RUSSELL R.A., John, London, 1797
RUSSELL R.A., John, London, 1797

Details
RUSSELL R.A., John, London, 1797
A GLOBE representing the VISIBLE SURFACE of the MOON constructed from TRIANGLES measured with a MICROMETER and accurately drawn and engraved from a long series of TELESCOPIC OBSERVATIONS by J. Russell, R.A.
BY HIS MAJESTY'S LETTERS PATENT, This Globe being part of the APPARATUS named the SELONOGRAPHIA, designed to exhibit the Lunar Libration &c. is Published by the Author, Newman Street, London June 14th.1797

An extremely rare 12-inch (30.5cm.) diamter lunar globe, made up of twelve hand-coloured stipple-engraved paper gores extending from lunar east to west, and two polar calottes, showing the lunar equator and Prime Meridian ungraduated, the craters, seas and mountains shaded to show relative heights but unnamed, some main craters marked with a cross, the back-side of the moon left blank save the two descriptive cartouches (neatly repaired crack to southern hemisphere of back-side), mounted by means of a screwed-on mahogany disc at the southern celestial pole, to a short turned pillar and circular plinth base with three bun feet -- 20in. (50.8cm.) high

See Front Cover, Colour Illustration and Details

Literature
DEKKER, Elly, Globes at Greenwich (Oxford & the National Maritime Museum, Greenwich, 1999) pp.125-7, 484-6. GLBO140
RYAN, W.F., 'John Russell, R.A. and early lunar mapping' Smithsonian Journal of History, vol. 1, pp.27-48

Lot Essay

John Russell (1745-1806) was elected Associate of the Royal Academy in 1782, and a full Academician in 1788. Born in Guildford, Surrey, he was apprenticed to Francis Cotes, the founder of the Royal Academy. Russell gained success and a certain amount of fame as a portraitist in pastel, earning himself the title of "Painter to the King". However, his overriding passion, it would appear, was the moon. The lunar globe here offered is the result of thirty years of close observation of the moon and its phases, starting presumably not long before 1764 when he produced his first drawing of the lunar surface. The major reason for such a long period of extended examination can be attributed to the lunar chracteristic known as libration. In effect, and as Dekker points out, "the Moon is a restless creature, always wobbling and showing a slightly different face all the time". Thus no two full moons look quite the same, and to someone of Russell's highly developed artistic sensibility, the constantly shifting play of light over the widely varied surface of the moon must have been a source of endless fascination and contemplation. Indeed, when speaking of the finished product, he declared that not only was it his desire to represent the craters and mountains of the lunar surface as faithfully as possible, but also to express the "feelings" he had when he first observed "the gibbous Moon through a Telescope".
The history of lunar mapping is well documented by Dekker, but Russell's is the oldest extant example of a lunar globe. Precedents include propositions by the astronomers Hevelius and Mayer, at separate times, to construct such a globe, but it would appear that neither saw the light of day. Christopher Wren is known to have constructed a relief globe of the moon in 1661, but this has now been lost. However, Russell's work was truly remarkable not only for the quality of the engraving on the gores, but the method for mounting the globe which was invented by Russell himself. The Selonographia mentioned on the cartouche on the sphere was the name given to the globe within its complex mounting. This consisted of a series of brass bands and circles fixed around the sphere, with a small earth ball and numerous gearing systems. This arrangement serves to represent - as the cartouche suggests - all possible aspects of the moon and its librations in relation to the earth and to the axes of the moon. Russell published a pamphlet to explain the use of the whole instrument, entitled Description of the Selenographia in which he mentions that relief versions of the globe are available. Dekker states that it would appear that at least one example was indeed made, but none have so far been found.

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