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
A comparison of the work of the several artists who have set their hand
to the draughting of figures for the numerous constellations is not
without interest. Attention may here be directed in passing to the
decidedly oriental cast of these figures as they appear on Arabic
globes.[206]
It is to be regretted that in the present very practical or scientific
day the star map, wanting the figures of the constellations or giving
them in but the faintest outline, has come to supplant the artistic and
not unscientific creations of earlier years.
The earliest references we have to globes, that is, to solid balls or
spheres, make mention of their mountings, that is, to their encasing
circles and their bases. The simplest mounting consisted of but a
meridian and a horizon circle with probably a simple supporting base.
The earliest spheres were doubtless made to revolve just as the globes
of today, around their polar axes which turn within sockets firmly
attached to the meridian circle. This meridian circle of brass or wood
was usually graduated from one to ninety degrees, that is, from the
equator to the poles, and being adjustable relative to the horizon
circle, a globe could be set with a polar elevation for any desired
latitude. Those who have had occasion to refer to the construction and
the uses of the globe more or less in detail, make mention of what they
call its threefold position. In the first of these positions either pole
may be at the vertical point, the equator and the horizon being parallel
or coinciding. This they termed a parallel sphere. In the second
position the equator and the horizon circle are set at right angles.
This they called a right sphere. In the third position, which was called
an oblique sphere, the pole could be set at any elevation from zero to
ninety degrees, counting from the horizon circle. In illustration of
this third position it may be said that for the latitude of New York
City, the north pole of the globe should be elevated 40 degrees 48
minutes above this circle.
Public-domain text, read in full here on John Shaqi.
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