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Spiru Haret was one of the first generation of Romanian mathematicians. The country sought independence from the Ottoman Empire and Russia, and the first major steps occurred at around the time Haret was born. Russian domination was removed after they were defeated by the western allies in the Crimean War and, although it would be some considerable time before formal independence came about, Romania was essentially set on the path of independence. A western style constitution was put in place in 1866.
Already while he was a high school student, Spiru Haret published two mathematics texts, one on algebra and one on trigonometry. He entered the University of Bucharest in 1869, taking courses on mathematics and physics. After one year of study he left the university to take up a teaching post at the Nifon Seminary in Bucharest but, after teaching for one year, he returned to the University of Bucharest to complete his degree. He graduated in 1874 with a mathematics and physics degree. At this time Romania had no leading mathematical experts so anyone wishing to take the subject further had to train abroad. The young country badly needed the train leading scientists, however, and Titu Maiorescu, the leading Romanian literary critic of the second half of the 19th century, organised a scholarship competition to provide funds for outstanding young scholars to study abroad. Haret won the competition which provided funds for him to study in Paris.
Haret studied mathematics and physics at the Sorbonne. He was awarded a mathematics diploma in 1875 and a physics diploma in the following year. After this he undertook research and defended his thesis Sur l'invariabilite des grandes axes des orbites planetaires (On the invariability of the major axis of planetary orbits) on 18 January 1878. The authors of  write:-
One of the most outstanding performances of Henri Poincaré in the realm of mathematics is subtly and closely related to Spiru Haret. Both got resounding results in maybe the most celebrated problem of dynamics: the n-body problem, initially aimed at modelling the planetary motions in our Solar System. Even if not decisive, Haret's results helped and determined Poincaré to search for, to find, and to offer new fundamental methods, primarily intended to tackle this problem, but revolutionary and useful for most domains of science. Haret's and Poincaré's achievements marked, respectively, the end of a old era and the beginning of a new era in celestial mechanics and, in general, in mathematics.
Which is the link between Haret's and Poincaré's achievements from the narrow standpoint of the concrete problem they studied? Haret proved instability of the model of the n-body problem, but considering frequencies (mean motions) to be incommensurable. Taking also into account commensurabilities, and using generalized Fourier series (which generate quasiperiodic solutions), Poincaré proved the divergence of these series, which means instability, confirming in this way Haret's result. Haret's and Poincaré's results show that the question of the Solar system's stability remains still unsolved. Haret's work marked the beginning of the end of an era, that of exclusively quantitative endeavours in mathematics.
Arpad Pal writes in  about the results of Haret's doctoral thesis. Here is part of the abstract of that paper:-
The present paper, dedicated to the 140th anniversary of the birthday of the Romanian mathematician, mechanicist, and astronomer Spiru Haret (1851 - 1912), is an attempt to state as a theorem his famous result concerning the well-known problem on the invariability of the major axes of planetary orbits, related to the stability of the solar-planetary system. "Spiru Haret's theorem" is to be naturally added to the logical succession of theorems with respect to this problem known as "Laplace-Lagrange theorem" and "Poisson's theorem". Using his own method to explain mathematically the phenomenon of secular acceleration of Moon's "mean motion", Spiru Haret gives a criterion for separating the higher order gravitational perturbations from every non-gravitational perturbation in the motion of natural or artificial celestial bodies ...
After defending his thesis in 1878, Haret returned to Romania. He was appointed Professor of Rational Mechanics at the Science Faculty of the University of Bucharest later in the same year. Although Haret continued to have a major impact on teaching at the university, he gave up research on mathematics and instead became involved in politics. He was Minister of Public Education on three different occasions, 1897-99, 1901-04 and 1907-10. His contribution to education in Romania was extraordinary and during these periods of office he built a modern educational system. These were effective reforms, for, between 1897 and 1910, the literacy rate in Romania increased from 22% to 39%.
Despite his political involvement, Haret retained his professorship at the University of Bucharest and, in addition, he also retained his professorship of analytical geometry at the Bridges and Roads' School in Bucharest to which he had been appointed in 1882. He retired from his professorships in 1910, the year he left office as Minister of Public Education, and in the following year he published his only other major scientific work. This was the book Mécanique social which is described by Malita in . The book:-
... was a pioneering effort in the mathematization of the social sciences, one of the first in which mathematical modelling was applied to the study of social problems. The book was ahead of its time and only now is its full significance being realized. Haret attempted to set up a system of mechanics that would describe the forces that govern social and economic phenomena.
We mentioned that this was his only other major work so we should, for completeness, note that he did produce two other papers. The first, published in 1880, studied the secular acceleration of the Moon and the second, published in 1912, was on Jupiter's Great Red Spot.
Article by: J J O'Connor and E F Robertson
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