An elliptical disc has a semi-major axis length of 5 and a semi-minor axis length of 2 . It is pushed against the corner of the first octant (where x ≥ 0 , y ≥ 0 and z ≥ 0 ). The elliptical disc cannot penetrate the coordinate planes (the x y , x z , and y z planes), and can only be tangent to them. In its final position, the unit normal to its plane is given by ( sin 3 π cos 6 π , sin 3 π sin 6 π , cos 3 π ) . The elliptical disc is oriented in such a way that its major axis makes an angle of + 6 π (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 ) is the tangency point with the y z plane, then find a + b .
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The unit normal specified by the problem is
n ^ = ( sin θ cos ϕ , sin θ sin ϕ , cos θ )
where θ = 3 π and ϕ = 6 π . 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 )
In addition, let
u ^ 2 = ( − sin ϕ , cos ϕ , 0 )
Then the three unit vectors u ^ 1 , u ^ 2 and n ^ make a right-handed reference frame.
The major axis of the ellipse makes an angle of ψ = 6 π with u ^ 1 . Thus, it is along the unit vector w ^ 1 , and the minor axis is along w ^ 2 , where
[ w ^ 1 , w ^ 2 ] = [ u ^ 1 , u ^ 2 ] R ( 6 π )
and where,
R ( 6 π ) = [ cos 6 π sin 6 π − sin 6 π cos 6 π ]
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
where a = 5 is the semi-major axis length and b = 2 is the semi-minor axis length, and where 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 plane, we're looking for t 1 ∈ [ 0 , 2 π ) , such that,
0 = z C + a cos t 1 w 1 z + b sin t 1 w 2 z
We also require that d t d r has a zero z -component at t = t 1 , that is,
0 = − a sin t 1 w 1 z + b cos t 1 w 2 z
The last equation can be solved quite easily for two possible values of t 1 that are separated by π .
To choose the correct one, we use the fact that 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
Similar formulas apply to x C and y C . Finally, to find the tangency point with the y z plane, we simply plug in
the value of t 3 into the parametric equation of the ellipse.
r ∗ = r C + a cos t 3 w ^ 1 + b sin t 3 w ^ 2
where, − a sin t 3 w 1 x + b cos t 3 w 2 x = 0
And this gives the required result, r ∗ = ( 0 , 3 . 1 9 8 2 5 , 6 . 2 5 4 9 3 ) making the answer ( 3 . 1 9 8 2 5 + 6 . 2 5 4 9 3 ) = 9 . 4 5 3 1 8
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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 , x z , and y z planes:
Since the unit normal vector to the plane of the disc is ( sin 3 π cos 6 π , sin 3 π sin 6 π , cos 3 π ) = ( 4 3 , 4 3 , 2 1 ) , the equation of the plane is 4 3 x + 4 3 y + 2 1 z = d , and its x -, y -, and z -intercepts ( A , B , and C ) solve to ( 3 4 d , 0 , 0 ) , ( 0 , 3 4 d , 0 ) , and ( 0 , 0 , 2 d ) , which by Pythagorean's Theorem makes the sides of the triangle 3 8 d , 3 2 2 1 d , and 3 2 1 3 d .
Now move △ A B C to a Cartesian coordinate system with A at ( 0 , 0 ) and B at ( 3 8 d , 0 ) :
C is 3 2 1 3 d away from A so by the distance formula C x 2 + C y 2 = 3 2 1 3 d , and C is 3 2 2 1 d away from B so ( C x − 3 8 d ) 2 + C y 2 = 3 2 2 1 d , and this solves to ( C x , C y ) = ( 3 2 d , 3 4 d ) . This means the equation of the line A C is y = 2 3 x and the equation of the line B C is y = − 3 2 ( x − 3 8 d ) .
The steepest descent of the plane is the altitude of △ A B C , so the ellipse is rotated 6 π counterclockwise from the vertical. Since the semi-major axis is 5 and the semi-minor axis is 2 , the equation of the ellipse before the rotation is 4 ( x − h ) 2 + 2 5 ( y − k ) 2 = 1 for center ( h , k ) , and is 4 0 0 7 9 ( x − h ) 2 + 2 0 0 2 1 3 ( x − h ) ( y − k ) + 4 0 0 3 7 ( y − k ) 2 = 1 after the rotation. Using implicit differentiation, the slope at any point on the ellipse solves to m = 2 1 3 ( x − h ) + 3 7 ( y − k ) − 7 9 ( x − h ) − 2 1 3 ( y − k ) .
The ellipse is tangent to y = 0 which has a slope of m = 0 at y = 0 . Then 4 0 0 7 9 ( x − h ) 2 + 2 0 0 2 1 3 ( x − h ) ( y − k ) + 4 0 0 3 7 ( y − k ) 2 = 1 and m = 2 1 3 ( x − h ) + 3 7 ( y − k ) − 7 9 ( x − h ) − 2 1 3 ( y − k ) with m = 0 and y = 0 solves to k = 2 7 9 .
The ellipse is also tangent to y = 2 3 x which has a slope of m = 2 3 . Then 4 0 0 7 9 ( x − h ) 2 + 2 0 0 2 1 3 ( x − h ) ( y − k ) + 4 0 0 3 7 ( y − k ) 2 = 1 and m = 2 1 3 ( x − h ) + 3 7 ( y − k ) − 7 9 ( x − h ) − 2 1 3 ( y − k ) with k = 2 7 9 , m = 2 3 , and y = 2 3 x solves to h = 1 2 1 ( 5 9 3 + 2 3 7 ) .
The ellipse is also tangent to y = − 3 2 ( x − 3 8 d ) which has a slope of m = − 3 2 at T . Then 4 0 0 7 9 ( x − h ) 2 + 2 0 0 2 1 3 ( x − h ) ( y − k ) + 4 0 0 3 7 ( y − k ) 2 = 1 and m = 2 1 3 ( x − h ) + 3 7 ( y − k ) − 7 9 ( x − h ) − 2 1 3 ( y − k ) with k = 2 7 9 , h = 1 2 1 ( 5 9 3 + 2 3 7 ) , m = − 3 2 and y = − 3 2 ( x − 3 8 d ) solves to x = T x = 2 3 1 1 + 1 2 5 9 3 + 1 2 2 3 7 , y = T y = 2 1 3 3 3 7 3 + 2 7 9 , and d = 3 2 1 ( 5 9 3 + 3 1 3 3 + 4 2 3 7 ) . We now know the coordinates of B are ( 1 2 1 ( 5 9 3 + 3 1 3 3 + 4 2 3 7 ) , 0 ) , and by the distance formula, B T 2 = 1 5 2 1 ( 7 3 0 7 + 3 7 3 1 5 2 1 ) .
Moving back to the three-dimensional picture, the equation of the line B C is z = 2 3 y + 2 d . Since T is on B C , T z = 2 3 T y + 2 d and by the distance formula ( T y − 3 4 d ) 2 + T z 2 = B T 2 , and since d = 3 2 1 ( 5 9 3 + 3 1 3 3 + 4 2 3 7 ) and B T 2 = 1 5 2 1 ( 7 3 0 7 + 3 7 3 1 5 2 1 ) , this solves numerically to ( T y , T z ) ≈ ( 3 . 1 9 8 , 6 . 2 5 5 ) .
Therefore, a = T y ≈ 3 . 1 9 8 and b = T z ≈ 6 . 2 5 5 , and a + b ≈ 3 . 1 9 3 + 6 . 2 5 5 ≈ 9 . 4 5 3 .