A parabola in the x y plane is given by v = 4 1 u 2 , where the coordinates ( x , y ) are related to the ( u , v ) coordinates by
[ x y ] = R [ u v ] + [ 5 2 ]
and R is the 2 × 2 rotation matrix by 3 0 ∘ counter clockwise, i.e.
R = [ cos 3 0 ∘ sin 3 0 ∘ − sin 3 0 ∘ cos 3 0 ∘ ]
Now, you apply the following transformation to the points on the parabola.
If p is a point on the parabola, you define its image p ′ as follows:
p ′ = A p + b
where
A = [ 1 0 − 3 2 ] , b = [ 1 − 4 ]
Given that the image of the parabola is another parabola, find the vertex of the new parabola and the direction of its axis. Let r 0 = ( r 0 x , r 0 y ) be the vertex and u = ( cos θ , sin θ ) ( θ in radians, 0 ≤ θ < 2 π ) be the unit vector along the axis pointing in the direction that the parabola opens up. Further, and just as important, by attaching a suitable reference coordinate frame O ′ x ′ y ′ to the new parabola, where O ′ is at the vertex, its equation can be written as
y ′ = a x ′ 2
with a > 0
Find 4 ( r 0 x − r 0 y ) + θ + a
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Here's an outline of one possible solution method that depends on parametric equations.
The coordinate vector in the u v reference frame is given parametrically by ( t , 4 1 t 2 ) = t ( 1 , 0 ) + t 2 ( 0 , 4 1 )
Hence the coordinate vector in the x y plane is given by
p = ( x , y ) = R ( u , v ) + ( 5 , 2 ) = R ( t ( 1 , 0 ) + t 2 ( 0 , 4 1 ) ) + ( 5 , 2 )
Note that ordered pairs are actually 2 × 1 column vectors. Next apply the transformation to obtain
p ′ = A p + b = A ( t R ( 1 , 0 ) + t 2 R ( 0 , 4 1 ) + ( 5 , 2 ) ) + b
and this can be written as
p ′ = v 0 + v 1 t + v 2 t 2 ( 1 ) ,
with v 0 = A ( 5 , 2 ) + b , v 1 = A R ( 1 , 0 ) , v 2 = A R ( 0 , 4 1 )
Equation ( 1 ) can be written as
p ′ = u 0 + c 1 u 1 ( t + t 0 ) + c 2 u 2 ( t + t 0 ) 2 ( 2 )
where u 1 and u 2 are unit vectors and mutually perpendicular to each other.
Expanding ( 2 ) and equating similar terms, results in,
v 0 = u 0 + c 1 u 1 t 0 + c 2 u 2 t 0 2 ( 3 )
v 1 = c 1 u 1 + 2 c 2 u 2 t 0 ( 4 )
v 2 = c 2 u 2 ( 5 )
Equation ( 5 ) determines u 2 and c 2 , as c 2 = ∣ v 2 ∣ , and u 2 = v 2 / c 2
This also determines u 1 as a unit vector that is perpendicular to u 2 .
Next, from equation ( 4 ) , by dot multiplying both sides with u 1 , we obtain
v 1 ⋅ u 1 = c 1
and by dot multiplying both sides with u 2 , we obtain
v 1 ⋅ u 2 = 2 c 2 t 0
hence c 1 and t 0 are now determined. Finally u 0 can be computed from equation ( 3 ) .
The vertex is u 0 , θ is the angle of u 2 , and a = c 1 2 c 2
Performing these calculations gives us r 0 = u 0 = ( 0 . 1 0 5 3 2 8 2 3 9 , − 0 . 4 3 7 6 8 9 2 8 6 ) , u 2 = ( − 0 . 8 7 2 8 5 0 7 3 4 , 0 . 4 8 7 9 8 7 2 9 1 ) , and a = 2 . 7 9 4 7 0 7 5 2 5
Hence, θ = 2 . 6 3 1 8 1 0 2 9 4 , and 4 ( r 0 x − r 0 y ) + θ + a = 7 . 5 9 8 5 8 7 9 1 9 ≈ 7 . 5 9 8 6