A Demonstration At Shippingport (June/July 1981 | Volume: 32, Issue: 4)

A Demonstration At Shippingport

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Authors: Richard Rhodes

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June/July 1981 | Volume 32, Issue 4

From the beginning it was clear—in this case the beginning was December 2, 1942, the day the first man-made nuclear reactor was nudged to criticality in a squash court beneath the west stands of the University of Chicago’s Stagg Field and incidentally the first day of wartime gasoline rationing—that the fissioning atom radiated heat energy and that such energy might, in the fullness of time, be applied to make electricity for power. Fifteen years would pass before nuclear electricity was generated in any quantity in the United States. That is rapid development or surprising delay, depending upon one’s perspective, but the fact is that despite its imposing technical lead in nuclear matters, the United States did not arrive first at the production of commercial nuclear power. Great Britain did. On a smaller scale, even the Soviet Union preceded us. The reasons are intriguing. How the United States contrived to back into the nuclear power business is instructive. “There are overtones in this development,” wrote the physicist and statesman J. Robert Oppenheimer in 1957, “that have been absent in power developments in other respects not wholly beyond comparison, such as the diesel engine and the gas turbine: overtones of pride and terror, of mystery and hope.” There are still such overtones today.

Enrico Fermi’s first “atomic pile,” literally a flattened spherical pile of graphite blocks plugged with cylinders of purified natural uranium, radiated heat equivalent to some two hundred watts of electricity, no more. The dark, dirty mechanism, its emergency quenching system three young men crouched on top the last layer of graphite, up under the ceiling, balancing buckets of cadmium solution, was designed to prove that a reactor would work, and it barely did—so barely that it required no cooling system and no shielding. It was simplicity itself. The graphite served as a sort of physical catalyst; the uranium did the work.

Uranium purified from ore consists of two isotopes—variant physical forms—in the proportions in which they are found today in nature: U 235, bomb material, an unstable substance continually undergoing radioactive decay, to the extent of seven parts per thousand; and U 238, stable “ordinary” uranium, the preponderant balance. U 235 atoms spontaneously eject neutrons from their nuclei as they decay; collisions with atoms of a suitable moderator can slow some of those neutrons sufficiently to allow other uranium atoms to capture them and, in so doing, to fission; in fissioning—splitting—some of the matter of the uranium is converted into energy in the awesome proportions of Einstein’s famous formula. The fissioning of one uranium atom, minuscule though it is, produces enough energy to make a grain of sand visibly jump.

It happens that the average number of neutrons emitted by a decaying atom of U 235 is slightly more than one. This happenstance suggested, to Fermi and his colleagues, that in a sufficiently “massive assembly of natural uranium and moderator, each decaying atom might fission at least one other atom, and some decaying atoms might fission