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
Were any person to attempt the construction of those telescopes, it
is possible he might not succeed in his first attempts without more
minute directions than I have yet given. The following directions
may perhaps tend to guide the experimenter in adjusting the eye-tube
to the speculum, which is a point that requires to be particularly
attended to, and on which depends the accurate performance of the
instrument. After having fixed the eye-piece nearly in the position
it should occupy, and directed the instrument to a particular object,
look along the arm of the telescope, from K (fig. 69.) to the extremity
of the eye-piece at H, and observe, whether it nearly coincides with
the object. If the object appear lower than this line of vision, the
eye-piece must be lowered, and if higher, it must be raised, by means
of the nuts and screws at _gd_ and _fe_, till the object and the line
of vision now stated nearly coincide. The eye-piece should be directed
as nearly perpendicular to the front of the speculum as possible, but
so that the reflected image of one’s head from the mirror shall not
interfere to obstruct the rays from the object. An object may be seen
with an approximate degree of distinctness, but not accurately, unless
this adjustment be pretty accurately made. The astronomical eye-pieces
used for these telescopes are fitted with a brass cap which slides on
the end next the eye, and is capable of being brought nearer to or
farther from the first eye-glass. In the centre of this cap, next the
eye, is a small hole, about the 1/40th or 1/50th of an inch diameter,
or about as wide as to admit the point of a pin or a moderate-sized
needle. The distance of this hole from the lens next the eye must be
adjusted by trial, till the whole field of view appear distinct. A
common astronomical eye-piece, without this addition, does not answer
well. I find by experience, that terrestrial eye-pieces, such as those
used in good achromatic telescopes, are, on the whole, best adapted to
this construction of a reflecting telescope.
I have sometimes used these instruments for the purpose of viewing
perspective prints, which they exhibit in a beautiful and interesting
manner. If a coloured perspective be placed at one end of a large
room or gallery, and strongly illuminated either by the sun or by two
candles, and one of the reflectors furnished with a _small magnifying
power_, placed at the opposite end of the room--the representation of
a street or a landscape will be seen in its true perspective, and will
appear even more pleasant and interesting than when viewed through
the common _optical diagonal machine_. If an inverting eye-piece be
used--which is most eligible in this experiment--the print, of course,
must be placed in an inverted position.
Public-domain text, read in full here on John Shaqi.
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