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Astronomy Unusually High Magnetic Fields in the Coma of 67P/Churyumov-Gerasimenko During Its High-Activity Phase C
Astronomy Unusually high magnetic fields in the coma of 67P/Churyumov-Gerasimenko during its high-activity phase C. Goetz, B. Tsurutani, Pierre Henri, M. Volwerk, E. Béhar, N. Edberg, A. Eriksson, R. Goldstein, P. Mokashi, H. Nilsson, et al. To cite this version: C. Goetz, B. Tsurutani, Pierre Henri, M. Volwerk, E. Béhar, et al.. Astronomy Unusually high mag- netic fields in the coma of 67P/Churyumov-Gerasimenko during its high-activity phase. Astronomy and Astrophysics - A&A, EDP Sciences, 2019, 630, pp.A38. 10.1051/0004-6361/201833544. hal- 02401155 HAL Id: hal-02401155 https://hal.archives-ouvertes.fr/hal-02401155 Submitted on 9 Dec 2019 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. A&A 630, A38 (2019) Astronomy https://doi.org/10.1051/0004-6361/201833544 & © ESO 2019 Astrophysics Rosetta mission full comet phase results Special issue Unusually high magnetic fields in the coma of 67P/Churyumov-Gerasimenko during its high-activity phase C. Goetz1, B. T. Tsurutani2, P. Henri3, M. Volwerk4, E. Behar5, N. J. T. Edberg6, A. Eriksson6, R. Goldstein7, P. Mokashi7, H. Nilsson4, I. Richter1, A. Wellbrock8, and K. -
Appendix 1: Venus Missions
Appendix 1: Venus Missions Sputnik 7 (USSR) Launch 02/04/1961 First attempted Venus atmosphere craft; upper stage failed to leave Earth orbit Venera 1 (USSR) Launch 02/12/1961 First attempted flyby; contact lost en route Mariner 1 (US) Launch 07/22/1961 Attempted flyby; launch failure Sputnik 19 (USSR) Launch 08/25/1962 Attempted flyby, stranded in Earth orbit Mariner 2 (US) Launch 08/27/1962 First successful Venus flyby Sputnik 20 (USSR) Launch 09/01/1962 Attempted flyby, upper stage failure Sputnik 21 (USSR) Launch 09/12/1962 Attempted flyby, upper stage failure Cosmos 21 (USSR) Launch 11/11/1963 Possible Venera engineering test flight or attempted flyby Venera 1964A (USSR) Launch 02/19/1964 Attempted flyby, launch failure Venera 1964B (USSR) Launch 03/01/1964 Attempted flyby, launch failure Cosmos 27 (USSR) Launch 03/27/1964 Attempted flyby, upper stage failure Zond 1 (USSR) Launch 04/02/1964 Venus flyby, contact lost May 14; flyby July 14 Venera 2 (USSR) Launch 11/12/1965 Venus flyby, contact lost en route Venera 3 (USSR) Launch 11/16/1965 Venus lander, contact lost en route, first Venus impact March 1, 1966 Cosmos 96 (USSR) Launch 11/23/1965 Possible attempted landing, craft fragmented in Earth orbit Venera 1965A (USSR) Launch 11/23/1965 Flyby attempt (launch failure) Venera 4 (USSR) Launch 06/12/1967 Successful atmospheric probe, arrived at Venus 10/18/1967 Mariner 5 (US) Launch 06/14/1967 Successful flyby 10/19/1967 Cosmos 167 (USSR) Launch 06/17/1967 Attempted atmospheric probe, stranded in Earth orbit Venera 5 (USSR) Launch 01/05/1969 Returned atmospheric data for 53 min on 05/16/1969 M. -
Early Observations of the Interstellar Comet 2I/Borisov
geosciences 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. -
Archons (Commanders) [NOTICE: They Are NOT Anlien Parasites], and Then, in a Mirror Image of the Great Emanations of the Pleroma, Hundreds of Lesser Angels
A R C H O N S HIDDEN RULERS THROUGH THE AGES A R C H O N S HIDDEN RULERS THROUGH THE AGES WATCH THIS IMPORTANT VIDEO UFOs, Aliens, and the Question of Contact MUST-SEE THE OCCULT REASON FOR PSYCHOPATHY Organic Portals: Aliens and Psychopaths KNOWLEDGE THROUGH GNOSIS Boris Mouravieff - GNOSIS IN THE BEGINNING ...1 The Gnostic core belief was a strong dualism: that the world of matter was deadening and inferior to a remote nonphysical home, to which an interior divine spark in most humans aspired to return after death. This led them to an absorption with the Jewish creation myths in Genesis, which they obsessively reinterpreted to formulate allegorical explanations of how humans ended up trapped in the world of matter. The basic Gnostic story, which varied in details from teacher to teacher, was this: In the beginning there was an unknowable, immaterial, and invisible God, sometimes called the Father of All and sometimes by other names. “He” was neither male nor female, and was composed of an implicitly finite amount of a living nonphysical substance. Surrounding this God was a great empty region called the Pleroma (the fullness). Beyond the Pleroma lay empty space. The God acted to fill the Pleroma through a series of emanations, a squeezing off of small portions of his/its nonphysical energetic divine material. In most accounts there are thirty emanations in fifteen complementary pairs, each getting slightly less of the divine material and therefore being slightly weaker. The emanations are called Aeons (eternities) and are mostly named personifications in Greek of abstract ideas. -
Transition Metal Complexes of Dicyanoacetylene
Louisiana State University LSU Digital Commons LSU Historical Dissertations and Theses Graduate School 1971 Transition Metal Complexes of Dicyanoacetylene: a Study of the Reaction Chemistry of Low Valence States of the Transition Metals, Platinum, Palladium, Nickel, Rhodium, and Iridium. Gregory Lloyd Mcclure Louisiana State University and Agricultural & Mechanical College Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_disstheses Recommended Citation Mcclure, Gregory Lloyd, "Transition Metal Complexes of Dicyanoacetylene: a Study of the Reaction Chemistry of Low Valence States of the Transition Metals, Platinum, Palladium, Nickel, Rhodium, and Iridium." (1971). LSU Historical Dissertations and Theses. 2001. https://digitalcommons.lsu.edu/gradschool_disstheses/2001 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Historical Dissertations and Theses by an authorized administrator of LSU Digital Commons. For more information, please contact [email protected]. 71-29,382 McCLURE, Gregory Lloyd, 1993- TRANSITION METAL COMPLEXES OF DICYANOACETYLENE: A STUDY OF THE REACTION CHEMISTRY OF LOW VALENCE STATES OF THE TRANSITION METALS, PLATINUM, PALLADIUM, NICKEL, RHODIUM, AND IRIDIUM. The Louisiana State University and Agricultural and Mechanical College, Ph.D., 1971 C hem i stry, inorgan ic University Microfilms, A XEROX Company , Ann Arbor. Michigan THIS DISSERTATION HAS BEEN MICROFILMED EXACTLY AS RECEIVED TRANSITION -
Ionization Photophysics and Spectroscopy of Dicyanoacetylene Sydney Leach, Martin Schwell, Gustavo A
Ionization photophysics and spectroscopy of dicyanoacetylene Sydney Leach, Martin Schwell, Gustavo A. Garcia, Yves Bénilan, Nicolas Fray, Marie-Claire Gazeau, François Gaie-Levrel, Norbert Champion, and Jean-Claude Guillemin Citation: The Journal of Chemical Physics 139, 184304 (2013); doi: 10.1063/1.4826467 View online: http://dx.doi.org/10.1063/1.4826467 View Table of Contents: http://scitation.aip.org/content/aip/journal/jcp/139/18?ver=pdfcov Published by the AIP Publishing This article is copyrighted as indicated in the article. Reuse of AIP content is subject to the terms at: http://scitation.aip.org/termsconditions. Downloaded to IP: 193.51.99.1 On: Wed, 05 Feb 2014 16:48:49 THE JOURNAL OF CHEMICAL PHYSICS 139, 184304 (2013) Ionization photophysics and spectroscopy of dicyanoacetylene Sydney Leach,1,a) Martin Schwell,2,a) Gustavo A. Garcia,3 Yves Bénilan,2 Nicolas Fray,2 Marie-Claire Gazeau,2 François Gaie-Levrel,3,b) Norbert Champion,1 and Jean-Claude Guillemin4 1LERMA UMR CNRS 8112, Observatoire de Paris-Meudon, 5 place Jules-Jansen, 92195 Meudon, France 2LISA UMR CNRS 7583, Université Paris-Est Créteil and Université Paris Diderot, Institut Pierre Simon Laplace, 61 Avenue du Général de Gaulle, 94010 Créteil, France 3Synchrotron SOLEIL, L’Orme des Merisiers, St. Aubin, B.P. 48, 91192 Gif-sur-Yvette Cedex, France 4Institut des Sciences Chimiques de Rennes, Ecole Nationale Supérieure de Chimie de Rennes, CNRS UMR 6226, 11 Allée de Beaulieu, CS 50837, 35708 Rennes Cedex 7, France (Received 17 June 2013; accepted 8 October 2013; published online 11 November 2013) Photoionization of dicyanoacetylene was studied using synchrotron radiation over the excitation range 8–25 eV, with photoelectron-photoion coincidence techniques. -
Interstellar Comet 2I/Borisov Exhibits a Structure Similar to Native Solar System Comets⋆
Mon. Not. R. Astron. Soc. 000, 1–5 (201X) Printed 4 April 2020 (MN LATEX style file v2.2) Interstellar Comet 2I/Borisov exhibits a structure similar to native Solar System comets⋆ F. Manzini1†, V. Oldani1, P. Ochner2,3, and L.R.Bedin2 1Stazione Astronomica di Sozzago, Cascina Guascona, I-28060 Sozzago (Novara), Italy 2INAF-Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, I-35122 Padova, Italy 3Department of Physics and Astronomy-University of Padova, Via F. Marzolo 8, I-35131 Padova, Italy Letter: Accepted 2020 April 1. Received 2020 April 1; in original form 2019 November 22. ABSTRACT We processed images taken with the Hubble Space Telescope (HST) to investigate any morphological features in the inner coma suggestive of a peculiar activity on the nucleus of the interstellar comet 2I/Borisov. The coma shows an evident elongation, in the position angle (PA) ∼0◦-180◦ direction, which appears related to the presence of a jet originating from a single active source on the nucleus. A counterpart of this jet directed towards PA ∼10◦ was detected through analysis of the changes of the inner coma morphology on HST images taken in different dates and processed with different filters. These findings indicate that the nucleus is probably rotating with a spin axis projected near the plane of the sky and oriented at PA ∼100◦-280◦, and that the active source is lying in a near-equatorial position. Subsequent observations of HST allowed us to determine the direction of the spin axis at RA = 17h20m ±15◦ and Dec = −35◦ ±10◦. Photometry of the nucleus on HST images of 12 October 2019 only span ∼7 hours, insufficient to reveal a rotational period. -
Closing the Gap Between Ground Based and In-Situ Observations of Cometary Dust Activity: Investigating Comet 67P to Gain a Deeper Understanding of Other Comets
Closing the gap between ground based and in-situ observations of cometary dust activity: Investigating comet 67P to gain a deeper understanding of other comets. Raphael Marschall & Oleksandra Ivanova et al. Abstract When cometary dust particles are ejected from the surface they are accelerated because of the surrounding gas flow from sublimating ices. As these particles travel millions of kilometres from their origin into the solar system they produce the magnificent tails commonly associated with comets. During their long journey the dust particles transition through different regimes of changing dominant forces such as gas drag, cometary gravity, solar radiation pressure, and solar gravity. The transition and link between the different regimes is to this day poorly understood. There are two main reasons for this. Firstly, the problem covers a vast range in spatial and temporal scales that need to be matched taking into account multiple transitions of the force regime. Furthermore, observational data covering these large spatial and temporal scales for at least one comet and thus characterising it in great detail has been lacking until recently. For comet 67P/Churyumov-Gerasimenko (hereafter 67P) a small number of large scale struc- tures in the outer dust coma and tail have been found from ground based observations. Con- versely ESA's Rosetta mission has shown many small scale structures defining the innermost coma close to the nucleus surface. This disconnect between the observations on these different scales has yet to be understood and explained. Solving this problem thus requires an interdisciplinary approach. This ISSI team shall bring together experts of the recent observational data from ground and in-situ of comet 67P as well as theorists that are able to model the dynamical processes over these different scales. -
FIRST COMETARY OBSERVATIONS with ALMA: C/2012 F6 (LEMMON) and C/2012 S1 (ISON) Martin Cordiner1,2, Stefanie Milam1, Michael Mumm
45th Lunar and Planetary Science Conference (2014) 2609.pdf FIRST COMETARY OBSERVATIONS WITH ALMA: C/2012 F6 (LEMMON) AND C/2012 S1 (ISON) Martin Cordiner1,2, Stefanie Milam1, Michael Mumma1, Steven Charnley1, Anthony Remijan3, Geronimo Vil- lanueva1,2, Lucas Paganini1,2, Jeremie Boissier4, Dominique Bockelee-Morvan5, Nicolas Biver5, Dariusz Lis6, Yi- Jehng Kuan7, Jacques Crovisier5, Iain Coulson9, Dante Minniti10 1Goddard Center for Astrobiology, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20770, USA; email: [email protected]. 2The Catholic University of America, 620 Michigan Ave. NE, Washington, DC 20064, USA. 3NRAO, Charlottesville, VA 22903, USA. 4IRAM, 300 Rue de la Piscine, 38406 Saint Martin d’Heres, France. 5Observatoire de Paris, Meudon, France. 6Caltech, Pasadena, CA 91125, USA. 7National Taiwan Normal University, Taipei, Taiwan. 9Joint As- tronomy Centre, Hilo, HI 96720, USA. 10Pontifica Universidad Catolica de Chile, Santigo, Chile. Introduction: Cometary ices are believed to have The observed visibilities were flagged, calibrated aggregated around the time the Solar System formed and imaged using standard routines in the NRAO (c. 4.5 Gyr ago), and have remained in a frozen, rela- CASA software (version 4.1.0). Image deconvolution tively quiescent state ever since. Ground-based studies was performed using the Hogbom algorithm with natu- of the compositions of cometary comae provide indi- ral weighting and a threshold flux level of twice the rect information on the compositions of the nuclear RMS noise. ices, and thus provide insight into the physical and chemical conditions of the early Solar Nebula. To real- Results: The data cubes show spectrally and spa- ize the full potential of gas-phase coma observations as tially-resolved structures in HCN, CH3OH and H2CO probes of solar system evolution therefore requires a emission in both comets, consistent with anisotropic complete understanding of the gas-release mecha- outgassing from their nuclei. -
Research Paper in Nature
Draft version November 1, 2017 Typeset using LATEX twocolumn style in AASTeX61 DISCOVERY AND CHARACTERIZATION OF THE FIRST KNOWN INTERSTELLAR OBJECT Karen J. Meech,1 Robert Weryk,1 Marco Micheli,2, 3 Jan T. Kleyna,1 Olivier Hainaut,4 Robert Jedicke,1 Richard J. Wainscoat,1 Kenneth C. Chambers,1 Jacqueline V. Keane,1 Andreea Petric,1 Larry Denneau,1 Eugene Magnier,1 Mark E. Huber,1 Heather Flewelling,1 Chris Waters,1 Eva Schunova-Lilly,1 and Serge Chastel1 1Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA 2ESA SSA-NEO Coordination Centre, Largo Galileo Galilei, 1, 00044 Frascati (RM), Italy 3INAF - Osservatorio Astronomico di Roma, Via Frascati, 33, 00040 Monte Porzio Catone (RM), Italy 4European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching bei M¨unchen,Germany (Received November 1, 2017; Revised TBD, 2017; Accepted TBD, 2017) Submitted to Nature ABSTRACT Nature Letters have no abstracts. Keywords: asteroids: individual (A/2017 U1) | comets: interstellar Corresponding author: Karen J. Meech [email protected] 2 Meech et al. 1. SUMMARY 22 confirmed that this object is unique, with the highest 29 Until very recently, all ∼750 000 known aster- known hyperbolic eccentricity of 1:188 ± 0:016 . Data oids and comets originated in our own solar sys- obtained by our team and other researchers between Oc- tem. These small bodies are made of primor- tober 14{29 refined its orbital eccentricity to a level of dial material, and knowledge of their composi- precision that confirms the hyperbolic nature at ∼ 300σ. tion, size distribution, and orbital dynamics is Designated as A/2017 U1, this object is clearly from essential for understanding the origin and evo- outside our solar system (Figure2). -
The Castalia Mission to Main Belt Comet 133P/Elst-Pizarro C
The Castalia mission to Main Belt Comet 133P/Elst-Pizarro C. Snodgrass, G.H. Jones, H. Boehnhardt, A. Gibbings, M. Homeister, N. Andre, P. Beck, M.S. Bentley, I. Bertini, N. Bowles, et al. To cite this version: C. Snodgrass, G.H. Jones, H. Boehnhardt, A. Gibbings, M. Homeister, et al.. The Castalia mission to Main Belt Comet 133P/Elst-Pizarro. Advances in Space Research, Elsevier, 2018, 62 (8), pp.1947- 1976. 10.1016/j.asr.2017.09.011. hal-02350051 HAL Id: hal-02350051 https://hal.archives-ouvertes.fr/hal-02350051 Submitted on 28 Aug 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. Distributed under a Creative Commons Attribution| 4.0 International License Available online at www.sciencedirect.com ScienceDirect Advances in Space Research 62 (2018) 1947–1976 www.elsevier.com/locate/asr The Castalia mission to Main Belt Comet 133P/Elst-Pizarro C. Snodgrass a,⇑, G.H. Jones b, H. Boehnhardt c, A. Gibbings d, M. Homeister d, N. Andre e, P. Beck f, M.S. Bentley g, I. Bertini h, N. Bowles i, M.T. Capria j, C. Carr k, M. -
Polymerization of Dicyanoacetylene † ‡ ○ † ○ ■ ¶ § ■ § ■ Huiyang Gou,*, , , Li Zhu, , Haw-Tyng Huang, , Arani Biswas, , Derek W
Article pubs.acs.org/cm From Linear Molecular Chains to Extended Polycyclic Networks: Polymerization of Dicyanoacetylene † ‡ ○ † ○ ■ ¶ § ■ § ■ Huiyang Gou,*, , , Li Zhu, , Haw-Tyng Huang, , Arani Biswas, , Derek W. Keefer, , ∥ ◆ ⊥ † ‡ † ‡ † Brian L. Chaloux, , Clemens Prescher, Liuxiang Yang, , Duck Young Kim, , Matthew D. Ward, ■ # # ∇ ∥ § ■ ¶ □ Jordan Lerach, Shengnan Wang, Artem R. Oganov, , Albert Epshteyn, John V. Badding, , , , † and Timothy A. Strobel*, † Geophysical Laboratory, Carnegie Institution of Washington, Washington, DC 20015, United States ‡ Center for High Pressure Science and Technology Advanced Research, Beijing 100094, China § Department of Chemistry, The Pennsylvania State University, University Park, Pennsylvania 16802, United States ■ Materials Research Institute, The Pennsylvania State University, University Park, Pennsylvania 16802, United States ¶ Department of Materials Science and Engineering, The Pennsylvania State University, University Park, Pennsylvania 16802, United States □ Department of Physics, The Pennsylvania State University, University Park, Pennsylvania 16802, United States ∥ Naval Research Laboratory, 4555 Overlook Avenue, SW, Washington, DC 20375, United States ⊥ Center for Advanced Radiation Sources, University of Chicago, Argonne, Illinois 60437, United States # Department of Geosciences, Center for Materials by Design, and Institute for Advanced Computational Science, State University of New York, Stony Brook, New York 11794-2100, United States ∇ Skolkovo Institute of Science and Technology,