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Tuesday
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February 9, 2010
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Astrometry Department History
The Astrometry Department has existed in various forms since the 19th
century. For much of its history its main concern has been the
operation of transit circles. In the late 1950's two departments, the
six-inch transit circle and the seven-inch transit circle divisions,
were responsible for the operation of the two instruments and the data
analysis and production of the observational catalogs. The Equatorial
Division operated the 26- inch refractor, mostly for double star
research. In 1969 the seven- inch transit circle was sent to El
Leoncito, Argentina to observe the southern component of the
International Reference Stars, the SRS. The six-inch transit circle
observed the northern component of the IRS, the AGK3. At the time the
names of the divisions were changed to Northern and Southern Transit
Circle Divisions. In 1977 the seven-inch transit circle was returned
to Washington where an image dissector micrometer system was developed
and installed. The two Divisions were combined with the Equatorial
Division to produce the Astrometry Department. The seven-inch transit
circle was sent to Black Birch, New Zealand, to observe the second
epoch of the SRS, while the six-inch transit circle observed the IRS
in the North. An 8-inch twin (yellow and blue lens) astrograph was
acquired and sent to Black Birch to photograph the southern sky.
These projects ended in 1995 and the seven-inch transit circle was
removed from Black Birch and placed in storage in Washington. The
six-inch transit circle remains operational (and celebrated 100 years
of operation in 1997 with a brief set of measurements made by
T. Rafferty), but the successful operation of the European Hipparcos
satellite effectively obsoleted the transit circles. In 1997 the
astrograph mentioned above was fitted with a new "red" lens and a
4kx4k CCD camera and sent to Cerro Tololo, Chile to begin a program of
observing the southern sky to unprecedented accuracy from the ground.
6-inch Transit Circle
| Director | Tenure from | Tenure to |
| J. C. Hammond |
1911 |
December 31, 1933 |
| C. B. Watts |
1934 |
1959 |
| A. Norwood Adams |
1959 |
1969 |
| Benny L. Klock |
1969 |
1976* |
* see Transit Circle Division below.
9-inch Transit Circle
| Director | Tenure from | Tenure to |
| A. N. Skinner |
1894 |
1900 |
| F. B. Littell |
July 30, 1901 |
September 3, 1903 |
| W. S. Eichelberger |
September 3, 1903 |
September 30, 1908 |
| F. B. Littell |
October 1, 1908 |
November 11, 1913 |
| H. R. Morgan |
November 11, 1913 |
1944** |
** the 9-inch Transit Circle Division was decommissioned at Morgan's retirement
in 1944
7-inch Transit Circle
| Director | Tenure from | Tenure to |
| Francis P. Scott |
1948 |
June 12, 1970 |
| Jack L. Schombert |
1970 |
1976*** |
*** see Transit Circle Division below
In 1977 the transit circle instruments were placed under a single
Transit Circle Division.
Transit Circle Division
| Director | Tenure from | Tenure to |
| Jack L. Schombert |
1976 |
1977 |
| James A. Hughes |
1977 |
1982 |
In 1982 the Transit Circle Division became the Astrometry Department.
Astrometry Department
| Director | Tenure from | Tenure to |
| James Hughes |
1982 |
Jan. 15, 1992 |
| F. Stephen Gauss |
May 9, 1993 |
June 2,2000 |
| Theodore J. Rafferty |
October 8, 2000 |
June 15, 2002 |
| Ralph A. Gaume |
June 16, 2002 |
present |
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