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  1. 26 de jun. de 2016 · Muy poco tiempo después de la distribución del «Commentariolus», Martín Lutero, un teólogo y fraile agustino, clavó en la puerta de la iglesia del palacio de Wittenberg sus 95 tesis contra ...

  2. De revolutionibus orbium coelestium escuchar ⓘ ( Sobre las revoluciones de las orbes celestes) es la obra fundamental del astrónomo Nicolás Copérnico, donde expone su teoría heliocéntrica. Comenzó a escribirla en 1506, terminándola en 1531, aunque no se publicó hasta el año de su muerte, en 1543, dedicándola al papa Paulo III .

  3. In the Commentariolus (Little Commentary), Nicolaus Copernicus outlined his revolutionary Copernican heliocentrism theory of the solar system, about three decades before he finally published his major six volume work De revolutionibus orbium coelestium in 1543. Copernicus did not publish the Commentariolus, and handed it only to few friends.

  4. The writings of Copernicus were unavailable in English until the publication of this 1939 translation from the original Latin. A three-part collection, it consists of the Commentariolus, Copernicus' sketch of his hypotheses for the heavenly motions; the Narratio prima, a popular introduction to Copernican theory; and the Letter against Werner, Copernicus' refutation of the views of a contemporary.

  5. 20 de dic. de 2022 · Commentariolus contains the fundamental axiom of ancient astronomy, which underlies all the other assumptions, namely, all motions of celestial bodies must be uniform and circular. This could well serve as a foundational axiom in Copernicus’s composition, and it is also coherent with his vision of a whole and integral universe (Goddu 2009 ).

  6. Commentariolus' use of Epitome, 111,2, and V, 22, is evident. So is Commentariolus' use of Giorgio Valla's Seek and Avoid as well as of Pliny's Natural History. What other sources were tapped by Commentariolus will have to be determined by further research. Copernicus sent out a few copies of Commentariolus, as we saw above.

  7. In the Commentariolus, Copernicus postulated that, if the Sun is assumed to be at rest and if Earth is assumed to be in motion, then the remaining planets fall into an orderly relationship whereby their sidereal periods increase from the Sun as follows: Mercury (88 days), Venus (225 days), Earth (1 year), Mars (1.9 years), Jupiter (12 years), and Saturn (30 years).