On the Construction of a Silvered Glass Telescope Fifteen and a half inches in aperture, and its use in celestial photography — Reading Notes

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In Category - Civil Engineering
Draper, Henry, 1837-1882 Project Gutenberg 2016 Not confirmed
Astronomy; Astronomical photography; Reflecting telescopes Readers of public-domain and historical texts
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Words 32,505
Reading time 142 min
Text sections 5

This digital edition of On the Construction of a Silvered Glass Telescope Fifteen and a half inches in aperture, and its use in celestial photography — Reading Notes is described by source-level measurements including 32,505 words, 2 hr 22 min estimated reading time, and 5 detected text sections.

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Henry Draper's 1865 Smithsonian monograph details the construction of a 15.5-inch silvered-glass telescope and its application to celestial photography, with precise technical descriptions of mirror polishing, optical testing, and early astrophotography.
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The text of this book has been preserved in its original form apart from correction of two typographic errors: embarrasment → embarrassment, Cassegranian → Cassegrainian. Inconsistent hyphenation has not been altered. A lengthy preliminary section concerning the Smithsonian Institution precedes the actual subject matter.

CONTRIBUTIONS TO KNOWLEDGE.

EVERY MAN IS A VALUABLE MEMBER OF SOCIETY, WHO, BY HIS OBSERVATIONS, RESEARCHES, AND EXPERIMENTS, PROCURES KNOWLEDGE FOR MEN.--SMITHSON.

PUBLISHED BY THE SMITHSONIAN INSTITUTION.

This volume forms the fourteenth of a series, composed of original memoirs on different branches of knowledge, published at the expense, and under the direction, of the Smithsonian Institution. The publication of this series forms part of a general plan adopted for carrying into effect the benevolent intentions of JAMES SMITHSON, Esq., of England. This gentleman left his property in trust to the United States of America, to found, at Washington, an institution which should bear his own name, and have for its objects the “_increase_ and _diffusion_ of knowledge among men.” This trust was accepted by the Government of the United States, and an Act of Congress was passed August 10, 1846, constituting the President and the other principal executive officers of the general government, the Chief Justice of the Supreme Court, the Mayor of Washington, and such other persons as they might elect honorary members, an establishment under the name of the “SMITHSONIAN INSTITUTION FOR THE INCREASE AND DIFFUSION OF KNOWLEDGE AMONG MEN.” The members and honorary members of this establishment are to hold stated and special meetings for the supervision of the affairs of the Institution, and for the advice and instruction of a Board of Regents, to whom the financial and other affairs are intrusted.

The Board of Regents consists of three members _ex officio_ of the establishment, namely, the Vice-President of the United States, the Chief Justice of the Supreme Court, and the Mayor of Washington, together with twelve other members, three of whom are appointed by the Senate from its own body, three by the House of Representatives from its members, and six persons appointed by a joint resolution of both houses. To this Board is given the power of electing a Secretary and other officers, for conducting the active operations of the Institution.

To carry into effect the purposes of the testator, the plan of organization should evidently embrace two objects: one, the increase of knowledge by the addition of new truths to the existing stock; the other, the diffusion of knowledge, thus increased, among men. No restriction is made in favor of any kind of knowledge; and, hence, each branch is entitled to, and should receive, a share of attention.

The Act of Congress, establishing the Institution, directs, as a part of the plan of organization, the formation of a Library, a Museum, and a Gallery of Art, together with provisions for physical research and popular lectures, while it leaves to the Regents the power of adopting such other parts of an organization as they may deem best suited to promote the objects of the bequest.

After much deliberation, the Regents resolved to divide the annual income into two parts--one part to be devoted to the increase and diffusion of knowledge by means of original research and publications--the other part of the income to be applied in accordance with the requirements of the Act of Congress, to the gradual formation of a Library, a Museum, and a Gallery of Art.

The following are the details of the parts of the general plan of organization provisionally adopted at the meeting of the Regents, Dec. 8, 1847.

DETAILS OF THE FIRST PART OF THE PLAN.

I. TO INCREASE KNOWLEDGE.--_It is proposed to stimulate research, by offering rewards for original memoirs on all subjects of investigation._

1. The memoirs thus obtained, to be published in a series of volumes, in a quarto form, and entitled “Smithsonian Contributions to Knowledge.”

2. No memoir, on subjects of physical science, to be accepted for publication, which does not furnish a positive addition to human knowledge, resting on original research; and all unverified speculations to be rejected.

3. Each memoir presented to the Institution, to be submitted for examination to a commission of persons of reputation for learning in the branch to which the memoir pertains; and to be accepted for publication only in case the report of this commission is favorable.

4. The commission to be chosen by the officers of the Institution, and the name of the author, as far as practicable, concealed, unless a favorable decision be made.

Henry Draper’s 1865 monograph, published as part of the Smithsonian Contributions to Knowledge, presents a detailed account of building a 15½-inch silvered-glass reflector and using it for celestial photography. The work is notable for its methodical, step-by-step exposition of mirror grinding, polishing, and figuring, as well as its candid discussion of practical challenges such as heat distribution, polishing powders, and the formation of zones on the mirror surface. Draper’s voice is that of a hands-on experimenter who values reproducible technique over theoretical abstraction.

Local Polishing and the Paraboloid

Draper devotes considerable attention to the process of local polishing, describing a method to avoid the zonal defects that commonly plague large mirrors. He explains how the polisher’s edge, if it changes direction many times in succession, will produce a zone on the surface unless the stroke is carefully managed. His solution involves a system where the outer excursion of the inner edge and the inner excursion of the outer edge meet and neutralize at a midway point. Once a spherical surface is achieved, the mirror is converted into a paraboloid by moving the polisher toward the edge and increasing the stroke. Draper claims that with this method, the difficulties of heat, irregular contact of the rosin, and distribution of polishing powders “entirely disappear.” The resulting surface is good almost to the extreme edge, and the “fleecy appearance” often seen on imperfect mirrors is absent.

Testing with Double Stars and Planetary Details

Draper evaluates his telescope’s performance by reference to specific astronomical tests. He reports that the parabolic surfaces define close double stars such as γ² Andromedae, showing the colors of the components. For unequal stars, a more severe test, the telescope reveals the close companion of Sirius—discovered by Alvan Clark’s refractor—and the sixth component of θ¹ Orionis. As an example of light-gathering power, Draper notes that the star Debilissima between ε and 5 Lyrae appears quintuple, a feat first noticed by Mr. Lassell; Herschel’s 18½-inch specula had recorded it only as double, and Lord Rosse did not see the fourth and fifth components. Jupiter’s moons show distinct disks with marked differences in diameter, and the planet’s surface is “literally covered with belts up to the poles.” Even under unsteady air, Venus displays bright and dark spots and irregularities on its inner edge.

Photography as the Ultimate Proof

Draper asserts that the best demonstration of the mirrors’ quality comes from the photographs taken with them. While the photographic images are not as sharp as the visual view, he emphasizes that an imperfect mirror will not yield good pictures. A photograph magnified to three feet corresponds to a power of 380. The text implies that photography imposes stricter demands on the optical figure than visual observation alone, making it a rigorous test of the telescope’s construction. Draper’s integration of photography into the evaluation process reflects his broader interest in capturing celestial objects permanently, a pursuit that would later lead to his pioneering astrophotographs of the Moon and stars.

Draper’s monograph rewards readers who attend to the interplay between mechanical precision and optical performance. The descriptions of polishing strokes, test objects, and photographic results are not merely technical notes but evidence of a systematic approach to instrument making. Readers interested in the history of telescope construction or early astrophotography will find here a primary document that bridges craft and science.

Flipping through Draper’s notes on his silvered-glass telescope, I kept thinking of the patience involved—polishing, testing, waiting for the stars. It reminded me of the quiet, steady care in Concrete Construction for the Home and the Farm — Reading Notes. Both books share that unhurried devotion to craft, where precision becomes almost a form of tenderness toward the future.

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