Conservation of rotational energy

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SUMMARY

The discussion focuses on the conservation of rotational energy in a cylindrical can of paint rolling down a roof. The correct distance from the edge of the house where the can lands is 6.18 meters, derived from the energy conservation equation mgH = (1/2)MV_cm^2(1+B). The user attempted to solve for the distance using kinematic equations but arrived at incorrect values of 41.8 meters and 26.0 meters. The key error lies in the application of energy conservation principles and the correct interpretation of the variables involved.

PREREQUISITES
  • Understanding of rotational dynamics, specifically the moment of inertia (I = 0.5MR^2).
  • Familiarity with energy conservation principles in physics.
  • Knowledge of kinematic equations for projectile motion.
  • Basic trigonometry for resolving components of motion (e.g., cos(30°), sin(30°)).
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  • Review the principles of conservation of energy in rotational motion.
  • Learn how to derive the equations of motion for rolling objects.
  • Study the application of kinematic equations in projectile motion scenarios.
  • Explore the effects of different angles on the trajectory of rolling objects.
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Students and educators in physics, particularly those studying rotational dynamics and energy conservation, as well as engineers involved in mechanics and motion analysis.

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A cylindrical can of paint with (I = .5MR^2) starts from rest and rolls down a roof as shown in the link
http://viewmorepics.myspace.com/index.cfm?fuseaction=viewImage&friendID=128765607&imageID=1424481748

Determine how far the can lands from the edge of the house.
This is my work, but I am not getting the correct answer. Please tell me where I messed up. The correct answer is 6.18m

mgH = (1/2)MV_cm^2 (1+B)
gH = (1/2)V_cm^2 (1+B)
3g = (1/2)V_cm^2(1+.5)
3g = (3/4)v_cm^2
4g = v_cm^2
v = 2SQRT(g)

Now, I know that x = x_0 + v_o*cos(theta)*t

x = 2SQRT(g)*cos(30)*t

To solve for t, I used y

y = 10 - 2SQRT(g)*sin(30)*t - (1/2)gt^2
0 = 20 - 4SQRT(g)*sin(30)*t - gt^2
0 = gt^2 + 2SQRT(g)*t - 20

t = 2SQRT(g) +/- SQRT[4g-4(g)(-20)]/2g
t = 7.72 seconds or 4.79

x = 2SQRT(g)*cos(30)*7.72
x = 41.8

x = 2SQRt(g)*cos(30)*4.79
x = 26.0

The correct answer is 6.18. My answer is too far off, but I don't know where I went wrong.
 
Last edited:
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I'm not sure what your initial equation is meant to represent, but note that total energy must be conserved. i.e,

gravitational potential = rotational kinetic energy + linear kinetic energy
 

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