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January 25, 20260 citations

Lunar reference systems and their realisations using INPOP ephemerides

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NRN. RambauxAFA. FiengaYSY. Seyffert

Key Points

  • The aim is to describe the lunar reference systems and assess the accuracy of their realizations in space and time.
  • Defined two lunar reference systems: Principal Axis (PA) and Mean Earth/Polar Axis (ME).
  • Realized the PA system using ephemerides based on lunar laser retro-reflectors.
  • Related the ME system to the PA system through rotation transformations.
  • Developed a transformation procedure based on series decomposition of librations and pole motion.
  • Estimated internal and external uncertainties of PA and ME systems using lunar laser retro-reflector positions.
  • Compared Euler angles and propagated their uncertainties.
  • Provided a new series of libration and polar motion data for lunar motion.

Abstract

Context. The definition of a reference system plays a crucial role in quantifying geodetic effects and in surface body cartography. Today, the development and specification of the lunar reference system is stimulated by future space missions, some of which will be manned, and by the needs of lunar space navigation. Aims. This paper aims to describe the lunar reference system in use and determine the accuracy of its realisation in space and time. At present, two lunar reference systems are defined: the Principal Axis system (PA system), based on the Moon’s principal axes of inertia, and the Mean Earth/Polar Axis (ME system), defined by the Earth’s mean position on the Moon surface. A first step towards a relativistic definition of the lunar time scale is also introduced in agreement with that proposed by the International Astronomical Union (IAU) and other recent realisations. Methods. We based the realisation of a PA lunar reference system on the choice of an ephemeris, which relied on the coordinates of the laser retro-reflectors on the Moon surface. We related the ME system and frame to the PA system and frame through a rotation transformation. This study provides a new method to determine the transformation procedure between the two systems, based on a series decomposition of librations and pole motion. Results. We used the comparisons of the position of the lunar laser retro-reflectors obtained with different ephemerides to estimate the internal and external uncertainties of the different realisations of the PA and ME systems. It also includes comparisons between Euler angles and the propagation of their uncertainties. Conclusions. This work provides the full expression of the transformation and a new series of libration and polar motion for the lunar motion. We also introduce possible realisations of lunar timescales, applicable depending on their use. The proposed procedure, with opportunities for future improvements, can help set new standards for lunar reference systems and their realisations.

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Cite This Study

Rambaux et al. (2026) studied this question.

synapsesocial.com/papers/6975b1eafeba4585c2d6d687https://doi.org/10.1051/0004-6361/202555962/pdf
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