The Physics of a Falling Rod
Imagine a uniform rod standing perfectly vertical on a frictionless floor. A slight nudge causes it to slip. To understand its motion, we must first analyze the forces acting on it.
The only external forces are gravity pulling it downwards (its weight, Mg) and the normal force from the floor pushing it upwards (N). Because the floor is perfectly smooth, there is absolutely zero friction. This means there are no horizontal forces acting on the rod.
According to Newton's Second Law, the acceleration of the Centre of Mass (CM) is directly proportional to the net external force. Since the net horizontal force is zero, the horizontal acceleration of the CM is zero.
Furthermore, the rod starts from rest, meaning its initial horizontal velocity is zero. With no horizontal acceleration and no initial horizontal velocity, the CM cannot move horizontally. It is constrained to fall vertically along the Y-axis. This elegant deduction tells us that the path of the Centre of Mass is a straight vertical line.
Tracking a Random Point
Now, let's find the trajectory of an arbitrary point P on the rod, located at a distance r from the lower end B.
Let's set up our coordinate system. The CM is at point C(0,yc) on the Y-axis, and the lower end is at point B(xb,0) on the X-axis. The distance between the CM and the lower end is exactly half the length of the rod, 2L. Let the rod make an angle θ with the horizontal X-axis.
To find the coordinates (x,y) of point P, we drop a perpendicular from P to the X-axis at point M. The x-coordinate is the distance OM, which can be written as the total distance OB minus the segment MB.
Using basic trigonometry in the right-angled triangle OBC, the base OB is:
Similarly, in the smaller right-angled triangle PMB, the base MB is:
Subtracting these gives us the x-coordinate of point P:
Factoring out cosθ, we get:
Rearranging this to isolate cosθ, we obtain our first parametric equation:
The Vertical Coordinate
Finding the y-coordinate is much simpler. It is just the height of point P above the ground, which corresponds to the perpendicular PM in our smaller triangle.
Using trigonometry again:
Isolating sinθ, we get our second parametric equation:
The Grand Synthesis
We now have expressions for both sinθ and cosθ. To find the trajectory, we must eliminate the variable θ. We can do this by invoking the fundamental trigonometric identity:
Substituting our derived expressions into this identity yields:
Rearranging this into the standard mathematical form, we get the final equation of the trajectory:
This is the unmistakable standard equation of an ellipse. Therefore, as the rod slips and falls, any given point on it (except the CM and the ends) traces out a beautiful elliptical path!