Everything about The Prime Meridian totally explained
The
Prime Meridian is the
meridian (line of
longitude) at which longitude is defined to be 0°.
Unlike the parallels of
latitude, which are defined by the rotational axis of the
Earth (the
poles being 90° and the
Equator 0°), the Prime Meridian is arbitrary. By international convention, the modern Prime Meridian is one passing through
Greenwich,
London,
United Kingdom, known as the
International Meridian or
Greenwich Meridian. Historically, various meridians have been used, including four different ones through Greenwich.
Heading south from the
North Pole, the Prime Meridian first passes through the
United Kingdom (the most northerly land on the meridian is the shore (53°45′34″N) southeast of the Sand-le-Mere caravan park east of
Kingston upon Hull, England). It then passes through
France,
Spain,
Algeria,
Mali,
Burkina Faso,
Togo, and
Ghana, and then through
Queen Maud Land to the
South Pole. The Prime Meridian and the opposite
180th meridian (at 180° longitude), which the
International Date Line generally follows, form a
great circle that divides the Earth into the
Eastern and
Western Hemispheres.
History
The Prime Meridian is ultimately arbitrary — a matter of convention — and various conventions have been used or advocated throughout history:
The Greenwich Meridian, based at the
Royal Observatory, Greenwich, was established by
Sir George Airy in 1851. By 1884, over two-thirds of all ships and tonnage used it as the reference meridian on their maps. In October of that year, at the behest of
U.S. President Chester A. Arthur, 41 delegates from 25 nations met in
Washington, D.C., USA, for the
International Meridian Conference. This conference selected the Greenwich Meridian as the official Prime Meridian due to its popularity. However, France abstained from the vote and French maps continued to use the
Paris Meridian for several decades.
Precise Greenwich Meridian
WGS84 longitudes, which are used by
satellite navigation systems, differ slightly from traditional longitudes. The WGS84 zero meridian is 102.5 metres (336.3 feet) to the east of the line marked at Greenwich.. The offset at other locations can be as much as 30″ east or west.
WGS84 uses the zero meridian as defined by the
Bureau International de l'Heure, which was defined by compilation of star observations in different countries. The plane of this geodetic meridian passes through the centre of the Earth, unlike the plane of the astronomical meridian which contains the direction of gravity (indicated by a
plumb line) which points opposite to the direction of the
zenith, to which astronomical instruments are aligned. The angle between these two meridian planes at the Royal Observatory, the east-west component of
vertical deflection, is 5.31”. The WGS84 datum is an average of the various
continental drifts. As a result, the astronomical meridian between the vertical crosshairs of Airy's transit telescope drifts toward the east as it's carried by the European portion of the Eurasian
tectonic plate, closer to the geodetic meridian, by about one centimetre per year.
Curiously, whether by accident or design, the location of the WGS84 0° meridian is marked in Greenwich by the presence of a waste basket on the path leading more or less due east from the observatory containing the transit telescope.
The zero meridian used by the
Ordnance Survey (
OSGB36 datum) is about six metres to the west of the line marked at Greenwich. This was the standard meridian before 1851, and the Ordnance Survey simply continued to use it.
Universal Time is notionally based on the WGS84 meridian. However, the standard international time
UTC can differ from the mean observed time on the meridian by up to about one second (equivalent to about 280 metres at Greenwich), because of changes in the Earth's rotation.
Leap seconds are inserted periodically to keep UTC in sync with the Earth.
The Greenwich Meridian is now marked at night by a
laser beam emitted from the observatory.
(External Link
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Other planetary bodies
The prime meridians of the following bodies in the
Solar System have been defined:
The prime meridian of the Moon lies directly in the middle of the face of the moon visible from Earth and passes near the crater Bruce.
The 20th meridian of Mercury is defined by a special small crater known as Hun Kal, which is Mayan for 20.
The prime meridian of Mars is defined by the crater Airy-0.Further Information
Get more info on 'Prime Meridian'.
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