An ellipsoid is pushed against the corner of the first octant (where and ). The ellipsoid cannot penetrate the coordinate planes (the , , and planes), and can only be tangent to them. It is oriented such that its first semi-axis which has a length of is along the vector , and its second semi-axis which is of length is along the vector , and the third semi-axis, of length is along the vector .
There are three tangency points with the three coordinate planes. If is the tangency point with the plane, then find .
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The parametric equation (vector equation) of points on the ellipsoid surface is
r ( θ , ϕ ) = r C + V u ( θ , ϕ )
where r C = ( x C , y C , z C ) is the position vector of the center of the ellipsoid. And the 3 × 3 matrix V is given by
V = [ v 1 , v 2 , v 3 ] = R D , with R being an orthogonal matrix whose columns are the unit vectors of three axes of the ellipsoid, and D is a diagonal matrix of the semi-axes lengths. Finally, the unit vector u ( θ , ϕ ) is specified as
u ( θ , ϕ ) = ( sin θ cos ϕ , sin θ sin ϕ , cos θ )
At the three tangency points, one of the coordinates vanishes, and the same coordinate of the derivatives of r ( θ , ϕ )
with respect to θ and to ϕ vanishes as well.
Let's take the tangent point with the x y plane. We know that at that point we'll have,
z C + v 1 z sin θ 1 cos ϕ 1 + v 2 z sin θ 1 sin ϕ 1 + v 3 z cos θ 1 = 0
In addition, by differentiating r with respect to θ and ϕ and setting the z -component to zero,
we obtain two more equations,
v 1 z cos θ 1 cos ϕ 1 + v 2 z cos θ 1 sin ϕ 1 − v 3 z sin θ 1 = 0
and
− v 1 z sin θ 1 sin ϕ 1 + v 2 z sin θ 1 cos ϕ 1 = 0
Now in the last equation, sin θ 1 = 0 is extraneous and can be ignored, and therefore we can divide by it, resulting in
− v 1 z sin ϕ 1 + v 2 z cos ϕ 1 = 0
And this can be solved for ϕ 1 , resulting in,
cos ϕ 1 = − v 1 z 2 + v 2 z 2 v 1 z and
sin ϕ 1 = − v 1 z 2 + v 2 z 2 v 2 z
Plugging in the angle ϕ 1 in the previous equation, we can now solve for θ 1 , in a similar fashion, and
the result is that,
cos θ 1 = − v 1 z 2 + v 2 z 2 + v 3 z 2 v 3 z
sin θ 1 = v 1 z 2 + v 2 z 2 + v 3 z 2 v 1 z 2 + v 2 z 2
The choice of signs for cos ϕ 1 , sin ϕ 1 , cos θ 1 and sin θ 1 guarantees that θ 1 ∈ [ 0 , π ] on the one hand, and also that the z -coordinate of the tangency point (which is 0) is as far as possible from z C (which is positive) for any values of v 1 z , v 2 z and v 3 z .
Plugging both θ 1 and ϕ 1 into the first equation, results in
z C = v 1 z 2 + v 2 z 2 + v 3 z 2
Similarly, we have,
x C = v 1 x 2 + v 2 x 2 + v 3 x 2
and
y C = v 1 y 2 + v 2 y 2 + v 3 y 2
So far we have found the center of the ellipsoid, and expressions for the angles θ and ϕ at the tangency point.
Now for the tangency point at the y z plane, we have the following,
cos ϕ 3 = − v 1 x 2 + v 2 x 2 v 1 x and
sin ϕ 3 = − v 1 x 2 + v 2 x 2 v 2 x
and
cos θ 3 = − v 1 x 2 + v 2 x 2 + v 3 x 2 v 3 x
sin θ 3 = v 1 x 2 + v 2 x 2 + v 3 x 2 v 1 x 2 + v 2 x 2
Using these values, we can find r ( θ 3 , ϕ 3 ) using the parametric representation of the ellipsoid. And the result is r ∗ = ( 0 , 2 . 8 5 5 1 6 6 , 6 . 5 3 1 7 5 1 ) , making the answer ( 2 . 8 5 5 1 6 6 + 6 . 5 3 1 7 5 1 ) = 9 . 3 8 6 9 1 7
Another approach to this problem is to consider the algebraic equation of the ellipsoid instead of the vector equation.
The algebraic equation of ellipsoid is given by,
( r − r C ) T R D R T ( r − r C ) = 1
where the matrix R is as before, but the diagonal matrix D = diag { a 2 1 , b 2 1 , c 2 1 } , where a , b and c are the semi-axes lengths. The gradient of the above expression (the normal to the surface) is given by,
∇ = 2 R D R T ( r − r C )
Let r 1 be the tangency point with the x y plane, then at that point the gradient is pointing in the opposite direction of k (the unit vector along the positive z axis ). Hence, there exist a positive constant α , such that,
R D R T ( r 1 − r C ) = − α k
and this implies that,
r 1 − r C = − α R D − 1 R T k ( ∗ )
Substituting this expression into the algebraic equation of the ellipsoid, and solving for α , we get,
α = k T R D − 1 R T k 1
Since the z coordinate of r 1 = 0 , it follows that, by pre-multiplying both sides of equation ( ∗ ) by k T ,
z C = α k T R D − 1 R T k = k T R D − 1 R T k
and similarly,
x C = i T R D − 1 R T i
y C = j T R D − 1 R T j
where i and j are the unit vector along the positive x and y axes. Thus we have determined r C
And using equation ( ∗ ) and its variations, we can obtain expressions for the three tangent points r 1 with the x y plane , r 2 , with the x z plane, and r 3 with the y z plane, and they are as follows,
r 1 = r C − k T R D − 1 R T k R D − 1 R T k
r 2 = r C − j T R D − 1 R T j R D − 1 R T j
r 3 = r C − i T R D − 1 R T i R D − 1 R T i