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
Supposing that an achromatic telescope of 3-1/2 feet focal length, and
3-1/4 inches aperture were offered for sale, and that it were required
to ascertain whether the object-glass, on which its excellence chiefly
depends--is a good one and duly adjusted;--some opinion may be formed
by laying the tube of the telescope in a horizontal position, on a
firm support, about the height of the eye,--and by placing a printed
card or a watch glass vertically, but in an inverted position, against
some wall or pillar, at 40 or 50 yards distant, so as to be exposed
to a clear sky. When the telescope is directed to this object, and
accurately adjusted to the eye--should the letters on the card, or the
strokes and dots on the watch-glass appear clearly and sharply defined,
without any mistiness or coloration, and if very small points appear
well defined--great hopes may be entertained that the glass will turn
out a good one. But a telescope may appear a good one, when viewing
common terrestrial objects, to eyes unaccustomed to discriminate
deviations from perfect vision, while it may turn out to be an
indifferent one, when directed to certain celestial objects. Instead
therefore of a printed card, fix a black board, or one half of a sheet
of black paper, in a vertical position at the same distance, and a
circular disk of white writing paper, about 1/4 of an inch in diameter,
on the centre of the black ground. Then having directed the telescope
to this object, and adjusted for the place of distinct vision, mark
with a black-lead pencil the sliding eye-tube, at the end of the main
tube, so that this position can always be known; and if this sliding
tube be gradually drawn out, or pushed in, while the eye beholds the
disk, it will gradually enlarge and lose its colour, till its edges
cease to be well-defined. Now, if the enlarged misty circle is observed
to be concentric with the disk itself, the object-glass is properly
centered, as it has reference to the tube; but if the misty circle goes
to one side of the disk, the cell of the object-glass is not at right
angles to the tube, and must have its screws removed and its holes
elongated, by a rattailed file, small enough to enter the holes. When
this has been done, the cell may be replaced, and the disk examined a
second time, and a slight stroke on one edge of the cell, by a wooden
mallet, will show by the alteration made in the position of the misty
portion of the disk, how the adjustment is to be effected, which is
known to be right when a motion in the sliding tube will make the
diluted disk enlarge in a circle concentric with the disk itself. When
the disk will enlarge so as to make a ring of diluted white light round
its circumference, as the sliding tube holding the eye-piece is pushed
in or drawn out, the cell may be finally fixed by the screws passing
through its elongated holes.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account