Rotational Dynamics - Basic Introduction - Free Educational videos for Students in K-12 | Lumos Learning

Rotational Dynamics - Basic Introduction - Free Educational videos for Students in k-12


Rotational Dynamics - Basic Introduction - By The Organic Chemistry Tutor



Transcript
00:00 a 10 kg block is attached to a 20 kg
00:04 pulley Which is a solid disk of Radius two m
00:09 . The block is released from rest , causing the
00:11 disk to spin . What is the angular acceleration of
00:16 the disk ? And how fast is the block fallen
00:19 after eight seconds . So how can we calculate the
00:24 angular acceleration of the disk ? What do we need
00:27 to do ? Well , let's identify the forces that
00:31 are in play here . So let's say that capital
00:35 M . Represents the mass of the disk and lower
00:38 case M . I'm not sure how that happened below
00:42 a case . Um represents the mass of the block
00:45 . Yeah . Now the block experience a downward weight
00:49 force of MG . And there's an upward tension force
00:54 that slows down the descent of the block and that
00:58 tension force also causes the disk to spin in the
01:03 clockwise direction . So with this information , how can
01:09 we use it to calculate the angle acceleration ? And
01:14 I'm going to describe T as being ft . So
01:17 that's the tension force . So I don't confuse that
01:21 with torque . So what we can do at this
01:27 point is right an expression for the network acting on
01:31 the disk . Now there's only one force acting on
01:34 a disk which is the tension force and torque is
01:37 force times the moment arm which in this case is
01:41 the radius of the circle . So the net torque
01:43 acting on the solid disc is the tension force multiplied
01:48 by the radius of the circle . Now let's focus
01:51 on the net force on a block . By the
01:54 way the disk is held in place so the disk
01:58 is allowed to spin but it can accelerate upward or
02:01 downward . Only the block can accelerate downward . So
02:05 we have to deal with the net force of the
02:07 block . So the net force in the y direction
02:13 of the block . It's based on these two forces
02:16 . So we have an upward tension force . So
02:19 it's going to be positive because it's directed in a
02:21 positive direction plus the downward wait for us which is
02:25 negative since it's going in a negative Y direction .
02:29 Now the net force , based on Newton's second law
02:32 , is mass times acceleration . So let's solve for
02:37 the tension force . Let's move this term to that
02:39 side . So M . A . Plus MG were
02:44 raised in the Y direction . That's going to be
02:47 equal to the tension force . Now , here's a
02:50 question for you , Emma , should it be positive
02:54 or negative ? Because the block is accelerated in the
02:59 negative Y direction is going down . We need to
03:01 put a negative in front of it . So we
03:04 could say that detention force is equal to positive MG
03:10 minus Mhm . So now at this point , what
03:15 I'm going to do is replace the tension force in
03:17 this equation with M . G minus M . E
03:22 . So the net torque acting on a disk ,
03:26 it's going to be mg minus M . A times
03:30 the radius . So now since I'm running out of
03:34 space , let's erase a few things now . The
03:40 acceleration or rather the linear acceleration is equal to the
03:44 angular acceleration times the radius . So let's replace A
03:48 with alpha times are so the network is now MG
03:54 minus M . Alpha times are times are . So
03:59 what I'm gonna do now is distribute our to these
04:01 two terms . And at the same time I'm going
04:04 to replace the network with inertia Times Alpha Based on
04:09 you in 2nd law for rotational motion . So that's
04:12 equal to mgr minus mm alpha times R squared .
04:20 Now my goal is to calculate the anglican celebration .
04:24 So I need to isolate this term . So what
04:27 I'm gonna do now is take this term . Move
04:29 it to the left side . So inertia times alpha
04:34 plus I am out for R squared is equal to
04:39 MGR Now this is the network acting on the disk
04:44 . So this is the inertia of the disc .
04:49 So right now let's factor out alpha . So what
04:53 we're going to have is alpha multiplied by the inertia
04:57 of the disc plus M R squared and that's equal
05:01 to MGR . So for this particular problem , the
05:06 angular acceleration can be calculated by taking the mass of
05:09 the block , multiplied by the gravitational acceleration times the
05:12 radius of the disk divided by the inertia of the
05:15 disk plus M R squared . Where lower case M
05:20 is the mass of the block . So now let's
05:22 go ahead and calculate alpha . So that's going to
05:28 be a massive 10 Times The gravitational acceleration of 9.8
05:33 . The radius of the disk is two m .
05:38 Now , I represents the inertia And the inertia of
05:42 a solid disc is 1/2 M . R squared ,
05:46 So the mass of the disk is 20 and the
05:51 radius is too , So half of 20 is 10
05:56 And 10 times two squared is 40 . So the
05:59 inertia of the disk is 40 Plus M . R
06:03 Squared , which is going to be 10 Times are
06:06 square , which is two square . So 10 times
06:10 9.8 is 98 , multiplied by two . So that's
06:14 196 , 10 times two squares 40 plus another 40
06:20 . That's gonna be 80 . So alpha is 196
06:25 divided by 80 . And so that's going to be
06:28 2.45 radiance per second squared . And so that's how
06:35 you can calculate the angle acceleration of the disc .
06:40 So that's how fast it's accelerated in this direction .
06:46 Now , what about heartbeat ? How Fast is the
06:50 block fallen after eight seconds . So how can we
06:53 find that answer ? Well , the first thing we
06:56 need to do is calculate the linear acceleration of the
06:59 disk . If we could find that , then we
07:02 could find out the acceleration of the block as it
07:04 falls down because they have to be the same because
07:07 they're attached to a rope and so they're going to
07:10 move at the same rate . The linear acceleration of
07:14 the disk is alpha , times are So we have
07:16 alpha , which is 2.45 And the radius of the
07:20 circle or the disk is two m , So 2.45
07:25 times two , It's 4.9 . So the linear acceleration
07:30 of the system is 4.9 m/s squared . And so
07:33 that's the acceleration of the block as it descends down
07:37 . So now we could find a final speed of
07:39 the block As it falls for eight seconds . So
07:44 the final speed is going to be the initial speed
07:47 plus 80 . The initial speed is zero because the
07:52 block was released from rest And the linear acceleration is
07:57 4.9 multiplied by eight . So 4.9 times eight Is
08:08 39.2 m/s . So that's the speed of the block
08:11 after eight seconds . Now , if we wanted to
08:14 find the velocity of the block , this would have
08:18 to be negative . The acceleration technically is negative for
08:21 the block because It's accelerating in the negative y direction
08:25 . And so the velocity is negative 39.2 m/s after
08:30 eight seconds . Now , let's say if you wanted
08:34 to find the distance , I wish to block .
08:37 So for these eight seconds , what would you do
08:43 ? So once you have Alpha , and once you
08:46 have the final speed , you can easily find a
08:47 distance at which the object fell . So you can
08:51 use this equation , the final squared is equal to
08:54 the initial square Plus two A . D . So
08:58 you know the final speed is 39.2 . Once you
09:01 square , the negative sign doesn't matter . The initial
09:03 speed is zero And you have the linear acceleration ,
09:06 which is 4.9 . So now you can find D
09:09 the vertical displacement of the object . So it's 39.2
09:14 square Which is 1536.64 And two times 4.9 is 9.8
09:24 . So take 1536.64 And divided by 9.8 . And
09:30 so d is 156.8 m . So that's how far
09:37 the object fell . I mean in the block ,
09:40 that's how far I fell after eight seconds . So
09:44 , consider this problem . We have a five kg
09:47 mass attached to a 20 kg pulley , which is
09:51 a solid disc and let's say the radius of the
09:54 pulley is three m , And that's attached to a
09:59 hanging mass of 10 kg . Now , once this
10:03 system is released from rest , we know the system
10:06 is going to accelerate in this direction . How can
10:09 we calculate the acceleration of the entire system ? So
10:15 , if you want to try this problem , feel
10:18 free to do so and see if you can get
10:21 the right answer positivity if you want to try it
10:24 . So , I'm going to show you two ways
10:25 in which you get the answer . A quick and
10:28 simple way . And also a step by step procedure
10:31 if you want to write out all the equations .
10:34 So , here's the quick and simple way to find
10:36 acceleration based on you . In second law , the
10:39 acceleration of the system is the net force acting on
10:43 the system , divided by the total mass of the
10:46 system . So the only force that's really driving the
10:52 system to motion is really the weight force of this
10:55 block . So that way force is the net force
11:00 acting on the entire system . So let's call this
11:03 M . two . Let's call this M . one
11:07 and this is going to be capital . M .
11:09 The mass of the disk . So the net force
11:11 of the system is M two G . Let's put
11:16 G here and then we need to divided by the
11:20 total mass of the system . So that's the mass
11:23 of the first block , plus the mass of the
11:25 hanging block . And we can't just use this mass
11:30 . We need to take into account this equation .
11:35 The inertia of a disk is 1/2 M . R
11:38 squared . Now for different shapes this number could vary
11:46 , so I'm going to put a constancy so I
11:49 like to think of it as inertial mass . You
11:52 could call it something else if you want , but
11:54 we need that see value to be in this equation
11:56 for this to work . So that's how you can
11:59 find the acceleration of the system for this type of
12:03 system . So let's go ahead and calculate it .
12:07 So M two is 10 . G is 9.8 .
12:11 M one is 5 . M two is 10 .
12:15 See for a disc is 1/2 And the mass of
12:20 the solid disc is 20 kg . So 10 times
12:24 9.8 is 98 , half of 20 is 10 Plus
12:29 another 10 , that's 20 plus five . So this
12:33 is going to be 25 98 divided by 25 Is
12:43 3.92 m/s squared . So this is the acceleration of
12:49 the entire system . So let's see if we can
12:51 get that answer . Using another process . So how
13:05 should we do this ? We need to indicate other
13:09 forces that is acting on the system . So we
13:13 got the downward way force em to G . And
13:16 there's an upward tension force that slows down the descent
13:19 of this object . Let's call that T to detention
13:23 force acting on block two . Now we have T
13:26 . one Which pulls Black 1 to the right Now
13:32 these two tension forces are acting on the Pulley .
13:38 So if T two lifts up the object , You
13:41 can be sure that T . two causes the disk
13:44 to be poured in the clockwise direction , And T
13:50 . one causes the disk to be pulled in the
13:54 counterclockwise direction opposite to that value . And so then
14:00 that torque acting on the disk is the difference between
14:05 these two hours . Now in another video I defined
14:09 a positive torque as a talk that causes counterclockwise rotation
14:15 . So T one Torque 1 is positive . Well
14:20 T1 rather detention force that creates that work is going
14:24 to be positive T . To this tension force will
14:28 create a negative torque because it will cause the disk
14:35 to rotate in a clockwise direction , which I signed
14:38 earlier as a negative torque value . So the network
14:41 of the system , It's going to be the positive
14:44 to work . T . one minus the negative torque
14:47 teach you . And the network is equal to inertia
14:51 times alpha in the same way as net force is
14:54 mass times acceleration . So the network is the inertia
14:58 times the angle acceleration Based on Newton's 2nd Law for
15:01 Rotational Motion . So that's gonna be the difference between
15:04 T . one or talk one minus talked to .
15:09 Now I'm going to take a moment to improve this
15:12 drawn so there is no confusion , so T one
15:20 is being directed opposite to this tension . They have
15:23 to be equal in the opposite direction , and t
15:26 to acting on the disk is in this direction .
15:30 Now T one is going to create a torque that
15:35 will cause the disk to spin in the counter clockwise
15:39 direction . So that's work is positive And T two
15:45 will create . Let's see if I can fit it
15:47 here , A negative torque which will cause this to
15:54 spin in the clockwise direction . And this has been
15:56 in a counterclockwise direction . Keep in mind , clockwise
16:00 rotation is negative . Counterclockwise rotation is associated for positive
16:06 to work . So as we said before , the
16:09 network Is going to be the positive toward T one
16:15 teach you . And so network is inertia times alpha
16:22 . Now the inertia of a solid disc is one
16:26 half times the mass of the disc times r squared
16:31 . Now , linear acceleration is equal to the angular
16:34 acceleration times are . So angular acceleration is linear acceleration
16:39 divided by art . So I'm going to replace Alpha
16:42 with a over our and so that's equal to this
16:54 stuff on the right side . So now let's cancel
17:00 our So what we have left over is 1/2 M
17:06 . R . A . Which is equal to Torque
17:08 one to work . One is equal to the tension
17:12 force times the moment arm , which is the radius
17:15 of the circle . So that's gonna be T one
17:18 times are And to work to it's going to be
17:21 T two times are . So we can divide both
17:25 sides by our So now we have 1/2 mm .
17:33 Which is the difference Between the two tension forces .
17:38 Now the network , is it positive or is it
17:42 negative ? What would you say ? Now ? We
17:44 know the whole system is moving in this direction ,
17:47 which means that the disk has a network that causes
17:51 it to rotate in the clockwise direction which is associated
17:56 with a negative torque . So therefore we need to
17:58 put a negative sign . So now let's save this
18:04 equation , we're going to get back to it so
18:08 I can erase some of the stuff above here because
18:11 I'm going to need a space soon . So I'm
18:27 going to rewrite the equation up here . T 1
18:30 . -52 Is -1/2 . And me now we need
18:42 to relate the tension forces to these two masses .
18:46 So now we need to write expressions for the net
18:48 force acting on each object . So let's start with
18:51 the first object mass one . The net force acting
18:55 on mass one is equal to this tension force because
18:59 there's no other forces acting on it , at least
19:02 in the X . Direction . So the net force
19:05 and that block is equal to Emma , So T
19:09 . one is equal to Emma . So that's the
19:12 first equation that we can right now let's move on
19:16 to block too . So the net force acting on
19:21 block two , which is associate with the wind direction
19:25 , That's going to be equal to the upward tension
19:27 force . T . two minus the downward wait for
19:30 M . Two G . Now keep in mind ,
19:32 MTG is negative because it's going in negative Y direction
19:35 , that's what we have the negative sign and he
19:37 is positive because it's going in a positive direction .
19:41 Now the net force acting on Block two is equal
19:44 to M . Two times A . And this is
19:46 supposed to be M . One A . Now because
19:50 this is moving in a negative Y direction , we
19:52 need to put a negative sign in front of them
19:54 to a . M . one is moving in the
19:57 positive X . Direction . So therefore it requires a
20:00 positive sign . So now I'm going to take this
20:07 term , move it to the left side . So
20:11 therefore M . two G Plus M . two A
20:15 . Is equal to T . two . So that's
20:18 the second equation that we need . So now our
20:21 next step is to replace T . one with M
20:24 . one a . And then replace T . two
20:28 with M . Two G plus mt way . Now
20:35 there's one small correction that I need to make that
20:40 should not be a plus sign since I have a
20:43 negative sign right there . So let's put that minus
20:45 sign . So now let's replace T . one with
20:52 M . One A . And then minus T .
20:59 Two . Which is this stuff here . So let's
21:03 put that in parentheses . So that's gonna be minus
21:05 M . Two G -M2 A . And all of
21:09 that is equal to negative 1/2 . Mhm . Yeah
21:24 so now let's distribute the negative sign . So this
21:27 is going to be M1 a -M two G plus
21:33 M two A . And that's equal to negative one
21:35 half M . A . So I'm going to take
21:38 this term , move it to the right side so
21:40 it becomes positive and then I'm going to take this
21:44 term , move it to the left side so that
21:47 becomes positive . So it's gonna be M . one
21:50 a . Plus , I am too eh Plus 1/2
21:55 capital Emma And that's equal to positive M two G
22:01 . So now I can factor out a from each
22:03 of these three terms . So it's gonna be A
22:06 times M one plus M two Plus 1/2 . And
22:13 that's gonna be equal to MTG . So I need
22:16 to divide both sides by this term . So this
22:19 is my final equation . The acceleration is equal to
22:23 the Darwin weight force , which is basically the net
22:25 force of the system divided by the total mass of
22:28 the system . Where you have to incorporate the c
22:35 . value which is 1/2 for disk . So now
22:40 let's plug everything in . So M2 is 10 ,
22:43 G is 9.8 . M one is 5 M .
22:47 Two is 10 plus one half Times the mass of
22:52 the disk , which is 20 . So this is
22:54 gonna be 98 Divided by 25 just like before .
22:59 And that's going to give us the same answer of
23:01 3.92 meters per second square . So that's the acceleration
23:07 of the whole system . So that's how you can
23:10 find it . So now you have two ways in
23:12 which you can come up with this equation .
Summarizer

DESCRIPTION:

This physics video tutorial provides a basic introduction into rotational dynamics. It explains how to calculate the acceleration of a hanging mass attached to a rotating pulley. Examples include pulleys with two hanging masses (atwood machine) and inclined planes with pulleys and kinetic friction.

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Rotational Dynamics - Basic Introduction is a free educational video by The Organic Chemistry Tutor.

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