On the
Earth, a 'circle of latitude' is an imaginary
east-
west circle that connects all locations with a given
latitude. A location's position along a circle of latitude is given by its
longitude.
Circles of latitude are often called 'parallels' because they are a fixed distance apart, and on some map projections, including the
Mercator projection, they are drawn parallel. They are also the intersections of the surface of the Earth with parallel planes. The length circles of latitude gets shorter the farther they are from the equator and closer to the
poles.
Arcs of circles of latitude are often used as boundaries between countries or regions that lack distinctive natural borders (e.g. in a desert).
Contrary to what might be assumed from their straight-line representation on some map projections, a circle of latitude is not, with the sole exception of the Equator, the shortest distance between two points lying on it. In other words, circles of latitude are not
great circles, and are not really "lines" in the
geometry of the sphere (see also
great-circle distance). It is for this reason that an aeroplane travelling between a European and North American city on the same latitude will fly further north, over
Greenland for example.
A circle of latitude is perpendicular to all
meridians at the intersection points, and is hence a special case of a
loxodrome.
Major circles of latitude

Diagram of major circles of latitude on the
Earth.
The five major circles of latitude are, from north to south:
★ The
Arctic Circle (66° 33′ 38″ N)
★ The
Tropic of Cancer (23° 26′ 22″ N)
★ The
Equator (0° N)
★ The
Tropic of Capricorn (23° 26′ 22″ S)
★ The
Antarctic Circle (66° 33′ 38″ S)
These circles of latitude (excluding the equator) mark the divisions between the five main
geographical zones.
Equator
The equator is the circle that is equidistant from both the
North Pole and
South Pole.
It divides the Earth into the
Northern Hemisphere and the
Southern Hemisphere.
Arctic and Antarctic Circles
The Arctic Circle marks the southernmost latitude (in the
Northern Hemisphere) at which the sun can remain continuously above or below the horizon for 24 hours. Similarly, the Antarctic Circle marks the northernmost latitude (in the
Southern Hemisphere) at which the sun can remain continuously above or below the horizon for 24 hours.
The latitude of these circles plus the Earth's
axial tilt is equal to 90°.
Tropics of Cancer and Capricorn
The Tropic of Cancer and Tropic of Capricorn respectively mark the northernmost and southernmost latitudes at which the sun may be seen directly overhead (at the
June solstice and
December solstice respectively).
The latitude of the tropic circles is equal to the Earth's
axial tilt.
Movement of the Tropics and the Arctic and Antarctic circles
:''See also:
Axial tilt.''
By definition, the positions of the Tropic of Cancer, Tropic of Capricorn, Arctic Circle and Antarctic Circle all depend on the
tilt of the Earth's axis relative to the plane of its orbit around the sun, known technically as the "obliquity of the ecliptic". As of 2000, the mean value of the tilt was about 23°26′21″. However, this angle is not constant, but has a complex motion determined by the superimposition of many different cycles with short to very long periods. As the axial tilt varies, so do the positions of the Tropics and the Arctic and Antarctic circles.
The main long-term cycle causes the axial tilt to fluctuate between about 22.5° and 24.5° with a 41,000 year periodicity. As a consequence of this cycle the ''average'' value of the tilt is currently decreasing by about 0.47″ per year. This causes the Tropics of Cancer and Capricorn to drift towards the equator by about 15 metres per year, and the Arctic and Antarctic Circles to drift towards the Poles by the same amount. As a result of the movement of the Tropics of Cancer and Capricorn, the area of the
Tropics decreases worldwide by about 1100 square kilometres per year on average.
The Earth's axial tilt is subject to additional shorter-term variations due to
nutation, of which the main term, with a period of 18.7 years, has an amplitude of 9"21 (corresponding to almost 300 metres north and south). There are then still many smaller terms, resulting in varying daily shifts of some metres in any direction.
Finally, the Earth's rotational axis is not exactly fixed with respect to the Earth, but undergoes very small fluctuations, called
polar motion, which have a small theoretical effect on the positions of the abovementioned parallels.
Short-term fluctuations over a matter of days do not directly affect the location of the extreme latitudes at which the sun may appear directly overhead, or at which 24-hour day or night is possible, except when they actually occur at the time of the solstices. Rather, they cause a theoretical shifting of the parallels, that would occur if the given axis tilt were maintained throughout the year.
Other notable parallels