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Announcements

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Announcements Remember -- Tuesday, Oct. 28th, 9:30 AM Second exam (covering Chapters 9-14 of HRW) Bring the following: 1 equation sheet – PowerPoint PPT presentation

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Title: Announcements


1
  • Announcements
  • Remember -- Tuesday, Oct. 28th, 930 AM Second
    exam (covering Chapters 9-14 of HRW) Bring the
    following
  • 1 equation sheet
  • Calculator
  • Pencil
  • Clear head
  • Note If you have kept up with your HW, you may
    drop your lowest exam grade
  • Today --Thursday, Oct. 23th, 4 PM Physics
    Colloquium by Professor Bernd Schüttler, Dept. of
    Physics, U. Ga will discuss the analysis of
    biological systems in terms of a physical and
    mathematical model
  • Todays lecture review Chapters 9-14, problem
    solving techniques

2
Gravitational forces and energy
m
r
v0
Energy needed to escape Earths gravitational
field, assuming an initial velocity
v0
3
Energy needed to go from one stable circular
orbit to another
R1
R2
4
Energy needed to go from one stable circular
orbit to another -- Example
How much energy is needed to take a satellite of
mass m100kg from the international space station
(R1RE390 km) to its usual orbit (R2RE600 km)?
R1
R2
5
Problem solving skills
Equation Sheet
Math skills
  • Advice
  • Keep basic concepts and equations at the top of
    your head.
  • Practice problem solving and math skills
  • Develop an equation sheet that you can consult.

6
  • Problem solving steps
  • Visualize problem labeling variables
  • Determine which basic physical principle applies
  • Write down the appropriate equations using the
    variables defined in step 1.
  • Check whether you have the correct amount of
    information to solve the problem (same number of
    knowns and unknowns.
  • Solve the equations.
  • Check whether your answer makes sense (units,
    order of magnitude, etc.).

7
Center
of mass
ri
rj
8
Position of the center of mass
Velocity of the center of mass
Acceleration of the center of mass
9
Physics of composite systems
Center-of-mass velocity Note that
10
A new way to look at Newtons second law
Define linear momentum p mv
  • Consequences
  • If F 0 ? ? p
    constant
  • For system of particles

11
Statement of conservation of momentum
If mechanical (kinetic) energy is conserved, then
12
Snapshot of a collision
Pi
Impulse
Pf
13
Angular motion
angular displacement ? q(t) angular velocity
? angular acceleration ?
s
natural unit 1 radian Relation to linear
variables sq r (qf-qi) vq r w
aq r a
14
r1
v1r1w
w
r2
v2r2w
Special case of constant angular acceleration a
a0 w(t) wi a0 t q(t) qi
wi t ½ a0 t2 ( w(t))2 wi2 2 a0
(q(t) - qi )
15
Newtons second law applied to center-of-mass
motion
Newtons second law applied to rotational motion
ri
mi
di
Fi
16
Object rotating with constant angular velocity (a
0)
w
R
vRw
v0
Kinetic energy associated with rotation

moment of inertia
17
Kinetic energy associated with rolling without
slipping
Distance to axis of rotation
Rolling
18
Torque and angular momentum Define angular
momentum For composite object
L Iw
Newtons law for torque
? If ttotal 0 then L constant
In the absence of a net torque on a system,
angular momentum is conserved.
19
Center-of-mass
Torque on an extended object due to gravity (near
surface of the earth) is the same as the torque
on a point mass M located at the center of mass.
mi
ri
rCM
20
Notion of equilibrium
Notion of stability
T- mg cos q 0 -mg sin q -maq
Fma ?
r
q
T
tI a ?
r mg sin q mr2 a mraq
Example of stable equilibrium.
mg(-j)
21
Analysis of stability
22
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