Popular Science Monthly/Volume 19/September 1881/Sketch of James Craig Watson
|←What Is a Molecule?||Popular Science Monthly Volume 19 September 1881 (1881)
Sketch of James Craig Watson
By Alexander Winchell
By ALEXANDER WINCHELL, LL.D.
JAMES CRAIG WATSON, Professor of Astronomy in the University of Wisconsin, and Director of the Washburne Observatory at Madison, Wisconsin, died on the morning of November 23, 1880, after an illness of one week, at the age of forty-two years and ten months. Professor Watson was one of the most gifted and distinguished of modern astronomers, and his life-work is identified with the name of the University of Michigan.
He was born of American parentage, during a sojourn of his parents in Middlesex (now Elgin) County, Ontario, January 28, 1838. The mathematical genius revealed by the boy at the early age of nine determined the father to secure him a liberal education, and the family accordingly removed to Ann Arbor in 1850. Here James displayed equal aptitude for mathematical and linguistic studies, and, being prepared for college, almost without the evidences of effort, he entered the University of Michigan in the autumn of 1853. He attained equal scholarly distinction as a student of ancient and modern languages and of mathematics. It is said that, before the close of his junior year, he had performed the phenomenal feat of reading from beginning to end the "Mécanique Céleste" of Laplace. During his senior year, he was the solitary pupil of Dr. Brünnow, and graduated in 1857. His mechanical tact was such that, in the absence of a mathematical bent, he would have become an eminent mechanician and inventor. While in college, some of his spare hours were spent in grinding lenses and the construction of a telescope. Other portions of his time he was compelled to devote to the earning of means to defray collegiate expenses.
During the two years succeeding his graduation, he was employed as assistant in the Observatory, and in the prosecution of studies for his second degree. In this work he .displayed such remarkable aptitude as an observer, and such marvelous rapidity in his computations, that, on the retirement of Dr. Brünnow, in June, 1859, young Watson succeeded him in the chair of Astronomy. He was already known as a frequent contributor to the "American Journal of Science," Brünnow's "Astronomical Notices," Gould's "Astronomical Journal," and the "Astronomische Nachrichten," of Altona. Not less than twelve 694 THE POPULAR SCIENCE MONTHLY.
communications, written before be was twenty-one, are recorded in tbe Royal Society's " Catalogue of Scientific Papers," wbicb also enumer- ates twenty-one otbers between 1859 and 1874. His wonderful keen- ness as an observer was signalized, wbile yet an undergraduate, by tbe discovery of a comet on tbe 29tb day of April, 1856, and, four montbs after graduation, by tbe discovery of a planet on tbe 20tb of October, 1857, wbicb, bowever, proved to bave been observed by Lutber a few days before, and bas been named Aglaia. His observations of Dona- ti's comet, in 1858, possess a standard value, and bis computation of tbe orbit is recognized as autboritative. Tbe interest awakened by tbis comet prompted to tbe preparation of " A Popular Treatise on Comets," publisbed early in 1860.
In 1860 Dr. Brtinnow resumed tbe directorsbip of tbe Observatory, and young Watson was assigned to tbe cbair of Pbysics in tbe uni- versity, wbicb be retained for tbree years, wben, on tbe final retire- ment of Dr. Brtinnow, Watson was made Professor of Astronomy and Director of tbe Observatory, a position wbicb be beld and bonored for sixteen years. Scarcely bad be been clotbed witb full control of tbe instruments, wben be resumed bis remarkable career of discovery. Tbere seemed almost a magic in bis powers. Unrecognized celestial objects seemed to crowd spontaneously upon bis notice. On Sej^tem- ber 14, 1863, be made bis first independent planetary discovery. Tbis was Eurynome. On January 9, 1864, be discovered tbe comet since known as 1,863, VI, wbicb Respigbi, as it proved, bad already noted. On tbe 9tb of October, 1865, be discovered a planet wbicb also proved to bave been announced by Peters, and bas since been named lo. He discovered Minerva, August 24, and Aurora, September 6, 1867. During 1868 be added no less tban six minor planets to tbe solar sys- tem, furnisbing tbe only instance in wbicb tbe list of planetary dis- coverers presents tbe same name four times in immediate succession.
Meantime be was engaged upon a work wbicb migbt well bave engrossed all bis powers, and must bave quite exceeded tbe abilities of any but a gifted matbematical genius. It was no less tban a complete digest of tbe results and metbods of all tbe great writers on tbeoreti- cal astronomy, and an independent development of tbe great principles of tbe science. " Having carefully read tbe works of tbe great mas- ters," be says in bis preface, " my plan was to j^rej^are a complete work on tbe subject, commencing witb tbe fundamental principles of dynamics, and systematically treating, from one point of view, all tbe problems presented." Tbis broad plan, conceived by a young man of twenty-eigbt, and completed wben twenty-nine, was executed witb ability so commanding, tbat tbe work, on its appearance in 1869, was immediately accepted as an autboritative exposition of tbe bigber principles and processes of dynamical astronomy, and was made a text-book at Leipsic, at Paris, and at Greenwicb. Tbe same year be was sent by tbe General Government on an expedition to observe tbe
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solar eclipse at Mount Pleasant, Iowa, and, in 1870, to Carlantini, Sici- ly, for a similar purpose. In 1874 he was appointed to the charge of an expedition to Peking, China, to observe the transit of Venus. His observations were favored by the weather, and conducted with con- summate skill. The results, though reduced and discussed, are not yet published. Even at the antipodes, fresh discoveries awaited him. He had already raised his list of planetary discoveries to seventeen, and now added Juewa^ the eighteenth. In 1876 he was one of the Judges of Awards at the Centennial Exposition, and wrote the cele- brated " Report on Horological Instruments." In 1878 also aj^peared his " Tables for the Calculation of Simple and Compound Interest," a work which, in spite of the subject, is marked by great originality, and demanded a vast amount of wearisome labor. The same year he was sent by the General Government in charge of an expedition to Wyoming, to observe the total solar eclipse. Professor Watson, hav- ing long entertained a belief in the existence of an intra-Mercurial planet, as well as of an extra-Neptunian one, gave special attention at this time to a search for the former, and was the first astronomer to note certainly (July 29, 1878) the existence and position of the planet Vulcan. He also satisfied himself of the existence of a second intra- Mercurial planet. This brought the number of his original planetary discoveries to twenty-six (including one lost July 29, 1873, and two anticipated). He was now animated by an intense desire to control instruments of suitable power and adjustment to confirm his last ob- servations, and enable him to detect the outlying planet beyond Nep- tune. Coincidently came the invitation to assume the charge of the Washburne Observatory at Madison, Wisconsin, which was to be improved and newly equipped with instruments far more efficient than those at Ann Arbor. The temptation was great, but he natu- rally clung to his alma mater, whose authorities made such efforts as they thought authorized to content their astronomer. But the requisite means could only be obtained by a grant from the Legisla- ture, a measure defeated by an inadequate appreciation of the honor shed upon the State by such a name as Watson's. Reluctantly, but sustained by a high and noble aspiration, he removed, in the summer of 1879, to Madison, and immediately devoted himself with intense energy to remodeling the observatory structure, and introducing some original provisions thought to be suited to the special researches on which he was bent. A cellar twenty feet deep was sunk at the bot- tom of the first slope of Observatory Hill. Into this, light was to be thrown through a long tube, from powerful reflectors on the top of the hill. This, with other accessory work, was actually in progress, when a severe cold brought on peritonitis, which over-confidence in his physi- cal powers permitted to reach a fatal stage before medical aid was summoned. His remains, accompanied by an escort from the Univer- sity of Wisconsin, were removed to Ann Arbor, where they lay in
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state, in the university, during the 25th of Xovember, and, on the fol- lowing day, with due honors and imposing ceremonies conducted by his late colleagues, were reverently laid beneath the shade of Oakwood Cemetery.
Professor Watson possessed extraordinary intellectual endowments. His quickness of perception nothing escaped. His mathematical intu- itions scorned the ordinary processes of calculation, and gave him a masterly command of mathematical logic and formulae, which made so many portions of his work on " Theoretical Astronomy " strictly original, and all parts virtually his owui. Yet he never mentions any chiim to originality, but pursues his majestic intellectual march with the dignity almost of an inspiration. His memory served him equally well. It was both circumstantial and philosophical. Every new ob- servation was immediately illuminated by all which he had previously observed or known, and he saw instantly the proper conclusions. His mechanical gifts gave him perfect command of instruments and their construction, and the Washburne Observatory would have been equipped with several of his inventions. His versatility extended to matters of business. He was for years the actuary of the Michigan Mutual Life Insurance Comj^any, and performed service pronounced invaluable. He managed his private means Avith such success that he died possessed of a considerable fortune, which his will secures to the National Academy of Science. Physically, he was vigorous and healthy, and reached, in the last years of his life, a weight of two hundred and forty pounds. His religious nature held fast to the fun- damental religious beliefs. He used to say it is impossible for a math- ematician to be an atheist, and his works offer frequent recognition of the being of the supreme Creator and Governor of the universe.
The world was not slow to recognize his worth. He was elected a member of the National Academy of Science in 1867, and of the Royal Academy of Sciences in Italy in 1870. He received the degree of Doctor of Philosophy from the University of Leipsic in 1870, and the French Academy of Sciences conferred upon him the Lalande gold medal for the discovery of six new planets in one year. Yale College honored him with the degree of Doctor of Philosophy in 1871. In 1875 the Khedive made him Knight Commander of the Imperial Order of Medjidieli of Turkey and Egypt. He was elected member of the American Philosophical Society in 1877, and received, the same year, the degree of Doctor of Laws from Columbia College. American Journal of Science.