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Estimating Mercury's 88-day libration amplitude from orbit
Authors:R Jehn  C Corral
Affiliation:a European Space Operations Centre, Robert-Bosch-Str. 5, Darmstadt 64293, Germany
b Space and Atmospheric Physics, Imperial College, London SW7 2BW, UK
Abstract:In this paper it is derived that the libration of Mercury can be described by View the MathML source where Φ0 is the unknown libration amplitude, M is Mercury's mean anomaly and K=−9.483. Φ0 can be determined by comparing pairs of images of the same landmarks taken by an orbiter at different positions of Mercury. If the angle between the orbit plane of a polar orbiter and Mercury's line of periapsis is between −60° and 60° and if one landmark at the equator is imaged per day with a relative precision of View the MathML source, then the libration amplitude can be determined in two Mercury years (176 days) with an accuracy of View the MathML source or better, which is sufficient to answer the question whether Mercury has a solid or fluid core.
Keywords:Mercury   BepiColombo   Libration amplitude   Spin-orbit resonance
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