Barycentric Coordinate Time
This article needs additional citations for verification. (November 2007) |
Barycentric Coordinate Time (TCB, from the
TCB was defined in 1991 by the International Astronomical Union, in Recommendation III of the XXIst General Assembly.[1] It was intended as one of the replacements for the problematic 1976 definition of Barycentric Dynamical Time (TDB). Unlike former astronomical time scales, TCB is defined in the context of the general theory of relativity. The relationships between TCB and other relativistic time scales are defined with fully general relativistic metrics. The transformation between TCB and Geocentric Coordinate Time (TCG) may be approximated with an uncertainty not larger than in rate as:[2]
Because the reference frame for TCB is not influenced by the gravitational potential caused by the Solar System, TCB ticks faster than clocks on the surface of the Earth by 1.550505 × 10−8 (about 490 milliseconds per year). Consequently, the values of physical constants to be used with calculations using TCB differ from the traditional values of physical constants (The traditional values were in a sense wrong, incorporating corrections for the difference in time scales). Adapting the large body of existing software to change from TDB to TCB is an ongoing task, and as of 2002[update] many calculations continued to use TDB in some form.
Time coordinates on the TCB scale are specified conventionally using traditional means of specifying days, inherited from slightly non-uniform time standards based on the rotation of the Earth. Specifically, both
See also
References
- ^ "IAU(1991) Recommendation III". Archived from the original on 2007-09-27. Retrieved 2006-04-28.
- ^ Petit, Gerard. "Comparision [sic] of "Old" and "New" Concepts: Coordinate Times and Time Transformations". p. 23. Archived from the original on 2022-01-20.
- S2CID 32887246.