'Latitude', usually denoted symbolically by the Greek letter
phi,
, gives the location of a place on
Earth north or south of the
equator. Lines of Latitude are the horizontal lines shown running east-to-west on maps. Technically, Latitude is an
angular measurement in
degrees (marked with °) ranging from 0° at the Equator (low latitude) to 90° at the poles (90° N for the
North Pole or 90° S for the
South Pole; high latitude). The
complementary angle of a latitude is called the '
colatitude'.
Circles of latitude
Main articles: Circle of latitude
All locations of a given latitude are collectively referred to as a ''
circle of latitude'' or ''line of latitude'' or ''parallel'', because they are
coplanar, and all such
planes are
parallel to the
equator. Lines of latitude other than the Equator are approximately
small circles on the surface of the Earth; they are not
geodesics since the shortest route between two points at the same latitude involves moving farther away from, then towards, the equator (see
great circle).
A specific latitude may then be combined with a specific
longitude to give a precise position on the Earth's surface (see
satellite navigation system).
Important named circles of latitude
Besides the equator, four other lines of latitude are named because of the role they play in the geometrical relationship with the Earth and the Sun:
★
Arctic Circle — 66° 33′ 39″ N
★
Tropic of Cancer — 23° 26′ 21″ N
★
Tropic of Capricorn — 23° 26′ 21″ S
★
Antarctic Circle — 66° 33′ 39″ S
Only at latitudes between the Tropics is it possible for the
sun to be at the
zenith. Only north of the
Arctic Circle or south of the
Antarctic Circle is the
midnight sun possible.
The reason that these lines have the values that they do lies in the
axial tilt of the Earth with respect to the sun, which is
23° 26′ 21.41″.
Note that the Arctic Circle and Tropic of Cancer and the Antarctic Circle and Tropic of Capricorn are colatitudes since the sum of their angles is 90°.
Subdivisions
As Earth is not a smooth
sphere, but slightly
oblate, a degree of latitude varies in length from about 111.3195 km at the equator to 110.9462 km at the poles.
A
degree of arc at a latitude not only varies with latitude, but also with the direction being faced. To simplify calculations where elliptical consideration is not important, the
nautical mile was created, equaling exactly 111.12 km per degree of arc or, sub-dividing into
minutes, 1852
metres per minute of arc. One minute of latitude can be further divided into 60 seconds. A latitude is thus specified as 13°19'43″ N (for greater precision, a decimal fraction can be added to the seconds). An alternative representation uses only degrees and minutes, where the seconds are expressed as a decimal fraction of minutes, thus the above example is expressed as 13°19.717' N. Degrees can also be expressed singularly, with both the minutes and seconds incorporated as a decimal number and rounded as desired (decimal degree notation): 13.32861° N. Sometimes, the north/south suffix is replaced by a negative sign for south (−90° for the
South Pole).
Effect of latitude
A region's latitude has a great effect on its
climate and
weather (see
Effect of sun angle on climate). Latitude more loosely determines tendencies in
polar auroras,
prevailing winds, and other physical characteristics of geographic locations.
Researchers at
Harvard's Center for International Development (CID) found in 2001 that only three
tropical economies —
Hong Kong,
Singapore, and part of
Taiwan — were classified as high-income by the
World Bank, while all countries within regions zoned as
temperate had either middle- or high-income economies.
[1]
Types of latitude
Because the
Earth is slightly flattened by its rotation, cartographers refer to a variety of auxiliary latitudes to precisely adapt spherical projections according to their purpose.
More generally, for other planets such as
Mars, geographic and geocentric latitude are called "planetographic" and "planetocentric" latitude, respectively. Most maps of Mars since 2002 use planetocentric coordinates.
Common "latitude"
★ In common usage, "latitude" refers to 'geodetic' or 'geographic latitude'
and is the angle between the
equatorial plane and a line that is
normal to the reference
spheroid, which approximates the shape of the
Earth to account for flattening of the poles and bulging of the equator.
The expressions following assume
elliptical polar sections with the '
angular eccentricity',
(which equals
, where
and
are the equatorial and polar radii), and that all sections parallel to the equatorial plane are circular. Geographic latitude (with longitude) then provides a
Gauss map.
Utilized in some of these conversions is a common elliptic
integrand:
::
Reduced latitude
★ 'Reduced' or 'parametric latitude',
, is the latitude of the same radius on the
sphere with the same equator.
::
Authalic latitude
★ 'Authalic latitude',
, gives an area-preserving transform to the sphere.
::
::
Rectifying latitude
★ 'Rectifying latitude',
, is the surface distance from the equator, scaled so the pole is 90°. Unfortunately, it involves
elliptic integration:
::
:::
Conformal latitude
★ 'Conformal latitude',
, gives an angle-preserving (
conformal) transform to the sphere.
::
Geocentric latitude
★ The 'geocentric latitude',
, is the angle between the equatorial plane and a line from the center of the
Earth.
::
Comparison of latitudes
The following plot shows the differences between the types of latitude. The data used is found in the table following the plot. Please note that the values in the table are in minutes, not degrees, and the plot reflects this as well. Also note that the conformal symbols are hidden behind the geocentric due to being very close in value.
:
| Approximate difference from geographic latitude ("Lat") |
|---|
Lat
| Reduced
| Authalic
| Rectifying
| Conformal
| Geocentric
|
|---|---|---|---|---|---|
| 0° | 0.00′ | 0.00′ | 0.00′ | 0.00′ | 0.00′ |
| 5° | 1.01′ | 1.35′ | 1.52′ | 2.02′ | 2.02′ |
| 10° | 1.99′ | 2.66′ | 2.99′ | 3.98′ | 3.98′ |
| 15° | 2.91′ | 3.89′ | 4.37′ | 5.82′ | 5.82′ |
| 20° | 3.75′ | 5.00′ | 5.62′ | 7.48′ | 7.48′ |
| 25° | 4.47′ | 5.96′ | 6.70′ | 8.92′ | 8.92′ |
| 30° | 5.05′ | 6.73′ | 7.57′ | 10.09′ | 10.09′ |
| 35° | 5.48′ | 7.31′ | 8.22′ | 10.95′ | 10.96′ |
| 40° | 5.75′ | 7.66′ | 8.62′ | 11.48′ | 11.49′ |
| 45° | 5.84′ | 7.78′ | 8.76′ | 11.67′ | 11.67′ |
| 50° | 5.75′ | 7.67′ | 8.63′ | 11.50′ | 11.50′ |
| 55° | 5.49′ | 7.32′ | 8.23′ | 10.97′ | 10.98′ |
| 60° | 5.06′ | 6.75′ | 7.59′ | 10.12′ | 10.13′ |
| 65° | 4.48′ | 5.97′ | 6.72′ | 8.95′ | 8.96′ |
| 70° | 3.76′ | 5.01′ | 5.64′ | 7.52′ | 7.52′ |
| 75° | 2.92′ | 3.90′ | 4.39′ | 5.85′ | 5.85′ |
| 80° | 2.00′ | 2.67′ | 3.00′ | 4.00′ | 4.01′ |
| 85° | 1.02′ | 1.35′ | 1.52′ | 2.03′ | 2.03′ |
| 90° | 0.00′ | 0.00′ | 0.00′ | 0.00′ | 0.00′ |
Astronomical latitude
A more obscure measure of latitude is the 'astronomical latitude', which is the angle between the equatorial plane and the
normal to the
geoid (ie a plumb line). It originated as the angle between horizon and pole star.
Astronomical latitude is not to be confused with
declination, the coordinate
astronomers use to describe the locations of stars north/south of the
celestial equator (see
equatorial coordinates), nor with
ecliptic latitude, the coordinate that astronomers use to describe the locations of stars north/south of the
ecliptic (see
ecliptic coordinates).
Palæolatitude
Continents move over time, due to
continental drift, taking whatever fossils and other features of interest they may have with them. Particularly when discussing fossils, it's often more useful to know where the fossil was when it was laid down, than where it is when it was dug up: this is called the ''palæolatitude'' of the fossil. The Palæolatitude can be constrained by
palæomagnetic data. If tiny magnetisable grains are present when the rock is being formed, these will align themselves with the Earth's magnetic field like compass needles. A
magnetometer can deduce the orientation of these grains by subjecting a sample to a magnetic field, and the
declination of the grains can be used to infer the latitude of deposition.
Further reading
★ John P. Snyder ''Map Projections: a working manual''
excerpts
See also
★
Cardinal direction
★
Geographic coordinate system
★
Geodetic system
★
Geodesy
★
Geotagging
★
Great-circle distance
★
Horse latitudes
★
List of cities by latitude
★
List of cities by longitude
★
Longitude
★
Navigation
★
World Geodetic System
Footnotes
1. Location, Location, Location. The relationship of climate to, and the effect of disease and agricultural productivity on, the economic success of a city or region.
References
★
Brain size, cranial morphology, climate, and time machines, Beals, K. L., Smith, C. L. & Dodd, S. M., , , Current Anthropology, 1984
★
The evolution of racial differences in intelligence, Lynn, R., , , Mankind Quarterly, 1991
External links
★
★
Free GeoCoder
★
GEONets Names Server, access to the
National Geospatial-Intelligence Agency's (NGA) database of foreign geographic feature names.
★
Look-up Latitude and Longitude
★
Resources for determining your latitude and longitude
★
Convert decimal degrees into degrees, minutes, seconds - Info about decimal to
sexagesimal conversion
★
Convert decimal degrees into degrees, minutes, seconds
★
Latitude and longitude converter – Convert latitude and longitude from degree, decimal form to degree, minutes, seconds form and vice versa. Also included a farthest point and a distance calculator.
★
Worldwide Index - Tageo.com – contains 2,700,000 coordinates of places including US towns
★
★ for each city it gives the satellite map location, country, province, coordinates (dd,dms), variant names and nearby places.
★
Distance calculation based on latitude and longitude - JavaScript version
★