It is useful to recall that the (late nineteenth-century) Baltimore Lectures of Lord Kelvin indicated that the likely sizes of atomic particles spanned almost two decades. Yet in the early years of the present century, Sir William Bragg's ansatz, together with the oil-drop e, gave the first reliable estimate of the scale of crystal interplanar spacings. The converse process of using an XRCD approach to obtain a value for the Avogadro constant was, prior to the advent of x-ray interferometry, limited by the need to connect optical and x-ray wavelengths before using the latter to estimate unit cell dimensions in crystals. Other limitations of these early measurements included the use of water as a density standard and the assignment of molar masses to individual specimens based on geochemical abundance averages. All these difficulties were overcome, in principle, with the application of x-ray/optical interferometry to the determination of lattice periods, the use of solid object density standards, and the determination of densities and isotopic abundances on individual monocrystalline specimens. While the present-day situation is addressed in other contributions to this workshop, the present essay attempts to place some of the early work in context and to look also to the future.
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