Abū Isḥāq Ibrāhīm ibn Yaḥyā al-Naqqāsh al-Zarqālī al-Tujibi^[1](Arabic: إبراهيم بن يحيى الزرقالي‎); also known asAl-ZarkaliorIbn Zarqala(1029–1087), was an Arab^[2][3][4]Muslim instrument maker, astrologer, and the most important astronomer from the western part of the Islamic world.^[1] 

  Although his name is conventionally given as al-Zarqālī, it is probable that the correct form was al-Zarqālluh.^[5]In Latin he was referred to asArzachelorArsechieles, a modified form ofArzachel, meaning ‘the engraver’.^[6]He lived in Toledo,Al-Andalusbefore moving to Córdoba later in his life. His works inspired a generation of Islamic astronomers in Al-Andalus, and later, after being translated, were very influential in Europe. His invention of the Saphaea (a perfected astrolabe) proved very popular and was widely used by navigators until the 16th century.^[7] 

  The crater Arzachel on the Moon is named after him.^[6] 

  Al-Zarqālī was born in a village near the outskirts of Toledo, the then capital of the Taifa of Toledo.  

  He was trained as a metalsmith and due to his burr skills he was nicknamedAl-Nekkach“the engraver of metals”. His Latinized name, ‘Arzachel’ is formed from the Arabical-Zarqali al-Naqqash, meaning ‘the engraver’.^[6] 

  He was particularly talented in Geometry andAstronomy. He is known to have taught and visited Córdoba on various occasions, and his extensive experience and knowledge eventually made him the foremost astronomer of his time. Al-Zarqālī was also an inventor, and his works helped to put Toledo at the intellectual center ofAl-Andalus. He is also referred to in the works of Chaucer, as ‘Arsechieles’.^[6] 

  In the year 1085 Toledo was taken by the Christian king of CastileAlfonso VI. Al-Zarqālī and his colleagues, such as Al‐Waqqashi (1017–1095) of Toledo, had to flee. It is unknown whether the aged Al-Zarqālī fled to Cordoba or died in a Moorish refugee camp.  

  His works influenced Ibn Bajjah (Avempace), Ibn Tufail (Abubacer), Ibn Rushd (Averroës), Ibn al-Kammad, Ibn al‐Haim al‐Ishbili and Nur ad-Din al-Betrugi (Alpetragius).  

  In the 12th century, Gerard of Cremona translated al-Zarqali’s works into Latin. He referred to Al-Zarqali as an astronomer and magician.^[6]Ragio Montanous wrote a book in the 15th century on the advantages of the Sahifah al-Zarqalia. In 1530, the German scholar Jacob Ziegler wrote a commentary on one of al-Zarqali’s works. In his “De Revolutionibus Orbium Coelestium”, in the year 1530, Nicolaus Copernicus quotes the works of al-Zarqali and Al-Battani.^[8] 

  Al-Zarqālī wrote two works on the construction of an instrument (an equatorium) for computing the position of the planets using diagrams of the Ptolemaic model. These works were translated into Spanish in the 13th century by order of King Alfonso X in a section of theLibros del Saber de Astronomiaentitled the “Libros de las laminas de los vii planetas”.  

  He also invented a perfected kind of astrolabe known as “the tablet of al-Zarqālī” (al-ṣafīḥā al-zarqāliyya), which was famous in Europe under the nameSaphaea.^[9][10] 

  There is a record of an al-Zarqālī who built a water clock, capable of determining the hours of the day and night and indicating the days of the lunar months.^[11]According to a report found in al-Zuhrī’sKitāb al-Juʿrāfīyya, his name is given as Abū al-Qāsim bin ʿAbd al-Raḥmān, also known as al-Zarqālī, which has made some historians think that this is a different person.^[5] 

  Al-Zarqali corrected geographical data fromPtolemyand Al-Khwarizmi. Specifically, he corrected Ptolemy’s estimate of the longitude of the Mediterranean sea from 62 degrees to the correct value of 42 degrees.^[8]In his treatise on the solar year, which survives only in a Hebrew translation, he was the first to demonstrate the motion of thesolar apogeerelative to the fixed background of the stars. He measured its rate of motion as 12.04 seconds per year, which is remarkably close to the modern calculation of 11.77 seconds.^[12]Al-Zarqālī’s model for the motion of the Sun, in which the center of the Sun’s deferent moved on a small, slowly rotating circle to reproduce the observed motion of the solar apogee, was discussed in the thirteenth century by Bernard of Verdun^[13]and in the fifteenth century by Regiomontanus and Peurbach. In the sixteenth century Copernicus employed this model, modified to heliocentric form, in hisDe Revolutionibus Orbium Coelestium.^[14] 

  Al-Zarqālī also contributed to the famousTables of Toledo, an adaptation of earlier astronomical data to the location of Toledo along with the addition of some new material.^[5]Al-Zarqālī was famous as well for his ownBook of Tables.Many “books of tables” had been compiled, but his almanac contained tables which allowed one to find the days on which the Coptic, Roman, lunar, and Persian months begin, other tables which give the position of planets at any given time, and still others facilitating the prediction of solar and lunar eclipses.  

  He also compiled an almanac that directly provided “the positions of the celestial bodies and need no further computation”. The work provided the true daily positions of the sun for four Julian years from 1088 to 1092, the true positions of the five planets every 5 or 10 days over a period of 8 years for Venus, 79 years for Mars, and so forth, as well as other related tables.^[15][16] 

  His Zij and Almanac were translated into Latin by Gerard of Cremona in the 12th century, and contributed to the rebirth of a mathematically basedastronomyin Christian Europe and were later incorporated into theTables of Toledoin the 12th century and theAlfonsine tablesin the 13th century.^[15] 

  In designing an instrument to deal with Ptolemy’s complex model for the planet Mercury, in which the center of the deferent moves on a secondary epicycle, al-Zarqālī noted that the path of the center of the primary epicycle is not a circle, as it is for the other planets. Instead it is approximately oval and similar to the shape of a pignon (or pine nut).^[17]Some writers have misinterpreted al-Zarqālī’s description of an earth-centered oval path for the center of the planet’s epicycle as an anticipation of Johannes Kepler’s sun-centered elliptical paths for the planets.^[18]Although this may be the first suggestion that aconic sectioncould play a role in astronomy, al-Zarqālī did not apply the ellipse to astronomical theory and neither he nor his Iberian or Maghrebi contemporaries used an elliptical deferent in their astronomical calculations.^[19] 

  Major Works and publications :