Geodesy and geophysics of Mercury: Prospects in view of the BepiColombo mission
Autor: | Hauke Hussmann, Alexander Stark |
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Rok vydání: | 2020 |
Předmět: |
010504 meteorology & atmospheric sciences
General Physics and Astronomy chemistry.chemical_element 01 natural sciences Outer core Mantle (geology) Astrobiology law.invention Orbiter law Planet 0103 physical sciences General Materials Science Physical and Theoretical Chemistry 010303 astronomy & astrophysics 0105 earth and related environmental sciences geography geography.geographical_feature_category Spacecraft business.industry Crust Mercury Mercury (element) Geophysics chemistry Volcano BepiColombo Mission business Geodesy Geology Solar system |
Zdroj: | The European Physical Journal Special Topics. 229:1379-1389 |
ISSN: | 1951-6401 1951-6355 |
DOI: | 10.1140/epjst/e2020-900211-4 |
Popis: | The BepiColombo mission, which is a joint mission of the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA), was launched successfully on October 20, 2018 from Kourou, French Guyana. The spacecraft is currently on its 7 yr cruise to Mercury. The main science campaign at Mercury will begin, however, no earlier than spring 2026, after two orbiters, the Mercury Planetary Orbiter (MPO) and the Mercury Magnetospheric Orbiter (MMO) have been inserted in their final orbits in late 2025. Mercury is an intriguing planetary object with respect to its dynamical state and evolution. The planet is differentiated and contains a large iron core overlain by a relatively thin silicate mantle and crust. Mercury is locked in a unique 3:2 spin-orbit coupling and its intrinsic magnetic dipole field shows that at least part of Mercury’s iron core is liquid. From libration measurements it has been concluded that Mercury’s outer core is liquid, decoupling the silicate mantle from the deep interior. Phases of global contraction and phases of volcanic activity are evidence for an eventful thermal evolution of the planet. In this paper the current knowledge on the evolution of Mercury, focusing on its dynamical, rotational and orbital state is summarized. Prospects for investigations with BepiColombo will be discussed. |
Databáze: | OpenAIRE |
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