Geodesy, Geophysics and Fundamental Physics Investigations of the BepiColombo Mission
Autor: | Nicola Tosi, Paolo Cappuccio, Francesco Santoli, Tim Van Hoolst, J. S. Oliveira, Daniel Heyner, Nicolas Thomas, Alexander Stark, Johannes Wicht, Luciano Iess, H. Hussmann, Ivan di Stefano, Antonio Genova, Johannes Benkhoff, Patrick Kolhey, Johannes Z. D. Mieth, Gregor Steinbrügge, Benoit Langlais |
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Přispěvatelé: | Genova, A. [0000-0001-5584-492X], Hussmann, H. [0000-0002-3816-0232], Van Hoolst, T. [0000-0002-9820-8584], Heyner, D. [0000-0001-7894-8246], Iess, L. [0000-0002-6230-5825], Santoli, F. [0000-0003-2493-0109], Thomas, N. [0000-0002-0146-0071], Cappuccio, P. [0000-0002-8758-6627], Di Stefano, I. [0000-0003-1491-6848], Langlais, B. [0000-0001-5207-304X], Oliveira, J. S. [0000-0002-4587-2895], Stark, A. [0000-0001-9110-1138], Steinbrügge, G. [0000-0002-1050-7759], Tosi, N. [0000-0002-4912-2848], Wicht, J. [0000-0002-2440-5091], Benkhoff, J. [0000-0002-4307-9703], Agenzia Spaziale Italiana (ASI), Bundesministerium für Wirtschaft und Energie (BMWi), Deutsches Zentrum für Luft- und Raumfahrt (DLR), Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) |
Jazyk: | angličtina |
Rok vydání: | 2021 |
Předmět: |
Solar System
Engineering Topography 010504 meteorology & atmospheric sciences BepiColombo Gravity [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] chemistry.chemical_element Astronomy & Astrophysics 01 natural sciences law.invention Orbiter Theories of gravitation Planetenphysik Planet law 0103 physical sciences Altimeter Internal structure 010303 astronomy & astrophysics 0105 earth and related environmental sciences Radio Science Science & Technology Spacecraft business.industry 520 Astronomy Planetengeodäsie Astronomy and Astrophysics Geophysics Mercury Geodesy 620 Engineering Mercury (element) Planetary science Magnetic field chemistry 13. Climate action Space and Planetary Science gravity internal structure magnetic field theories of gravitation thermal evolution topography Physical Sciences business Thermal evolution |
Zdroj: | Genova, Antonio; Hussmann, Hauke; Van Hoolst, Tim; Heyner, Daniel; Iess, Luciano; Santoli, Francesco; Thomas, Nicolas; Cappuccio, Paolo; di Stefano, Ivan; Kolhey, Patrick; Langlais, Benoit; Mieth, Johannes Z. D.; Oliveira, Joana S.; Stark, Alexander; Steinbrügge, Gregor; Tosi, Nicola; Wicht, Johannes; Benkhoff, Johannes (2021). Geodesy, Geophysics and Fundamental Physics Investigations of the BepiColombo Mission. Space science reviews, 217(2) Springer 10.1007/s11214-021-00808-9 DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial instname Space Science Reviews Space Science Reviews, Springer Verlag, 2021, 217 (2), ⟨10.1007/s11214-021-00808-9⟩ |
ISSN: | 0038-6308 1572-9672 |
Popis: | Open access funding provided by Università degli Studi di Roma La Sapienza within the CRUI-CARE Agreement. In preparation for the ESA/JAXA BepiColombo mission to Mercury, thematic working groups had been established for coordinating the activities within the BepiColombo Science Working Team in specific fields. Here we describe the scientific goals of the Geodesy and Geophysics Working Group (GGWG) that aims at addressing fundamental questions regarding Mercury’s internal structure and evolution. This multidisciplinary investigation will also test the gravity laws by using the planet Mercury as a proof mass. The instruments on the Mercury Planetary Orbiter (MPO), which are devoted to accomplishing the GGWG science objectives, include the BepiColombo Laser Altimeter (BELA), the Mercury orbiter radio science experiment (MORE), and the MPO magnetometer (MPO-MAG). The onboard Italian spring accelerometer (ISA) will greatly aid the orbit reconstruction needed by the gravity investigation and laser altimetry. We report the current knowledge on the geophysics, geodesy, and evolution of Mercury after the successful NASA mission MESSENGER and set the prospects for the BepiColombo science investigations based on the latest findings on Mercury’s interior. The MPO spacecraft of the BepiColombo mission will provide extremely accurate measurements of Mercury’s topography, gravity, and magnetic field, extending and improving MESSENGER data coverage, in particular in the southern hemisphere. Furthermore, the dual-spacecraft configuration of the BepiColombo mission with the Mio spacecraft at higher altitudes than the MPO spacecraft will be fundamental for decoupling the internal and external contributions of Mercury’s magnetic field. Thanks to the synergy between the geophysical instrument suite and to the complementary instruments dedicated to the investigations on Mercury’s surface, composition, and environment, the BepiColombo mission is poised to advance our understanding of the interior and evolution of the innermost planet of the solar system. We are grateful to the ESA spacecraft operations team for supporting and planning the scientific observations during BepiColombo cruise and orbital mission. A.G. and L.I. thank A. Di Ruscio (Sapienza University of Rome) for his support in the numerical simulations of the MORE investigation. A.G. and L.I. acknowledge funding from the Italian Space Agency (ASI) grant N. 2017-40-H.0. T.V.H. was financially supported by the Belgian Research Action through Interdisciplinary Networks (BRAIN.be 2.0 project STEM) and by the Belgian PRODEX program managed by the European Space Agency in collaboration with the Belgian Federal Science Policy Office. D.H. was financially supported by the German Ministerium für Wirtschaft und Energie and the German Zentrum für Luft- und Raumfahrt under contract 50 QW 1501. F.S. was financially supported by ASI through the cooperation agreement N. 2017-47-H.0. We acknowledge Gregory A. Neumann and an anonymous referee for their helpful comments to improve the quality of this paper. The data used in this study for the numerical simulations of the BepiColombo mission are available at https://www.cosmos.esa.int/web/spice/spice-for-bepicolombo. Peerreview |
Databáze: | OpenAIRE |
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