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Nicolaus Copernicus POLISH ASTRONOMER

Nicolaus

Copernicus,

Polish Mikołaj

Kopernik,

German Nikolaus

Kopernikus, (born February 19, 1473, Toruń, Royal Prussia, Poland—died May 24, 1543, Frauenburg, East Prussia [now Frombork, Poland]), Polish astronomer who proposed that the planets have the Sun as the fixed point to which their motions are to be referred; that Earth is a planet which, besides orbiting the Sun annually, also turns once daily on its own axis; and that very slow long-term changes in the direction of this axis account for the precession of the equinoxes. This representation of the heavens is usually called the heliocentric, or “Sun-centred,” system—derived from the Greek helios, meaning “Sun.” Copernicus’s theory had important consequences for later thinkers

of

the

Scientific Revolution,

including

such

major

figures

as Galileo, Kepler, Descartes, and Newton. Copernicus probably hit upon his main idea sometime between 1508 and 1514, and during those years he wrote a manuscript usually called the Commentariolus (“Little Commentary”). However, the book that contains the final version of his theory, De revolutionibus orbium coelestium libri vi (“Six Books Concerning the Revolutions of the Heavenly Orbs”), did not appear in print until 1543, the year of his death.

Early Life And Education Certain facts about Copernicus’s early life are well established, although a biography written by his ardent disciple Georg Joachim Rheticus (1514–74) is unfortunately lost. According to a later horoscope, Nicolaus Copernicus was born on February 19, 1473, in Toruń, a city in north-central Poland on the Vistula River south of the major Baltic seaport of Gdańsk. His father, Nicolaus, was a well-to-do merchant, and his mother, Barbara Watzenrode, also came from a leading merchant family. Nicolaus was the youngest of four children. After his father’s death, sometime between 1483 and 1485, his mother’s brother Lucas Watzenrode (1447–1512) took his nephew under his protection. Watzenrode, soon to be bishop of the chapter of Varmia (Warmia), saw to young Nicolaus’s education and his future career as a church canon. (See Researcher’s Note for information about Copernicus’s nationality.)

Between 1491 and about 1494 Copernicus studied liberal arts— including astronomy and astrology—at the University of Cracow (Kraków). Like many students of his time, however, he left before completing his degree, resuming his studies in Italy at the University of Bologna, where his uncle had obtained a doctorate in canon law in 1473. The Bologna period (1496–1500) was short but significant. For a time Copernicus lived in the same house as the principal astronomer at the university, Domenico Maria de Novara (Latin: Domenicus Maria Novaria Ferrariensis; 1454–1504). Novara had the responsibility of issuing annual astrological prognostications for the city, forecasts that included all social groups but gave special attention to the fate of the Italian princes and their enemies. Copernicus, as is known from Rheticus, was “assistant and witness” to some of Novara’s observations, and his involvement with the production of the annual forecasts means that he was intimately familiar with the practice of astrology. Novara also probably introduced Copernicus to two important books that framed his future problematic as a student of the heavens: Epitoma in Almagestum Ptolemaei (“Epitome of Ptolemy’s Almagest”) by Johann Müller (also known as Regiomontanus, 1436–76) and Disputationes adversus astrologianm divinatricenm (“Disputations against Divinatory Astrology”) by Giovanni Pico della Mirandola (1463–94). The first provided a summary of the foundations of Ptolemy’s astronomy, with Regiomontanus’s corrections and critical expansions of certain important planetary models that might have been suggestive to Copernicus of directions leading to the heliocentric hypothesis. Pico’s Disputationes offered a devastating skeptical attack on the foundations of astrology that reverberated into the 17th century. Among Pico’s criticisms was the charge that, because astronomers disagreed about the order of the planets, astrologers could not be certain about the strengths of the powers issuing from the planets.

Only 27 recorded observations are known for Copernicus’s entire life (he undoubtedly made more than that), most of them concerning eclipses, alignments, and conjunctions of planets and stars. The first such known observation occurred on March 9, 1497, at Bologna. In De revolutionibus, book 4, chapter 27, Copernicus reported that he had seen the Moon eclipse “the brightest star in the eye of the Bull,” Alpha Tauri (Aldebaran). By the time he published this observation in 1543, he had made it the basis of a theoretical claim: that it confirmed exactly the size of the apparent lunar diameter. But in 1497 he was probably using it to assist in checking the new- and full-moon tables derived from the commonly used Alfonsine Tables and employed in Novara’s forecast for the year 1498.

In 1500 Copernicus spoke before an interested audience in Rome on mathematical subjects, but the exact content of his lectures is unknown. In 1501 he stayed briefly in Frauenburg but soon returned to Italy to continue his studies, this time at the University of Padua, where he pursued medical studies between 1501 and 1503. At this time medicine was closely allied with astrology, as the stars were thought to influence the body’s dispositions. Thus, Copernicus’s astrological experience at Bologna was better training for medicine than one might imagine today. Copernicus later painted a selfportrait; it is likely that he acquired the necessary artistic skills while in Padua, since there was a flourishing community of painters there and in nearby Venice. In May 1503 Copernicus finally received a doctorate—like his uncle, in canon law—but from an Italian university where he had not studied: the University of Ferrara. When he returned to Poland, Bishop Watzenrode arranged a sinecure for him: an in absentia teaching post at Wrocław. Copernicus’s actual duties at the bishopric palace, however, were largely

administrative and medical. As a church canon, he collected rents from church-owned lands; secured military defenses; oversaw chapter finances; managed the bakery, brewery, and mills; and cared for the medical needs of the other canons and his uncle. (Despite serving as a canon, Copernicus did not become a priest.) Copernicus’s astronomical work took place in his spare time, apart from these other obligations. He used the knowledge of Greek that he had acquired during his Italian studies to prepare a Latin translation of the aphorisms of an obscure 7th-century Byzantine historian and poet, Theophylactus Simocattes. The work was published in Cracow in 1509 and dedicated to his uncle. It was during the last years of Watzenrode’s life that Copernicus evidently came up with the idea on which his subsequent fame was to rest.

Nicolaus Copernicus Copernicus’s reputation outside local Polish circles as an astronomer of considerable ability is evident from the fact that in 1514 he was invited to offer his opinion at the church’s Fifth Lateran Council on the critical problem of the reform of the calendar. The civil calendar then in use was still the one produced under the reign of Julius Caesar, and, over the centuries, it had fallen seriously out of alignment with the actual positions of the Sun. This rendered the dates of crucial feast days, such as Easter, highly problematic. Whether Copernicus ever offered any views on how to reform the calendar is not known; in any event, he never attended any of the council’s sessions. The

leading calendar reformer was Paul of Middelburg, bishop of Fossombrone. When Copernicus composed his dedication to De revolutionibus in 1542, he remarked that “mathematics is written for mathematicians.” Here he distinguished between those, like Paul, whose mathematical abilities were good enough to understand his work and others who had no such ability and for whom his work was not intended

Copernicus’s Astronomical Work The contested state of planetary theory in the late 15th century and Pico’s attack on astrology’s foundations together constitute the principal historical considerations in constructing the background to Copernicus’s achievement. In Copernicus’s period, astrology and astronomy were considered subdivisions of a common subject called the “science of the stars,” whose main aim was to provide a description of the arrangement of the heavens as well as the theoretical tools and tables of motions that would permit accurate construction of horoscopes and annual prognostications. At this time the terms astrologer, astronomer, and mathematician were virtually interchangeable; they generally denoted anyone who studied the heavens using mathematical techniques. Pico claimed that astrology ought to be condemned because its practitioners were in disagreement about everything, from the divisions of the zodiac to the minutest observations to the order of the planets. A second long-standing disagreement, not mentioned by Pico, concerned the status of the planetary models. From antiquity, astronomical modeling was governed by the premise that the planets move with uniform angular motion on fixed radii at a constant distance from their centres of motion. Two types of models derived from this premise.

Copernican heliocentrism

Heliocentric model from Nicolaus Copernicus' De revolutionibus orbium coelestium (On the Revolutions of the Heavenly Spheres

Copernican

heliocentrism is

the

name

given

to

the

astronomical model developed by Nicolaus Copernicus and published in 1543. This model positioned the Sun near the center of the Universe, motionless,

with Earth and

the

other planets orbiting around

it

in

circular paths, modified by epicycles, and at uniform speeds. The

Copernican model displaced the geocentric model of Ptolemy that had prevailed for centuries, which had placed Earth at the center of the Universe. Copernican heliocentrism is often regarded as the launching point to modern astronomy and the Scientific Revolution. Copernicus was aware that the ancient Greek Aristarchus had already proposed a heliocentric theory, and cited him as a proponent of it in a reference that was deleted before publication; however, there is no evidence that Copernicus had knowledge of, or access to, the specific details of Aristarchus' theory.[1] Although he had circulated an outline of his own heliocentric theory to colleagues sometime before 1514, he did not decide to publish it until he was urged to do so late in his life by his pupil Rheticus. Copernicus's challenge was to present a practical alternative to the Ptolemaic model by more elegantly and accurately determining

the

length

of

a

solar

year

while

preserving

the metaphysical implications of a mathematically ordered cosmos. Thus, his heliocentric model retained several of the Ptolemaic elements, causing inaccuracies such as the planets' circular orbits, epicycles, and uniform speeds,[2] while at the same time introducing such innovative ideas as: 

The Earth is one of several planets revolving around a stationary sun in a determined order.



The Earth has three motions: daily rotation, annual revolution, and annual tilting of its axis.



Retrograde motion of the planets is explained by the Earth's motion.



The distance from the Earth to the Sun is small compared to the distance from the Sun to the stars.

Contents 1Heliocentrism before Copernicus

 o

1.1Antiquity

o

1.2Middle Ages 

1.2.1Islamic astronomers



1.2.2European astronomers 

1.2.2.1Ptolemaic system



1.2.2.2Post-Ptolemy

2Copernican theory



2.1De revolutionibus orbium coelestium

o 

3Early criticisms



4Copernican Revolution



5Modern views o

5.1Substantially correct

o

5.2Modern historiography



6See also



7Notes



8References



9Further reading



10External links...


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