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Problem Sets:
Problem
A pair of identical ellipitcal gears are locked in motion. The half long and short axis of the ellipical gears are $a$ and $b$, respectively. Gear 1 is rotating around one of the focal point $O_1$ at constant angular velocity $\omega_1$, while gear 2 is rotating around one of its focal point $O_2$, and the contact point of the two gears is on the line $O_1O_2$. The distance between $O_1$ and $O_2$ is $2a$. Find the angular velocity $\omega_2$ when the angle between the $O_1$'s long axis and $O_1O_2$ is $\phi$.
The angular velocity of gear 2, $\omega_2$, is given by:
$$\omega_2 = \omega_1 \frac{b^2}{2a^2 - b^2 - 2a\sqrt{a^2-b^2} \cos\phi}$$The problem can be solved by applying the no-slip condition at the contact point of the two gears and using the geometric properties of an ellipse.
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Kinematic Condition Let $r_1$ and $r_2$ be the distances from the rotation centers $O_1$ and $O_2$ to the contact point $P$, respectively. Since the gears are locked in motion, there is no slipping at the contact point. The tangential velocities of the two gears at point $P$ must be equal.
$$v_1 = v_2$$As the contact point lies on the line $O_1O_2$, the velocities are perpendicular to this line. Their magnitudes are given by:
$$\omega_1 r_1 = \omega_2 r_2$$This gives the ratio of the angular velocities:
$$\frac{\omega_2}{\omega_1} = \frac{r_1}{r_2}$$ -
Geometric Constraints The problem states that the distance between the centers of rotation is $O_1O_2 = 2a$. Since the contact point $P$ lies on the line segment $O_1O_2$, the sum of the distances from the foci to the contact point is:
$$r_1 + r_2 = 2a \quad \implies \quad r_2 = 2a - r_1$$Substituting this into the kinematic relation gives $\omega_2$ in terms of $r_1$:
$$\omega_2 = \omega_1 \frac{r_1}{2a - r_1}$$ -
Ellipse Polar Equation The shape of each gear is an ellipse. The distance from a focus to a point on the ellipse can be described by the polar equation. With the origin at the focus $O_1$, the distance $r_1$ to a point on the perimeter is given by:
$$r_1(\phi) = \frac{a(1-e^2)}{1 - e \cos\phi}$$where $\phi$ is the angle between the major axis and the line segment $O_1P$ (which is the line $O_1O_2$), and $e$ is the eccentricity of the ellipse. The eccentricity is defined as $e = c/a = \sqrt{a^2-b^2}/a$.
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Derivation of $\omega_2$ Substitute the expression for $r_1(\phi)$ into the equation for $\omega_2$:
$$\omega_2 = \omega_1 \frac{\frac{a(1-e^2)}{1 - e \cos\phi}}{2a - \frac{a(1-e^2)}{1 - e \cos\phi}}$$Simplify the expression:
$$\omega_2 = \omega_1 \frac{a(1-e^2)}{2a(1 - e \cos\phi) - a(1-e^2)} = \omega_1 \frac{a(1-e^2)}{2a - 2ae \cos\phi - a + ae^2}$$ $$\omega_2 = \omega_1 \frac{a(1-e^2)}{a + ae^2 - 2ae \cos\phi} = \omega_1 \frac{1-e^2}{1 + e^2 - 2e \cos\phi}$$To express this in terms of the given parameters $a$ and $b$, we use $e^2 = \frac{a^2-b^2}{a^2}$:
$$1 - e^2 = 1 - \frac{a^2-b^2}{a^2} = \frac{b^2}{a^2}$$ $$1 + e^2 = 1 + \frac{a^2-b^2}{a^2} = \frac{2a^2-b^2}{a^2}$$Substituting these into the expression for $\omega_2$:
$$\omega_2 = \omega_1 \frac{b^2/a^2}{\frac{2a^2-b^2}{a^2} - 2\frac{\sqrt{a^2-b^2}}{a}\cos\phi}$$ $$\omega_2 = \omega_1 \frac{b^2}{2a^2-b^2 - 2a\sqrt{a^2-b^2}\cos\phi}$$