A 100 m 2 solar plane is couple to a flywheel such that it converts incident sunlight into mechanical energy of rotation with 1% efficiency.
Text Solution
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Sol. The kinetic energy of rotation of the flywheel is E =
I ω 2 2 , where I =
mR 2 , giving
ω 0 =
= 
= 1136 rad/s. Ans.
Measure time from the instant the flywheel is released, when it is rotating with angular velocity ω 0 . After its released the only horizontal force on the flywheel is the frictional force as shown in fig. The equations of motion are

I
= – fR, m
= f
At time t 1 when the flywheel stops slipping, let its angular velocity be ω 1 . The boundary conditions are ω = ω 0 , v = 0 at t = 0, ω = ω 1 , v = v 1 = R ω 1 at t = t 1 . The above equations integrate to give
I ( ω 1 – ω 0 ) = –fRt 1
mv = mR ω 1 = ft 1
Note that these equations can also be obtained directly by an impulse consideration. Solving these we have
ω 1 =
, t 1 =
,
as I =
mR 2 , f = µmg. The distance covered by the flywheel before it stops slipping is
S =
t 1 2 =
µg
= 
= 18290 m. Ans.
At t 1 the speed of the center of mass is
v 1 = R ω 1 =
= 189.3 ms –1 . Ans.
At time 0 < t < t 1 , the equation of motion integrates to
I ( ω – ω 0 ) = –f Rt.
mv = ft.
At 0 < t < t 1 , the flywheel both slips and rolls. Only the slipping part of the motion casues dissipation of energy into heat. The slipping velocity is
v – R ω =
– R ω 0
and the total dissipation of energy into heat is
Q = – 
=
+ R ω 0 f t 1
=
= 2.688 × 10 7 J.
This can also be obtained by considering the change in the kinetic energy of the flywheel:
Q = I ω 0 2 – 
=
.
–
=
,
Same as the above.
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