gptkbp:instanceOf
|
physical phenomenon
|
gptkbp:alsoKnownAs
|
gptkb:law_of_universal_gravitation
|
gptkbp:appliesTo
|
all objects with mass
|
gptkbp:category
|
classical physics
|
gptkbp:constantInEquation
|
gravitational constant (G)
|
gptkbp:describes
|
gravitational attraction between masses
|
gptkbp:domain
|
physics
|
gptkbp:form
|
F = G * (m1 * m2) / r^2
|
gptkbp:formedBy
|
gptkb:Isaac_Newton
1687
|
https://www.w3.org/2000/01/rdf-schema#label
|
Newton's law of gravity
|
gptkbp:influenced
|
gptkb:classical_mechanics
gptkb:Einstein's_theory_of_general_relativity
|
gptkbp:influencedBy
|
gptkb:Kepler's_laws_of_planetary_motion
|
gptkbp:limitation
|
does not account for relativistic effects
not accurate at very high masses or speeds
|
gptkbp:publishedIn
|
gptkb:PhilosophiƦ_Naturalis_Principia_Mathematica
|
gptkbp:relatedConcept
|
gravitational field
inverse-square law
gravitational potential energy
|
gptkbp:replacedBy
|
general relativity (in strong gravitational fields)
|
gptkbp:unitOfForce
|
newton (N)
|
gptkbp:usedFor
|
calculating planetary orbits
engineering satellite trajectories
predicting motion of celestial bodies
|
gptkbp:bfsParent
|
gptkb:Gravity_model_of_trade
|
gptkbp:bfsLayer
|
8
|