1.
where T is time in seconds, l is string length in centimeters, and G is
gravity.
2. solar day  24 hours (variable).
3. sidereal day  23 hours, 56 minutes, 4.09 seconds.
4. mean solar day  average solar day across a year 
24 hours on average.
5. second (old measure of)  1/86,400 of the mean solar
day.
6. second (present measure of)  9,192,631,770 periods of the
radiation corresponding to the transition between the two hyperfine levels
of the ground state of the cesium133 atom.
7. Coordinated Universal Time (UTC)weighted average of the various
atomic time scales.
8. Ephemeris Time  is determined by the orbital motion of the
Earth about the Sun (not affected by earth's rotational wobble).
9. Universal Time (UT0)  is equivalent to mean solar time at
the Greenwich Meridian (Greenwich Mean Time, or GMT).
10. The Earth requires 4 minutes to bring Sun back into same
point of sky every day. (Solar Day)
11. Stars set and rise on sidereal schedule.
12. Atomic time, with the unit of duration the Systeme International
(SI) second defined as the duration of 9,192,631,770 cycles of radiation
corresponding to the transition between two hyperfine levels of the ground
state of cesium 133.
13. TAI is the International Atomic Time scale, a statistical
timescale based on a large number of atomic clocks.
14. Universal time (UT) is counted from 0 hours at midnight, with unit of
duration the mean solar day, defined to be as uniform as possible
despite variations in the rotation of the Earth.
15. UT0 is the rotational timescale of a particular place
of observation. It is observed as the diurnal motion of stars or extraterrestrial
radio sources.
16. UT1 is computed by correcting UT0 for the effect of
polar motion on the longitude of the observing site. It varies from
uniformity because of the irregularities in the Earth's rotation.
17. Coordinated Universal Time (UTC) differs from TAI
by an integral number of seconds. UTC is kept within 0.9 seconds of UT1
by the introduction of onesecond steps to UTC, the "leap second"
usually being a positive step.
18. Dynamical Time replaced ephemeris time as the independent
argument in dynamical theories and ephemerides. Its unit of duration is
based on the orbital motions of the Earth, Moon, and planets.
19. Terrestrial Time (TT), (or Terrestrial Dynamical Time,
TDT), with unit of duration 86400 SI seconds on the geoid, is the independent
argument of apparent geocentric ephemerides. TDT= TAI + 32.184 seconds.
20. Barycentric Dynamical Time (TDB), is the independent
argument of ephemerides and dynamical theories that are referred to the
solar system barycenter. TDB varies from TT only by periodic variations.

21. Geocentric Coordinate Time (TCG) is a coordinate time
having its spatial origin at the center of mass of the Earth. TCG
differs from TT as: TCG  TT = Lg * (JD 2443144.5) * 86400 seconds, with
Lg = 6.969291e10.
22. Barycentric Coordinate Time (TCB)is a coordinate time
having its spatial origin at the solar system barycenter. TCB differs
from TDB in rate. The two are related by: TCB  TDB =Lb * (JD 2443144.5)
* 86400 seconds, with Lb =1.550505e08.
23. Sidereal Time, with unit of duration the period of
the Earth's rotation with respect to a point nearly fixed with respect
to the stars, is the hour angle of the vernal equinox.
24. Delta T is the difference between Earth rotational
time (UT1) and dynamical time (TDT). Predicted values of TDT  UT are provided
by the Earth Orientation Department.
25. Julian Day Number is a count of days elapsed since
Greenwich mean noon on 1 January 4713 B.C., Julian proleptic calendar.
The Julian Date is, then, the Julian day number followed by the fraction
of the day elapsed since the preceding noon.
26. We frequently make use of the Modified Julian Date
(MJD), which is defined as MJD =JD  2400000.5.
27. A MJD day thus begins at midnight, civil date. Julian
dates can be expressed in UT, TAI, TDT, among others, and so for precise applications
the timescale should be specified, for example, MJD 49135.3824 TAI.
28. one (1) mean solar day = 1.0027379093 sidereal days.
29. sidereal month  27.3 days (one moon revolution).
30. lunar month  29.5 days (time between full moons).
31. sidereal revolution period  revolution relative to stars.
32. synodic revolution period  oribital period as seen from earth.
33. SRP  one sidereal day.
34. SyRP  one solar day.
35. leap second  compensation in atomic clocks for earth's irregular
rotational period.
36. millennium  1000 years.
37. century  100 years.
38. decade  10 years.
39. leap year  366 days.
40. year  365 days.
41. hour  60 minutes.
42. minute  60 seconds.
43. millisecond  .001 seconds (1E3).
44. microsecond  .000001 seconds (1E6).
45. nanosecond  1E9 seconds.
46. picosecond  1E12 seconds.
47. femtosecond  1E15 seconds.
48. attosecond  1E18 seconds.
