Antarctic Circle

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Map of the Antarctic with the Antarctic Circle in blue. Antarctic circle.svg
Map of the Antarctic with the Antarctic Circle in blue.

The Antarctic Circle is the most southerly of the five major circles of latitude that mark maps of Earth. The region south of this circle is known as the Antarctic, and the zone immediately to the north is called the Southern Temperate Zone. South of the Antarctic Circle, the Sun is above the horizon for 24 continuous hours at least once per year (and therefore visible at midnight) and the centre of the Sun (ignoring refraction) is below the horizon for 24 continuous hours at least once per year (and therefore not visible at noon); this is also true within the equivalent polar circle in the Northern Hemisphere, the Arctic Circle.

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The position of the Antarctic Circle is not fixed and currently runs 66°33′49.8″ south of the Equator. [1] This figure may be slightly inaccurate because it does not allow for the effects of astronomical nutation, which can be up to 10″. Its latitude depends on the Earth's axial tilt, which fluctuates within a margin of more than 2° over a 41,000-year period, due to tidal forces resulting from the orbit of the Moon. [2] Consequently, the Antarctic Circle is currently drifting southwards at a speed of about 14.5 m (48 ft) per year.

Midnight sun and polar night

Relationship of Earth's axial tilt (e) to the tropical and polar circles Axial tilt vs tropical and polar circles.svg
Relationship of Earth's axial tilt (ε) to the tropical and polar circles

The Antarctic Circle is the northernmost latitude in the Southern Hemisphere at which the centre of the sun can remain continuously above the horizon for twenty-four hours; as a result, at least once each year at any location within the Antarctic Circle the centre of the sun is visible at local midnight, and at least once the centre of the sun is below the horizon at local noon. [3] [4]

Directly on the Antarctic Circle these events occur, in principle, exactly once per year: at the December and June solstices, respectively. However, because of atmospheric refraction and mirages, and because the sun appears as a disk and not a point, part of the midnight sun may be seen on the night of the southern summer solstice up to about 50 minutes (′) (90 km (56 mi)) north of the Antarctic Circle; similarly, on the day of the southern winter solstice, part of the sun may be seen up to about 50′ south of the Antarctic Circle. That is true at sea level; those limits increase with elevation above sea level, although in mountainous regions there is often no direct view of the true horizon. Mirages on the Antarctic continent tend to be even more spectacular than in Arctic regions, creating, for example, a series of apparent sunsets and sunrises while in reality the sun remains below the horizon.

Human habitation

An iceberg near the Antarctic Circle north of Detaille Island Antarctic Circle Icberg.JPG
An iceberg near the Antarctic Circle north of Detaille Island

There is no permanent human population south of the Antarctic Circle, but there are several research stations in Antarctica operated by various nations that are inhabited by teams of scientists who rotate on a seasonal basis. In previous centuries some semi-permanent whaling stations were established on the continent, and some whalers would live there for a year or more. At least eleven children have been born in Antarctica, albeit in stations north of the Antarctic Circle. [5]

Geography

Map all coordinates using: OpenStreetMap

The circumference of the Antarctic Circle is roughly 16,000 kilometres (9,900 mi). [6] The area south of the Circle is about 20,000,000 km2 (7,700,000 sq mi) and covers roughly 4% of Earth's surface. [7] Most of the continent of Antarctica is within the Antarctic Circle.

Sites along the Circle

Starting at the prime meridian and heading eastwards, the Antarctic Circle passes through:

Co-ordinatesCountry, territory or seaNotes
66°34′S0°0′E / 66.567°S 0.000°E / -66.567; 0.000 (Prime Meridian) Southern Ocean North of Queen Maud Land and Enderby Land
66°34′S50°32′E / 66.567°S 50.533°E / -66.567; 50.533 (Antarctica) AntarcticaEnderby Land Territory claimed by Flag of Australia (converted).svg  Australia
66°34′S57°19′E / 66.567°S 57.317°E / -66.567; 57.317 (Southern Ocean) Southern Ocean North of the Amery Ice Shelf
66°34′S82°6′E / 66.567°S 82.100°E / -66.567; 82.100 (Antarctica) Antarctica Territory claimed by Flag of Australia (converted).svg  Australia
66°34′S89°14′E / 66.567°S 89.233°E / -66.567; 89.233 (Southern Ocean) Southern Ocean
66°34′S91°29′E / 66.567°S 91.483°E / -66.567; 91.483 (Antarctica) Antarctica Territory claimed by Flag of Australia (converted).svg  Australia
66°34′S92°21′E / 66.567°S 92.350°E / -66.567; 92.350 (Southern Ocean) Southern Ocean
66°34′S93°52′E / 66.567°S 93.867°E / -66.567; 93.867 (Antarctica) Antarctica Territory claimed by Flag of Australia (converted).svg  Australia
66°34′S107°45′E / 66.567°S 107.750°E / -66.567; 107.750 (Southern Ocean) Southern Ocean Vincennes Bay
66°34′S110°12′E / 66.567°S 110.200°E / -66.567; 110.200 (Antarctica) AntarcticaWilkes Land Territory claimed by Flag of Australia (converted).svg  Australia
66°34′S116°35′E / 66.567°S 116.583°E / -66.567; 116.583 (Southern Ocean) Southern Ocean
66°34′S121°31′E / 66.567°S 121.517°E / -66.567; 121.517 (Antarctica) AntarcticaWilkes Land Territory claimed by Flag of Australia (converted).svg  Australia
66°34′S127°9′E / 66.567°S 127.150°E / -66.567; 127.150 (Southern Ocean) Southern Ocean
66°34′S129°38′E / 66.567°S 129.633°E / -66.567; 129.633 (Antarctica) AntarcticaWilkes Land Territory claimed by Flag of Australia (converted).svg  Australia
66°34′S136°0′E / 66.567°S 136.000°E / -66.567; 136.000 (Antarctica) AntarcticaAdélie Land Territory claimed by Flag of France.svg  France
66°34′S138°56′E / 66.567°S 138.933°E / -66.567; 138.933 (Southern Ocean) Southern Ocean
66°34′S162°44′E / 66.567°S 162.733°E / -66.567; 162.733 Balleny IslandsBorradaile Island Territory claimed by Flag of New Zealand.svg  New Zealand
66°34′S162°45′E / 66.567°S 162.750°E / -66.567; 162.750 (Southern Ocean) Southern Ocean Passing just north of Adelaide Island (claimed by Flag of Argentina.svg  Argentina, Flag of Chile.svg  Chile and Flag of the United Kingdom.svg  United Kingdom)
66°34′S65°44′W / 66.567°S 65.733°W / -66.567; -65.733 (Antarctica) AntarcticaAntarctic Peninsula, Graham Land and Larsen Ice Shelf Territory claimed by Flag of Argentina.svg  Argentina, Flag of Chile.svg  Chile and Flag of the United Kingdom.svg  United Kingdom
66°34′S60°21′W / 66.567°S 60.350°W / -66.567; -60.350 (Southern Ocean) Southern Ocean Passing through the Weddell Sea and into an unnamed part of the ocean

See also

Related Research Articles

<span class="mw-page-title-main">Declination</span> Astronomical coordinate analogous to latitude

In astronomy, declination is one of the two angles that locate a point on the celestial sphere in the equatorial coordinate system, the other being hour angle. The declination angle is measured north (positive) or south (negative) of the celestial equator, along the hour circle passing through the point in question.

<span class="mw-page-title-main">Northern Hemisphere</span> Half of Earth that is north of the Equator

The Northern Hemisphere is the half of Earth that is north of the Equator. For other planets in the Solar System, north is defined as being in the same celestial hemisphere relative to the invariable plane of the Solar System as Earth's North Pole.

A solstice is an event that occurs when the Sun reaches its most northerly or southerly excursion relative to the celestial equator on the celestial sphere. Two solstices occur annually, around June 21 and December 21. In many countries, the seasons of the year are determined by the solstices and the equinoxes.

<span class="mw-page-title-main">Tropic of Cancer</span> Line of northernmost latitude at which the Sun can be directly overhead

The Tropic of Cancer, which is also referred to as the Northern Tropic, is the most northerly circle of latitude on Earth at which the Sun can be directly overhead. This occurs on the June solstice, when the Northern Hemisphere is tilted toward the Sun to its maximum extent. It also reaches 90 degrees below the horizon at solar midnight on the December Solstice. Using a continuously updated formula, the circle is currently 23°26′10.2″ (or 23.43615°) north of the Equator.

<span class="mw-page-title-main">Tropic of Capricorn</span> Line of southernmost latitude at which the sun can be directly overhead

The Tropic of Capricorn is the circle of latitude that contains the subsolar point at the December solstice. It is thus the southernmost latitude where the Sun can be seen directly overhead. It also reaches 90 degrees below the horizon at solar midnight on the June Solstice. Its northern equivalent is the Tropic of Cancer.

<span class="mw-page-title-main">Circumpolar star</span> Star that never sets due to its apparent proximity to a celestial pole

A circumpolar star is a star that, as viewed from a given latitude on Earth, never sets below the horizon due to its apparent proximity to one of the celestial poles. Circumpolar stars are therefore visible from said location toward the nearest pole for the entire night on every night of the year. Others are called seasonal stars.

<span class="mw-page-title-main">Circle of latitude</span> Geographic notion

A circle of latitude or line of latitude on Earth is an abstract east–west small circle connecting all locations around Earth at a given latitude coordinate line.

<span class="mw-page-title-main">Polar circle</span> Circle of latitude

A polar circle is a geographic term for a conditional circular line (arc) referring either to the Arctic Circle or the Antarctic Circle. These are two of the keynote circles of latitude (parallels). On Earth, the Arctic Circle is currently drifting northwards at a speed of about 14.5 m per year and is now at a mean latitude of 66°33′49.8″ N; the Antarctic Circle is currently drifting southwards at a speed of about 14.5 m per year and is now at a mean latitude of 66°33′49.8″ S. Polar circles are often equated with polar regions of Earth. Due to their inherent climate environment, the bulk of the Arctic Circle, much of which is sea, is sparsely settled whereas this applies to all of Antarctica which is mainly land and sheltered ice shelves.

In observational astronomy, culmination is the passage of a celestial object across the observer's local meridian. These events were also known as meridian transits, used in timekeeping and navigation, and measured precisely using a transit telescope.

<span class="mw-page-title-main">Sunset</span> Daily falling of the Sun below the horizon

Sunset is the disappearance of the Sun below the horizon of the Earth due to its rotation. As viewed from everywhere on Earth, it is a phenomenon that happens approximately once every 24 hours, except in areas close to the poles. The equinox Sun sets due west at the moment of both the spring and autumn equinoxes. As viewed from the Northern Hemisphere, the Sun sets to the northwest in the spring and summer, and to the southwest in the autumn and winter; these seasons are reversed for the Southern Hemisphere.

<span class="mw-page-title-main">Midnight sun</span> Natural phenomenon when daylight lasts for a whole day

Midnight sun is a natural phenomenon that occurs in the summer months in places north of the Arctic Circle or south of the Antarctic Circle, when the Sun remains visible at the local midnight. When midnight sun is seen in the Arctic, the Sun appears to move from left to right. In Antarctica, the equivalent apparent motion is from right to left. This occurs at latitudes from 65°44' to 90° north or south, and does not stop exactly at the Arctic Circle or the Antarctic Circle, due to refraction.

<span class="mw-page-title-main">Twilight</span> Atmospheric illumination by the Sun below the horizon

Twilight is light produced by sunlight scattering in the upper atmosphere, when the Sun is below the horizon, which illuminates the lower atmosphere and the Earth's surface. The word twilight can also refer to the periods of time when this illumination occurs.

<span class="mw-page-title-main">Polar night</span> Night lasting for more than 24 hours

Polar night is a phenomenon in the northernmost and southernmost regions of Earth where night lasts for more than 24 hours. This occurs only inside the polar circles. The opposite phenomenon, polar day, or midnight sun, occurs when the Sun remains above the horizon for more than 24 hours.

<span class="mw-page-title-main">Geographical zone</span> Major regions of Earths surface demarcated by latitude

The five main latitude regions of Earth's surface comprise geographical zones, divided by the major circles of latitude. The differences between them relate to climate. They are as follows:

  1. The North Frigid Zone, between the North Pole at 90° N and the Arctic Circle at 66°33′48.7" N, covers 4.12% of Earth's surface.
  2. The North Temperate Zone, between the Arctic Circle at 66°33′48.7" N and the Tropic of Cancer at 23°26'11.3" N, covers 25.99% of Earth's surface.
  3. The Torrid Zone, between the Tropic of Cancer at 23°26'11.3" N and the Tropic of Capricorn at 23°26'11.3" S, covers 39.78% of Earth's surface.
  4. The South Temperate Zone, between the Tropic of Capricorn at 23°26'11.3" S and the Antarctic Circle at 66°33'48.7" S, covers 25.99% of Earth's surface.
  5. The South Frigid Zone, from the Antarctic Circle at 66°33'48.7" S and the South Pole at 90° S, covers 4.12% of Earth's surface.
<span class="mw-page-title-main">Daytime</span> Period of a day in which a location experiences natural illumination

Daytime as observed on Earth is the period of the day during which a given location experiences natural illumination from direct sunlight. Daytime occurs when the Sun appears above the local horizon, that is, anywhere on the globe's hemisphere facing the Sun. In direct sunlight the movement of the sun can be recorded and observed using a sundial that casts a shadow that slowly moves during the day. Other planets and natural satellites that rotate relative to a luminous primary body, such as a local star, also experience daytime, but this article primarily discusses daytime on Earth.

<span class="mw-page-title-main">Sun path</span> Arc-like path that the Sun appears to follow across the sky

Sun path, sometimes also called day arc, refers to the daily and seasonal arc-like path that the Sun appears to follow across the sky as the Earth rotates and orbits the Sun. The Sun's path affects the length of daytime experienced and amount of daylight received along a certain latitude during a given season.

The 66th parallel north is a circle of latitude that is 66 degrees north of the Earth's equatorial plane, about 61 km south of the Arctic Circle. It crosses the Atlantic Ocean, Europe, Asia and North America.

<span class="mw-page-title-main">Equator</span> Imaginary line halfway between Earths North and South poles

The equator is a circle of latitude that divides a spheroid, such as Earth, into the Northern and Southern hemispheres. On Earth, the Equator is an imaginary line located at 0 degrees latitude, about 40,075 km (24,901 mi) in circumference, halfway between the North and South poles. The term can also be used for any other celestial body that is roughly spherical.

<span class="mw-page-title-main">Arctic Circle</span> Boundary of the Arctic

The Arctic Circle is one of the two polar circles, and the most northerly of the five major circles of latitude as shown on maps of Earth at about 66° 34' N. Its southern equivalent is the Antarctic Circle.

The roughly spherical shape of Earth can be empirically evidenced by many different types of observation, ranging from ground level, flight, or orbit. The spherical shape causes a number of effects and phenomena that combined disprove flat Earth beliefs. These include the visibility of distant objects on Earth's surface; lunar eclipses; appearance of the Moon; observation of the sky from altitude; observation of certain fixed stars from different locations; observing the Sun; surface navigation; grid distortion on a spherical surface; weather systems; gravity; and modern technology.

References

  1. "Obliquity of the Ecliptic (Eps Mean)". Neoprogrammics.com. Archived from the original on 2017-06-12. Retrieved 2014-05-13.
  2. Berger, A.L. (1976). "Obliquity and Precession for the Last 5000000 Years". Astronomy and Astrophysics . 51 (1): 127–135. Bibcode:1976A&A....51..127B.
  3. Burn, Chris. The Polar Night (PDF). The Aurora Research Institute. Archived (PDF) from the original on 6 August 2023. Retrieved 28 September 2015.
  4. NB: This refers to the true geometric centre which actually appears higher in the sky because of refraction by the atmosphere.
  5. "World record Baby, it's cold outside". International Antarctic Centre. Retrieved 2024-02-18.
  6. Nuttall, Mark (2004). Encyclopedia of the Arctic Volumes 1, 2 and 3. Routledge. p. 115. ISBN   978-1579584368. Archived from the original on 15 January 2023. Retrieved 26 July 2016.
  7. William M. Marsh; Martin M. Kaufman (2012). Physical Geography: Great Systems and Global Environments. Cambridge University Press. p. 24. ISBN   978-0-521-76428-5. Archived from the original on 2023-01-15. Retrieved 2021-11-27.

66°33′50″S0°0′0″W / 66.56389°S -0.00000°E / -66.56389; -0.00000 (Prime Meridian)