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Greg Smye-Rumsby
2003

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Elevation view
The Accuracy
The Movement
The Difficulties
The Lens

The Telescope

Illustration of Craig's Telescope
possibly by G. F. Sargent
courtesy Corporation of London ©

The telescope was of a novel design - slung on a pulley on the outside of a tall brick tower.

By carefully reconstructing the plans of the basic telescope, it is possible to begin to understand how the telescope operated and discover some interesting facts about its limitations.

The tube was constructed very much in the manner of a steam ship of the time, having separate panels of steel riveted together along seams. The great length of the tube would have required internal strengthening otherwise it would tend to sag.

Wandsworth Prison
A photograph of Wandsworth Prison today.

In some of the journal and press reports of the time there were references to the angles of inclination to which the telescope could be positioned. However, on examination of the construction plans, it becomes clear that the telescope was unlikely to have been able to point to the horizon or indeed any higher than about 74° from horizontal: even after having allowed for some licence in the dimensions of the tower (the brickwork may have measured 64 feet in height, but this figure may not have included the rotating wooden roof structure). Indeed the telescope could not be raised any higher whatever the height of the tower, because the dimensions of the cradle hoop supporting the telescope tube would have become prohibitive!

The tower was made of brick, but what type and colour. On the site of the old assylum north of the telelscope, Wandsworth Prison was built just a few years before the telescope. The bricks for this came from Frying Pan brickworks. It may be that for simplicity's sake the bricks for the tower came also from this source.

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Telescope elevation
The telescope shown in elevation
.

plan movie of rotation

This plan view shows part of the outer ring to the right and the central tower supporting the telescope toward the left.

fine movement
medium movement
full rotational movement

The operator could simply move the end of the 'scope with small lateral movements using the eyepiece "dolly" controls. Greater sweeps of the sky would require the rotation of the tower top and base.

The Accuracy

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Since the telescope appeared not to have any means of calibration with reference to the sky, all the target objects to which the telescope was pointed needed to be visible to the naked eye. There did not seem to be a system for acurately pointing the instrument - there was no finderscope to speak of. Although not shown in the limited illustrations, there may have been some kind of simple viewing tube or primitive "gunsight".

In order to set the telescope to a particular azimuth, the observer may have placed marker flags around the perimeter of the azimuth rail. However, the accuracy of this particular method would only have been made less uncertain if the altazimuth housing at the top of the tower also had some kind of calibration.

The Movement

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Moving the 'scope around would probably have required a "knack". Since the eyepiece end of the tube rested in a sling on a wooden "dolly", small pointing corrections would have been undertaken by simply slewing the 'scope "left and right" and "up and down" one or two degrees without having to move any other part of the instrument. Indeed, with some training, tracking something like Venus or the Moon, would have become second nature.

It seems that from the little technical information we have, there are several ways to move the whole telescope. It would certainly have been easier with several people to assist, but essentially it could just about have been operated by just one individual!

Firstly, the telescope would have been readied for use. This would have required removing the lens cover, releasing the "brakes" on the azimuth armature and those at the top of the tower in the rotable wooden altazimuth housing. After attaching the large 3-metre steel dewcap (this may have required assistance!), the operator would then have winched up the tube from its near-horizontal "parking" position and attached the eyepiece unit.

Front elevationThe operator would then have rotated the whole instrument, bringing it to within a few degrees of the correct position by pulling on "reigns" attached to the altazimuth housing while nudging the azimuth armature as he / she walked around the tower. Once this course setting had been made to the azimuth, the "reigns" would have been tied up to the azimuth "dolly", this in turn would have been pushed either away from the tower or toward it - depending on the altitude of the observation. It has to be remembered that the inward/outward movement of the "dolly" has to be accompanied by the raising or lowering of the telescope tube - this is achieved by turning the handle on the small winch on the opposite side of the tower. Although the telescope is said to have weighed about three tons it was counterweighted, therefore the effort in changing its inclination would have required little effort.

If the winch "reeved" rope onto a drum, it would only have required two or three turns at any one time. Indeed the rope would have passed from the underside of the telescope tube down to ground level, passing through a system of guide wheels attached to the underside of the track around the tower to the opposite side, onto the winch and then up vertically to the underside of the counterweight.

Once it was ascertained that the target object was nearly in the telescope's field of view, the azimuth armature could have been moved perhaps as much as ten degrees without having to rotate the tower (much more than this, the telescope tube would have made contact with the tower, the torque on the instrument would then have become dangerous!). The smallest of adjustments to the eyepiece "dolly" would then have brought the target object into view.

At the top of the tower is the altazimuth housing, this is designed to hold the telescope tube while allowing it to be raised and lowered and also rotated to the correct azimuth bearing. Around the outside of the structure there appear to be four grilled openings, spaced at 90° intervals. These could have been used as communication ports. So, to facilitate the easier use of the 'scope, an assistant would have remained in the tower during use. Instructions would have been "yelled" up from the ground. Instead of using the "reigns" to position the tower in azimuth, the assistant would have simply moved the tower around by hand. A good idea would have been to mark compass bearings on the static rail inside the housing, sadly this would not have been very useful as the telescope itself was not directly in contact with the tower!

The Difficulties

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As has already been seen the telescope was not the easiest of instruments to use. The telescope could only be operated during fair weather with extremely light winds.

Although the tower could have its floors weighted to provide vibration damping, the external chains supporting the tube may have resonated much in the manner of a guitar string.

It is interesting, but in the illustration by Sargent, small flags are shown attached to the "reigns" at regular intervals. These could be for many reasons. Apart from decoration, they may have been to scare birds so their acidic droppings did not rot the ropes, the may also have been for crude calibration of the telescope tube in some way or they may have been to dampen vibration from wind.

One aspect of the 'scope that might have played a role in damping, was its shear weight!

The Lens

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As the lens' whereabouts is unknown at present it is only possible to use references from publications at the time to guess as to what may have been so wrong with it.

The LensThe lens was made by Mr. F. Slater of Somers Place in Euston Square. It was a composite of two pieces of glass, one of flint and the other of plate. The plate glass lens had a positive focal length of 9,182mm, the fractive index being 15103. The flint glass component had a negative focal length of 15,201.9mm with a refractive index of 16308. Combined, they formed an achromatic lens (reduced colour fringing especially at the edge of the field) with a focal length of 23,164.8mm.

We know it was 24-inches in diameter - a huge size for the time. There have also been references to the fact that on many occasions in order for it to work at all, it needed to be stopped out (masking the central part of the lens and only allowing light to pass through the outer circumference). Certainly any error in figuring could have easily been corrected. Alas, this appears never to have been underatken!!

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