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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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
surface form: 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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