to Observe Them Steven Coe Galaxies and How to Observe Them Wolfgang Steinicke and Richard Jakiel Related titles Field Guide to the Deep Sky Objects Mike Inglis Deep Sky Observing Steven R. Coe The Deep-Sky Observer’s Year Grant Privett and Paul Parsons The Practical Astronomer’s Deep-Sky Companion Jess K. Gilmour Observing the Caldwell Objects David Ratledge Choosing and Using a Schmidt-Cassegrain Telescope Rod Mollise Martin Mobberley Supernovae and How to Observe Them with 167 Illustrations Martin Mobberley [email protected] Library of Congress Control Number: 2006928727 ISBN-10: 0-387-35257-0 e-ISBN-10: 0-387-46269-4 ISBN-13: 978-0387-35257-2 e-ISBN-13: 978-0387-46269-1 Printed on acid-free paper. © 2007 Springer Science+Business Media, LLC All rights reserved. This work may not be translated or copied in whole or in part without the written permission of the publisher (Springer Science+Business Media, LLC, 233 Spring Street, New York, NY 10013, USA), except for brief excerpts in connection with reviews or scholarly analysis. Use in connection with any form of information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed is forbidden. The use in this publication of trade names, trademarks, service marks, and similar terms, even if they are not identified as such, is not to be taken as an expression of opinion as to whether or not they are subject to proprietary rights. -
Comet ISON! (Comet of the Century?)
1 Mr. Justin J McCollum (BS, MS Physics) Lab Physics Coordinator Dept. of Physics Lamar University 2 Table of Contents ISON network………………..….………………….…...3 – 6 C/2012 S1 Discoverers………….…...……….…...…7 – 10 CoLiTech System…………………….……….….………...11 Discovery & Prediscovery……………….…….………...12 Early Orbital Analysis…………………….……….…….…13 Speculations of Comet ISON…………..…………14 - 15 Oort or Oort – Opik Cloud………….……........16 – 17 Origin of Comet ISON……….………………….……….18 Sungrazer Comets…………………………………….19 - 20 Evolution of Comet ISON………………………………21 Facts about Comet ISON…………………....…..22 – 23 ISON a Pristine Comet?...............................24 – 25 Photometry & Current Brightness……………..26 – 27 Nature and State of the Coma…………………..28 – 30 Central Nucleus of Comet ISON………………31 – 32 Nucleus to the Tail……………………………….…..……33 Nature & State of the Tail…………………………34 – 35 Future & Expectations………………………….....36 – 39 Getting to know more about Comets!...........40 – 46 After Perihelion Passage!..............................47 – 49 Catching the Comet in December!…………….50 – 53 ISON in the Daytime…….…………………………….…54 NASA Involvement!.............................................55 C/2012 S1 Orbital Structure………………..…………..56 Ephemeris Terminology………………………………...57 Data Spreadsheet Introduction………………………..58 Data Table Spreadsheets…………………………..59 - 60 Comet ISON Updates………………………………61 - 62 Knowing where & how to find ISON……...…63 – 64 Current ISON Observing Campaign………….65 – 66 Comet ISON photo contest…………………………….67 End Page……………………………………………………...68 3 Imperial Academy of -
Gaspard Duchêne Full Publication List
Gaspard Duch^ene Full Publication List Department of Astronomy Tel: +1 510 642 5275 501 Campbell Hall { UC Berkeley Fax: +1 510 467 2674 Berkeley CA 94720-3411 USA [email protected] REFEREED PUBLICATIONS 1) Using polarimetry to check rotation alignement in PMS binary stars. Principles of the method and first results, Monin, M´enard & Duch^ene, 1998, A&A, 339, 113 2) Binary fraction in low-mass star-forming regions: a reexamination of the possible excesses and implications, Duch^ene, 1999, A&A, 341, 547 3) Low-mass binaries in the young cluster IC 348: implications for binary formation and evolution, Duch^ene, Bouvier & Simon, 1999, A&A, 343, 831 4) Accretion in Taurus PMS binaries: a spectroscopic study, Duch^ene, Monin, Bouvier & M´enard, 1999, A&A, 351, 954 5) Near-infrared polarimetry of the GG Tau circumbinary ring, Silber, Gledhill, Duch^ene & M´enard, 2000, ApJL, 536, L89 6) The formation and evolution of binary systems. III. Low-mass binaries in the Praesepe cluster, Bouvier, Duch^ene, Mermilliod & Simon, 2001, A&A, 375, 989 7) Visual binaries among high-mass stars { An adaptive optics survey of OB stars in the NGC 6611 cluster, Duch^ene, Simon, Eisloffel & Bouvier, 2001, A&A, 379, 147 8) Resolved near-Infrared spectroscopy of the mysterious pre-main sequence binary system T Tau S, Duch^ene, Ghez & McCabe, 2002, ApJ, 568, 771 9) NICMOS images of the GG Tau circumbinary disk, McCabe, Duch^ene & Ghez, 2002, ApJ, 575, 974 10) Polarization in the young cluster NGC 6611: circumstellar interstellar or ... both ?, Bastien, M´enard,Corporon,