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The Comet Interceptor Mission.
Jones, Geraint H; Snodgrass, Colin; Tubiana, Cecilia; Küppers, Michael; Kawakita, Hideyo; Lara, Luisa M; Agarwal, Jessica; André, Nicolas; Attree, Nicholas; Auster, Uli; Bagnulo, Stefano; Bannister, Michele; Beth, Arnaud; Bowles, Neil; Coates, Andrew; Colangeli, Luigi; Corral van Damme, Carlos; Da Deppo, Vania; De Keyser, Johan; Della Corte, Vincenzo; Edberg, Niklas; El-Maarry, Mohamed Ramy; Faggi, Sara; Fulle, Marco; Funase, Ryu; Galand, Marina; Goetz, Charlotte; Groussin, Olivier; Guilbert-Lepoutre, Aurélie; Henri, Pierre; Kasahara, Satoshi; Kereszturi, Akos; Kidger, Mark; Knight, Matthew; Kokotanekova, Rosita; Kolmasova, Ivana; Kossacki, Konrad; Kührt, Ekkehard; Kwon, Yuna; La Forgia, Fiorangela; Levasseur-Regourd, Anny-Chantal; Lippi, Manuela; Longobardo, Andrea; Marschall, Raphael; Morawski, Marek; Muñoz, Olga; Näsilä, Antti; Nilsson, Hans; Opitom, Cyrielle; Pajusalu, Mihkel.
Afiliación
  • Jones GH; Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, UK.
  • Snodgrass C; The Centre for Planetary Sciences at UCL/Birkbeck, London, UK.
  • Tubiana C; The University of Edinburgh, Edinburgh, UK.
  • Küppers M; INAF, IAPS, Rome, Italy.
  • Kawakita H; European Space Agency (ESA), European Space Astronomy Centre (ESAC), Madrid, Spain.
  • Lara LM; Koyama Astronomical Observatory, Kyoto Sangyo University, Kyoto, Japan.
  • Agarwal J; Instituto de Astrofisica de Andalucía - CSIC, Granada, Spain.
  • André N; Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany.
  • Attree N; IRAP, CNRS, University Toulouse 3, CNES, Toulouse, France.
  • Auster U; Instituto de Astrofisica de Andalucía - CSIC, Granada, Spain.
  • Bagnulo S; Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany.
  • Bannister M; Armagh Observatory and Planetarium, Armagh, UK.
  • Beth A; University of Canterbury, Christchurch, New Zealand.
  • Bowles N; Department of Physics, Imperial College London, London, UK.
  • Coates A; Department of Physics, University of Oxford, Oxford, UK.
  • Colangeli L; Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, UK.
  • Corral van Damme C; The Centre for Planetary Sciences at UCL/Birkbeck, London, UK.
  • Da Deppo V; European Space Agency, ESTEC, Noordwijk, The Netherlands.
  • De Keyser J; European Space Agency, ESTEC, Noordwijk, The Netherlands.
  • Della Corte V; CNR-Institute for Photonics and Nanotechnologies, Padova, Italy.
  • Edberg N; Royal Belgian Institute of Space Aeronomy, Brussels, Belgium.
  • El-Maarry MR; INAF, IAPS, Rome, Italy.
  • Faggi S; Swedish Institute of Space Physics, Uppsala/Kiruna, Sweden.
  • Fulle M; Space and Planetary Science Center and Department of Earth Sciences, Khalifa University, Abu Dhabi, United Arab Emirates.
  • Funase R; NASA Goddard Space Flight Center, Greenbelt, USA.
  • Galand M; INAF - Osservatorio Astronomico di Trieste, Trieste, Italy.
  • Goetz C; Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Kanagawa, Japan.
  • Groussin O; Department of Physics, Imperial College London, London, UK.
  • Guilbert-Lepoutre A; European Space Agency, ESTEC, Noordwijk, The Netherlands.
  • Henri P; Laboratoire d'Astrophysique de Marseille, Aix-Marseille Université, CNRS, Marseille, France.
  • Kasahara S; LGL-TPE, CNRS, ENS, Université Lyon1, UJM, Lyon, France.
  • Kereszturi A; Laboratoire Lagrange, CNRS, OCA, Université Côte d'Azur, and LPC2E, CNRS, Université d'Orléans, CNES, Orléans, France.
  • Kidger M; The University of Tokyo, Tokyo, Japan.
  • Knight M; Konkoly Astronomical Institute, Research Centre for Astronomy and Earth Sciences, HUN-REN, Budapest, Hungary.
  • Kokotanekova R; European Space Agency (ESA), European Space Astronomy Centre (ESAC), Madrid, Spain.
  • Kolmasova I; U.S. Naval Academy, Annapolis, USA.
  • Kossacki K; Institute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences, Sofia, Bulgaria.
  • Kührt E; Institute of Atmospheric Physics of the Czech Academy of Sciences, Prague, Czech Republic.
  • Kwon Y; Faculty of Physics, University of Warsaw, Warsaw, Poland.
  • La Forgia F; DLR, Institute of Optical Sensor Systems, Berlin, Germany.
  • Levasseur-Regourd AC; Caltech/IPAC, 1200 E California Blvd, MC 100-22 Pasadena, CA 91125, USA.
  • Lippi M; Department of Physics and Astronomy, University of Padova, Padova, Italy.
  • Longobardo A; LATMOS, Sorbonne Université, CNRS, CNES, Paris, France.
  • Marschall R; Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany.
  • Morawski M; INAF, IAPS, Rome, Italy.
  • Muñoz O; CNRS, Laboratoire J.-L. Lagrange, Observatoire de la Côte d'Azur, Nice, France.
  • Näsilä A; Space Research Centre of the Polish Academy of Sciences, Warsaw, Poland.
  • Nilsson H; Instituto de Astrofisica de Andalucía - CSIC, Granada, Spain.
  • Opitom C; VTT Technical Research Centre of Finland Ltd, Espoo, Finland.
  • Pajusalu M; Swedish Institute of Space Physics, Uppsala/Kiruna, Sweden.
Space Sci Rev ; 220(1): 9, 2024.
Article en En | MEDLINE | ID: mdl-38282745
ABSTRACT
Here we describe the novel, multi-point Comet Interceptor mission. It is dedicated to the exploration of a little-processed long-period comet, possibly entering the inner Solar System for the first time, or to encounter an interstellar object originating at another star. The objectives of the mission are to address the following questions What are the surface composition, shape, morphology, and structure of the target object? What is the composition of the gas and dust in the coma, its connection to the nucleus, and the nature of its interaction with the solar wind? The mission was proposed to the European Space Agency in 2018, and formally adopted by the agency in June 2022, for launch in 2029 together with the Ariel mission. Comet Interceptor will take advantage of the opportunity presented by ESA's F-Class call for fast, flexible, low-cost missions to which it was proposed. The call required a launch to a halo orbit around the Sun-Earth L2 point. The mission can take advantage of this placement to wait for the discovery of a suitable comet reachable with its minimum ΔV capability of 600 ms-1. Comet Interceptor will be unique in encountering and studying, at a nominal closest approach distance of 1000 km, a comet that represents a near-pristine sample of material from the formation of the Solar System. It will also add a capability that no previous cometary mission has had, which is to deploy two sub-probes - B1, provided by the Japanese space agency, JAXA, and B2 - that will follow different trajectories through the coma. While the main probe passes at a nominal 1000 km distance, probes B1 and B2 will follow different chords through the coma at distances of 850 km and 400 km, respectively. The result will be unique, simultaneous, spatially resolved information of the 3-dimensional properties of the target comet and its interaction with the space environment. We present the mission's science background leading to these objectives, as well as an overview of the scientific instruments, mission design, and schedule.
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Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Space Sci Rev Año: 2024 Tipo del documento: Article

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Space Sci Rev Año: 2024 Tipo del documento: Article