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Over its long history, the buildings of the Royal Observatory in Greenwich were enlarged and altered many times, reflecting changing needs and expectations of astronomers and funders, but also the constraints of a limited site and small budgets. The most significant expansion took place in the late nineteenth century, overseen by the eighth Astronomer Royal, William Christie, a programme that is put in the context of changing attitudes toward scientific funding, Christie's ambitious plans for the work and staffing of the Observatory and his desire to develop a national institution that could stand with more recently founded European and American rivals. Examination of the archives reveals the range of strategies Christie was required to use to acquire consent and financial backing from the Admiralty, as well as his opportunistic approach. While hindsight might lead to criticism of his decisions, Christie eventually succeeded in completing a large building – the New Physical Observatory – that, in its decoration, celebrated Greenwich's past while, in its name, style, structure and contents, it was intended to signal the institution's modernization and future promise.
In the early nineteenth century, Norwegian mathematician and astronomer Christopher Hansteen (1784–1873) contributed significantly to international collaboration in the study of terrestrial magnetism. In particular, Hansteen was influential in the origin and orientation of the magnetic lobby in Britain, a campaign which resulted in a global network of fixed geomagnetic observatories. In retrospect, however, his contribution was diminished, because his four-pole theory in Untersuchungen der Magnetismus der Erde (1819) was ultimately refuted by Carl Friedrich Gauss in Allgemeine Theorie des Erdmagnetismus (1839). Yet Hansteen's main contribution was practical rather than theoretical. His major impact was related to the circulation of his instruments and techniques. From the mid-1820s, ‘Hansteen's magnetometer’ was distributed all over the British Isles and throughout the international scientific community devoted to studying terrestrial magnetism. Thus in the decades before the magnetic crusade, Hansteen had established an international system of observation, standardization and representation based on measurements with his small and portable magnetometers.
In the late 1950s and early 1960s, the elite world of institutional British science attempted to take control of the BBC's management of science broadcasting. Delegations of scientists met BBC managers to propose an increased role for scientists in planning science broadcasts to a degree that threatened to compromise the BBC's authority and autonomy. The culmination was a set of proposals to the Pilkington Committee in 1960, principally from the Royal Society and the British Association for the Advancement of Science, under which a scientist-manager was to be appointed head of a unified science division in the BBC. BBC managers resisted these proposals. The outcome, in 1964, was a compromise giving the scientists little of what they wanted, and proving practically and strategically useful for the BBC. The article frames the story as a contest of jurisdiction between elite science and the BBC, and draws on scholarship relating to the social nature of authority and professions, and to the popularization of science. It shows the fundamentally different beliefs held by the scientists and the BBC about the purpose of science broadcasts and about the nature of the audience. The historical narrative is based on unpublished archive documents, and it contributes to the small but growing body of work on the historical background to the presentation of science in the broadcast media.
While the British Empire conventionally is recognized as a source of research subjects and objects in anthropology, and a site where anthropological expertise might inform public administration, the settler-colonial affiliations and experiences of many leading physical anthropologists could also directly shape theories of human variation, both physical and cultural. Antipodean anthropologists like Grafton Elliot Smith were pre-adapted to diffusionist models that explained cultural achievement in terms of the migration, contact and mixing of peoples. Trained in comparative methods, these fractious cosmopolitans also favoured a dynamic human biology, often emphasizing the heterogeneity and environmental plasticity of body form and function, and viewing fixed, static racial typologies and hierarchies sceptically. By following leading representatives of empire anatomy and physical anthropology, such as Elliot Smith and Frederic Wood Jones, around the globe, it is possible to recover the colonial entanglements and biases of interwar British anthropology, moving beyond a simple inventory of imperial sources, and crediting human biology and social anthropology not just as colonial sciences but as the sciences of itinerant colonials.
To those not engaged in the practice of scientific research, or telling the story of this enterprise, the image of empirical observation may conjure up images of boredom more than anything else. Yet surprisingly, the profoundly uninteresting nature of research to many science workers and readers in history has received little attention. This paper seeks to examine one moment of encroaching boredom: nineteenth-century positional astronomy as practised at leading observatories. Though possibly a coincidence, this new form of astronomical observation arose only a few decades before the English term ‘boredom’, for which the Oxford English Dictionary has no record prior to 1850. Through examining forms of observatory labour and publications, I offer in this paper an example of how boring work and reading helped shape a scientific discipline.