Nicolaus Copernicus Guide, Meaning , Facts, Information and Description
Nicolaus (or Nicholas) Copernicus, (original name Kopernik or Koppernigk, Polish Mikołaj Kopernik, German Nikolaus Kopernikus February 19, 1473 – May 24, 1543) was an astronomer, mathematician and an economist who developed a heliocentric (Sun-centred) theory of the solar system in a form detailed enough to make it scientifically useful. He was also a church canon, governor and administrator, a jurist, astrologer and a doctor. His theory about the Sun as the centre of the solar system, turning over the traditional geocentric theory (that placed Earth at the centre of the Universe), is considered one of the most important discoveries ever, and is the fundamental starting point of modern astronomy and modern science itself (it inaugurated the Scientific Revolution). His theory affected many other aspects of human life. Nicolaus Copernicus University in Toruń, established 1945, is named after him.
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2 The Copernican heliocentric system 3 Copernicus and Copernicanism 4 Discussion 5 Quotes 6 Reference 7 External links |
Biography
Copernicus was born in 1473 in the city of Torun in Royal Prussia, Poland. His father Nikolas, a citizen of Krakow (at that time the capital of Poland), moved there in 1460 and became a respected citizen of Torun as well, once the war with Teutonic Knights was over. He was ten years of age when his father, a wealthy businessman and copper trader, died. Little is known of his mother, Barbara Watzenrode, but she appears to have predeceased her husband. His maternal uncle, Lucas Watzenrode, a church canon and later the Prince-Bishop governor of Warmia, raised him and his three other siblings after the death of Copernicus' father. His brother Andrew became canon in Frombork. A sister, Barbara, became a Benedictine nun and the other sister, Katharina, married a businessman and city councillor, Barthel Gertner.
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In 1491 Copernicus entered the University of Krakow, and here he encountered astronomy for the first time, thanks to his teacher Albert Brudzewski. This science soon fascinated him, as his books (stolen by Swedes during The Deluge, and now in Uppsala's library) show. After four years and a brief stay in Torun, he moved to Italy, where he studied law and medicine at the universities of Bologna and Padua. His uncle financed his education and wished for him to become a bishop as well. However, while studying canon and civil law at Ferrara, he met his teacher Domenico Maria Novara da Ferrara, a famous astronomer. He followed his lessons and became a disciple and assistant.
The first observation Copernicus made in 1497 together with Domenico Novara, are recorded in De revolutionibus orbium coelestium.
In 1497 his uncle was ordained the bishop of Warmia and Copernicus was named a canon in the Frombork cathedral, but he waited in Italy for the great Jubilee of 1500, so he went to Rome, where he could observe a lunar eclipse and where he gave some lessons of astronomy or math (unfortunately nothing of this remains to us).
He would have then visited Frombork only in 1501. As soon as he reached this town, he asked and obtained permission to return to Italy to complete his studies in Padua (with Guarico and Fracastoro) and in Ferrara (with Bianchini), where in 1503 received his doctoral degree in canon law. It has been supposed that it was in Padua that he gained access to those passages of Cicero and Plato about the opinion of Ancients on the movement of the Earth, having the first intuition of his theory. His collection of observations and ideas on the theory started in 1504.
Having left Italy at the end of his studies, he came to live and work in Frombork. Some time before his return to Warmia, he had received a position at the Collegiate Church of the Holy Cross in Wrocław;, Silesia, which he held for many years until he resigned a few years prior to his death, when he progressively became ill. Throughout his lifetime he made astronomical observations and calculations, but always in his spare time and never as a profession.
Copernicus worked for years with Prussian diet on monetary reform and published some studies about the value of money; as a governor of Warmia, he administered taxes and dealt out justice. It was at this time that Copernicus came up with one of the earliest iterations of the theory now known as Gresham's Law. During these years he also travelled extensively on government business and as a diplomat, on the behalf of the Prince-Bishop of Warmia.
In 1514 he made his "Commentariolus" - a short, handwritten text describing his ideas about the heliocentric hypothesis - available to his friends. From there he continued gathering evidence for a more detailed work.
During the war between Teutonic Order and Kingdom of Poland (1519-1524) Copernicus successfully defended Olsztyn on the head of royal troops besiged by the troops of Albert of Brandenburg.
In 1533 Copernicus delivered a series of lectures in Rome outlining his theory and received no reprimand from the Church. In 1536 his work was already in a definitive form, and some rumours about his theory had reached the scientists of all Europe. From many parts of the continent, Copernicus received invitations to publish it, but he felt quite apprehensive of persecution for his revolutionary work by the establishment of the time. The cardinal Nicola Schonberg of Capua wrote him for a copy of his manuscript, and this made Copernicus, who saw in this a certain nervousness of the Church, even more frightened of eventual reactions.
Copernicus was still completing his work (even if he was not convinced to publish it), when in 1539 Georg Joachim Rheticus, a great mathematician at Wittenberg, directly arrived in Frombork. Philipp Melanchthon had arranged with several astronomers for Rheticus to visit and study with them. Rheticus became a disciple of Copernicus' and stayed with him for two years, in which he wrote a book, Narratio prima, in which he included the essence of the theory.
In 1542, in the name of Copernicus, Rheticus published a treatise on trigonometry (later included in the second book of De revolutionibus). Under the strong pressure from Rheticus, and having seen that the first general reception of his work had not been favorable, Copernicus finally agreed to give the book to his close friend Tiedemann Giese, (the bishop of Chelmno Land), to be delivered to Rheticus for printing at Nuremberg.
Legend says that the first printed copy of De revolutionibus was put in Copernicus's hands the same day of his death, so that he could say goodbye to his opus vitae. He - allegedly - awoke from his stroke induced coma, looked at his book, and died peacefully.
Copernicus was buried in the Frombork Cathedral. However, a group of archaeologists searching for the body of Copernicus in 2004 failed to find the corpse of the astronomer. They found, however, several interesting graves from various time periods. The search for the body of Copernicus will continue in 2005.
See also discussion about Copernicus' nationality.
Aristarchus of Samos (3rd century BC) developed some theories by Heraclides Ponticus (already talking about a revolution of our planet on its axis) to propose what is, to the best of our knowledge, the first serious model of a heliocentric solar system. Unfortunately, his work about his heliocentric hypothesis did not survive, so we can only speculate about what led him to his conclusions. It is notable that, according to Plutarch, a contemporary of Aristarchus accused him of impiety for "putting the Earth in motion".
Copernicus cited Aristarchus and Philolaus in an early manuscript of his book which has survived, stating: "Philolaus believed in the mobility of the earth, and some even say that Aristarchus of Samos was of that opinion." For reasons unknown he crossed out this passage before publication of his book.
Copernicus' major theory was published in the book De revolutionibus orbium coelestium ("On the Revolutions of the Heavenly Spheres") in the year of his death 1543, even though he had arrived at it several decades earlier.
This book marks the beginning of the shift from a geocentric (and anthropocentric) universe with the Earth at its centre. Copernicus held that the Earth is another planet revolving around the fixed sun once a year, and turning on its axis once a day. He arrived at the correct order of the known planets and explained the precession of the equinoxes correctly by a slow change in the position of the Earth's rotational axis. He also gave a clear account of the cause of the seasons: that the Earth's axis is not perpendicular to the plane of its orbit. He added another motion to the Earth, by which the axis is kept pointed throughout the year at the same place in the heavens; from the time of Galileo it has been recognized that for it not to point to the same place would be a motion.
He also replaced Ptolemy's equant circles with epicycles. This is the main source of the statement that his system had even more epicycles than Ptolemy's. With this change his system had only uniform circular motions, correcting what seemed to be a defect in Ptolemy's system. Unfortunately, uniform circular motion is not what happens in the solar system, which runs on elliptical orbits; and this model was no more precise in predicting ephemerides than the then current tables based on Ptolemy's model. Furthermore, he badly underestimated the size of the solar system, like most of the astronomers of the time.
The system nevertheless had a large influence on scientists such as Galileo, Tycho Brahe, and Johannes Kepler, who adopted, championed and (especially in Kepler's case) improved the model.
Galileo's observation of the phases of Venus produced, however, the first observational evidence for Copernicus' theory.
The Copernican system can be summarized in seven propositions, as Copernicus himself collected them in a Compendium of De revolutionibus... that was found and published in 1878:
The work of Copernicus, "On the Revolution of Celestial Spheres" (1543), dedicated to the Pope Paul III, is divided into 6 books.
The first book contains a general vision of the heliocentric theory, and a summarized exposition of his idea on the World.
The second book is mainly theoretical and reports the principles of spherical astronomy and a list of stars (as a basis for the arguments developed in the following books).
The third book is mainly dedicated to the apparent movements of the Sun and to related phenomena.
The fourth book contains a similar description of the Moon and its orbital movements.
The fifth and the sixth books contain the concrete exposition of the new system.
Many meanings have been seen in his theory, quite apart from its scientific value. His work cut across science and religion, dogmatism and freedom of scientific investigation. His academic standing is often compared with Galileo.
When his work was published, it contradicted then accepted religious dogma: the suggestion being that there is no need for an entity (God) that from outside could give a soul, a power and a life to the World and to Human beings when science can explain everything attributed to Him.
However, Copernicanism also opened a way to immanence, the view that the divine force, or the divine being, pervades through all things that exist, which has been developed further in modern philosophy. Immanentism also leads into subjectivism: the theory that perception creates reality, and that there is no underlying, true, reality that exists independent of perception. Accordingly some find that Copernicanism demolished the foundations of mediaeval science and metaphysics.
One of the consequences of Copernicanism is that scientific laws must not necessarily coincide with appearance. This contrasts with Aristotle's system, which placed much more value on knowledge gained from the senses.
Copernicus' innovation was a scientific revolution. Some say "the" revolution ([1]). Immanuel Kant, for instance, caught the symbolic character of Copernicus' revolution (of which he put in evidence the trascendental rationalism) postulating that human rationality was the real legislator of observed phenomena. More recent philosophers also have found Copernicanism to remain valid and retain valuable philosophical meaning.
Copernicus' lived in early 16th century Prussia and Poland, and was influenced by the cultural, religious, and social contexts of life at the time. He was well educated. At the University of Kraków, which he attended in 1491 and 1492, Copernicus studied both mathematics and astronomy in common with all university students of that time. There is evidence that his interest in these subjects continued after he had left Kraków.
The Earth-centred Ptolemaic cosmology had been the accepted model of the universe since the 2nd century BC. Ptolemy's model explained each planet's circular motion individually and was the first model of the universe to explain some of the eccentric behaviour of the planets. It maintained that all planetary motion, and the motion of the Moon, the Sun, and the stars was circular, around a stationary Earth.
An accurate calculation of the astronomical year was important to a clergyman, like Copernicus, allowing him to forecast properly the various festivals that comprised the liturgical calendar. The mathematical confusion that Copernicus said caused him to develop an alternative to the geocentric model derived from an inadequate reconciliation of the Aristotelian model and amendments to it by Ptolemy.
The Ptolemaic geocentric model was complicated and inconsistent in Copernicus' estimations and observations, including one in 1497 of the star Aldebaran, that did not coincide with predictions made by Ptolemy. Nor did the Ptolemaic model explain precession. Precession is the phenomenon by which the Earth's axis "wobbles". This characteristic of the Earth's movement is apparent only with observation over long periods of time. In Copernicus' view, Ptolemy's explanation failed to provide an accurate mathematical description of the universe. His heliocentric universe theory accomplished this by dispensing with individual explanations for the motion of each planet, and replacing them with a description that applied to all the planets, including the Earth.
Copernicus' mathematical experience engendered in his thought a desire for a simpler and more elegant model of the universe. He was acquainted with ideas espoused by other classical authors. Some of the ideas expressed by Philalaus (5th century BC) and Heraclides (4th century BC), proposed cosmological models in which the Earth moved. Aristarchus (3rd century BC) proposed an openly heliocentric model of the universe. Heraclides' description of the revolutions of Mercury and Venus around the Sun might have led Copernicus to consider that the other planets, including the Earth, did the same.
Elegance was a consequence of the overall simplicity of Copernicus' cosmology and much of this seeming simplicity resulted from his retention of circular orbits for the planets around the central Sun. Copernicus used the eccentrics, epicycles, and equants of Ptolemaic cosmology, but added three kinds of motion to describe the observed behaviour of the Earth:
In his own preface to his work, dedicated to Pope Paul III, Copernicus took care to point out that his motives for developing a cosmology that included a moving, rather than a stationary, Earth, were inspired by his dissatisfaction with the mathematical and astronomical descriptions of the geocentric model, and were not intended to defy the written Word. "Mathematics", he says, "is written for mathematicians". Copernicus seems to have been benefited from the attitude of the bishops who were his superiors in the church - Johann Dantiscus and Tiedmann Giese. Both preferred, at least initially, to promote tolerance of differing views within the church rather than open discord, and both encouraged Copernicus' publication of his scientific beliefs. However, the lenient attitudes in Chelmno, where Copernicus carried out much of his work, began to change and might have contributed to Copernicus' isolation in the last years of his life. For orthodox Catholics, the Copernican model of the universe might have seemed too radically different from the geocentric model, sustained as it was by its agreement with many scriptural references. They might not have been ready to change to an understanding of the Bible as a source only of moral and spiritual, rather than scientific, wisdom.
As far as Copernicus was concerned, the Sun, a distinctive element in classical thought, held the central and most important position in the universe, gave added credence to his cosmology. His reverence for the sun can be seen in the most famous passage of de Revolutionibus:
DC Goodman, CA Russell, eds. The Rise of Scientific Europe 1500-1800. Bath, UK: Hodder &
This is an Article on Nicolaus Copernicus. Page Contains Information, Facts Details or Explanation Guide About Nicolaus Copernicus The Copernican heliocentric system
Earlier theories
Much has been written about earlier heliocentric theories. Philolaus (4th century BC) was one of the first to suppose a movement of the Earth, probably inspired by Pythagoras's theories on a spherical Globe.Copernican Theory
These propositions represent the exact contrary of what the dominant geocentric propositions stated.De Revolutionibus Orbium Coelestium
Main article: De Revolutionibus Orbium Coelestium. Copernicus and Copernicanism
Copernicus' theories have an extraordinary relevance in the history of human knowledge. Many authors suggest that only Euclidean geometry, Charles Darwin's Evolutionism, or Newton's physics could have a similar influence on human culture in general and on science in particular.Discussion
Until 1543, the year that Copernicus died, and the year in which his de Revolutionibus was published, and for many years afterwards, Copernicus' description of the motion of the Earth was not ratified by empirical evidence. In his unauthorized and anonymous preface to de Revolutionibus, Andreas Osiander was technically correct when he made reference to "the hypothesis of this work". However, its consistency with the observed behaviour of the universe in a time before the telescope made more detailed observation and the gathering of more accurate measurements practicable, gave the Copernican model its strongest support. Not much more than a century later, Kepler had certainly despatched the circular orbits of the planets and replaced them with ellipses, but the Copernican heliocentric universe was still intact.
In this discussion of Copernicus' reasons for discarding such a long-held belief as the geocentric cosmology of Ptolemy, we can see that the Copernican revolution was simmering against a background revolution of theological thought — the Reformation. Neo-Platonic and classical ideas formed the intellectual environment in which Copernicus worked. Although not holding ordained office within the Catholic Church, Copernicus was devout and unwilling to be openly defiant of the Church's teaching, but, in common with supporters of the Reformation, Copernicus was criticizing orthodox theory and belief. His reasons for doing so lay in his dissatisfaction with the inadequacies of the geocentric model, in his strong belief in the truth of the solution to the problem that he developed, its elegance and relative simplicity, and its coincidence with observation and with the classical ideals to which he had subscribed since his youth.Quotes
Goethe:
Copernicus:
See also: inferior planet, superior planetReference
External links
