Estimating Mercury's 88-day libration amplitude from orbit |
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Authors: | R Jehn C Corral |
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Affiliation: | a European Space Operations Centre, Robert-Bosch-Str. 5, Darmstadt 64293, Germany b Space and Atmospheric Physics, Imperial College, London SW7 2BW, UK |
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Abstract: | In this paper it is derived that the libration of Mercury can be described by 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 , then the libration amplitude can be determined in two Mercury years (176 days) with an accuracy of or better, which is sufficient to answer the question whether Mercury has a solid or fluid core. |
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Keywords: | Mercury BepiColombo Libration amplitude Spin-orbit resonance |
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