High-precision Relativistic Timescales for Cislunar Navigation

Abstract We present a unified post-Newtonian framework for relativistic timing and coordinate transformations across the Barycentric, Geocentric, and Lunicentric Celestial Reference Systems ( LCRS ) and six timescales: Barycentric Coordinate Time ( TCB) , Geocentric Coordinate Time (TCG), Terrestrial Time (TT), Barycentric Dynamical Time ( TDB ), Lunicentric Coordinate Time ( TCL )​​​, and Lunar Time ( TL ). Following IAU Resolution II (2024), we implement an LCRS metric with time coordinate TCL , linked to TCB via the IAU B1.5 prescription with lunar quantities. We truncate all series to retain contributions above a fractional threshold of 5 × 10 −18 and timing terms exceeding 0.1 ps, expanding the lunar gravity to degree ℓ = 9 with Love number variations and including external tidal and inertial multipoles through the octupole. We derive closed-form mappings among TCB , TCG , TT , TDB , TCL, and TL, giving proper-to-coordinate time conversions and one-/two-way time-transfer corrections at subpicosecond accuracy. Secular rates and periodic perturbations from kinematic dilation, lunar monopole and multipoles, Earth tides, and gravitomagnetism are evaluated for clocks on the lunar surface in Very Low and Low Lunar Orbits, in elliptical lunar frozen orbits, at the Earth–Moon L1 point, and in Near-rectilinear Halo Orbits ( NRHOs ). Harmonics through ℓ = 9 and tides through ℓ = 8 suffice to meet 5 × 10 −18 stability in deep cislunar regimes (e.g., NRHO, L1), supporting subpicosend synchronization and centimeter-level navigation, whereas near-surface and Very Low Lunar Orbits require much higher degree (typically <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msub> <mml:mrow> <mml:mi>ℓ</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>max</mml:mi> </mml:mrow> </mml:msub> <mml:mo>≳</mml:mo> <mml:mn>300</mml:mn> </mml:math> ). The framework implements the IAU LCRS/TCL prescription and supplies accuracy budgets for high-precision time/frequency transfer, relativistic geodesy, quantum links, and fundamental tests beyond low Earth orbit.

Authors

Publication Details

Journal
The Astrophysical Journal
Published
2026-01-16
DOI
https://doi.org/10.3847/1538-4357/ae25ff
Citations
1
Primary Topic
Geophysics and Gravity Measurements
Type
article
Field-Weighted Citation Impact
28.32
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article

High-precision Relativistic Timescales for Cislunar Navigation

Slava G. Turyshev
1 citations
The Astrophysical Journal
Geophysics and Gravity Measurements
28.32
article

High-precision Relativistic Timescales for Cislunar Navigation

Slava G. Turyshev
article en
1 citations

Abstract

Abstract We present a unified post-Newtonian framework for relativistic timing and coordinate transformations across the Barycentric, Geocentric, and Lunicentric Celestial Reference Systems ( LCRS ) and six timescales: Barycentric Coordinate Time ( TCB) , Geocentric Coordinate Time (TCG), Terrestrial Time (TT), Barycentric Dynamical Time ( TDB ), Lunicentric Coordinate Time ( TCL )​​​, and Lunar Time ( TL ). Following IAU Resolution II (2024), we implement an LCRS metric with time coordinate TCL , linked to TCB via the IAU B1.5 prescription with lunar quantities. We truncate all series to retain contributions above a fractional threshold of 5 × 10 −18 and timing terms exceeding 0.1 ps, expanding the lunar gravity to degree ℓ = 9 with Love number variations and including external tidal and inertial multipoles through the octupole. We derive closed-form mappings among TCB , TCG , TT , TDB , TCL, and TL, giving proper-to-coordinate time conversions and one-/two-way time-transfer corrections at subpicosecond accuracy. Secular rates and periodic perturbations from kinematic dilation, lunar monopole and multipoles, Earth tides, and gravitomagnetism are evaluated for clocks on the lunar surface in Very Low and Low Lunar Orbits, in elliptical lunar frozen orbits, at the Earth–Moon L1 point, and in Near-rectilinear Halo Orbits ( NRHOs ). Harmonics through ℓ = 9 and tides through ℓ = 8 suffice to meet 5 × 10 −18 stability in deep cislunar regimes (e.g., NRHO, L1), supporting subpicosend synchronization and centimeter-level navigation, whereas near-surface and Very Low Lunar Orbits require much higher degree (typically <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msub> <mml:mrow> <mml:mi>ℓ</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>max</mml:mi> </mml:mrow> </mml:msub> <mml:mo>≳</mml:mo> <mml:mn>300</mml:mn> </mml:math> ). The framework implements the IAU LCRS/TCL prescription and supplies accuracy budgets for high-precision time/frequency transfer, relativistic geodesy, quantum links, and fundamental tests beyond low Earth orbit.

The Astrophysical JournalVol. 997(1)
Openalex Percentile: Top 2%
Geophysics and Gravity Measurements
28.32
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High-precision Relativistic Timescales for Cislunar Navigation — Slava G. Turyshev · The Astrophysical Journal (2026) | TGRS Research Map | TGRS