During my father’s experiments on light, and more particularly when

engaged in the invention of portrait photography, he found that the

ammonio-sulphate of copper, a deep blue liquid, will separate the more

refrangible rays of light, the rays concerned in photography, from the

rest. If a beam of sunlight be passed through such a solution, inclosed

between parallel plates of glass, and then condensed upon an object on

the stage of a microscope, a blue colored image will be formed on the

ground glass, above the eyepiece. If the place of best definition be

carefully ascertained, and a sensitive plate put in the stead of the

ground glass, a sharp photograph will always result.

Besides, there is no danger of burning up the object, as there would

be if the unabsorbed sunlight were condensed on it, and hence a much

larger beam of light and much higher powers can be used. The best

results are attained when an image of the sun produced by a short

focussed lens is made to fall upon and coincide with the transparent

object. In 1856 we obtained photographs of frog’s blood disks,

navicula angulata, and several other similar objects under a power of

700 diameters, excellently defined. Since then several hundreds of

microscopic pictures have been taken.

In the figure, _a_ is the heliostat, _b_ a lens of three inches

aperture, _c_ the glass cell for the ammonio-sulphate of copper, _d_

the object on the stage of the microscope _e_, _f_ the camera for the

ground glass or sensitive plate. Above the figure the course of the

rays is shown by dotted lines.

* * * * *

In concluding this account of a Silvered Glass Telescope I may answer

an inquiry which doubtless will be made by many of my readers, whether

this kind of reflector can ever rival in size and efficiency such

great metallic specula as those of Sir William Herschel, the Earl of

Rosse, and Mr. Lassell? My experience in the matter, strengthened by

the recent successful attempt of M. Foucault to figure such a surface

more than thirty inches in diameter, assures me that not only can the

four and six feet telescopes of those astronomers be equalled, but even

excelled. It is merely an affair of expense and patience. I hope that

the minute details I have given in this paper may lead some one to make

the effort.

HASTINGS, WESTCHESTER COUNTY,

NEW YORK, 1863.

_Postscript._--Since writing the above I have completed a photograph

of the moon 50 inches in diameter. The original negative from which it

has been made, bears this magnifying well, and the picture has a very

imposing effect.

PUBLISHED BY THE SMITHSONIAN INSTITUTION,

WASHINGTON CITY,

JULY, 1864.

On the Construction of a Silvered Glass Telescope Fifteen and a half inches in aperture, and its use in celestial photography · 第 7 / 7 段