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Biografi Abū Sahl al-Qūhī


(fl. Baghdad, c. 970–1000)


Abū Sahl Wayjan ibn Rustam al-Qūhī (al-Kūhī; Persian: ابوسهل بیژن کوهی Abusahl Bijan-e Koohi) was a Persian mathematician, physicist and astronomer. He was from Kuh (or Quh), an area in Tabaristan, Amol, and flourished in Baghdad in the 10th century. He is considered one of the greatest Muslim geometers, with many mathematical and astronomical writings ascribed to him.


Engraving of al-Qūhī's perfect compass to draw conic sections

Al-Qūhī was the leader of the astronomers working in 988 AD at the observatory built by the Buwayhid amir Sharaf al-Dawla in Badhdad. He wrote a treatise on the astrolabe in which he solves a number of difficult geometric problems.

In mathematics he devoted his attention to those Archimedean and Apollonian problems leading to equations higher than the second degree. He solved some of them and discussed the conditions of solvability. For example, he was able to solve the problem of inscribing an equilateral pentagon into a square, resulting in a fourth degree equation. He also wrote a treatise on the "perfect compass", a compass with one leg of variable length that allows users to draw any conic section: straight lines, circles, ellipses, parabolas and hyperbolas. It is likely that al-Qūhī invented the device.
Like Aristotle, al-Qūhī proposed that the weight of bodies varies with their distance from the center of the Earth.

The correspondence between al-Qūhī and Abu Ishaq al-Sabi, a high civil servant interested in mathematics, has been preserved.

Abū Sahl Wayjan, born Rustam al-Qūhīi (in many manuscripts “al-Kūhū”), has come to be recognized by modern scholarship as one of the great geometers of tenth-century Islam. He was the only geometer in medieval Islam to obtain exact results on centers of gravity, and he also gave an elegant method for finding the side of a regular heptagon and the volume of a segment of a paraboloid. One of a number of geometers who worked in eastern Iraq and Iran, he enjoyed the patronage of three Būyid rulers: 'Adud al-Daulah, Samsam al-Daulah, and Sharaf al-Daulah, whose combined reigns cover the period 962–989. His contemporaries regarded his work highly, Ibn al-Haytham referring to al-Qūhīi’s On the Measurement of the Paraboloid and al-Bīirūnī citing his On the Complete Compass. In the twelfth century, 'Umar alKhayyami cited him as one of the “distinguished mathematicians of Iraq,” and al-Khazini summarized some of al-Quhi’s work on centers of gravity in the former’s Balance of Wisdom.

Work in Geometry Al-Qūhī’s more than thirty extant treatises reveal him as primarily a geometer, a subject he described in the preface to his treatise on the regular heptagon as “the leader who is to be followed when it comes to honesty.” In his correspondence with Abū Ishaq alSābī, he praised mathematics as a demonstrative science, whose goal was to seek the truth—not numerical approximations.

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In his treatise On Rising Times, he wrote that he had also investigated astronomy as well as centers of gravity and optics. His Perfect Compass, for example, represented a step beyond Ibn Sinā’s pointwise constructions of conic sections and described an instrument al-Qūhī characterized as useful for drawing these sections on sundials and astrolabes.

Yet these areas appealed to him primarily as sources for geometrical problems. His lengthy Treatise on the Construction of the Astrolabe with Proofs was principally devoted to the problem of completing the lines of an astrolabe, given certain of its circles and points. His On the Distance from the Center of the Earth to the Shooting Stars set out a method that is mathematically correct, though impractical at the time, for finding the distance and size of these objects. In his Rising Times, al-Qūhī took a conservative stance vis-à-vis the new trigonometrical theorems he had heard about, and he showed how the classical Menelaus’s theorem might be used to solve a sequence of standard problems in spherical astronomy. (He emphasized that he had not devoted much attention to studying methods for constructing astronomical tables.)

Al-Qūhū took special interest in problems stemming from the works of Euclid, Apollonius, and Archimedes. In his Revision of Euclid’s Elements, I, he reorganized the latter by eliminating all of its constructions, using the parallel postulate much earlier, devising a new proof of the Pythagorean theorem, and giving an ostensible proof of the fourth postulate on the equality of right angles.
Al-Qūhīs studies of Elements, II provide twelve new propsoitions, very much in the spirit of the first ten propositions of that work, as well as a short Lemmas to the Conics, whose introduction describes it as “necessary in the second and third books of The Conics.”

Archimedean Tradition Unique in medieval Islam are al Qūhī’s results on centers of gravity of plane and solid figures, results very much in the tradition of Archimedes. This research, he said in the preface to On the Volume of the Paraboloid, motivated his work on that question. Although al-Khāzinī’s Balance of Wisdom summarizes some of his work on centers of gravity, scholars have only al-Qūhī’s correspondence with al-Sābī on the subject, in which he correctly located the centers of gravity of triangles (and cones) and segments of parabolas (and paraboloids), as well as of hemispheres (a result not found in Archimedes’s works). He conjectured, on the basis of these results, that the center of gravity of a semicircle divides the radius perpendicular to its diameter into two parts, so that the part nearer the diameter has to the radius the ratio of 3:7. He was fully aware, and defended the implication, of this result, namely that the ratio of the circumference of a circle to its diameter is 28/9, an insistence that earned him the incredulity of his correspondent and the severe censure of Abū al-Futūh al-Sari in his Falsification of the Premises of the Discourse of Abū Sahl al-Qūhī.

Also closely related to the medieval Islamic tradition of Archimedes’s work is Al-Qūhī’s Construction of a Regular Heptagon in the Circle. By the mid-tenth century, geometers such as al-Sijzī had become dissatisfied with Greek verging constructions, calling them “moving geometry.” (Verging constructions demanded that one insert a line segment of given length so that its endpoints rest on two given curves and so that it points [or “verges”] towards a given point.) Archimedes’s construction of the regular heptagon went beyond the usual verging construction in demanding not that the line inserted between two straight lines have a certain length but that the two triangles created thereby have equal areas. (One of al-Q¯hī’s contemporaries, Abū al-Jūd, described this particularly opaque auxiliary construction as “perhaps more difficult than the task itself.”) It was in the context of this discussion of the limits of a proper construction that al-Quhi wrote, in his preface to the work, that he had done what Archimedes had been unable to do. By this he meant that his construction used not verging but the intersection of conic sections.
Influence of Apollonius Al-Qūhimacr;’s On Tangent Circles deals with constructing circles tangent to two given circles or straight lines (or passing through two given points) and having their centers on a given line. This is reminiscent of Apollonius’s famous three-circles problem. Al-Qūhī also considered the case when the line is not just straight or a conic section but any curved line (though what he meant by that is not specified).

Al-Qūhī used freely the classical method of analysis and synthesis, familiar from his study of the works of Apollonius. One example is his Drawing Two Lines from a Known Point, a work probably motivated by his Treatise on the Astrolabe, in which he cited two results from Drawing Two Lines. Among the dozen problems he considers in Drawing Two Lines, the following is a typical one: Point A and line (not necessarily straight) BG are given; assuming this, draw two straight line segments from A to BG, containing a given angle, so that the two segments AB and AG have to each other a given ratio.

Al-Qūhī’s analysis of each problem reduces it to a previously analyzed problem, but no synthesis is ever given. Work like this on analysis was likely the motivation for his treatise, Additions to the Data, which adds a number of new propositions and a new notion to Euclid’s Data.


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