Analyzing the Setup
Imagine you are standing in a room, watching a ladder of constant length c slide down a wall. The ladder touches the floor at point A(a,0) and the wall at point B(0,b).
As it slides, the points A and B move, but the ladder itself remains rigid. This rigidity is our anchor. The distance between A and B is fixed, leading us to the fundamental constraint of our problem:
This equation is the heartbeat of our entire journey.
The Rectangle and the Perpendicular
Now, let us complete the rectangle OAPB. With O at the origin, A at (a,0), and B at (0,b), the fourth vertex P is naturally at (a,b).
We are interested in the foot of the perpendicular M dropped from P onto the line AB. To find M, we first need the equation of the line AB. Using the intercept form, we have:
This can be rearranged into the general form bx+ay−ab=0.
Next, we consider the line PM. Since PM is perpendicular to AB, its slope is the negative reciprocal of the slope of AB. The slope of AB is −ab, so the slope of PM is ba.
Using the point-slope form at P(a,b), we get y−b=ba(x−a), which simplifies to:
The Algebraic Dance
We now have a system of two linear equations: bx+ay=ab and ax−by=a2−b2. Our goal is to find the intersection point M(x,y).
Multiplying the first equation by b and the second by a, we get:
b2x+aby=ab2
a2x−aby=a3−ab2
Adding these two equations causes the y terms to vanish, leaving us with (a2+b2)x=a3. Recalling our constraint a2+b2=c2, we find:
By a symmetric process, we find:
The Grand Unveiling
We have x and y in terms of a and b. To find the locus, we must eliminate a and b. From our expressions, we have a=(xc2)1/3 and b=(yc2)1/3.
Substituting these into our constraint a2+b2=c2, we get:
Distributing the exponent, we have x2/3c4/3+y2/3c4/3=c2. Dividing both sides by c4/3, we arrive at the beautiful final equation:
This elegant curve is known as an Astroid, a star-like shape that emerges from the simple motion of a sliding ladder. You have just derived the equation of a classic geometric curve!