Lunar Time in General Relativity
Sergei M. Kopeikin, George H. Kaplan

TL;DR
This paper develops a relativistic framework for defining and transforming Lunar Coordinate Time (TCL) relative to Geocentric Coordinate Time (TCG), enabling precise lunar clock synchronization accounting for relativistic effects within the Earth-Moon system.
Contribution
It introduces a new relativistic TCL--TCG transformation algorithm that accounts for multiple gravitational and kinematic effects with nanosecond precision.
Findings
The algorithm accurately models lunar clock variations relative to Earth clocks.
Validation confirms the equivalence of TCL formalism with local inertial frame approaches.
Achieves nanosecond-level precision within the Earth's Hill sphere.
Abstract
We introduce the general-relativistic definition of Lunar Coordinate Time (TCL) based on the IAU 2000 resolutions that provide a framework for relativistic reference systems. From this foundation, we derive a transformation equation that describes the relative rate of TCL with respect to Geocentric Coordinate Time (TCG) for various locations of the clock on lunar surface. This equation serves as the cornerstone for constructing a relativistic TCL--TCG time conversion algorithm. Using this algorithm, we can compute both secular and periodic variations in the rate of an atomic clock placed on the Moon, relative to an identical clock on Earth. The algorithm accounts for various effects, including time dilation caused by the Moon's orbital motion around Earth, gravitational potentials of both Earth and Moon, and direct and indirect time dilation effects due to tidal perturbations caused by…
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Taxonomy
TopicsRelativity and Gravitational Theory · History and Developments in Astronomy · Cosmology and Gravitation Theories
