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Bound in attractive, contemporary Parisian calf with some discreet repairs. The boards are blind-ruled and adorned with gold-tooled ornaments. This is one of very few to have appeared on the market in a contemporary binding. The text is in excellent condition, with just minor blemishes (small early erasure of an ownership inscription on the title just slightly touching the "D." in the date. Light damp-staining to first six leaves.) Collation as in Horblit; this copy without the errata leaf -printed separately and later- that is found in a minority of copies (about 20 percent). Preserved in a morocco-backed box. Provenance: At the foot of the title-page, an early signature has been thoroughly lined through. 17th- or 18th-century inscription on title of the Jesuit College of Paris. Bookplate of Gustavus Wynne Cook (1867-1940, amateur astronomer, collector, and benefactor of the Franklin Institute). Franklin Institute bookplate. Sold at Sotheby Parke-Bernet, New York, November 1977, lot 85. Purchased by Pierre Berès at Sotheby's London, 21 October 1980 and sold to a prominent Spanish private collector. "The earliest of the three books of science that most clarified the relationship of man and his universe (along with Newton's Principia and Darwin's Origin of Species)." - Dibner, Heralds of Science, 3. This work is the foundation of the heliocentric theory of the planetary system and the most important scientific text of the 16th century. Copernicus began to work on astronomy on his own. Sometime between 1510 and 1514 he wrote an essay that has come to be known as the Commentariolus that introduced his new cosmological idea, the heliocentric system, and he sent copies to various astronomers. He continued making astronomical observations whenever he could, hampered by the poor position for observations in Frombork and his many pressing responsibilities as canon. Nevertheless, he kept working on his manuscript of On the Revolutions. In 1539 a young mathematician named Georg Joachim Rheticus (1514-1574) from the University of Wittenberg came to study with Copernicus. Rheticus brought Copernicus books in mathematics, in part to show Copernicus the quality of printing that was available in the German-speaking cities. He published an introduction to Copernicus's ideas, the Narratio prima (First Report). Most importantly, he convinced Copernicus to publish On the Revolutions. Rheticus oversaw most of the printing of the book, and on 24 May 1543 Copernicus held a copy of the finished work on his deathbed. It is impossible to date when Copernicus first began to espouse the heliocentric theory. Had he done so during his lecture in Rome, such a radical theory would have occasioned comment, but there was none, so it is likely that he adopted this theory after 1500. His first heliocentric writing was his Commentariolus. It was a small manuscript that was circulated but never printed. We do not know when he wrote this, but a professor in Cracow cataloged his books in 1514 and made reference to a "manuscript of six leaves expounding the theory of an author who asserts that the earth moves while the sun stands still" (Rosen, 1971, 343). Thus, Copernicus probably adopted the heliocentric theory sometime between 1508 and 1514. Rosen (1971, 345) suggested that Copernicus's "interest in determining planetary positions in 1512-1514 may reasonably be linked with his decisions to leave his uncle's episcopal palace in 1510 and to build his own outdoor observatory in 1513." In other words, it was the result of a period of intense concentration on cosmology that was facilitated by his leaving his uncle and the attendant focus on church politics and medicine. In the Commentariolus, Copernicus listed assumptions that he believed solved the problems of ancient astronomy. He stated that the earth is only the center of gravity and center of the moon's orbit; that all the spheres encircle the sun, which is close to the center of the universe; that the universe is mutable.

Nicolaus Copernicus' groundbreaking work on heliocentrism is encapsulated in his seminal book "De revolutionibus orbium coelestium" (On the Revolutions of the Heavenly Spheres). This work, published in 1543, marked a significant departure from the geocentric model that had dominated astronomical thought for centuries. Copernicus proposed that the Sun, rather than the Earth, was at the center of the universe, with the Earth and other planets revolving around it. "De revolutionibus" begins with seven axioms outlining the heliocentric theory. These include the notions that the Earth rotates daily on its axis and revolves annually around the Sun. Copernicus provided detailed mathematical proofs and astronomical observations to support his heliocentric model. He described the motions of the planets more accurately than the Ptolemaic system, which placed the Earth at the center. While still using some elements of the Ptolemaic system, like epicycles, Copernicus significantly simplified the complex system of planetary motions. The publication of "De revolutionibus" is often considered the starting point of the Scientific Revolution. It fundamentally changed the way humanity understood the cosmos and our place within it. Initially, the book did not cause a major stir, but eventually, the Catholic Church condemned it, placing it on the Index of Forbidden Books in 1616 due to its contradiction with the geocentric view supported by the Church. Despite this, Copernicus' heliocentric theory paved the way for later astronomers like Johannes Kepler and Galileo Galilei, who further developed and provided more evidence for the heliocentric model. The book is divided into six parts. Book I outlines the heliocentric theory and provides a general explanation of the universe. Book II covers the principles of spherical astronomy as a basis for the heliocentric theory. Book III discusses the precession of the equinoxes and the apparent motion of the Sun. Book IV focuses on the Moon and its motion. Book V examines the motions of the planets, including retrograde motion. Finally, Book VI discusses the order of the planets and the orbit of the Earth, as well as an explanation of the various phenomena observed from Earth. Nicolaus Copernicus' "De revolutionibus orbium coelestium" was a groundbreaking work that challenged the long-held geocentric model of the universe. By placing the Sun at the center and describing the motions of the planets around it, Copernicus laid the foundation for modern astronomy and the scientific revolution. His work fundamentally altered humanity's understanding of the cosmos and set the stage for future astronomical discoveries. This work is now rare and highly valuable.