Circular motion, friction and forces

AI Thread Summary
The discussion revolves around understanding the forces acting on a cylinder in circular motion, particularly the role of friction as the centripetal force. Participants emphasize the importance of drawing a diagram to visualize the forces and calculating the maximum frictional force using the formula F = μN. The conversation also covers how to derive radial acceleration and its relationship with velocity and radius, leading to a calculation for the maximum distance the cylinder can be from the center without falling off. Clarifications are made regarding the use of variables and units in calculations, ensuring a better understanding of the physics involved. Overall, the thread provides insights into applying theoretical concepts to practical problems in circular motion.
hankrinsen
Messages
7
Reaction score
1
Homework Statement
A sylinder with a mass of 5kg is placed on a distance R from the rotation centre of a carousel. The carousel uses 2 seconds on one round. How far away from the centre can we place the sylinder without it falling of, given a friction number of 0.7 (maximum).
Relevant Equations
friction = μ*n
I am not really sure how to go about this. I have been sick for a couple of weeks and fallen behind a bit. Can anyone help me out please? Thank you
 
Physics news on Phys.org
Hi @hankrinsen, sorry to hear about that! Hope you're better now, and

:welcome:

Have you tried drawing a diagram of the setup?
 
1587294508169.png

This is attached to the assignment. English is my second language, so i might have misunderstood what you mean by diagram
 
  • Like
Likes etotheipi
That's a good start; what forces are acting on the cylinder, and what are their magnitudes and directions? It is good practice to draw all the forces onto the diagram.
 
I have found that the sum of forces must be facing inwards towards the circle, And I have come to the conclusion that the friction is the centripetal force in this instance. The friction force should be the only force working here. Therefore I am confused as to how i calculate when the cylinder will fall of. Friction force should be 0.7*9.81*5 = 34.335N
 
I think height of the cylinder is also matter
 
wrobel said:
I think height of the cylinder is also matter
How? The height is not given
 
hankrinsen said:
I have found that the sum of forces must be facing inwards towards the circle, And I have come to the conclusion that the friction is the centripetal force in this instance. The friction force should be the only force working here. Therefore I am confused as to how i calculate when the cylinder will fall of. Friction force should be 0.7*9.81*5 = 34.335N

That's right, friction provides the centripetal force. The formula ##F = \mu N## you've given corresponds to the maximum possible frictional force (more generally we might say ##F \leq \mu N##).

So you've calculated the maximum centripetal force, and that must correspond to your highest possible radial acceleration. Since the angular velocity is fixed, that naturally corresponds to the highest possible radius.

What is the formula for radial acceleration for circular motion, and then can you apply ##F_r = ma_r##?
 
hankrinsen said:
How? The height is not given
the cylinder can topple over
 
  • #10
etotheipi said:
That's right, friction provides the centripetal force. The formula ##F = \mu N## you've given corresponds to the maximum possible frictional force (more generally we might say ##F \leq \mu N##).

So you've calculated the maximum centripetal force, and that must correspond to your highest possible radial acceleration. Since the angular velocity is fixed, that naturally corresponds to the highest possible radius.

What is the formula for radial acceleration for circular motion, and then can you apply ##F_r = ma_r##?
So this means the highest possible radial acceleration must be 6.867 m/s^2.
The radial acceleration --> A=v^2/r ---> 6.367=v^2/r

To find velocity i find the circumference of one rotation and divide it by time. It takes 2 seconds to finish one rotation with a circumference of 2*pi*r, so the velocity is pi*r

I put it in the equation for max radial acceleration; 6.367 = ((pi*r)^2)/r ---> 6.367 = pi^2*r --> r = 6.367/pi^2

Which gives me that it can be put a maximum og 0.645r from the center without falling off? I might be way off here...
 
  • #11
hankrinsen said:
So this means the highest possible radial acceleration must be 6.867 m/s^2.
The radial acceleration --> A=v^2/r ---> 6.367=v^2/r

To find velocity i find the circumference of one rotation and divide it by time. It takes 2 seconds to finish one rotation with a circumference of 2*pi*r, so the velocity is pi*r

I put it in the equation for max radial acceleration; 6.367 = ((pi*r)^2)/r ---> 6.367 = pi^2*r --> r = 6.367/pi^2

Which gives me that it can be put a maximum og 0.645r from the center without falling off? I might be way off here...

Most of this looks good, though I'm not sure why you included an ##r## in your final answer. You already gave that ##r = \frac{a_r}{{\pi}^2}##, and this should just give you a number. Also, make sure to use the unrounded value for ##a_r##, and try to avoid truncating the decimal too soon!

Notice also that ##a_r = \frac{v^2}{r} = \frac{r^2 \omega^2}{r} = r \omega^{2}##; this last expression can be a little faster if you're dealing with time periods, where ##\omega = \frac{2\pi}{T}##. But your consideration of time for one revolution is also perfectly valid.

In that way, I might have solved it like ##\mu N = mr\omega^2 \implies 0.7 \times 9.81 = r \times (\frac{2\pi}{2})^{2}##.
 
  • #12
etotheipi said:
Most of this looks good, though I'm not sure why you included an ##r## in your final answer. You already gave that ##r = \frac{a_r}{{\pi}^2}##, and this should just give you a number. Also, make sure to use the unrounded value for ##a_r##, and try to avoid truncating the decimal too soon!

Notice also that ##a_r = \frac{v^2}{r} = \frac{r^2 \omega^2}{r} = r \omega^{2}##; this last expression can be a little faster if you're dealing with time periods, where ##\omega = \frac{2\pi}{T}##. But your consideration of time for one revolution is also perfectly valid.

In that way, I might have solved it like ##\mu N = mr\omega^2 \implies 0.7 \times 9.81 = r \times (\frac{2\pi}{2})^{2}##.
aha, i thought that since the distance from center is given as r in the assignment, i should give the answer as r aswell, since i can't really know if they are talking about meters or what..
 
  • #13
hankrinsen said:
aha, i thought that since the distance from center is given as r in the assignment, i should give the answer as r aswell, since i can't really know if they are talking about meters or what..

Well in this case ##r## just represents a distance, and you can give a distance as a product of a certain number and a chosen unit. Since you did the calculation with other SI quantities, these units are going to simplify down to metres; however, so long as you're careful, you can give ##r## in whatever units you like.
 
  • #14
Alright, thank you very much! I understand it a bit more now.
 
Back
Top