Animated Solution for Mathematics - Conic Sections: Let d be the perpendicular distance from the centre of the ellipse a2x2+b2y2=1 to the tangent drawn at a point P on the ellipse. If F1 and F2 are the two foci of the ellipse, then show that (PF1−PF2)2=4a2(1−d2b2).
Visualized Solution
The Ellipse and its Foci
Standard ellipse: a2x2+b2y2=1
Foci are located at F1(−ae,0) and F2(ae,0)
Here, e is the eccentricity: e2=1−a2b2
Point P and the Tangent
Let P be any point on the ellipse.
Parametric coordinates of P: (acosθ,bsinθ)
A tangent line is drawn passing through P.
Equation of the Tangent
Using the point of contact form, the tangent equation is:
axcosθ+bysinθ=1
This represents a straight line in the form Ax+By+C=0.
The Perpendicular Distance d
d is the perpendicular distance from the center (0,0) to the tangent.
Formula: Distance from origin to Ax+By+C=0 is A2+B2∣C∣
Calculating d21
Substituting A=acosθ, B=bsinθ, C=−1:
d=a2cos2θ+b2sin2θ∣−1∣
Squaring and inverting gives:
d21=a2cos2θ+b2sin2θ
Focal Distances PF1 and PF2
The distances from point P to the foci are called focal distances.
Standard formulas in terms of eccentricity e:
PF1=a+exP
PF2=a−exP
Substituting xP=acosθ
Since xP=acosθ, we substitute this into the focal distances:
PF1=a+aecosθ=a(1+ecosθ)
PF2=a−aecosθ=a(1−ecosθ)
Difference of Focal Distances
We need to find the difference PF1−PF2:
PF1−PF2=a(1+ecosθ)−a(1−ecosθ)
PF1−PF2=2aecosθ
Evaluating the Left Hand Side (LHS)
The Left Hand Side of our target equation is (PF1−PF2)2.
Squaring our result:
LHS=(2aecosθ)2
LHS=4a2e2cos2θ
Evaluating the Right Hand Side (RHS)
The Right Hand Side is 4a2(1−d2b2).
Let's focus on the term d2b2.
Using our earlier result for d21:
d2b2=b2(a2cos2θ+b2sin2θ)
Simplifying d2b2
Distributing b2 inside the bracket:
d2b2=a2b2cos2θ+b2b2sin2θ
d2b2=a2b2cos2θ+sin2θ
Calculating 1−d2b2
Substitute this back into the bracket:
1−d2b2=1−(a2b2cos2θ+sin2θ)
Grouping terms:
=(1−sin2θ)−a2b2cos2θ
Using Trigonometric Identity
We know the fundamental identity: 1−sin2θ=cos2θ
Substituting this in:
=cos2θ−a2b2cos2θ
Factoring out cos2θ:
=cos2θ(1−a2b2)
Connecting with Eccentricity
Recall the eccentricity formula for an ellipse: e2=1−a2b2
Therefore, the expression becomes:
1−d2b2=e2cos2θ
Finalizing the Proof
Multiply by 4a2 to get the full RHS:
RHS=4a2(e2cos2θ)=4a2e2cos2θ
Comparing with our earlier result:
LHS=4a2e2cos2θ
Hence, LHS=RHS. Proved!
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The Sigma Insight: Equation of Tangent and Normal
Solution Diagram
The Elegance of the Ellipse
A Geometric Journey
Imagine you are standing at the center of an ellipse, looking out at a point P dancing along its perimeter. This isn't just a curve; it is a perfect balance of geometry and algebra.
Today, we are going to unravel a beautiful relationship involving the tangent at P and the two foci, F1 and F2. Let's take a breath and walk through this derivation together.
Phase 1
Setting the Stage
We begin with the standard ellipse equation:
a2x2+b2y2=1
The foci, F1(−ae,0) and F2(ae,0), are the heart of this shape. To make our journey easier, we choose a point P on the ellipse using parametric coordinates: P(acosθ,bsinθ).
These coordinates automatically satisfy the ellipse equation, saving us from algebraic nightmares later. Using the point-of-contact form, the equation of the tangent line at P is:
axcosθ+bysinθ=1
Phase 2
The Perpendicular Distance
The problem introduces d, the perpendicular distance from the center (0,0) to this tangent. Using the standard formula for the distance from the origin to a line Ax+By+C=0, which is A2+B2∣C∣, we find:
d=a2cos2θ+b2sin2θ∣−1∣
Squaring and inverting this gives us a powerful tool:
d21=a2cos2θ+b2sin2θ
Phase 3
The Focal Distances
Now, let's look at the focal distances, PF1 and PF2. A fundamental property of the ellipse tells us that PF1=a+exP and PF2=a−exP.
Since our xP=acosθ, these become PF1=a(1+ecosθ) and PF2=a(1−ecosθ). When we subtract these, the a terms vanish:
PF1−PF2=2aecosθ
Squaring this gives us our Left Hand Side (LHS):
(PF1−PF2)2=4a2e2cos2θ
Phase 4
The Grand Unification
Now, let's tackle the Right Hand Side (RHS): 4a2(1−d2b2). We first evaluate d2b2 using our earlier expression:
d2b2=b2(a2cos2θ+b2sin2θ)=a2b2cos2θ+sin2θ
Substitute this into the RHS expression:
1−(a2b2cos2θ+sin2θ)=(1−sin2θ)−a2b2cos2θ
Using the identity 1−sin2θ=cos2θ, this simplifies to cos2θ(1−a2b2). Since e2=1−a2b2, the expression becomes e2cos2θ.
Multiplying by 4a2, we obtain 4a2e2cos2θ. The LHS and RHS match perfectly, confirming the identity: