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
3. The next operation is to obtain the drawing. Having placed the
Camera in front of the scene to be represented, and the lens being
adjusted to the proper focus, the ground-glass of the Camera is
withdrawn, and the prepared plate is substituted for it; and the
whole is left till the natural images are drawn by the natural light
from the object. The time necessary to leave the plate for a complete
delineation of the objects, depends upon the intensity of the light.
Objects in the shade will require more time for their delineation
than those in the broad light. The full clear light of the south of
Europe, Spain, Italy, and particularly, the more glowing brilliancy
of tropical countries, will effect the object much more speedily than
the duller luminosity of a northern clime. Some hours of the day are
likewise more favourable than others. Daguerre states, that ‘the most
favourable, is from 7 A.M. to 3 o’clock P.M., and
that a drawing could be effected in Paris in 3 or 4 minutes, in June
and July, which would require 5 or 6, in May and August, and 7 or 8 in
April and September.’ In the progress of this art, at the present time,
portraits and other objects are frequently delineated in the course of
a few seconds.
4. Immediately after removing the plate from the Camera, it is next
placed over the vapour of mercury, which is placed in a cup at the
bottom of a box, and a spirit lamp applied to its bottom, till the
temperature rise to 140 of Fahrenheit. This process is intended to
bring out the image, which is not visible when withdrawn from the
Camera; but in the course of a few minutes a faint tracery will
begin to appear, and in a very short time the figure will be clearly
developed.
5. The next operation is _to fix the impression_. In order to this, the
coating on which the design was impressed must be removed, to preserve
it from being decomposed by the rays of light. For this purpose, the
plate is placed in a trough containing common water, plunging, and
withdrawing it immediately, and then plunging it into a solution of
salt and water, till the yellow coating has disappeared.
Such is a very brief sketch of the _photogenic_ processes of Daguerre.
Other substances, however, more easily prepared, have been recommended
by Mr. Talbot, F.R.S., who appears, about the same time, to have
invented a process somewhat similar to that of Daguerre. The following
are his directions for the preparation of _Photogenic Paper_.
Public-domain text, read in full here on John Shaqi.
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