The following time conversions are accurate at the millisecond level.
Some are exact while others have differences at the microsecond level.
| System |
Description |
UT1 |
UTC |
TT |
TAI |
GPS |
| UT1 |
Mean Solar Time |
UT1 |
UTC = UT1 - DUT1 |
TT = UT1 + 32.184 s + LS - DUT1 |
TAI = UT1 - DUT1 + LS |
GPS = UT1 - DUT1 + LS - 19 s |
| UTC |
Civil Time |
UT1 = UTC + DUT1 |
UTC |
TT = UTC + 32.184 s + LS |
TAI = UTC + LS |
GPS = UTC + LS - 19 s |
| TT |
Terrestrial (Ephemeris) Time |
UT1 = TT - 32.184 s - LS + DUT1 |
UTC = TT - 32.184 s - LS |
TT |
TAI = TT - 32.184 s |
GPS = TT - 51.184 s |
| TAI |
Atomic Time |
UT1 = TAI + DUT1 - LS |
UTC = TAI - LS |
TT = TAI + 32.184 s |
TAI |
GPS = TAI - 19 s |
| GPS |
GPS Time |
UT1 = GPS + DUT1 - LS + 19 s |
UTC = GPS - LS + 19 s |
TT = GPS + 51.184 s |
TAI = GPS + 19 s |
GPS |
Definitions:
- LS = TAI - UTC = Leap Seconds from http://maia.usno.navy.mil/ser7/tai-utc.dat
- DUT1 = UT1 - UTC from http://maia.usno.navy.mil/ser7/ser7.dat or http://maia.usno.navy.mil/search/search.html
[edit] Sidereal time
Sidereal time
is the measurement of time relative to a distant star (instead of solar
time that is relative to the sun). It is used in astronomy to predict
when a star will be overhead. Due to the orbit of the earth around the
sun a sidereal day is 4 minutes (1/366th) less than a solar day.
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