The Ghost From the Grand Banks and the Deep Range

  Needless to say, there are Mandelbrot “fan magazines,” containing hints on speeding up programs, notes from explorers in far-off regions of the set—and even samples of a new literary genre, Fractalfiction. The newsletter of the field is Amygdala, edited by Rollo Silver, who also supplies software (Box 111, San Cristobal, NM 87564).

  Undoubtedly the best way of appreciating the set is through the videotapes that have been made of it, usually with accompanying music. Most celebrated is “Nothing But Zooms” from Art Matrix (P.O. Box 880, Ithaca, NY 14851). I have also enjoyed “A Fractal Ballet” (The Fractal Stuff Company, P.O. Box 5202, Spokane, WA 99205-5202).

  Strictly speaking, the “Utter West” of the M-Set is at exactly–2, not –1.999 . . . to infinity, as stated in Chapter 18. Anyone care to split the difference?

  I do not know if there have been any cases of Mandelmania in real life, but I expect to receive reports as soon as this book appears—and waive all responsibility in advance.

  APPENDIX: THE COLORS OF INFINITY

  In November 1989, when receiving the Association of Space Explorers Special Achievement Award in Riyadh, Saudi Arabia, I had the privilege of addressing the largest gathering of astronauts and cosmonauts ever assembled at one place. (More than fifty, including Apollo 11’s Buzz Aldrin and Mike Collins, and the first “space walker” Alexei Leonov, who is no longer embarrassed at sharing the dedication of 2010: Odyssey Two with Andrei Sakharov.) I decided to expand their horizons by introducing them to something really large, and, with astronaut Prince Sultan bin Salman bin Abdul Aziz in the chair, delivered a lavishly illustrated lecture “The Colors of Infinity: Exploring the Fractal Universe.”

  The material that follows is extracted from my speech; another portion appears at the beginning of Chapter 15. I’m only sorry that I cannot illustrate it with the gorgeous 35-millimeter slides—and videos—I used at Riyadh.

  Today, everybody is familiar with graphs—especially the one with time along the horizontal axis, and the cost of living climbing steadily up the vertical one. The idea that any point on a plane can be expressed by two numbers, usually written x and y, now appears so obvious that it seems quite surprising that the world of mathematics had to wait until 1637 for Descartes to invent it.

  We are still discovering the consequences of that apparently simple idea, and the most amazing is now just ten years old. It’s called the Mandelbrot Set (from now on, the M-Set) and you’re soon going to meet it everywhere—in the design of fabrics, wallpaper, jewelry, and linoleum. And, I’m afraid, it will be popping out of your TV screen in every other commercial.

  Yet the most astonishing feature of the M-Set is its basic simplicity. Unlike almost everything else in modern mathematics, any schoolchild can understand how it is produced. Its generation involves nothing more advanced than addition and multiplication; there’s no need for such complexities as subtraction and—heaven forbid!—division, let alone any of the more exotic beasts from the mathematical menagerie.

  There can be few people in the civilized world who have not encountered Einstein’s famous E = mc2, or who would consider it too hopelessly complicated to understand. Well, the equation that defines the M-Set contains the same number of terms, and indeed looks very similar. Here it is.

  Z = z2 + c

  Not very terrifying, is it? Yet the lifetime of the Universe would not be long enough to explore all its ramifications.

  The z’s and the c in Mandelbrot’s equation are all numbers, not (as in Einstein’s) physical quantities like mass and energy. They are the coordinates which specify the position of a point, and the equation controls the way in which it moves, to trace out a pattern.

  There’s a very simple analog familiar to everyone—those children’s books with blank pages sprinkled with numbers, which when joined up in the right order reveal hidden—and often surprising—pictures. The image on a TV screen is produced by a sophisticated application of the same principle.

  In theory, anyone who can add and multiply could plot out the M-Set with pen or pencil on a sheet of squared paper. However, as we’ll see later, there are certain practical difficulties—notably the fact that a human life span is seldom more than a hundred years. So the set is invariably computer-generated, and usually shown on a visual display unit.

  Now, there are two ways of locating a point in space. The more common employs some kind of grid reference—west-east, north-south, or on squared graph paper, a horizontal X-axis and a vertical Y-axis. But there’s also the system used in radar, now familiar to most people thanks to countless movies. Here the position of an object is given by (1) its distance from the origin, and (2) its direction, or compass bearing. Incidentally, this is the natural system—the one you use automatically and unconsciously when you play any ball game. Then you’re concerned with distances and angles, with yourself as the origin.

  So think of a computer’s VDU as a radar screen, with a single blip on it, whose movements are going to trace out the M-Set. However, before we switch on our radar, I want to make the equation even simpler, to:

  Z = z2

  I’ve thrown c away, for the moment, and left only the z’s. Now let me define them more precisely.

  Small z is the initial range of the blip—the distance at which it starts. Big Z is its final distance from the origin. Thus if it was initially 2 units away, by obeying this equation it would promptly hop to a distance of 4.

  Nothing to get very excited about, but now comes the modification that makes all the difference:

  That double arrow is a two-way traffic sign, indicating that the numbers flow in both directions. This time, we don’t stop at Z = 4; we make that equal to a new z—which promptly gives us a second Z of 16, and so on. In no time we’ve generated the series

  256, 65536, 4294967296 . . .

  and the spot that started only 2 units from the center is heading toward infinity in giant steps of ever-increasing magnitude.

  This process of going around and around a loop is called “iteration.” It’s like a dog chasing its own tail, except that a dog doesn’t get anywhere. But mathematical iteration can take us to some very strange places indeed—as we shall soon discover.

  Now we’re ready to turn on our radar. Most displays have range circles at 10, 20 . . . 100 kilometers from the center. We will require only a single circle, at a range of 1. There’s no need to specify any units, as we’re dealing with pure numbers. Make them centimeters or light-years, as you please.

  Let’s suppose that the initial position of our blip is anywhere on this circle—the bearing doesn’t matter. So z is 1.

  And because 1 squared is still 1, so is Z. And it remains at that value, because no matter how many times you square 1, it always remains exactly 1. The blip may hop around and around the circle, but it always stays on it.

  Now consider the case where the initial z is greater than 1. We’ve already seen how rapidly the blip shoots off to infinity if z equals 2—but the same thing will happen sooner or later, even if it’s only a microscopic shade more than 1—say 1.000000000000000000001. Watch:

  At the first squaring, Z becomes

  1.000000000000000000002

  then

  1.000000000000000000004

  1.000000000000000000008

  1.000000000000000000016

  1.000000000000000000032

  and so on for pages of printout. For all practical purposes, the value is still exactly 1. The blip hasn’t moved visibly outward or inward; it’s still on the circle at range 1.

  But those zeros are slowly being whittled away, as the digits march inexorably across from the right. Quite suddenly, something appears in the third, second, first decimal place—and the numbers explode after a very few additional terms, as this example shows:

  1.001 1.002 1.004 1.008 1.016 1.032

  1.066 1.136 1.292 1.668 2.783 7.745

  59.987 3598.467 12948970

  167675700000000

  28115140000000000000000000000

  (Ov
erflow)

  There could be a million—a billion—zeros on the right-hand side, and the result would still be the same. Eventually the digits would creep up to the decimal point—and then Z would take off to infinity.

  Now let’s look at the other case. Suppose z is a microscopic amount less than 1—say something like

  .99999999999999999999

  As before, nothing much happens for a long time as we go around the loop, except that the numbers on the far right get steadily smaller. But after a few thousand or million iterations—catastrophe! Z suddenly shrinks to nothing, dissolving in an endless string of zeros. . . .

  Check it out on your computer. It can only handle twelve digits? Well, no matter how many you had to play with, you’d still get the same answer. Trust me. . . .

  The results of this “program” can be summarized in three laws that may seem too trivial to be worth formulating. But no mathematical truth is trivial, and in a few more steps these laws will take us into a universe of mind-boggling wonder and beauty.

  Here are the three laws of the “Squaring” Program:

  1. If the input z is exactly equal to 1, the output Z always remains 1.

  2. If the input is more than 1, the output eventually becomes infinite.

  3. If the input is less than 1, the output eventually becomes zero.

  That circle of radius 1 is therefore a kind of map—or, if you like, fence—dividing the plane into two distinct territories. Outside it, numbers which obey the squaring law have the freedom of infinity; numbers inside it are prisoners, trapped and doomed to ultimate extinction.

  At this point, someone may say: “You’ve only talked about ranges—distances from the origin. To fix the blip’s position, you have to give its bearing as well. What about that?”

  Very true. Fortunately, in this selection process—this division of the z’s into two distinct classes—bearings are irrelevant; the same thing happens whichever direction r is pointing. For this simple example—let’s call it the S-set—we can ignore them. When we come on to the more complicated case of the M-Set, where the bearing is important, there’s a very neat mathematical trick which takes care of it, by using complex or imaginary numbers (which really aren’t at all complex, still less imaginary). But we don’t need them here, and I promise not to mention them again.

  The S-set lies inside a map, and its frontier is the circle enclosing it. That circle is simply a continuous line with no thickness. If you could examine it with a microscope of infinite power, it would always look exactly the same. You could expand the S-set to the size of the Universe; its boundary would still be a line of zero thickness. Yet there are no holes in it; it’s an absolutely impenetrable barrier, forever separating the z’s less than one from those greater than one.

  Now, at last, we’re ready to tackle the M-Set, where these commonsense ideas are turned upside down. Fasten your seat belts.

  During the 1970s, the French mathematician Benoit Mandelbrot, working at Harvard and IBM, started to investigate the equation which has made him famous, and which I will now write in the dynamic form:

  The only difference between this and the equation we have used to describe the S-set is the term c. This—not z—is now the starting point of our mapping operation. The first time around the loop, z is put equal to zero.

  It seems a trifling change, and no one could have imagined the universe it would reveal. Mandelbrot himself did not obtain the first crude glimpses until the spring of 1980, when vague patterns started to emerge on computer printouts. He had begun to peer through Keats’

  Charm’d magic casements, opening on the foam

  Of perilous seas, in faery lands forlorn . . .

  As we shall learn later, that word “foam” is surprisingly appropriate.

  The new equation asks and answers the same question as the earlier one: What shape is the “territory” mapped out when we put numbers into it? For the S-set it was a circle with radius 1. Let’s see what happens when we start with this value in the M-equation. You should be able to do it in your head—for the first few steps. After a few dozen, even a supercomputer may blow a gasket.

  For starters, z = 0, c = 1. So Z = 1

  First loop: Z = 12 + 1 = 2

  Second loop: Z = 22 + 1 = 5

  Third loop: Z = 52 + 1 = 26

  Fourth loop: Z = 262 + 1 . . . and so on.

  I once set my computer to work out the higher terms (about the limit of my programming ability) and it produced only two more values before it had to start approximating:

  1, 2, 5, 26, 677, 458330,

  21006640000

  4412789000000000000000

  At that point it gave up, because it doesn’t believe there are any numbers with more than 38 digits.

  However, even the first two or three terms are quite enough to show that the M-Set must have a very different shape from the perfectly circular S-set. A point at distance 1 is in the S-set; indeed, it defines its boundary. A point at that same distance may be outside the boundary of the M-Set.

  Note that I say “may,” not “must.” It all depends on the initial direction, or bearing, of the starting point, which we have been able to ignore hitherto because it did not affect our discussion of the (perfectly symmetrical) S-set. As it turns out, the M-Set is only symmetrical about the X, or horizontal, axis.

  One might have guessed that, from the nature of the equation. But no one could possibly have intuited its real appearance. If the question had been put to me in virginal pre-Mandelbrot days, I would probably have hazarded: “Something like an ellipse, squashed along the Y-axis.” I might even (though I doubt it) have correctly guessed that it would be shifted toward the left, or minus, direction.

  At this point, I would like to try a thought experiment on you. The M-Set being literally indescribable, here’s my attempt to describe it:

  Imagine you’re looking straight down on a rather plump turtle, swimming westward. It’s been crossed with a swordfish, so has a narrow spike pointing ahead of it. Its entire perimeter is festooned with bizarre marine growths—and with baby turtles of assorted sizes, which have smaller weeds growing on them. . . .

  I defy you to find a description like that in any math textbook. And if you think you can do better when you’ve seen the real beast, you’re welcome to try. (I suspect that the insect world might provide better analogies; there may even be a Mandelbeetle lurking in the Brazilian rain forests. Too bad we’ll never know.)

  Here is the first crude approximation, shorn of details—much like Conroy Castle’s “Lake Mandelbrot” (Chapter 18). If you like to fill its blank spaces with the medieval cartographers’ favorite “Here be dragons” you will hardly be exaggerating.

  First of all, note that—as I’ve already remarked—it’s shifted to the left (or west, if you prefer of the S-set, which of course extends from +1 to –1 along the X-axis. The M-Set only gets to 0.25 on the right along the axis, though above and below the axis it bulges out to just beyond 0.4.

  On the left-hand side, the map stretches to about –1.4, and then it sprouts a peculiar spike—or antenna—which reaches out to exactly –2.0. As far as the M-Set is concerned, there is nothing beyond this point; it is the edge of the Universe. Mandelbrot fans call it the “Utter West,” and you might like to see what happens when you make c equal to –2. Z doesn’t converge to zero—but it doesn’t escape to infinity either, so the point belongs to the set—just. But if you make c the slightest bit larger, say –2.00000 . . . 000001, before you know it you’re passing Pluto and heading for Quasar West.

  Now we come to the most important distinction between the two sets. The S-set has a nice, clean line for its boundary. The frontier of the M-Set is, to say the least, fuzzy. Just how fuzzy you will begin to understand when we start to “zoom” into it; only then will we see the incredible flora and fauna which flourish in that disputed territory.

  The boundary—if one can call it that—of the M-Set is not a simple line; it is something which Euclid never
imagined, and for which there is no word in ordinary language. Mandelbrot, whose command of English (and American) is awesome, has ransacked the dictionary for suggestive nouns. A few examples: foams, sponges, dusts, webs, nets, curds. He himself coined the technical name fractal, and is now putting up a spirited rearguard action to stop anyone from defining it too precisely.

  Computers can easily make “snapshots” of the M-Set at any magnification, and even in black and white they are fascinating. However, by a simple trick they can be colored, and transformed into objects of amazing, even surreal, beauty.

  The original equation, of course, is no more concerned with color than is Euclid’s Elements of Geometry. But if we instruct the computer to color any given region in accordance with the number of times z goes around the loop before it decides whether or not it belongs to the M-Set, the results are gorgeous.

  Thus the colors, though arbitrary, are not meaningless. An exact analogy is found in cartography. Think of the contour lines on a relief map, which show elevations above sea level. The spaces between them are often colored so that the eye can more easily grasp the information conveyed. Ditto with bathymetric charts; the deeper the ocean, the darker the blue. The mapmaker can make the colors anything he likes, and is guided by aesthetics as much as geography.