Non-Euclidean geometries were created after failures to prove Euclid’s fifth parallel postulate using the other four postulates, 5 common notions, 23 definitions, and 28 theorems. The five postulates are: (1) to draw a straight line from any point to any point, (2) to produce a finite straight line continuously in a straight line, (3) to describe a circle with any center and distance, (4) that all right angles are equal to one another, and (5) if a straight line falling on two straight lines makes the interior angles in the same side less than two right angles, the two straight lines, if produced indefinitely meet on that side on which are the angles less than the two right angles. The Egyptian Ptolemy made the 1st attempt in the first century. The Persian Nasir-Eddin (1201-74) made the 2nd recorded attempt, next came Wallis, Saccheri, Fenn, Playfair, Legendre, Klügel, Lambert, Schweikart, Taurinus, and many others between the mid 16th century and the end of the 18th century. It is believed that no major discovery of mathematics is the work of one person. But at best, a decisive step or proof may be credited to an individual. This cumulative development of mathematics also applies to the discovery of non-Euclidean geometries. Nonetheless, the futile efforts to prove the fifth postulate became known as the foremost scandal of mathematical incompetency for mathematics in general and for geometry in particular.
The first break came in 1799 where and when Carl Friedrich Gauss was finally convinced that the parallel postulate cannot be deduced from the other axioms. He began the serious development of a new and possibly applied geometry based mostly on his practical experiences in land surveying and geodesy. This was the birth of spherical geometry. Its practical applications are in spherical trigonometry. Without it global maritime commerce would not have been possible. Thus begins the era of scratching surfaces of given spheres. They are mathematical idealization of the more realistic ellipsoidal volume of planet earth whose quadric equations in a proper coordinate system is x²/a²+y²/b²+z²/c²=1. Another branch known as hyperbolic non-Euclidean geometry was credited to the independent publications of Lobatchevsky and Bolyai in the early part of the 19th century whose proper quadric equations are the hyperboloid of one sheet and the hyperboloid of two sheets given respectively by x²/a²+y²/b²-z²/c²=1 and x²/a²+y²/b²-z²/c²=-1. Their practical applications could be found in space-time travel into the past or into the future.


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