Sigma Percentile
JEE Advanced 1991
LEVELJEE Main

Animated Solution for Mathematics - Conic Sections: Three normals are drawn from the point to the curve . Show that must be greater than . One normal is always the x-axis. Find for which the other two normals are perpendicular to each other.

Enter Numerical Value:

Visualized Solution

Visualizing the Parabola and Point

  • Given curve:
  • Point on the x-axis:
  • Goal: Find condition for three distinct normals and specific for perpendicularity.

General Equation of a Normal

  • For a standard parabola , the normal in slope form is:

Finding the value of

  • Comparing our curve with

Substituting into the Normal Equation

  • Substitute into the normal equation:

Passing the Normal through

  • The normal passes through the given point .
  • Substitute and :

Factorizing the Equation

  • Rearrange and factor out :

The First Normal (The x-axis)

  • Case 1:
  • Substitute into the normal equation:
  • This proves one normal is always the x-axis.

Condition for the Other Two Normals

  • Case 2:
  • Rearranging for :

Proving

  • For three distinct normals, we need two more real, non-zero values for .
  • Therefore,

The Perpendicularity Condition

  • Let the slopes of the other two normals be and .
  • Condition for them to be perpendicular:

Using the Product of Roots

  • From , the equation is
  • This is a quadratic in :
  • Product of roots () =

Solving for

  • Equate the product of roots to :

The Sigma Insight: Equation of Tangent and Normal

Solution Diagram

Analyzing the Setup

Imagine you are standing at the vertex of a perfectly smooth, reflective parabolic mirror defined by the equation . You are holding a laser pointer at a point on the axis of symmetry.
You want to fire beams that hit the parabola such that they strike it 'normally'—meaning they hit the surface at a perfect 90-degree angle. We aim to determine how many such beams can be fired and the condition under which two of those beams are perpendicular to each other.

The Universal Language of Parabolas

To solve this, we first need to speak the language of parabolas. While our curve is , the standard form is our most powerful tool.
By comparing the two, we immediately see that , which gives us the focal parameter . This is the heartbeat of the parabola; it dictates how 'wide' or 'narrow' the curve opens.
Now, we invoke the general equation of a normal to a parabola in slope form: . This equation is a masterpiece of coordinate geometry.
Substituting our value of , the equation simplifies to:

The Point of Intersection

We are firing our normals from the point . This means that for any normal we draw, the coordinates must satisfy the equation of that line.
Plugging these into our equation, we get:
If we factor out , we are left with a beautiful cubic structure:
This equation is the key to the entire mystery. It tells us that there are three possible slopes for our normals. The first solution is , which corresponds to the x-axis itself, confirming that the axis of symmetry is always a normal to the parabola.

The Threshold of Existence

But what about the other two normals? They come from the quadratic part: .
Rearranging this, we find . For these two normals to actually exist as real lines, must be positive.
This forces the condition , or simply . If were less than , the normals would vanish into the realm of imaginary numbers. We have just proven that to see three distinct normals, our point must be far enough away from the vertex.

The Grand Finale

Perpendicularity
Finally, we reach the most thrilling part of our journey. We want the two non-axial normals to be perpendicular.
If their slopes are and , the condition for perpendicularity is . From our quadratic equation , we can identify the product of the roots.
In a quadratic , the product of the roots is simply the constant term. Here, that constant is . Setting this equal to , we get:
Solving this simple linear equation:
And there it is! When , the two normals are perfectly perpendicular. You have navigated the cubic landscape, respected the geometric constraints, and arrived at the precise coordinate where the physics of the parabola aligns in perfect harmony.

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