In the 1820s, Stockholm Observatory undertook a significant upgrade of its instruments. The new acquisitions included a meridian circle, crafted by Traugott Ertel in Munich, which – after extensive delays – was finally installed at the observatory in 1834. Despite its advanced capabilities, the instrument saw limited use during its first forty years, as observatory directors were largely occupied with geodetic projects for the Crown. The meridian circle only reached its full scientific potential when Hugo Gyldén became the Academy Astronomer in 1871, marking the end of the Observatory's geodetic era. In addition to observations for a major zone project, from 1879 the instrument became the engine of the Swedish standard time system. Throughout the nineteenth century it also had an important role as the zero meridian for the military's geodetic pursuits. The instrument remained in use until the Observatory relocated to Saltsjöbaden in 1931. This paper explores the various roles played by the Ertel meridian circle during its century-long history, with a focus on the strategies employed by astronomers to preserve the ageing instrument's relevance.
Johan Kärnfelt (Sun,) studied this question.
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