Unit 7 · Topic 01
Universal gravitation
Newtonian gravitation is a mutual, attractive, vector interaction of unlimited range.
Unit 7Universal gravitationOpen navigation
Concept 01
A mutual force
Essential The minimum you should retain
Two point masses attract with equal magnitudes |F|=Gm₁m₂/r² and opposite directions along their center line.
UnderstandInterpret and connect
Doubling r reduces the magnitude to F/4; accelerations may differ although the forces do not.
DeepenFormulation and conditions
The vector form on m due to M is F=−GMm/r² r_hat: the sign expresses attraction.
ExploreConnections for further study
The small value of G makes the interaction between many everyday objects imperceptible.
Worked example
Attraction between two masses
Masses of 1000 kg and 1500 kg are 2.0 m apart; G=6.674×10^-11 N·m²/kg².
- m₁=1000 kg
- m₂=1500 kg
- r=2.0 m
Find |F|.
- Model
.
- Substitution
F=(6.674×10^-11)(1000)(1500)/(2.0)².
- Result
F=2.50×10^-5 N.
- Direction
Each force points toward the other mass.
Mathematical relation
Universal gravitation
Mutual attractive gravitational force.
Direction is toward the source and magnitude falls as 1/r².
DeepenVariables, conditions, and checks
Variables
- G
- gravitational constant; usual unit: N·m²/kg²
- r
- center-to-center distance; usual unit: m
Conditions of application
- Point masses or spherical bodies in the appropriate exterior region; r>0.
Dimensional check
N.
The pair forces have equal magnitude and opposite directions; doubling r reduces F to F₀/4.
Concept 02
Equal magnitude, different acceleration
Essential The minimum you should retain
Each body exerts a gravitational force of equal magnitude and opposite direction on the other.
UnderstandInterpret and connect
The larger mass usually accelerates less because a=F/m, not because it receives less force.
DeepenFormulation and conditions
The pair acts on different bodies and does not cancel when analyzing either body alone.
ExploreConnections for further study
Linear-momentum conservation of the system is consistent with this internal pair.
Concept 03
Adding contributions
Essential The minimum you should retain
The effect of several masses is the vector sum of their forces or fields.
UnderstandInterpret and connect
Contributions in different directions must not be added as magnitudes.
DeepenFormulation and conditions
Each vector uses its own distance and direction before being resolved into components.
ExploreConnections for further study
Zero-field points can arise by cancellation even though every contribution is nonzero.
Each contribution is calculated with its own direction, and the resultant is a vector sum.
Concept 04
When the point-mass model works
Essential The minimum you should retain
Outside a spherically symmetric distribution, the field equals that of a central point mass.
UnderstandInterpret and connect
The equivalence depends on symmetry and on being in the exterior region.
DeepenFormulation and conditions
It cannot be extended to arbitrary distributions without integrating their density.
ExploreConnections for further study
Newton's law is highly accurate in its regime but is not the fundamental theory of spacetime.
Concept review
Common errors
Each warning includes a concrete way to review the reasoning, not only an incorrect-answer marker.
Believing the larger body exerts a larger gravitational force on the smaller one.
Force magnitudes are equal; accelerations differ because masses differ.
Doubling r and halving F.
F∝1/r², so doubling r divides F by four.