BepiColombo - Mission Overview and Science Goals View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2021-12-08

AUTHORS

J. Benkhoff, G. Murakami, W. Baumjohann, S. Besse, E. Bunce, M. Casale, G. Cremosese, K.-H. Glassmeier, H. Hayakawa, D. Heyner, H. Hiesinger, J. Huovelin, H. Hussmann, V. Iafolla, L. Iess, Y. Kasaba, M. Kobayashi, A. Milillo, I. G. Mitrofanov, E. Montagnon, M. Novara, S. Orsini, E. Quemerais, U. Reininghaus, Y. Saito, F. Santoli, D. Stramaccioni, O. Sutherland, N. Thomas, I. Yoshikawa, J. Zender

ABSTRACT

BepiColombo is a joint mission between the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA, to perform a comprehensive exploration of Mercury. Launched on 20th\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$20^{\mathrm{th}}$\end{document} October 2018 from the European spaceport in Kourou, French Guiana, the spacecraft is now en route to Mercury.Two orbiters have been sent to Mercury and will be put into dedicated, polar orbits around the planet to study the planet and its environment. One orbiter, Mio, is provided by JAXA, and one orbiter, MPO, is provided by ESA. The scientific payload of both spacecraft will provide detailed information necessary to understand the origin and evolution of the planet itself and its surrounding environment. Mercury is the planet closest to the Sun, the only terrestrial planet besides Earth with a self-sustained magnetic field, and the smallest planet in our Solar System. It is a key planet for understanding the evolutionary history of our Solar System and therefore also for the question of how the Earth and our Planetary System were formed.The scientific objectives focus on a global characterization of Mercury through the investigation of its interior, surface, exosphere, and magnetosphere. In addition, instrumentation onboard BepiColombo will be used to test Einstein’s theory of general relativity. Major effort was put into optimizing the scientific return of the mission by defining a payload such that individual measurements can be interrelated and complement each other. More... »

PAGES

90

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  • Journal

    TITLE

    Space Science Reviews

    ISSUE

    8

    VOLUME

    217

    Author Affiliations

  • ESA/ESTEC, Keplerlaan 1, 2200 AG, Noordwijk, The Netherlands
  • JAXA, 3-1-1 Yoshinodai, 299-8510, Sagamihara, Kanagawa, Japan
  • Space Research Institute, Austrian Academy of Sciences, Graz, Austria
  • ESAC, P.O. Box 78, 28691, Vilanueva de la Canada, Spain
  • School of Physics and Astronomy, University of Leicester, University Road, LE17RH, Leicester, UK
  • INAF-Osservatorio Astronomico di Padova, Padova, Italy
  • Institut für Geophysik und Extrateresstrische Physik, Technische Universität Braunschweig, Braunschweig, Germany
  • Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 252-5210, Sagamihara, Kanagawa, Japan
  • Institut für Planetologie, Westfälische Wilhelms-Universität, Wilhelm-Klemm-Str. 10, 48149, Münster, Germany
  • Department of Physics, University of Helsinki, Helsinki, Finland
  • Institute of Planetary Research, German Aerospace Center, Rutherfordstr. 2, 12489, Berlin, Germany
  • INAF-IAPS (Institute for Astrophysics and Planetology from Space), via del Fosso del Cavaliere 100, 00133, Rome, Italy
  • Dipartimento di ingegneria meccanica e aerospaziale, Universitá La Sapienza, Roma, Italy
  • Planetary Plasma and Atmospheric Research Center, Graduate School of Science, Tohoku University, 980-8578, Sendai, Miyagi, Japan
  • Chiba Institute of Technology, Planetary Exploration Research Center, 2-17-1, Tsudanuma, 275-0016, Narashino, Chiba, Japan
  • Institute for Space Research, Moscow, Russian Federation
  • European Space Agency, European Space Operations Center, Darmstadt, Germany
  • LATMOS, Universite Versailles Saint-Quentin, Guyancourt, France
  • Physikalisches Institut, University of Bern, Sidlerstr. 5, CH-3012, Bern, Switzerland
  • Department of Complexity Science and Engineering, University of Tokyo, 277-13 8561, Kashiwa, Chiba, Japan
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s11214-021-00861-4

    DOI

    http://dx.doi.org/10.1007/s11214-021-00861-4

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1143720498


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