Georg Purbach
Encyclopedia : G : GE : GEO : Georg Purbach
Georg Purbach (also Georg von Peuerbach, Peurbach, Purbach, Purbachius, his real surname is unknown) (born May 30, 1423 in Purbach near Linz – April 8, 1461 in Vienna) was an Austrian astronomer and mathematician.
He is credited with the invention of several scientific instruments, including the regula, the geometrical square, and the "Jacob's Staff." The Purbach crater on the Moon is named after him.
About the year 1440 he received the degree of master of philosophy and the free arts, cum insigni laude, at the University of Vienna. His teacher in mathematics was probably Johann von Gmünden.
In 1448 he went on a trip to Italy for the sake of study. There, Giovanni Bianchini of Ferrara and Cardinal Nicholas of Cusa, then in Rome, became interested in the young man and induced him to lecture on astronomy at the University of Ferrara. He refused offers of professorships at Bologna and Padua, and also the appointment as court astronomer to King Ladislaus of Hungary, but went back to Vienna in 1450 to teach. He lectured on philology and classical literature. His scientific teaching was done chiefly in private, his most famous pupil being Johann Müller of Königsberg, later known as Regiomontanus.
Purbach has been called the father of observational and mathematical astronomy in the West. He began to work up Ptolemy's Almagest, replacing chords by sines, and calculating tables of sines for every minute of arc for a radius of 600,000 units. This was the first transition from the duodecimal to the decimal system. His observations were made with very simple instruments, an ordinary plumb-line being used for measuring the angles of elevation of the stars. Cardinal Bessarion invited him to Rome to study Ptolemy in the original Greek and not from a faulty Latin translation. He accepted on condition that Müller go with him. On account of the master's death the pupil went alone to complete the work.
Purbach is also noted for his great attempt to reconcile the opposing theories of the universe, the so-called homocentric spheres of Eudoxus of Cnidus and Aristotle, with Ptolemy's epicyclic trains. This work, *Theoricæ, etc., had an enormous success and remained the basis of academic instruction in astronomy until years after Copernicus had swept away all these hypotheses.
He worked at the Observatory of Oradea/Nagyvarad in Transylvania and established in his "Tabula Varadiensis" this Transylvanian town's observatory as laying on the prime meridian of Earth.
Twenty works of him are known. Among these, the following are the most important:
- Theoricæ novæ planetarum, id est septem errantium siderum nec non octavi seu firmamenti (1st ed., Nuremberg, 1472, by Regiomontanus; followed by many others in Milan and Ingolstadt);
- Sex primi libri epitomatis Almagesti, completed by Regiomontanus (Venice, 1496; Basle, 1534; Nuremberg, 1550);
- Tabulæ eclypsium super meridiano Viennensi (2nd ed., Vienna, 1514);
- Quadratum goemetricum meridiano (Nuremberg, 1516);
- Nova tabula sinus de decem minutis in decem per multas, etc., completed by Regiomontanus (Nuremberg, 1541).
External links
- John J. O'Connor and Edmund F. Robertson. [] at the MacTutor History of Mathematics archive.
This article incorporates text from the public-domain Catholic Encyclopedia.
From Wikipedia, the Free Encyclopedia. Original article here. Support Wikipedia by contributing or donating.
All text is available under the terms of the GNU Free Documentation License See Wikipedia Copyrights for details.