On 2011-07-11 12:43, Tony Finch wrote:

Quartz clocks can be more stable than Earth rotation: see for example
http://www.ieee-uffc.org/main/history.asp?file=marrison

  Thanks for this interesting reference!

   The first outstanding application of the quartz clock to astronomy was
   made in Germany with the installation at the Physikalisch-Technische
   Reichsanstalt. This was described by Scheibe and Adelsberger in 1932 and
   1934, and reports of its splendid performance continued periodically. It
   was with this installation that it was possible for the first time to
   observe and measure variations in the earth's rate occurring over
   intervals as short as a few weeks. Previous measurements of such
   variations, involving studies of motion of the moon, the planets, and
   Jupiter's satellites, had required years to obtain comparable
   information which, of course, by nature, could never reveal short-term
   factors.

  Yes, quartz clocks are much better than pendulum clocks in
  interpolating astronomical time between observations. But they
  are not good enough to establish an _independent_ time scale to
  which astromnomical time could be referred. Their long term
  stability is not good enough for that purpose (apparently even
  today, see eg McCarthy, Seidelmann: "TIME -- From Earth Rotation
   to Atomic Physics", page 151).

I thought this innovation was one of the reasons for moving to ephemeris
time as the basis for calibrating clocks, instead of relying on transit
instruments.

  Ephemeris time was introduced because the dynamical ephemeris (of
  the Moon mostly) at the time showed that its time coordinate
  differed from universal time, and this could no longer be ascribed
  to defects in the theory. Quartz clocks have been instrumental
  (since around 1937) in showing the variations of the length of day,
  which are the cause of the difference between UT and ET. And
  since the length of the second of UT in the early 19th century
  is not an easily reproducible definition, the second was redefined
  in 1954 using the rate of ET at 1900.0 (which is not so easy to
  reproduce either).

  But ephemeris time was deduced from astronomical observations of the
  Moon, not from quartz clocks. (Even today, astrometric observations
  of inertial time are not superfluous -- they reveal a slight
  difference between the rates d(TT) of TT and d(TAI) of TAI.)

  Michael Deckers.
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