View source for Physics:Barycentric Dynamical Time

{{Short description|Linear scaling of Barycentric Coordinate Time}}
'''Barycentric Dynamical Time''' ('''TDB''', from the [[Social:French language|French]] '''<span dir="ltr" lang="fr">Temps Dynamique Barycentrique</span>''') is a relativistic [[Physics:Coordinate time|coordinate time]] scale, intended for astronomical use as a [[Physics:Time standard|time standard]] to take account of [[Physics:Time dilation|time dilation]]<ref>Explanations given with (a) [http://www.iau.org/static/resolutions/IAU1991_French.pdf IAU resolutions 1991], under Resolution A.4, at 'Notes for recommendation III', and [http://www.iau.org/static/resolutions/IAU2006_Resol3.pdf IAU 2006 resolution 3], and its footnotes; and (b) explanations and references cited at "[[Physics:Time dilation#Time dilation due to gravitation and motion together|Time dilation -- due to gravitation and motion together]]".</ref> when calculating orbits and [[Astronomy:Ephemeris|astronomical ephemerides]] of [[Astronomy:Planet|planet]]s, [[Astronomy:Asteroid|asteroid]]s, [[Astronomy:Comet|comet]]s and interplanetary [[Engineering:Spacecraft|spacecraft]] in the [[Astronomy:Solar System|Solar System]]. TDB is now (since 2006) defined as a linear scaling of [[Astronomy:Barycentric Coordinate Time|Barycentric Coordinate Time]] (TCB). A feature that distinguishes TDB from TCB is that TDB, when observed from the Earth's surface, has a difference from [[Astronomy:Terrestrial Time|Terrestrial Time (TT)]] that is about as small as can be practically arranged with consistent definition: the differences are mainly periodic,<ref name=clem67>The periodic differences, due to relativistic effects, between a coordinate time scale applicable to the Solar-System barycenter, and time measured at the Earth's surface, were first estimated and are explained in: G M Clemence & V Szebehely, [http://articles.adsabs.harvard.edu/abs/1967AJ.....72.1324C "Annual variation of an atomic clock"], Astronomical Journal, Vol.72 (1967), p.1324-6.</ref> and overall will remain at less than 2 milliseconds for several millennia.<ref>[http://www.iau.org/static/resolutions/IAU2006_Resol3.pdf IAU 2006 resolution 3], see Recommendation and footnotes, note 3.</ref>

TDB applies to the Solar-System-barycentric reference frame, and was first defined in 1976 as a successor to the (non-relativistic) former standard of [[Astronomy:Ephemeris time|ephemeris time]] (adopted by the IAU in 1952 and superseded 1976). In 2006, after a history of multiple time-scale definitions and deprecation since the 1970s,<ref>(a)P K Seidelmann & T Fukushima (1992), [http://articles.adsabs.harvard.edu/full/1992A%26A...265..833S "Why new time scales?"], ''Astronomy & Astrophysics'' vol.265 (1992), pages 833-838: and (b) IAU resolution (1991) A.4(recommendation V), which recommended limiting the use of TDB (previously defined 1976-79) to cases "where discontinuity with previous work is deemed to be undesirable".</ref> a redefinition of TDB was approved by the IAU. The 2006 IAU redefinition of TDB as an international standard expressly acknowledged that the long-established [[Astronomy:Ephemeris time#JPL ephemeris time argument Teph|JPL ephemeris time argument T<sub>eph</sub>]], as implemented in [[Organization:Jet Propulsion Laboratory Development Ephemeris|JPL Development Ephemeris]] DE405, "is for practical purposes the same as TDB defined in this Resolution"<ref>[http://www.iau.org/static/resolutions/IAU2006_Resol3.pdf IAU 2006 resolution 3], see footnotes, note 4.</ref> (By 2006, ephemeris DE405 had already been in use for a few years as the official basis for planetary and lunar ephemerides in the [[Astronomy:Astronomical Almanac|Astronomical Almanac]]; it was the basis for editions for 2003 through 2014; in the edition for 2015 it is superseded by DE430).<ref>See US Naval Observatory (Naval Oceanography Portal), [http://aa.usno.navy.mil/publications/docs/asa_history.php "History of the Astronomical Almanac"] {{Webarchive|url=https://web.archive.org/web/20090305231056/http://aa.usno.navy.mil/publications/docs/asa_history.php |date=2009-03-05 }} (accessed October 2015); also, for details of DE405:- E M Standish (1998), [ftp://ssd.jpl.nasa.gov/pub/eph/planets/ioms/de405.iom.pdf JPL Planetary and Lunar Ephemerides, DE405/LE405], Jet Propulsion Laboratory Interoffice Memorandum 312F-98-48, August 26, 1998; also, the Astronomical Almanac for 2015 commences use of the more  recent JPL ephemeris version DE430, which is now based expressly on TDB, see section L, especially page L-4 [https://books.google.com/books?id=Pr0H9aSEfKYC&pg=SL12-PA4 Astronomical Almanac for 2015, page L-4] (accessed October 2015).</ref>

==Definition==

IAU resolution 3 of 2006<ref>[http://www.iau.org/static/resolutions/IAU2006_Resol3.pdf IAU 2006 resolution 3]</ref> defines TDB as a linear transformation of [[Astronomy:Barycentric Coordinate Time|TCB]]. TCB diverges from both TDB and TT. TCB progresses faster at a differential rate of about 0.5 second/year, while TDB and TT remain close.<ref name=timgraf>[http://www.ucolick.org/~sla/leapsecs/deltat.png Fig. 1 at p.835, a graph giving an overview of the rate differences and offsets between various standard time scales], present and past, defined by the IAU: for description see P K Seidelmann & T Fukushima (1992), [http://articles.adsabs.harvard.edu/full/1992A%26A...265..833S "Why new time scales?"], ''Astronomy & Astrophysics'' vol.265 (1992), pages 833-838.</ref> As of the beginning of 2011, the difference between TDB and TCB is about 16.6 seconds.

:TDB = TCB − L{{sub|B}}×(JD{{sub|TCB}} − T{{sub|0}})×86400 + TDB{{sub|0}}

where L{{sub|B}} = 1.550519768{{E|−8}}, TDB{{sub|0}} = −6.55{{E|−5}} s, T{{sub|0}} = 2443144.5003725, and JD{{sub|TCB}} is the TCB [[Astronomy:Julian day|Julian date]] (that is, a quantity which was equal to T{{sub|0}} on 1977 January 1 00:00:00 [[Physics:International Atomic Time|TAI]] at the geocenter and which increases by one every 86400 seconds of TCB). 

==History==
{{seealso|Ephemeris time#History of ephemeris time (1952 standard)}}

From the 17th century to the late 19th century, planetary ephemerides were calculated using time scales based on the Earth's rotation: usually the mean solar time of one of the principal observatories, such as Paris or Greenwich. After 1884, mean solar time at Greenwich became a standard, later named [[Astronomy:Universal Time|Universal Time]] (UT). But in the later 19th and early 20th centuries, with the increasing precision of astronomical measurements, it began to be suspected, and was eventually established, that the rotation of the Earth (i.e. the length of the day) showed irregularities on short time scales, and was slowing down on longer time scales. [[Astronomy:Ephemeris time|Ephemeris time]] was consequently developed as a standard that was free from the irregularities of Earth rotation, by defining the time "as the independent variable of the equations of celestial mechanics", and it was at first measured astronomically, relying on the existing gravitational theories of the motions of the Earth about the Sun and of the Moon about the Earth.

After the caesium [[Engineering:Atomic clock|atomic clock]] was invented, such clocks were used increasingly from the late 1950s as [[Astronomy:Ephemeris time#Secondary realizations by atomic clocks|secondary realizations of ephemeris time (ET)]]. These secondary realizations improved on the original ET standard by the improved uniformity of the atomic clocks, and (e.g. in the late 1960s) they were used to provide standard time for planetary ephemeris calculations and in astrodynamics.

But ET in principle did not yet take account of relativity theory. The size of the periodic part of the variations due to [[Physics:Time dilation|time dilation]] between earth-based atomic clocks and the [[Physics:Coordinate time|coordinate time]] of the Solar-System barycentric reference frame had been estimated at under 2 milliseconds,<ref name=clem67/> but in spite of this small size, it was increasingly considered in the early 1970s that time standards should be made suitable for applications in which differences due to relativistic time dilation could no longer be neglected.

In 1976, two new time scales were defined<ref>They were defined in substance in 1976 but given their names in 1979.</ref> to replace ET (in the ephemerides for 1984 and afterwards) to take account of relativity. ET's direct successor for measuring time on a geocentric basis was Terrestrial Dynamical Time (TDT). The new time scale to supersede ET for planetary ephemerides was to be Barycentric Dynamical Time (TDB). TDB was to tick uniformly in a reference frame comoving with the [[Barycenter|barycenter]] of the Solar System. (As with any [[Physics:Coordinate time|coordinate time]], a corresponding clock, to coincide in rate, would need not only to be at rest in that reference frame, but also (an unattainable hypothetical condition) to be located outside all of the relevant [[Physics:Gravity well|gravity well]]s.) In addition, TDB was to have (as observed/evaluated at the Earth's surface), over the long term average, the same rate as TDT (now [[Astronomy:Terrestrial Time|TT]]). TDT and TDB were defined in a series of resolutions at the same 1976 meeting of the [[Organization:International Astronomical Union|International Astronomical Union]].

It was eventually realized that TDB was not well defined because it was not accompanied by a general relativistic metric and because the exact relationship between TDB and TDT had not been specified. (It was also later criticized as being not physically possible in exact accordance with its original definition: among other things the 1976 definition excluded a necessary small offset for the initial epoch of 1977.)<ref>E M Standish (1998), [http://articles.adsabs.harvard.edu/full/1998A%26A...336..381S "Time scales in the JPL and CfA ephemerides"], ''Astronomy and Astrophysics'', v.336 (1998), p.381-384.</ref> After the difficulties were appreciated, in 1991 the IAU refined the official definitions of timescales by creating additional new time scales: [[Astronomy:Barycentric Coordinate Time|Barycentric Coordinate Time]] (TCB) and [[Astronomy:Geocentric Coordinate Time|Geocentric Coordinate Time]] (TCG). TCB was intended as a replacement for TDB, and TCG was its equivalent for use in near-Earth space. TDT was also renamed to [[Astronomy:Terrestrial Time|Terrestrial Time]] (TT), because of doubts raised about the appropriateness of the word "dynamical" in that connection.

In 2006 TDB was redefined by IAU 2006 resolution 3; the 'new' TDB was expressly acknowledged as equivalent for practical purposes to [[Astronomy:Ephemeris time#JPL ephemeris time argument Teph|JPL ephemeris time argument T<sub>eph</sub>]]; the difference between TDB according to the 2006 standard and [[Astronomy:Terrestrial Time|TT]] (both as observed from the surface of the Earth), remains under 2 ms for several millennia around the present epoch.<ref>[http://www.iau.org/static/resolutions/IAU2006_Resol3.pdf IAU 2006 resolution 3], see especially footnotes 3 and 4.</ref>

==Use of TDB==

TDB is a successor of Ephemeris Time (ET), in that ET can be seen (within the limits of the lesser accuracy and precision achievable in its time) to be an approximation to TDB as well as to Terrestrial Time (TT) (see [[Astronomy:Ephemeris time#Implementations|Ephemeris time § Implementations]]). TDB in the form of the very closely analogous, and practically equivalent, time scale T<sub>eph</sub> continues to be used for the important DE405 planetary and lunar ephemerides from the [[Organization:Jet Propulsion Laboratory|Jet Propulsion Laboratory]].

Arguments have been put forward for the continued practical use of TDB rather than TCB based on the very small size of the difference between TDB and TT, not exceeding 0.002 second, which can be neglected for many applications. It has been argued that the smallness of this difference makes for a lower risk of damage if TDB is ever confused with TT, compared to the possible damage of confusing TCB and TT, which have a relative linear drift of about 0.5 second per year,<ref>S A Klioner (2008), "Relativistic scaling of astronomical quantities and the system of astronomical units", ''Astronomy and Astrophysics'', vol.478 (2008), pp.951-958, at page 953.</ref> (the difference was close to zero at the start of 1977, and by 2009 was already over a quarter of a minute and increasing).<ref name=timgraf/>

==References==
{{reflist}}

==External links==
* [http://aa.usno.navy.mil/publications/docs/Circular_179.pdf United States Naval Observatory Circular 179 : The IAU Resolutions on Astronomical Reference Systems, Time Scales, and Earth Rotation Models Explanation and Implementation] {{Webarchive|url=https://web.archive.org/web/20080216100325/http://aa.usno.navy.mil/publications/docs/Circular_179.pdf |date=2008-02-16 }}


{{Time measurement and standards}}

[[Category:General relativity]]
[[Category:Special relativity]]
[[Category:Time scales]]

{{Sourceattribution|Barycentric Dynamical Time}}