Terrestrial and Celestial Globes Volume 2: Their History and Construction Including a Consideration of their Value as Aids in the Study of Geography and AstronomyStevenson, Edward Luther
History
Terrestrial and Celestial Globes Volume 2: Their History and Construction Including a Consideration of their Value as Aids in the Study of Geography and Astronomy
Stevenson, Edward Luther
Geography -- History; Globes
The mounting of the globe is artistic and substantial, consisting of the
usual horizon circle, octagonal on its outer edge, but circular on the
inner edge to receive the globe ball, and having pasted on its upper
surface the usual engraved paper strips and all that there is engraved
thereon in the best examples of globe making. The meridian circle of
wood, within which the sphere is made to revolve, is graduated. The
supporting base consists of four exquisitely turned columns, braced at
bottom with correspondingly well-turned crossbars.
The celestial globe has a mounting altogether like that of the
terrestrial, and in the character of the map engraving there is
agreement. The figures of the several constellations are copies of these
drawn by Tycho Brahe, and all have been exquisitely colored. Stars from
the first to the sixth magnitude are represented, while special
attention is called to the new star in Cassiopeia first appearing in the
year 1572, and to the comets of the years 1597 and 1616. Near Ursa Major
is the author and date legend reading “In hoc Caelesto Globo notantur
omnes stellae fixae, ad annum 1636 accommodatae, quae iuxta
observationes Tychonis Brahae maximo illo Jansonii anno 1622 edito
positae sunt, additis stellis quae a nauclero Petro Theod. circa Polum
Australem notatae sunt ... Romae ex chalcographia Dominici de Rubeis,
her. Jo. Jac. de Rubeis anno 1695.”
The twelve gores of the map have been mounted so as to join at the north
and south poles of the ecliptic, there however being a small covering
disc at each pole, so frequently employed since Mercator’s day, the
globe itself being made to revolve on its equatorial axes.
Public-domain text, read in full here on John Shaqi.
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