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Mercury's interior structure, rotation, and tides

VanHoolst, T. and Sohl, F. and Holin, I. and Verhoeven, O. and Dehant, V. and Spohn, T. (2007) Mercury's interior structure, rotation, and tides. Space Science Reviews, 132 (2-4), pp. 203-227. Springer. DOI: 10.1007/s11214-007-9202-6.

Full text not available from this repository.

Abstract

This review addresses the deep interior structure of Mercury. Mercury is thought to consist of similar chemical reservoirs (core, mantle, crust) as the other terrestrial planets, but with a relatively much larger core. Constraints on Mercury’s composition and internal structure are reviewed, and possible interior models are described. Large advances in our knowledge of Mercury’s interior are not only expected from imaging of characteristic surface features but particularly from geodetic observations of the gravity field, the rotation, and the tides of Mercury. The low-degree gravity field of Mercury gives information on the differences of the principal moments of inertia, which are a measure of the mass concentration toward the center of the planet. Mercury’s unique rotation presents several clues to the deep interior. From observations of the mean obliquity of Mercury and the low-degree gravity data, the moments of inertia can be obtained, and deviations from the mean rotation speed (librations) offer an exciting possibility to determine the moment of inertia of the mantle. Due to its proximity to the Sun, Mercury has the largest tides of the Solar System planets. Since tides are sensitive to the existence and location of liquid layers, tidal observations are ideally suited to study the physical state and size of the core of Mercury.

Document Type:Article
Title:Mercury's interior structure, rotation, and tides
Authors:
AuthorsInstitution or Email of Authors
VanHoolst, T.Royal Observatory of Belgium, Brussels, Belgium
Sohl, F.UNSPECIFIED
Holin, I.Space research institute, Moscow, Russia
Verhoeven, O.Royal Observatory of Belgium, Brussels, Belgium
Dehant, V.Royal Observatory of Belgium, Brussels, Belgium
Spohn, T.UNSPECIFIED
Date:October 2007
Journal or Publication Title:Space Science Reviews
Refereed publication:Yes
In ISI Web of Science:Yes
Volume:132
DOI: 10.1007/s11214-007-9202-6
Page Range:pp. 203-227
Publisher:Springer
Status:Published
Keywords:Mercury, Interior, Composition, Rotation, Libration, Tides
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Vorhaben Vergleichende Planetologie (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Deposited By: Stefanie Musiol
Deposited On:15 Jan 2008
Last Modified:27 Apr 2009 13:33

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