Rotational Dynamics
Student Name
θ
1
(rad)
θ
2
(rad)
r
pulley
(m)
m
hang.
(kg)
t
1
(s)
t
2
(s)
α
(rad/s
2
)
ω
0
(rad/s)
The default angular positions may be reset if necessary.
Credits
Authored by Kevork Spartalian, University of Vermont.