This article examines a 3.5-foot transit instrument crafted by John Bird and used at the Stockholm Observatory in the late 18th and early 19th centuries. It argues that the instrument functioned not as an isolated precision device but as part of an interconnected operating chain comprising regulator clocks, calibration tools, architectural infrastructure and established observational routines. By tracing its acquisition, installation and daily use, the study shows how precision in meridian astronomy – particularly in time determination – was achieved through the continual stabilisation of a fragile and labour-intensive system.
Johan Kärnfelt (Fri,) studied this question.