The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomyDick, Thomas
Science
The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomy
Dick, Thomas
Astronomical instruments; Astronomy; Telescopes
The _Finder_ is placed at AE, either on the top or the left side of
the tube of the telescope. When high magnifying powers are applied to
any telescope, it is sometimes difficult, on account of the smallness
of the field of view, to direct the main tube of the telescope to the
object. But the Finder, which is a telescope with a small power, and
consequently has a large field of view--when directed to any object, it
is easily found, and being brought to the centre of the field, where
two cross hairs intersect each other, it will then be seen in the
larger telescope. B is the eye-tube for terrestrial objects, containing
4 glasses, and C, one of the astronomical eye-pieces. A socket is
represented at _g_, containing a stained glass, which is screwed to any
of the eye-pieces, to protect the eye from the glare of light, when
viewing the spots of the sun. The brass nut above _f_, is intended for
the adjustment of the eye-piece to distinct vision. The 3-1/2 feet
telescope is sometimes mounted in this form.
Fig. 59, represents a 5 or 6 feet telescope, mounted on a stand of a
new construction by Dollond. It possesses the advantage of supporting
the telescope in two places, which renders it extremely steady--a
property of great importance when viewing celestial objects with high
magnifying powers. It possesses likewise, the advantage of enabling the
observer to continue seated at the same height from the floor, although
the telescope be raised to any altitude--_the elevation being entirely
at the object end_, although it may be changed from the horizon to
the zenith. The frame-work is composed of bars of mahogany, and rests
on three castors, two of which are made fast to their respective legs
in the usual way, and the third stands under the middle of the lower
horizontal bar that connects the two opposite legs, so that the frame
has all the advantages of a tripod. As it becomes very inconvenient to
stoop to the eye end of a telescope, when the altitude of an object is
considerable, and the centre of motion at the middle of the tube, this
construction of a stand serves to remedy such inconvenience.
[Illustration: _figure 59._]
_Proportions of curvature of the lenses which form an achromatic
object-glass._
Public-domain text, read in full here on John Shaqi.
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