Equator

An equator is an imaginary circle on the surface of a rotating sphere. As any three-dimensional object, a sphere rotates around a line through its mass center; this line is known as rotation axis. In absence of external torques, a rotation axis is fixed in space. The two places where the rotation axis intersects the surface of the sphere are the poles (the North Pole and the South Pole). The equator is defined as the intersection of the surface of the sphere with a plane (the equatorial plane) that passes through the center of the sphere and is orthogonal to its rotation axis. The equator is a great circle, that is, its center coincides with the center of the sphere. Clearly the equator is midway between the poles and divides the sphere exactly into two halves, the Northern and Southern hemisphere, hence the name (literally equator means divider in equal parts, hemi [ἡμι] is Greek for half). Note that usually the term hemisphere denotes the surface of the half-sphere, not the half-sphere itself.

Earth

PD Image

The Earth is the sphere for which the concept of equator is most important. On Earth the equator services as a reference for geographical coordinates. It is the zero of latitude, i.e., the equator has by definition zero degrees (0°) latitude, the North Pole has by definition ninety degrees latitude (90°N) and the South Pole has latitude 90°S.

In 1980 the Earth's equatorial radius was fixed to the nearest meter at a value of 6 378 137 m by the International Union of Geodesy and Geophysics. This gives the equatorial length equal to 40 075 017 m ≈ 40 075 km. The linear velocity (with respect to an inertial system fixed to the Sun) of a point on Earth, resulting from the diurnal rotation with its angular period of 23h 56 min, is highest on the equator and is about 40075/23.934 ≈ 1674 km/h. Obviously, the linear velocity decreases going north or south and is zero on both poles.

The length of a degree of longitude on the equator (and therewith the lengh of the circumference of the Earth at the equator) was first determined around 1740 by a French expedition to Peru. Scientific members were Pierre Bouguer, Charles Marie de La Condamine, and the leader of the expedition, Louis Godin.

An important circle on the Northern hemisphere (not a great circle) is the Tropic of Capricorn. This is the latitude where the Sun seems exactly overhead once a year—at the summer solstice (around June 21). In 2010 it was at 23º 26′ 17″ north of the equator (the Earth axis "wobbles" somewhat due to external torques so that the latitude of the tropic varies a little in time). The Arctic circle is the polar circle at latitude 90°−23º 26′ 17″ ≈ 66° 34′. It is the northern most latitude on Earth that just sees the sun for a very brief period above the horizon at the winter solstice (around December 22). On the Southern hemisphere these circles are called the Tropic of Capricorn and the Antarctic circle, respectively.

The area around the equator bounded by the Tropic of Cancer and the Tropic of Capricorn, sees the Sun exactly overhead (at 90°) twice a year and at other times under an angle that deviates at most 46° from overhead position. Hence this area on Earth receives a large amount of solar energy all year round and is consequently on average the hottest region on Earth. This region (the "Tropics") hardly experiences any seasons.

Sky

Another important sphere is the celestial sphere. Its equatorial plane coincides with Earth's equatorial plane and the celestial equator divides the sky into a Northern and Southern sky. The celestial equatorial plane makes an angle of 23° 26' with the ecliptic. See the article ecliptic for illustrations.