De sphaera mundi

Last updated
A volvelle from a sixteenth-century edition of Sacrobosco's De Sphaera Sacrobosco Lunar eclipse.jpg
A volvelle from a sixteenth-century edition of Sacrobosco's De Sphaera

De sphaera mundi (Latin title meaning On the Sphere of the World, sometimes rendered The Sphere of the Cosmos; the Latin title is also given as Tractatus de sphaera, Textus de sphaera, or simply De sphaera) is a medieval introduction to the basic elements of astronomy written by Johannes de Sacrobosco (John of Holywood) c. 1230. Based heavily on Ptolemy's Almagest , and drawing additional ideas from Islamic astronomy, it was one of the most influential works of pre-Copernican astronomy in Europe.

Contents

Reception

Sacrobosco's De sphaera mundi was the most successful of several competing thirteenth-century textbooks on this topic. It was used in universities for hundreds of years and the manuscript copied many times before the invention of the printing press; hundreds of manuscript copies have survived. The first printed edition appeared in 1472 in Ferrara, and at least 84 editions were printed in the next two hundred years. The work was frequently supplemented with commentaries on the original text. The number of copies and commentaries reflects its importance as a university text. [1]

Content

The 'sphere of the world' is not the earth but the heavens, and Sacrobosco quotes Theodosius saying it is a solid body. It is divided into nine parts: the "first moved" ( primum mobile ), the sphere of the fixed stars (the firmament), and the seven planets, Saturn, Jupiter, Mars, the sun, Venus, Mercury and the moon. There is a 'right' sphere and an oblique sphere: the right sphere is only observed by those at the equator (if there are such people), everyone else sees the oblique sphere. There are two movements: one of the heavens from east to west on its axis through the Arctic and Antarctic poles, the other of the inferior spheres at 23° in the opposite direction on their own axes.[ citation needed ]

The world, or universe, is divided into two parts: the elementary and the ethereal. The elementary consists of four parts: the earth, about which is water, then air, then fire, reaching up to the moon. Above this is the ethereal which is immutable and called the 'fifth essence' by the philosophers. All are mobile except heavy earth which is the center of the world.[ citation needed ]

The universe as a machine

Sacrobosco spoke of the universe as the machina mundi, the machine of the world, suggesting that the reported eclipse of the Sun at the crucifixion of Jesus was a disturbance of the order of that machine. This concept is similar to the clockwork universe analogy that became very popular centuries later, during the Enlightenment. [2] :465

Spherical Earth

Picture from a 1550 edition of De sphaera, showing how the curvature of the Earth makes the mast of an approaching ship appear first Sacrobosco-1550-B3r-detail01.jpg
Picture from a 1550 edition of De sphaera, showing how the curvature of the Earth makes the mast of an approaching ship appear first

Though principally about the universe, De sphaera 1230 A.D. contains a clear description of the Earth as a sphere which agrees with widespread opinion in Europe during the higher Middle Ages, in contrast to statements of some 19th- and 20th-century historians that medieval scholars thought the Earth was flat. [3] :19,26–27 As evidence for the Earth being a sphere, in Chapter One he cites the observation that stars rise and set sooner for those in the east ("Orientals"), and lunar eclipses happen earlier; that stars near the North Pole are visible to those further north and those in the south can see different ones; that at sea one can see further by climbing up the mast; and that water seeks its natural shape which is round, as a drop.

See also

Related Research Articles

<i>Almagest</i> Astronomical treatise by Claudius Ptolemy

The Almagest is a 2nd-century mathematical and astronomical treatise on the apparent motions of the stars and planetary paths, written by Claudius Ptolemy in Koine Greek. One of the most influential scientific texts in history, it canonized a geocentric model of the Universe that was accepted for more than 1,200 years from its origin in Hellenistic Alexandria, in the medieval Byzantine and Islamic worlds, and in Western Europe through the Middle Ages and early Renaissance until Copernicus. It is also a key source of information about ancient Greek astronomy.

<span class="mw-page-title-main">History of geodesy</span>

The history of geodesy (/dʒiːˈɒdɪsi/) began during antiquity and ultimately blossomed during the Age of Enlightenment.

Tractatus is Latin for "treatise". It may refer to:

<span class="mw-page-title-main">Celestial spheres</span> Elements of some cosmological models

The celestial spheres, or celestial orbs, were the fundamental entities of the cosmological models developed by Plato, Eudoxus, Aristotle, Ptolemy, Copernicus, and others. In these celestial models, the apparent motions of the fixed stars and planets are accounted for by treating them as embedded in rotating spheres made of an aetherial, transparent fifth element (quintessence), like gems set in orbs. Since it was believed that the fixed stars did not change their positions relative to one another, it was argued that they must be on the surface of a single starry sphere.

<span class="mw-page-title-main">Fixed stars</span> Astronomical bodies that appear not to move relative to each other in the night sky

In astronomy, the fixed stars are the luminary points, mainly stars, that appear not to move relative to one another against the darkness of the night sky in the background. This is in contrast to those lights visible to naked eye, namely planets and comets, that appear to move slowly among those "fixed" stars.

<span class="mw-page-title-main">Johannes de Sacrobosco</span>

Johannes de Sacrobosco, also written Ioannes de Sacro Bosco, later called John of Holywood or John of Holybush, was a scholar, monk, and astronomer who taught at the University of Paris.

<span class="mw-page-title-main">Mashallah ibn Athari</span> 8/9th century Persian Jewish astrologer and astronomer

Māshāʾallāh ibn Atharī, known as Mashallah, was an 8th century Persian Jewish astrologer, astronomer, and mathematician. Originally from Khorasan, he lived in Basra during the reigns of the Abbasid caliphs al-Manṣūr and al-Ma’mūn, and was among those who introduced astrology and astronomy to Baghdad. The bibliographer ibn al-Nadim described Mashallah "as virtuous and in his time a leader in the science of jurisprudence, i.e. the science of judgments of the stars". Mashallah served as a court astrologer for the Abbasid caliphate and wrote works on astrology in Arabic. Some Latin translations survive.

<span class="mw-page-title-main">Lynn Thorndike</span> American historian

Lynn Thorndike was an American historian of medieval science and alchemy. He was the son of a clergyman, Edward R. Thorndike, and the younger brother of Ashley Horace Thorndike, an American educator and expert on William Shakespeare, and Edward Lee Thorndike, known for being the father of modern educational psychology.

<span class="mw-page-title-main">Giuseppe Biancani</span> Italian Jesuit astronomer, mathematician, and selenographer (1566–1624)

Giuseppe Biancani, SJ (1566–1624) was an Italian Jesuit astronomer, mathematician, and selenographer, after whom the crater Blancanus on the Moon is named.

<span class="mw-page-title-main">Clockwork universe</span> Deterministic model of the universe

In the history of science, the clockwork universe compares the universe to a mechanical clock. It continues ticking along, as a perfect machine, with its gears governed by the laws of physics, making every aspect of the machine predictable.

<span class="mw-page-title-main">Ancient Greek astronomy</span> Astronomy as practiced in the Hellenistic world of classical antiquity

Ancient Greek astronomy is the astronomy written in the Greek language during classical antiquity. Greek astronomy is understood to include the Ancient Greek, Hellenistic, Greco-Roman, and late antique eras. It is not limited geographically to Greece or to ethnic Greeks, as the Greek language had become the language of scholarship throughout the Hellenistic world following the conquests of Alexander. This phase of Greek astronomy is also known as Hellenistic astronomy, while the pre-Hellenistic phase is known as Classical Greek astronomy. During the Hellenistic and Roman periods, many of the Greek and non-Greek astronomers working in the Greek tradition studied at the Museum and the Library of Alexandria in Ptolemaic Egypt.

Solomon ben Abraham Abigdor, born in Provence in 1384, was a Hebrew translator, physician, and mystic.

Petrus de Dacia, also called Philomena and Peder Nattergal, was a Danish scholar who lived in the 13th century. He worked mainly in Paris and Italy, writing in Latin. He published a calendar of new moon dates for the years 1292-1367. In 1292, he published a book on mathematics that contained a new method for the calculation of cubic roots. He also described a mechanical instrument to predict solar and lunar eclipses as seen from Paris.

<span class="mw-page-title-main">Erasmus Oswald Schreckenfuchs</span>

Erasmus Oswald Schreckenfuchs (1511–1579) was an Austrian humanist, astronomer and Hebraist.

Francesco Capuano Di Manfredonia was an Italian astronomer, professor, and member of the clergy. Up until the 1880s there wasn't a lot known about Capuano, and the little bit that was known was derived directly from his printed works.

Jacques du Chevreul was a French mathematician, astronomer, and philosopher.

<span class="mw-page-title-main">Pedro Ciruelo</span>

Pedro Sánchez Ciruelo was a Spanish philosopher, theologian, mathematician, astrologer, astronomer and writer on topics of natural philosophy.

André do Avelar also known as "Andre dauellar" was an author and professor who published astronomical works at the University of Coimbra. His works sought to explain astronomy, astrology, and the calendar year to the people of Lisbon. Despite his esteem he would later be sentenced to life in prison by the Inquisition as he was accused of being a Judaizer.

Johannes Paulus Lauratius de Fundis was a medieval astronomer and professor of astrology in Bologna. He is known for several manuscript works including Tractatus reprobationis eorum que scripsit Nicolaus Orrem (1451) and Nova theorica planetarum.

References

  1. Olaf Pedersen, "In Quest of Sacrobosco", Journal for the History of Astronomy, 16 (1985): 175-221. Pedersen identifies 35 printings in Venice, another 35 in Paris, and more in 14 other cities throughout Europe.
  2. Grant, Edward (1974). A Source Book in Medieval Science. Cambridge: Harvard University Press.
  3. Russell, Jeffrey Burton (1991). Inventing the Flat Earth . New York: Praeger. ISBN   0-275-93956-1.

Sources