The polar coordinates description of an ellipse is given by:
r ( θ ) = 5 + 3 cos θ + 2 sin θ 1
Find the sum of its semi-major and semi-minor axes lengths.
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Since r = 5 + 1 3 cos ( θ + α ) 1 for some angle α , we see that 1 2 1 ( 5 − 1 3 ) = ( 5 + 1 3 ) − 1 ≤ r ≤ ( 5 − 1 3 ) − 1 = 1 2 1 ( 5 + 1 3 ) . Since the maximum and minimum distances from the focus of an elliptical orbit are a ( 1 + e ) and a ( 1 − e ) , we deduce that a = 1 2 5 and a e = 1 2 1 1 3 . Thus e = 5 1 3 and hence b = 1 2 1 , so a + b = 1 2 1 ( 5 + 1 2 ) = 0 . 7 0 5 3 4 1 8 0 1 3 .
Polar equation of an ellipse is
r ( θ ) = 1 + e cos θ l ,
where l = a b 2 = semi latus rectum,
e = 1 − a 2 b 2 = eccentricity,
a , b are the semi-major and the semi-minor axes of the ellipse respectively.
Here
r ( θ ) = 5 + 3 cos θ + 2 sin θ 1
= 1 + 5 1 3 cos ( θ − tan − 1 3 2 ) 5 1
So, l = a b 2 = 5 1 ,
e = 1 − a 2 b 2 = 5 1 3
Solving we get a = 1 2 5 ,
b = 1 2 1 , and
a + b = 1 2 5 + 1 2 ≈
7 0 5 3 4 1 8
We're given that,
r = a + b cos θ + c sin θ 1
From the definition of polar coordinates, we have the polar-to-rectangular coordinates relation
x = r cos θ , y = r sin θ ( 1 ) .
First, we'll eliminate having to deal with three constants a, b, c , by combining b cos θ and c sin θ into one θ -shifted sinusoid. If ϕ = Arctan2 ( b , c ) , then,
r = a + b ′ cos ( θ − ϕ ) 1
where b ′ = b 2 + c 2 . Rotating our x -axis to θ = ϕ , the equation becomes,
r = a + b ′ cos θ 1 ( 2 )
In the following, we will replace b ′ with b , for simplicity of notation.
Using ( 1 ) and ( 2 ) , we get,
x ( a + b cos θ ) = cos θ ( 3 . 1 )
y ( a + b cos θ ) = sin θ ( 3 . 2 )
Equations ( 3 ) are a linear system in cos θ and sin θ , and if we define
u = [ cos θ sin θ ]
then, this linear system can be written as A u = B , where
A = [ ( x b − 1 ) y b 0 − 1 ]
and
B = [ − x a − y a ]
Solving, we get,
cos θ = 1 − b x a x and sin θ = 1 − b x a y
Now since cos 2 θ + sin 2 θ = 1 , then,
( a x ) 2 + ( a y ) 2 = ( 1 − b x ) 2
→ a 2 ( x 2 + y 2 ) = 1 + b 2 x 2 − 2 b x
→ ( a 2 − b 2 ) x 2 + a 2 y 2 − 2 b x = 1
Completing the square in x , we obtain,
( a 2 − b 2 ) ( x − a 2 − b 2 b ) 2 + a 2 y = 1 + a 2 − b 2 b 2 = a 2 − b 2 a 2
Dividing by the right hand side,
a 2 ( a 2 − b 2 ) 2 ( x − x 0 ) 2 + ( a 2 − b 2 ) y 2 = 1 ( 4 )
where x 0 = a 2 − b 2 b
From equation (4) , it is evident that the semi-major axis is given by a 2 − b 2 a and the semi-minor axis is given by a 2 − b 2 1 .
In this problem a = 5 , b = 3 , c = 2 , so our b ′ = 1 3 which we replaced with b .
Hence the semi-major axis = 2 5 − 1 3 5 = 1 2 5 , and the semi-minor axis is 1 2 1 . Their sum comes to ≈ 0 . 7 0 5 3 .
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Let A cos ( θ + ϕ ) = 3 cos θ + 2 sin θ . Expanding and solving gives A = 1 3 and ϕ = − arccos 1 3 3 , so r = 5 + 1 3 cos ( θ − ϕ ) 1 Let's rotate the entire ellipse by removing ϕ to simplify this equation. This does not affect the shape of the ellipse. r = 5 + 1 3 cos ( θ ) 1 5 r + 1 3 r cos ( θ ) = 1 2 5 r 2 = ( 1 − 1 3 r cos ( θ ) ) 2 Now we convert to Cartesian coordinates with r 2 = x 2 + y 2 and r cos θ = x 2 5 x 2 + 2 5 y 2 = ( 1 − 1 3 x ) 2 Expanding and completing the square for the x terms gives 1 2 ( x + 1 2 1 3 ) 2 + 2 5 y 2 = 1 2 2 5 Let's translate the entire ellipse in the x direction by removing 1 2 1 3 . This does not affect the shape of the ellipse. 1 2 x 2 + 2 5 y 2 = 1 2 2 5 2 5 1 4 4 x 2 + 1 2 y 2 = 1 This is the equation of an ellipse with semi-major axis 1 4 4 2 5 = 1 2 5 and semi-minor axis 1 2 1 , so the answer is 1 2 5 + 1 2 1 ≈ 0 . 7 0 5 3