Animated Solution for Mathematics - Conic Sections: If the normal at an end of a latus rectum of an ellipse passes through an extremity of the minor axis, then the eccentricity e of the ellipse satisfies :
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Visualized Solution
Define the Ellipse and Key Points
Standard Ellipse: a2x2+b2y2=1
End of Latus Rectum (L): (ae,ab2)
Extremity of Minor Axis (B′): (0,−b)
Equation of the Normal
General Normal Equation at (x1,y1):
x1a2x−y1b2y=a2−b2
Substitution of Point L
Substitute x1=ae and y1=ab2:
aea2x−b2/ab2y=a2−b2
Simplifying the Normal Equation
Cancel out common terms:
eax−ay=a2−b2
Applying the Given Condition
The normal passes through B′(0,−b).
Substitute x=0 and y=−b.
Substituting B′ into Normal
ea(0)−a(−b)=a2−b2
Simplifying the Relation
0+ab=a2−b2
Result: ab=a2−b2
Relating to Eccentricity
We need an equation in terms of e.
Recall the eccentricity formula: b2=a2(1−e2)
Rearranged: a2b2=1−e2
Dividing by a2
Divide ab=a2−b2 by a2:
a2ab=a2a2−a2b2
ab=1−a2b2
Substituting Eccentricity
Substitute a2b2=1−e2
And ab=1−e2
Equation becomes: 1−e2=e2
Squaring Both Sides
Square both sides to remove the radical:
(1−e2)2=(e2)2
1−e2=e4
Final Polynomial Equation
Rearrange 1−e2=e4:
e4+e2−1=0
This is the required condition for the eccentricity.
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The Sigma Insight: Equation of Tangent and Normal
Solution Diagram
Analyzing the Setup
We define our arena using the standard ellipse equation:
a2x2+b2y2=1
The latus rectum is a vertical line at x=ae. The upper end of this latus rectum, denoted as L, has the coordinates:
L=(ae,ab2)
We also identify the extremity of the minor axis, B′, which is located at (0,−b). These points serve as our geometric anchors.
The Normal as a Scalpel
To construct the normal at point L, we utilize the general equation of the normal to an ellipse at any point (x1,y1):
x1a2x−y1b2y=a2−b2
Substituting our point L(ae,ab2) into this equation, where x1=ae and y1=ab2, we obtain:
aea2x−b2/ab2y=a2−b2
Simplifying the terms, the expression reduces to:
eax−ay=a2−b2
The Intersection
The problem states that this normal line passes through the extremity of the minor axis, B′(0,−b). Therefore, the point (0,−b) must satisfy the equation of the normal.
Substituting x=0 and y=−b into the normal equation:
ea(0)−a(−b)=a2−b2
This simplifies to the elegant relation:
ab=a2−b2
The Bridge to Eccentricity
We recall the fundamental identity for an ellipse, b2=a2(1−e2), which implies a2b2=1−e2. Dividing our relation ab=a2−b2 by a2, we get:
ab=1−a2b2
Substituting ab=1−e2 and a2b2=1−e2 into the equation, we obtain:
1−e2=1−(1−e2)=e2
Squaring both sides to eliminate the radical yields 1−e2=e4. Rearranging the terms, we arrive at the final condition: