Immediately after becoming superintendent, Maury moved the depot to a building between 24th and 25th Streets, N. W., known formerly as 2222–24 Pennsylvania Avenue, and to the rather limited accommodations here he brought his family. Meanwhile a new building was being constructed on a reservation at 23d and E Streets, N. W., where the Naval Medical School is now located,—a site covering about seventeen acres which had been reserved by General Washington for a great university. This new building was to be of brick, in the form of a square about 50 feet by 50, surmounted by a dome 23 feet in diameter, with wings to the south, east, and west. Later, in 1847, the superintendent’s residence was constructed and connected with the main building by an extension of the east wing.
An Engraving of the United States Naval Observatory Buildings as They Appeared When Maury Was Superintendent about 1845
From an engraving in the title page of “Astronomical and Meteorological Observations Made during the Year 1875, at the U. S. Naval Observatory,” 1878.
The name of the institution varied. As the Depot of Charts and Instruments it was officially known from 1830 to 1844; but for the next ten years the names Naval Observatory and National Observatory were used indiscriminately, sometimes even in the same publication. In December, 1854, the Secretary of the Navy instructed that it should henceforth be called the United States Naval Observatory and Hydrographical Office, and as such it was known until the establishment of the Hydrographic Office as a separate division in 1866. Since that date the official name of the institution has been the United States Naval Observatory.
Near the close of September, 1844, the Observatory was reported to be completed, and on October 1 Maury was ordered to take charge with a staff of line officers and professors of mathematics of the navy, and civilian professors. Lieutenant James M. Gilliss, Maury’s predecessor, had been greatly interested in astronomy, especially that field of the science having to do with navigation, and it was largely through his exertions that the necessary legislation had been passed making possible a building, adapted not merely to the housing of charts and instruments but suitable as well for astronomical observations. He had been sent to Europe to consult about the purchasing of instruments for the new Observatory, and there were those who thought that he should have been made its first superintendent.
However scantily informed Maury may have been in the beginning as to the great advance in astronomical science recently made in Europe, his great energy and native ability soon enabled him to overcome any such handicaps. He assisted with his own hands in the installation of the instruments, in which he took great delight, writing that the Great Refraction Circle was such an exquisite piece of machinery and so beautiful that he would like to wear it round his neck as an ornament. He was constantly endeavoring to secure better and larger instruments, and wrote with pride when the Observatory, as far as equipment was concerned, became the second most important in the world and needed only a larger telescope to make it the very first of all. Maury quickly saw the value of the Electro-Chronograph, invented by John Locke of Cincinnati, in determining longitude with the aid of the magnetic telegraph, seeing that it would practically double the number of observations that one observer could make; and it was largely through him that Congress was persuaded to appropriate the $10,000 necessary for installing the instrument at the Observatory.
Maury was, moreover, by no means a mere figurehead in the making of astronomical observations, but soon mastered the details of this work which might have been left wholly to his subordinates. During the first two years he was the principal observer with the equatorial, and it is interesting to note how often his name appears as the observer in the published extracts from the notebooks of the Observatory. That he had much more than a mere passing interest in astronomy is evident from the following account of his emotions during an astronomical observation: “To me the simple passage through the transit instrument of a star across the meridian is the height of astronomical sublimity. At the dead hour of the night, when the world is hushed in sleep and all is still; when there is not a sound to be heard save the dead beat escapement of the clock, counting with hollow voice the footsteps of time in his ceaseless round, I turn to the Ephemeris and find there, by calculation made years ago, that when that clock tells a certain hour, a star which I never saw will be in the field of the telescope for a moment, flit through, and then disappear. The instrument is set;—I look; the star, mute with eloquence that gathers sublimity from the silence of the night, comes smiling and dancing into the field, and at the instant predicted even to the fraction of a second it makes its transit and is gone! With emotions too deep for the organs of speech, the heart swells out with unutterable anthems; we then see that there is harmony in the heavens above; and though we cannot hear, we feel the ‘music of the spheres’”.[3]
Maury’s first volume of astronomical observations, the first indeed to be issued from an American observatory, appeared in 1846. Though this was pioneer work, it was important enough to cause one of the most distinguished astronomers of Europe to conclude that it had placed the American observatory in the front rank with the oldest and best institutions of the kind in Europe. In the appendix to this volume, Maury gives very generous credit and praise to his helpers, among whom were at this time the distinguished mathematicians Hubbard, Keith, and Coffin; but he adds that he considers himself alone responsible for the accuracy of the work as nothing had been published until it had passed his supervision and approval.
A very ambitious work which Maury began during the year 1845 was a catalogue of the stars. The aim was to cover every point of space in the visible heavens with telescopes, get the position of every star, cluster, and nebula, and record both magnitude and color, with the angle of position and the distance of binary stars together with descriptions and drawings of all clusters and nebulæ. No astronomical work on such an extensive scale had ever before been executed or even attempted, though the value and importance of it were manifold and difficult of full estimation. Maury wrote that it was his intention to make a contribution to astronomy that would be worthy of the nation and the age, and to so execute the undertaking that future astronomers would value it so highly as to say that such a star was not visible in the heavens at the date of the Washington Catalogue because it is not recorded therein.