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coordinate-time-systems

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UpdatedJune 23, 2026 at 08:46

Reason about coordinate reference frames and time scales correctly (any astrodynamics work) — which frame/scale/representation a value is actually in, the concerns to resolve before trusting it, and what to look up. Use when interpreting or choosing frames (ECI/ECEF, GCRS/ITRS/CIRS/TIRS, J2000/EME2000, TEME, ICRF, LVLH/RTN/RSW, body-fixed), time scales (TAI/UTC/UT1/TT/TDB/GPS), or state representations (Cartesian/Keplerian/equinoctial); or when reasoning about frame/scale conversions, covariance transforms, interpolation, leap seconds, ERA/GMST/GAST, EOP/ΔUT1, polar motion, frame bias, or realizations — and also when reviewing or verifying frame/time/coordinate work (use it as a checklist of the traps, even for code you could write unaided). The companion skill `coordinate-time-implementation` covers expressing and testing these in orts/arika code.

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