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The physics behind satellite motion, elliptical orbits, and the escape speed required to leave earth's gravitational pull. Topics include newton's laws of motion, circular motion, gravitational potential energy, and torque. Students will learn about the relationship between linear and angular velocity, the forces causing rotation, and the significance of mechanical equilibrium.
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What happens to the trajectory of the
projectile when the horizontal
component of the velocity is large?
we need to know about
(1) Newton’s universal law of gravitation,
where the magnitude of the force of gravity
is
(2) circular motion
11 2 2
2
1 2
g
G 6.67x 10 Nm /kg
r
mm
F G
angular displacement:
f i
the good old average linear velocity? Think
back to arc length
av
s r| |.
f i
av
The radial acceleration is directed inward towards
the center of the circle. It’s magnitude is given by
r
v
a
2
r
what happens to a projectile launched with a
large horizontal velocity? Will it start to orbit
the Earth? How large is large?
satellite orbiting the Earth some distance
above the Earth’s surface? What is its speed?
What law do we need to invoke to determine
the satellite speed?
to obtain
g i
.
r
Gm
v
E
E
Dark Matter?
Our galaxy: The
Milky Way
about energy. What is the more general
expression for gravitational potential
energy now that we have a more general
expression for the force of gravity?
GPE mgh.
1 2
equilibrium means that the sum of the
forces on the system is zero and the sum
of the torques on the system is also zero.