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A report of the Mercury & Venus Section (Director: P. G. Abel). Presented here is a short report discussing the observations communicated to the Director regarding the transit of Mercury which occurred in 2019. A number of interesting features were recorded by those BAA members who were able to observe the transit, which was a difficult one for UK-based observers.

The chance discovery of a letter from T. G. E. Elger (1836–1897) to the telescope maker G. Calver (1834–1927) has shed further light on Elger’s time at Manor Cottage, Kempston, Bedfordshire, between 1881 and 1890. This has enabled additional information to be added to the author’s biographical paper previously published in the Journal.1 The period he spent in residence at Manor Cottage appears to have been an important time in Elger’s life, both in relation to his continued support of selenography and to the establishment of the BAA Lunar Section.

The edge-rind artefact is a spurious defect commonly affecting the appearance of the sharper limb of Mars in digital images. Although frequently seen, very little has been written about its appearance or cause. This paper is an attempt to remedy this. It proposes that the artefact is primarily a diffraction effect, whose severity is related to the relative visibility of the Airy disc pattern, and accentuated by contrast-enhancing processing methods commonly used in planetary imaging. The artefact is possibly modified by effects such as variations in seeing, tube currents, optical aberrations or misalignments, as well as the presence of albedo regions ‘hidden’ at the edge of the planet.