Equator
View on Wikipedia


The equator is the circle of latitude that divides Earth into the Northern and Southern hemispheres. It 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.[1] The term can also be used for any other celestial body that is roughly spherical.
In spatial (3D) geometry, as applied in astronomy, the equator of a rotating spheroid (such as a planet) is the parallel (circle of latitude) at which latitude is defined to be 0°. It is an imaginary line on the spheroid, equidistant from its poles, dividing it into northern and southern hemispheres. In other words, it is the intersection of the spheroid with the plane perpendicular to its axis of rotation and midway between its geographical poles.
On and near the equator (on Earth), noontime sunlight appears almost directly overhead (no more than about 23° from the zenith) every day, year-round. Consequently, the equator has a rather stable daytime temperature throughout the year. On the equinoxes (approximately 20 March and 23 September) the subsolar point crosses Earth's equator at a shallow angle, sunlight shines perpendicular to Earth's axis of rotation, and all latitudes have nearly a 12-hour day and 12-hour night.[2]
Etymology
[edit]The name is derived from medieval Latin word aequator, in the phrase circulus aequator diei et noctis, meaning 'circle equalizing day and night', from the Latin word aequare 'make equal'.[3]
Overview
[edit]Right: Road sign marking the equator near Nanyuki, Kenya
The latitude of the Earth's equator is, by definition, 0° (zero degrees) of arc. The equator is one of the five notable circles of latitude on Earth; the other four are the two polar circles (the Arctic Circle and the Antarctic Circle) and the two tropical circles (the Tropic of Cancer and the Tropic of Capricorn). The equator is the only line of latitude which is also a great circle—meaning, one whose plane passes through the center of the globe. The plane of Earth's equator, when projected outwards to the celestial sphere, defines the celestial equator.
In the cycle of Earth's seasons, the equatorial plane runs through the Sun twice a year: on the equinoxes in March and September. To a person on Earth, the Sun appears to travel along the equator (or along the celestial equator) at these times.


Locations on the equator experience the shortest sunrises and sunsets because the Sun's daily path is nearly perpendicular to the horizon for most of the year. The length of daylight (sunrise to sunset) is almost constant throughout the year; it is about 14 minutes longer than nighttime due to atmospheric refraction and the fact that sunrise begins (or sunset ends) as the upper limb, not the center, of the Sun's disk contacts the horizon.
Earth bulges slightly at the equator; its average diameter is 12,742 km (7,918 mi), but the diameter at the equator is about 43 km (27 mi) greater than at the poles.[1]
Sites near the equator, such as the Guiana Space Centre in Kourou, French Guiana, are good locations for spaceports as they have the fastest rotational speed of any latitude, 460 m (1,509 ft)/sec. The added velocity reduces the fuel needed to launch spacecraft eastward (in the direction of Earth's rotation) to orbit, while simultaneously avoiding costly maneuvers to flatten inclination during missions such as the Apollo Moon landings.[4]
Geodesy
[edit]Precise location
[edit]The precise location of the equator is not truly fixed; the true equatorial plane is perpendicular to the Earth's rotation axis, which drifts about 9 metres (30 ft) during a year.
Geological samples show that the equator significantly changed positions between 48 and 12 million years ago, as sediment deposited by ocean thermal currents at the equator shifted. The deposits by thermal currents are determined by the axis of Earth, which determines solar coverage of Earth's surface. Changes in Earth's axis can also be observed in the geographical layout of volcanic island chains, which are created by shifting hot spots under Earth's crust as the axis and crust move.[5] This is consistent with the Indian tectonic plate colliding with the Eurasian tectonic plate, which is causing the Himalayan uplift.
Exact length
[edit]The International Association of Geodesy (IAG) and the International Astronomical Union (IAU) use an equatorial radius of 6,378.1366 km (3,963.1903 mi) (codified as the IAU 2009 value).[6] This equatorial radius is also in the 2003 and 2010 IERS Conventions.[7] It is also the equatorial radius used for the IERS 2003 ellipsoid. If it were really circular, the length of the equator would then be exactly 2π times the radius, namely 40,075.0142 km (24,901.4594 mi). The GRS 80 (Geodetic Reference System 1980) as approved and adopted by the IUGG at its Canberra, Australia meeting of 1979 has an equatorial radius of 6,378.137 km (3,963.191 mi). The WGS 84 (World Geodetic System 1984) which is a standard for use in cartography, geodesy, and satellite navigation including GPS, also has an equatorial radius of 6,378.137 km (3,963.191 mi). For both GRS 80 and WGS 84, this results in a length for the equator of 40,075.0167 km (24,901.4609 mi).
The geographical mile is defined as one arc-minute of the equator, so it has different values depending on which radius is assumed. For example, by WSG-84, the distance is 1,855.3248 metres (6,087.024 ft), while by IAU-2000, it is 1,855.3257 metres (6,087.027 ft). This is a difference of less than one millimetre (0.039 in) over the total distance (approximately 1.86 kilometres or 1.16 miles).
Earth is commonly modeled as a sphere flattened 0.336% along its axis. This makes the equator 0.16% longer than a meridian (a great circle passing through the two poles). The IUGG standard meridian is, to the nearest millimetre, 40,007.862917 kilometres (24,859.733480 mi), one arc-minute of which is 1,852.216 metres (6,076.82 ft), explaining the SI standardization of the nautical mile as 1,852 metres (6,076 ft), more than 3 metres (9.8 ft) less than the geographical mile.
The sea-level surface of Earth (the geoid) is irregular, so the actual length of the equator is not so easy to determine. Aviation Week and Space Technology on 9 October 1961 reported that measurements using the Transit IV-A satellite had shown the equatorial diameter from longitude 11° West to 169° East to be 300 metres (1,000 ft) greater than its diameter ninety degrees away.[8]
Equatorial countries and territories
[edit]


The equator passes over approximately 8714 km of land (21.7%) and 31,361 km of sea (78.3%).[10] It passes through the land of eleven sovereign states. Indonesia is the country straddling the greatest length of the equatorial line across both land and sea. Starting at the Prime Meridian and heading eastwards, the equator passes through:
The equator also passes through the territorial seas of three countries: Maldives (south of Gaafu Dhaalu Atoll), Kiribati (south of Buariki Island), and the United States (south of Baker Island).
Despite its name, no part of Equatorial Guinea lies on the equator. However, its island of Annobón is 155 km (96 mi) south of the equator, and the rest of the country lies to the north. France (Mayotte, Réunion), Norway (Bouvet Island), and the United Kingdom (British Antarctic Territory, British Indian Ocean Territory, Falkland Islands, Pitcairn Islands, Saint Helena, Ascension and Tristan da Cunha, South Georgia and the South Sandwich Islands) are the other three Northern Hemisphere-based countries which have territories in the Southern Hemisphere.
Equatorial seasons and climate
[edit]
Diagram of the seasons, showing the situation at the December solstice. Regardless of the time of day (i.e. Earth's rotation on its axis), the North Pole will be dark, and the South Pole will be illuminated; see also polar night and polar day. In addition to the density of incident light, the dissipation of light in the atmosphere is greater when it falls at a shallow angle. Note that the equator is not under the subsolar point during this time of year.
Seasons result from the tilt of Earth's axis away from a line perpendicular to the plane of its revolution around the Sun. Throughout the year, the Northern and Southern hemispheres are alternately turned either toward or away from the Sun, depending on Earth's position in its orbit. The hemisphere turned toward the Sun receives more sunlight and is in summer, while the other hemisphere receives less sun and is in winter (see solstice).
At the equinoxes, Earth's axis is perpendicular to the Sun rather than tilted toward or away, meaning that day and night are both about 12 hours long across the whole of Earth.
Near the equator, this means the variation in the strength of solar radiation is different relative to the time of year than it is at higher latitudes: maximum solar radiation is received during the equinoxes, when a place at the equator is under the subsolar point at high noon, and the intermediate seasons of spring and autumn occur at higher latitudes; and the minimum occurs during both solstices, when either pole is tilted towards or away from the sun, resulting in either summer or winter in both hemispheres. This also results in a corresponding movement of the equator away from the subsolar point, which is then situated over or near the relevant tropic circle. Nevertheless, temperatures are high year-round due to the Earth's axial tilt of 23.5° not being enough to create a low minimum midday declination to sufficiently weaken the Sun's rays even during the solstices. High year-round temperatures extend to about 25° north or south of the equator, although the moderate seasonal temperature difference is defined by the opposing solstices (as it is at higher latitudes) near the poleward limits of this range.
Near the equator, there is little temperature change throughout the year, though there may be dramatic differences in rainfall and humidity. The terms summer, autumn, winter and spring do not generally apply. Lowlands around the equator generally have a tropical rainforest climate, also known as an equatorial climate, though cold ocean currents cause some regions to have tropical monsoon climates with a dry season in the middle of the year, and the Somali Current generated by the Asian monsoon due to continental heating via the high Tibetan Plateau causes Greater Somalia to have an arid climate despite its equatorial location.
Average annual temperatures in equatorial lowlands are around 31 °C (88 °F) during the afternoon and 23 °C (73 °F) around sunrise. Rainfall is very high away from cold ocean current upwelling zones, from 2,500 to 3,500 mm (100 to 140 in) per year. There are about 200 rainy days per year and average annual sunshine hours are around 2,000. Despite high year-round sea level temperatures, some higher altitudes such as the Andes and Mount Kilimanjaro have glaciers. The highest point on the equator is at the elevation of 4,690 metres (15,387 ft), at 0°0′0″N 77°59′31″W / 0.00000°N 77.99194°W, found on the southern slopes of Volcán Cayambe [summit 5,790 metres (18,996 ft)] in Ecuador. This is slightly above the snow line and is the only place on the equator where snow lies on the ground. At the equator, the snow line is around 1,000 metres (3,300 ft) lower than on Mount Everest and as much as 2,000 metres (6,600 ft) lower than the highest snow line in the world, near the Tropic of Capricorn on Llullaillaco.
| Climate data for Libreville, Gabon in Africa | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Month | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec | Year |
| Mean daily maximum °C (°F) | 29.5 (85.1) |
30.0 (86.0) |
30.2 (86.4) |
30.1 (86.2) |
29.4 (84.9) |
27.6 (81.7) |
26.4 (79.5) |
26.8 (80.2) |
27.5 (81.5) |
28.0 (82.4) |
28.4 (83.1) |
29.0 (84.2) |
28.58 (83.44) |
| Daily mean °C (°F) | 26.8 (80.2) |
27.0 (80.6) |
27.1 (80.8) |
26.6 (79.9) |
26.7 (80.1) |
25.4 (77.7) |
24.3 (75.7) |
24.3 (75.7) |
25.4 (77.7) |
25.7 (78.3) |
25.9 (78.6) |
26.2 (79.2) |
25.95 (78.71) |
| Mean daily minimum °C (°F) | 24.1 (75.4) |
24.0 (75.2) |
23.9 (75.0) |
23.1 (73.6) |
24.0 (75.2) |
23.2 (73.8) |
22.1 (71.8) |
21.8 (71.2) |
23.2 (73.8) |
23.4 (74.1) |
23.4 (74.1) |
23.4 (74.1) |
23.30 (73.94) |
| Average rainfall mm (inches) | 250.3 (9.85) |
243.1 (9.57) |
363.2 (14.30) |
339.0 (13.35) |
247.3 (9.74) |
54.1 (2.13) |
6.6 (0.26) |
13.7 (0.54) |
104.0 (4.09) |
427.2 (16.82) |
490.0 (19.29) |
303.2 (11.94) |
2,841.7 (111.88) |
| Average rainy days (≥ 0.1 mm) | 17.9 | 14.8 | 19.5 | 19.2 | 16.0 | 3.70 | 1.70 | 4.90 | 14.5 | 25.0 | 22.6 | 17.6 | 177.4 |
| Mean monthly sunshine hours | 176.7 | 182.7 | 176.7 | 177.0 | 158.1 | 132.0 | 117.8 | 89.90 | 96.00 | 111.6 | 135.0 | 167.4 | 1,720.9 |
| Source: World Meteorological Organization (UN),[11] Hong Kong Observatory[12] | |||||||||||||
| Climate data for Pontianak, Indonesia in Asia | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Month | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec | Year |
| Mean daily maximum °C (°F) | 32.4 (90.3) |
32.7 (90.9) |
32.9 (91.2) |
33.2 (91.8) |
33.0 (91.4) |
33.2 (91.8) |
32.9 (91.2) |
33.4 (92.1) |
32.6 (90.7) |
32.6 (90.7) |
32.2 (90.0) |
32.0 (89.6) |
32.7 (90.9) |
| Daily mean °C (°F) | 27.6 (81.7) |
27.7 (81.9) |
28.0 (82.4) |
28.2 (82.8) |
28.2 (82.8) |
28.2 (82.8) |
27.7 (81.9) |
27.9 (82.2) |
27.6 (81.7) |
27.7 (81.9) |
27.4 (81.3) |
27.2 (81.0) |
27.7 (81.9) |
| Mean daily minimum °C (°F) | 22.7 (72.9) |
22.6 (72.7) |
23.0 (73.4) |
23.2 (73.8) |
23.4 (74.1) |
23.1 (73.6) |
22.5 (72.5) |
22.3 (72.1) |
22.6 (72.7) |
22.8 (73.0) |
22.6 (72.7) |
22.4 (72.3) |
22.7 (72.9) |
| Average rainfall mm (inches) | 260 (10.2) |
215 (8.5) |
254 (10.0) |
292 (11.5) |
256 (10.1) |
212 (8.3) |
201 (7.9) |
180 (7.1) |
295 (11.6) |
329 (13.0) |
400 (15.7) |
302 (11.9) |
3,196 (125.8) |
| Average rainy days (≥ 0.1 mm) | 15 | 13 | 21 | 22 | 20 | 18 | 16 | 25 | 14 | 27 | 25 | 22 | 238 |
| Source: World Meteorological Organization (UN)[13] | |||||||||||||
| Climate data for Macapá, Brazil in South America | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Month | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec | Year |
| Mean daily maximum °C (°F) | 29.7 (85.5) |
29.2 (84.6) |
29.3 (84.7) |
29.5 (85.1) |
30.0 (86.0) |
30.3 (86.5) |
30.6 (87.1) |
31.5 (88.7) |
32.1 (89.8) |
32.6 (90.7) |
32.3 (90.1) |
31.4 (88.5) |
30.71 (87.28) |
| Daily mean °C (°F) | 26.5 (79.7) |
26.2 (79.2) |
26.3 (79.3) |
26.4 (79.5) |
26.8 (80.2) |
26.8 (80.2) |
26.8 (80.2) |
27.4 (81.3) |
27.8 (82.0) |
28.1 (82.6) |
27.9 (82.2) |
27.4 (81.3) |
27.03 (80.65) |
| Mean daily minimum °C (°F) | 23.0 (73.4) |
23.1 (73.6) |
23.2 (73.8) |
23.5 (74.3) |
23.5 (74.3) |
23.2 (73.8) |
22.9 (73.2) |
23.3 (73.9) |
23.4 (74.1) |
23.5 (74.3) |
23.5 (74.3) |
23.4 (74.1) |
23.29 (73.92) |
| Average rainfall mm (inches) | 299.6 (11.80) |
347.0 (13.66) |
407.2 (16.03) |
384.3 (15.13) |
351.5 (13.84) |
220.1 (8.67) |
184.8 (7.28) |
98.0 (3.86) |
42.6 (1.68) |
35.5 (1.40) |
58.4 (2.30) |
142.5 (5.61) |
2,571.5 (101.26) |
| Average rainy days (≥ 0.1 mm) | 23 | 22 | 24 | 24 | 25 | 22 | 19 | 13 | 6 | 5 | 6 | 14 | 203 |
| Mean monthly sunshine hours | 148.8 | 113.1 | 108.5 | 114.0 | 151.9 | 189.0 | 226.3 | 272.8 | 273.0 | 282.1 | 252.0 | 204.6 | 2,336.1 |
| Source: World Meteorological Organization (UN),[14] Hong Kong Observatory[15] | |||||||||||||
Line-crossing ceremonies
[edit]There is a widespread maritime tradition of holding ceremonies to mark a sailor's first crossing of the equator. In the past, these ceremonies have been notorious for their brutality, especially in naval practice. [citation needed] Milder line-crossing ceremonies, typically featuring King Neptune, are also held for passengers' entertainment on some civilian ocean liners and cruise ships.[citation needed]
See also
[edit]References
[edit]- ^ a b "Equator". National Geographic - Education. 6 September 2011. Archived from the original on 9 May 2022. Retrieved 9 March 2021.
- ^ Kher, Aparna. "Equinox: Almost Equal Day and Night". timeanddate.com. Retrieved 5 November 2021.
- ^ "Definition of equator". Oxford Dictionaries. Archived from the original on 23 May 2018. Retrieved 5 May 2018.
- ^ William Barnaby Faherty; Charles D. Benson (1978). "Moonport: A History of Apollo Launch Facilities and Operations". NASA History Series. p. Chapter 1.2: A Saturn Launch Site. NASA Special Publication-4204. Archived from the original on 15 September 2018. Retrieved 8 May 2019.
Equatorial launch sites offered certain advantages over facilities within the continental United States. A launching due east from a site on the equator could take advantage of the earth's maximum rotational velocity (460 m/s (1,510 ft/s)) to achieve orbital speed. The more frequent overhead passage of the orbiting vehicle above an equatorial base would facilitate tracking and communications. Most important, an equatorial launch site would avoid the costly dogleg technique, a prerequisite for placing rockets into equatorial orbit from sites such as Cape Canaveral, Florida (28 degrees north latitude). The necessary correction in the space vehicle's trajectory could be very expensive - engineers estimated that doglegging a Saturn vehicle into a low-altitude equatorial orbit from Cape Canaveral used enough extra propellant to reduce the payload by as much as 80%. In higher orbits, the penalty was less severe but still involved at least a 20% loss of payload.
- ^ Funk, Anna (26 November 2018). "Millions of Years Ago, the Poles Moved — And It Could Have Triggered an Ice Age". Discover Magazine. Archived from the original on 24 September 2023.
- ^ Luzum, Brian; Capitaine, Nicole; Fienga, Agnès; Folkner, William; Fukushima, Toshio; Hilton, James; Hohenkerk, Catherine; Krasinsky, George; Petit, Gérard; Pitjeva, Elena; Soffel, Michael; Wallace, Patrick (2011). "The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy" (PDF). Celest Mech Dyn Astr. 110 (4): 293–304. Bibcode:2011CeMDA.110..293L. doi:10.1007/s10569-011-9352-4. S2CID 122755461. Archived (PDF) from the original on 1 August 2023.
- ^ "General definitions and numerical standards" (PDF). IERS Technical Note 36. Archived from the original (PDF) on 18 December 2018.
- ^ Booda, Larry (9 October 1961). "Transit IV-A Proves Equator Is Elliptical". Space Technology. Aviation Week and Space Technology. Washington, DC, USA: McGraw-Hill. pp. 32–33.
- ^ Instituto Geográfico Militar de Ecuador (24 January 2005). "Memoria Técnica de la Determinación de la Latitud Cero" (in Spanish).
- ^ "Countries on the Equator". 20 March 2019.
- ^ "Weather Information for Libreville". World Weather Information Service. World Meteorological Organization.
- ^ "Climatological Normals of Libreville". Hong Kong Observatory. Archived from the original on 26 October 2019.
- ^ "Weather Information for Pontianak". World Weather Information Service. World Meteorological Organization.
- ^ "Weather Information for Macapa". World Weather Information Service. World Meteorological Organization.
- ^ "Climatological Normals of Macapa". Hong Kong Observatory. Archived from the original on 26 October 2019.
Sources
[edit]- Moritz, H (September 1980). "Geodetic Reference System 1980". Bulletin Géodésique. 54 (3). Berlin: Springer-Verlag: 395–405. Bibcode:1980BGeod..54..395M. doi:10.1007/BF02521480. S2CID 198209711. (IUGG/WGS-84 data)
- Taff, Laurence G (1981). Computational Spherical Astronomy. New York: Wiley. ISBN 0-471-06257-X. OCLC 6532537. (IAU data)
Equator
View on GrokipediaDefinition and Geography
Overview
The Equator is defined as the great circle on Earth's surface at 0° latitude, formed by the intersection of the planet's surface with the plane perpendicular to its axis of rotation and midway between the poles.[9][10] This imaginary line equally divides the Earth into the Northern and Southern Hemispheres and serves as the fundamental reference point for all latitudinal measurements, with lines of latitude extending north and south from it up to 90° at the poles.[1][11] The Equator intersects the Prime Meridian at the coordinates 0° N, 0° E, located in the Gulf of Guinea in the Atlantic Ocean off the western coast of Africa.[12] As a great circle, it encircles the globe completely, spanning approximately 40,075 kilometers in circumference and passing through diverse oceanic and terrestrial regions.[13] Earth's rotation causes a slight equatorial bulge, making the planet an oblate spheroid rather than a perfect sphere; the equatorial diameter measures about 12,756 kilometers, compared to the polar diameter of roughly 12,714 kilometers.[14][15] This equatorial region also demarcates the central band of the tropics, which extend to about 23.5° latitude north and south, influencing the transition to temperate zones beyond.[16]Precise Location
The Equator is defined in the World Geodetic System 1984 (WGS 84) as the locus of points on the Earth's surface at latitude 0°, forming the great circle where the geodetic latitude is zero and intersecting the reference ellipsoid in the equatorial plane perpendicular to the Earth's rotation axis. This system models the Earth as an oblate spheroid with a semi-major axis (equatorial radius) of 6,378,137 meters and a flattening factor of 1/298.257223563, providing a standardized reference for global positioning.[17] The Equator intersects key meridians at precise coordinates within this framework; for instance, it crosses the Prime Meridian (0° longitude) at 0°00′00″N, 0°00′00″E, a point situated in the Gulf of Guinea in the Atlantic Ocean, approximately 610 kilometers south of Ghana's coast. Due to the Earth's oblateness, the Equator's path on the surface deviates slightly from a perfect circle, following the bulging equatorial region where the radius is maximized, resulting in a geoid that is about 21 kilometers wider at the equator than at the poles.[18][19] Modern determination of the Equator's position relies on satellite geodesy, particularly the Global Positioning System (GPS), which uses trilateration to compute locations by measuring pseudoranges to at least four satellites in orbit, achieving accuracies sufficient to verify 0° latitude points. Historically, positions along the Equator were established through triangulation surveys, involving angular measurements from networks of ground control points to propagate latitude values across continents. Notable crossing points include the Mitad del Mundo monument in Ecuador, located at approximately 0°00′08″S, 78°27′21″W near Quito, commemorating the French Geodesic Mission's 18th-century measurements.[20][21][22]Dimensions and Length
The equator represents the longest parallel on Earth's surface, forming a great circle with a circumference of approximately 40,075 kilometers.[23] This measurement is derived from the equatorial radius of the World Geodetic System 1984 (WGS 84) ellipsoid model, where the semi-major axis is 6,378.137 kilometers, yielding .[24] Earth's rotation imparts a centrifugal force that counteracts gravity more strongly at the equator than at the poles, resulting in an oblate spheroid shape with an equatorial bulge. This causes the equatorial radius to be about 21 kilometers greater than the polar radius, widening the equatorial diameter by roughly 43 kilometers compared to the polar diameter.[25] The equator's length is not fixed, as tidal forces from the Moon and Sun induce periodic deformations in Earth's crust and oceans, known as solid Earth tides. These effects cause variations in the equatorial radius of up to 30 centimeters, with annual fluctuations around 20 centimeters primarily from ocean loading and gravitational interactions.[26][27] In comparison to other parallels of latitude, the equator's full circumference dwarfs shorter circles at higher latitudes, where lengths scale by the cosine of the latitude (e.g., the 60° parallel is half as long). Historically, ancient measurements like Eratosthenes' third-century BCE estimate of about 40,000 kilometers—based on solar angles between Syene and Alexandria—foreshadowed modern values with remarkable precision.[21]Etymology and History
Etymology
The term "equator" derives from the Medieval Latin aequator, literally meaning "equalizer," specifically referring to the equalizer of day and night lengths on the celestial sphere.[28] This nomenclature highlights the astronomical observation that, at this great circle perpendicular to Earth's axis, daylight and darkness are of equal duration during the equinoxes.[29] The concept traces its linguistic roots to ancient Greek astronomy, where the celestial equator was termed ho isēmerinos kuklos (ὁ ἰσημερινός κύκλος), meaning "the circle with days of equal duration" or "equinoctial circle," from isos (equal) and hēmera (day).[30] This term, used by Ptolemy in his Almagest (circa 150 CE), described the great circle intersecting the ecliptic at points where the Sun's path yields equal day and night, influencing later Latin adaptations in medieval texts.[30] The Latin aequator diei et noctis ("equalizer of day and night") first appeared in 14th-century astronomical writings, marking the term's formal recording in European scholarship.[28] The word entered English in the late 14th century as "equatour," borrowed via Old French équateur, and was popularized by cartographers building on Ptolemaic geography, who applied it to both the celestial and terrestrial lines.[29] Related terms include "equinoctial," which denotes the quality of equal day and night and often refers to the same line, distinguishing the celestial equator (projected onto the sky) from the terrestrial equator (Earth's surface circle).[28] While "equinoctial" emphasizes the temporal equality during equinoxes, "equator" focuses on the spatial division, a nuance rooted in Hellenistic astronomy's evolution into medieval Latin usage.[30]Historical Exploration and Mapping
The earliest significant efforts to understand and map the Equator date back to ancient Greece in the 3rd century BCE, when Eratosthenes of Cyrene calculated the Earth's circumference with remarkable accuracy using observations tied to latitudinal differences near the tropics. By noting that the Sun was directly overhead at Syene (modern Aswan) on the summer solstice while casting a shadow at Alexandria about 800 kilometers north, he measured an angle of 7.2 degrees, or one-fiftieth of a full circle, leading to an estimate of approximately 252,000 stadia for the circumference—within 2% of the modern equatorial value of 40,075 kilometers.[31] This computation assumed a spherical Earth and provided the foundational framework for later equatorial mapping by establishing a baseline for global scale.[32] During the Age of Exploration, European voyages began to cross and document the Equator directly, confirming its position through navigation. Ferdinand Magellan's expedition of 1519–1522, the first to circumnavigate the globe, crossed the Equator multiple times in the Pacific Ocean, notably on February 13, 1521, while heading northwest from South America toward Asia.[33] These crossings, amid severe hardships like scurvy and supply shortages, allowed the crew to verify the Earth's sphericity and the Equator's role as the dividing line of hemispheres using rudimentary celestial navigation.[33] In the 18th century, scientific expeditions focused on precise measurements along the Equator to resolve debates about Earth's shape. The French Geodesic Mission of 1735–1744, led by figures like Pierre Bouguer and Charles Marie de La Condamine, measured an arc of the meridian near Quito (in present-day Ecuador) to test whether Earth was oblate or prolate.[34] Their triangulation surveys over rugged Andean terrain revealed a slight equatorial bulge, confirming Isaac Newton's predictions and providing the first empirical data on the planet's equatorial radius, which was about 21 kilometers larger than the polar radius.[35] This mission not only refined maps of equatorial South America but also advanced geodesy for global positioning.[34] The 19th century saw astronomical events leveraged for equatorial mapping, such as the 1874 Transit of Venus, where international expeditions observed Venus crossing the Sun's disk to measure solar parallax and improve latitude calculations. Stations in subtropical and tropical regions, including Hawaii and Rodriguez Island, contributed data that enhanced the accuracy of Earth's orbital parameters, indirectly refining equatorial coordinates.[36] Post-World War II advancements in the 20th century shifted to technological methods, with aerial surveys using converted military aircraft enabling detailed photomapping of equatorial terrains in Africa and South America by the 1950s.[37] Early satellites like TIROS-1 (1960) and Landsat-1 (1972) further revolutionized global mapping, providing orbital imagery that precisely delineated the Equator across vast ocean and land expanses.[38]Human Geography and Territories
Countries and Territories
The Equator intersects the landmasses or territorial waters of 13 sovereign nations, spanning South America, Africa, Asia, and the Pacific, with significant portions traversing oceanic exclusive economic zones in the Atlantic, Pacific, and Indian Oceans. These crossings highlight the line's global distribution, covering approximately 40,075 km in total circumference, of which about 78.7% passes over water.[3] In South America, the Equator enters from the Pacific Ocean and crosses three countries, entering Ecuador near the Gulf of Guayaquil and continuing eastward through the Andes foothills before reaching Colombia and then Brazil, where it traverses the northern Amazon basin—the longest continuous land segment—before exiting into the Atlantic.[39] Ecuador derives its name from the Spanish term "ecuador," meaning equator, reflecting its central position where the line bisects the mainland and extends to the Galápagos Islands territory, straddling both hemispheres across volcanic landscapes.[40] Colombia sees a shorter segment in its southern Amazonian departments near the border with Ecuador and Peru, while Brazil's extensive crossing through Amazonas and Roraima states underscores the region's vast equatorial rainforests.[39] In Africa, the Equator emerges from the Atlantic to cross seven countries, starting with the island nation of São Tomé and Príncipe in the Gulf of Guinea, where it passes near the capital. It then moves through Gabon's coastal rainforests, the northern Republic of the Congo, and a substantial portion of the Democratic Republic of the Congo's central Congo Basin, before entering Uganda near Lake Victoria, crossing Kenya's central highlands, and briefly touching Somalia's Puntland region near the Indian Ocean.[3] These African segments, totaling around 3,500 km of land, weave through equatorial forests and savannas.[39] Further east, the Equator traverses the Indian Ocean's exclusive economic zone of the Maldives south of Gaafu Dhaalu Atoll without touching land, enters Indonesia across Sumatra, Borneo (Kalimantan), Sulawesi, and Halmahera islands for multiple segments exceeding 2,000 km combined, and continues into the Pacific to cross Kiribati's Line Islands territory, including atolls like Teraina and Tabuaeran.[41] These insular and maritime passages emphasize the Equator's role in defining oceanic boundaries and island jurisdictions.[39]| Country/Territory | Crossing Type | Key Geographical Extent |
|---|---|---|
| Ecuador (including Galápagos Islands) | Land (mainland and islands) | Bisects Andes and volcanic archipelago; ~300 km on mainland.[40] |
| Colombia | Land | Southern Amazon region near Ecuador border; ~100 km.[39] |
| Brazil | Land | Northern Amazon through Amazonas and Roraima; >2,500 km. |
| São Tomé and Príncipe | Land (islands) | Gulf of Guinea islands near equator's midline.[3] |
| Gabon | Land | Western coastal rainforests; ~200 km.[3] |
| Republic of the Congo | Land | Northern Congo Basin; ~500 km.[39] |
| Democratic Republic of the Congo | Land | Central Congo River basin; ~2,000 km.[3] |
| Uganda | Land | Southern near Lake Victoria; ~300 km.[39] |
| Kenya | Land | Central highlands; ~400 km.[3] |
| Somalia | Land | Northern Puntland; ~50 km.[39] |
| Maldives | Maritime (EEZ) | South of Gaafu Dhaalu Atoll in Indian Ocean.[41] |
| Indonesia | Land (multiple islands) | Sumatra, Borneo, Sulawesi, Halmahera; >2,000 km total.[39] |
| Kiribati (Line Islands) | Land (islands) and maritime | Northern Line Islands atolls in Pacific; ~100 km on land.[41] |

