Book III

E115609

Book III is the final section of Newton’s *Philosophiæ Naturalis Principia Mathematica*, in which he applies his laws of motion and universal gravitation to explain the motions of celestial bodies and the structure of the solar system.

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Label Occurrences
Book III canonical 1

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Statements (47)

Predicate Object
instanceOf book section ⓘ
appliesTo comets ⓘ
moons ⓘ
planets ⓘ
the Sun ⓘ
author Isaac Newton ⓘ
basedOn results of Book I (Principia) ⓘ
results of Book II (Principia) ⓘ
centralConcept inverse-square law of attraction ⓘ
universal gravitation ⓘ
contains Rules of Reasoning in Philosophy ⓘ
demonstrates Sun-centered planetary system ⓘ
gravitational attraction between all masses ⓘ
discipline astronomy ⓘ
natural philosophy ⓘ
physics ⓘ
explains Kepler's laws of planetary motion ⓘ
cometary orbits ⓘ
elliptical planetary orbits ⓘ
irregularities in planetary motions ⓘ
motion of the Moon ⓘ
precession of the equinoxes ⓘ
stability of the solar system ⓘ
tides ⓘ
focusesOn application of laws of motion ⓘ
application of universal gravitation ⓘ
motions of celestial bodies ⓘ
structure of the solar system ⓘ
genre mathematical physics ⓘ
hasAlternativeName System of the World ⓘ
hasTopic empirical tests of gravitational theory ⓘ
gravitational explanation of planetary motions ⓘ
mass distribution in the solar system ⓘ
historicalPeriod Scientific Revolution ⓘ
influenced 18th-century astronomy ⓘ
development of celestial mechanics ⓘ
subsequent theories of the solar system ⓘ
language Latin ⓘ
partOf Philosophiæ Naturalis Principia Mathematica ⓘ
positionInWork final book ⓘ
third book ⓘ
publicationContext first published with Principia in 1687 ⓘ
subjectOf celestial mechanics ⓘ
supportsTheory heliocentrism ⓘ
usesTheory Newtonian mechanics ⓘ
law of universal gravitation ⓘ
workType scientific treatise section ⓘ

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Full triples — surface form annotated when it differs from this entity's canonical label.