Faster access than browser!Similarities between Cosmology and Deferent and epicycle
Cosmology and Deferent and epicycle have 17 things in common (in Unionpedia): Almagest, Aristarchus of Samos, Aristotle, Astronomy, De revolutionibus orbium coelestium, Equant, Galileo Galilei, Geocentric model, Heliocentrism, Isaac Newton, Johannes Kepler, Kepler's laws of planetary motion, Moon, Newton's law of universal gravitation, Nicolaus Copernicus, Planet, Ptolemy.
Almagest
The Almagest is a 2nd-century Greek-language mathematical and astronomical treatise on the apparent motions of the stars and planetary paths, written by Claudius Ptolemy. One of the most influential scientific texts of all time, its geocentric model was accepted for more than 1200 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.
Almagest and Cosmology · Almagest and Deferent and epicycle ·
Aristarchus of Samos
Aristarchus of Samos (Ἀρίσταρχος ὁ Σάμιος, Aristarkhos ho Samios; c. 310 – c. 230 BC) was an ancient Greek astronomer and mathematician who presented the first known model that placed the Sun at the center of the known universe with the Earth revolving around it (see Solar system).
Aristarchus of Samos and Cosmology · Aristarchus of Samos and Deferent and epicycle ·
Aristotle
Aristotle (Ἀριστοτέλης Aristotélēs,; 384–322 BC) was an ancient Greek philosopher and scientist born in the city of Stagira, Chalkidiki, in the north of Classical Greece.
Aristotle and Cosmology · Aristotle and Deferent and epicycle ·
Astronomy
Astronomy (from ἀστρονομία) is a natural science that studies celestial objects and phenomena.
Astronomy and Cosmology · Astronomy and Deferent and epicycle ·
De revolutionibus orbium coelestium
De revolutionibus orbium coelestium (On the Revolutions of the Heavenly Spheres) is the seminal work on the heliocentric theory of the Renaissance astronomer Nicolaus Copernicus (1473–1543).
Cosmology and De revolutionibus orbium coelestium · De revolutionibus orbium coelestium and Deferent and epicycle ·
Equant
Equant (or punctum aequans) is a mathematical concept developed by Claudius Ptolemy in the 2nd century AD to account for the observed motion of the planets.
Cosmology and Equant · Deferent and epicycle and Equant ·
Galileo Galilei
Galileo Galilei (15 February 1564Drake (1978, p. 1). The date of Galileo's birth is given according to the Julian calendar, which was then in force throughout Christendom. In 1582 it was replaced in Italy and several other Catholic countries with the Gregorian calendar. Unless otherwise indicated, dates in this article are given according to the Gregorian calendar. – 8 January 1642) was an Italian polymath.
Cosmology and Galileo Galilei · Deferent and epicycle and Galileo Galilei ·
Geocentric model
In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a superseded description of the universe with Earth at the center.
Cosmology and Geocentric model · Deferent and epicycle and Geocentric model ·
Heliocentrism
Heliocentrism is the astronomical model in which the Earth and planets revolve around the Sun at the center of the Solar System.
Cosmology and Heliocentrism · Deferent and epicycle and Heliocentrism ·
Isaac Newton
Sir Isaac Newton (25 December 1642 – 20 March 1726/27) was an English mathematician, astronomer, theologian, author and physicist (described in his own day as a "natural philosopher") who is widely recognised as one of the most influential scientists of all time, and a key figure in the scientific revolution.
Cosmology and Isaac Newton · Deferent and epicycle and Isaac Newton ·
Johannes Kepler
Johannes Kepler (December 27, 1571 – November 15, 1630) was a German mathematician, astronomer, and astrologer.
Cosmology and Johannes Kepler · Deferent and epicycle and Johannes Kepler ·
Kepler's laws of planetary motion
In astronomy, Kepler's laws of planetary motion are three scientific laws describing the motion of planets around the Sun.
Cosmology and Kepler's laws of planetary motion · Deferent and epicycle and Kepler's laws of planetary motion ·
Moon
The Moon is an astronomical body that orbits planet Earth and is Earth's only permanent natural satellite.
Cosmology and Moon · Deferent and epicycle and Moon ·
Newton's law of universal gravitation
Newton's law of universal gravitation states that a particle attracts every other particle in the universe with a force which is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.
Cosmology and Newton's law of universal gravitation · Deferent and epicycle and Newton's law of universal gravitation ·
Nicolaus Copernicus
Nicolaus Copernicus (Mikołaj Kopernik; Nikolaus Kopernikus; Niklas Koppernigk; 19 February 1473 – 24 May 1543) was a Renaissance-era mathematician and astronomer who formulated a model of the universe that placed the Sun rather than the Earth at the center of the universe, likely independently of Aristarchus of Samos, who had formulated such a model some eighteen centuries earlier.
Cosmology and Nicolaus Copernicus · Deferent and epicycle and Nicolaus Copernicus ·
Planet
A planet is an astronomical body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.
Cosmology and Planet · Deferent and epicycle and Planet ·
Ptolemy
Claudius Ptolemy (Κλαύδιος Πτολεμαῖος, Klaúdios Ptolemaîos; Claudius Ptolemaeus) was a Greco-Roman mathematician, astronomer, geographer, astrologer, and poet of a single epigram in the Greek Anthology.
The list above answers the following questions
- What Cosmology and Deferent and epicycle have in common
- What are the similarities between Cosmology and Deferent and epicycle
Cosmology and Deferent and epicycle Comparison
Cosmology has 249 relations, while Deferent and epicycle has 82. As they have in common 17, the Jaccard index is 5.14% = 17 / (249 + 82).
References
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