Islamic astronomy (also called Arabic astronomy or Islamicate astronomy) refers to the astronomical theories, observational practices, and instruments developed within the Islamic world from roughly the 8th to the 16th centuries CE, encompassing scholars writing primarily in Arabic and Persian across a geographic range from Spain to Central Asia. The term is used by historians of science to denote a tradition rather than a single school of thought, and its boundaries-chronological, geographic, and methodological-are themselves subject to differing scholarly framings; see islamic-astronomy-viewpoint-definitional-scope-viewpoint.

Modern historians of science generally treat Islamic astronomy as a distinct and sophisticated tradition that synthesized earlier Greek (notably Ptolemaic), Indian, and Persian astronomical knowledge, and that produced original contributions in planetary modeling, observational instrumentation, and mathematical methods. Centers of activity included Baghdad, Damascus, Cairo, Cordoba, Samarkand, and Maragha, often supported by observatories and patronage from rulers. Among the most discussed figures and works are al-Battani's revisions to Ptolemaic solar and stellar parameters, the Maragha school's critiques of Ptolemaic astronomy (including work attributed to Qutb al-Din al-Shirazi's Tadhkira fi 'ilm al-hay'a), and the Zij-i Ilkhani, an astronomical handbook produced under Nasir al-Din al-Tusi at the Maragha observatory. For a fuller historical account, see Islamic Astronomy - History.

A central area of ongoing scholarly discussion concerns the degree and nature of the relationship between late Islamic astronomical models-particularly those of the Maragha school-and the heliocentric model proposed by Nicolaus Copernicus in De revolutionibus orbium coelestium (1543, Julian calendar). Some historians argue for direct or indirect transmission of specific mathematical devices, while others caution against overstating the connection or argue similarities arose independently. This question is treated in detail at islamic-astronomy-debate-transmission-debate.

There is broad consensus among historians of science that Islamic astronomers preserved, critiqued, and substantially extended Greek astronomical models, and that the Tusi-couple-a geometrical device developed by Nasir al-Din al-Tusi to eliminate Ptolemy's equant-was an original mathematical contribution of the Maragha school. See islamic-astronomy-greek-synthesis-consensus. Whether this and related devices were transmitted to and employed by Copernicus, versus arrived at independently, is not settled and is addressed separately in the debate noted above.

• Transmissionist viewpoint - holds that specific mathematical and observational techniques from the Maragha school and related traditions were transmitted to European astronomers, including Copernicus, through channels such as Byzantine Greek manuscripts, Italian humanist networks, or other contact points, and that this transmission was a meaningful contributor to the Copernican model. See islamic-astronomy-transmissionist-viewpoint.
• Independent-discovery viewpoint - holds that mathematical similarities between Islamic devices like the Tusi-couple and elements of Copernicus's model are better explained by independent derivation from shared Ptolemaic problems, given the absence of direct documentary evidence of transmission to Copernicus specifically. See islamic-astronomy-independent-discovery-viewpoint.
• Continuity viewpoint - frames Islamic astronomy as a continuous link in an unbroken chain of astronomical inquiry from Babylonian and Greek antecedents through to early modern Europe, emphasizing cumulative development over any single transmission event. See islamic-astronomy-continuity-viewpoint.
• Decline-and-rupture viewpoint - holds that Islamic astronomical inquiry, after a period of innovation associated with figures such as al-Battani and the Maragha school, underwent institutional and intellectual decline in subsequent centuries, a characterization disputed by some historians as overly schematic. See islamic-astronomy-decline-rupture-viewpoint.

• The “Islamic debt” debate over whether and to what extent Copernicus's heliocentric model depended on prior Islamic astronomical work, particularly Maragha-school devices, remains a documented and active dispute among historians of science with identifiable competing camps and publications. See islamic-astronomy-controversy-islamic-debt-controversy.

• Islamic Astronomy - History
• islamic-astronomy-debate-transmission-debate
• islamic-astronomy-greek-synthesis-consensus
• islamic-astronomy-transmissionist-viewpoint
• islamic-astronomy-independent-discovery-viewpoint
• islamic-astronomy-continuity-viewpoint
• islamic-astronomy-decline-rupture-viewpoint
• islamic-astronomy-controversy-islamic-debt-controversy
• Heliocentrism
• Ptolemaic Astronomy

1. George Saliba, *Islamic Science and the Making of the European Renaissance* (Cambridge, MA: MIT Press, 2007).
2. F. Jamil Ragep, “Copernicus and His Islamic Predecessors: Some Historical Remarks,” *History of Science* 45, no. 1 (2007): 65-81.
3. Edward S. Kennedy, “A Survey of Islamic Astronomical Tables,” *Transactions of the American Philosophical Society* 46, no. 2 (1956): 123-177.
4. Willy Hartner, “The Tusi-Couple: A Discussion of the Material,” in *Studies in Astronomy, Astrology and Mechanics in Islamic Civilization* (Istanbul: International Congress for the History of Sciences, 1977).
5. David A. King, *Astronomy in the Service of Islam* (Aldershot: Variorum, 1993).
6. Nasir al-Din al-Tusi, *Zij-i Ilkhani* (Maragha, 13th century).
7. Qutb al-Din al-Shirazi, *al-Tadhkira fi 'ilm al-hay'a* (13th century).
8. Nicolaus Copernicus, *De revolutionibus orbium coelestium* (Nuremberg, 1543).