Terrestrial Time
Quick Summary
Terrestrial Time (TT) is a specialized timescale used to describe the motion of objects in space. It was formerly known as Terrestrial Dynamical Time (TDT) and is the successor to Ephemeris Time (ET). TT is defined as exactly 32.184 seconds offset from International Atomic Time (TAI) as of January 1, 1977. For times before 1955, TT is extrapolated backward using ET, which was based on the length of the tropical year in 1900. TT is crucial for geocentric ephemerides, which are tables of the predicted positions of celestial bodies.1
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Terrestrial Time (TT)—formerly Terrestrial Dynamical Time (TDT), the successor to Ephemeris Time (ET)—is the theoretical timescale of geocentric ephemerides, and it is specified as TT = TAI* + 32.184 seconds, where TAI* denotes a reprocessed computation of International Atomic Time (TAI) and the 32.184-second offset…
Read MoreTerrestrial Time (TT)—formerly Terrestrial Dynamical Time (TDT), the successor to Ephemeris Time (ET)—is the theoretical timescale of geocentric ephemerides, and it is specified as TT = TAI* + 32.184 seconds, where TAI* denotes a reprocessed computation of International Atomic Time (TAI) and the 32.184-second offset…
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timeTDB and TDTTerrestrial Dynamical Time (TDT) is an auxiliary scale defined by the equation TDT = TAI + 32.184 s. Its unit is the SI second. The constant difference between TDT and TAI makes TDT continuous with ET for periods before TAI was defined (mid-1955). TDT is…
Read MoreTerrestrial Dynamical Time (TDT) is an auxiliary scale defined by the equation TDT = TAI + 32.184 s. Its unit is the SI second. The constant difference between TDT and TAI makes TDT continuous with ET for periods before TAI was defined (mid-1955). TDT is…
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