# logarithmic spiral

In the logarithmic, or equiangular, spiral the angle α between a tangent at any point and the radius drawn from the center is constant. The lengths of the radii to the curve are proportional to the logarithms of the angles between the radii and the initial horizontal direction.

Logarithmic spirals occur in nature, generally revealing the effects of accelerating growth as in the spiral shells of snails and various other mollusks, such as the pearly Nautilus (above) of the Indian and Pacific oceans, and in flowers (below).

A logarithmic spiral, also known as an **equiangular
spiral**, is a type of spiral that is seen commonly in the natural world. Wonderful examples
are found in the shells of some molluscs,
such as that of the nautilus and the fossil ammonites, and also in spider webs. The logarithmic spiral is an example of a transcendental plane curve.

The angle any tangent to the curve makes with a tangent to a circle at the same radius, known as the **pitch angle**, is constant
and results in a logarithmic spiral being *self-similar*: in other
words, any part of it looks like any other part (though possibly rotated).
Hawks approach their prey in the form of a logarithmic spiral and their
sharpest view is at an angle to their flight direction that is the same
as the spiral's pitch. On an altogether different scale, the arms of spiral
galaxies are roughly logarithmic spirals. Our own galaxy, the Milky Way,
is believed to have four major arms, each of which is a logarithmic spiral
with pitch of about 12°. Approximate logarithmic spirals with a pitch
of about 17° can be generated using Fibonacci numbers or the golden
ratio.

In polar coordinates (*r*, *θ*) the equation of the logarithmic spiral is

*r* = *a b*^{θ}

with positive real numbers *a* and *b*. Changing *a* rotates
the spiral while *b* controls how tightly and in which direction it
is wrapped.

It can be distinguished from the Archimedean
spiral by the fact that the distance between the arms of a logarithmic
spiral increase in a geometric sequence while in an Archimedean spiral this distance is constant. Starting at a
point *P* and moving inwards along the spiral, one has to circle the
origin infinitely often before reaching it; yet, the total distance covered
is finite. This was first realized by the Italian physicist Evangelista Torricelli in the seventeenth century, even before calculus had been invented. The
total distance covered is *r */sin *θ* where *θ* is the pitch angle and *r* is the straight-line distance from *P* to the origin.

The logarithmic spiral was first described by René Descartes and later studied in depth by Jakob Bernoulli,
who called it *Spiralis mirabilis* (the Wonderful Spiral) and wanted
one engraved on his tombstone. He did get a spiral, but unfortunately it
was a rather crudely cut Archimedean type; accompanying it is the inscription *Eaden mutato resurgo* ("Although changed, I shall arise the
same").