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Unit 8: Space Physics (Physics Only)
8.2 Orbital Motion, Natural and Artificial Satellites
8.2.1 Circular Orbits
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What are the two main types of orbital motion?
Circular and elliptical
The gravitational force between two objects is given by
F
=
F =
F
=
G
m
1
m
2
r
2
G \frac{m_{1} m_{2}}{r^{2}}
G
r
2
m
1
m
2
, where
r
r
r
is the distance between their centers
Orbital motion is primarily due to
gravitational
attraction.
Match the type of orbit with its characteristic:
Circular ↔️ Constant speed and distance
Elliptical ↔️ Varying speed and distance
In a circular orbit, the gravitational force provides the
centripetal
force needed to keep the object moving in a circle.
In a circular
orbit
, the object's speed is constant.
What is an example of an object in a circular orbit?
Artificial satellites
The equation
G
m
1
m
2
r
2
=
\frac{G m_{1} m_{2}}{r^{2}} =
r
2
G
m
1
m
2
=
m
v
2
r
\frac{m v^{2}}{r}
r
m
v
2
shows the balance between gravitational and centripetal forces in a circular orbit.
In a circular orbit, the object's distance from the
central
object remains constant.
What is an example of a circular orbit in our solar system?
Artificial satellites around Earth
The orbital speed
v
v
v
in a circular orbit can be calculated using the equation
v
=
v =
v
=
G
m
1
r
\sqrt{\frac{G m_{1}}{r}}
r
G
m
1
, where
r
r
r
is the radius
What equation shows the relationship between orbital speed and radius?
G
m
1
m
2
r
2
=
\frac{G m_{1} m_{2}}{r^{2}} =
r
2
G
m
1
m
2
=
m
v
2
r
\frac{m v^{2}}{r}
r
m
v
2
The equation \frac{G m_{1} m_{2}}{r^{2}} = \frac{m v^{2}}{r}</latex> can be simplified to show the relationship between orbital speed and
radius
Rearranging the equation
G
m
1
m
2
r
2
=
\frac{G m_{1} m_{2}}{r^{2}} =
r
2
G
m
1
m
2
=
m
v
2
r
\frac{m v^{2}}{r}
r
m
v
2
for v results in
v
=
v =
v
=
G
m
1
r
\sqrt{\frac{G m_{1}}{r}}
r
G
m
1
.
What is the relationship between orbital speed and radius according to the equation
v
=
v =
v
=
G
m
1
r
\sqrt{\frac{G m_{1}}{r}}
r
G
m
1
?
Inversely proportional
For satellites around Earth, as the orbital radius increases, their speed
decreases
What are the two main types of orbits?
Circular and elliptical
A circular orbit maintains a constant speed and distance from the
central
object.
Orbital motion is caused by mutual gravitational
attraction
What law governs gravitational force?
Universal Gravitation
In a circular orbit, gravitational force and
centripetal
force are balanced.
As the orbital radius increases, what happens to the orbital speed?
Decreases
In a circular orbit, gravitational force provides the necessary
centripetal
force.
The balance between gravitational and centripetal forces in a circular orbit can be represented by the equation
G
m
1
m
2
r
2
=
G \frac{m_{1} m_{2}}{r^{2}} =
G
r
2
m
1
m
2
=
m
v
2
r
\frac{mv^{2}}{r}
r
m
v
2
.
What is the equation for centripetal force?
F
c
=
F_{c} =
F
c
=
m
v
2
r
\frac{mv^{2}}{r}
r
m
v
2
In a circular orbit, gravitational force provides the necessary
centripetal
force.
What is the equation for gravitational force?
F
=
F =
F
=
G
m
1
m
2
r
2
G \frac{m_{1} m_{2}}{r^{2}}
G
r
2
m
1
m
2
The balance between gravitational force and centripetal force in a circular orbit is represented by the equation
G
m
1
m
2
r
2
\frac{G m_{1} m_{2}}{r^{2}}
r
2
G
m
1
m
2
What is the equation for the balance between gravitational force and centripetal force?
G
m
1
m
2
r
2
=
\frac{G m_{1} m_{2}}{r^{2}} =
r
2
G
m
1
m
2
=
m
v
2
r
\frac{mv^{2}}{r}
r
m
v
2
A circular orbit is maintained by a balance between gravitational and
centripetal forces
.
What is the gravitational constant denoted by?
G
G
G
What two forces maintain a circular orbit?
Gravitational and centripetal
A circular orbit requires a precise balance between gravitational and
centripetal
forces.
The gravitational force is given by
F
=
F =
F
=
G
m
1
m
2
r
2
G \frac{m_{1} m_{2}}{r^{2}}
G
r
2
m
1
m
2
, where
G
G
G
is the gravitational constant
What do
m
1
m_{1}
m
1
and
m
2
m_{2}
m
2
represent in the gravitational force equation?
Masses of the objects
What does
r
r
r
represent in the gravitational force equation?
Distance between centers
The centripetal force is given by
F
c
=
F_{c} =
F
c
=
m
v
2
r
\frac{mv^{2}}{r}
r
m
v
2
, where
m
m
m
is the mass of the satellite
What does
v
v
v
represent in the centripetal force equation?
Orbital speed
What does
r
r
r
represent in the centripetal force equation?
Orbital radius
For a circular orbit to be stable, the gravitational force must equal the
centripetal
force.
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