North Pole

When not otherwise qualified, the term North Pole usually refers to the Geographic North Pole – the northernmost point on the surface of the Earth, where the Earth's axis of rotation intersects the Earth's surface. Other "North Poles" include:

The Magnetic North Pole – the point on the Earth's surface where the Earth's magnetic field points directly downwards. This pole is constantly wandering; as of 2005 it was located at approximately 82.7° N, 114.4° W.
The Geomagnetic North Pole – the point of intersection of the Earth's surface with the axis of a simple magnetic dipole (like a bar magnet) that best approximates the Earth's actual more complex magnetic field. Like the Magnetic North Pole it constantly wanders; as of 2005 it was located at approximately 79.74°N, 71.78°W.
The Northern Pole of Inaccessibility – the point in the Arctic Ocean farthest from land, at 84°03′N 174°51′W / 84.050°N 174.850°W / 84.050; -174.850.
The North Celestial Pole – an imaginary point in the northern sky towards which the Earth's axis of rotation points.

Originally by analogy with the earth's magnetic field, the terms "north pole" and "south pole" are also applied to magnets in general, in order to distinguish one "end" of the magnet from the other. For this use see under Magnet and Magnetism.

Geographic North Pole

The Geographic North Pole (usually simply called the "North Pole") is, subject to the caveats explained below, defined as one of the two points where the Earth's axis of rotation meets the Earth's surface (the other being the South Pole, diametrically opposite). The Geographic North Pole defines latitude 90° North, as well the direction of True North. At the North Pole all directions point south.

While the South Pole lies on a continental land mass, the North Pole is located in the middle of the Arctic Ocean. There is no land at the North Pole, just waters that are almost permanently covered with constantly shifting sea ice.

The Earth's axis of rotation – and hence the position of the North Pole – was commonly believed to be fixed until, in the 18th century, the mathematician Leonhard Euler predicted that the axis might "wobble" slightly. Around the beginning of the 20th century astronomers noticed a small apparent "variation of latitude", as determined for a fixed point on Earth from the observation of stars. Part of this variation could be attributed to a wandering of the Pole, by a range of a few meters. The wandering has several periodic components and an irregular component. The component with a period of about 435 days is identified with the 8 month wandering predicted by Euler and is now called the Chandler wobble after its discoverer. This "wobble" means that a definition of the Pole based on the axis of rotation is not useful when more than about 1'' precision is required.

It is desirable to tie the system of Earth coordinates (latitude, longitude, and elevations or orography) to fixed landforms. Of course, given continental drift and the rising and falling of land due to volcanos, erosion and so on, there is no system in which all geographic features are fixed. Yet the International Earth Rotation and Reference Systems Service and the International Astronomical Union have defined a framework called the International Terrestrial Reference System that does an admirable job. The North Pole of this system now defines geographic North for precision work, and it does not quite coincide with the rotation axis. See also polar motion.

Expeditions

The Polaris expedition, an American attempt in 1871 led by Charles Francis Hall, ended in disaster.

In April 1895 Fridtjof Nansen reached the latitude 86° 14´ N.

The first expedition to the pole was generally accepted to have been made on April 6, 1909 by Anglo-American Navy engineer Robert Edwin Peary, African-American Matthew Henson, and four Inuit men named Ootah, Shevjenko (who assumed the nickname "Seeglo"), Egingwah, and Ooquesah. However the party that accompanied Peary on the final stage of the journey included no one who was trained in navigation and could independently confirm his own navigational work, which some have controversially claimed to be particularly sloppy as he approached the Pole.

The distances and speeds Peary claimed to have achieved once the last support party turned back border on the incredible, almost three times that which he had accomplished up to that point. Peary's account of a beeline journey to the pole and back -- the only thing that might have allowed him to travel at such a speed -- is contradicted by Henson's account of tortuous detours to avoid pressure ridges and open leads. But the controversy swung back in Peary's favour in 2005 when the British explorer Tom Avery and four companions recreated Peary's journey with replica wooden sleds and Canadian Eskimo Dog teams, reaching the North Pole in 36 days, 22 hours - nearly five hours faster than Peary.

The first undisputed sight of the pole was on May 12 1926 by Norwegian explorer Roald Amundsen and his American sponsor Lincoln Ellsworth from the airship Norge. Norge, though Norwegian owned, was designed and piloted by the Italian Umberto Nobile. The flight started from Svalbard and crossed the icecap to Alaska. Nobile, along with several scientists and crew from the Norge overflew the Pole a second time on May 24 1928 in the Airship Italia.

On May 3, 1952 U.S. Air Force Lieutenant Colonel Joseph O. Fletcher and Lieutenant William P. Benedict landed a plane at the geographic North Pole. Flying with them was scientist Albert P. Crary.

The United States Navy submarine USS Nautilus (SSN-571) crossed the North Pole on August 3, 1958, and on March 17, 1959, the USS Skate (SSN-578) surfaced at the pole, becoming the first naval vessel to reach it.

Sir Wally Herbert led the team that made the first surface crossing of the Arctic Ocean (1968-69) - and by its longest axis - a feat that has never been repeated. In so doing the team became the first to reach the North Geographic Pole by surface travel without the assistance of airlifts. In addition no one alive today has personally surveyed and mapped on the ground a larger area of Antarctica than Sir Wally. He has been awarded the Polar Medal and was knighted in 2000 for services to polar exploration.

Ralph Plaisted made the first confirmed surface conquest of the North Pole on April 19, 1968.

The Soviet nuclear powered icebreaker Arktika on August 17, 1977, completed the first surface vessel journey to the North pole.

In 2005, the United States Navy submarine USS Charlotte (SSN-766) surfaced through 61 inches of ice at the North Pole and spent 18 hours there. [1]

North Magnetic Pole

The North Magnetic Pole is one of several locations on the Earth's surface known as the "North Pole". Its definition, as the point where the geomagnetic field points vertically downwards, i.e. the dip is 90°, was proposed in 1600 by Sir William Gilbert, a courtier of Queen Elizabeth I, and is still used. It should not be confused with the less frequently used North Geomagnetic Pole. Magnetic North is the place to which all magnetic compasses point, although since the pole marked "N" on a bar magnet points north, and only opposite magnetic poles are attracted to each other, the Earth's magnetic north is actually a south magnetic pole.

The orientation of magnetic fields of planets can flip over, an event which is called a geomagnetic reversal. The Earth's poles have done this repeatedly throughout history, and 500,000 years ago, the south magnetic pole was at the South Pole. It is thought that this occurs when the circulation of liquid nickel/iron in the Earth's outer core is disrupted and then reestablishes itself in the opposite direction. It is not known what causes these disruptions. Proof of this can be seen at mid-ocean ridges where tectonic plates move apart, and the sea bed is filled in with magma. As the magma comes out of the mantle, the magnetic particles in it are attracted slightly to the North Pole, and when the poles switch, so does the direction in which the metallic elements face. Therefore, on the sea bed, parallel bands of alternating magnetic fields are found.

The first expedition to reach this pole was led by James Clark Ross, who found it at Cape Adelaide on the Boothia Peninsula on June 1, 1831. Roald Amundsen found Magnetic North in a slightly different location in 1903. The third observation of Magnetic North was by Canadian government scientists Paul Serson and Jack Clark, of the Dominion Astrophysical Observatory, who found the pole at Allen Lake on Prince of Wales Island.

The Canadian government has made several measurements since, which show that the North Magnetic Pole is continually moving northwest. In 1996 an expedition certified its location by magnetometer and theodolite at 78°35.7′N 104°11.9′W / 78.5950°N 104.1983°W / 78.5950; -104.1983. Its location (in 2005) is 82°07′N 114°04′W / 82.117°N 114.067°W / 82.117; -114.067, near Ellesmere Island, the biggest of the Queen Elizabeth Islands, in Canada. During the 20th century it has moved 1100 km, and since 1970 its rate of motion has accelerated from 9 km/year to 41 km/year (2001-2003 average; see also Polar drift). If it maintains its present speed and direction it will reach Siberia in about 50 years, but it is expected to veer from its present course and slow down.

This movement is on top of a daily or diurnal variation in which Magnetic North describes a rough ellipse, with a maximum deviation of 80 km from its mean position. This effect is due to disturbances of the geomagnetic field by the sun. A line drawn from one magnetic pole to the other does not go through the centre of the Earth; it actually misses it by about 530 km.

The angular difference between Magnetic North and true North varies with location, and is called the magnetic declination.

North Geomagnetic Pole

The North Geomagnetic Pole is the pole of the Earth's geomagnetic field closest to true north. The first-order approximation of the Earth's magnetic field is that of a single magnetic dipole (like a bar magnet), tilted about 11° with respect to Earth's rotation axis and centered at the Earth's core. The residuals form the nondipole field. The Geomagnetic poles are the places where the axis of this dipole intersects the Earth's surface. Because the dipole approximation is far from a perfect fit to the Earth's magnetic field, the magnetic field is not quite vertical at the geomagnetic poles. The locations of true vertical field orientation are the magnetic poles, and these are about 30 degrees of longitude away from the geomagnetic poles.

Like the North Magnetic Pole, the geomagnetic north pole is a south magnetic pole, because it attracts the north pole of a bar magnet. It is the centre of the region in the magnetosphere in which the Aurora Borealis can be seen. Its present location is 78°30′N 69°00′W / 78.5°N 69°W / 78.5; -69, near Qaanaaq in Greenland, however it is now drifting away from North America and toward Siberia. The first voyage to this pole was by David Hempleman-Adams in 1992.

Northern Pole of Inaccessibility

The Northern Pole of Inaccessibility, located at 84°03′N 174°51′W / 84.050°N 174.850°W / 84.050; -174.850, is the point farthest from any northern coastline, about 1100 km from the nearest coast. It is a geographic construct, not an actual physical phenomenon. It was first reached by Sir Hubert Wilkins, who flew by aircraft in 1927; in 1958 a Russian icebreaker reached this point.

Defining North Poles in astronomy

Astronomers define the north "geographic" pole of a planet or other object in the solar system by the planetary pole that is in the same ecliptic hemisphere as the Earth's north pole. More accurately, «The north pole is that pole of rotation that lies on the north side of the invariable plane of the solar system» [2]. This means some objects will have directions of rotation opposite the "normal" (i.e., not counter-clockwise as seen from above the north pole). Another frequently used definition uses the right-hand rule to define the north pole: it is then the pole around which the object rotates counterclockwise [3]. When using the first definition (the IAU's), an object's axial tilt will always be 90° or less, but its rotation period may be negative (retrograde rotation); when using the second definition, axial tilts may be greater than 90° but rotation periods will always be positive.

For the magnetic poles, their names are decided upon by the direction that their field lines emerge or enter the planet's crust. If they enter the same way as they do for Earth at the north pole, we call this the planet's north magnetic pole.

Some bodies in the solar system, including Saturn's moon Hyperion and the asteroid 4179 Toutatis, lack a stable geographic north pole. They rotate chaotically because of their irregular shape and gravitational influences from nearby planets and moons, and as a result the instantaneous pole wanders over their surface, and may vanish altogether for brief periods (when the object comes to a complete standstill with respect to the distant stars).

The projection of a planet's north geographic pole onto the celestial sphere gives its north celestial pole.

In the particular (but frequent) case of synchronous satellites, four more poles can be defined. They are the near, far, leading, and trailing poles. Take Io for example; this moon of Jupiter rotates synchronously, so its orientation with respect to Jupiter stays constant. There will be a single, unmoving point of its surface where Jupiter is at the zenith, exactly overhead —this is the near pole, also called the sub- or pro-Jovian point. At the antipode of this point is the far pole, where Jupiter lies at the nadir; it is also called the anti-Jovian point. There will also be a single unmoving point which is furthest along Io's orbit (best defined as the point most removed from the plane formed by the north-south and near-far axes, on the leading side) —this is the leading pole. At its antipode lies the trailing pole. Io can thus be divided into north and south hemispheres, into pro- and anti-Jovian hemispheres, and into leading and trailing hemispheres. Note that these poles are mean poles because the points are not, strictly speaking, unmoving: there is constant jiggling about the mean orientation, because Io's orbit is slightly eccentric and the gravity of the other moons disturbs it regularly.

Day and night

During the summer months, the North Pole experiences twenty-four hours of daylight daily but during the winter months the North Pole experiences twenty-four hours of darkness daily. Sunrise and sunset do not occur in a twenty-four hour cycle. At the north pole, sunrise begins at the Vernal equinox taking three months for the sun to reach its highest point at the summer solstice when sunset begins, taking three months to reach sunset at the Autumnal equinox. A similar effect can be observed at the South Pole, with a six month difference. This day/night effect is in stark contrast to what is observed at the Equator.

This effect is caused by a combination of the Earth's axial tilt and its rotation around the sun. The direction and angle of axial tilt of the Earth remains fairly constant (on a yearly basis) in its plane of rotation around the sun. Hence during the summer, the North Pole is always facing the sun's rays but during the winter, it always faces away from the sun.

Territorial claims to the North Pole (Arctic)

In 1925, based upon the Sector Principle, Canada became the first country to extend its boundaries northward to the North Pole, at least on paper, between 60°W and 141°W longitude, a claim that is not universally recognized (there is in fact 770 km of ocean between the pole and Canada's northernmost land point). In addition, Canada claims the water between its Arctic Islands as internal waters. The claim is not recognized by the United States, which argues the Northwest Passage is an international waterway, despite its minimal usage for shipping. Denmark (Greenland), Russia and Norway have made similar claims, which are also opposed by the United States.

Otherwise, until 1999, the North Pole and Arctic Ocean had been generally considered international territory. However, as the polar ice has begun to recede at a rate higher than expected (see global warming), several countries have made moves to claim, or to enforce pre-existing claims to, the waters or seabed at the Pole. Russia made its first claim in 2001, claiming Lomonosov Ridge, an underwater mountain ridge underneath the Pole, as a natural extension of Siberia. This claim was contested by Norway, Canada, the United States and Denmark in 2004. The Danish autonomous province of Greenland has the nearest coastline to the North Pole, and Denmark argues the Lomonosov Ridge is in fact an extension of Greenland.

The potential value of the North Pole and the area around resides not so much in shipping but in the possibility that lucrative petroleum and natural gas reserves exist below the sea floor. Such reserves are known to exist under the Beaufort Sea, and further exploration elsewhere in the Arctic might become more feasible if global warming opens up the Northwest Passage as a regular channel of international shipping and commerce, particularly if Canada is not able to enforce her claim to it.

Magnetic declination

Magnetic north is determined by the earth’s magnetic field and is not the same as true (or geographic) north. The location of the magnetic north pole changes slowly over time, but it is currently northwest of Hudson Bay in northern Canada (approximately 700 km [450 mi] from the true north pole). Maps are based on the geographic north pole because it does not change over time, so north is always at the top of a quadrangle map. However, the direction indicated as north by a compass needle does not correspond to the north marked on a map. The angle between a straight north-south line and the north indicated by the compass is called the magnetic declination, and varies from place to place.

Magnetic declination has been measured throughout many countries, including the U.S, and can be corrected for on a compass. The line of zero declination in the U.S. runs from magnetic north through Lake Superior and across the western panhandle of Florida. Along this line, true north is the same as magnetic north. West of the line of zero declination, a compass will give a reading that is east of true north. Conversely, east of the line of zero declination, a compass reading will be west of true north. The exact amount by which the declination of the compass needs to be adjusted to reconcile magnetic north to true north is given in the map legend to the left of the map scale.

Cultural references to the North Pole

In many versions of the Santa Claus mythos, the North Pole is the place where Santa Claus lives, and where his workshop is located.

References

External links

Arctic Council
The Northern Forum
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North Pole Web Cam
The short Arctic summer of 2004
The puzzling Arctic summer of 2003
FAQ on the Arctic and the North Pole
Polar Controversies Still Rage article by Roderick Eime
Magnetic Poles locations since 1600 Download the KMZ file. For Google Earth Users.
The Polar Race a biennial race to the 1996 certified position of the Magnetic North Pole
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Daylight, Darkness and Changing of the Seasons at the North Pole

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