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Drawing on a half century of scholarship, of Polish studies of Copernicus and Cracow University, and of Copernicus's sources, this book offers a comprehensive re-evaluation of Copernicus's achievement, and explains his commitment to the uniform, circular motions of celestial bodies, and his views about hypotheses.
Taking into account the most important results of the scholarly literature since 1973 and the best Polish scholarship of the past century, this is the first comprehensive study of Copernicus's achievement in English that examines Copernicus's path to heliocentrism from the perspective of late medieval philosophy, the Renaissance recovery of ancient literature and science, and early-modern editions of books that Copernicus used. The principal goals are to explain his commitment to the existence of celestial spheres, and the logical foundations for his views about hypotheses. In doing so, the work elucidates the logical and philosophical background that contributed to his accomplishments, and explains the limitations of his achievement. Medieval and Early Modern Science, 12
An account of the Copernican Revolution, focusing on the significance of the plurality of the revolution which encompassed not only mathematical astronomy, but also conceptual changes in cosmology, physics, philosophy, and religion.
Between Copernicus and Galileo is the story of Christoph Clavius, the Jesuit astronomer and teacher whose work helped set the standards by which Galileo's famous claims appeared so radical, and whose teachings guided the intellectual and scientific agenda of the Church in the central years of the Scientific Revolution. Though relatively unknown today, Clavius was enormously influential throughout Europe in the late sixteenth and early seventeenth centuries through his astronomy books—the standard texts used in many colleges and universities, and the tools with which Descartes, Gassendi, and Mersenne, among many others, learned their astronomy. James Lattis uses Clavius's own publications as well as archival materials to trace the central role Clavius played in integrating traditional Ptolemaic astronomy and Aristotelian natural philosophy into an orthodox cosmology. Although Clavius strongly resisted the new cosmologies of Copernicus and Tycho, Galileo's invention of the telescope ultimately eroded the Ptolemaic world view. By tracing Clavius's views from medieval cosmology the seventeenth century, Lattis illuminates the conceptual shift from Ptolemaic to Copernican astronomy and the social, intellectual, and theological impact of the Scientific Revolution.
Galileo’s Dialogue Concerning the Two Chief World Systems, published in Florence in 1632, was the most proximate cause of his being brought to trial before the Inquisition. Using the dialogue form, a genre common in classical philosophical works, Galileo masterfully demonstrates the truth of the Copernican system over the Ptolemaic one, proving, for the first time, that the earth revolves around the sun. Its influence is incalculable. The Dialogue is not only one of the most important scientific treatises ever written, but a work of supreme clarity and accessibility, remaining as readable now as when it was first published. This edition uses the definitive text established by the University of California Press, in Stillman Drake’s translation, and includes a Foreword by Albert Einstein and a new Introduction by J. L. Heilbron.
The book examines why and how Copernicus became a Copernican and what his affirmation of heliocentrism and geokinetism means in the context of the Scientific Revolution. In examining his texts and sociocultural context the work analyses the appearance of a revolutionary figure of Copernicus as a Platonist astronomer-philosopher.
This major work by the German philosopher Hans Blumenberg is a monumental rethinking of the significance of the Copernican revolution for our understanding of modernity.
Recovering the forgotten discipline of Natural Philosophy for the modern world This book argues for the retrieval of 'natural philosophy', a concept that faded into comparative obscurity as individual scientific disciplines became established and institutionalized. Natural philosophy was understood in the early modern period as a way of exploring the human relationship with the natural world, encompassing what would now be seen as the distinct disciplines of the natural sciences, mathematics, music, philosophy, and theology. The first part of the work represents a critical conversation with the tradition, identifying the essential characteristics of natural philosophy, particularly its emphasis on both learning about and learning from nature. After noting the factors which led to the disintegration of natural philosophy during the nineteenth century, the second part of the work sets out the reasons why natural philosophy should be retrieved, and a creative and innovative proposal for how this might be done. This draws on Karl Popper's 'Three Worlds' and Mary Midgley's notion of using multiple maps in bringing together the many aspects of the human encounter with the natural world. Such a retrieved or 're-imagined' natural philosophy is able to encourage both human attentiveness and respectfulness towards Nature, while enfolding both the desire to understand the natural world, and the need to preserve the affective, imaginative, and aesthetic aspects of the human response to nature.
In 1984, Noel Swerdlow and Otto Neugebauer argued that Nicolaus Copernicus (1473–1543) explained planetary motion by using mathematical devices and astronomical models originally developed by Islamic astronomers in the thirteenth and fourteenth centuries. Was this a parallel development, or did Copernicus somehow learn of the work of his predecessors, and if so, how? And if Copernicus did use material from the Islamic world, how then should we understand the European context of his innovative cosmology? Although Copernicus’s work has been subject to a number of excellent studies, there has been little attention paid to the sources and diverse cultures that might have inspired him. Foregrounding the importance of interactions between Islamic and European astronomers and philosophers, Before Copernicus explores the multi-cultural, multi-religious, and multi-lingual context of learning on the eve of the Copernican revolution, determining the relationship between Copernicus and his predecessors. Essays by Christopher Celenza and Nancy Bisaha delve into the European cultural and intellectual contexts of the fifteenth century, revealing both the profound differences between “them” and “us,” and the nascent attitudes that would mark the turn to modernity. Michael Shank, F. Jamil Ragep, Sally Ragep, and Robert Morrison depict the vibrant and creative work of astronomers in the Christian, Islamic, and Jewish worlds. In other essays, Rivka Feldhay, Raz Chen-Morris, and Edith Sylla demonstrate the importance of shifting outlooks that were critical for the emergence of a new worldview. Highlighting the often-neglected intercultural exchange between Islam and early modern Europe, Before Copernicus reimagines the scientific revolution in a global context.
In Measuring Shadows, Raz Chen-Morris demonstrates that a close study of Kepler’s Optics is essential to understanding his astronomical work and his scientific epistemology. He explores Kepler’s radical break from scientific and epistemological traditions and shows how the seventeenth-century astronomer posited new ways to view scientific truth and knowledge. Chen-Morris reveals how Kepler’s ideas about the formation of images on the retina and the geometrics of the camera obscura, as well as his astronomical observations, advanced the argument that physical reality could only be described through artificially produced shadows, reflections, and refractions. Breaking from medieval and Renaissance traditions that insisted upon direct sensory perception, Kepler advocated for instruments as mediators between the eye and physical reality, and for mathematical language to describe motion. It was only through this kind of knowledge, he argued, that observation could produce certainty about the heavens. Not only was this conception of visibility crucial to advancing the early modern understanding of vision and the retina, but it affected how people during that period approached and understood the world around them.