Acquired during the reporting year 1939/40 (1 May 1939 – 30 April 1940), the telescope was installed in the Altazimuth Pavilion. Mounted on a brick pier specially constructed for it on top of the existing pier, it replaced Christie’s Altazimuth Telescope, which was removed to make way for it.
The telescope ‘was broken in half when thrown from its mounting’ when the Pavilion was struck by enemy action on the night of October 21/22 October 1940, though the object glass was undamaged.
The impersonal micrometer that had belonged to the instrument was fitted to the Bamberg Broken Transit in the reporting year 1946/7 prior to that instrument being brought into use with the Time Service at Abinger.
The origin and proposed use of the telescope was described by Spencer Jones in his 1940 Annual Report to the Board of Visitors. It has been transcribed below:
‘A small transit Instrument made by Messrs. Cooke, Troughton and Simms Ltd. has been purchased from the Crown Agents for the Colonies. This instrument was constructed for time determinations at Singapore but was not used as it found that time to a sufficient degree of accuracy could be obtained by recording time signals from various countries. The instrument is of more modern design than the small transit instruments hitherto used as [at] the Observatory, which were constructed for use by expeditions to observe the Transit of Venus in 1874. After thorough overhaul In the workshop and the fitting of a new contact wheel to the impersonal micrometer, to change from a. ‘make’ to a ‘break’ circuit, the telescope was mounted in the the Altazimuth dome. A personal equation machine is under construction in the workshop and will be fitted to the south collimator [of the Altazimuth]. An artificial star will be travelled along in either direction by a geared reversible motor; a gear box is provided to enable the star to be moved at a rate corresponding to the speed of an equatorial star, or to one-half or one-quarter of that speed. The north collimator will be used to provide a check on the stability in azimuth of the telescope. It is hoped that observations with the two small transit instruments [this one and the one used for time determinations in the Transit Pavilion] on the same night, in conjunction with observations with the Reversible Transit Circle, will give some information about fluctuating errors of instrumental origin.’