A Mercury orientation model including non-zero obliquity and librations

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A Mercury orientation model including non-zero obliquity and librations

Planetary orientation models describe the orientation of the spin axis and prime meridian of planets in inertial space as a function of time. The models are required for the planning and execution of Earth-based or space-based observational work, e.g. to compute viewing geometries and to tie observations to planetary coordinate systems. The current orientation model for Mercury is inadequate be...

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ژورنال

عنوان ژورنال: Celestial Mechanics and Dynamical Astronomy

سال: 2009

ISSN: 0923-2958,1572-9478

DOI: 10.1007/s10569-009-9234-1