three theorems on parabolas


In the Cartesian plane, pick a point with coordinates (0,2⁢f) (subtle hint!) and construct (1) the set S of segments s joining F=(0,2⁢f) with the points (x,0), and (2) the set B of right-bisectors b of the segments s∈S.

Theorem 1 :

The envelope described by the lines of the set B is a parabolaPlanetmathPlanetmath with x-axis as directrix and focal length |f|.

Proof:

We’re lucky in that we don’t need a fancy definition of envelope; considering a line to be a set of points it’s just the boundary of the set C=∪b∈Bb. Strategy: fix an x coordinate and find the max/minimum of possible y’s in C with that x. But first we’ll pick an s from S by picking a point p=(w,0) on the x axis. The midpointMathworldPlanetmathPlanetmathPlanetmath of the segment s∈S through p is M=(w2,f). Also, the slope of this s is -2⁢fw. The corresponding right-bisector will also pass through (w2,f) and will have slope w2⁢f. Its equation is therefore

2⁢y-2⁢f2⁢x-w=w2⁢f.

Equivalently,

y=f+w⁢x2⁢f-w24⁢f.

By any of many very famous theoremsMathworldPlanetmath (Euclid book II theorem twenty-something, Cauchy-Schwarz-Bunyakovski (overkill), differential calculus, what you will) for fixed x, y is an extremumMathworldPlanetmath for w=x only, and therefore the envelope has equation

y=f+x24⁢f.

I could say I’m done right now because we “know” that this is a parabola, with focal length f and x-axis as directrix. I don’t want to, though. The most popular definition of parabola I know of is “set of points equidistant from some line d and some point f.” The line responsible for the point on the envelope with given ordinate x was found to bisect the segment s∈S through H=(x,0). So pick an extra point Q∈b∈B where b is the perpendicular bisectorMathworldPlanetmath of s. We then have ∠⁢F⁢M⁢Q=∠⁢Q⁢M⁢H because they’re both right anglesMathworldPlanetmathPlanetmath, lengths F⁢M=M⁢H, and Q⁢M is common to both trianglesMathworldPlanetmath F⁢M⁢Q and H⁢M⁢Q. Therefore two sides and the angles they contain are respectively equal in the triangles F⁢M⁢Q and H⁢M⁢Q, and so respective angles and respective sides are all equal. In particular, F⁢Q=Q⁢H. Also, since Q and H have the same x coordinate, the line Q⁢H is the perpendicularPlanetmathPlanetmathPlanetmath to the x-axis, and so Q, a general point on the envelope, is equidistant from F and the x-axis. Therefore etc.

QED.

Because of this construction, it is clear that the lines of B are all tangentPlanetmathPlanetmathPlanetmath to the parabola in question.

We’re not done yet. Pick a random point P outside C (“inside” the parabola), and call the parabola π (just to be nasty). Here’s a nice quicky:

Theorem 2 The Reflector Law:

For R∈π, the length of the path P⁢R⁢F is minimalPlanetmathPlanetmath when P⁢R produced is perpendicular to the x-axis.

Proof:

Quite simply, assume P⁢R produced is not necessarily perpendicular to the x-axis. Because π is a parabola, the segment from R perpendicular to the x-axis has the same length as R⁢F. So let this perpendicular hit the x-axis at H. We then have that the length of P⁢R⁢H equals that of P⁢R⁢F. But P⁢R⁢H (and hence P⁢R⁢F) is minimal when it’s a straight line; that is, when P⁢R produced is perpendicular to the x-axis.

QED

Hey! I called that theorem the “reflector law”. Perhaps it didn’t look like one. (It is in the Lagrangian formulation), but it’s fairly easy to show (it’s a similarMathworldPlanetmathPlanetmath argumentMathworldPlanetmath) that the shortest path from a point to a line to a point makes and “reflected” angles equal.

One last marvelous tidbit. This will take more time, though. Let b be tangent to π at R, and let n be perpendicular to b at R. We will call n the to π at R. Let n meet the x-axis at G.

Theorem 3 :

The radius of the “best-fit circle” to π at R is twice the length R⁢G.

Proof:

(Note: the ≈’s need to be phrased in terms of upper and lower bounds, so I can use the sandwich theorem, but the proof schema is exactly what is required).

Take two points R,R′ on π some small distanceMathworldPlanetmath ϵ from each other (we don’t actually use ϵ, it’s just a psychological trick). Construct the tangent t and normal n at R, normal n′ at R′. Let n,n′ intersect at O, and t intersect the x-axis at G. R⁢F,R′⁢F. Erect perpendiculars g,g′ to the x-axis through R,R′ respectively. R⁢R′. Let g intersect the x-axis at H. Let P,P′ be points on g,g′ not in C. Construct R⁢E perpendicular to R⁢F with E in R′⁢F. We now have

  • i)

    ∠⁢P⁢R⁢O=∠⁢O⁢R⁢F=∠⁢G⁢R⁢H≈∠⁢P′⁢R′⁢O=∠⁢O⁢R′⁢F

  • iii)

    E⁢R≈F⁢R⋅∠⁢E⁢F⁢R

  • v)

    ∠⁢R′⁢R⁢E+∠⁢E⁢R⁢O≈π2 (That’s the number π, not the parabola)

  • vii)

    ∠⁢E⁢R⁢O+∠⁢O⁢R⁢F=π2

  • ix)

    ∠⁢R′⁢E⁢R≈π2

  • xi)

    ∠⁢R′⁢O⁢R=12⁢∠⁢R′⁢F⁢R

  • xiii)

    R′⁢R≈O⁢R⋅∠⁢R′⁢O⁢R

  • xv)

    F⁢R=R⁢H

From (iii),(iv) and (i) we have ∠⁢R′⁢R⁢E≈∠⁢G⁢R⁢H, and since R′ is close to R, and if we let R′ approach R, the approximations approach equality. Therefore, we have that triangle R′⁢R⁢E approaches similarity with G⁢R⁢H. Therefore we have R⁢R′:E⁢R≈R⁢G:R⁢H. Combining this with (ii),(vi),(vii), and (viii) it follows that R⁢O≈2⁢R⁢G, and in the limit R′→R, R⁢O=2⁢R⁢G.

QED

This last theorem is a very nice way of short-cutting all the messy calculus needed to derive the Schwarzschild “Black-Hole” solution to Einstein’s equations, and that’s why I enjoy it so.

Title three theorems on parabolas
Canonical name ThreeTheoremsOnParabolas
Date of creation 2013-03-22 12:40:51
Last modified on 2013-03-22 12:40:51
Owner CWoo (3771)
Last modified by CWoo (3771)
Numerical id 19
Author CWoo (3771)
Entry type Topic
Classification msc 51N20
Related topic PropertiesOfParabola