THE “URANOMETRIA ARGENTINA.”—The publication of this great and meritorious work is just announced, though, so far as we know, the complete volume has not yet reached Europe. The system of observations upon which it is based was designed and commenced by Dr. B. A. Gould, the distinguished director of the Argentine Observatory, immediately after his arrival at Cordoba in September, 1870, on accepting the superintendence of the new establishment, and while awaiting the completion of the observatory buildings and the arrival of telescopes which had been ordered in Europe, but delayed by the outbreak of the Franco-German war, and the work upon it has been continued with more or less attention to the present year. It was intended to represent in a series of charts and accompanying catalogue the sky from the south pole as far as 10° north of the equator, as it appears to the naked eye, showing all stars down to a round magnitude fixed at 7.0, with their characteristics of duplicity, variability, and colour, and the milky-way in all its ramifications and gradations of brightness. The actual observations were assigned to the four assistants, Messrs. Rock, Davis, Hathaway, and Thome, who had proceeded to Cordoba from the United States, the first three returning home at the expiration of three years, when the Uranometry was already finished as to its general details. Mr. Thome subsequently reviewed the entire work twice, and with the result that Dr. Gould considers it improbable that any star so bright as 7.0, on a scale which it has been desired to extend accurately from Argelander's, will have escaped insertion, while notwithstanding the great degree of nicety implied, he thinks the magnitudes are essentially correct to the nearest tenth. During the first two years the work was continued on all cloudless nights, both summer and winter, at an average of six hours' work each night. The total number of stars of which the magnitudes have been assigned is 10,649, anne total estimates of magnitudes 44,510, or more than four for each star.
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