Elliptical disc in the corner

Geometry Level pending

An elliptical disc has a semi-major axis length of 5 5 and a semi-minor axis length of 2 2 . It is pushed against the corner of the first octant (where x 0 , y 0 x \ge 0 , y \ge 0 and z 0 z \ge 0 ). The elliptical disc cannot penetrate the coordinate planes (the x y xy , x z xz , and y z yz planes), and can only be tangent to them. In its final position, the unit normal to its plane is given by ( sin π 3 cos π 6 , sin π 3 sin π 6 , cos π 3 ) (\sin \frac{\pi}{3} \cos \frac{\pi}{6} , \sin \frac{\pi}{3} \sin \frac{\pi}{6} , \cos \frac{\pi}{3}) . The elliptical disc is oriented in such a way that its major axis makes an angle of + π 6 +\dfrac{\pi}{6} (counterclockwise) with the direction of the steepest descent on its plane. There are three tangency points with the three coordinate planes. If ( 0 , a , b ) (0, a, b) is the tangency point with the y z yz plane, then find a + b a + b .


The answer is 9.453.

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2 solutions

David Vreken
Feb 7, 2019

The elliptical disc is tangent to the three sides of the triangle formed by the extension of the plane that is on the x y xy , x z xz , and y z yz planes:

Since the unit normal vector to the plane of the disc is ( sin π 3 cos π 6 , sin π 3 sin π 6 , cos π 3 ) = ( 3 4 , 3 4 , 1 2 ) (\sin \frac{\pi}{3} \cos \frac{\pi}{6}, \sin \frac{\pi}{3} \sin \frac{\pi}{6}, \cos \frac{\pi}{3}) = (\frac{3}{4}, \frac{\sqrt{3}}{4}, \frac{1}{2}) , the equation of the plane is 3 4 x + 3 4 y + 1 2 z = d \frac{3}{4}x + \frac{\sqrt{3}}{4}y + \frac{1}{2}z = d , and its x x -, y y -, and z z -intercepts ( A A , B B , and C C ) solve to ( 4 3 d , 0 , 0 ) (\frac{4}{3}d, 0, 0) , ( 0 , 4 3 d , 0 ) (0, \frac{4}{\sqrt{3}}d, 0) , and ( 0 , 0 , 2 d ) (0, 0, 2d) , which by Pythagorean's Theorem makes the sides of the triangle 8 3 d \frac{8}{3}d , 2 21 3 d \frac{2\sqrt{21}}{3}d , and 2 13 3 d \frac{2\sqrt{13}}{3}d .

Now move A B C \triangle ABC to a Cartesian coordinate system with A A at ( 0 , 0 ) (0, 0) and B B at ( 8 3 d , 0 ) (\frac{8}{3}d, 0) :

C C is 2 13 3 d \frac{2\sqrt{13}}{3}d away from A A so by the distance formula C x 2 + C y 2 = 2 13 3 d \sqrt{C_x^2 + C_y^2} = \frac{2\sqrt{13}}{3}d , and C C is 2 21 3 d \frac{2\sqrt{21}}{3}d away from B B so ( C x 8 3 d ) 2 + C y 2 = 2 21 3 d \sqrt{(C_x - \frac{8}{3}d)^2 + C_y^2} = \frac{2\sqrt{21}}{3}d , and this solves to ( C x , C y ) = ( 2 3 d , 4 3 d ) (C_x, C_y) = (\frac{2}{3}d, \frac{4}{\sqrt{3}}d) . This means the equation of the line A C AC is y = 2 3 x y = 2\sqrt{3}x and the equation of the line B C BC is y = 2 3 ( x 8 3 d ) y = -\frac{2}{\sqrt{3}}(x - \frac{8}{3}d) .

The steepest descent of the plane is the altitude of A B C \triangle ABC , so the ellipse is rotated π 6 \frac{\pi}{6} counterclockwise from the vertical. Since the semi-major axis is 5 5 and the semi-minor axis is 2 2 , the equation of the ellipse before the rotation is ( x h ) 2 4 + ( y k ) 2 25 = 1 \frac{(x - h)^2}{4} + \frac{(y - k)^2}{25} = 1 for center ( h , k ) (h, k) , and is 79 ( x h ) 2 400 + 21 3 ( x h ) ( y k ) 200 + 37 ( y k ) 2 400 = 1 \frac{79(x - h)^2}{400} + \frac{21\sqrt{3}(x - h)(y - k)}{200} + \frac{37(y - k)^2}{400} = 1 after the rotation. Using implicit differentiation, the slope at any point on the ellipse solves to m = 79 ( x h ) 21 3 ( y k ) 21 3 ( x h ) + 37 ( y k ) m = \frac{-79(x - h) - 21\sqrt{3}(y - k)}{21\sqrt{3}(x - h) + 37(y - k)} .

The ellipse is tangent to y = 0 y = 0 which has a slope of m = 0 m = 0 at y = 0 y = 0 . Then 79 ( x h ) 2 400 + 21 3 ( x h ) ( y k ) 200 + 37 ( y k ) 2 400 = 1 \frac{79(x - h)^2}{400} + \frac{21\sqrt{3}(x - h)(y - k)}{200} + \frac{37(y - k)^2}{400} = 1 and m = 79 ( x h ) 21 3 ( y k ) 21 3 ( x h ) + 37 ( y k ) m = \frac{-79(x - h) - 21\sqrt{3}(y - k)}{21\sqrt{3}(x - h) + 37(y - k)} with m = 0 m = 0 and y = 0 y = 0 solves to k = 79 2 k = \frac{\sqrt{79}}{2} .

The ellipse is also tangent to y = 2 3 x y = 2\sqrt{3}x which has a slope of m = 2 3 m = 2\sqrt{3} . Then 79 ( x h ) 2 400 + 21 3 ( x h ) ( y k ) 200 + 37 ( y k ) 2 400 = 1 \frac{79(x - h)^2}{400} + \frac{21\sqrt{3}(x - h)(y - k)}{200} + \frac{37(y - k)^2}{400} = 1 and m = 79 ( x h ) 21 3 ( y k ) 21 3 ( x h ) + 37 ( y k ) m = \frac{-79(x - h) - 21\sqrt{3}(y - k)}{21\sqrt{3}(x - h) + 37(y - k)} with k = 79 2 k = \frac{\sqrt{79}}{2} , m = 2 3 m = 2\sqrt{3} , and y = 2 3 x y = 2\sqrt{3}x solves to h = 1 12 ( 5 93 + 237 ) h = \frac{1}{12}(5\sqrt{93} + \sqrt{237}) .

The ellipse is also tangent to y = 2 3 ( x 8 3 d ) y = -\frac{2}{\sqrt{3}}(x - \frac{8}{3}d) which has a slope of m = 2 3 m = -\frac{2}{\sqrt{3}} at T T . Then 79 ( x h ) 2 400 + 21 3 ( x h ) ( y k ) 200 + 37 ( y k ) 2 400 = 1 \frac{79(x - h)^2}{400} + \frac{21\sqrt{3}(x - h)(y - k)}{200} + \frac{37(y - k)^2}{400} = 1 and m = 79 ( x h ) 21 3 ( y k ) 21 3 ( x h ) + 37 ( y k ) m = \frac{-79(x - h) - 21\sqrt{3}(y - k)}{21\sqrt{3}(x - h) + 37(y - k)} with k = 79 2 k = \frac{\sqrt{79}}{2} , h = 1 12 ( 5 93 + 237 ) h = \frac{1}{12}(5\sqrt{93} + \sqrt{237}) , m = 2 3 m = -\frac{2}{\sqrt{3}} and y = 2 3 ( x 8 3 d ) y = -\frac{2}{\sqrt{3}}(x - \frac{8}{3}d) solves to x = T x = 11 2 3 + 5 93 12 + 237 12 x = T_x = \frac{11}{2\sqrt{3}} + \frac{5\sqrt{93}}{12} + \frac{\sqrt{237}}{12} , y = T y = 37 3 2 133 + 79 2 y = T_y = \frac{37\sqrt{3}}{2\sqrt{133}} + \frac{\sqrt{79}}{2} , and d = 1 32 ( 5 93 + 3 133 + 4 237 ) d = \frac{1}{32}(5\sqrt{93} + 3\sqrt{133} + 4\sqrt{237}) . We now know the coordinates of B B are ( 1 12 ( 5 93 + 3 133 + 4 237 ) , 0 ) (\frac{1}{12}(5\sqrt{93} + 3\sqrt{133} + 4\sqrt{237}), 0) , and by the distance formula, B T 2 = 1 152 ( 7307 + 37 31521 ) BT^2 = \frac{1}{152}(7307 + 37\sqrt{31521}) .

Moving back to the three-dimensional picture, the equation of the line B C BC is z = 3 2 y + 2 d z = \frac{\sqrt{3}}{2}y + 2d . Since T T is on B C BC , T z = 3 2 T y + 2 d T_z = \frac{\sqrt{3}}{2}T_y + 2d and by the distance formula ( T y 4 3 d ) 2 + T z 2 = B T 2 (T_y - \frac{4}{\sqrt{3}}d)^2 + T_z^2 = BT^2 , and since d = 1 32 ( 5 93 + 3 133 + 4 237 ) d = \frac{1}{32}(5\sqrt{93} + 3\sqrt{133} + 4\sqrt{237}) and B T 2 = 1 152 ( 7307 + 37 31521 ) BT^2 = \frac{1}{152}(7307 + 37\sqrt{31521}) , this solves numerically to ( T y , T z ) ( 3.198 , 6.255 ) (T_y, T_z) \approx (3.198, 6.255) .

Therefore, a = T y 3.198 a = T_y \approx 3.198 and b = T z 6.255 b = T_z \approx 6.255 , and a + b 3.193 + 6.255 9.453 a + b \approx 3.193 + 6.255 \approx \boxed{9.453} .

You've done it again. Excellent Work.

Hosam Hajjir - 2 years, 4 months ago

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Another great problem!

David Vreken - 2 years, 4 months ago
Hosam Hajjir
Feb 7, 2019

The unit normal specified by the problem is

n ^ = ( sin θ cos ϕ , sin θ sin ϕ , cos θ ) \hat{n} = ( \sin \theta \cos \phi, \sin \theta \sin \phi , \cos \theta)

where θ = π 3 \theta = \frac{\pi}{3} and ϕ = π 6 \phi = \frac{\pi}{6} . The unit vector in the direction of the steepest descent is given by,

u ^ 1 = ( cos θ cos ϕ , cos θ sin ϕ , sin θ ) \hat{u}_1 = ( \cos \theta \cos \phi, \cos \theta \sin \phi, -\sin \theta)

In addition, let

u ^ 2 = ( sin ϕ , cos ϕ , 0 ) \hat{u}_2 = ( -\sin \phi, \cos \phi, 0 )

Then the three unit vectors u ^ 1 , u ^ 2 \hat{u}_1 , \hat{u}_2 and n ^ \hat{n} make a right-handed reference frame.

The major axis of the ellipse makes an angle of ψ = π 6 \psi = \dfrac{\pi}{6} with u ^ 1 \hat{u}_1 . Thus, it is along the unit vector w ^ 1 \hat{w}_1 , and the minor axis is along w ^ 2 \hat{w}_2 , where

[ w ^ 1 , w ^ 2 ] = [ u ^ 1 , u ^ 2 ] R ( π 6 ) [ \hat{w}_1 , \hat{w}_2 ] = [ \hat{u}_1 , \hat{u}_2 ] R(\frac{\pi}{6})

and where,

R ( π 6 ) = [ cos π 6 sin π 6 sin π 6 cos π 6 ] R(\frac{\pi}{6}) = \begin{bmatrix} \cos \frac{\pi}{6} && -\sin \frac{\pi}{6} \\ \sin \frac{\pi}{6} && \cos \frac{\pi}{6} \end{bmatrix}

Now the points on the perimeter of the ellipse can be parameterized as:

r ( t ) = r C + a cos t w ^ 1 + b sin t w ^ 2 \vec{r}(t) = \vec{r_C} + a \cos t \hspace{4pt} \hat{w}_1 + b \sin t \hspace{4pt} \hat{w}_2

where a = 5 a = 5 is the semi-major axis length and b = 2 b = 2 is the semi-minor axis length, and where r C = ( x C , y C , z C ) \vec{r_C} = (x_C, y_C, z_C) is the position vector of the center of the ellipse. Tangency to the three coordinate planes implies that, for the x y xy plane, we're looking for t 1 [ 0 , 2 π ) t_1 \in [0, 2\pi ) , such that,

0 = z C + a cos t 1 w 1 z + b sin t 1 w 2 z 0 = z_C + a \cos t_1 \hspace{4pt} {w_{1z}} + b \sin t_1 \hspace{4pt} {w_{2z}}

We also require that d r d t \dfrac{d\vec{r}}{dt} has a zero z z -component at t = t 1 t=t_1 , that is,

0 = a sin t 1 w 1 z + b cos t 1 w 2 z 0 = -a \sin t_1 \hspace{4pt} {w_{1z}} + b \cos t_1 \hspace{4pt} {w_{2z}}

The last equation can be solved quite easily for two possible values of t 1 t_1 that are separated by π \pi .

To choose the correct one, we use the fact that z C z_C is positive, and after some trigonometry, we deduce that,

z C = a 2 w 1 z 2 + b 2 w 2 z 2 z_C = \sqrt{ a^2 {w_{1z}}^2 + b^2 {w_{2z}}^2 }

Similar formulas apply to x C x_C and y C y_C . Finally, to find the tangency point with the y z yz plane, we simply plug in

the value of t 3 t_3 into the parametric equation of the ellipse.

r = r C + a cos t 3 w ^ 1 + b sin t 3 w ^ 2 {\vec{r}}^* = \vec{r_C} + a \cos t_3 \hspace{4pt} \hat{w}_1 + b \sin t_3 \hspace{4pt} \hat{w}_2

where, a sin t 3 w 1 x + b cos t 3 w 2 x = 0 -a \sin t_3 \hspace{4pt} {w_{1x}} + b \cos t_3 \hspace{4pt} {w_{2x}} = 0

And this gives the required result, r = ( 0 , 3.19825 , 6.25493 ) {\vec{r}}^* = (0,3.19825, 6.25493) making the answer ( 3.19825 + 6.25493 ) = 9.45318 (3.19825+6.25493) = \boxed{9.45318}

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