Noon Was a Place

For most of human history, noon was something that happened to a town, not a number on a dial. Then the trains came.

Noon used to happen to a place. The sun climbed, reached the top of its arc over one particular town, and for a moment the shadows stood straight down and short. That was noon. It belonged to the ground it fell on, the way weather did.

Travel east and noon came earlier. Travel west and it came later. Every settlement with a clock kept its own reading of the sky, and the readings disagreed politely, a few minutes at a time, all the way across the continent. Before 1883, North America ran on more than 144 local times1. A traveler crossing the country did not pass through an afternoon. He passed through hundreds of slightly different afternoons, each one locally correct.

None of this was a problem while everything moved at walking speed. A four minute discrepancy between two towns matters to nobody when the trip between them takes two days. The discrepancy only becomes visible when the machine connecting the towns moves faster than the difference. Then it becomes dangerous.

The railroads found this out in the worst available way. By 1883 the companies were scheduling trains against 56 different standards of time at once, and the front page of the New York Times was complaining about it in print2. Conductors carried conversion tables. Two trains on one track, running toward each other under two honest clocks, could both be on time and meet in the middle. The sun was a fine timekeeper for a village. It was a poor one for a network.

So the railroads did something no government had managed. On Sunday, November 18, 1883, at noon, they stopped the sun.

William F. Allen, secretary of the General Time Convention, had drawn the replacement: four zones, each pinned to a meridian fifteen degrees from the next, the 75th, the 90th, the 105th, the 120th. Inside a zone, every clock would read the same. When the telegraph signal went out that day, station clocks across the continent were reset to the new noon, and towns that had already watched the sun cross got to watch the hands do it again. The newspapers named it the Day of Two Noons3.

Crowds gathered at depots to watch the clock hands move. Think about what they were watching. Not a machine being repaired. A definition being repealed. For the whole of recorded history, noon had been a measurement, the sun reporting its position. After that Sunday, noon was an agreement. The sky kept doing what it had always done. It had simply been outvoted.

The government caught up thirty five years later. The Standard Time Act of 1918 wrote the railroad arrangement into federal law, which is the usual order of things: the network builds the standard, the state arrives to notarize it4.

The costs were real and mostly invisible, which is why nobody itemizes them. A town at the western edge of a zone now eats lunch an hour before its sun reaches the top of the sky. A town at the eastern edge eats in what its sky calls mid morning. Both call it noon, and both are right, because right stopped meaning the sun a long time ago. China took the logic to its end in 1949 and put the entire country, five zones wide, on a single Beijing time5. In the far west of that country the clock says noon close to three hours before the sun agrees. The agreement holds anyway. That is what agreements do.

The trade was worth it, and the trains stopped meeting in the middle. Then the telegraph, then the telephone exchange, then the power grid, then everything else that hums in sequence moved onto the shared fiction, and the fiction became load bearing. Remove it now and the failure would not look like confusion. It would look like silence, one system at a time.

The modern phone finishes the job the railroads started. It does not ask the sun anything. It asks a server, which asks an atomic clock, which counts the vibrations of cesium atoms and reports a number that no sky ever produced. The satellites overhead carry clocks corrected for the fact that time itself runs at different rates at different altitudes and speeds, a correction no stationmaster ever had to make. Your noon is now delivered from orbit, averaged, adjusted, and entirely indifferent to the shadow at your feet.

The sundial in the garden still works. It still reports the old noon, the local one, the one that belongs to that patch of ground. It is not wrong. It is answering a question nobody asks anymore, with perfect accuracy, in a language the network retired in 1883.

Stand in a field at the western edge of your time zone on a clear day and watch the shadows shorten toward a noon the clock reached an hour ago. The sun is late to its own appointment, and it has been late since a Sunday in 1883, when the trains decided that a shared fiction beats a local fact, and the whole world, eventually, agreed to be on time for something the sky never scheduled.

1.Bureau of Transportation Statistics, “History of Time Zones and Daylight Saving Time”: before zones were established in 1883, North America had more than 144 local times. bts.gov

2.“Fifty six standards of time are now employed by the various railroads of the country in preparing their schedules of running times,” New York Times, April 19, 1883, as quoted in accounts of the standardization fight. thoughtco.com

3.Library of Congress, “The Day of Two Noons”: on November 18, 1883, railroad station clocks were reset as standard time noon was reached in each zone, so some places marked noon twice. guides.loc.gov

4.The Standard Time Act of 1918 gave the Interstate Commerce Commission authority over zone boundaries and adopted five official zones; the Department of Transportation took over time zone regulation in 1966. bts.gov

5.China moved from five time zones to one, Beijing Time, in 1949, a decision made in the name of national unity. interestingfacts.com