Pedal equation

From testwiki
Revision as of 07:04, 27 January 2025 by imported>Citation bot (Alter: pages, url. URLs might have been anonymized. Add: bibcode, issue. | Use this bot. Report bugs. | Suggested by Dominic3203 | Category:Coordinate systems | #UCB_Category 12/45)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to navigation Jump to search

Template:Short description

In Euclidean geometry, for a plane curve Template:Mvar and a given fixed point Template:Mvar, the pedal equation of the curve is a relation between Template:Mvar and Template:Mvar where Template:Mvar is the distance from Template:Mvar to a point on Template:Mvar and Template:Mvar is the perpendicular distance from Template:Mvar to the tangent line to Template:Mvar at the point. The point Template:Mvar is called the pedal point and the values Template:Mvar and Template:Mvar are sometimes called the pedal coordinates of a point relative to the curve and the pedal point. It is also useful to measure the distance of Template:Mvar to the normal Template:Mvar (the contrapedal coordinate) even though it is not an independent quantity and it relates to Template:Math as pc:=r2p2.

Some curves have particularly simple pedal equations and knowing the pedal equation of a curve may simplify the calculation of certain of its properties such as curvature. These coordinates are also well suited for solving certain type of force problems in classical mechanics and celestial mechanics.

Equations

Cartesian coordinates

For C given in rectangular coordinates by f(xy) = 0, and with O taken to be the origin, the pedal coordinates of the point (xy) are given by:[1]

r=x2+y2
p=xfx+yfy(fx)2+(fy)2.

The pedal equation can be found by eliminating x and y from these equations and the equation of the curve.

The expression for p may be simplified if the equation of the curve is written in homogeneous coordinates by introducing a variable z, so that the equation of the curve is g(xyz) = 0. The value of p is then given by[2]

p=gz(gx)2+(gy)2

where the result is evaluated at z=1

Polar coordinates

For C given in polar coordinates by r = f(θ), then

p=rsinϕ

where ϕ is the polar tangential angle given by

r=drdθtanϕ.

The pedal equation can be found by eliminating θ from these equations.[3]

Alternatively, from the above we can find that

|drdθ|=rpcp,

where pc:=r2p2 is the "contrapedal" coordinate, i.e. distance to the normal. This implies that if a curve satisfies an autonomous differential equation in polar coordinates of the form:

f(r,|drdθ|)=0,

its pedal equation becomes

f(r,rpcp)=0.

Example

As an example take the logarithmic spiral with the spiral angle α:

r=aecosαsinαθ.

Differentiating with respect to θ we obtain

drdθ=cosαsinαaecosαsinαθ=cosαsinαr,

hence

|drdθ|=|cosαsinα|r,

and thus in pedal coordinates we get

rppc=|cosαsinα|r,|sinα|pc=|cosα|p,

or using the fact that pc2=r2p2 we obtain

p=|sinα|r.

This approach can be generalized to include autonomous differential equations of any order as follows:[4] A curve C which a solution of an n-th order autonomous differential equation (n1) in polar coordinates

f(r,|r'θ|,r'θ,|r'θ|,rθ(2j),|rθ(2j+1)|,,rθ(n))=0,

is the pedal curve of a curve given in pedal coordinates by

f(p,pc,pcpc,pc(pcpc),,(pcp)np)=0,

where the differentiation is done with respect to p.

Force problems

Solutions to some force problems of classical mechanics can be surprisingly easily obtained in pedal coordinates.

Consider a dynamical system:

x¨=F(|x|2)x+2G(|x|2)x˙,

describing an evolution of a test particle (with position x and velocity x˙) in the plane in the presence of central F and Lorentz like G potential. The quantities:

L=xx˙+G(|x|2),c=|x˙|2F(|x|2),

are conserved in this system.

Then the curve traced by x is given in pedal coordinates by

(LG(r2))2p2=F(r2)+c,

with the pedal point at the origin. This fact was discovered by P. Blaschke in 2017.[5]

Example

As an example consider the so-called Kepler problem, i.e. central force problem, where the force varies inversely as a square of the distance:

x¨=M|x|3x,

we can arrive at the solution immediately in pedal coordinates

L22p2=Mr+c,,

where L corresponds to the particle's angular momentum and c to its energy. Thus we have obtained the equation of a conic section in pedal coordinates.

Inversely, for a given curve C, we can easily deduce what forces do we have to impose on a test particle to move along it.

Pedal equations for specific curves

Sinusoidal spirals

For a sinusoidal spiral written in the form

rn=ansin(nθ)

the polar tangential angle is

ψ=nθ

which produces the pedal equation

pan=rn+1.

The pedal equation for a number of familiar curves can be obtained setting n to specific values:[6]

n Curve Pedal point Pedal eq.
All Circle with radius a Center pan=rn+1
1 Circle with diameter a Point on circumference pa = r2
−1 Line Point distance a from line p = a
Template:Frac Cardioid Cusp p2a = r3
Template:Frac Parabola Focus p2 = ar
2 Lemniscate of Bernoulli Center pa2 = r3
−2 Rectangular hyperbola Center rp = a2

Spirals

A spiral shaped curve of the form

r=cθα,

satisfies the equation

drdθ=αrα1α,

and thus can be easily converted into pedal coordinates as

1p2=α2c2αr2+2α+1r2.

Special cases include:

α Curve Pedal point Pedal eq.
1 Spiral of Archimedes Origin 1p2=1r2+c2r4
−1 Hyperbolic spiral Origin 1p2=1r2+1c2
Template:Frac Fermat's spiral Origin 1p2=1r2+c44r6
Template:Frac Lituus Origin 1p2=1r2+r24c4

Epi- and hypocycloids

For an epi- or hypocycloid given by parametric equations

x(θ)=(a+b)cosθbcos(a+bbθ)
y(θ)=(a+b)sinθbsin(a+bbθ),

the pedal equation with respect to the origin is[7]

r2=a2+4(a+b)b(a+2b)2p2

or[8]

p2=A(r2a2)

with

A=(a+2b)24(a+b)b.

Special cases obtained by setting b=Template:Frac for specific values of n include:

n Curve Pedal eq.
1, −Template:Frac Cardioid p2=98(r2a2)
2, −Template:Frac Nephroid p2=43(r2a2)
−3, −Template:Frac Deltoid p2=18(r2a2)
−4, −Template:Frac Astroid p2=13(r2a2)

Other curves

Other pedal equations are:,[9]

Curve Equation Pedal point Pedal eq.
Line ax+by+c=0 Origin p=|c|a2+b2
Point (x0,y0) Origin r=x02+y02
Circle |xa|=R Origin 2pR=r2+R2|a|2
Involute of a circle r=acosα, θ=tanαα Origin pc=|a|
Ellipse x2a2+y2b2=1 Center a2b2p2+r2=a2+b2
Hyperbola x2a2y2b2=1 Center a2b2p2+r2=a2b2
Ellipse x2a2+y2b2=1 Focus b2p2=2ar1
Hyperbola x2a2y2b2=1 Focus b2p2=2ar+1
Logarithmic spiral r=aeθcotα Pole p=rsinα
Cartesian oval |x|+α|xa|=C, Focus (b(1α2)r2)24p2=Cbr+(1α2)Cr((1α2)C2+b), b:=C2α2|a|2
Cassini oval |x||xa|=C, Focus (3C2+r4|a|2r2)2p2=4C2(2C2r2+2r2|a|2).
Cassini oval |xa||x+a|=C, Center 2Rpr=r4+R2|a|2.

See also

References

Template:Reflist

  1. Yates §1
  2. Edwards p. 161
  3. Yates p. 166, Edwards p. 162
  4. Blaschke Proposition 1
  5. Blaschke Theorem 2
  6. Yates p. 168, Edwards p. 162
  7. Edwards p. 163
  8. Yates p. 163
  9. Yates p. 169, Edwards p. 163, Blaschke sec. 2.1