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Suppose that at the exact instant (from the viewpoint of the person on the embankment) when lightning strikes at points A and B, there is a<br />

passenger at the midpoint of the train, M t , just passing the observer who is at the midpoint alongside the tracks, M. If the train was motionless<br />

relative to the embankment, the passenger inside would see the lightning flashes simultaneously, just as the observer on the embankment would.<br />

But if the train is moving to the right relative to the embankment, the observer inside will be rushing closer toward place B while the light signals<br />

are traveling. Thus he will be positioned slightly to the right by the time the light arrives; as a result, he will see the light from the strike at place B<br />

before he will see the light from the strike at place A. So he will assert that lightning hit at B before it did so at A, and the strikes were not<br />

simultaneous.<br />

“We thus arrive at the important result: Events that are simultaneous with reference to the embankment are not simultaneous with respect to the<br />

train,” said Einstein. The principle of relativity says that there is no way to decree that the embankment is “at rest” and the train “in motion.” We can<br />

say only that they are in motion relative to each other. So there is no “real” or “right” answer. There is no way to say that any two events are<br />

“absolutely” or “really” simultaneous. 43<br />

This is a simple insight, but also a radical one. It means that there is no absolute time. Instead, all moving reference frames have their own<br />

relative time. Although Einstein refrained from saying that this leap was as truly “revolutionary” as the one he made about light quanta, it did in fact<br />

transform science. “This was a change in the very foundation of physics, an unexpected and very radical change that required all the courage of a<br />

young and revolutionary genius,” noted Werner Heisenberg, who later contributed to a similar feat with his principle of quantum uncertainty. 44<br />

In his 1905 paper, Einstein used a vivid image, which we can imagine him conceiving as he watched the trains moving into the Bern station past<br />

the rows of clocks that were synchronized with the one atop the town’s famed tower. “Our judgments in which time plays a part are always<br />

judgments of simultaneous events,” he wrote. “If, for instance, I say, ‘That train arrives here at 7 o’clock,’ I mean something like this: ‘The pointing of<br />

the small hand of my watch to 7 and the arrival of the train are simultaneous events.’ ” Once again, however, observers who are moving rapidly<br />

relative to one another will have a different view on whether two distant events are simultaneous.<br />

The concept of absolute time—meaning a time that exists in “reality” and tick-tocks along independent of any observations of it—had been a<br />

mainstay of physics ever since Newton had made it a premise of his Principia 216 years earlier. The same was true for absolute space and<br />

distance.“Absolute, true, and mathematical time, of itself and from its own nature, flows equably without relation to anything external,” he famously<br />

wrote in Book 1 of the Principia. “Absolute space, in its own nature, without relation to anything external, remains always similar and immovable.”<br />

But even Newton seemed discomforted by the fact that these concepts could not be directly observed. “Absolute time is not an object of<br />

perception,” he admitted. He resorted to relying on the presence of God to get him out of the dilemma. “The Deity endures forever and is<br />

everywhere present, and by existing always and everywhere, He constitutes duration and space.” 45<br />

Ernst Mach, whose books had influenced Einstein and his fellow members of the Olympia Academy, lambasted Newton’s notion of absolute time<br />

as a “useless metaphysical concept” that “cannot be produced in experience.” Newton, he charged, “acted contrary to his expressed intention only<br />

to investigate actual facts.” 46<br />

Henri Poincaré also pointed out the weakness of Newton’s concept of absolute time in his book Science and Hypothesis, another favorite of the<br />

Olympia Academy. “Not only do we have no direct intuition of the equality of two times, we do not even have one of the simultaneity of two events<br />

occurring in different places,” he wrote. 47<br />

Both Mach and Poincaré were, it thus seems, useful in providing a foundation for Einstein’s great breakthrough. But he owed even more, he later<br />

said, to the skepticism he learned from the Scottish philosopher David Hume regarding mental constructs that were divorced from purely factual<br />

observations.<br />

Given the number of times in his papers that he uses thought experiments involving moving trains and distant clocks, it is also logical to surmise<br />

that he was helped in visualizing and articulating his thoughts by the trains that moved past Bern’s clock tower and the rows of synchronized clocks<br />

on the station platform. Indeed, there is a tale that involves him discussing his new theory with friends by pointing to (or at least referring to) the<br />

synchronized clocks of Bern and the unsynchronized steeple clock visible in the neighboring village of Muni. 48<br />

Peter Galison provides a thought-provoking study of the technological ethos in his book Einstein’s Clocks, Poincaré’s Maps. Clock coordination<br />

was in the air at the time. Bern had inaugurated an urban time network of electrically synchronized clocks in 1890, and a decade later, by the time<br />

Einstein had arrived, finding ways to make them more accurate and coordinate them with clocks in other cities became a Swiss passion.<br />

In addition, Einstein’s chief duty at the patent office, in partnership with Besso, was evaluating electromechanical devices. This included a flood<br />

of applications for ways to synchronize clocks by using electric signals. From 1901 to 1904, Galison notes, there were twenty-eight such patents<br />

issued in Bern.<br />

One of them, for example, was called “Installation with Central Clock for Indicating the Time Simultaneously in Several Places Separated from<br />

One Another.” A similar application arrived on April 25, just three weeks before Einstein had his breakthrough conversation with Besso; it involved<br />

a clock with an electromagnetically controlled pendulum that could be coordinated with another such clock through an electric signal. What these<br />

applications had in common was that they used signals that traveled at the speed of light. 49<br />

We should be careful not to overemphasize the role played by the technological backdrop of the patent office. Although clocks are part of<br />

Einstein’s description of his theory, his point is about the difficulties that observers in relative motion have in using light signals to synchronize<br />

them, something that was not an issue for the patent applicants. 50<br />

Nevertheless, it is interesting to note that almost the entire first two sections of his relativity paper deal directly and in vivid practical detail (in a<br />

manner so different from the writings of, say, Lorentz and Maxwell) with the two real-world technological phenomena he knew best. He writes about<br />

the generation of “electric currents of the same magnitude” due to the “equality of relative motion” of coils and magnets, and the use of “a light<br />

signal” to make sure that “two clocks are synchronous.”<br />

As Einstein himself stated, his time in the patent office “stimulated me to see the physical ramifications of theoretical concepts.” 51 And Alexander<br />

Moszkowski, who compiled a book in 1921 based on conversations with Einstein, noted that Einstein believed there was “a definite connection<br />

between the knowledge acquired at the patent office and the theoretical results.” 52<br />

“On the Electrodynamics of Moving Bodies”<br />

Now let’s look at how Einstein articulated all of this in the famous paper that the Annalen der Physik received on June 30, 1905. For all its<br />

momentous import, it may be one of the most spunky and enjoyable papers in all of science. Most of its insights are conveyed in words and vivid<br />

thought experiments, rather than in complex equations. There is some math involved, but it is mainly what a good high school senior could

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