Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Barycentric Coordinate Time

From Wikipedia, the free encyclopedia
Time standard for calculations pertaining to orbits
icon
This articleneeds additional citations forverification. Please helpimprove this article byadding citations to reliable sources. Unsourced material may be challenged and removed.
Find sources: "Barycentric Coordinate Time" – news ·newspapers ·books ·scholar ·JSTOR
(November 2007) (Learn how and when to remove this message)

Barycentric Coordinate Time (TCB, from theFrenchTemps-coordonnée barycentrique) is acoordinatetime standard intended to be used as the independent variable of time for all calculations pertaining to orbits ofplanets,asteroids,comets, and interplanetaryspacecraft in theSolar System. It is equivalent to theproper time experienced by a clock at rest in a coordinate frameco-moving with thebarycenter (center of mass) of the Solar System[citation needed]: that is, a clock that performs exactly the same movements as the Solar System but is outside the system'sgravity well. It is therefore not influenced by thegravitational time dilation caused by theSun and the rest of the system.TCB is the time coordinate for theBarycentric Celestial Reference System (BCRS).

TCB was defined in 1991 by theInternational Astronomical Union, in Recommendation III of the XXIst General Assembly.[1] It was intended as one of the replacements for the problematic 1976 definition ofBarycentric Dynamical Time (TDB). Unlike former astronomical time scales, TCB is defined in the context of thegeneral theory of relativity. The relationships between TCB and other relativistic time scales are defined with fullygeneral relativistic metrics. The transformation between TCB andGeocentric Coordinate Time (TCG) may be approximated with an uncertainty not larger than5×1018{\displaystyle 5\times 10^{-18}} in rate as:[2]

TCBTCG=c2[t0t(vE22+w0ext(xE))dt+vEirEi]c4[t0t(18vE432vE2w0ext(xE)+4vEiwexti(xE)+12w0ext2(xE))dt(3w0ext(xE)+vE22)vEirEi]{\displaystyle {\begin{aligned}TCB-TCG&=c^{-2}\left[\int _{t_{0}}^{t}\left({\frac {v_{E}^{2}}{2}}+w_{0ext}(\mathbf {x} _{E})\right)dt+v_{E}^{i}r_{E}^{i}\right]\\&-c^{-4}\left[\int _{t_{0}}^{t}\left(-{\frac {1}{8}}v_{E}^{4}-{\frac {3}{2}}v_{E}^{2}w_{0ext}(\mathbf {x} _{E})+4v_{E}^{i}w_{ext}^{i}(\mathbf {x} _{E})+{\frac {1}{2}}w_{0ext}^{2}(\mathbf {x} _{E})\right)dt\right.\\&\qquad \qquad \left.-\left(3w_{0ext}(\mathbf {x} _{E})+{\frac {v_{E}^{2}}{2}}\right)v_{E}^{i}r_{E}^{i}\right]\end{aligned}}}wherexEi{\displaystyle x_{E}^{i}} andvEi{\displaystyle v_{E}^{i}} are the barycentric coordinate position and velocity of the geocenter,rEi=xixEi{\displaystyle r_{E}^{i}=x^{i}-x_{E}^{i}} withxi{\displaystyle x^{i}} the barycentric position of the observer,t=TCB{\displaystyle t=TCB},t0{\displaystyle t_{0}} is the origin of TCB and TCG defined so that 1977 January 1, 00:00:00TAI is 1977 January 1, 00:00:32.184 TCG / TCB,w0ext(xE){\displaystyle w_{0ext}(\mathbf {x} _{E})} is the sumAGMArA{\displaystyle \scriptstyle \sum _{A}{\frac {GM_{A}}{r_{A}}}} ofgravitational potentials for all solar system bodies apart from the Earth evaluated at the geocenter, andwexti(xE){\displaystyle w_{ext}^{i}(\mathbf {x} _{E})} is similarly the sumAGMArAvAi{\displaystyle \scriptstyle \sum _{A}{\frac {GM_{A}}{r_{A}}}v_{A}^{i}}. The approximation discards higher powers ofrEi{\displaystyle r_{E}^{i}} as they have been found to be negligible.[3]

Because the reference frame for TCB is not influenced by thegravitational 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, bothJulian Dates and theGregorian calendar are used. For continuity with its predecessorEphemeris Time, TCB was set to match ET at around Julian Date 2443144.5 (1977-01-01T00Z). More precisely, it was defined that TCB instant 1977-01-01T00:00:32.184 corresponds exactly to theInternational Atomic Time (TAI) instant 1977-01-01T00:00:00.000, at thegeocenter. This is also the instant at which TAI introduced corrections for gravitational time dilation.

See also

[edit]

References

[edit]
  1. ^"IAU(1991) Recommendation III". Archived fromthe original on 2007-09-27. Retrieved2006-04-28.
  2. ^Petit, Gerard."Comparision [sic] of "Old" and "New" Concepts: Coordinate Times and Time Transformations". p. 23. Archived fromthe original on 2022-01-20.
  3. ^Soffel, M.; Klioner, S. A.; Petit, G.; Wolf, P.; Kopeikin, S. M.; Bretagnon, P.; Brumberg, V. A.; Capitaine, N.; Damour, T.; Fukushima, T.; Guinot, B.; Huang, T.-Y.; Lindegren, L.; Ma, C.; Nordtvedt, K.; Ries, J. C.; Seidelmann, P. K.; Vokrouhlick, D.; Will, C. M.; Xu, C. (December 2003)."The IAU 2000 Resolutions for Astrometry, Celestial Mechanics, and Metrology in the Relativistic Framework: Explanatory Supplement".The Astronomical Journal.126 (6):2687–2706.arXiv:astro-ph/0303376.Bibcode:2003AJ....126.2687S.doi:10.1086/378162.S2CID 32887246.
International standards
template illustration
template illustration
Obsolete standards
Time in physics
Horology
Calendar
Archaeology and geology
Astronomical chronology
Otherunits of time
Related topics
Retrieved from "https://en.wikipedia.org/w/index.php?title=Barycentric_Coordinate_Time&oldid=1269979281"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp