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Gravitational Fields & Circular Motion, Lecture notes of Physics

ALevel Physics Cambridge resources Gravitational Fields & Circular Motion

Typology: Lecture notes

2024/2025

Available from 07/07/2025

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Gravitational Field  Region around a mass where gravitational forces are experienced
Gravitational Field Strength  Force per unit mass, (g) → (acceleration)
Equipotential lines : all horizontal lines have the same G.P. (
ϕ
)
F
=
w
=
mg
g
=
w
m
[constant]
Measured in
ms
2
Gravitational Potential Energy
G
.
P
.
E
. =
mgh
Gravitational Constant
(
G
) = 6.67 × 1011
F
=
GmM
r
2
m
 Mass of object 1
M
 Mass of object 2
r
 Distance between the 2 masses
Gravitational Field Strength
w
=
mg
g
=
GM
r
2
Gravitational Potential G.P.) (
ϕ
)  Gravitational Potential Energy G.P.E per unit mass
work
=
F
×
distance
Gravitational Fields & Circular Motion
Gravitational Fields
Uniform Fields
Force
Gravitational Field Strength
Radial Fields
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Gravitational Field Region around a mass where gravitational forces are experienced

Gravitational Field Strength Force per unit mass, (g) → (acceleration)

Equipotential lines : all horizontal lines have the same G.P. (ϕ)

F = w = mg

g = (^) mw [constant]

Measured in ms− Gravitational Potential Energy

G. P. E. = mgh

Gravitational Constant (G) = 6.67 × 10−

F = G

mM

r^2

m Mass of object 1 M Mass of object 2 r Distance between the 2 masses

Gravitational Field Strength

w = mg

g = G

M

r^2

Gravitational Potential G.P.) ( ϕ ) Gravitational Potential Energy G.P.E per unit mass work = F × distance

Gravitational Fields & Circular Motion

Gravitational Fields

Uniform Fields

Force

Gravitational Field Strength

Radial Fields

G. P. E = −G

M

r

d dx (Graviational P otential) =^ Gravitational F ield Strength d dx (−G^ M r ) =^ G^ M r^2

 At ∞ G.P.E. is 0  Work is being done on the mass by the field  The force is Attraction Force reducing the distance between the 2 masses Note : as you approach infinity the G.P.E. becomes more positive

Radian : angle subtended between 2 radii where the length of the arc equals the radius

Objects in circular motion have constant speed but changing velocity Objects in circular motion are not at equilibrium, they are affected by a net centripetal force

Displacement (S)

S = θr

θ Angle in radians

Angular Velocity / Frequency ( ω )

t

or ω =

T

T Periodic Time

Velocity (v)

v = ωr

Acceleration (a)

a =

v^2

r

or ω²r

Force (F)

F =

mv^2

r

or mω²r

F = G mMr 2 mv r 2 = G mM r^2

v = √^ GMr

Note The orbiting velocity is independent of the mass of the satallite

Polar satellites

conditions rotates around the poles period time between 90 and 105

Why is G.P.E always negative

Circular Motion

Orbits

Orbiting Speed