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gptkbp:instanceOf
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physical phenomenon
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gptkbp:alsoKnownAs
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gptkb:Newton's_law_of_universal_gravitation
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gptkbp:appliesTo
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macroscopic objects
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gptkbp:assumes
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instantaneous action at a distance
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gptkbp:category
|
classical physics
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gptkbp:describes
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gravitational attraction between masses
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gptkbp:form
|
F = G * (m1 * m2) / r^2
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gptkbp:formedBy
|
gptkb:Isaac_Newton
1687
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|
https://www.w3.org/2000/01/rdf-schema#label
|
Newtonian gravity
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gptkbp:influenced
|
gptkb:classical_mechanics
celestial mechanics
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gptkbp:involvesConstant
|
gravitational constant
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gptkbp:limitation
|
does not account for relativistic effects
inaccurate at very high velocities
inaccurate for very strong gravitational fields
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gptkbp:precededBy
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gptkb:Aristotelian_physics
|
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gptkbp:publishedIn
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gptkb:Philosophiæ_Naturalis_Principia_Mathematica
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gptkbp:replacedBy
|
gptkb:general_relativity
|
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gptkbp:usedFor
|
calculating satellite orbits
predicting planetary motion
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gptkbp:bfsParent
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gptkb:General_Theory_of_Relativity
gptkb:general_relativity
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gptkbp:bfsLayer
|
4
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