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though it did not help him get an academic job, it did make it possible for him to become known, finally, as Dr. Einstein.<br />

Brownian Motion, May 1905<br />

Eleven days after finishing his dissertation, Einstein produced another paper exploring evidence of things unseen. As he had been doing since<br />

1901, he relied on statistical analysis of the random actions of invisible particles to show how they were reflected in the visible world.<br />

In doing so, Einstein explained a phenomenon, known as Brownian motion, that had been puzzling scientists for almost eighty years: why small<br />

particles suspended in a liquid such as water are observed to jiggle around. And as a byproduct, he pretty much settled once and for all that atoms<br />

and molecules actually existed as physical objects.<br />

Brownian motion was named after the Scottish botanist Robert Brown, who in 1828 had published detailed observations about how minuscule<br />

pollen particles suspended in water can be seen to wiggle and wander when examined under a strong microscope. The study was replicated with<br />

other particles, including filings from the Sphinx, and a variety of explanations was offered. Perhaps it had something to do with tiny water currents<br />

or the effect of light. But none of these theories proved plausible.<br />

With the rise in the 1870s of the kinetic theory, which used the random motions of molecules to explain things like the behavior of gases, some<br />

tried to use it to explain Brownian motion. But because the suspended particles were 10,000 times larger than a water molecule, it seemed that a<br />

molecule would not have the power to budge the particle any more than a baseball could budge an object that was a half-mile in diameter. 32<br />

Einstein showed that even though one collision could not budge a particle, the effect of millions of random collisions per second could explain the<br />

jig observed by Brown. “In this paper,” he announced in his first sentence, “it will be shown that, according to the molecular-kinetic theory of heat,<br />

bodies of a microscopically visible size suspended in liquids must, as a result of thermal molecular motions, perform motions of such magnitudes<br />

that they can be easily observed with a microscope.” 33<br />

He went on to say something that seems, on the surface, somewhat puzzling: his paper was not an attempt to explain the observations of<br />

Brownian motion. Indeed, he acted as if he wasn’t even sure that the motions he deduced from his theory were the same as those observed by<br />

Brown: “It is possible that the motions to be discussed here are identical with so-called Brownian molecular motion; however, the data available to<br />

me on the latter are so imprecise that I could not form a judgment on the question.” Later, he distanced his work even further from intending to be an<br />

explanation of Brownian motion: “I discovered that, according to atomistic theory, there would have to be a movement of suspended microscopic<br />

particles open to observations, without knowing that observations concerning the Brownian motion were already long familiar.” 34<br />

At first glance his demurral that he was dealing with Brownian motion seems odd, even disingenuous. After all, he had written Conrad Habicht a<br />

few months earlier, “Such movement of suspended bodies has actually been observed by physiologists who call it Brownian molecular motion.” Yet<br />

Einstein’s point was both true and significant: his paper did not start with the observed facts of Brownian motion and build toward an explanation of<br />

it. Rather, it was a continuation of his earlier statistical analysis of how the actions of molecules could be manifest in the visible world.<br />

In other words, Einstein wanted to assert that he had produced a theory that was deduced from grand principles and postulates, not a theory that<br />

was constructed by examining physical data (just as he had made plain that his light quanta paper had not started with the photo-electric effect data<br />

gathered by Philipp Lenard). It was a distinction he would also make, as we shall soon see, when insisting that his theory of relativity did not derive<br />

merely from trying to explain experimental results about the speed of light and the ether.<br />

Einstein realized that a bump from a single water molecule would not cause a suspended pollen particle to move enough to be visible. However,<br />

at any given moment, the particle was being hit from all sides by thousands of molecules. There would be some moments when a lot more bumps<br />

happened to hit one particular side of the particle. Then, in another moment, a different side might get the heaviest barrage.<br />

The result would be random little lurches that would result in what is known as a random walk. The best way for us to envision this is to imagine a<br />

drunk who starts at a lamppost and lurches one step in a random direction every second. After two such lurches he may have gone back and forth<br />

to return to the lamp. Or he may be two steps away in the same direction. Or he may be one step west and one step northeast. A little mathematical<br />

plotting and charting reveals an interesting thing about such a random walk: statistically, the drunk’s distance from the lamp will be proportional to<br />

the square root of the number of seconds that have elapsed. 35<br />

Einstein realized that it was neither possible nor necessary to measure each zig and zag of Brownian motion, nor to measure the particle’s<br />

velocity at any moment. But it was rather easy to measure the total distances of randomly lurching particles as these distances grew over time.<br />

Einstein wanted concrete predictions that could be tested, so he used both his theoretical knowledge and experimental data about viscosity and<br />

diffusion rates to come up with precise predictions showing the distance a particle should move depending on its size and the temperature of the<br />

liquid. For example, he predicted, in the case of a particle with a diameter of one thousandth of a millimeter in water at 17 degrees centigrade, “the<br />

mean displacement in one minute would be about 6 microns.”<br />

Here was something that could actually be tested, and with great consequence. “If the motion discussed here can be observed,” he wrote, “then<br />

classical thermodynamics can no longer be viewed as strictly valid.” Better at theorizing than at conducting experiments, Einstein ended his paper<br />

with a charming exhortation: “Let us hope that a researcher will soon succeed in solving the problem presented here, which is so important for the<br />

theory of heat.”<br />

Within months, a German experimenter named Henry Seidentopf, using a powerful microscope, confirmed Einstein’s predictions. For all<br />

practical purposes, the physical reality of atoms and molecules was now conclusively proven. “At the time atoms and molecules were still far from<br />

being regarded as real,” the theoretical physicist Max Born later recalled. “I think that these investigations of Einstein have done more than any<br />

other work to convince physicists of the reality of atoms and molecules.” 36<br />

As lagniappe, Einstein’s paper also provided yet another way to determine Avogadro’s number. “It bristles with new ideas,” Abraham Pais said<br />

of the paper. “The final conclusion, that Avogadro’s number can essentially be determined from observations with an ordinary microscope, never<br />

fails to cause a moment of astonishment even if one has read the paper before and therefore knows the punch line.”<br />

A strength of Einstein’s mind was that it could juggle a variety of ideas simultaneously. Even as he was pondering dancing particles in a liquid, he<br />

had been wrestling with a different theory that involved moving bodies and the speed of light. A day or so after sending in his Brownian motion<br />

paper, he was talking to his friend Michele Besso when a new brainstorm struck. It would produce, as he wrote Habicht in his famous letter of that<br />

month, “a modification of the theory of space and time.”

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