Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Ephemeris time
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==JPL ephemeris time argument T<sub>eph</sub>== High-precision [[ephemeris|ephemerides]] of sun, moon and planets were developed and calculated at the [[Jet Propulsion Laboratory]] (JPL) over a long period, and the latest available were adopted for the ephemerides in the [[Astronomical Almanac]] starting in 1984. Although not an IAU standard, the ephemeris time argument T<sub>eph</sub> has been in use at that institution since the 1960s. The time scale represented by T<sub>eph</sub> has been characterized as a [[principle of relativity|relativistic]] coordinate time that differs from [[Terrestrial Time]] only by small periodic terms with an amplitude not exceeding 2 milliseconds of time: it is linearly related to, but distinct (by an offset and constant rate which is of the order of 0.5 s/a) from the [[Barycentric Coordinate Time|TCB]] time scale adopted in 1991 as a standard by the [[IAU]]. Thus for clocks on or near the [[geoid]], T<sub>eph</sub> (within 2 milliseconds), but not so closely TCB, can be used as approximations to Terrestrial Time, and via the standard ephemerides T<sub>eph</sub> is in widespread use.<ref name="EMS1998"/> Partly in acknowledgement of the widespread use of T<sub>eph</sub> via the JPL ephemerides, IAU resolution 3 of 2006<ref>{{cite web| url = http://www.iau.org/static/resolutions/IAU2006_Resol3.pdf| title = IAU 2006 resolution 3}}</ref> (re-)defined [[Barycentric Dynamical Time]] (TDB) as a current standard. As re-defined in 2006, TDB is a linear transformation of [[Barycentric Coordinate Time|TCB]]. The same IAU resolution also stated (in note 4) that the "independent time argument of the JPL ephemeris [[DE405]], which is called T<sub>eph</sub>" (here the IAU source cites<ref name="EMS1998"/>), "is for practical purposes the same as [[Barycentric Dynamical Time|TDB]] defined in this Resolution". Thus the new TDB, like T<sub>eph</sub>, is essentially a more refined continuation of the older ephemeris time ET and (apart from the {{nowrap|< 2 ms}} periodic fluctuations) has the same mean rate as that established for ET in the 1950s.
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Ephemeris time
(section)
Add topic