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Omschrijving

This book provides the first comprehensive analysis of planetary observations preserved in Ibn Yunus's (d. 1009 CE) Hakimi zij, a unique treasure from the classical period of Islamic astronomy (9th -10th centuries). It offers readers a detailed reconstruction of how medieval astronomers observed, tested, and refined quantitative planetary theories developed on the basis of Ptolemaic models, revealing the dynamic interplay between empirical practice and theoretical innovation.

The study focuses on the observational records of Habash, al-Mahani, Ibn Yunus, and the Banu Amajur family, situating them within the broader intellectual tradition of early Islamic astronomy. By examining these selective but invaluable reports, the book demonstrates how astronomers used conjunctions, appulses, and occultations to evaluate the accuracy of planetary theories and to propose corrective strategies to refine them. The analysis is broadened to include other prominent figures, such as Battani, Ibn al-Alam, Kushyar, and Biruni, in order to assess whether and in what manner their theories were contingent upon observational activities and empirical methodologies.

The main topics include: the methodological link between observation and theory in Islamic astronomy; technical reconstructions of sky configurations to assess visibility, precision, and instrument capability; the identification of anomalies in Ptolemaic planetary models and the corrective strategies (istidrak/tashih) devised by Islamic astronomers; and the transformation of tools from printed ephemerides to modern sky-simulation software that now allow scholars to revisit ancient records with clarity.

These topics are important and relevant because they challenge the prevailing narrative of Islamic astronomy. The evidence shows a vibrant culture of empirical testing, methodological innovation, and theoretical refinement. The book highlights how Islamic astronomers recognized deep-seated deficiencies in Ptolemaic models and developed heuristic remedies, anticipating later scientific transformations.

Historians of science, scholars of Islamic intellectual history, astronomers interested in the evolution of observational practice, and early-career researchers seeking methodological clarity in the study of historical astronomy will find great value in this text.