Per Harold:
Gayle Moholland, Director of the Unobskey
School in Calais, arranged with Asst. City Manager Jim Porter to
have the town maintenance crew move the 3100 pound astronomical transit
stone from the foot of the Calais Observatory knoll across from Dunkin
Donuts, back up to it's original position. The top of the stone, as I suspected,
matches the image from the publication. The crew that moved the stone
are Mark Magoon, David Townsend, and Dan Dineen.
The
stone is described as being smooth on top and the south side. The
observer would stand south (behind) the stone, his back toward Lincoln
Street, point the telescope at the Meridian Mark in St. Stephen, then
skyward. So the stone would be longer in the east-west direction. A
simple compass could be used to line up the stone in the east-west
direction, allowing for about a 20 degree declination. True North is
about 20 degrees right of where the compass points, if you are facing
north.
Per
Gayle:
The stone has been moved and is now resting in it's old home. There was
no bolt of any kind, but there are many letters and marks on it. It is
covered with mud on the side that was in the ground. I'll get that
cleaned off today.
There was no question as to where to set it. It fits snug as a bug
within the cut out area of the stone. The city crew did it for us.
Pictures are attached. I'll take more once I get the mud off it.
Click on photo to enlarge.
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| On
Our Way |
Nearing
Summit |
Inspecting
the Site |
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| How
We Gonna Do This? |
Final
List |
Almost
in Place |
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Transit
Stone Upright |
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The image below shows an Astronomical Transit sitting on what appears to
be a wooden box covered with material made in the same
manner as the stone at Calais. I am sure that some of
these were made from concrete at hundreds of Coast Survey
observatories around the world. Yes, concrete did exist
in 1857, there is a concrete pad, or rather 'beton' under the
Epping East Base stone. Are there any
Astronomical Transit's still in existence? Probably not,
as they were probably modified into Davidson Meridian
Transits. The Davidson transit could also make star
observations for Latitude, negating the need for the Zenith
Telescope such as used at Calais. The Coast Survey was
very frugal, and often times instruments were built and
rebuilt as technology changed. The Davidson
Meridian Instrument was replaced later by Bamberg and Wild T-4
astronomical instruments, so called 'broken back' instruments,
as you looked into the end of the trunnion to a mirror which
was in the main telescope I believe that the
crank below may have been used to 'transit' the instrument,
that is, flip it around 180 degrees so that reverse readings
could be made. Obviously, when a star passed the Calais
Meridian, you could not 'transit' the instrument and observe
on the same star. Therefore some stars were observed in
Direct mode, and some in Reverse mode. Note the two oil
lamps that shown via mirrors into the telescope tube. The Zenith
Telescope shown here, No. 4, IS the one used
at Calais in 1857. Latitude observations were not done
in 1866, that was just the serious business of finishing the
longitude work. The Smithsonian may have only the
photograph. . Also attached are
some images of an Astronomical Transit in the Smithsonian,
again showing the crank apparatus on bottom. I tossed in one
photo of Skip Theberge and the Wild T-4, the last instrument
used by C&GS for astronomic observations. This
replaced the Bamberg Transit. It would be
interesting if the Smithsonian would loan the Zenith Telescope
No. 4, and an Astronomical Transit in the future, perhaps at
the dedication of Meridian Park.........sorry folks, I have
yet to find a good image of a Hardy Clock, but there has to be
some Chronographic Registers out there. Please look for 3
indentations in the top of the stone that would accommodate
the footpads of the Zenith Telescope. They should be
equally spaced around a circle. The Astronomic
transit should have 4 indentations. Both instruments
were probably anchored down with plaster of paris. They might have
made some small drill holes to help hold the instrument in
place.
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| Astronomical
Transit |
Astronomical
Transit |
See
note below |
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Geodetic Transit
(Astronomic Transit)A
Catalogue number: PH*307210
Inscriptions: "Troughton & Simms,
London, 1849" and "U. S. C. S. No. 6"
Dimensions: telescope 3 inches aperture, 46
inches long; striding level 26 inches
Discussion: Troughton & Simms made this
instrument for the United States Coast Survey in 1849. It has a
double-cone horizontal axis, two lamps for illuminating this
axis, a large striding level, two small vertical circles
attached to the telescope tube, and a solid iron base. By 1880,
The Coast Survey had added the eccentric cam apparatus to the
base, to facilitate the reversal of the telescope.
Ref: "Determination of Time by Means of
the Transit Instrument," United States Coast and
Geodetic Survey Report (1880): 205-227 and pl. 62. |
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Zenith Telescope #4 |
| Skip Theberge |
Zenith Telescope
Catalogue number: PH*316660
Inscriptions: "Troughton & Simms,
London, 1849" and "U. S. C. S. Z. T. No. 4"
Dimensions: telescope 3.25 inches aperture, 46
inches long; horizontal circle 10.5 inches diameter; vertical
arc 5.5 inches radius
Discussion: This is the last of the four
zenith telescopes that Troughton & Simms made for the United
States Coast Survey, and that was used for the determination of
latitude by the Talcott method. It arrived in the United States
in 1849. When the Survey agreed join in the variation of
latitude (polar motion) program organized by the International
Geodetic Association and found that no other instruments were
available, it decided to have zenith telescopes No. 2 and No. 4
"remodeled at the Survey Office." Edwin Smith, chief
of the Instrument Division, explained that "every
precaution" was taken to make these instruments "as
perfect as possible under the circumstances." The new
features included: base and leveling screws; vertical axis; wyes
for horizontal axis of telescope, with adjustment for level;
larger horizontal axis for the telescope; new micrometer screw
and reconstruction of micrometer box and slide; improved clamp
to telescope; two fine levels attached to telescope; striding
level for the telescope axis. In addition, the whole instrument
was polished and bronzed, and provided with electric lamps and
batteries "for illumination of telescope field, the reading
of levels, etc." Zenith telescope No. 2 was used in Hawaii
in 1891-1892, while zenith telescope No. 4 was used at
Rockville, Md.
Ref: [E. Smith], "On the Variation of
Latitude at Rockville, Md., as Determined from Observations Made
in 1891 and 1892 in Cooperation with the International Geodetic
Association," United States Coast and Geodetic Survey
Report for 1892, Appendix No. 1, pp. 4-5, with illustration.
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