Shifting Prime Meridian

If you’ve ever been to the Royal Observatory in Greenwich, London, it might come as a shock to learn that the Prime Meridian line located there is in the wrong place. In fact, it’s out by about 100 metres. But the question is – was prime Meridian always there? It was shifted in the Royal Observatory itself.

Present Day Prime Meridian

Marker of Old Prime Meridian

 

 

 

 

 

 

 

 

 

 

Lines of latitude and longitude began crisscrossing our worldview in ancient times, at least three centuries before the birth of Christ. By a.d. 150, the cartographer and astronomer Ptolemy had plotted them on the twenty-seven maps of his first world atlas. Also for this landmark volume, Ptolemy listed all the place names in an index, in alphabetical order, with the latitude and longitude of each—as well as he could gauge them from travelers’ reports. Ptolemy himself had only an armchair appreciation of the wider world. A common misconception of his day held that anyone living below the Equator would melt into deformity from the horrible heat.

Ptolemy was free, however, to lay his prime meridian, the zero-degree longitude line, wherever he liked. He chose to run it through the Fortunate Islands (now called the Canary & Madeira Islands) off the northwest coast of Africa. Later mapmakers moved the prime meridian to the Azores and to the Cape Verde Islands, as well as to Rome, Copenhagen, Jerusalem, St. Petersburg, Pisa, Paris, and Philadelphia, among other places, before it settled down at last in London. As the world turns, any line drawn from pole to pole may serve as well as any other for a starting line of reference. The placement of the prime meridian is a purely political decision.

In 1884, at the International Meridian Conference held in Washington, D.C., representatives from twenty-six countries voted to make the common practice official. They declared the Greenwich meridian the prime meridian of the world. This decision did not sit well with the French, however, who continued to recognize their own Paris Observatory meridian, a little more than two degrees east of Greenwich, as the starting line for another twenty- seven years, until 1911. (Even then, they hesitated to refer directly to Greenwich mean time, preferring the locution “Paris Mean Time, retarded by nine minutes twenty-one seconds.”)

 

Since the late 19th century, the Greenwich Meridian has been the line at which most maps mark 0° longitude, the starting point for measuring geographical coordinates in an east-west direction. But we now know that the line, a physical representation of which is visited by thousands of tourists every year, should more precisely be 0.001472° (or 102.5 m) further east.

How did the Victorian astronomers who created the Meridian get their calculations wrong? It comes down to the fact that the Earth is not a perfect sphere. In order to determine the precise angle at which to position the line as it ran through the Greenwich Observatory, its creators used early instruments that were aimed vertically at what are called “clock-stars” in the night sky. These are the brighter stars, whose positions have been observed over long periods of time and can be used as reference points in the sky.

To find the exact vertical direction (a line pointing at the precise centre of the Earth’s mass) the Observatory’s astronomers first found the exact horizontal direction (at 90° to the vertical) by looking at the surface of a pool of mercury in a basin.


Today, we have the significant advantage of access to the satellite-based Global Positioning System (GPS), which does not rely on the Earth’s varying gravitational force and uses a more accurate method to calculate the centre of the planet’s mass. This has enabled scientists to determine the true vertical direction and in doing so produced a new meridian slightly to the east of the old one. Because the Earth isn’t a perfect sphere, it was impossible to simply move the new line over and maintain an accurate coordinate system.
This method, however, assumed that the Earth’s gravitational force that created the horizontal surface on the mercury was both uniform and straight down. But because the Earth is not perfectly round and local gravitational forces vary with terrain, the surface of the mercury at Greenwich was not precisely horizontal relative to the centre of the Earth’s mass. As a result, the vertical line to the stars and therefore the meridian line on the ground were slightly skewed.

Does it matter?

So what are the implications of this apparent inaccuracy, particularly given that it is the location from where every place on Earth is measured and from which all clocks are ultimately set? Fortunately, the answer is none, really.

We must remember that the position of the Prime Meridian is actually rather arbitrary and could theoretically be located anywhere. Its location through Greenwich was agreed at the International Meridian Conference of 1884 because it was the most popular candidate. Before this point, roughly ten other prime meridians were also in use, including ones through various other cities including Paris and Cadiz.

Because all important scientific measurements are today made using GPS and not the original location of the Greenwich Meridian, the impact of the error is actually minimal. Arguably, the main issues are confined to the Royal Observatory itself and how it plans to address the issue at the tourist site. There is certainly an argument for a new marker at the “true” Prime Meridian 102m to the east (although being set in one of London’s heavily regulated Royal Parks might make this somewhat problematic).

And where should we envisage the true Prime Meridian? Certainly, the new location is the more accurate line and the one that will be used in the future. But we shouldn’t forget the groundbreaking work that was conducted by scientists in centuries past with only limited tools. The fact that the two lines are just 100m apart is testament to their hard work and ingenuity and so disregarding the old line would be disrespectful. The old line will remain a historic and scientific curiosity, while the new one will allow for ever more accurate navigation within the Earth’s terrestrial, oceanic and atmospheric system.

 

Source(s):

The Conversion

Longitude (Book)

History of Astronomy

About Rashid Faridi

I am Rashid Aziz Faridi ,Writer, Teacher and a Voracious Reader.
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