Facts and Figures about Time Zones

What are time zones and why do we have them?

In order to efficiently use and measure time, everyone in the world would like to fix noon as the time at which the sun is at its highest point in the sky (i.e. when it is crossing the meridian). However, this seems to be impossible without the use of time zones. Since the Earth rotates at the rate of 15 degrees every hour, the sun is at its highest point in the sky at different times in the day for different countries around the globe. The idea behind time zones is that we can divide the world into 24 equal slices or zones, 15 degrees each, and adjust the clocks accordingly for each zone. We can thus preserve the need to fix noon as the time when the sun is highest in the sky for each country and yet also make it easy to understand times between different zones. The person who famously proposed this was Sir Sanford Fleming, a Scottish-born Canadian, in the late 19th century. Although well-received, this system would only be instituted worldwide in 1929, establishing arguably the most crucial system of the modern world.

How does it all work?

Time zones are measured by reference to a specific point, namely the Greenwich Meridian. This is sometimes called the Prime Meridian, and it is located at the Royal Observatory in Greenwich, England. We have commonly referred to time at this point as Greenwich Mean Time or Universal Time (abbreviated as GMT), though in recent years it has been used to refer to the more accurate Coordinated Universal Time (abbreviated as UTC) which uses an atomic time scale. UTC is used as a starting point to determine time in other countries worldwide. So, for example, if a country is stated as having the time UTC+3, this means that when it is noon in Greenwich, it is 3pm in that country.

Major world cities and their time zones

Beijing: UTC+8
Brussels: UTC+1
Buenos Aires: UTC-3
Cairo: UTC+2
Jakarta: UTC+7
London (U.K.): UTC
Los Angeles: UTC-8
Madrid: UTC+1
Melbourne: UTC-10
Mexico City: UTC-6
Moscow: UTC+3
New Delhi: UTC+5.30
New York: UTC-5
Paris: UTC+1
Rome: UTC+1
Sydney: UTC+10
Tokyo: UTC+9
Washington DC: UTC-5

The International Date Line

The International Date Line (IDL) is an imaginary line on the opposite side of the world from the Prime Meridian. It is 180 degrees both East and West from Greenwich, which means that on either side of the line it is a different day. This is because the IDL intersects the time zones which are UTC+12 and UTC-12. Even though the IDL mostly passes through the ocean, it could quite easily confuse travellers who experience a change in day just by crossing over. The position of the IDL has in fact changed several times since time zones were introduced. It has been made to zig-zag around countries so no one on land is affected, though this still creates problems for those flying or sailing through. Crossing it whilst travelling East means subtracting a day, and crossing it whilst travelling West means adding a day. To illustrate this often confusing notion, if you fly from Tonga to Samoa by air, the journey takes approximately two hours, but the passenger officially arrives the day before they left.

Interesting facts about time zones

Advice for travellers

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