The stereoscope : $b its history, theory, and construction, with its application to the fine and useful arts and to educationBrewster, David
History
The stereoscope : $b its history, theory, and construction, with its application to the fine and useful arts and to education
Brewster, David
Stereoscope
Mr. Elliot was led to the study of binocular vision in consequence
of having written an Essay, so early as 1823, for the Class of Logic
in the University of Edinburgh, “On the means by which we obtain
our knowledge of distances by the Eye.” Ever since that date he was
familiar with the idea, that the relief of solid bodies seen by the
eye was produced by the union of the dissimilar pictures of them in
each eye, but he never imagined that this idea was his own, believing
that it was known to every student of vision. Previous to or during the
year 1834, he had resolved to construct an instrument for uniting two
dissimilar pictures, or of constructing a stereoscope; but he delayed
doing this till the year 1839, when he was requested to prepare an
original communication for the Polytechnic Society, which had been
recently established in Liverpool. He was thus induced to construct
the instrument which he had projected, and he exhibited it to his
friends, Mr. Richard Adie, optician, and Mr. George Hamilton, lecturer
on chemistry in Liverpool, who bear testimony to its existence at that
date. This simple stereoscope, without lenses or mirrors, consisted of
a wooden box 18 inches long, 7 broad, and 4½ deep, and at the bottom
of it, or rather its farther end, was placed a slide containing two
dissimilar pictures of a landscape as seen by each eye. Photography did
not then exist, to enable Mr. Elliot to procure two views of the same
scene, as seen by each eye, but he drew the transparency of a landscape
with three distances. The _first_ and most remote was the moon and
the sky, and a stream of water from which the moon was reflected, the
two moons being placed nearly at the distance of the two eyes, or 2½
inches, and the two reflected moons at the same distance. The _second_
distance was marked by an old cross about a hundred feet off; and the
_third_ distance by the withered branch of a tree, thirty feet from the
observer. In the right-hand picture, one arm of the cross just touched
the disc of the moon, while, in the left-hand one, it projected over
one-third of the disc. The branch of the tree touched the outline of a
distant hill in the one picture, but was “a full moon’s-breadth” from
it on the other. When these dissimilar pictures were united by the
eyes, a landscape, certainly a very imperfect one, was seen in relief,
composed of three distances.
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.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account