Rigid body kinematics

Rigid bodies

A rigid body is an extended area of material that includes all the points inside it, and which moves so that the distances and angles between all its points remain constant. The location of a rigid body can be described by the position of one point $P$ inside it, together with the rotation angle of the body (one angle in 2D, three angles in 3D).

	location description	velocity description
point mass	position vector $ \vec{r}_P $	velocity vector $ \vec{v}_P $
rigid body in 2D	position vector $ \vec{r}_P $ angle $\theta$	velocity vector $ \vec{v}_P $ angular velocity $ \omega $
rigid body in 3D	position vector $ \vec{r}_P $ angles $ \theta,\phi,\psi $	velocity vector $ \vec{v}_P $ angular velocity vector $ \vec{\omega} $

Neither point masses nor rigid bodies can physically exist, as no body can really be a single point with no extent, and no extended body can be exactly rigid. Despite this, these are very useful models for mechanics and dynamics.

Application alert!

Steering geometry uses rigid bodies.

Rigid body kinematics can be used to analyze how steering with the front wheels affects how an entire vehicle turns.

Rotating rigid bodies

All points on a rigid body have the same angular rotation angles, as we can see on the figure below. Because the angular velocity is the derivative of the rotation angles, this means that every point on a rigid body has the same angular velocity $ \vec{\omega} $, and also the same angular acceleration $ \vec{\alpha} $.

In 2D the angle $ \theta $ of a rigid body the angle of rotation from a fixed reference (typically the $ \hat\imath $ direction), measured positive counter-clockwise. The angular velocity is $ \omega = \dot\theta $ and the angular acceleration is $ \alpha = \dot\omega = \ddot\theta $. The vector versions of these are $ \vec\omega = \omega \, \hat{k} $ and $ \vec\alpha = \alpha\,\hat{k} $, where $ \hat{k} $ is the out-of-plane direction.

Show:

All points on a rigid body rotate at the same rate. Body $ \mathcal{B}_1 $ is rotated by angle $\theta_1$, so its angular velocity is $ \omega_1 = \dot{\theta}_1 $, and similarly for the second body.

Warning: Labeling angular quantities on rigid bodies. #rkg-ww

Angular quantities ($ \theta , \omega , \alpha $)for rigid bodies should not be labeled with points. If P and Q are points on a rigid body, we do not write $ \omega_P $ or $ \omega_Q $ for the angular velocity about these points.

Instead, we label angular quantities according to the body. If we have two rigid bodies $ B_1 $ and $ B_2 $, then $ \omega_1 $ is the angular velocity of the first body (and all points on it) and $ \omega_2 $ is the angular velocity of the second body.

Did you know?

Rotations in 3D are significantly more complicated than rotations in 2D. Unlike positions, velocities, etc, which simply go from 2D vectors to 3D vectors, rotational quantities go from scalars in 2D to full 3D vectors in 3D. Angular velocity and angular acceleration are somewhat straightforward, so equations #rkg-er hold in both 2D and 3D, but understanding the rotations themselves is significantly more complicated. There are three main ways that 3D rotations can be represented:

Detailed study of rotations in 3D is necessary for a full understanding of topics ranging from satellite attitude control to articulated robot construction, and is usually covered in advanced dynamics courses.

Points on rigid bodies

If we know how one point $P$ on a rigid body is moving and we also know how the body is rotating, then we can calculate the movement of any other point $Q$ on the same body. The formulas for this are given below.

Rigid body point relations. #rkg-er

$$ \begin{aligned}\vec{r}_Q &= \vec{r}_P + \vec{r}_{PQ} \\\vec{v}_Q &= \vec{v}_P+ \vec{\omega} \times \vec{r}_{PQ} \\\vec{a}_Q &= \vec{a}_P+ \vec{\alpha} \times \vec{r}_{PQ}+ \vec{\omega} \times (\vec{\omega} \times \vec{r}_{PQ})\end{aligned} $$

Points $P$ and $Q$ are two locations on a rigid body. Vectors $ \vec{\omega} $ and $ \vec{\alpha} $ are the angular velocity and angular acceleration of the rigid body.

The first equation is simply the definition of the offset vector $ \vec{r}_{PQ} $. Differentiating the first equation gives

$$ \begin{aligned} \vec{r}_Q &= \vec{r}_P + \vec{r}_{PQ} \\ \dot{\vec{r}}_Q &= \dot{\vec{r}}_P + \dot{\vec{r}}_{PQ} \\ \vec{v}_Q &= \vec{v}_P + \vec{\omega} \times \vec{r}_{PQ}, \end{aligned} $$

where the derivative of $ \vec{r}_{PQ} $ comes from the rotation formula, given that this offset vector is simply rotating with the rigid body.

If we differentiate again then we obtain

$$ \begin{aligned} \vec{v}_Q &= \vec{v}_P + \vec{\omega} \times \vec{r}_{PQ} \\ \dot{\vec{v}}_Q &= \dot{\vec{v}}_P + \dot{\vec{\omega}} \times \vec{r}_{PQ} + \vec{\omega} \times \dot{\vec{r}}_{PQ} \\ \vec{a}_Q &= \vec{a}_P + \vec{\alpha} \times \vec{r}_{PQ} + \vec{\omega} \times (\vec{\omega} \times \vec{r}_{PQ}), \end{aligned} $$

where we use the fact that $ \vec{\alpha} = \dot{\vec{\omega}} $.

Warning: Cross product order #rkg-wc

Because cross products are not associative, it is very important to compute the centripetal acceleration term with the parentheses as shown. That is, we must not compute $ (\vec{\omega} \times \vec{\omega}) \times \vec{r}_{PQ} $, as this is always zero.

The term $ \vec{\omega} \times (\vec{\omega} \times \vec{r}_{PQ}) $ in the acceleration equation above is called the centripetal (center-seeking) term, as it is always in the direction $ -\vec{r}_{PQ} $ and so acts from $Q$ towards the “center” $P$.

Show: none position velocity acceleration

Two points $P$ and $Q$ on a moving and accelerating rigid body.

Example Problem: Points on a rigid body #rkg-xp

A rectangular block is sliding along the ground so that the contact point $P$ is moving at a constant speed of $3\rm\ m/s$ to the left. The block is rotating clockwise and just before point $Q$ hits the ground the angular velocity is $2\rm\ rad/s$ clockwise and the angular acceleration is $3\rm\ rad/s^2$ clockwise. What is the velocity and acceleration of $Q$ just before impact?

Using the regular $ \hat\imath,\hat\jmath $ basis, the known information just before impact is

$$ \vec{r}_{PQ} = 2\,\hat\imath \qquad \vec{v}_P = -3\,\hat\imath \qquad \vec{a}_P = 0 \qquad \vec\omega = -2\,\hat{k} \qquad \vec\alpha = -3\,\hat{k}. $$

The velocity and acceleration of $Q$ are given by

$$ \begin{aligned} \vec{v}_Q &= \vec{v}_P + \vec{\omega} \times \vec{r}_{PQ} \\ &= -3\,\hat\imath - 2\,\hat{k} \times 2\,\hat\imath \\ &= -3\,\hat\imath - 4\,\hat\jmath \\ \vec{a}_Q &= \vec{a}_P + \vec{\alpha} \times \vec{r}_{PQ} + \vec{\omega} \times (\vec{\omega} \times \vec{r}_{PQ}) \\ &= 0 - 3\,\hat{k} \times 2\,\hat\imath - 2\,\hat{k} \times (-2\,\hat{k} \times 2\,\hat\imath) \\ &= -6\,\hat\jmath - 2\,\hat{k} \times (-4\,\hat\jmath) \\ &= -8\,\hat\imath - 6\,\hat\jmath. \end{aligned} $$

Example Problem: Coupled rigid bodies #rkg-xc

Three rigid bodies (two rods and a block) are coupled by pins at $O$, $P$, and $Q$ as shown. Body $ \mathcal{B}_3 $ cannot rotate and must slide horizontally along the ground. The rod lengths are $ OP = 3\sqrt{2}\rm\ m $ and $ PQ = 5\rm\ m $, and points $O$ and $Q$ are the same height above the ground.

At the instant shown, $ \theta_1 = 45^\circ $, $ \omega_1 = 4\rm\ rad/s $ . What are $ \omega_2 $ and $ \vec{v}_Q $ at this instant?

Taking a regular $ \hat\imath,\hat\jmath $ basis at $O$, we can use the rod lengths and angles to find the relative position vectors:

$$ \begin{aligned} \vec{r}_{OP} &= 3\hat\imath + 3\hat\jmath\rm\ m \\ \vec{r}_{PQ} &= 4\hat\imath - 3\hat\jmath\rm\ m. \end{aligned} $$

Using the vector angular velocities $ \vec{\omega}_1 = \omega_1\,\hat{k} $ and $ \vec{\omega}_2 = \omega_2\,\hat{k} $, we can now use #rkg-er to find first $ \vec{v}_P $ and then $ \vec{v}_Q $ in terms of the unknown angular velocity $\omega_2$:

$$ \begin{aligned} \vec{v}_{P} &= \vec{v}_O + \vec{\omega}_1 \times \vec{r}_{OP} \\ &= 4\hat{k} \times (3\hat\imath + 3\hat\jmath) \\ &= -12\hat\imath + 12\hat\jmath{\rm\ m/s} \\ \vec{v}_{Q} &= \vec{v}_P + \vec{\omega}_2 \times \vec{r}_{PQ} \\ &= (-12\hat\imath + 12\hat\jmath{\rm\ m/s}) + \omega_2\,\hat{k} \times (4\hat\imath - 3\hat\jmath) \\ &= (-12 + 3\omega_2)\,\hat\imath + (12 + 4\omega_2)\,\hat\jmath{\rm\ m/s}. \end{aligned} $$

The last piece of information that we need to use is the constraint on the motion of $ \mathcal{B}_3 $, namely that it can only slide horizontally. This can be expressed by saying that the vertical component of $ \vec{v}_Q $ is zero, or more generally that the component in the normal direction $ \hat{e}_n = \hat\jmath $ is zero. That is:

$$ \begin{aligned} 0 &= \vec{v}_Q \cdot \hat{e}_n \\ &= \Big((-12 + 3\omega_2)\,\hat\imath + (12 + 4\omega_2)\,\hat\jmath\Big) \cdot \hat\jmath \\ &= 12 + 4\omega_2 \\ \omega_2 &= -3{\rm\ rad/s}. \end{aligned} $$

Substituting this back into the expression above for $ \vec{v}_Q $ gives:

$$ \vec{v}_Q = -21\hat\imath{\rm\ m/s}, $$

which does indeed have no vertical component, as expected.

Warning: Rigid body points may be accelerating even if $\vec{a}_P = 0$ and $\alpha = 0$. #rkg-wa

If $ \vec{\alpha} = 0 $ and $ \vec{a}_P = 0 $ for a rigid body then we would normally say that the body itself is not accelerating. This does not mean, however, that the points on the bodies are not accelerating. If the body is rotating (so $ \vec{\omega} \ne 0 $) then the centripetal acceleration means that in fact most points on the body are accelerating at any time.

Constrained motion

One of the most common type of motion is constrained motion, where an object is restricted to move in a certain way.

Generally, a point constrained to move in a specific direction obeys the following equation:

Constraint equation for a point $P$. #rkc-pc

$$ \vec{v}_P \cdot \hat{n}_P = 0 $$

where $ \hat{n}_P $ is the normal vector to the motion of point $P$.

The above equation is difficult to apply to a system with a collection of points or particles. It is not the only way to derive constraint equations. For example, rigid body kinematics equations (also known as relative motion equations) are derived using the definition of a rigid body. Namely, the distance and angles between all points remain constant. See rigid body relations. It is often best to look at examples of constrained motion to see how constraint equations are differentiated to obtain velocity and acceleration.

We can visualize the motion of several constrained systems, shown on the figure below.

System:

rod-circular

slider-crank

rod-circular

slider-crank

Example Problem: Sliding rod #rkc-xcl

A uniform rod leaning against a wall has a fixed length of $\ell = 10 \rm\ m$. The bottom of the rod at point $P$ is $8 \rm\ m$ from the wall. Point $P$ is moving away from the wall at a speed of $6 \rm\ m/s$. The rod maintains contact with the wall and ground at all times. What is $ \vec{v}_Q $ of point $Q$, the point at the top of the rod?

To solve this, note the question states that the rod's length is fixed, and is not permitted to lose contact with the wall and ground. Therefore, the constraint equation is given by the Pythagorean theorem:

$$ \begin{aligned} x_P^2 + y_Q^2 = \ell^2 \end{aligned} $$

This becomes a related rates problem from calculus 1.

Differentiating with respect to time, keeping in mind the chain rule:

$$ \begin{aligned} 2x_P\dot{x}_P + 2y_Q\dot{y}_Q = 0 \end{aligned} $$

The quantity we're interested in is $ \dot{y}_Q $ , or $ v_Q $, and $ y_Q = \sqrt{\ell^2 - x_P^2} $ .

Solving yields $ \vec{v}_Q = -8\hat{\jmath} \rm\ m/s $ .

Another way to solve this is using the rigid body relations, knowing that the distance and angles from the top to the bottom of the rod remains constant, which is a rigid body by definition. Using rigid body relations:

$$ \begin{aligned} \vec{v}_Q &= \vec{v}_P + \vec\omega \times \vec{r}_{PQ} \\ &= \vec{v}_P + \omega_z \vec{r}_{PQ}^{\perp} \end{aligned} $$

where we have two unknowns:$ \vec{v}_Q $ , and $\vec\omega$, and $ \vec{r}_{PQ} = -\ell \cos\theta \hat{\imath} + \ell \sin\theta \hat{\jmath} \rm\ m $, where $ \theta = \cos^{-1}\left(\frac{x_P}{\ell}\right) $.

Therefore, $ \vec{r}_{PQ}^{\perp} = -\ell \sin\theta \hat{\imath} - \ell \cos\theta \hat{\jmath} \rm\ m $ .

Expanding the vector equation into its two scalar equations yields:

$$ \begin{aligned} v_{Qx} &= v_{Px} - \omega_z \ell \sin\theta \\ v_{Qy} &= v_{Py} - \omega_z \ell \cos\theta \end{aligned} $$

Since the top of the rod can only move vertically, $ v_{Qx} = 0, and \omega_z = \frac{v_{Px}}{\ell \sin\theta} \rm\ rad/s $

Since the bottom of the rod can only move horizontally, $ v_{Py} = 0, and v_{Qy} = -\omega_z \ell \cos\theta \rm\ m/s $

Plugging in $\omega_z$ expression:

$$ v_{Qy} = -\frac{v_{Px}}{\ell \sin\theta} \ell \cos\theta = -v_{Px}\cot\theta \rm\ m/s $$

Plugging in the numbers yields the same result of $ \vec{v}_{Q} = -8\hat{\jmath} \rm\ m/s $ .

Note in the rigid body relations method, we implicitly used the constraint equation for a point. Namely, we know that the top of the rod can only move vertically, so $ \vec{v}_Q \cdot \hat{n}_Q = 0 $ , where $ \hat{n}_Q = \hat{\imath} $ and $ \vec{v}_P \cdot \hat{n}_P = 0 $ , where $ \hat{n}_P = \hat{\jmath} $.

In general, the steps involved in analyzing systems with constrained motions are as follows:

Solution procedure for constrained motion. #rkc-cp

$$ \begin{aligned}&\text{1. Write down constraint equation in terms of distances/positions.} \\&\text{2. Differentiate once or twice with respect to time to obtain} \\& \quad \vec{v} \quad \text{and} \ \vec{a} \ \text{relationships.} \\&\text{3. Solve for the desired quantity.}\end{aligned} $$

Example Problem: Compound pulley system #rkc-xcp

Consider the compound pulley system shown, consisting of two massless pulleys $A, B$. Pulley $A$ is free to move vertically, and pulley $B$ is fixed to the top. The two pulleys are connected by an inextensible, massless rope. One block of mass $m_1$ is connected to pulley $A$ by a string, and another block of mass $m_2$ is hanging from the rope connecting the two pulleys. Assume the pulleys' radii are negligbile. If $m_2$ moves downwards at a velocity $v_2 = 6 \rm\ m/s$ and acceleration $a_2 = 2 \rm\ m/s^2$, what are the velocity and acceleration of $m_1$?

We will begin by underlining important information given in the question. Namely:

The rope is inextensible, meaning the total length of the rope remains constant. This is our constraint.
The pulleys are massless, meaning we do not need to consider any rotational motion they may exhibit.
The pulleys radii' are negligbile, meaning we do not need to consider their radii as a part of the total length of the rope.

Using the solution procedure highlighted in #rkc-cp:

1. Write down constraint equation in terms of distances/positions. If the rope's length remains constant, we need to choose a reference line to relate the distances of the masses to that reference line and set it equal to the rope's length. The following figure shows the reference line, as well as the masses' distances from that line.

Note that $y_1$ is only extended to pulley $A$. Since the pulleys are massless, they will not rotate, and therefore $m_1$ and pulley $A$ will translate vertically together at the same rate.

Now, we can write the total length of the rope in terms of those two distances. The total length of the rope,$L$ will be:

$$ 2y_1 + y_2 = L $$

2. Differentiate once or twice with respect to time to obtain $ \vec{v} $ and $ \vec{a} $ relationships. Now, we can take two derivatives with respect to time to obtain the relationship between the speeds $ v_1, v_2 $ , and the accelerations $ a_1, a_2 $ .

$$ \begin{aligned} 2v_1 + v_2 &= 0 \\ 2a_1 + a_2 &= 0 \end{aligned} $$

Notice that the length of the rope does not matter ultimately. This makes sense, as the length of the rope is constant, and therefore does not change with time.

3. Solve for the desired quantity. We are interested in both the velocity and acceleration of $m_1$.
Solving for $ \vec{v}_1 = \frac{-\vec{v}_2}{2} = 3\hat{\jmath}\rm\ m/s $ and $ \vec{a}_1 = \frac{-\vec{a}_2}{2} = \hat{\jmath}\rm\ m/s^2 $

Reflecting on the result obtained, it makes sense. The distance $m_1$ has to travel up the rope is two times more than the length $m_2$ has to travel. We can also draw a free-body diagram to understand this result further. We will return to this example further down when constraint forces are covered.

Reference material

Calculus and vectors
Rigid bodies
Kinetics of point masses
Kinetics of rigid bodies
Free body diagrams
Energy and work

Applications

Four-bar linkages

Four-bar linkages are a prominent example of constrained motion being in effect.

Constraint forces

If an object is constrained to move in a specific direction, by Newton's second law, there must be forces or moments preventing the movement of the object in that direction. Those are called constraint forces.

The approach to solving for constraint forces is the same approach to solve for any forces/moments that are not constraint forces. Namely, drawing a free body diagram, and applying Newton's equations. See the solution procedure with Newton's equations.

Let's return to our example of the rod leaning against a wall.

Example Problem: Constraint forces on a sliding rod. #rkc-xcf

A uniform rod of mass $m$ and length $\ell$ is leaning against a frictionless wall at an angle $\phi$ as shown. The rod starts sliding along a frictionless ground under the influence of gravity $ \vec{g} $. What are the expressions of the constraint forces $ \vec{F}_P, \vec{F}_Q $ that ensure the rod maintains contact with the wall and ground at all times?

We will begin by drawing a free body diagram on the rod.

Note that due to the constraint placed on the rod, point $P$ can only slide along the ground and therefore by #rkc-pc, $ \vec{F}_P $ acts vertically. Similarly for point $Q$, $ \vec{F}_Q $ acts horizontally.

Applying Newton's second law:

$$ \sum \vec{F}_{ext} = m\vec{a}_C $$

Breaking it up into the scalar equations. Note we will use $ \ddot{x}_C, \ddot{y}_C $ to denote the acceleration of the center of mass $C$ in each direction.

$$ \begin{aligned} F_Q &= m\ddot{x}_C \\ F_P - mg &= m\ddot{y}_C \end{aligned} $$

Now we can apply the solution procedure detailed in #rkc-cp to find the acceleration of point $C$. Due to our constraint, the following applies at all times:

$$ x_C = \frac{\ell}{2}\sin\phi \qquad \qquad y_C = \frac{\ell}{2}\cos\phi $$

Differentiating twice, keeping in mind the chain rule:

$$ \begin{aligned} \ddot{x}_C &= -\frac{\ell\dot\theta^2}{2}\sin\phi + \frac{\ell\ddot\theta}{2}\cos\phi \\ \ddot{y}_C &= -\frac{\ell\dot\theta^2}{2}\cos\phi - \frac{\ell\ddot\theta}{2}\sin\phi \end{aligned} $$

Plugging into Newton's second law equations and solving for each constraint force yields:

$$ \begin{aligned} F_Q &= -\frac{m\ell\dot\theta^2}{2}\sin\phi + \frac{m\ell\ddot\theta}{2}\cos\phi \\ F_P &= -\frac{m\ell\dot\theta^2}{2}\cos\phi - \frac{m\ell\ddot\theta}{2}\sin\phi + mg \end{aligned} $$

Example Problem: Instance where rod loses contact with a wall. #rkc-xlc

A uniform rod of mass $m$ and length $\ell$ is leaning against a frictionless wall at rest at an angle $\phi$ as shown. The rod starts sliding on a frictionless ground under the influence of gravity $ \vec{g} $. At what angle $\theta$ does the rod lose contact with the wall?

While there is contact with the wall, our constraint still holds. This means our constraint forces expressions from #rkc-cf still hold. We are only interested in the constraint force from the wall on the rod, $ \vec{F}_Q $. at $ \theta $:

$$ F_Q = -\frac{m\ell\dot\theta^2}{2}\sin\theta + \frac{m\ell\ddot\theta}{2}\cos\theta $$

If the rod loses contact with the wall, then $ \vec{F}_Q = 0 $. We have two unknowns: the angular velocity $\dot\theta$ and the angular acceleration $\ddot\theta$. However, we know that $ \ddot\theta = \frac{d\dot\theta}{dt} $ , so if we obtain an expression for $ \dot\theta $, then finding $ \ddot\theta $ is possible. We can use conservation of energy to obtain an expression for $ \dot\theta $.

Using the work-energy theorem:

$$ W = \Delta T + \Delta V $$

The rod is sliding along frictionless surfaces, so there are no non-conservative forces present, and constraint forces do no work (See work done by a constraint force)

Therefore:

$$ \begin{aligned} T_1 + V_1 &= T_2 + V_2 \\ 0 + mgh_{C, 1} &= \frac{1}{2}mv_C^2 + \frac{1}{2}I_{C, \hat{k}}\omega^2 + mgh_{C, 2} \end{aligned} $$

From before:

$$ \begin{aligned} h_{C, 1} = y_{C, 1} = \ell\cos\phi \qquad h_{C, 2} = y_{C, 2} = \ell\cos\theta \end{aligned} $$

And the velocity of the center of mass at $ \theta $:

$$ \begin{aligned} \vec{v}_C &= \dot{x}_{C,2}\hat{\imath} + \dot{y}_{C, 2}\hat{\jmath} \\ &= \ell\dot\theta\cos\theta \hat{\imath} - \ell\dot\theta\sin\theta \hat{\jmath} \end{aligned} $$

So $ v_C $ is simply $ l\dot\theta $.

Plugging into our energy conservation, where $ I_{C, \hat{k}} = \frac{1}{12}m\ell^2 $:

$$ \begin{aligned} mg\ell\cos\phi &= \frac{1}{2}m(\ell\dot\theta)^2 + \frac{1}{2}\left(\frac{1}{12}m\ell^2 \right) \dot\theta^2 + mg\ell\cos\theta \\ mg\ell\cos\phi &= \frac{1}{2}m\ell^2 \dot\theta^2 + \frac{1}{24}m\ell^2 \dot\theta^2 + mg\ell\cos\theta \\ mg\ell\cos\phi &= \frac{13}{24}m\ell^2 \dot\theta^2 + mg\ell\cos\theta \end{aligned} $$

Solving for $ \dot\theta^2 $ :

$$ \dot\theta^2 = \frac{24g}{13\ell}\left(\cos\phi - \cos\theta\right) $$

Differentiating to obtain $ \ddot\theta $ :

$$ \begin{aligned} 2\dot\theta\ddot\theta &= \frac{24g}{13\ell}\sin\theta\dot\theta \\ \ddot\theta & = \frac{12g}{13\ell}\sin\theta \end{aligned} $$

Plugging our results into $ F_Q $ :

$$ \begin{aligned} F_Q &= -\frac{m\ell\frac{24g}{13\ell}\left(\cos\phi - \cos\theta\right)}{2}\sin\theta + \frac{m\ell\frac{12g}{13\ell}\sin\theta}{2}\cos\theta \\ &= -\frac{12}{13}mg\sin\theta \left(\cos\phi - \cos\theta\right) + \frac{6}{13}mg\cos\theta\sin\theta \\ \end{aligned} $$

Setting $ F_Q=0 $ :

$$ \begin{aligned} \frac{12}{13}mg\sin\theta \left(\cos\phi - \cos\theta\right) &= \frac{6}{13}mg\cos\theta\sin\theta \\ 2\left(\cos\phi - \cos\theta\right) &= \cos\theta \\ 2\cos\phi - 2\cos\theta - \cos\theta &= 0 \\ 2\cos\phi - 3\cos\theta &= 0 \\ \end{aligned} $$

Solving for $ \theta $ yields $ \theta = \arccos\left(\frac{2}{3}\cos\phi\right) $ , or when the rod has fallen 2/3 of the original height. Note if the rod was unconstrained, the constraint we used still holds until the rod has fallen 2/3 of the original height. We can use rigid body relations to find the velocity of point $Q$ once the rod loses contact with the wall, and it will have both vertical and horizontal components of velocity, as expected.

Example Problem: Tension in a compound pulley system. #rkc-xtp

Consider the compound pulley system shown, consisting of two massless pulleys $A, B$. Pulley $A$ is free to move vertically, and pulley $B$ is fixed to the top. The two pulleys are connected by an inextensible, massless rope. One block of mass $m_1$ is connected to pulley $A$ by a string, and another block of mass $m_2$ is hanging from the rope connecting the two pulleys. Assume the pulleys' radii are negligbile, and the rope can only slip. What is the tension $T$ in the rope?

We added one more assumption to the ones made in #rkc-xcp. Namely, the rope can only slip. This simply means that the tension is the same at any point in the rope.

We will begin by drawing a free body diagram and applying Newton's second law on three bodies: $ m_1 $, $ m_2 $ and pulley $A$. We will neglect pulley $B$ as it is fixed to the wall, and the results obtained from it are trivial.

The free body diagram on pulley $A$ is as follows:

Applying Newton's second law:

$$ 2T - T_2 = m_A a_A $$

Since the pulley is massless, that means $ T_2 = 2T $ .

The free body diagram on $ m_1 $ is as follows:

Applying Newton's second law:

$$ 2T - m_1 g = m_1 a_1 $$

Finally, the free body diagram on $ m_2 $ is as follows:

Applying Newton's second law:

$$ T - m_2 g = m_2 a_2 $$

We have 3 unknowns, 2 equations. We apply our constraint equation from #rkc-xcp to relate the accelerations of $ m_1 $ and $ m_2 $:

$$ 2a_1 + a_2 = 0 $$

Solving for $T$ from Newton's second law on $ m_2 $:

$$ T = m_2 a_2 + m_2 g $$

Plugging it into Newton's second law on $ m_1 $:

$$ 2m_2 a_2 + 2m_2 g - m_1 g = m_1 a_1 $$

Since $ a_2 = -2a_1 $ :

$$ \begin{aligned} -4m_2 a_1 + 2m_2 g - m_1g &= m_1 a_1 \\ g\left(2m_2 - m_1 \right) &= a_1\left(m_1 + 4m_2\right) \end{aligned} $$

Solving for $ a_1 $ :

$$ a_1 = \frac{g\left(2m_2 - m_1 \right)}{m_1 + 4m_2} $$

Plugging that result into Newton's second law on $ m_1 $ and solving for $T$:

$$ T = \frac{m_1\frac{g\left(2m_2 - m_1 \right)}{m_1 + 4m_2} + m_1g}{2} $$

Simplifying a little by multiplying the top and bottom by $ m_1 + 4m_2 $ :

$$ T = \frac{m_1g(2m_2 - m_1) + m_1g(m_1 + 4m_2)}{2(m_1 + 4m_2)} $$

We obtain our final result for the tension in the rope $T$:

$$ T = \frac{3m_1m_2g}{m_1 + 4m_2} $$

Gears

Larger gear - > slower spin
Accelerations - > tangential are equal but centripetal are not
Opposite direction

Standard sign convention

$ \omega_{1z} $ and $ \omega_{2z} $ have opposite signs (the gears rotate in opposite direction)
Smaller gears rotate faster

Example: Rotating gears. #rkc-gsc

Example: Rotating gears with chain. #rkc-csc

	location description	velocity description
point mass	position vector \( \vec{r}_P \)	velocity vector \( \vec{v}_P \)
rigid body in 2D	position vector \( \vec{r}_P \) angle \(\theta\)	velocity vector \( \vec{v}_P \) angular velocity \( \omega \)
rigid body in 3D	position vector \( \vec{r}_P \) angles \( \theta,\phi,\psi \)	velocity vector \( \vec{v}_P \) angular velocity vector \( \vec{\omega} \)

Movement:	translation	var. translation	rotation	var. rotation	slide
	hinge	circle	spin	reverse spin	oscillation

Rigid body kinematics

Rigid bodies

Rotating rigid bodies

Points on rigid bodies

Rigid bodies in 2D

Constrained motion

Constraint forces

Gears

Standard sign convention

Acceleration in contact (no slip)

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