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gptkbp:instanceOf
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set of physical laws
|
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gptkbp:alsoKnownAs
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gptkb:Newton's_laws_of_motion
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gptkbp:appliesTo
|
macroscopic objects
|
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gptkbp:basisFor
|
gptkb:classical_mechanics
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gptkbp:compatibleWith
|
relativistic speeds
quantum scale
|
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gptkbp:consistsOf
|
gptkb:First_law_of_motion
gptkb:Second_law_of_motion
gptkb:Third_law_of_motion
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gptkbp:field
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gptkb:classical_mechanics
|
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gptkbp:firstLaw
|
An object at rest stays at rest and an object in motion stays in motion unless acted upon by a net external force.
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gptkbp:formedBy
|
gptkb:Isaac_Newton
1687
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|
https://www.w3.org/2000/01/rdf-schema#label
|
Newton's laws
|
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gptkbp:influenced
|
gptkb:astronomy
engineering
physics
|
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gptkbp:language
|
gptkb:Latin
|
|
gptkbp:publishedIn
|
gptkb:Philosophiæ_Naturalis_Principia_Mathematica
|
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gptkbp:secondLaw
|
The acceleration of an object is proportional to the net force acting on it and inversely proportional to its mass (F=ma).
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gptkbp:thirdLaw
|
For every action, there is an equal and opposite reaction.
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gptkbp:bfsParent
|
gptkb:Euler-Lagrange_equation
|
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gptkbp:bfsLayer
|
5
|