USNO Circular 179 - U.S. Naval Observatory
USNO Circular 179 - U.S. Naval Observatory
USNO Circular 179 - U.S. Naval Observatory
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Chapter 2<br />
Time Scales<br />
Relevant IAU resolutions: A4.III, A4.IV, A4.V, A4.VI of 1991; C7 of 1994; B1.3, B1.5, B1.7, B1.8,<br />
B1.9, and B2 of 2000<br />
Summary The IAU has not established any new time scales since 1991, but more<br />
recent IAU resolutions have redefined or clarified those already in use, with no loss of<br />
continuity. There are two classes of time scales used in astronomy, one based on the<br />
SI (atomic) second, the other based on the rotation of the Earth. The SI second has<br />
a simple definition that allows it to be used (in practice or in theory) in any reference<br />
system. Time scales based on the SI second include TAI and TT for practical applications,<br />
and TCG and TCB for theoretical developments. The latter are to be used<br />
for relativistically correct dynamical theories in the geocentric and barycentric reference<br />
systems, respectively. Closely related to these are two time scales, TDB and Teph,<br />
used in the current generation of ephemerides. Time scales based on the rotation of<br />
the Earth include mean and apparent sidereal time and UT1. Because of irregularities<br />
in the Earth’s rotation, and its tidal deceleration, Earth-rotation-based time scales do<br />
not advance at a uniform rate, and they increasingly lag behind the SI-second-based<br />
time scales. UT1 is now defined to be a linear function of a quantity called the Earth<br />
Rotation Angle, θ. In the formula for mean sidereal time, θ now constitutes the “fast<br />
term”. The widely disseminated time scale UTC is a hybrid: it advances by SI seconds<br />
but is subject to one-second corrections (leap seconds) to keep it within 0. s 9 of UT1.<br />
That procedure is now the subject of debate and there is a movement to eliminate leap<br />
seconds from UTC.<br />
2.1 Different Flavors of Time<br />
The phrase time scale is used quite freely in astronomical contexts, but there is sufficient confusion<br />
surrounding astronomical times scales that it is worthwhile revisiting the basic concept. A time scale<br />
is simply a well defined way of measuring time based on a specific periodic natural phenomenon.<br />
The definition of a time scale must provide a description of the phenomenon to be used (what<br />
defines a period, and under what conditions), the rate of advance (how many time units correspond<br />
to the natural period), and an initial epoch (the time reading at some identifiable event). For<br />
example, we could define a time scale where the swing of a certain kind of pendulum, in vacuum at<br />
sea level, defines one second, and where the time 00:00:00 corresponds to the transit of a specified<br />
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