Book VI

E112013

Book VI is the concluding section of Nicolaus Copernicus’s seminal astronomical work *De revolutionibus orbium coelestium*, in which he further develops and applies his heliocentric model.

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Book VI canonical 1

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Statements (40)

Predicate Object
instanceOf book section ⓘ
aimsTo enable astronomers to compute planetary positions using heliocentrism ⓘ
show the adequacy of the heliocentric model for predictive astronomy ⓘ
author Nicolaus Copernicus ⓘ
contains mathematical derivations ⓘ
tables of planetary motion ⓘ
worked numerical examples ⓘ
field astronomy ⓘ
mathematical astronomy ⓘ
focusesOn application of the heliocentric system ⓘ
construction of astronomical tables based on heliocentrism ⓘ
numerical methods for predicting planetary motion ⓘ
practical computation of planetary positions ⓘ
refinement of planetary models introduced in earlier books ⓘ
historicalPeriod Renaissance ⓘ
influenced early modern astronomical practice ⓘ
later planetary tables by early modern astronomers ⓘ
influencedBy Ptolemaic astronomical tradition ⓘ
medieval mathematical astronomy ⓘ
language Latin ⓘ
mainTopic astronomical tables ⓘ
computational procedures in astronomy ⓘ
heliocentric model ⓘ
planetary latitudes ⓘ
planetary longitudes ⓘ
planetary positions ⓘ
planetary theory ⓘ
partOf De revolutionibus orbium coelestium ⓘ
positionInWork final book ⓘ
sixth book ⓘ
publicationYear 1543 ⓘ
publishedIn Nuremberg ⓘ
relatedTo Book V (De revolutionibus orbium coelestium) ⓘ
significance demonstrates practical astronomical use of the heliocentric system ⓘ
provides computational foundation for Copernicus’s heliocentric theory ⓘ
usesModel Sun-centered cosmos ⓘ
circular planetary orbits ⓘ
epicycles and deferents ⓘ
uniform circular motion ⓘ
workType scholarly treatise section ⓘ

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