Two ellipses have the equations
7 x 2 + 8 x y + 1 3 y 2 − 3 6 x − 4 2 y − 4 3 = 0
(drawn in blue), and
3 3 x 2 − 2 8 x y + 1 2 y 2 − 1 0 4 x + 3 2 y − 1 3 7 = 0
(drawn in orange). Find the area of the region that is common to both ellipses (shaded in light green). If this area is A , then enter ⌊ 1 0 0 0 A ⌋ as your answer.
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I will take advantage of the graph provided to get a much simpler solution.
Rotate the ellipses with respect to their center ( 2 , 1 ) so that the coordinates of the intersection points are ( ± 5 , ± 5 ) . In these rotated axes centered at ( 2 , 1 ) the ellipses have equations of the form a 2 x 2 + b 2 y 2 = 1 where the major semi-axis a of each one is read from the graph and b can be calculated substituting one of the intersection points. After little manipulation, the ellipses become:
The square has an area of 2 0 . We just need to calculate the extra area limited by the sides of the square and the four arches.
We get integrals of the form ∫ − x 0 x 0 a 2 − x 2 d x which are quite straightforward to solve using the variable change x = a sin θ , d x = a cos θ d θ :
∫ − x 0 x 0 a 2 − x 2 d x = 2 × ∫ 0 arcsin ( a x 0 ) cos 2 θ d θ = 2 × ∫ 0 arcsin ( a x 0 ) cos 2 θ d θ = 2 × ∫ 0 arcsin ( a x 0 ) 2 1 + 2 1 cos 2 θ d θ = [ θ + 2 1 sin 2 θ ] 0 arcsin ( a x 0 )
Using x 0 = 5 and the values of a for each ellipse we obtain:
The total area is A = A s q u a r e + 2 × A b l u e + 2 × A o r a n g e ≈ 2 2 . 9 0 5 5 4 0 ⟹ ⌊ 1 0 0 0 A ⌋ = 2 2 9 0 5
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 |
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The given equation of the first ellipse can be written using matrices as
r T A r + b T r + c = 0 ( 1 )
where
r = [ x y ] T
A = [ 7 4 4 1 3 ]
b T = [ − 3 6 − 4 2 ]
c = − 4 3
The first step is to find the center of this ellipse. It is given by
r 0 = − 2 1 A − 1 b ( 2 )
One can verify that equation (1) be re-written as,
( r − r 0 ) T A ( r − r 0 ) = − c + r 0 T A r 0 ( 3 )
Define the matrix Q as follows
Q = − c + r 0 T A r 0 A ( 4 )
then, from equation (3) and (4), we obtain
( r − r 0 ) T Q ( r − r 0 ) = 1 ( 5 )
The next step is to diagonalize Q , and write it as Q = R D R T
The procedure is as follows,
Let θ = 2 1 tan − 1 Q 1 1 − Q 2 2 2 Q 1 2 ( 6 )
Then
R = [ cos θ sin θ − sin θ cos θ ] ( 7 )
and
D = diag { d 1 1 , d 2 2 } ( 8 . 1 )
with
d 1 1 = Q 1 1 cos 2 θ + Q 2 2 sin 2 θ + 2 Q 1 2 cos θ sin θ ( 8 . 2 )
d 2 2 = Q 1 1 sin 2 θ + Q 2 2 cos 2 θ − 2 Q 1 2 cos θ sin θ ( 8 . 3 )
Replacing matrix Q in equation (5) by its diagonalized form, we obtain
( r − r 0 ) T R D R T ( r − r 0 ) = 1 ( 9 )
For an ellipse, the diagonal matrix D has positive entries, and therefore can be factored as D = D 2 1 D 2 1
Using this factorization, and defining the vector
u = D 2 1 R T ( r − r 0 ) ( 1 0 )
then it follows that u T u = 1 , thus vector u is a unit vector, and can therefore be parameterized as u = [ cos t , sin t ] T .
Solving for r in terms of u gives,
r = r 0 + R D − 2 1 u = r 0 + V u ( 1 1 )
The columns of matrix V are vectors extending along the major and minor axes directions and having lengths of the semi-major
and semi-minor axes.
The same procedure can be applied to the second ellipse, and we'll end up with the following parametric equations for
the two ellipses,
r 1 ( t ) = r C 1 + V 1 u 1 ( t ) ( 1 2 . 1 )
r 2 ( s ) = r C 2 + V 2 u 2 ( s ) ( 1 2 . 2 )
Performing the calculations detailed above, the reader can verify that,
r C 1 = r C 2 = [ 2 1 ] T
V 1 = ⎣ ⎢ ⎡ 4 − 2 3 2 3 4 ⎦ ⎥ ⎤
V 2 = ⎣ ⎢ ⎡ 2 3 − 2 2 3 3 6 ⎦ ⎥ ⎤
We next have to find the points of intersection of the two ellipses, so we set up the equation,
r 1 ( t ) = r 2 ( s ) ⟹ r C 1 + V 1 u 1 ( t ) = r C 2 + V 2 u 2 ( s ) ( 1 3 )
Solving for u 1 ( t ) , we obtain,
u 1 ( t ) = V 1 − 1 ( r C 2 − r C 1 + V 2 u 2 ( s ) ) = e + F u 2 ( s ) ( 1 4 )
where e = V 1 − 1 ( r C 2 − r C 1 ) and F = V 1 − 1 V 2
Since u 1 is a unit vector, we have u 1 T u 1 = 1 , and this leads to,
( e + F u 2 ) T ( e + F u 2 ) = 1 ( 1 5 )
Expanding the left hand side of (15),
u 2 T F T F u 2 + 2 u 2 T F T e + e T e = 1 ( 1 6 )
For reference, let's define G = F T F , h = 2 F T e , q = e T e − 1 , then equation (16) can be written as,
u 2 T G u 2 + u 2 T h + q = 0 ( 1 7 )
Recall that u 2 = [ cos s , sin s ] T , thus expanding equation (17) yields,
G 1 1 cos 2 s + G 2 2 sin 2 s + 2 G 1 2 sin s cos s + h 1 cos s + h 2 sin s + q = 0 ( 1 8 )
Using the identities cos 2 s = 2 1 ( 1 + cos ( 2 s ) ) , and sin 2 s = 2 1 ( 1 − cos ( 2 s ) ) as well as 2 sin s cos s = sin ( 2 s ) , equation (18) becomes,
c 1 cos s + c 2 sin s + c 3 cos 2 s + c 4 sin 2 s + c 5 = 0 ( 1 9 )
where c 1 = h 1 , c 2 = h 2 , c 3 = 2 1 ( G 1 1 − G 2 2 ) , c 4 = G 1 2 , c 5 = q + 2 1 ( G 1 1 + G 2 2 )
After performing all the calculations above, equation (19) produces four solutions, and they are,
s 1 = 0 . 3 3 9 8 3 6 9 0 9 s 2 = 2 . 8 0 1 7 5 5 7 4 4 s 3 = 3 . 4 8 1 4 2 9 5 6 3 s 4 = 5 . 9 4 3 3 4 8 3 9 8
The corresponding values for parameter t of the first ellipse are,
t 1 = 1 . 0 4 7 1 9 7 5 5 1 t 2 = 2 . 0 9 4 3 9 5 1 0 2 t 3 = 4 . 1 8 8 7 9 0 2 0 5 t 4 = 5 . 2 3 5 9 8 7 7 5 6
The four solution for s (and also the four corresponding solutions of t ) correspond in turn to the Cartesian points:
P 1 = ( 5 , 2 ) , P 2 = ( 1 , 4 ) , P 3 = ( − 1 , 0 ) , P 4 = ( 3 , − 2 )
The region common to both ellipses is bounded by the first ellipse for t ∈ [ t 1 , t 2 ] and for t ∈ [ t 3 , t 4 ] and is bounded by the second ellipse for s ∈ [ s 2 , s 3 ] and for s ∈ [ s 4 , s 1 + 2 π ]
The area enclosed by the parametric curve r ( t ) = ( x ( t ) , y ( t ) ) whose t -derivative is r ′ ( t ) = ( x ′ ( t ) , y ′ ( t ) ) is given by the formula
Area = 2 1 ∣ ∣ ∣ ∣ ∫ t i t f x ( t ) y ′ ( t ) − x ′ ( t ) y ( t ) d t ∣ ∣ ∣ ∣ ( 2 0 )
If we extend the vector r ( t ) and its t -derivative into three dimensions, by padding our r ( t ) and r ′ ( t ) with a zero z coordinate, then the above integral can be written conveniently using cross product notation as,
Area = 2 1 ∣ ∣ ∣ ∣ ∫ t i t f ( r ( t ) × r ′ ( t ) ) z d t ∣ ∣ ∣ ∣ ( 2 1 )
where ( ⋅ ) z is the z coordinate of its vector argument. We have to use this formula four times corresponding to the four intervals that we have. Now let's see what this evaluation entails. We have
r ( t ) = r C + V u
If V = [ v 1 v 2 ] , where v 1 and v 2 are the columns of V , then we have,
r ( t ) = r C + v 1 cos t + v 2 sin t
and its t -derivative is,
r ′ ( t ) = − v 1 sin t + v 2 cos t
Hence,
r ( t ) × r ′ ( t ) = − ( r C × v 1 ) sin t + ( r C × v 2 ) cos t + ( v 1 × v 2 ) ( cos 2 t + sin 2 t )
which simplifies to,
r ( t ) × r ′ ( t ) = − ( r C × v 1 ) sin t + ( r C × v 2 ) cos t + v 1 × v 2
Evaluating the area integral over a given interval [ t i , t f ] yields,
A k = 2 1 ( ( r C × v 1 ) z ( cos t f − cos t i ) + ( r C × v 2 ) z ( sin t f − sin t i ) + ( v 1 × v 2 ) z ( t f − t i ) ) k = 1 , 2 , 3 , 4
In this particular problem, and since r C 1 = r C 2 we can shift the center of our parametric curves to the origin, and this simplifies the above formula into
A k = 2 1 ( v 1 × v 2 ) z ( t f − t i ) k = 1 , 2 , 3 , 4
From matrix V 1 and V 2 above, we have, for the first ellipse, ( v 1 × v 2 ) z = 3 2 0 , and for the second ellipse, ( v 1 × v 2 ) z = 2 2 4 5
Plugging in the t and s values we found, the area is given by,
Area = 2 1 ( 3 2 0 ( t 2 − t 1 + t 4 − t 3 ) + 2 2 4 5 ( s 3 − s 2 + s 1 + 2 π − s 4 ) )
This evaluates to, Area = A = 2 2 . 9 0 5 5 4 0 0 0 4 3 , and this makes the answer ⌊ 1 0 0 0 A ⌋ = 2 2 9 0 5 .
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Solving the two ellipse equations, the points of intersection are P ( 1 , 4 ) , Q ( 5 , 2 ) , R ( 3 , − 2 ) , and S ( − 1 , 0 ) .
Using the distance formula, the sides of quadrilateral P Q R S are P Q = Q R = R S = P R = 2 0 and the diagonals are P R = Q S = 4 0 , therefore P Q R S is a square with an area of A P Q R S = 2 0 .
The equation of the line with P Q is y = − 2 1 x + 2 9 and the equation of the line with P R is y = 2 x + 2 .
The equation of the upper part of the blue ellipse rearranges to y = 1 3 1 ( 5 − 3 x 2 + 1 2 x + 4 0 − 4 x + 2 1 ) , and the equation of the upper part of the orange ellipse rearranges to y = 6 1 ( 5 − 2 x 2 + 8 x + 1 9 + 7 x − 8 ) .
The area of the section between the blue ellipse and P Q is then A P Q = ∫ 1 5 ( ( 1 3 1 ( 5 − 3 x 2 + 1 2 x + 4 0 − 4 x + 2 1 ) ) − ( − 2 1 x + 2 9 ) ) d x , and the area of the section between the orange ellipse and P R is A P R = ∫ − 1 1 ( ( 6 1 ( 5 − 2 x 2 + 8 x + 1 9 + 7 x − 8 ) ) − ( 2 x + 2 ) ) d x .
By symmetry, A R S = A P Q and A Q R = A P R , so the total shaded area is A = 2 A P Q + 2 A P R + A P Q R S ≈ 2 2 . 9 0 5 5 , which makes ⌊ 1 0 0 0 A ⌋ = 2 2 9 0 5 .