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 following, among many others, are some of the objects on which I
have tried many amusing experiments with telescopes fitted up with
the long tubes to which I allude. The telescope to which I shall
more particularly advert is an achromatic, mounted on a pedestal,
having an object-glass about 19 inches focal length, and 1-5/8 inch
diameter, with magnifying powers for distant objects of 13 and 20
times. When this instrument is directed to a miniature portrait,
3-1/2 inches in length, placed in a good light, at the distance of
about 8 or 10 feet, it appears as large as an oil-painting four or
five feet long, and represents the individual as large as life. The
features of the face appear to stand out in bold relief: and perhaps
there is no representation of the human figure that more resembles
the living prototype, than in this exhibition, provided the miniature
is finely executed. In this case the tube requires to be pulled out
four or five inches from the point of distinct vision for distant
objects, and consequently the magnifying power is proportionally
increased. Another class of objects to which such a telescope may be
applied is _Perspective prints_, either of public buildings, streets
or landscapes. When viewed in this way they present a panoramic
appearance, and seem nearly as natural as life--just in the same manner
as they appear in the Optical Diagonal Machine, or when reflected in
a large concave mirror--with this advantage, that, while in these
instruments the left hand side of the print appears where the right
should be,--the objects seen through the telescope appear exactly in
their natural position. In this case, however, the telescope should
have a small magnifying power, not exceeding 5 or 6 times, so as to
take in the whole of the landscape. If an astronomical eye-piece be
used, the print will require to be inverted.
Public-domain text, read in full here on John Shaqi.
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