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Gravitational Fields
although Earth and the
Moon do not touch,
they still exert forces on
each other
Michael Faraday
developed the idea of a
field to explain “action
at a distance”
a field is defined as a sphere of influence where one object can exert a force on another without direct contact
all masses are surrounded by a gravitational field
the field exerts a force on any other mass placed in the field
direction of the field is
always to the centre of
the object causing the
field
field direction is indicated
by the use of field lines
the field lines indicate the
direction of the force
acting on another mass
placed in the field
Field lines that are far
apart mean the field is
weaker here
The field is radially
inward
near the surface of Earth, the field lines appear to be at right angles to the surface
The parallel field lines means the direction is the same
Equal spaces between the field lines means the magnitude is the same
gravitational fields are vector fields
(magnitude and direction)
the field extends to infinity
The gravitational field vector at any location
in space is found by placing a test mass m at
that point and measuring the force acting on
it.
g
gF
gm
Gravitational
field strength
Units N/kg
(same as m/s2)
gravitational
force acting
on mass in
field
Mass in gravity field
(‘test mass’)
Magnitude of gravitational field strength
g = field strength N/kg at a
point in space
G= Universal Gravitational Constant
m = mass of object causing field
r = distance from centre of object causing the field
2r
Gmg
the value of g depends on the distance from
the centre of the planet and geology (value of
g is higher close to dense rock such as metal
ore deposits)
Astronauts repair the
Hubble move than 300
km above the coast of
Australia
Yellow and red are regions of high g values
Chicxulub
gravity map
Example
Determine the magnitude of the gravitational
field strength on the surface of Mars (mass =
6.37 x 1023 kg, r = 3.43 x 106 m).
Solution
2
211 236.67 10 6.37 10
2
263.43 10
gGm
r
mN kg
kg
m
g
g = 3.61 N/kg
Example
Determine the
acceleration of gravity
900 km above the
surface of Earth.
Solution
3
2
211 246.67 10 5.97 10
2
266.37 10 900 10
Gm
r
mN kg
kg
m
g
g
m
g = 7.53 N/kg
When many masses are present, each mass
contributes its own field to each point in space.
To find the net field strength, use vector algebra
to find the value and direction.
Example
Two 6.9 x 103 kg objects are arranged as shown.
Determine the net gravitational field at point P.
A B
Solution find the field
caused by each
mass
Ignore mass B, the
field caused by A
will not be
influenced by mass
B.
3
11
2
2116.67 10 6.9 10
2
2130
2.723 10 / left
A
Gm
r
mN kg
kg
g
gm
N kg
Ignore mass
A, find the
field caused
by mass B
3
10
2
2116.67 10 6.9 10
2
250
1.8409 10 / left
B
Gm
r
mN kg
kg
g
gm
N kg
Net |g| = 2.1 x 10-10 N/kg left
Tides
Tides rise and fall because the moon's
gravity pulls the water into a tidal bulge which
the earth rotates under.
On the side of the Earth nearest to the moon, the
pull from the Moon is the strongest. It's clearly
stronger than the pull from the Moon at locations
on Earth further away from the Moon
Because the gravitational pull from the Moon is
less at the farthest-from-the-Moon point than it
is at other locations on the surface of the Earth,
the water at this point is literally left behind.
The sun and
the moon can
make tides
much larger
than usual,
depending on
their position
Inertial & Gravitational Mass
Inertial mass measures the inertial resistance
to acceleration of the body when responding to
all types of force.
𝑎 =𝐹𝑛𝑒𝑡𝑚
Inertial & Gravitational Mass
Gravitational mass is determined by the
strength of the gravitational force experienced
by an object when in the gravitational field g.
𝐹𝑔 = 𝑚𝑔
Inertial mass and gravitational mass are equal
AP Example
A plant’s radius is measured from orbit to be
7.01 x 106 m. An ‘away team’ lands and
measures the gravitational field strength to be
10.4 N/kg.
A) determine the mass of the planet
B)
Determine the average density of the planet.
m
V 34
3V r
C)
If the density of the surface material is 2.7,
what conclusions can you make about the
planet?
Practice
P 219: 1, 2
P 220: 1, 2, 3